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|Picture taken on April 27 show a Martian polar storm more than 1,000 miles (1,600 km) across. The residual north polar water-ice cap is at top. A belt of clouds can be seen in the planet's equatorial regions and northern mid-latitudes, as well as in the southern polar regions. The volcano Ascraeus Mons can be seen as a dark spot poking above the cloud deck. Credit: Jim Bell, Steve Lee, Mike Wolff and NASA A high-resolution version of this photo is available from the Hubble web site. Follow the link at the bottom of this story.|
The system is similar to so-called "spiral" storms observed more than 20 years ago by NASA's Viking Orbiter spacecraft, but it is nearly three times as large as the largest previously detected Martian spiral storm system. The storm is nearly 1,100 miles across from east to west and 900 miles from north to south. The eye of the storm is nearly 200 miles in diameter. The system is larger than the planet's residual north polar ice cap, and is comparable in size to similarly shaped terrestrial hurricanes.
The storm was detected using the Hubble's Wide Field Planetary Camera-2 by a team of astronomers observing Mars near its closest approach to Earth in nearly eight years. Jim Bell, assistant professor of astronomy at Cornell University, principal investigator on the team of astronomers obtaining and analyzing the Hubble images, says the observations were somewhat serendipitous in that they were made during the same season that the storms were first detected by Viking.
"These rapidly growing and decaying systems do appear to be typical of the Martian polar weather at this season, which is mid northern summer," says Bell. "The storm we detected from Hubble appears anomalous because of its size, but I wouldn't be surprised if the Mars Global Surveyor spacecraft sees other storms of this size eventually as well."
The storm consists of at least three, and perhaps more, bands of clouds organized into a spiral structure and wrapped counterclockwise around a hollow central core or "eye." The storm appeared in the middle of the Martian northern hemisphere's summer season, after the planet's seasonal carbon dioxide polar cap had completely sublimated away, leaving only the underlying residual water-ice cap. The smaller spiral storms seen previously by Viking were also detected during the northern summer season, and also at high northern latitudes.
|View of the Martian north polar region shows the location of the storm relative to the bright and dark features in this area. The data indicate that the storm is fairly dust-free and therefore likely composed mostly of water-ice clouds. The bright surface region beneath the eye of the storm can be seen clearly. Credit: Jim Bell, Steve Lee, Mike Wolff and NASA A high-resolution copy of this photo is available from the Hubble web site. Follow the link at the end of this story.|
The general appearance of the Martian storm seems consistent with an intense low pressure vortex with rising air causing cloud formation, possibly with a small core that is cloud-free, like the eye of a hurricane. The storm may have been initiated by an unstable frontal system, and then amplified by the strong temperature contrast between the relatively warm high-latitude Martian dark regions and the much colder and stable polar atmosphere.
When first imaged by Hubble on April 27, 1999, the storm was located near 65 degrees north latitude and 85 degrees west longitude. When next imaged about six hours later, the storm appeared to have moved only slightly eastward, but seemed to be in the process of dissipating. The storm has not been seen again in subsequent Hubble telescope images, but these have been centered on the opposite side of the planet. The storm might have been a short-lived phenomenon, which would be consistent with the short lifetimes (several days) observed for smaller spiral storms by Viking.
"It seems that our knowledge of the high-latitude weather on Mars is limited by the fact that even Viking, from orbit 20 years ago, could not observe the polar regions very frequently," says Cornell's Bell. "So our HST finding, and forthcoming results from the Mars Global Surveyor spacecraft, may simply be revealing all this activity up there because it's the first time we've been able to look in a detailed and dedicated way with high-resolution instruments during this season."
The team of astronomers, besides Bell, operator of HST, included Michael Wolff and R. Todd Clancy (Space Telescope Science Institute), Steven Lee (University of Colorado), Philip James (University of Toledo), and Michael Ravine (Malin Space Science Systems, Inc.).
Related World Wide Web sites: The following sites provide additional information on this news release. Some might not be part of the Cornell University community, and Cornell has no control over their content or availability.
-- Pictures of the Mars cyclone from the Hubble site, with detailed captions: http://oposite.stsci.edu/pubinfo/pr/1999/22
-- Hubble Space Telescope latest observations: http://oposite.stsci.edu/pubinfo/latest
-- Hubble page with links to higher resolution digital versions (300 dpi JPEG and TIFF):