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3D Space Rendering by VisionaryFX™, LLC.
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Full-scale model of the International Space Station
Space Vehicle Mock-up Facility
Johnson Space Center, Houston, Texas
This image captures several important targets of the Cassini mission:
icy moons, rings, and the gaps in the rings that may contain small
undiscovered moons.
Mimas (398 kilometers, or 247 miles across) is easily seen near lower
right. Epimetheus (116 kilometers, or 72 miles across) is visible left
of center.
The 4,800-kilometer- (2,980-mile-) wide Cassini division is the dark
swath at upper left. The Encke Gap (325 kilometers, or 202 miles wide)
is visible as a dark curve near the edge of the A ring. The thin F ring
is seen here, exterior to the main rings.
The image was taken in visible light with the Cassini spacecraft narrow
angle camera on Sept. 10, 2004, at a distance of 8.9 million kilometers
(5.5 million miles) from Mimas and at a Sun-Mimas-spacecraft or phase,
angle of 84 degrees. The image scale is 53 kilometers (33 miles) per
pixel. The image was magnified by a factor of four to aid visibility.
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 Cassini-Huygens mission for NASA's Office of Space Science,
Washington, D.C. The Cassini orbiter and its two onboard cameras, were
designed, developed and assembled at JPL. The imaging team is based at
the Space Science Institute, Boulder, Colo.
For more information, about the Cassini-Huygens mission visit,
saturn.jpl.nasa.gov/ and the Cassini imaging team home page,
credit: NASA/JPL/Space Science Institute
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.
Dedicated to my dad, who loved the Tom Swift novels.
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A front view of the main hanger/control module.
The floor will have dark bluishgrey tile (on order). I didn't quite like the dark red. I might use those for the reactor/generator building.
Eventually there will be installed internal LED lighting via the conduits and access hatch in the center. I'd like to use a keychain LCD photo player for the main viewer in there.
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
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
Note the angle of the "burn marks" you can see how steep the orbiter reenters the Earth's atmosphere.