View allAll Photos Tagged deepspace

Andromeda Galaxy a.k.a. Messier 31

 

……………..............................................

 

Andromeda, the largest galaxy in the so-called Local Group of Galaxies to which our galaxy also belongs, is 2.5 million light-years away and can be seen (even with the naked eye) in the constellation Andromeda. As general information, Andromeda is about 1.5 times larger than the Milky Way, with a diameter of 220,000 light-years (compared to the Milky Way which is 120-140,000 light-years in diameter) and contains more than 2 times as many stars. Although the first mention of this celestial object dates from 960, the first to give a more detailed description was the German astronomer Simon Marius, in the 1600s.

It should also be mentioned that Andromeda and the Milky Way are approaching with about 100 miles per second, experts estimate that in about 3-4 billion years the 2 galaxies will collide and thus form a new giant galaxy.

 

Equipment and settings:

 

Mount: Skywatcher EQ6R Pro

Telescope: Skywatcher Evostar 72/420 + 0.85 reducer

Camera: ASI 533MM Pro

Filters: Astrodon LRGB+Ha

Integration: 4h40'

Edit in Pixinsight.

Location: my Bortle 6+ backyard

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Contains: M 82, Bode's nebulae, NGC 3034

M 82, Bode's nebulae, NGC 3034

M82 was previously believed to be an irregular galaxy. In 2005, however, two symmetric spiral arms were discovered in near-infrared images of M82.

 

This image was photographed at my home in Valencia.

  

Imaging telescope or lens:AG14

Mount: Software Bisque Paramount MX

 

Frames:

Chroma LRGB Ha CCD Filter set

Baader Luminance 2": 40x600" bin 2x2

Integration: 36 hours

Locations: Home observatory, Valencia, Spain

moonrocksastro.com/index.php/2016/02/26/m78-reflection-ne...

 

The nebula Messier 78 is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included by Charles Messier in his catalog of comet-like objects that same year.

M78 is the brightest diffuse reflection nebula of a group of nebulae that include NGC 2064, NGC 2067 and NGC 2071. This group belongs to the Orion Molecular Cloud Complex and is about 1,600 light years distant from Earth. M78 is easily found in small telescopes as a hazy patch and involves two stars of 10th magnitude. These two stars, HD 38563A and HD 38563B, are responsible for making the cloud of dust in M78 visible by reflecting their light.

 

Ha x 1800 x 4 Lume x 600x 40 RGB x 10 x 30 plus close up data from last year.

 

Imaging telescope or lens: Vixen VSD

Imaging camera: Starlight Express SXVR-H18

Mount: Sky-Watcher NEQ6 and Pro Paramount MX

Guiding telescope or lens: Vixen VSD

Software: Sequence Generator Pro

Filter: Baader H-alpha 3.5 Nm pluss Baader RGBL

Accessory: Starlight Xpress Lodestar Guider

Messier 42 (M42, the Great Orion Nebula, and Running Man Nebula. Shot with my one-shot color camera with no color adulteration.

Technical Info:

50 x 300 sec. Badder UV/IR Cut filter

10 x 60 sec. Badder UV/IR Cut filter

10 x 30 sec Badder UV/IR Cut filter

Explore Scientific 102mm f/7 Imaging APO Refractor

Sensor cooled to -5°C on my ZWO ASI2490 MC Pro

Calibration frames: Bias, Darks and Flats.

Plate solving- PlateSolver 2 via N.I.N.A.

Image stacking with DeepSkyStacker and finished in Photoshop

The Orion Nebula and the Running Man Nebula must be the most imaged nebulas in the night sky. In this project I wanted to get the surrounding dust and gasses that are not normally seen in most wide field Orion Nebula images. To be able to capture the faint dust and the super bright core and everything in-between I took a set of 3 different exposures to create an HDR image. The image required using a masked stretch of 300 iterations to be able to compress all the details into a workable image.

