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iss050e037546 (Feb. 1, 2017) --- Peggy Whitson, Expedition 50 Flight Engineer; Shane Kimbrough, Expedition 50 Commander; and European Space Agency (ESA) astronaut Thomas Pesquet pose with Robonaut in the U.S. Destiny laboratory.
The system includes two alternate plywood components with very sharp spikes instead of the rubberized gasketing material. This is very similar to the spikes that are used on the Aigner X-Guide component.
PictionID:44808567 - Title:Atlas Payload Component Details: Worker with Satellite - Catalog:14_014194 - Filename:14_014194.TIF - - - Image from the Convair/General Dynamics Astronautics Atlas Negative Collection. The processing, cataloging and digitization of these images has been made possible by a generous National Historical Publications and Records grant from the National Archives and Records Administration---Please Tag these images so that the information can be permanently stored with the digital file.---Repository: San Diego Air and Space Museum
Size comparison. The middle tube is an 807, and the right one a 12AT7. The splash of blue in the middle of the 803 tube is the reflection of a book on my desk.
The Space Shuttle orbiter is the spaceplane component of the Space Shuttle, a partially reusable orbital spacecraft system that was part of the discontinued Space Shuttle program. Operated from 1977 to 2011 by NASA, the U.S. space agency, this vehicle could carry astronauts and payloads into low Earth orbit, perform in-space operations, then re-enter the atmosphere and land as a glider, returning its crew and any on-board payload to the Earth.
Six orbiters were built for flight: Enterprise, Columbia, Challenger, Discovery, Atlantis, and Endeavour. All were built in Palmdale, California, by the Pittsburgh, Pennsylvania-based Rockwell International company. The first orbiter, Enterprise, made its maiden flight in 1977. An unpowered glider, it was carried by a modified Boeing 747 airliner called the Shuttle Carrier Aircraft and released for a series of atmospheric test flights and landings. Enterprise was partially disassembled and retired after completion of critical testing. The remaining orbiters were fully operational spacecraft, and were launched vertically as part of the Space Shuttle stack.
Columbia was the first space-worthy orbiter; it made its inaugural flight in 1981. Challenger, Discovery, and Atlantis followed in 1983, 1984, and 1985 respectively. In 1986, Challenger was destroyed in an accident shortly after its 10th launch. Endeavour was built as Challenger's successor, and was first launched in 1992. In 2003, Columbia was destroyed during re-entry, leaving just three remaining orbiters. Discovery completed its final flight on March 9, 2011, and Endeavour completed its final flight on June 1, 2011. Atlantis completed the final Shuttle flight, STS-135, on July 21, 2011.
In addition to their crews and payloads, the reusable orbiter carried most of the Space Shuttle System's liquid-propellant rocket system, but both the liquid hydrogen fuel and the liquid oxygen oxidizer for its three main rocket engines were fed from an external cryogenic propellant tank. Additionally, two reusable solid rocket boosters (SRBs) provided additional thrust for approximately the first two minutes of launch. The orbiters themselves did carry hypergolic propellants for their Reaction Control System (RCS) thrusters and Orbital Maneuvering System (OMS) engines.
Wikipedia: <a href="https://en.wikipedia.org/wiki/Space_Shuttle_orbiter" rel="noreferrer nofollow">en.wikipedia.org/wiki/Space_Shuttle_orbiter</a>
The Chevrolet Corvette (C3) was a sports car that was produced by Chevrolet for the 1968 through 1982 model years. Engines and chassis components were mostly carried over from the previous generation, but the body and interior were new. It set new sales records with 53,807 produced for the 1979 model year. The C3 is the third generation of the Chevrolet Corvette, and marks the second time the Corvette would carry the Stingray name, though only for the 1969 - 1976 model years. This time it was a single word as opposed to Sting Ray as used for the 1963 - 1967 C2 generation. The name would then be retired until 2014 when it was re-introduced with the release of the C7.
11th Annual, Royal City, Show & Shine,
New Westminster, British Columbia, Canada
For a short video on this show;
youtu.be/rnHFWt52hMs
PictionID:44723552 - Title:Atlas Program Component - Catalog:14_013260 - Filename:14_013260.TIF - - - Image from the Convair/General Dynamics Astronautics Atlas Negative Collection. The processing, cataloging and digitization of these images has been made possible by a generous National Historical Publications and Records grant from the National Archives and Records Administration---Please Tag these images so that the information can be permanently stored with the digital file.---Repository: San Diego Air and Space Museum
This model car was number D38 in the Tomica Dandy range of die-cast toy cars. It was made in Japan to 1:43rd scale and issued in 1983. This model car represents the Nissan Skyline RS Turbo C which is a modified Silhouette Formula to Group C specifications. The main identifying feature is the full width rear spoiler. On the Nissan Skyline RS Turbo KDR30 Super Silhouette this rear wing isn’t full width. Both real cars feature on the cover on the 1983 Tomy catalogue. The Skyline Silhouette retains the "silhouette" and engine block of the production R30 Skyline as these were the only concessions in this formula and accounts for ultra wide fenders and equally massive wings! Thoughtfully, Tomica Dandy also made the ordinary production R30 Skyline in 1:43rd scale (there is a version available in red and black) and posing these both together provides a superb 3D visual of the width difference between these two cars.
As a toy car from the 1980’s the level of detail is extremely good and the front section includes cast details for grilles and NACA ducts. Overall Tomica Dandy’s were superior to the competition of the period, exhibited flawless paint finish and tampo printing. The latter utilised for certain aspects of the competition finish. This includes driver names, racing numbers, sponsors names which include TOMICA. Further decoration was available with an enclosed decal sheet. The whole of the front section is removable by lifting the component and then moving it forward. Once this has been removed the engine detail can be seen as can the radiator and lighting section. The former is in black plastic and the latter is represented as a plated plastic component. Both doors open giving access to a miniature racing interior. The main section is in grey plastic and includes dashboard details, gear shift lever and fire extinguisher. Further details include a red drivers seat and a black steering wheel both plastic items. Rubber tyres replicate racing slicks and the hubs in gold plastic provide a basic representation of the real life versions. The axles feature spring suspension. Rear lights are in clear red plastic and the headlights are plated parts. There is little detailing on the metal baseplate but as this replicates a competition car this is expected. However, there are cast details on the front section. Windows are in clear plastic and the windscreen features a rear view mirror.
Tomica Dandy overview
Following on from their success with small scale toy cars, Tomica decided to launch their Dandy range in 1972. Size wise Dandy were comparable with Corgi Toys and Dinky Toys, and as with these ranges the scale varied between releases. However, gradually the majority of models issued followed the Solido line and were in 1:43rd scale. All Dandy series model numbers were prefixed with a D to avoid confusion with Tomica’s miniature series. In 1984 the whole Dandy range was restructured and subsidiary ranges were introduced. Another restructure followed in 1988 and then in 1993 Tomica decided to discontinue their Dandy range. However, from this time Tomica have reissued certain Dandy models either under their own name or in liaison with model shops or distributors.
On a personal level I have always been impressed with the quality of Dandy models and where there are opening parts the fit is perfect and they close with a reassuring click. Even if a Dandy model is turned upside down these opening parts stay shut! This is certainly worth mentioning as this level of precision didn’t manifest in toy cars from most other manufacturers and the only one that is comparable in this area is Solido with their classic 100 series. The Dandy range extended the availability of quality toy cars into the early 1990‘s and provided collectors of toy cars with new releases during this period. Unfortunately, they were not officially released in certain markets and collectors had to rely on local model shops to gain access to this superb range of models.
Please do not use this image on websites, blogs or other media without my permission. Thanks.
Chris
Universal Studios Florida is a theme park located in Orlando, Florida. Opened on June 7, 1990, the park's theme is the entertainment industry, in particular movies and television. Universal Studios Florida inspires its guests to "ride the movies", and it features numerous attractions and live shows. The park is one component of the larger Universal Orlando Resort.
In 2013, the park hosted an estimated 7.06 million guests, ranking it the eighth-most visited theme park in the United States, and ranking it sixteenth worldwide.[2]
Contents [hide]
1 History 1.1 Park history
1.2 Branding
1.3 Timeline
1.4 Previous attractions
2 Park design 2.1 Production Central
2.2 New York
2.3 San Francisco
2.4 London/Diagon Alley
2.5 World Expo
2.6 Woody Woodpecker's Kidzone
2.7 Hollywood
3 Character appearances
4 Production facilities
5 Annual events 5.1 Grad Bash and Gradventure
5.2 Halloween Horror Nights
5.3 Macy's Holiday Parade
5.4 Mardi Gras
5.5 Rock the Universe
5.6 Summer Concert Series
6 Universal's Express Pass
7 Attendance
8 See also
9 References
10 External links
History[edit]
This section needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed. (August 2010)
The original entrance to the theme park.
Over the years, Universal Studios Florida has not limited itself to attractions based on its own vast film library. It has occasionally licensed popular characters from other rival studios, many of whom did not operate theme parks themselves. Some examples include Ghostbusters and Men in Black, (Sony's Columbia Pictures), The Simpsons (20th Century Fox) and Shrek (DreamWorks Animation).
Many of the park's past and present attractions were developed with the actual creators of the films they were based on, and feature the original stars as part of the experience. Steven Spielberg helped create E.T. Adventure and was a creative consultant for Back to the Future: The Ride, Twister...Ride it Out, An American Tail Theatre, Jaws, Men in Black: Alien Attack and Transformers: The Ride.
In many current rides, the original stars reprised their film roles including: Rip Torn and Will Smith in Men in Black: Alien Attack, Brendan Fraser for Revenge of the Mummy: The Ride, Bill Paxton and Helen Hunt in Twister...Ride it Out, Arnold Schwarzenegger, Edward Furlong and Linda Hamilton reprised their roles for Terminator 2: 3-D Battle Across Time, Mike Myers, Eddie Murphy, Cameron Diaz, and John Lithgow for Shrek 4D, Steve Carell, Miranda Cosgrove, Dana Gaier, and Elsie Fisher reprised their roles from Despicable Me for Despicable Me: Minion Mayhem, and Peter Cullen and Frank Welker reprised their roles as Optimus Prime and Megatron for Transformers: The Ride.
In many former rides, the many original stars were also to reprise their film roles such as: Christopher Lloyd and Thomas F. Wilson in Back to the Future: The Ride, Roy Scheider recorded a voice over for the conclusion of Jaws, Alfred Hitchcock and Anthony Perkins appeared in Alfred Hitchcock: The Art of Making Movies, additionally, various Nicktoon voice actors reprised their roles in Jimmy Neutron's Nicktoon Blast.
Park history[edit]
From its inception in 1982,[3] Universal Studios Florida was designed as a theme park and a working studio. It was also the first time that Universal Studios had constructed an amusement park "from the ground up." However, the proposed project was put on hold until 1986, when a meeting between Steven Spielberg, a co-founder for the park, and Peter N. Alexander prompted for the creation of a Back to the Future simulator ride in addition to the already planned King Kong based ride.[4]
A major component of the original park in Hollywood is its studio tour, which featured several special-effects exhibits and encounters built into the tour, such as an attack by the great white shark from the film Jaws. For its Florida park, Universal Studios took the concepts of the Hollywood tour scenes and developed them into larger, stand-alone attractions. As an example, in Hollywood, the studio tour trams travel close to a shoreline and are "attacked" by Jaws before they travel to the next part of the tour. In Florida, guests entered the "Jaws" attraction and would board a boat touring the fictitious Amity Harbor, where they encountered the shark, then exited back into the park at the conclusion of the attraction. Universal Studios Florida originally had a Studio Tour attraction that visited the production facilities, but that tour has since been discontinued.
Branding[edit]
Previous slogans for Universal Studios Florida were: See the Stars. Ride the Movies. (1990 - 1998); No one makes believe like we do! (1990 - 1998); Ride the Movies (1998 - 2008); Jump into the Action (2008–2012). The current slogan is: Experience the Movies (2012–present).
Timeline[edit]
1986: Land clearing takes place on the swamp land purchased by MCA/Universal that would hold the park.
1987: Universal Studios Florida is announced at a press conference on the Hollywood property, with a planned opening date of December 1989.
1988: Universal Studios Florida's opening date is delayed from December, 1989 to May 1, 1990. Shortly following, MCA/Universal releases a video detailing the future park, which stars Christopher Lloyd as the Universal character Doc Brown interacting with the various attractions at the Florida park.[5] Universal Studios allows guests to witness the production of television shows and motion pictures in the Florida park's soundstages in middle 1988, while the rest of the studio/park is still under construction.[6]
1989: MCA/Universal Studios claims that The Walt Disney Company and its CEO, Michael Eisner copied several concepts of the Universal Studios Florida park, and integrated them into Disney's recently opened Disney/MGM Studios park.[7]
1990: On January 31, Universal Studios Florida's opening date is again delayed from May 1, 1990 to June 7, 1990.[8] Universal Studios Florida begins soft openings for the general public in late May.[9] Many of the park's attractions are not yet open at the time, and still under testing. Universal Studios Florida is officially opened with a grand opening style ceremony on June 7.[10] The park opens with five themed areas: The Front Lot (entrance area), Production Central, New York, San Francisco/Amity, Expo Center, Hollywood as well as a Lagoon located in the center of the park. The Front Lot and Production Central areas are referred to as "In Production", the New York section is referred to as "Now Shooting", the San Francisco and Amity sections are referred to as "On Location" and the Expo Center area is referred to as "The World of CineMagic Center". Nickelodeon Studios also opened on this day where there was a grand opening ceremony hosted by Marc Summers. Due to massive technical problems with the original Kongfrontation, Earthquake: The Big One and Jaws rides, Universal begins a temporary voucher service to allow guests to re-visit the studio/park when the attractions are operating.[10] Jaws is temporarily closed by Universal on September 30 due to persistent major technical problems. During the shut-down, Universal sues the original designer of the Jaws ride,[11] Ride & Show Engineering, and hires Totally Fun Company to create a re-designed version of most of the ride.
