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Dolores Beasley
Headquarters, Washington
(Phone: 202/358-1753)

Gay Yee Hill/Spitzer; Carolina Martinez/Cassini
Jet Propulsion Laboratory, Pasadena, Calif.
(Phone: 818/354-0344/9382)

Feb. 11, 2005
RELEASE : 05-043
NASA & the Universe Send a Celestial Valentine
The candles are lit; the champagne is on ice. All you need now are flowers and a ring. This Valentine's Day, NASA's Spitzer and Cassini spacecraft provide you with both, in two intriguing new images.

And, as a valentine from the Earth, Landsat 7 gives a bird's eye view of Heart Mountain, a dramatic 8,123-foot peak just north of Cody, Wyo.

NASA's Cassini-Huygens mission and Spitzer Space Telescope have captured images of Saturn's rings and the Ring Nebula, respectively, to bring home spectacular views of two of the most looked-at objects in the sky. The Cassini image shows the most detailed color mosaic of Saturn's shimmering rings. Spitzer imaged the outer shell of the Ring Nebula, which looks surprisingly similar to the delicate petals of a camellia blossom.

Located about 2,000 light-years from Earth in the constellation Lyra, the Ring Nebula is a favorite target of amateur astronomers. Also known as Messier Object 57 and NGC 6720, it is one of the best examples of a planetary nebula, a shell of material ejected from a dying star. The "ring" is a thick cylinder of glowing gas and dust around the doomed star. As the star begins to run out of fuel, its core becomes smaller and hotter, boiling off its outer layers. The Spitzer Space Telescope's powerful infrared vision detected this material expelled from the withering star.

Previous images of the Ring Nebula taken by visible-light telescopes usually showed just the inner glowing loop of gas around the star. The outer regions are especially prominent in this new image because Spitzer sees the infrared light from hydrogen molecules. The molecules emit infrared light because they have absorbed ultraviolet radiation from the star or have been heated by the wind from the star.

Cassini's new view of Saturn's dazzling ring system, evident in a stunning natural-color mosaic, reveals the color and diversity present in this gem of the solar system. Gaps, gravitational resonances and wave patterns are all present, and the delicate color variations across the ring system are clearly visible. Named in order of discovery, the labels that scientists have assigned to the major rings do not indicate their relative positions. From the planet outward, they are known as the D, C, B, A, F, G and E rings.

The Cassini image was acquired on Dec. 12, 2004, at a distance of approximately 1.1 million miles. The Spitzer image was obtained on April 20, 2004.

Heart Mountain's summit is composed of limestone formed several hundred million years ago, but it rests on significantly younger rocks. A geological mystery lies at the core of Heart Mountain. About 50 million years ago, the Paleozoic limestone of Heart Mountain slid off the Beartooth plateau 25 miles to the west, and came to rest in its present position. Geologists continue to debate the root cause of this motion. A Landsat 7 image gives a bird's eye view of Heart Mountain's terrain.

NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif., manages the Cassini-Huygens and Spitzer Space Telescope missions for NASA's Science Mission Directorate, Washington. Landsat 7, launched in 1999, provides images of the land surface and surrounding costal regions to national and international users. The Landsat program is a partnership between NASA and the U.S. Geological Survey (USGS).

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. 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. Science operations for the Spitzer Space Telescope are conducted at the Spitzer Science Center at Caltech in Pasadena.

The new pictures are available online at

The Landsat 7 image of Heart Mountain is available at:


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