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After she disappeared behind cloud cover, the sun cast a shadow of Endeavour's contrail across the sky. STS-134 Space Shuttle Endeavour's last launch. Titusville, Florida. May 16, 2011
Estival at electro space with Nat the cat
Visit this location at Electro Space - Electronic Music DJ Community & Events in Second Life
Steevz Diner is one of the most popular spots this side of Betelgeuse, with 4-quasar rated dishes, some of the hottest drinks in the galaxy (including the Pangalactic Gargle Blaster) and live music every night!
Inspired by The Resturant at the End of the Universe
This one was actually used as the backdrop for a book (kindle edition), entitled "Grace".
You can't get a sense of the detail on these unless you View On Black.
Space age science park in Singapore called Biopolis. The names of the research buildings were Nanos, Genome, Synapse etc. I visited a research group in Helios.
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Construction wall at the Ferry dock TTC side of the Seven Seas Lagoon, when I returned in October I found that a water fountain had been added here and at the other space at the TTC that was walled off at the time at the base of the ramps to the monorail station, and here too.
NASA's Spitzer Space Telescope has captured a new, infrared view of the choppy star-making cloud called M17, also known as the Omega Nebula or the Swan Nebula.
The cloud, located about 6,000 light-years away in the constellation Sagittarius, is dominated by a central group of massive stars -- the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speeding boats.
Three of these bow shocks are nestled in the upper left side of the central cavity, but are difficult to spot in this view. They are composed of compressed gas in addition to dust that glows at infrared wavelengths Spitzer can see. The smiley-shaped bow shocks curve away from the stellar winds of the central massive stars.
This picture was taken with Spitzer's infrared array camera. It is a four-color composite, in which light with a wavelength of 3.6 microns is blue; 4.5-micron light is green; 5.8-micron light is orange; and 8-micron light is red. Dust is red, hot gas is green and white is where gas and dust intermingle. Foreground and background stars appear scattered through the image.
I've been having problems with these 3 legged creeps, they look into my ships window only on dark cold nights. Lately this particular one seems to be getting a bit to aggresive, tapping on the partanium shield. It's time to take him/it out so the crosshairs of my de-plexer are as you can see, "Zeroing in for the kiLL"...
Deutsches Museum, Munich.
I can't remember what this was for sure but I think it was some kind of tape recorder associated with the (NASA?) space program.
The opposition effect, a brightness surge that is visible on Saturn's
rings when the sun is directly behind the spacecraft, is captured here as
a colorful halo of light moving across Saturn's sunlit rings.
The rainbow of color seen here is actually an artifact and a by-product of
the spot's movement and the way the color image was produced. Cassini
acquires color images by taking sequential exposures using red, green and
blue spectral filters, which are then composited together to form a color
view. The bright patch traveled across the rings between exposures taken
for this view, creating a series of three colorful spots showing its
position at three separate moments.
See PIA08247 for more information about the opposition effect. PIA08267
shows a movie sequence of the bright spot traveling across the rings.
This view looks toward the sunlit side of the rings from about 9 degrees
below the ringplane.
The images in this view were acquired with the Cassini spacecraft
wide-angle camera on June 12, 2007, at a distance of approximately 523,000
kilometers (325,000 miles) from Saturn. Image scale is 31 kilometers (19
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
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute