[FPSPACE] Fwd: Cassini Spies Bright Venus From Saturn Orbit

LARRY KLAES ljk4 at msn.com
Mon Mar 4 14:30:23 EST 2013



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-----Original Message-----
From: NASA Jet Propulsion Laboratory
Sent: 3/4/2013 6:34:20 PM
To: Larry Klaes
Subject: Cassini Spies Bright Venus From Saturn Orbit
[http://www.kintera.org/atf/cf/{127BCCB8-B18B-48EC-86CC-B465A792975E}/NASA-NEWS-600-1172.GIF]

Image advisory: 2013-079                                                                    March. 4, 2013

Cassini Spies Bright Venus From Saturn Orbit

[http://www.jpl.nasa.gov/images/cassini/20130304/pia14935-640.jpg]<http://www.jpl.nasa.gov/news/news.php?release=2013-079&cid=release_2013-079img>

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-079&cid=release_2013-079

PASADENA, Calif. - A distant world gleaming in sunlight, Earth's twin planet, Venus, shines like a bright beacon in images taken by NASA's Cassini spacecraft in orbit around Saturn.

One special image of Venus and Saturn was taken last November when Cassini was placed in the shadow of Saturn. This allowed Cassini to look in the direction of the sun and Venus, and take a backlit image of Saturn and its rings in a particular viewing geometry called "high solar phase." This observing position reveals details about the rings and Saturn's atmosphere that cannot be seen in lower solar phase.

One of the Venus and Saturn images being released today is a combination of separate red, green and blue images covering the planet and main rings and processed to produce true color. Last December, a false-color version of the mosaic was released.

Another image, taken in January, captures Venus just beyond the limb of Saturn and in close proximity to Saturn's G ring, a thin ring just beyond the main Saturnian rings. The diffuse E ring, which is outside the G ring and created by the spray of the moon Enceladus, also is visible.

These images can be found at http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA14935 and http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA14936.

Venus is, along with Mercury, Earth and Mars, one of the rocky "terrestrial" planets in the solar system that orbit relatively close to the sun. Though Venus has an atmosphere of carbon dioxide that reaches nearly 900 degrees Fahrenheit (500 degrees Celsius) and a surface pressure 100 times that of Earth's, it is considered a twin to our planet because of their similar sizes, masses, rocky compositions and close orbits. It is covered in thick sulfuric acid clouds, making it very bright.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team consists of scientists from the U.S., England, France and Germany. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information, visit http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov .

Jia-Rui Cook 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
jccook at jpl.nasa.gov

Steve Mullins 720-974-5859
Space Science Institute, Boulder, Colo.
media at ciclops.org


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