1991: Universal adds four new attractions to the park: The Blues Brothers Show, StreetBusters, The Screen Test Home Video Adventure and How to Make a Mega Movie Deal.[12] Back to the Future: The Ride officially opens in the World Expo Center area of the park, in a grand opening ceremony.[13] The ride is considered to be a success, and receives positive reception from theme park critics.[14] Fright Nights debuts at the park. In 1992, it is renamed to Halloween Horror Nights.
1993: Jaws is re-opened, with many scenes altered. MCA/Universal announces plans to expand Universal Studios Florida into the Universal City, Florida resort complex, including a second theme park and multiple hotels.[15]
1995: Universal Studios Florida celebrates its 5th anniversary. A Day in the Park with Barney opens in the World Expo area. The Production Studio Tour is closed due to a dwindle in the studios' recent Film/TV production.
1996: Terminator 2: 3-D Battle Across Time opens in the Hollywood area.[16]
1997: Universal announces that Ghostbusters Spooktacular will be replaced by Twister...Ride it Out, with a planned opening date of Spring 1998[17] Universal Studios announces that the sole Studio park will be expanded into the Universal Studios Escape, including the Islands of Adventure park, Universal CityWalk Orlando and multiple hotels. The Islands of Adventure Preview Center opens in the New York area, replacing The Screen Test Home Video Adventure. It is meant to give guests a preview of the up-coming Islands of Adventure park, as well as expansion of the Studio park into the Universal Studios Escape resort.
1998: The expansion begins as the original open parking lot for Universal Studios Florida is demolished and replaced by CityWalk and a parking garage complex.[18] Universal delays the opening of Twister...Ride it Out from March, 1998 to May 4, 1998 out of respect for the 42 deaths caused by a recent El Nino outbreak of tornadoes in the central Florida area. Twister...Ride it Out opens in the New York area, replacing Ghostbusters Spooktacular.[19] A new area of the park, Woody Woodpecker's Kidzone, is officially opened, holding the attractions Curious George Goes to Town, StarToons and the previously opened Fievel's Playland, E.T. Adventure, Animal Actors Stage and A Day in the Park with Barney; CityWalk opens outside of the park.
1999: Woody Woodpecker's Nuthouse Coaster opens in the Woody Woodpecker's Kidzone area. Islands of Adventure opens next door to Universal Studios Florida.[20]
2000: Men in Black: Alien Attack opens in the World Expo area, on the former site of The Swamp Thing Set. Universal Studios Florida's 10th anniversary celebration.
2001: Animal Planet Live opens, replacing Animal Actors Stage.
2002: Universal Studios Escape is renamed Universal Orlando Resort. Kongfrontation closes in a closing ceremony. Halloween Horror Nights is moved to Islands of Adventure. Macy's Holiday Parade debuts at the park.
2003: Jimmy Neutron's Nicktoon Blast opens, replacing The Funtastic World of Hanna-Barbera.[21] Shrek 4-D opens with Donkey's Photo Finish, replacing Alfred Hitchcock: The Art of Making Movies and Stage 54 respectively.[22]
2004: Revenge of the Mummy: The Ride opens, replacing Kongfrontation.[23] Halloween Horror Nights takes place in both Universal Studios Florida and Islands of Adventure.
2005: Universal Express Plus is introduced, replacing Universal Express. Nickelodeon Studios closes after nearly 15 years. Fear Factor Live opens, replacing The Wild Wild Wild West Stunt Show. Universal Studios Florida celebrates its 15th anniversary.
2006: Delancey Street Preview Center opens in the New York area. Universal 360: A Cinesphere Spectacular opens, replacing Dynamite Nights Stunt Spectacular. Animal Planet Live is closed, and replaced by Animal Actors on Location. Halloween Horror Nights returns to Universal Studios Florida for its "Sweet 16".
2007: Back to the Future: The Ride closes on March 30.[24] Blue Man Group Sharp Aquos Theatre opens in CityWalk, replacing Nickelodeon Studios. Earthquake: The Big One closes in the San Francisco area on November 5.
2008: Disaster!: A Major Motion Picture Ride...Starring You! opens, replacing Earthquake: The Big One.[25] Universal announces Hollywood Rip Ride Rockit, with a planned opening of Spring 2009. The Simpsons Ride opens, replacing Back to the Future: The Ride.[26]
2009: The Universal Music Plaza Stage opens, replacing The Boneyard. Hollywood Rip Ride Rockit opens.
2010: The 20th anniversary of Universal Studios Florida in June, as well as Halloween Horror Nights in October.
2011: The 10th anniversary of Macy's Holiday Parade at the park.[27]
2012: Jaws and the surrounding Amity themed area closes, as announced on December 2, 2011.[28] Universal announces the additions of Universal’s Cinematic Spectacular: 100 Years of Movie Memories and Universal's Superstar Parade to the park, with openings on May 8, 2012.[29] Despicable Me: Minion Mayhem, opens replacing Jimmy Neutron's Nicktoon Blast; as announced on March 14, 2011 as "...one of many exciting things planned for the next couple of years".[30] Universal Orlando Resort announced Transformers: The Ride will officially open in the summer of 2013, replacing Soundstages 44 and 54, which were demolished on June 24, 2012.[31] SpongeBob StorePants,a gift shop themed after SpongeBob SquarePants opened in Woody Woodpecker's Kidzone replacing the Universal Cartoon Store
2013: The opening date for Transformers The Ride is announced for June 20, 2013. Details of The Wizarding World of Harry Potter expansion are officially announced. Details for the new Simpsons Land are announced and expected to open in the summer of 2013. Transformers: The Ride officially opens in the Production Central area replacing Soundstage 44. Simpsons Fast Food Boulevard (renamed Springfield U.S.A.) concludes its expansion as it includes one new ride: Kang and Kodos Twirl 'n' Hurl.
2014: The opening date for The Wizarding World of Harry Potter Diagon Alley is announced for July 8, 2014 amid the Diagon Alley preview red carpet premiere on June 18, 2014 with Domhnall Gleeson, Bonnie Wright, Evanna Lynch, Matthew Lewis, James and Oliver Phelps, Tom Felton, Robbie Coltrane, Warwick Davis and Helena Bonham Carter attending the premiere. King's Cross station opens on July 1, 2014 as well as the Hogwarts Express Hogsmeade station at Universal's Islands of Adventure, connecting park visitors to both theme Harry Potter theme parks via a full scale replica of the train that appears in the Harry Potter film series. Diagon Alley officially opens, replacing Jaws and the Amity section of the park.
Previous attractions[edit]
Main article: List of former Universal Studios Florida attractions
The previous icon of the Jaws ride is still a popular photo spot.
Like all theme parks, attractions are sometimes closed due to aging and replaced with more contemporary attractions. Universal has seen this happen several times. Some notable closures include Kongfrontation, Back to the Future: The Ride, The Funtastic World of Hanna-Barbera and Jaws. The closures of Kongfrontation, Back to the Future, and Jaws have been given homages by the park to honor veteran visitors who revered the former rides.
Park design[edit]
Main article: List of Universal Studios Florida attractions
Universal Studios Florida features seven themed areas all situated around a large lagoon. In 2012, this lagoon was the site of Universal’s Cinematic Spectacular: 100 Years of Movie Memories, a thematic display that showcased scenes from various Universal films, featuring lasers, projectors and fountains, and pyrotechnics.
The seven surrounding themed areas, clockwise from the entrance, are Production Central, New York, San Francisco, London/Diagon Alley, World Expo, Woody Woodpecker's Kidzone and Hollywood. Each area features a combination of rides, shows, attractions, character appearances, dining outlets and merchandise stores. A new area, based on Harry Potter's Diagon Alley was added to the park in the July of 2014.
Production Central[edit]
Ride
Year opened
Manufacturer
Despicable Me: Minion Mayhem 2012 Intamin
Shrek 4-D 2003 PDI/DreamWorks
Hollywood Rip, Ride, Rockit 2009 Maurer Söhne
Transformers: The Ride 3D 2013 Oceaneering International
The Universal Music Plaza Stage 2009
The area is also home to a variety of dining outlets and merchandise shops. Food and beverage items can be purchased from Beverly Hills Boulangerie or Universal Studios' Classic Monsters Cafe while merchandise can be bought from a variety of themed stores including Universal Studios Store, Studio Sweets, It's a Wrap!, Super Silly Stuff, Shrek's Ye Olde Souvenir Shoppe, and Transformers: Supply Vault.[32][33]
Crawler crane with telescopic boom, based on the components of the Liebherr LTM 1800 (boom and upper structure) and LR 1550 (crawler undercarriage).
I built this model many years ago. It is still based on the old 9V components with geared and non-geared motors, as well as micromotors.
Motorized functions include:
- Independent drive of left and right crawlers
- Four support rams
- Two support rams on long cantilevered support beams for the erection of long boom systems.
- Slewing of the upper structure
- Four winches
- Independent extension of first and second telescopic boom stage.
- The cab can swing out from transport position
- Auxiliary winch on the front end of the upper structure
Further functions include:
- Variable counterweight of more than 4.5 kg, consisting of 12x250g, 4x285g and a base plate of about 500g
- Openable sliding door on tiltable cab
The crane can be set up with the telescopic boom alone. Height is then up to 2.4m. A luffing jib can be added, but the boom can't be extended in this mode. Height is also somewhere around 2.4m with a reach of about 1.7m.
PictionID:44808664 - Title:Atlas Payload Component - Catalog:14_014202 - Filename:14_014202.TIF - - - Image from the Convair/General Dynamics Astronautics Atlas Negative Collection. The processing, cataloging and digitization of these images has been made possible by a generous National Historical Publications and Records grant from the National Archives and Records Administration---Please Tag these images so that the information can be permanently stored with the digital file.---Repository: San Diego Air and Space Museum
YJ04 LYK was one of 4 vehicles taken out of the Yorkshire Coastliner fleet after the conclusion of the summer 2010 timetable, in order to go to Harrogate.
The move was necessary on order for Harrogate to send off 2 of it's own 2003 reg Wright Eclipse Gemini's to Blackburn for a complete overhaul of the engine, drivetrain, and other components - new seats and exterior panels have been installed to the H&D buses to make them look like Gemini 2's whilst also delivering similar emissions.
Meanwhile, the four former Yorkshire Coastliner Volvo B7TL Wright Eclipse Gemini 1's would help to operate route 36 between Ripon, Harrogate, and Leeds and deliver a slight improvement in service frequency. Because putting them into a new livery would have taken time and money, new vinyls were applied instead explaining why these buses wee being used - and they got the local nickname of the "red cog buses" for obvious reasons. The front of the bus was given the tag "Yes! it is a 36" as people would not be familiar with the livery.
As Yorkshire Coastliner got four new Gemini 2's in April 2011, these Gemini 1's were supposed to go across to Lancashire to boost services over there. However, instead 403 has come back across for Coastliner services, and would seem to be based at the York depot for the time being. Still in the 'cross dress' bit-of-both livery, YJ04LYK is seen leaving York station on a service 844 to Leeds... despite the front saying "yes! it is a 36"!
PictionID:44808627 - Title:Atlas Payload Component - Catalog:14_014199 - Filename:14_014199.TIF - - - Image from the Convair/General Dynamics Astronautics Atlas Negative Collection. The processing, cataloging and digitization of these images has been made possible by a generous National Historical Publications and Records grant from the National Archives and Records Administration---Please Tag these images so that the information can be permanently stored with the digital file.---Repository: San Diego Air and Space Museum
This alternate pusher component is designed to secure to the sliding table with a lever actuated clamping post. The bumper component has the same rubberized gasketing material along one edge to help secure stock wedged between the two plywood components that make up the system. Also shown in this photo is an alternate plywood "bumper" component.
This is the "pusher" half the the RUWI component system. It is a plywood panel approximately 1-inch thick with a handle and rubberized gasketing applied to the front edge, and an adjustable mechanism for setting the angle of the panel and securing it to the sliding table. Unlike a Fritz & Franz design, this component pivots which I consider a disadvantage.
A technician with the John C. Stennis Space Center's Fluid Component Facility studies samples to determine cleanliness of valves and fittings used on pipes that transport liquid fuel and propellants. The clean room where the technicians work is similar to a hospital surgical room.
Credit: NASA
Image Number: 95-081-19
Date: 1995
Nationaal Archief/Spaarnestad Photo/J. de Jong
Nederlands: De groentenboer, die ook diepvries en conserven verkoopt, doet appels in de tas van de klant met oorwarmers, Hengelo 1947.
English: Greengrocer. The Netherlands, Hengelo, 1947.
