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Full-scale model of the International Space Station
Space Vehicle Mock-up Facility
Johnson Space Center, Houston, Texas
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Copyright: ©2012, Christian Kaden
Licence: Creative Commons BY-NC-ND 4.0
ID: IMG_7763
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This Confined Space Rescue Course is applicable to a variety of industries that have confined spaces on their worksites including but not limited to oil and gas, construction, office buildings, industrial, rail, manufacturing and any area that meets the definition of confined space.
spent a sunny day at Mission Bay. Kite flying is a must out that way. I wish I had been able to play. Must do it again, another day....
Dedicated to my dad, who loved the Tom Swift novels.
NEW from Crowabout StudioB at Deviant Scrap: Space Cadets Elements www.deviantscrap.com/shop/product.php?productid=21802&...
Space Cadets Papers www.deviantscrap.com/shop/product.php?productid=21801&...
The Cassini spacecraft delivers this stunning vista showing small,
battered Epimetheus and smog-enshrouded Titan, with Saturn's A and F
rings stretching across the scene.
The prominent dark region visible in the A ring is the Encke Gap, in
which the moon Pan and several narrow ringlets reside. Moon-driven
features that mark the A ring are easily seen to the left and right of
the Encke Gap. The Encke Gap is 325 kilometers (200 miles) wide. Pan is
26 kilometers (16 miles) across.
In an optical illusion, the narrow F ring, outside the A ring, appears to
fade across the disk of Titan. A couple of bright clumps can be seen in
the F ring.
Epimetheus is 116 kilometers (72 miles) across and giant Titan is 5,150
kilometers (3,200 miles) across.
The image was taken in visible light with the Cassini spacecraft
narrow-angle camera on April 28, 2006, at a distance of approximately
667,000 kilometers (415,000 miles) from Epimetheus and 1.8 million
kilometers (1.1 million miles) from Titan. The image captures the
illuminated side of the rings. The image scale is 4 kilometers (2 miles)
per pixel on Epimetheus and 11 kilometers (7 miles) per pixel on Titan.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
This view is part of a montage of images from the NASA Cassini and Voyager
missions shown in PIA07714. The inset image from the montage is presented
here by itself and in its original
orientation.
Cassini has observed the D-ring at much higher resolution than was
possible for Voyager, revealing surprising fine-scale structures. This
narrow-angle camera image was taken on May 21, 2005, and shows the region
between the D ring feature named D73 and the inner edge of the C-ring at
2 kilometer (1 mile) per pixel resolution. This region contains a periodic
wave-like structure with a wavelength of 30 kilometers (19 miles). The
faint horizontal bands in the image are instrumental artifacts.
The fine structure in the D-ring (visible here) could be related to
perturbations from the planet or its magnetic field. The Cassini results
provide information about the dynamics of ring particles in a new regime
-- one very close to the planet and sparsely populated by icy particles
the size of dust.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter was designed, developed and assembled at JPL.
For more information about the Cassini-Huygens mission visit saturn.jpl.nasa.gov.
For additional images visit the Cassini imaging team homepage ciclops.org.
credit: NASA/JPL/Space Science Institute
Yay! I've discovered that, at least during a full moon, 15 seconds is just enough time to achieve some long exposures in open spaces. I've been frustrated by the limitations of my little digital in regards to night photography, so I was deeply satisfied to find that I could make it work. And thanks to Graham I've discovered that i do actually have a bulb setting on my film camera (it was hiding, the sneaky thing), so now there's no stopping me!
ISO 200, f/2.8, 15sec
Smithsonian National Air and Space Museum
Steven F. Udvar-Hazy Center
Discovery was the third Space Shuttle orbiter vehicle to fly in space. It entered service in 1984 and retired from spaceflight as the oldest and most accomplished orbiter, the champion of the shuttle fleet. Discovery flew on 39 Earth-orbital missions, spent a total of 365 days in space, and traveled almost 240 million kilometers (150 million miles)--more than the other orbiters. It shuttled 184 men and women into space and back, many of whom flew more than once, for a record-setting total crew count of 251.
Because Discovery flew every kind of mission the Space Shuttle was meant to fly, it embodies well the 30-year history of U.S. human spaceflight from 1981 to 2011. Named for renowned sailing ships of exploration, Discovery is preserved as intact as possible as it last flew in 2011 on the 133rd Space Shuttle mission.
NASA transferred Discovery to the Smithsonian in April 2012 after a delivery flight over the nation's capital.
Captured by the Light L16. Photography by Amaal Said www.amaalsaid.com/
Full blog post here: captured.light.co/spaces-of-belonging
Two of Saturn's ring moons are captured in this Cassini spacecraft view,
along with the signature of another. This image was taken not long after
Prometheus passed, leaving a trail of dark gores in the inner edge of the
F ring.
Pan (26 kilometers, or 16 miles across) orbits Saturn about 4,090
kilometers (2,540 miles) closer than Atlas (32 kilometers, or 20 miles
across), meaning that Pan orbits faster, always overtaking its slower
moving sibling.
This view looks toward the unilluminated side of the rings from about 25
degrees above the ringplane. The image was taken in visible light with the
Cassini spacecraft narrow-angle camera on Jan. 23, 2008. The view was
obtained at a distance of approximately 1.8 million kilometers (1.1
million miles) from both moons. Image scale is 11 kilometers (7 miles) per
pixel.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
The Cassini imaging team homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
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Soon after World War II, the United States and the Soviet Union became locked in a global conflict pitting democracy against communism. Space became a critical theater in this Cold War, as each side competed to best the other's achievements in what became known as the Space Race.
This gallery tells about that U.S.-Soviet space rivalry and its aftermath, from the military origins of the Space Race, through the race to the Moon and the development of reconnaissance satellites, to cooperative ventures between the two former rivals and efforts to maintain a human presence in space. Some of the many highlights include a German V-1 "buzz bomb" and V 2 missile, Soviet and U.S. spacecraft and space suits, a Skylab Orbital Workshop, and a full-size test version of the Hubble Space Telescope.
This spectacular image shows Prometheus (at left) and Pandora (at right),
with their flock of icy ring particles (the F ring) between them. Pandora
is exterior to the ring, and closer to the spacecraft here. Each of the
shepherd satellites has an unusual shape, with a few craters clearly
visible.
The effect of Prometheus (102 kilometers, or 63 miles across) on the F
ring is visible as it pulls material out of the ring when it is farthest
from Saturn in its orbit. Pandora is 84 kilometers (52 miles) across.
The image was taken in polarized green light with the Cassini spacecraft
narrow-angle camera on Oct. 29, 2005, at a distance of approximately
459,000 kilometers (285,000 miles) from Pandora and 483,500 kilometers
(300,500 miles) from Prometheus. The image scale is 3 kilometers (2
miles) per pixel on Pandora and 3 kilometers (2 miles) per pixel on
Prometheus. The view was acquired from about a third of a degree below
the ringplane.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team homepage is at
credit: NASA/JPL/Space Science Institute