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Mars and Tharsis Main Content
NASA Center: Hubble Space Telescope Center
Image # : PR99-27B
Date : 06/30/1999

Title

Mars and Tharsis

Full Description

Taking advantage of Mars's closest approach to Earth in eight years, astronomers using NASA's Hubble Space Telescope have taken the space- based observatory's sharpest views yet of the Red Planet. The telescope's Wide Field and Planetary Camera 2 snapped these images between April 27 and May 6, when Mars was 54 million miles (87 million kilometers) from Earth. From this distance the telescope could see Martian features as small as 12 miles (19 kilometers) wide. The telescope obtained four images, which together show the entire planet. Each view depicts the planet as it completes one quarter of its daily rotation. In these views the north polar cap is tilted toward the Earth and is visible prominently at the top of each picture. The images were taken in the middle of the Martian northern summer, when the polar cap had shrunk to its smallest size. During this season the Sun shines continuously on the polar cap. Previous telescopic and spacecraft observations have shown that this summertime "residual" polar cap is composed of water ice, just like Earth's polar caps. These Hubble telescope snapshots reveal that substantial changes in the bright and dark markings on Mars have occurred in the 20 years since the NASA Viking spacecraft missions first mapped the planet. The Martian surface is dynamic and ever changing. Some regions that were dark 20 years ago are now bright red; some areas that were bright red are now dark. Winds move sand and dust from region to region, often in spectacular dust storms. Over long timescales many of the larger bright and dark markings remain stable, but smaller details come and go as they are covered and then uncovered by sand and dust. This image is centered on the region of the planet known as Tharsis, home of the largest volcanoes in the solar system. The bright, ring- like feature just to the left of center is the volcano Olympus Mons, which is more than 340 miles (550 kilometers) across and 17 miles (27 kilometers) high. Thick deposits of fine-grained, windblown dust cover most of this hemisphere. The colors indicate that the dust is heavily oxidized ("rusted"), and millions (or perhaps billions) of years of dust storms have homogenized its composition. Prominent late afternoon clouds along the right limb of the planet can be seen.

Keywords

Hubble Space Telescope HST Mars Pathfinder Viking Wide Field Planetary Camera WFPC Olympus Mons Tharsis Acidalia Elysium Syrtis Major

Subject Category

Planet-Mars, Hubble, Planetary Astronomy,

Reference Numbers

  • Center: HSTI
  • Center Number: PR99-27B
  • GRIN DataBase Number: GPN-2000-000928

Source Information

  • Creator/Photographer: NASA, Steve Lee University of Colorado, Jim Bell Cornell University,
  • Original Source: DIGITAL

Image Information ( Copyright Notification )

ResolutionFormatWidth
(Pixels)		Height
(Pixels)		Size
(KBytes)
Thumbnail .jpg 36 36 6
Small .jpg 256 256 34
Medium .jpg 600 600 125
Large .jpg 800 800 218

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