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Meer foto’s van Spaarnestad Photo zijn te vinden op onze beeldbank: www.spaarnestadphoto.nl/
SoulRider.222 / Eric Rider © 2023
------ As of 1/1/2023 ------- (nearly 41 pounds - and all human powered, which makes this an insane weight, I know)
Main:
2015 Kona Supreme Operator frame
Roach top tube pad
2022 Manitou Dorado Comp 203mm coil fork (with Pro model polished crowns)
2022 Marzocchi Bomber CR 203mm coil shock
Fox M8 x 38mm shock hardware mounting kit
Fox 400# coil spring (241.3mm x 76mm / 9.5 x 3.0)
THE front fender
Ground Keeper rear fender
Seating:
Jagwire Lex SL dropper post cable kit
Kona seatpost collar
Wolf Tooth Dropper Remote
PNW Cascade external dropper post
SDG Radar seat
Drivetrain:
Hope F20 pedals
2006 E13 (e. thirteen) SRS chain guide
Shimano Zee FC-M645 cranks (Boost)
Generic CNC Hollowtech II crank bolt
Renthal 1XR 34 tooth chainring
Wolf Tooth Components bash ring
Wolf Tooth Components chainring bolts
Specialty Racing Products (SRP) chainring bolts
KMC X10 chain (10 speed)
Shimano XT M800 BB92 Hollowtech II press-fit bottom bracket (Boost)
Transmission:
MicroSHIFT Advent X derailleur (10 speed)
MicroSHIFT Advent X Trail Trigger Pro shifter (10 speed)
MicroSHIFT Advent X 11-52 tooth cassette (10 speed)
Jagwire Lex SL shift cable and housing
Cockpit:
FSA Orbit C-40 headset with ABEC sealed cartridge bearings (lower = 36° x 45° / upper = 45° x 45°)
FSA 1.5 to 1.125 reducer crown race
Wolf Tooth headset bling kit
Renthal FatBar 35mm handlebar
Renthal Integra II 35mm direct mount stem
ODI Rogue Lock-On grips
Rear wheel:
Industry Nine Hydra MTN HG hub (12x157mm Super Boost)
DT Swiss Competition (14/15/14) double butted stainless steel spokes
DT Swiss brass nipples
Spank Spoon 32 rim (32 hole, 26 inch, 32mm outer width, Schrader valve)
Maxxis High Roller II Kevlar bead tire (26 x 2.40)
Rear brake:
Shimano 180mm R/P180 rear caliper adaptor
Galfer Wave 180mm rear rotor
2020 Hope Tech 3 E4 rear brake
Front wheel:
Hope Pro 4 front hub (20x110mm Standard)
DT Swiss Competition (14/15/14) double butted stainless steel spokes
DT Swiss brass nipples
Spank Spoon 32 rim (32 hole, 26 inch, 32mm outer width, Schrader valve)
Maxxis Minion DHF EXO (26 x 2.50)
Front brake:
Manitou 5mm rotor adaptor (20x110 Boost)
Shimano SM-RT75 203mm front rotor
2010 Hope Tech M4 front brake
All my wheels were custom made. Hand-built by Universal Cycles in Oregon.
PictionID:44808603 - Title:Atlas Payload Component - Catalog:14_014197 - Filename:14_014197.TIF - - - Image from the Convair/General Dynamics Astronautics Atlas Negative Collection. The processing, cataloging and digitization of these images has been made possible by a generous National Historical Publications and Records grant from the National Archives and Records Administration---Please Tag these images so that the information can be permanently stored with the digital file.---Repository: San Diego Air and Space Museum
“Cuatro Torres Business Area” (CTBA). Antigua Ciudad Deportiva del Real Madrid. Paseo de la Castellana. Los componentes más recientes de la Skyline de Madrid
El parque empresarial “Cuatro Torres Business Area” (CTBA) se edifica sobre los terrenos de la antigua Ciudad Deportiva del Real Madrid al extremo norte del paseo de la Castellana, conformado por cuatro rascacielos, los edificios más altos de España. El conjunto comprende un anillo de circulación subterráneo que da servicio a aparcamientos y plantas bajo rasante de cada uno de los edificios. Proyectado en 2002-2003, la construcción se inició en 2004 y la urbanización se culmina en 2009 con la inclusión de algunas interesantes esculturas como la Menina de Manolo Valdés entre las torres CajaMadrid y Sacyr Vallehermoso.
En este recinto se situará además el Centro Internacional de Convenciones de Madrid con un auditorio principal con capacidad para 3.500 personas, según proyecto del equipo formado por Emilio Tuñón y Luis Moreno Mansilla ganadores del concurso convocado en 2007. El edificio propuesto se conforma mediante un círculo erigido verticalmente que se presenta como un disco solar delante de las dos torres centrales.
El Conjunto es fruto de la operación urbanística llevada a cabo por el Real Madrid Club de Fútbol, siendo presidente el empresario Florentino Pérez, por lo que algunos han dado a las torres el nombre de cada uno de los jugadores “galácticos” que fichó el citado presidente como consecuencia de la operación: Figo, Ronaldo, Zidane y Beckham.
Torre CajaMadrid (inicialmente Torre Repsol)
Arquitecto: Norman Foster & Partners
Estructura: Halvorson & Partners - Gilsanz Murray Steficek LLP. Instalaciones: Aguilera Ingenieros. Responsables del proyecto de construcción José Ramón Burgos Morcillo y Pedro González Lejarriaga
Es el edificio más alto de España, con 45 plantas y 250 metros de altura. Proyecto: 2003. Edificado entre 2004 y 2009. La estructura está compuesta por un entramado de acero, que permite una planta rectangular de oficinas, soportado por dos grandes núcleos de hormigón, que encierran los elementos de comunicación vertical y de servicio, que se unen en el remate superior mediante un elemento tipo puente. La fachada se cubre de vidrio en la zona de oficinas y de placas de acero inoxidable en los núcleos de hormigón. Las plantas de oficinas se agrupan en tres cuerpos prismáticos intercalados entre los dos núcleos verticales que los sustentan, conformando una geometría que da su característica imagen al edificio.
Una vez iniciada la construcción, Repsol decidió cambiar la ubicación de su futura sede por lo que el edificio en obras fue adquirido por Caja Madrid con el fin de convertirlo en su sede principal en 2009
Torre Sacyr Vallehermoso (Hotel Eurostars Madrid Tower)
Arquitectos: Carlos Rubio Carvajal y Enrique Álvarez-Sala Walter (R&AS).
Estructura: MC2, Julio Martínez Calzón y Miguel Gómez Navarro. Instalaciones: UTE Aguilera-Úrculo.
Proyectada en 2003, promovida por el Grupo SYV, se construye entre 2004 y 2008, con una altura de 236 metros y 52 plantas
Los autores conciben el edificio a partir del análisis de geometrías rigurosas, capaces de albergar diferentes usos aportando la flexibilidad necesaria. Se configura mediante la superposición de un centro de congresos, un hotel de gran lujo, que ocupa los dos tercios inferiores, y unas oficinas en alquiler, sobre las 17 plantas superiores.
Su planta se genera mediante un triángulo equilátero cuyos lados son curvos, tres arcos que envuelven a tres cilindros situados en posición triangular, optimizando la longitud de la fachada en relación con la superficie construida. Tres pliegues verticales dividen el edificio en gajos, haciéndolo más esbelto e introduciendo luz y ventilación en el núcleo central. Las fachadas, compuestas de una doble piel formada por escamas de vidrio y aluminio que ofrecen una resistencia mínima al viento, presentan una imagen singular dentro del Conjunto, con su tonalidad oscura.
Torre de Cristal
Arquitecto: César Pelli.
Colaboradores: Íñigo Ortiz y Enrique León.
Promovido por la compañía aseguradora Mutua Madrileña, es el edificio más alto de España, junto a la Torre Caja Madrid, con una altura de 250 metros distribuidos en 52 plantas. Proyectada por el arquitecto de origen argentino afincado en New York Cesar Pelli en 2003, se edifica entre 2004 y 2009. Las plantas varían a lo largo de la altura, generando cuatro planos con biseles oblicuos, que confieren a las fachadas del edificio, formadas por muros cortina de vidrio, la apariencia de un cristal tallado, rematado por un plano inclinado bajo el que se conforma un jardín cubierto de invierno. Un gran bloque de cristal transparente, cuyas caras captan la luz “como si fuera un diamante tallado”. La variedad de los ángulos que delimitan cada uno de las caras da vida y movimiento a la torre a través de la diferente intensidad de luz que éstas reflejen durante el día. Su destino es el de oficinas de alquiler. Uno de los atractivos del edificio, que finalmente no autorizó el Ayuntamiento, era una especie de faro situado en su parte más alta, destinado a iluminar el invernadero, que haría visible el rascacielos desde varios puntos de la ciudad.
Torre Espacio
Arquitecto Henry N. Cobb de la firma Pei Cobb Freed & Partners, fundada por Ieoh Ming Pei. Colaborador: José Bruguera.
Colaborador en la dirección de las obras: Reid Fenwick Asociados, de Madrid. Estructura: MC2. Instalaciones: R. Úrculo Ingenieros Consultores.
Proyectada en 2003, promovida por la Inmobiliaria Espacio S.L, se construye entre 2004 y 2008, con una altura de 236 metros y 57 plantas sobre el nivel del suelo. La fachada está formada por un muro cortina de vidrio. Las plantas, varían de forma y dimensiones a lo largo de su altura, pasando del cuadrado en la base, hasta alcanzar la forma de un ojo abierto, es decir dos arcos de circunferencia secantes, en su culminación; dando al edificio una fisonomía exterior muy variable, desde un prisma a una botella, dependiendo del punto de vista. Las aristas son curvas y las fachadas no son planas, por lo que hubo que dotar de un especial diseño a los soportes de hormigón. Alberga, entre otras, oficinas de empresas pertenecientes al grupo promotor como la Inmobiliaria Espacio o la constructora OHL, y algunas embajadas. Cuenta con dos áreas de descanso de ocho metros de altura situadas en las plantas 18 y 33. Su sistema de climatización está compuesto por el "Techo Frío" emisor y la “fachada activa” de doble capa con movimiento de aire interior.
Durante su construcción, en septiembre de 2006 se declaró un incendio entre la planta 40 y 42, la última en construcción en ese momento, pero no afectó a su estructura.
not so grainy on larger size [all sizes]
constructive components made of paper tubes, rolls of aluminum (offset) rubber and some wire, exceeds of the press of a newspaper
sort of shigeru ban
An incredible classy build with all the best components. Zeke went all out on this build and the result is stunning! The fully flamed finish was the perfect choice for such a vintage looking build, ready for the street or the track. Photos by Andrew Hibma (www.hibmaphotography.ca)
Frame:
F5 Pista, columbus zona tubing
Fork/Headset:
Tange headset
Crankset/Bottom Bracket:
165 sugino75, shimano
Pedals:
Allcity track pedals, mks cages
Drivetrain/Cog/Chainring/Chain:
17t all-city, kmc
Handlebars/Stem:
Nitto steel track drops, Nitto Pearl
Saddle/Seatpost:
brooks cambium
Brakes:
sram apex
Front Wheel/Hub/Tire:
hplusson tb14, dura ace 7600, vitoria supercorsa
Rear Wheel/Hub/Tire:
hplusson tb14, dura ace 7600, vitoria supercorsa
The International Space Station (ISS) is a space station (habitable artificial satellite) in low Earth orbit. The ISS programme is a joint project between five participating space agencies: NASA (United States), Roscosmos (Russia), JAXA (Japan), ESA (Europe), and CSA (Canada).[6][7] The ownership and use of the space station is established by intergovernmental treaties and agreements.[8]
The ISS serves as a microgravity and space environment research laboratory in which crew members conduct experiments in biology, human biology, physics, astronomy, meteorology, and other fields.[9][10][11] The station is suited for the testing of spacecraft systems and equipment required for missions to the Moon and Mars.[12] The ISS maintains an orbit with an average altitude of 400 kilometres (250 mi) by means of reboost manoeuvres using the engines of the Zvezda module or visiting spacecraft.[13] It circles the Earth in roughly 92 minutes and completes 15.5 orbits per day.[14]
The station is divided into two sections, the Russian Orbital Segment (ROS), which is operated by Russia, and the United States Orbital Segment (USOS), which is shared by many nations. Roscosmos has endorsed the continued operation of ISS through 2024,[15] but had previously proposed using elements of the Russian segment to construct a new Russian space station called OPSEK.[16]As of December 2018, the station is expected to operate until 2030.[17]
The first ISS component was launched in 1998, with the first long-term residents arriving on 2 November 2000.[18] Since then, the station has been continuously occupied for 18 years and 359 days.[19] This is the longest continuous human presence in low Earth orbit, having surpassed the previous record of 9 years and 357 days held by Mir. The latest major pressurised module was fitted in 2011, with an experimental inflatable space habitat added in 2016. Development and assembly of the station continues, with several major new Russian elements scheduled for launch starting in 2020. The ISS is the largest human-made body in low Earth orbit and can often be seen with the naked eye from Earth.[20][21] The ISS consists of pressurised habitation modules, structural trusses, solar arrays, radiators, docking ports, experiment bays and robotic arms. Major ISS modules have been launched by Russian Proton and Soyuz rockets and US Space Shuttles.[22]
The ISS is the ninth space station to be inhabited by crews, following the Soviet and later Russian Salyut, Almaz, and Mir stations as well as Skylab from the US. The station is serviced by a variety of visiting spacecraft: the Russian Soyuz and Progress, the US Dragon and Cygnus, the Japanese H-II Transfer Vehicle,[6] and the European Automated Transfer Vehicle. The Dragon spacecraft allows the return of pressurised cargo to Earth (downmass), which is used for example to repatriate scientific experiments for further analysis. The Soyuz return capsule has minimal downmass capability next to the astronauts.