 

More information can be found at: astrob.in/afonwi/0/

 

Detail Summary:

Imaged from Gérgal, Spain on the 22 December 2022

Bortle class 4-5

SQM 20.6 - 20.9

 

WO GT81 385mm Telescope f/4.7

CGX Mount

ASI 2600MC Pro -5C Imaging Camera

Baader Moon & Sky Glow filter

 

Total imaging time 5 hours:

36x 30s Gain 0 : 18 mins

36x 180s Gain 0 : 1 hour 48 mins

36x 300s Gain 100 : 3 hours

Beautiful Milky Way as I saw it rising above Diskit in Himalayas, a luminous river of countless stars.

Like three years ago, starting the new season with a wonderful and enchanting Hubble's Variable Nebula (NGC 2261)

Previous approach: www.flickr.com/photos/olegbr/8552071862/in/dateposted/

I wanted to personally check whether it still variable ...

It was found that this is so :)

 

Here animation L-channel 200%: olegbr.astroclub.kiev.ua/files/astrofoto/NGC2261/NGC2261_...

 

Of course, 3 years - a very large interval for observing the changes in the nebula. Everything is much faster: www.umanitoba.ca/science/astronomy/cbrown/imaging/hvn/ana...

 

In 2013-2016 animation, I drew attention to the star just above the nebula, which is for 3 years significantly shifted to the right.

To heighten the effect, combined with the current picture image DSS., For about 60 years, the offset is already pretty decent. olegbr.astroclub.kiev.ua/files/astrofoto/NGC2261/NGC2261_...

 

Here www.astrosurf.com/mcianci/ngc2261.html Italian colleague calculated that the proper motion (proper motion) of the star 0.2" per year. The name is NLTT 16798 and is listed as High Proper Motion Star: simbad.u-strasbg.fr/simbad/sim-id?Ident=NLTT+16798

 

Explanation: What causes Hubble's Variable Nebula to vary? The unusual nebula pictured above changes its appearance noticeably in just a few weeks. Discovered over 200 years ago and subsequently cataloged as NGC 2661, the remarkable nebula is named for Edwin Hubble, who studied it earlier this century. Hubble's Variable Nebula is a reflection nebula made of gas and fine dust fanning out from the star R Monocerotis. The faint nebula is about one light-year across and lies about 2500 light-years away towards the constellation of Monocerotis. A leading variability explanation for Hubble's Variable Nebula holds that dense knots of opaque dust pass close to R Mon and cast moving shadows onto the reflecting dust seen in the rest of the nebula. (text:http://apod.nasa.gov/apod/ap991020.html)

 

This picture was photographed during 4 and 6 February 2016 in Khlepcha observatory, Ukraine.

 

Equipment: home assembled reflector 10 in., f/3.8

Mount WhiteSwan-180 with a control system «Eqdrive Standart», camera QSI-583wsg, Televue Paracorr-2. Off-axis guidecamera QHY5L-II.

LRGB filter set Baader Planetarium.

 

L = 29 * 600 seconds , bin.1, RGB = 11 * 300-450 seconds, bin.2 each filter. About 8 hours.

 

FWHM source in L filter 2.10"-2.97", sum in L channel - 2.55"

 

The height above the horizon from 40° to 48°, the scale of 1"/ pixel.

 

Processed Pixinsight 1.8 and Photoshop CS6

M45 The Pliedies also known as The Seven Sisters is an asterism and an open star cluster in the constellation Taurus. M45 is at a distance of about 444 light years and is the nearest star cluster to Earth.

Apologies for the same type of shot two night's on the bounce but once I have an idea I'm like a dog with a rat :)

 

Same rig up as yesterday, minus stars and el wire plus sun.

 

I made the sun from a ping pong ball, under lit by the lp brushes orange filter.

 

I used a nd filter held over the bottom half of the sun to begin so the rings would show up better in front.

 

Quick tripod swap then onto the rings which appear to disappear behind the sun as I span my phone quicker on the top 1/4 of it's rotation. I made them more pronounced in front by moving the phone more slowly.

 

Straight out the camera deep space light art.

This image is a mosaic of three panels. M 81 and m82 shot using a 14" Newtonian from the home in Valencia.

This image Contains: M81 and it's companion dwarf galaxy Holmberg IX, NGC 3034 and M 82.

M81 and M82 are a pair of galaxies in the constellation Ursa Major. Messier 81 and Messier 82 can both be viewed easily using binoculars and small telescopes.

Imaging telescope or lens:AG14

Mount: Software Bisque Paramount MX

Frames:

Chroma LRGB & Ha CCD Filter set

Integration: +- 36 hours x 3

Locations: Home observatory, Valencia,

Spain

#Astrophotography #Space

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Ou4 the Giant Squid Nebula, Data in from last night 1800 x 14 at F3

Ha Tonight! Looking at the individual subs there is not much to see but when they are all stacked and treated the elusive squid begins to reveal it's self.

Per la morte non c'è spazio, ma le vite volano e si aggiungono alle stelle

nell'alto cielo.

 

Publio Virgilio Marone poeta romano 70-19 a.C.

 

Si dice che la nostra galassia contenga più o meno 100 miliardi di stelle... e si calcola che questo numero sia paragonabile a quello degli esseri umani esistiti nei circa 200.000 anni di evoluzione dell'uomo moderno.

C'è una stella per ciascuno...e quando si guarda la via lattea in una notte perfetta, questo pensiero diventa ancora più profondo.

 

Foto scattata con obbiettivo fish eye, isola di La Rèunion.

 

#stelle #reunion #astronomy #alberi #foglie #nuvole #clouds #mankind #stars #200miliardi #billions #life #death #deep #deepspace

DESCRIPTION: Very nice target for smaller telescopes and camera lenses. I am surprised of data quality because I was shooting during astronomical twilight and nebulae were only approx 15° above south light polluted horizon… All comments are welcome, you can be critique and please constructive.

  

OBJECT: M 8 The Lagoon Nebula, M 20 The Trifid Nebula, Constelation Sagittarius, M8 apparent magnitude 6, apparent dimension 90’ x 40’, M20 apparent magnitude 6,3, apparent dimension 28’ x 28’, FOV 2,7° x 1,8°.

  

GEAR: Nikon Z7 Kolari Full Spectrum + Nikkor 500/5,6 PF, Astronomic UV/IR/L2 Clip in filter, Rollei Astroklar light pollution filter, Dew heater strip, sensor pixel scale 1,79 arcsec/px, tracking mount iOptron CEM60EC - 3 star alignment, no auto guiding.

  

ACQUISITION: July 3-4, 2021, Struz, CZ, Subexposure 180s, f 5,6, ISO 640, Interval 15 s, RAW-M, Light 19x, Dark 20x, Bias 20x, Flat 20x, DarkFlats 10x. Total exposure time 57 min. Astronomical twilight, no wind, 9°C, No Moon, Light polluted backyard - Bortle 5.

  

STACKING AND POST PROCESSING: AstroPixelProcessor (stacking, background neutralization, light pollution removal, calibrate background) , Adobe Photoshop CC 2020 ( black and white point settings, stretching, dim stars, enhance DSO, contrast setting, no noise reduction). Cropped 2,3x x, image size 3840 x 2560 px.

 

Photo showing Turbulence at the Ars Electronica Center’s Deep Space 8K.

 

Turbulence is an ongoing series of high-resolution visual experiments with particles simulated in various virtual environments by the award-winning interdisciplinary studio MELT. The three-part work was created exclusively for the Ars Electronica Center's Deep Space 8K.

An LRGB image of M92 Globular Cluster.

A total of 300 minutes exposure using a StellaMira 104m Refractor mounted on a 10 Micron GM1000 mount.

IC434 Horsehead Nebula and NGC 2024 are located in the constellation of Orion. The bright star to the left of the horsehead is Alnitak, the first of the three stars that make up Orions belt. This image was made up of a combination of Red Green and Blue using a colour camera with a UV/IR filter and the Red channel of a narrowband filter to enhance the hydrogen gas in the nebula.