The ISS has been visited by astronauts, cosmonauts and space tourists from 18 different nations. As of 14 March 2019, 236 people from 18 countries had visited the space station, many of them multiple times. The United States sent 149 people, Russia sent 47, nine were Japanese, eight were Canadian, five were Italian, four were French, three were German, and there were one each from Belgium, Brazil, Denmark, Kazakhstan, Malaysia, the Netherlands, South Africa, United Arab Emirates, South Korea, Spain, Sweden, and the United Kingdom.[23]
Contents
1 Purpose
2 Manufacturing
3 Assembly
4 Structure
5 Systems
6 Operations
7 Mission controls
8 Fleet operations
9 Life aboard
10 Crew health and safety
11 Orbital debris threats
12 End of mission
13 Cost
14 International co-operation
15 Sightings from Earth
16 See also
17 Notes
18 References
19 Further reading
20 External links
Purpose
The ISS was originally intended to be a laboratory, observatory, and factory while providing transportation, maintenance, and a low Earth orbit staging base for possible future missions to the Moon, Mars, and asteroids. However, not all of the uses envisioned in the initial Memorandum of Understanding between NASA and Roskosmos have come to fruition.[24] In the 2010 United States National Space Policy, the ISS was given additional roles of serving commercial, diplomatic[25] and educational purposes.[26]
Scientific research
Main article: Scientific research on the International Space Station
Comet Lovejoy photographed by Expedition 30 commander Dan Burbank
Expedition 8 Commander and Science Officer Michael Foale conducts an inspection of the Microgravity Science Glovebox
Fisheye view of several labs
CubeSats are deployed by the NanoRacks CubeSat Deployer
The ISS provides a platform to conduct scientific research, with power, data, cooling, and crew available to support experiments. Small uncrewed spacecraft can also provide platforms for experiments, especially those involving zero gravity and exposure to space, but space stations offer a long-term environment where studies can be performed potentially for decades, combined with ready access by human researchers.[27][28]
The ISS simplifies individual experiments by allowing groups of experiments to share the same launches and crew time. Research is conducted in a wide variety of fields, including astrobiology, astronomy, physical sciences, materials science, space weather, meteorology, and human research including space medicine and the life sciences.[9][10][11][29][30] Scientists on Earth have timely access to the data and can suggest experimental modifications to the crew. If follow-on experiments are necessary, the routinely scheduled launches of resupply craft allows new hardware to be launched with relative ease.[28] Crews fly expeditions of several months' duration, providing approximately 160 person-hours per week of labour with a crew of 6. However, a considerable amount of crew time is taken up by station maintenance.[9][31]
Perhaps the most notable ISS experiment is the Alpha Magnetic Spectrometer (AMS), which is intended to detect dark matter and answer other fundamental questions about our universe and is as important as the Hubble Space Telescope according to NASA. Currently docked on station, it could not have been easily accommodated on a free flying satellite platform because of its power and bandwidth needs.[32][33] On 3 April 2013, scientists reported that hints of dark matter may have been detected by the AMS.[34][35][36][37][38][39] According to the scientists, "The first results from the space-borne Alpha Magnetic Spectrometer confirm an unexplained excess of high-energy positrons in Earth-bound cosmic rays."
The space environment is hostile to life. Unprotected presence in space is characterised by an intense radiation field (consisting primarily of protons and other subatomic charged particles from the solar wind, in addition to cosmic rays), high vacuum, extreme temperatures, and microgravity.[40] Some simple forms of life called extremophiles,[41] as well as small invertebrates called tardigrades[42] can survive in this environment in an extremely dry state through desiccation.
Medical research improves knowledge about the effects of long-term space exposure on the human body, including muscle atrophy, bone loss, and fluid shift. This data will be used to determine whether high duration human spaceflight and space colonisation are feasible. As of 2006, data on bone loss and muscular atrophy suggest that there would be a significant risk of fractures and movement problems if astronauts landed on a planet after a lengthy interplanetary cruise, such as the six-month interval required to travel to Mars.[43][44]
Medical studies are conducted aboard the ISS on behalf of the National Space Biomedical Research Institute (NSBRI). Prominent among these is the Advanced Diagnostic Ultrasound in Microgravity study in which astronauts perform ultrasound scans under the guidance of remote experts. The study considers the diagnosis and treatment of medical conditions in space. Usually, there is no physician on board the ISS and diagnosis of medical conditions is a challenge. It is anticipated that remotely guided ultrasound scans will have application on Earth in emergency and rural care situations where access to a trained physician is difficult.[45][46][47]
Free fall
ISS crew member storing samples
A comparison between the combustion of a candle on Earth (left) and in a free fall environment, such as that found on the ISS (right)
Gravity at the altitude of the ISS is approximately 90% as strong as at Earth's surface, but objects in orbit are in a continuous state of freefall, resulting in an apparent state of weightlessness.[48] This perceived weightlessness is disturbed by five separate effects:[49]
Drag from the residual atmosphere.
Vibration from the movements of mechanical systems and the crew.
Actuation of the on-board attitude control moment gyroscopes.
Thruster firings for attitude or orbital changes.
Gravity-gradient effects, also known as tidal effects. Items at different locations within the ISS would, if not attached to the station, follow slightly different orbits. Being mechanically interconnected these items experience small forces that keep the station moving as a rigid body.
Researchers are investigating the effect of the station's near-weightless environment on the evolution, development, growth and internal processes of plants and animals. In response to some of this data, NASA wants to investigate microgravity's effects on the growth of three-dimensional, human-like tissues, and the unusual protein crystals that can be formed in space.[10]
Investigating the physics of fluids in microgravity will provide better models of the behaviour of fluids. Because fluids can be almost completely combined in microgravity, physicists investigate fluids that do not mix well on Earth. In addition, examining reactions that are slowed by low gravity and low temperatures will improve our understanding of superconductivity.[10]
The study of materials science is an important ISS research activity, with the objective of reaping economic benefits through the improvement of techniques used on the ground.[50] Other areas of interest include the effect of the low gravity environment on combustion, through the study of the efficiency of burning and control of emissions and pollutants. These findings may improve current knowledge about energy production, and lead to economic and environmental benefits. Future plans are for the researchers aboard the ISS to examine aerosols, ozone, water vapour, and oxides in Earth's atmosphere, as well as cosmic rays, cosmic dust, antimatter, and dark matter in the universe.[10]
Exploration
A 3D plan of the Russia-based MARS-500 complex, used for ground-based experiments which complement ISS-based preparations for a human mission to Mars
The ISS provides a location in the relative safety of Low Earth Orbit to test spacecraft systems that will be required for long-duration missions to the Moon and Mars. This provides experience in operations, maintenance as well as repair and replacement activities on-orbit, which will be essential skills in operating spacecraft farther from Earth, mission risks can be reduced and the capabilities of interplanetary spacecraft advanced.[12] Referring to the MARS-500 experiment, ESA states that "Whereas the ISS is essential for answering questions concerning the possible impact of weightlessness, radiation and other space-specific factors, aspects such as the effect of long-term isolation and confinement can be more appropriately addressed via ground-based simulations".[51] Sergey Krasnov, the head of human space flight programmes for Russia's space agency, Roscosmos, in 2011 suggested a "shorter version" of MARS-500 may be carried out on the ISS.[52]
In 2009, noting the value of the partnership framework itself, Sergey Krasnov wrote, "When compared with partners acting separately, partners developing complementary abilities and resources could give us much more assurance of the success and safety of space exploration. The ISS is helping further advance near-Earth space exploration and realisation of prospective programmes of research and exploration of the Solar system, including the Moon and Mars."[53] A crewed mission to Mars may be a multinational effort involving space agencies and countries outside the current ISS partnership. In 2010, ESA Director-General Jean-Jacques Dordain stated his agency was ready to propose to the other four partners that China, India and South Korea be invited to join the ISS partnership.[54] NASA chief Charlie Bolden stated in February 2011, "Any mission to Mars is likely to be a global effort".[55] Currently, US federal legislation prevents NASA co-operation with China on space projects.[56]
Education and cultural outreach
Original Jules Verne manuscripts displayed by crew inside Jules Verne ATV
The ISS crew provides opportunities for students on Earth by running student-developed experiments, making educational demonstrations, allowing for student participation in classroom versions of ISS experiments, and directly engaging students using radio, videolink and email.[6][57] ESA offers a wide range of free teaching materials that can be downloaded for use in classrooms.[58] In one lesson, students can navigate a 3-D model of the interior and exterior of the ISS, and face spontaneous challenges to solve in real time.[59]
JAXA aims to inspire children to "pursue craftsmanship" and to heighten their "awareness of the importance of life and their responsibilities in society."[60] Through a series of education guides, a deeper understanding of the past and near-term future of crewed space flight, as well as that of Earth and life, will be learned.[61][62] In the JAXA Seeds in Space experiments, the mutation effects of spaceflight on plant seeds aboard the ISS is explored. Students grow sunflower seeds which flew on the ISS for about nine months. In the first phase of Kibō utilisation from 2008 to mid-2010, researchers from more than a dozen Japanese universities conducted experiments in diverse fields.[63]
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ESA Astronaut Paolo Nespoli's spoken voice, recorded about the ISS in November 2017, for Wikipedia
Cultural activities are another major objective. Tetsuo Tanaka, director of JAXA's Space Environment and Utilization Center, says "There is something about space that touches even people who are not interested in science."[64]
Amateur Radio on the ISS (ARISS) is a volunteer programme which encourages students worldwide to pursue careers in science, technology, engineering and mathematics through amateur radio communications opportunities with the ISS crew. ARISS is an international working group, consisting of delegations from nine countries including several countries in Europe as well as Japan, Russia, Canada, and the United States. In areas where radio equipment cannot be used, speakerphones connect students to ground stations which then connect the calls to the station.[65]
First Orbit is a feature-length documentary film about Vostok 1, the first crewed space flight around the Earth. By matching the orbit of the International Space Station to that of Vostok 1 as closely as possible, in terms of ground path and time of day, documentary filmmaker Christopher Riley and ESA astronaut Paolo Nespoli were able to film the view that Yuri Gagarin saw on his pioneering orbital space flight. This new footage was cut together with the original Vostok 1 mission audio recordings sourced from the Russian State Archive. Nespoli, during Expedition 26/27, filmed the majority of the footage for this documentary film, and as a result is credited as its director of photography.[66] The film was streamed through the website firstorbit.org in a global YouTube premiere in 2011, under a free licence.[67]
In May 2013, commander Chris Hadfield shot a music video of David Bowie's "Space Oddity" on board the station; the film was released on YouTube.[68] It was the first music video ever to be filmed in space.[69]
In November 2017, while participating in Expedition 52/53 on the ISS, Paolo Nespoli made two recordings (one in English the other in his native Italian) of his spoken voice, for use on Wikipedia articles. These were the first content made specifically for Wikipedia, in space.[70][71]
Manufacturing
Main article: Manufacturing of the International Space Station
ISS module Node 2 manufacturing and processing in the SSPF
Since the International Space Station is a multi-national collaborative project, the components for in-orbit assembly were manufactured in various countries around the world. Beginning in the mid 1990s, the U.S. components Destiny, Unity, the Integrated Truss Structure, and the solar arrays were fabricated at the Marshall Space Flight Center and the Michoud Assembly Facility. These modules were delivered to the Operations and Checkout Building and the Space Station Processing Facility for final assembly and processing for launch.[72]
The Russian modules, including Zarya and Zvezda, were manufactured at the Khrunichev State Research and Production Space Center in Moscow. Zvezda was initially manufactured in 1985 as a component for Mir-2, but was never launched and instead became the ISS Service Module.[73]
The European Space Agency Columbus module was manufactured at the European Space Research and Technology Centre (ESTEC) in the Netherlands, along with many other contractors throughout Europe.[74] The other ESA-built modules - Harmony, Tranquility, the Leonardo MPLM, and the Cupola - were initially manufactured at the Thales Alenia Space factory located at the Cannes Mandelieu Space Center. The structural steel hulls of the modules were transported by aircraft to the Kennedy Space Center SSPF for launch processing.[75]
The Japanese Experiment Module Kibō, was fabricated in various technology manufacturing facilities in Japan, at the NASDA (now JAXA) Tanegashima Space Center, and the Institute of Space and Astronautical Science. The Kibo module was transported by ship and flown by aircraft to the KSC Space Station Processing Facility.[76]
The Mobile Servicing System, consisting of the Canadarm2 and the Dextre grapple fixture, was manufactured at various factories in Canada and the United States under contract by the Canadian Space Agency. The mobile base system, a connecting framework for Canadarm2 mounted on rails, was built by Northrop Grumman.
Assembly
Main articles: Assembly of the International Space Station and List of ISS spacewalks
The assembly of the International Space Station, a major endeavour in space architecture, began in November 1998.[3] Russian modules launched and docked robotically, with the exception of Rassvet. All other modules were delivered by the Space Shuttle, which required installation by ISS and shuttle crewmembers using the Canadarm2 (SSRMS) and extra-vehicular activities (EVAs); as of 5 June 2011, they had added 159 components during more than 1,000 hours of EVA (see List of ISS spacewalks). 127 of these spacewalks originated from the station, and the remaining 32 were launched from the airlocks of docked Space Shuttles.[77] The beta angle of the station had to be considered at all times during construction.[78]
The first module of the ISS, Zarya, was launched on 20 November 1998 on an autonomous Russian Proton rocket. It provided propulsion, attitude control, communications, electrical power, but lacked long-term life support functions. Two weeks later, a passive NASA module Unity was launched aboard Space Shuttle flight STS-88 and attached to Zarya by astronauts during EVAs. This module has two Pressurised Mating Adapter (PMAs), one connects permanently to Zarya, the other allowed the Space Shuttle to dock to the space station. At that time, the Russian station Mir was still inhabited, and the ISS remained uncrewed for two years. On 12 July 2000, Zvezda was launched into orbit. Preprogrammed commands on board deployed its solar arrays and communications antenna. It then became the passive target for a rendezvous with Zarya and Unity: it maintained a station-keeping orbit while the Zarya-Unity vehicle performed the rendezvous and docking via ground control and the Russian automated rendezvous and docking system. Zarya's computer transferred control of the station to Zvezda's computer soon after docking. Zvezda added sleeping quarters, a toilet, kitchen, CO2 scrubbers, dehumidifier, oxygen generators, exercise equipment, plus data, voice and television communications with mission control. This enabled permanent habitation of the station.[79][80]
The first resident crew, Expedition 1, arrived in November 2000 on Soyuz TM-31. At the end of the first day on the station, astronaut Bill Shepherd requested the use of the radio call sign "Alpha", which he and cosmonaut Krikalev preferred to the more cumbersome "International Space Station".[81] The name "Alpha" had previously been used for the station in the early 1990s,[82] and its use was authorised for the whole of Expedition 1.[83] Shepherd had been advocating the use of a new name to project managers for some time. Referencing a naval tradition in a pre-launch news conference he had said: "For thousands of years, humans have been going to sea in ships. People have designed and built these vessels, launched them with a good feeling that a name will bring good fortune to the crew and success to their voyage."[84] Yuri Semenov, the President of Russian Space Corporation Energia at the time, disapproved of the name "Alpha" as he felt that Mir was the first modular space station, so the names "Beta" or "Mir 2" for the ISS would have been more fitting.[83][85][86]
Expedition 1 arrived midway between the flights of STS-92 and STS-97. These two Space Shuttle flights each added segments of the station's Integrated Truss Structure, which provided the station with Ku-band communication for US television, additional attitude support needed for the additional mass of the USOS, and substantial solar arrays supplementing the station's existing 4 solar arrays.[87]
Over the next two year, the station continued to expand. A Soyuz-U rocket delivered the Pirs docking compartment. The Space Shuttles Discovery, Atlantis, and Endeavour delivered the Destiny laboratory and Quest airlock, in addition to the station's main robot arm, the Canadarm2, and several more segments of the Integrated Truss Structure.
The expansion schedule was interrupted by the Space Shuttle Columbia disaster in 2003 and a resulting hiatus in flights. The Space Shuttle was grounded until 2005 with STS-114 flown by Discovery.[88]
Assembly resumed in 2006 with the arrival of STS-115 with Atlantis, which delivered the station's second set of solar arrays. Several more truss segments and a third set of arrays were delivered on STS-116, STS-117, and STS-118. As a result of the major expansion of the station's power-generating capabilities, more pressurised modules could be accommodated, and the Harmony node and Columbus European laboratory were added. These were soon followed by the first two components of Kibō. In March 2009, STS-119 completed the Integrated Truss Structure with the installation of the fourth and final set of solar arrays. The final section of Kibō was delivered in July 2009 on STS-127, followed by the Russian Poisk module. The third node, Tranquility, was delivered in February 2010 during STS-130 by the Space Shuttle Endeavour, alongside the Cupola, followed in May 2010 by the penultimate Russian module, Rassvet. Rassvet was delivered by Space Shuttle Atlantis on STS-132 in exchange for the Russian Proton delivery of the US-funded Zarya module in 1998.[89] The last pressurised module of the USOS, Leonardo, was brought to the station in February 2011 on the final flight of Discovery, STS-133.[90] The Alpha Magnetic Spectrometer was delivered by Endeavour on STS-134 the same year.[91]
As of June 2011, the station consisted of 15 pressurised modules and the Integrated Truss Structure. Five modules are still to be launched, including the Nauka with the European Robotic Arm, the Prichal module, and two power modules called NEM-1 and NEM-2.[92] As of March 2019, Russia's future primary research module Nauka is set to launch in the summer of 2020, along with the European Robotic Arm which will be able to relocate itself to different parts of the Russian modules of the station.[93]
The gross mass of the station changes over time. The total launch mass of the modules on orbit is about 417,289 kg (919,965 lb) (as of 3 September 2011).[94] The mass of experiments, spare parts, personal effects, crew, foodstuff, clothing, propellants, water supplies, gas supplies, docked spacecraft, and other items add to the total mass of the station. Hydrogen gas is constantly vented overboard by the oxygen generators.
The ISS is a third generation[95] modular space station.[96] Modular stations can allow modules to be added to or removed from the existing structure, allowing greater flexibility.
Below is a diagram of major station components. The blue areas are pressurised sections accessible by the crew without using spacesuits. The station's unpressurised superstructure is indicated in red. Other unpressurised components are yellow. The Unity node joins directly to the Destiny laboratory. For clarity, they are shown apart.
Zarya
Zarya as seen by Space Shuttle Endeavour during STS-88
Zarya (Russian: Заря́, lit. 'Dawn'), also known as the Functional Cargo Block or FGB (from the Russian: "Функционально-грузовой блок", lit. 'Funktsionalno-gruzovoy blok' or ФГБ), is the first module of the ISS to be launched.[97] The FGB provided electrical power, storage, propulsion, and guidance to the ISS during the initial stage of assembly. With the launch and assembly in orbit of other modules with more specialized functionality, Zarya is now[when?] primarily used for storage, both inside the pressurized section and in the externally mounted fuel tanks. The Zarya is a descendant of the TKS spacecraft designed for the Russian Salyut program. The name Zarya, which means sunrise,[97] was given to the FGB because it signified the dawn of a new era of international cooperation in space. Although it was built by a Russian company, it is owned by the United States.[98]
Zarya was built from December 1994 to January 1998 at the Khrunichev State Research and Production Space Center (KhSC) in Moscow.[97]
Zarya was launched on 20 November 1998 on a Russian Proton rocket from Baikonur Cosmodrome Site 81 in Kazakhstan to a 400 km (250 mi) high orbit with a designed lifetime of at least 15 years. After Zarya reached orbit, STS-88 launched on 4 December 1998 to attach the Unity module.
Unity
Unity as seen by Space Shuttle Endeavour during STS-88
Main article: Unity (ISS module)
The Unity connecting module, also known as Node 1, is the first U.S.-built component of the ISS. It connects the Russian and United States segments of the station, and is where crew eat meals together.
The module is cylindrical in shape, with six berthing locations (forward, aft, port, starboard, zenith, and nadir) facilitating connections to other modules. Unity measures 4.57 metres (15.0 ft) in diameter, is 5.47 metres (17.9 ft) long, made of steel, and was built for NASA by Boeing in a manufacturing facility at the Marshall Space Flight Center in Huntsville, Alabama. Unity is the first of the three connecting modules; the other two are Harmony and Tranquility.
Unity was carried into orbit as the primary cargo of the Space Shuttle Endeavour on STS-88, the first Space Shuttle mission dedicated to assembly of the station. On 6 December 1998, the STS-88 crew mated the aft berthing port of Unity with the forward hatch of the already orbiting Zarya module. This was the first connection made between two station modules.
Zvezda
Zvezda as seen by Space Shuttle Endeavour during STS-97
Main article: Zvezda (ISS module)
Zvezda (Russian: Звезда́, meaning "star"), Salyut DOS-8, also known as the Zvezda Service Module, is a module of the ISS. It was the third module launched to the station, and provides all of the station's life support systems, some of which are supplemented in the USOS, as well as living quarters for two crew members. It is the structural and functional center of the Russian Orbital Segment, which is the Russian part of the ISS. Crew assemble here to deal with emergencies on the station.[99][100][101]
The basic structural frame of Zvezda, known as "DOS-8", was initially built in the mid-1980s to be the core of the Mir-2 space station. This means that Zvezda is similar in layout to the core module (DOS-7) of the Mir space station. It was in fact labeled as Mir-2 for quite some time in the factory. Its design lineage thus extends back to the original Salyut stations. The space frame was completed in February 1985 and major internal equipment was installed by October 1986.
The rocket used for launch to the ISS carried advertising; it was emblazoned with the logo of Pizza Hut restaurants,[102][103][104] for which they are reported to have paid more than US$1 million.[105] The money helped support Khrunichev State Research and Production Space Center and the Russian advertising agencies that orchestrated the event.[106]
On 26 July 2000, Zvezda became the third component of the ISS when it docked at the aft port of Zarya. (U.S. Unity module had already been attached to the Zarya.) Later in July, the computers aboard Zarya handed over ISS commanding functions to computers on Zvezda.[107]
Destiny
The Destiny module being installed on the ISS
Main article: Destiny (ISS module)
The Destiny module, also known as the U.S. Lab, is the primary operating facility for U.S. research payloads aboard the International Space Station (ISS).[108][109] It was berthed to the Unity module and activated over a period of five days in February, 2001.[110] Destiny is NASA's first permanent operating orbital research station since Skylab was vacated in February 1974.
The Boeing Company began construction of the 14.5-tonne (32,000 lb) research laboratory in 1995 at the Michoud Assembly Facility and then the Marshall Space Flight Center in Huntsville, Alabama.[108] Destiny was shipped to the Kennedy Space Center in Florida in 1998, and was turned over to NASA for pre-launch preparations in August 2000. It launched on 7 February 2001 aboard the Space Shuttle Atlantis on STS-98.[110]
Quest
Quest Joint Airlock Module
Main article: Quest Joint Airlock
The Quest Joint Airlock, previously known as the Joint Airlock Module, is the primary airlock for the ISS. Quest was designed to host spacewalks with both Extravehicular Mobility Unit (EMU) spacesuits and Orlan space suits. The airlock was launched on STS-104 on 14 July 2001. Before Quest was attached, Russian spacewalks using Orlan suits could only be done from the Zvezda service module, and American spacewalks using EMUs were only possible when a Space Shuttle was docked. The arrival of Pirs docking compartment on September 16, 2001 provided another airlock from which Orlan spacewalks can be conducted.[citation needed]
Pirs and Poisk
The Pirs module attached to the ISS.
Poisk after arriving at the ISS on 12 November 2009.
Main articles: Pirs (ISS module) and Poisk (ISS module)
Pirs (Russian: Пирс, lit. 'pier') and Poisk (Russian: По́иск, lit. 'search') are Russian airlock modules, each having 2 identical hatches. An outward-opening hatch on the Mir space station failed after it swung open too fast after unlatching, because of a small amount of air pressure remaining in the airlock.[111] All EVA hatches on the ISS open inwards and are pressure-sealing. Pirs was used to store, service, and refurbish Russian Orlan suits and provided contingency entry for crew using the slightly bulkier American suits. The outermost docking ports on both airlocks allow docking of Soyuz and Progress spacecraft, and the automatic transfer of propellants to and from storage on the ROS.[112]
Pirs was launched on 14 September 2001, as ISS Assembly Mission 4R, on a Russian Soyuz-U rocket, using a modified Progress spacecraft, Progress M-SO1, as an upper stage. Poisk was launched on 10 November 2009[113][114] attached to a modified Progress spacecraft, called Progress M-MIM2, on a Soyuz-U rocket from Launch Pad 1 at the Baikonur Cosmodrome in Kazakhstan.
Harmony
Harmony shown connected to Columbus, Kibo, and Destiny. PMA-2 faces. The nadir and zenith locations are open.
Main article: Harmony (ISS module)
Harmony, also known as Node 2, is the "utility hub" of the ISS. It connects the laboratory modules of the United States, Europe and Japan, as well as providing electrical power and electronic data. Sleeping cabins for four of the six crew are housed here.[115]
Harmony was successfully launched into space aboard Space Shuttle flight STS-120 on October 23, 2007.[116][117] After temporarily being attached to the port side of the Unity node,[118][119] it was moved to its permanent location on the forward end of the Destiny laboratory on November 14, 2007.[120] Harmony added 2,666 cubic feet (75.5 m3) to the station's living volume, an increase of almost 20 percent, from 15,000 cu ft (420 m3) to 17,666 cu ft (500.2 m3). Its successful installation meant that from NASA's perspective, the station was "U.S. Core Complete".
Tranquility
Tranquility in 2011
Main article: Tranquility (ISS module)
Tranquility, also known as Node 3, is a module of the ISS. It contains environmental control systems, life support systems, a toilet, exercise equipment, and an observation cupola.
ESA and the Italian Space Agency had Tranquility built by Thales Alenia Space. A ceremony on November 20, 2009 transferred ownership of the module to NASA.[121] On February 8, 2010, NASA launched the module on the Space Shuttle's STS-130 mission.