 

Imaged from my home in Gergal, Spain over 6 nights in January and February 2023.

 

Full imaging details and a high resolution image are available at astrob.in/full/jssebn/0/

 

Imaging summary:

 

Location: Gergal, Spain

Scope: William Optics GT 81

Camera: ZWO ASI2600MC Pro

Mount: Sky-Watcher EQ6-R Pro

Filters: ZWO UV/IR Cut, Optolong L-Ultimate Dual Narrowband

Integration: 170x 600s L-Ultimate, 229x 60s UV/IR

Total Integration: 15h 29m

It is finished! I have been slowly trying to learn deep-space photography using my camera, a telephoto lens, and a star tracker. It is the most challenging type of photography that I have attempted, and the editing process on this photo nearly broke me...BUT...I got it done. This photo was taken last weekend on Sunday, September 1st into the early morning hours on Labor Day (Monday), September 2nd. This was taken a few miles northwest of Munising Michigan in the UP. This photo combines 66 minutes (33 images exposed for 2 minutes each) of exposure time. The long exposure time allows the faint galaxy light to be collected in the data captured. Photo was taken with a Nikon Z6iii, Tamron 150-600mm lens, & ioptron skyguider pro. 33 exposures set at 2 minutes long, ISO 3200, f/6.3, focal length 550mm.

 

(Explore # 230)

 

www.rossellet.com

The Medusa Nebula, also known as Abell 21, is a planetary nebula located in the constellation Gemini, about 1,500 light-years from Earth. It is the remnant of a dying star that shed its outer layers, forming a complex, glowing shell of ionized gas. Its twisted, filamentary appearance and faint greenish hue give it a resemblance to the serpent-haired figure from Greek mythology, inspiring its name.

M 42 ZWO Seestar S50 A diffuse nebula in the Milky Way south of Orions belt in the constellation of Orion. 1,500 Light years away from Earth

NGC 6960 which is commonly known as the Veil Nebula or The Witch’s Broom is the western half of the Cygnus Loop. This is a large supernova remnant in the constellation of Cygnus.

Technical Info:

197 x 300 sec. Astronomik Ha 12 nm filter

212 x 300 sec. Astronomik OIII 12 nm filter

148 x 300 sec Astronomik SII 12 nm filter

Gain 200, Offset 50, Binning 1x1

Total Integration 46.4 hours

Explore Scientific 102mm f/7 APO Refractor, Sensor cooled to -15°C on ZWO ASI1600MM Pro (mono)

Calibration frames: Bias, Darks, and Flats.

Plate Solve-PlateSolver 2 via N.IN.A. 2.0

Image processing Pixinsight 2.0 and Photoshop 2022

A slightly better shot of M31,

as I slowly improve my Astrophotography.

In un gioco di colori, in primo piano, risplendono stelle nate da pochi milioni di anni, che convertono parte della propria massa in energia, con giovanile entusiasmo. la loro luce si disperde nell'ambiente circostante andando ad influenzare l'aspetto delle nubi di colore rossastro in cui sono immerse.

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In a play of colors, in the foreground, stars, born from a few million years shine, converting part of their mass into energy, with youthful enthusiasm. their light is dispersed in the surrounding environment, influencing the appearance of the reddish clouds in which they are immersed.

SH2-124 is a faint emission nebula located in the constellation of Cygnus.

 

Imaging telescope: Vixen VSD 100 f/3

Imaging camera: 9.2mp Sony SX814

Mount: Software Bisque Paramount MX

Guiding telescope or lens: Vixen VSD 100 f/3

Filters: Chroma OIII 3nm, Chroma Ha 3nm and Chroma SII 3nm

Dates: Nov..Dec...2016

Frames: 46x1800" at F3

Integration: 45.0 hours

 

Locations: Home observatory, Valencia, Spain

A Ha-OIII-RGB composite of Messier 78 (NGC 2068) is my first attempt at this deep sky object and this type of post-processing. It was imaged in the northern hemisphere in my yard.

 

M78 is the brightest diffuse reflection nebula of a group of nebulae that includes NGC 2064, NGC 2067 and NGC 2071. This group belongs to the Orion B molecular cloud complex and is about 1,350 light-years distant from Earth.

 

Subframes

66 Light (RGB) x 300 sec

21 Ha x 300 sec

30 OIII x 300 sec

Flat x 44

Dark x 25

Bias x 78

Total time 9.75 hrs

The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated in the Milky Way, being south of Orion's Belt in the constellation of Orion. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is located at a distance of 1,344 light years approx and is the closest region of massive star formation to Earth. The M42 nebula is estimated to be 24 light years across. It has a mass of about 2000 times the mass of the Sun. Older texts frequently refer to the Orion Nebula as the Great Nebula in Orion or the Great Orion Nebula

 

The Orion Nebula is one of the most scrutinized and photographed objects in the night sky, and is among the most intensely studied celestial features.[8] The nebula has revealed much about the process of how stars and planetary systems are formed from collapsing clouds of gas and dust. Astronomers have directly observed protoplanetary disks, brown dwarfs, intense and turbulent motions of the gas, and the photo-ionizing effects of massive nearby stars in the nebula.

 

​Details

M: Avalon Linear Fast Reverse and Mesu 200

T: Takahashi FSQ85 0.73x and AT 8" RC CF

C: QSI690-wsg with 3nm Ha filter and Hutech IDAS filter, QSI683-wsg with Baader red, green and blue filters

 

14x1800s Ha (FSQ85) 16x45s Ha (FSQ85) 79x40s Ha (2x2 bin AT 8" RC)

31x600s Lum (FSQ85)

Red - 50x300s (FSQ85), 15x10s, 20x60s

Green - 50x300s (FSQ85), 15x10s, 20x60s

Blue - 50x300s (FSQ85), 15x10s, 20x60s

 

There is a total of 26 hours, 32 minutes and 10 seconds

M33 is located in the triangle-shaped constellation Triangulum, earning it the nickname the Triangulum galaxy. About half the size of our Milky Way galaxy, M33 is the third-largest member of our Local Group of galaxies following the Andromeda galaxy (M31) and the Milky Way (NASA)

 

A hybrid image using RGB and Ha data from a narrow band filter to enhance the nebulas in the galaxy.

 

More details can be viewed at: astrob.in/ap9f53/0/

 

Location: Gergal, Spain, Jan 2023

Scope: William Optics GT 81

Camera: ZWO ASI2600MC Pro

Mount: Celestron CGX

Filters: Baader Moon & Sky Glow, Optolong L-Ultimate dual narrow band

Integration: 79x 600s RGB,31x 600s NB

Total Integration: 18h 20m

The Rosette Nebula is a cluster and nebula which is at a distance of 5,000 light-years from Earth and measure roughly 130 light years in diameter. Technical Info:

49 x 120 sec. Astronomik UV/IR Cut filter

49 x 300 sec. Astronomik Ha 12nm Filter

48 x 300 sec Astronomik OIII 12nm Filter

41 x 300 sec Astronomik SII 12nm Filter

Gain 200, Offset 50, Binning 1x1

Total 14.8 hours

Explore Scientific 102mm f/7 APO Refractor

Sensor cooled to -10°C on ZWO ASI1600MM Pro (mono)

Calibration frames: Bias, Darks, and Flats.

ASTAP via N.I.N.A. 1.11

Image stacking with DeepSkyStacker 4.2.5 and finished in Photoshop CC 2021

A Bright Globular Cluster in Carina

 

2022-05-29

The Elephant's Trunk is a part of the larger nebula IC 1396. This pillar of dense star/planet forming areas is more than 20 light years long. Though it lies about 2500 light years away, if unaided human eyes were able to see it in our night sky, the Trunk would appear around the same length as a full moon. For a sense of scale, if you place our Sun next to it in this image, the Sun and all its major planets (including Earth) would fit neatly into one pixel.