Columbus
The Columbus module on the ISS
Main article: Columbus (ISS module)
Columbus is a science laboratory that is part of the ISS and is the largest single contribution to the ISS made by the European Space Agency (ESA).
Like the Harmony and Tranquility modules, the Columbus laboratory was constructed in Turin, Italy by Thales Alenia Space. The functional equipment and software of the lab was designed by EADS in Bremen, Germany. It was also integrated in Bremen before being flown to the Kennedy Space Center (KSC) in Florida in an Airbus Beluga. It was launched aboard Space Shuttle Atlantis on 7 February 2008 on flight STS-122. It is designed for ten years of operation. The module is controlled by the Columbus Control Centre, located at the German Space Operations Centre, part of the German Aerospace Center in Oberpfaffenhofen near Munich, Germany.
The European Space Agency has spent €1.4 billion (about US$2 billion) on building Columbus, including the experiments that will fly in it and the ground control infrastructure necessary to operate them.[122]
Kibō
Kibō Exposed Facility on the right
Main article: Kibo (ISS module)
The Japanese Experiment Module (JEM), nicknamed Kibo (きぼう Kibō, Hope), is a Japanese science module for the ISS developed by JAXA. It is the largest single ISS module, and is attached to the Harmony module. The first two pieces of the module were launched on Space Shuttle missions STS-123 and STS-124. The third and final components were launched on STS-127.[123]
Pressurised Module
Experiment Logistics Module
Exposed Facility
Experiment Logistics Module
Remote Manipulator System
Cupola
The Cupola's windows with shutters open.
Main article: Cupola (ISS module)
The Cupola is an ESA-built observatory module of the ISS. Its name derives from the Italian word cupola, which means "dome". Its seven windows are used to conduct experiments, dockings and observations of Earth. It was launched aboard Space Shuttle mission STS-130 on 8 February 2010 and attached to the Tranquility (Node 3) module. With the Cupola attached, ISS assembly reached 85 percent completion. The Cupola's central window has a diameter of 80 cm (31 in).[124]
Rassvet
Rassvet as seen from the Cupola module during STS-132 with a Progress in the lower right
Main article: Rassvet (ISS module)
Rassvet (Russian: Рассве́т; lit. "dawn"), also known as the Mini-Research Module 1 (MRM-1) (Russian: Малый исследовательский модуль, МИМ 1) and formerly known as the Docking Cargo Module (DCM), is a component of the ISS. The module's design is similar to the Mir Docking Module launched on STS-74 in 1995. Rassvet is primarily used for cargo storage and as a docking port for visiting spacecraft. It was flown to the ISS aboard Space Shuttle Atlantis on the STS-132 mission on May 14, 2010,[125] and was connected to the ISS on May 18.[126] The hatch connecting Rassvet with the ISS was first opened on May 20.[127] On 28 June 2010, the Soyuz TMA-19 spacecraft performed the first docking with the module.[128]
Leonardo
Leonardo Permanent Multipurpose Module
Main article: Leonardo (ISS module)
The Leonardo Permanent Multipurpose Module (PMM) is a module of the ISS. It was flown into space aboard the Space Shuttle on STS-133 on 24 February 2011 and installed on 1 March. Leonardo is primarily used for storage of spares, supplies and waste on the ISS, which was until then stored in many different places within the space station. The Leonardo PMM was a Multi-Purpose Logistics Module (MPLM) before 2011, but was modified into its current configuration. It was formerly one of three MPLM used for bringing cargo to and from the ISS with the Space Shuttle. The module was named for Italian polymath Leonardo da Vinci.
Bigelow Expandable Activity Module
Progression of expansion of BEAM
Main article: Bigelow Expandable Activity Module
The Bigelow Expandable Activity Module (BEAM) is an experimental expandable space station module developed by Bigelow Aerospace, under contract to NASA, for testing as a temporary module on the ISS from 2016 to at least 2020. It arrived at the ISS on 10 April 2016,[129] was berthed to the station on 16 April, and was expanded and pressurized on 28 May 2016.
International Docking Adapter
IDA-1 upright
Main article: International Docking Adapter
The International Docking Adapter (IDA) is a spacecraft docking system adapter developed to convert APAS-95 to the NASA Docking System (NDS)/International Docking System Standard (IDSS). An IDA is placed on each of the ISS' two open Pressurized Mating Adapters (PMAs), both of which are connected to the Harmony module.
IDA-1 was lost during the launch failure of SpaceX CRS-7 on 28 June 2015.[130][131][132]
IDA-2 was launched on SpaceX CRS-9 on 18 July 2016.[133] It was attached and connected to PMA-2 during a spacewalk on 19 August 2016.[134] First docking was achieved with the arrival of Crew Dragon Demo-1 on 3 March 2019. [135]
IDA-3 was launched on the SpaceX CRS-18 mission in July 2019.[136] IDA-3 is constructed mostly from spare parts to speed construction.[137] It was attached and connected to PMA-3 during a spacewalk on 21 August 2019. [138]
Unpressurised elements
ISS Truss Components breakdown showing Trusses and all ORUs in situ
The ISS has a large number of external components that do not require pressurisation. The largest of these is the Integrated Truss Structure (ITS), to which the station's main solar arrays and thermal radiators are mounted.[139] The ITS consists of ten separate segments forming a structure 108.5 m (356 ft) long.[3]
The station was intended to have several smaller external components, such as six robotic arms, three External Stowage Platforms (ESPs) and four ExPRESS Logistics Carriers (ELCs).[140][141] While these platforms allow experiments (including MISSE, the STP-H3 and the Robotic Refueling Mission) to be deployed and conducted in the vacuum of space by providing electricity and processing experimental data locally, their primary function is to store spare Orbital Replacement Units (ORUs). ORUs are parts that can be replaced when they fail or pass their design life, including pumps, storage tanks, antennas, and battery units. Such units are replaced either by astronauts during EVA or by robotic arms.[142] Several shuttle missions were dedicated to the delivery of ORUs, including STS-129,[143] STS-133[144] and STS-134.[145] As of January 2011, only one other mode of transportation of ORUs had been utilised – the Japanese cargo vessel HTV-2 – which delivered an FHRC and CTC-2 via its Exposed Pallet (EP).[146][needs update]
Construction of the Integrated Truss Structure over New Zealand.
There are also smaller exposure facilities mounted directly to laboratory modules; the Kibō Exposed Facility serves as an external 'porch' for the Kibō complex,[147] and a facility on the European Columbus laboratory provides power and data connections for experiments such as the European Technology Exposure Facility[148][149] and the Atomic Clock Ensemble in Space.[150] A remote sensing instrument, SAGE III-ISS, was delivered to the station in February 2017 aboard CRS-10,[151] and the NICER experiment was delivered aboard CRS-11 in June 2017.[152] The largest scientific payload externally mounted to the ISS is the Alpha Magnetic Spectrometer (AMS), a particle physics experiment launched on STS-134 in May 2011, and mounted externally on the ITS. The AMS measures cosmic rays to look for evidence of dark matter and antimatter.[153][154]
The commercial Bartolomeo External Payload Hosting Platform, manufactured by Airbus, is due to launch in May 2019 aboard a commercial ISS resupply vehicle and be attached to the European Columbus module. It will provide a further 12 external payload slots, supplementing the eight on the ExPRESS Logistics Carriers, ten on Kibō, and four on Columbus. The system is designed to be robotically serviced and will require no astronaut intervention. It is named after Christopher Columbus's younger brother.[155][156][157]
Robotic arms and cargo cranes
Commander Volkov stands on Pirs with his back to the Soyuz whilst operating the manual Strela crane holding photographer Kononenko.
Dextre, like many of the station's experiments and robotic arms, can be operated from Earth and perform tasks while the crew sleeps.
The Integrated Truss Structure serves as a base for the station's primary remote manipulator system, called the Mobile Servicing System (MSS), which is composed of three main components. Canadarm2, the largest robotic arm on the ISS, has a mass of 1,800 kilograms (4,000 lb) and is used to dock and manipulate spacecraft and modules on the USOS, hold crew members and equipment in place during EVAs and move Dextre around to perform tasks.[158] Dextre is a 1,560 kg (3,440 lb) robotic manipulator with two arms, a rotating torso and has power tools, lights and video for replacing orbital replacement units (ORUs) and performing other tasks requiring fine control.[159] The Mobile Base System (MBS) is a platform which rides on rails along the length of the station's main truss. It serves as a mobile base for Canadarm2 and Dextre, allowing the robotic arms to reach all parts of the USOS.[160] To gain access to the Russian Segment a grapple fixture was added to Zarya on STS-134, so that Canadarm2 can inchworm itself onto the ROS.[161] Also installed during STS-134 was the 15 m (50 ft) Orbiter Boom Sensor System (OBSS), which had been used to inspect heat shield tiles on Space Shuttle missions and can be used on station to increase the reach of the MSS.[161] Staff on Earth or the station can operate the MSS components via remote control, performing work outside the station without space walks.
Japan's Remote Manipulator System, which services the Kibō Exposed Facility,[162] was launched on STS-124 and is attached to the Kibō Pressurised Module.[163] The arm is similar to the Space Shuttle arm as it is permanently attached at one end and has a latching end effector for standard grapple fixtures at the other.
The European Robotic Arm, which will service the Russian Orbital Segment, will be launched alongside the Multipurpose Laboratory Module in 2017.[164] The ROS does not require spacecraft or modules to be manipulated, as all spacecraft and modules dock automatically and may be discarded the same way. Crew use the two Strela (Russian: Стрела́; lit. Arrow) cargo cranes during EVAs for moving crew and equipment around the ROS. Each Strela crane has a mass of 45 kg (99 lb).
Planned componments
Nauka
Artist's rendering of the Nauka module docked to Zvezda.
Main article: Nauka (ISS module)
Nauka (Russian: Нау́ка; lit. Science), also known as the Multipurpose Laboratory Module (MLM), (Russian: Многофункциональный лабораторный модуль, or МЛМ), is a component of the ISS which has not yet been launched into space. The MLM is funded by the Roscosmos State Corporation. In the original ISS plans, Nauka was to use the location of the Docking and Stowage Module. Later, the DSM was replaced by the Rassvet module and it was moved to Zarya's nadir port. Planners anticipate Nauka will dock at Zvezda's nadir port, replacing Pirs.[165]
The launch of Nauka, initially planned for 2007, has been repeatedly delayed for various reasons. As of September 2019, the launch to the ISS is assigned to no earlier than December 2020.[166] After this date, the warranties of some of Nauka's systems will expire.
Prichal
Mockup of the Prichal module at the Yuri Gagarin Cosmonaut Training Center
Main article: Prichal (ISS module)
Prichal, also known as Uzlovoy Module or UM (Russian: Узловой Модуль "Причал", Nodal Module Berth),[167] is a 4-tonne (8,800 lb)[168] ball-shaped module that will allow docking of two scientific and power modules during the final stage of the station assembly, and provide the Russian segment additional docking ports to receive Soyuz MS and Progress MS spacecraft. UM is due to be launched in 2022.[169] It will be integrated with a special version of the Progress cargo ship and launched by a standard Soyuz rocket, docking to the nadir port of the Nauka module. One port is equipped with an active hybrid docking port, which enables docking with the MLM module. The remaining five ports are passive hybrids, enabling docking of Soyuz and Progress vehicles, as well as heavier modules and future spacecraft with modified docking systems. The node module was intended to serve as the only permanent element of the cancelled OPSEK.[170][171]
Science Power Modules 1 and 2
Science Power Module 1 (SPM-1, also known as NEM-1) Science Power Module 2 (SPM-2, also known as NEM-2) are modules planned to arrive at the ISS in 2022.[169][172][173] It is going to dock to the Prichal module, which is planned to be attached to the Nauka module.[173] If Nauka is cancelled, then the Prichal, SPM-1, and SPM-2 would dock at the zenith port of Zvezda. SPM-1 and SPM-2 would also be required components for the OPSEK space station.[174]
Bishop Airlock Module
Main article: Bishop Airlock Module
The NanoRacks Bishop Airlock Module is a commercially-funded airlock module intended to be launched to the ISS on SpaceX CRS-21 in August 2020.[175][176] The module is being built by NanoRacks, Thales Alenia Space, and Boeing.[177] It will be used to deploy CubeSats, small satellites, and other external payloads for NASA, CASIS, and other commercial and governmental customers.[178]
Cancelled componments
The cancelled Habitation module under construction at Michoud in 1997
Several modules planned for the station were cancelled over the course of the ISS programme. Reasons include budgetary constraints, the modules becoming unnecessary, and station redesigns after the 2003 Columbia disaster. The US Centrifuge Accommodations Module would have hosted science experiments in varying levels of artificial gravity.[179] The US Habitation Module would have served as the station's living quarters. Instead, the sleep stations are now spread throughout the station.[180] The US Interim Control Module and ISS Propulsion Module would have replaced the functions of Zvezda in case of a launch failure.[181] Two Russian Research Modules were planned for scientific research.[182] They would have docked to a Russian Universal Docking Module.[183] The Russian Science Power Platform would have supplied power to the Russian Orbital Segment independent of the ITS solar arrays.
Systems
Life support
Main articles: ISS ECLSS and Chemical oxygen generator
The critical systems are the atmosphere control system, the water supply system, the food supply facilities, the sanitation and hygiene equipment, and fire detection and suppression equipment. The Russian Orbital Segment's life support systems are contained in the Zvezda service module. Some of these systems are supplemented by equipment in the USOS. The MLM Nauka laboratory has a complete set of life support systems.
Atmospheric control systems
A flowchart diagram showing the components of the ISS life support system.
The interactions between the components of the ISS Environmental Control and Life Support System (ECLSS)
The atmosphere on board the ISS is similar to the Earth's.[184] Normal air pressure on the ISS is 101.3 kPa (14.69 psi);[185] the same as at sea level on Earth. An Earth-like atmosphere offers benefits for crew comfort, and is much safer than a pure oxygen atmosphere, because of the increased risk of a fire such as that responsible for the deaths of the Apollo 1 crew.[186] Earth-like atmospheric conditions have been maintained on all Russian and Soviet spacecraft.[187]
The Elektron system aboard Zvezda and a similar system in Destiny generate oxygen aboard the station.[188] The crew has a backup option in the form of bottled oxygen and Solid Fuel Oxygen Generation (SFOG) canisters, a chemical oxygen generator system.[189] Carbon dioxide is removed from the air by the Vozdukh system in Zvezda. Other by-products of human metabolism, such as methane from the intestines and ammonia from sweat, are removed by activated charcoal filters.[189]
Part of the ROS atmosphere control system is the oxygen supply. Triple-redundancy is provided by the Elektron unit, solid fuel generators, and stored oxygen. The primary supply of oxygen is the Elektron unit which produces O
2 and H
2 by electrolysis of water and vents H2 overboard. The 1 kW (1.3 hp) system uses approximately one litre of water per crew member per day. This water is either brought from Earth or recycled from other systems. Mir was the first spacecraft to use recycled water for oxygen production. The secondary oxygen supply is provided by burning O
2-producing Vika cartridges (see also ISS ECLSS). Each 'candle' takes 5–20 minutes to decompose at 450–500 °C (842–932 °F), producing 600 litres (130 imp gal; 160 US gal) of O
2. This unit is manually operated.[190]
The US Orbital Segment has redundant supplies of oxygen, from a pressurised storage tank on the Quest airlock module delivered in 2001, supplemented ten years later by ESA-built Advanced Closed-Loop System (ACLS) in the Tranquility module (Node 3), which produces O
2 by electrolysis.[191] Hydrogen produced is combined with carbon dioxide from the cabin atmosphere and converted to water and methane.
Power and thermal control
Main articles: Electrical system of the International Space Station and External Active Thermal Control System
Russian solar arrays, backlit by sunset
One of the eight truss mounted pairs of USOS solar arrays
Double-sided solar arrays provide electrical power to the ISS. These bifacial cells collect direct sunlight on one side and light reflected off from the Earth on the other, and are more efficient and operate at a lower temperature than single-sided cells commonly used on Earth.[192]
The Russian segment of the station, like most spacecraft, uses 28 volt low voltage DC from four rotating solar arrays mounted on Zarya and Zvezda. The USOS uses 130–180 V DC from the USOS PV array, power is stabilised and distributed at 160 V DC and converted to the user-required 124 V DC. The higher distribution voltage allows smaller, lighter conductors, at the expense of crew safety. The two station segments share power with converters.
The USOS solar arrays are arranged as four wing pairs, for a total production of 75 to 90 kilowatts.[193] These arrays normally track the sun to maximise power generation. Each array is about 375 m2 (4,036 sq ft) in area and 58 m (190 ft) long. In the complete configuration, the solar arrays track the sun by rotating the alpha gimbal once per orbit; the beta gimbal follows slower changes in the angle of the sun to the orbital plane. The Night Glider mode aligns the solar arrays parallel to the ground at night to reduce the significant aerodynamic drag at the station's relatively low orbital altitude.[194]
The station originally used rechargeable nickel–hydrogen batteries (NiH
2) for continuous power during the 35 minutes of every 90-minute orbit that it is eclipsed by the Earth. The batteries are recharged on the day side of the orbit. They had a 6.5-year lifetime (over 37,000 charge/discharge cycles) and were regularly replaced over the anticipated 20-year life of the station.[195] Starting in 2016, the nickel–hydrogen batteries were replaced by lithium-ion batteries, which are expected to last until the end of the ISS program.[196]
The station's large solar panels generate a high potential voltage difference between the station and the ionosphere. This could cause arcing through insulating surfaces and sputtering of conductive surfaces as ions are accelerated by the spacecraft plasma sheath. To mitigate this, plasma contactor units (PCU)s create current paths between the station and the ambient plasma field.[197]
ISS External Active Thermal Control System (EATCS) diagram
The station's systems and experiments consume a large amount of electrical power, almost all of which is converted to heat. To keep the internal temperature within workable limits, a passive thermal control system (PTCS) is made of external surface materials, insulation such as MLI, and heat pipes. If the PTCS cannot keep up with the heat load, an External Active Thermal Control System (EATCS) maintains the temperature. The EATCS consists of an internal, non-toxic, water coolant loop used to cool and dehumidify the atmosphere, which transfers collected heat into an external liquid ammonia loop. From the heat exchangers, ammonia is pumped into external radiators that emit heat as infrared radiation, then back to the station.[198] The EATCS provides cooling for all the US pressurised modules, including Kibō and Columbus, as well as the main power distribution electronics of the S0, S1 and P1 trusses. It can reject up to 70 kW. This is much more than the 14 kW of the Early External Active Thermal Control System (EEATCS) via the Early Ammonia Servicer (EAS), which was launched on STS-105 and installed onto the P6 Truss.[199]
Communications and computers
Main articles: Tracking and Data Relay Satellite and Luch (satellite)
See also: ThinkPad § Use in space
Diagram showing communications links between the ISS and other elements.
The communications systems used by the ISS
* Luch satellite and the Space Shuttle are not currently[when?] in use
Radio communications provide telemetry and scientific data links between the station and Mission Control Centres. Radio links are also used during rendezvous and docking procedures and for audio and video communication between crew members, flight controllers and family members. As a result, the ISS is equipped with internal and external communication systems used for different purposes.[200]
The Russian Orbital Segment communicates directly with the ground via the Lira antenna mounted to Zvezda.[6][201] The Lira antenna also has the capability to use the Luch data relay satellite system.[6] This system fell into disrepair during the 1990s, and so was not used during the early years of the ISS,[6][202][203] although two new Luch satellites—Luch-5A and Luch-5B—were launched in 2011 and 2012 respectively to restore the operational capability of the system.[204] Another Russian communications system is the Voskhod-M, which enables internal telephone communications between Zvezda, Zarya, Pirs, Poisk, and the USOS and provides a VHF radio link to ground control centres via antennas on Zvezda's exterior.[205]
The US Orbital Segment (USOS) makes use of two separate radio links mounted in the Z1 truss structure: the S band (audio) and Ku band (audio, video and data) systems. These transmissions are routed via the United States Tracking and Data Relay Satellite System (TDRSS) in geostationary orbit, allowing for almost continuous real-time communications with NASA's Mission Control Center (MCC-H) in Houston.[22][6][200] Data channels for the Canadarm2, European Columbus laboratory and Japanese Kibō modules were originally also routed via the S band and Ku band systems, with the European Data Relay System and a similar Japanese system intended to eventually complement the TDRSS in this role.[22][206] Communications between modules are carried on an internal wireless network.[207]
An array of laptops in the US lab
Laptop computers surround the Canadarm2 console
UHF radio is used by astronauts and cosmonauts conducting EVAs and other spacecraft that dock to or undock from the station.[6] Automated spacecraft are fitted with their own communications equipment; the ATV uses a laser attached to the spacecraft and the Proximity Communications Equipment attached to Zvezda to accurately dock with the station.[208][209]
The ISS is equipped with about 100 IBM/Lenovo ThinkPad and HP ZBook 15 laptop computers. The laptops have run Windows 95, Windows 2000, Windows XP, Windows 7, Windows 10 and Linux operating systems.[210] Each computer is a commercial off-the-shelf purchase which is then modified for safety and operation including updates to connectors, cooling and power to accommodate the station's 28V DC power system and weightless environment. Heat generated by the laptops does not rise but stagnates around the laptop, so additional forced ventilation is required. Laptops aboard the ISS are connected to the station's wireless LAN via Wi-Fi, which connects to the ground via Ku band. This provides speeds of 10 Mbit/s download and 3 Mbit/s upload from the station, comparable to home DSL connection speeds.[211][212] Laptop hard drives occasionally fail and must be replaced.[213] Other computer hardware failures include instances in 2001, 2007 and 2017; some of these failures have required EVAs to replace computer modules in externally mounted devices.[214][215][216][217]
The operating system used for key station functions is the Debian Linux distribution.[218] The migration from Microsoft Windows was made in May 2013 for reasons of reliability, stability and flexibility.[219]
In 2017, an SG100 Cloud Computer was launched to the ISS as part of OA-7 mission.[220] It was manufactured by NCSIST and designed in collaboration with Academia Sinica, and National Central University under contract for NASA.[221]
Operations
Expeditions and private flights
See also the list of International Space Station expeditions (professional crew), space tourism (private travellers), and the list of human spaceflights to the ISS (both).
Zarya and Unity were entered for the first time on 10 December 1998.
Soyuz TM-31 being prepared to bring the first resident crew to the station in October 2000
ISS was slowly assembled over a decade of spaceflights and crews
Each permanent crew is given an expedition number. Expeditions run up to six months, from launch until undocking, an 'increment' covers the same time period, but includes cargo ships and all activities. Expeditions 1 to 6 consisted of 3 person crews, Expeditions 7 to 12 were reduced to the safe minimum of two following the destruction of the NASA Shuttle Columbia. From Expedition 13 the crew gradually increased to 6 around 2010.[222][223] With the arrival of the US Commercial Crew vehicles in the late 2010s, expedition size may be increased to seven crew members, the number ISS is designed for.[224][225]
Gennady Padalka, member of Expeditions 9, 19/20, 31/32, and 43/44, and Commander of Expedition 11, has spent more time in space than anyone else, a total of 878 days, 11 hours, and 29 minutes.[226] Peggy Whitson has spent the most time in space of any American, totalling 665 days, 22 hours, and 22 minutes during her time on Expeditions 5, 16, and 50/51/52.[227]
Travellers who pay for their own passage into space are termed spaceflight participants by Roscosmos and NASA, and are sometimes referred to as space tourists, a term they generally dislike.[note 1] All seven were transported to the ISS on Russian Soyuz spacecraft. When professional crews change over in numbers not divisible by the three seats in a Soyuz, and a short-stay crewmember is not sent, the spare seat is sold by MirCorp through Space Adventures. When the space shuttle retired in 2011, and the station's crew size was reduced to 6, space tourism was halted, as the partners relied on Russian transport seats for access to the station. Soyuz flight schedules increase after 2013, allowing 5 Soyuz flights (15 seats) with only two expeditions (12 seats) required.[233] The remaining seats are sold for around US$40 million to members of the public who can pass a medical exam. ESA and NASA criticised private spaceflight at the beginning of the ISS, and NASA initially resisted training Dennis Tito, the first person to pay for his own passage to the ISS.[note 2]
Anousheh Ansari became the first Iranian in space and the first self-funded woman to fly to the station. Officials reported that her education and experience make her much more than a tourist, and her performance in training had been "excellent."[234] Ansari herself dismisses the idea that she is a tourist. She did Russian and European studies involving medicine and microbiology during her 10-day stay. The documentary Space Tourists follows her journey to the station, where she fulfilled "an age-old dream of man: to leave our planet as a "normal person" and travel into outer space."[235]
In 2008, spaceflight participant Richard Garriott placed a geocache aboard the ISS during his flight.[236] This is currently the only non-terrestrial geocache in existence.[237] At the same time, the Immortality Drive, an electronic record of eight digitised human DNA sequences, was placed aboard the ISS.[238]
Orbit
Graph showing the changing altitude of the ISS from November 1998 until November 2018
Animation of ISS orbit from 14 September 2018 to 14 November 2018. Earth is not shown.
The ISS is maintained in a nearly circular orbit with a minimum mean altitude of 330 km (205 mi) and a maximum of 410 km (255 mi), in the centre of the thermosphere, at an inclination of 51.6 degrees to Earth's equator. This orbit was selected because it is the lowest inclination that can be directly reached by Russian Soyuz and Progress spacecraft launched from Baikonur Cosmodrome at 46° N latitude without overflying China or dropping spent rocket stages in inhabited areas.[239][240] It travels at an average speed of 27,724 kilometres per hour (17,227 mph), and completes 15.54 orbits per day (93 minutes per orbit).[2][14] The station's altitude was allowed to fall around the time of each NASA shuttle flight to permit heavier loads to be transferred to the station. After the retirement of the shuttle, the nominal orbit of the space station was raised in altitude.[241][242] Other, more frequent supply ships do not require this adjustment as they are substantially higher performance vehicles.[28][243]
Orbital boosting can be performed by the station's two main engines on the Zvezda service module, or Russian or European spacecraft docked to Zvezda's aft port. The ATV is constructed with the possibility of adding a second docking port to its aft end, allowing other craft to dock and boost the station. It takes approximately two orbits (three hours) for the boost to a higher altitude to be completed.[243] Maintaining ISS altitude uses about 7.5 tonnes of chemical fuel per annum[244] at an annual cost of about $210 million.[245]
Orbits of the ISS, shown in April 2013
The Russian Orbital Segment contains the Data Management System, which handles Guidance, Navigation and Control (ROS GNC) for the entire station.[246] Initially, Zarya, the first module of the station, controlled the station until a short time after the Russian service module Zvezda docked and was transferred control. Zvezda contains the ESA built DMS-R Data Management System.[247] Using two fault-tolerant computers (FTC), Zvezda computes the station's position and orbital trajectory using redundant Earth horizon sensors, Solar
Francisco Sá Carneiro Airport. Maia - Portugal
Olympus XA2 + Fujichrome Velvia 50 (Expired April 2004)
(all the parts are grouped separately)
Includes stock, trigger, handgaurd, shotgun shell, and carry handle/sights
Another master component finished this afternoon, each kit will require two of these so I'll be making multiple moulds from the one master.