 

OTA: PlaneWave CDK14

MOUNT: Planewave L350

CAMERA: SBIG STX-16803

GUIDER: Astrodon Mega MOAG

GUIDE CAMERA: Starlight Xpress UltraStar

REDUCER: N/A

SOFTWARE: Planewave PWI3 & PWI4, SGP, PhD2, Pixinsight, Photoshop, Topaz

FILTERS: Astrodon

LOCATION: SRO

COPYRIGHT: 2019 JKLOVELACE

  

SII 20 x 1200 sec;

NII 14 x 1200 sec;

Hα 24 x 1200 sec;

OIII 16 x 1200 sec;

 

Red 24 x 300 sec;

Green 24 x 300 sec;

Blue 17 x 300 sec.

 

Total integration 30.08 hours.

Binning 1x1

Camera Temp -25C

 

DSO Color Mapping: SN-HO-OH

Original Image Scale (Pix): 0.72

 

To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space

M31 NGC 224. 200,000 Lightyears Wide 2.5 Million light years from Earth with satellite galaxy M32

The Crescent Nebula is a faint emission nebula in the constellation of Cygnus, at around 5000 light-years away from Earth. Discovered by William Herschel in 1792.

 

Imaged from my backyard in Gérgal, Almería, Spain

 

8 imaging sessions 16th- 27th May 2022

Ha 66x 300s BIN 2x2 Gain 200 -10C

Oiii 257x 300s BIN 2x2 Gain 200 -10C

 

Ha 5.5 Hours

Oiii 21 Hours

 

Telescope: Celestron C11 Edge HD x0.7 f/7 @ 1960mm

Image Camera: ZWO ASI 6200MM Pro

Guiding: ZWO OAG L with ZWO ASI 192MM Mini

Filters: ZWO Ha 7nm, ZWO Oiii 7nm

Mount: Skywatcher EQ6-R Pro

Computer: PrimaLuceLab Eagle 4

 

Capture software: NINA, PHD2, Sharpcap Pro

Processing software: PixInsight, StarXterminator, NoiseXterminator, Adobe Lightroom, Topaz Sharpen AI

NGC 4565 lies at a distance of approximately 40 million light years from our own Galaxy in the constellation of Coma Berenices. Its size is approximately 162,000 light years across at the longest edge and 20, 000 light years at the centre bulge. To the lower right of NGC 4565 is the smaller galaxy NGC 4562. This small galaxy is moving away from NGC 4565 at the rate of 123,000 km per second.

 

Imaged over 3 nights from my home in Gérgal, Spain.

 

A higher resolution image with imaging details can be found on my Astrobin page at: astrob.in/full/st1ss3/0/

 

Thank you for looking.

 

Technical summary:

Captured: 22,23,25-03-2023

Imaging Sessions: 3

Location: Gérgal, Andalucía, Spain

Bortle Class: 4

 

Total Integration: 20h 30m

Filters:

Red 48x 300s 4h 00m BIN 2 Gain 100 -5C SQM 20.6

Green 48x 300s 4h 00m BIN 2 Gain 100 -5C SQM 20.5

Blue 438 300s 4h 00m BIN 2 Gain 100 -5C SQM 20.6

UV/IR 102x 300s 8h 30m BIN 2 Gain 100 -5C SQM 20.6

Pixel Scale: 0.5 arcsec/pixel

 

Telescope: Celestron C11 Edge HD f/10 2800mm

Image Camera: ZWO ASI 6200MM Pro

Guiding: ZWO OAG L with ZWO ASI 192MM Mini

Filters: Astronomik R, G, B, UV/IR

Mount: Skywatcher EQ6-R Pro

Computer: Minix NUC

 

Capture software: NINA, PHD2

Processing Software: PixInsight, Adobe Lightroom

 

From yesterday's bright sun posting to today's moon hanging is deep space...

 

Taken in August '24 with my 200-500mm telephoto lens, paired with my cropped sensor Nikon D500.

 

Enlarge for a more immersive view :)

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