The comparison between my new master and the original MPC piece is .....noticeable!
Some background:
The VF-1 was developed by Stonewell/Bellcom/Shinnakasu for the U.N. Spacy by using alien Overtechnology obtained from the SDF-1 Macross alien spaceship. Its production was preceded by an aerodynamic proving version of its airframe, the VF-X. Unlike all later VF vehicles, the VF-X (sometimes referred to as VF-X1) was strictly a conventional/non-transformable jet aircraft, even though it incorporated many structural components and several key technologies that were vital for the transformable VF-1’s successful development that ran in parallel. Therefore, the VF-X was never intended as an air superiority fighter, but rather a flight-capable analogue test bed and proof of concept for the VF-1’s basic layout and major components. In this role, however, the VF-X made vital contributions to systems’ development that were later incorporated into the VF-1’s serial production and sped the program up considerably.
VF-X production started in early 2006, with four airframes built. The flight tests began in February 2007. The first prototype (“01”) was piloted and evaluated by ace pilot Roy Fokker, in order to explore the aircraft’s flight envelope, general handling and for external stores carriage tests. The three other VF-Xs successively joined the test program, each with a different focus. “02” was primarily tasked with the flight control and pilot interface program, “03” was allocated to the engine, vectoring thrust and steering systems development, and “04” was primarily involved in structural and fatigue tests.
In November 2007, the successful VF-X tests and the flights of the VF-X-1 (the first fully transformable VF-1 prototype, which had been under construction in parallel to the VF-X program) led to formal adoption of the “Valkyrie” variable fighter by the United Nations Government.
The space-capable VF-1's combat debut was on February 7, 2009, during the Battle of South Ataria Island - the first battle of Space War I - and remained the mainstay fighter of the U.N. Spacy for the entire conflict.
Introduced in 2008, the VF-1 proved to be an extremely capable craft, successfully combating a variety of Zentraedi mecha, even in most sorties which saw UN Spacy forces significantly outnumbered. The versatility of the Valkyrie design enabled the variable fighter to act as both large-scale infantry and as air/space superiority fighter. The signature skills of U.N. Spacy ace pilot Maximilian Jenius exemplified the effectiveness of the variable systems as he near-constantly transformed the Valkyrie in battle to seize advantages of each mode as combat conditions changed from moment to moment.
The basic VF-1 was deployed in four sub-variants (designated A, D, J, and S) and its success was increased by continued development of various enhancements. These included the GBP-1S "Armored Valkyrie” external armor and infantry weapons pack, so-called FAST Packs for "Super Valkyries” for orbital use, and the additional RÖ-X2 heavy cannon pack weapon system for the VF-1S “Strike Valkyrie” with additional firepower.
After the end of Space War I, the VF-1 continued to be manufactured both in the Sol system and throughout the UNG space colonies. Although the VF-1 would eventually be replaced as the primary Variable Fighter of the U.N. Spacy by the more capable, but also much bigger, VF-4 Lightning III in 2020, a long service record and continued production after the war proved the lasting worth of the design.
The VF-1 was without doubt the most recognizable variable fighter of Space War I and was seen as a vibrant symbol of the U.N. Spacy even into the first year of the New Era 0001 in 2013. At the end of 2015 the final rollout of the VF-1 was celebrated at a special ceremony, commemorating this most famous of variable fighters. The VF-1 Valkryie was built from 2006 to 2013 with a total production of 5,459 VF-1 variable fighters with several variants (VF-1A = 5,093, VF-1D = 85, VF-1J = 49, VF-1S = 30, VF-1G = 12, VE-1 = 122, VT-1 = 68), and several upgrade programs were introduced.
The fighter remained active in many second line units and continued to show its worthiness years later, e. g. through Milia Jenius who would use her old VF-1 fighter in defense of the colonization fleet - 35 years after the type's service introduction.
General characteristics:
Accommodation: One pilot in a Marty & Beck Mk-7 zero/zero ejection seat
Length 14.23 meters
Wingspan 14.78 meters (at 20° minimum sweep)
Height 3.84 meters
Empty weight: 13.25 metric tons
Standard T-O mass: 18.5 metric tons
Power Plant:
2x Shinnakasu Heavy Industry/P&W/Roice FF-2001 thermonuclear reaction turbine engines, output 650 MW each, rated at 11,500 kg in standard or in overboost (225.63 kN x 2)
4 x Shinnakasu Heavy Industry NBS-1 high-thrust vernier thrusters (1 x counter reverse vernier thruster nozzle mounted on the side of each leg nacelle/air intake, 1 x wing thruster roll control system on each wingtip);
Performance:
Top speed: Mach 2.71 at 10,000 m; Mach 3.87 at 30,000+ m
Thrust-to-weight ratio: empty 3.47; standard T-O 2.49; maximum T-O 1.24
Armament:
None installed, but the VF-X had 4x underwing hard points for a wide variety of ordnance, plus a ventral hardpoint for a Howard GU-11 55 mm three-barrel Gatling gun pod with 200 RPG, fired at 1,200 rds/min or other stores like test instruments
The model and its assembly:
Another submission to the “Prototypes” group build at whatifmodelers.com in July 2020. Being a VF-1 fan (and have built maybe twenty o these simple Arii kits), adding a VF-X was, more or less, a must – even more so because I had a suitable Valkyrie Fighter kit at hand for the conversion. As a side note, I have actually built something quite similar from a VF-1D many years ago: a fictional, non-transformable advanced trainer, without knowing about the VF-X at all.
Thanks to the “Macross - Perfect Memory” source book, the differences between the transformable VF-1 and its early testbed were easy to identify:
- Fixed legs with faired ducts from the intakes on (thighs)
- Ankle recesses disappeared
- Less and slightly different panel lines on the back and on the nose
- ventral head unit deleted and a respective fairing installed instead
- Levelled underside (shoulder fairings of the folded arms were cut down)
- Leg attachment points on the nose deleted
- No small, circular vernier thrusters all around the hull
- Some new/different venting grills (created mostly with 0.5mm black decal stripes)
Beyond the changes, the VF-1A was basically built OOB. Thankfully, the VF-X already features the later VF-1’s vectored thrust nozzles/feet, so that no changes had to be made in this respect. A pilot figure was added to the cockpit for the beauty pics, and after the flight scenes had been shot, the canopy remained open on a swing arm for static display. For the same reason, the model was built with the landing gear extended.
As a test aircraft, the underwing pylons and their AMM-1 ordnance were left away and the attachment points hidden with putty. I also omitted the ventral gun pod and left the aircraft clean. However, for the flight scene pictures, I implanted an adapter for a display holder made from wire.
In order to emphasize the test vehicle character of the VF-X, I gave the model a scratched spin recovery parachute installation between the fins, using a real world F-22 testbed as benchmark. It consists of styrene profiles, quite a delicate construction. For the same reason I gave the VF-X a long sensor boom on the nose, which changes the Valkyrie’s look, too. Finally, some small blade antennae were added to the nose and to the spine behind the cockpit.
Painting and markings:
To be honest, I have no idea if there was only a single VF-X prototype in the Macross universe, or more. Just one appears in the TV series in episode #33, and lack of suitable information and my personal lack of Japanese language proficiency prevents any deeper research. However, this would not keep me from inventing a personal interpretation of the canonical VF-X, especially because I do not really like the original livery from the TV series: an overall light grey with some simple black trim and “TEST” written on the (fixed) legs. Yamato did an 1:60 scale toy of the VF-X, but it was/is just a VF-1 with a ventral fairing; they added some shading to the basic grey – but this does not make the aircraft more attractive, IMHO.
When I looked at the original conceptual drawing of the VF-X in the “Macross - Perfect Memory” source book, however, I was immediately reminded of the F-15 prototypes from the Seventies (and this program used a total of twelve machines!). These featured originally a light grey (FS 36375?) overall base, to which bright dayglo orange markings on wings, fins and fuselage were soon added – in a very similar pattern to the VF-X. I think the VF-X livery was actually inspired by this, the time frame matches well with the production of the Macross TV series, too, and that’s what I adapted for my model.
In order to come close to the F-15 prototype livery, I gave “my” VF-X an overall basic coat of RAL 7047 “Telegrau 4”, one of German Telekom’s corporate colors and a very pale grey that can easily be mistaken for white when you do not have a contrast reference.
The cockpit received a medium grey finish, the ejection seat became black with brown cushions; the pilot figure is a 1:100 seated passenger from an architecture supplies, painted like an early VF-1 pilot in a white/blue suit. The jet nozzles/feet were painted with Revell 91 (Iron) and later treated with grinded graphite for a more metallic finish. The landing gear became classic white (I used Revell 301, which is a very pure tone, as contrast to the RAL 7047 on the hull), the air intake ducts and the internal sections of the VG wings were painted with dark grey (Revell 77).
For some diversity I took inspiration from the Yamato VF-X toy and added slightly darker (Humbrol 166, RAF Light Aircraft Grey) areas to the hull and the legs. Next, the panel lines were emphasized through a thinned black ink wash, but I did no panel post shading so that the VF-X would not look too dirty or worn.
Onto this basis I applied the orange dayglo markings. On the wings and fins, these were painted – they were applied with spray paint from a rattle can, involving lots of masking. The leading edges on wings and fins were created with grey decal sheet material, too. At this stage, some surface details and more fake panel lines were added with a soft pencil.
The orange cheatline under the cockpit is a personal addition; I found that some more orange had to be added to the nose for visual balance, and I eventually went for the simple, trimmed stripe (TL Modellbau material) instead of trying to apply decal sheet material around the jagged air intakes (F-15 prototype style). The black “TEST”, “VFX” and “U.N. Spacy” markings were designed at the computer and printed on clear inkjet decal paper. Even though the “real” VF-X does not feature the UNS “kite” insignia, I decided to add them to the model. These come from the OOB sheet, which also provided most (slightly yellowed) stencils.
Finally, the model was sealed with a coat of matt acrylic varnish (Italeri).
A rather different VF-1 project (and it is – to my astonishment – #28 in my 1:100 VF-1 Fighter mode collection!!!), with more changes to the basic model kit than one might expect at first sight. VF-X and VF-1 differ considerably from each other, despite identical outlines! However, I like the outcome, and I think that going a different route from the canonical grey/black livery paid out, the bright orange markings really make this VF-X stand out, and it looks IMHO more like a testbed than the “real” aircraft from the TV series.
The Space Shuttle orbiter is the spaceplane component of the Space Shuttle, a partially reusable orbital spacecraft system that was part of the discontinued Space Shuttle program. Operated from 1977 to 2011 by NASA, the U.S. space agency, this vehicle could carry astronauts and payloads into low Earth orbit, perform in-space operations, then re-enter the atmosphere and land as a glider, returning its crew and any on-board payload to the Earth.
Six orbiters were built for flight: Enterprise, Columbia, Challenger, Discovery, Atlantis, and Endeavour. All were built in Palmdale, California, by the Pittsburgh, Pennsylvania-based Rockwell International company. The first orbiter, Enterprise, made its maiden flight in 1977. An unpowered glider, it was carried by a modified Boeing 747 airliner called the Shuttle Carrier Aircraft and released for a series of atmospheric test flights and landings. Enterprise was partially disassembled and retired after completion of critical testing. The remaining orbiters were fully operational spacecraft, and were launched vertically as part of the Space Shuttle stack.
Columbia was the first space-worthy orbiter; it made its inaugural flight in 1981. Challenger, Discovery, and Atlantis followed in 1983, 1984, and 1985 respectively. In 1986, Challenger was destroyed in an accident shortly after its 10th launch. Endeavour was built as Challenger's successor, and was first launched in 1992. In 2003, Columbia was destroyed during re-entry, leaving just three remaining orbiters. Discovery completed its final flight on March 9, 2011, and Endeavour completed its final flight on June 1, 2011. Atlantis completed the final Shuttle flight, STS-135, on July 21, 2011.
In addition to their crews and payloads, the reusable orbiter carried most of the Space Shuttle System's liquid-propellant rocket system, but both the liquid hydrogen fuel and the liquid oxygen oxidizer for its three main rocket engines were fed from an external cryogenic propellant tank. Additionally, two reusable solid rocket boosters (SRBs) provided additional thrust for approximately the first two minutes of launch. The orbiters themselves did carry hypergolic propellants for their Reaction Control System (RCS) thrusters and Orbital Maneuvering System (OMS) engines.
Wikipedia: <a href="https://en.wikipedia.org/wiki/Space_Shuttle_orbiter" rel="noreferrer nofollow">en.wikipedia.org/wiki/Space_Shuttle_orbiter</a>