Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sistemasolare/Marte/prc9927.txt Дата изменения: Wed Jun 30 17:01:00 1999 Дата индексирования: Sat Dec 22 12:08:46 2007 Кодировка: Поисковые слова: п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п

EMBARGOED UNTIL: 9:00 am (EDT) June 30, 1999

PHOTO NO.: STScI-PRC99-27


A CLOSER ENCOUNTER WITH MARS

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. NASA is
releasing these images to commemorate the second anniversary of the Mars
Pathfinder landing. The lander and its rover, Sojourner, touched down
on the Red Planet's rolling hills on July 4, 1997, embarking on an
historic three-month mission to gather information on the planet's
atmosphere, climate, and geology.

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.

The upper-left image is centered near the location of the Pathfinder
landing site. Dark sand dunes that surround the polar cap merge into a
large, dark region called Acidalia. This area, as shown by images from
the Hubble telescope and other spacecraft, is composed of dark,
sand-sized grains of pulverized volcanic rock. Below and to the left of
Acidalia are the massive Martian canyon systems of Valles Marineris,
some of which form long linear markings that were once thought by some
to be canals. Early morning clouds can be seen along the left limb of
the planet, and a large cyclonic storm composed of water ice is churning
near the polar cap.

The upper-right 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.

The lower-left image is centered near another volcanic region known as
Elysium. This area shows many small, dark markings that have been
observed by the Hubble telescope and other spacecraft to change as a
result of the movement of sand and dust across the Martian surface. In
the upper left of this image, at high northern latitudes, a large
chevron-shaped area of water ice clouds mark a storm front. Along the
right limb, a large cloud system has formed around the Olympus Mons
volcano.

The lower-right image is centered on the dark feature known as Syrtis
Major, first seen telescopically by the astronomer Christiaan Huygens in
the 17th century. Many small, dark, circular impact craters can be seen
in this region, attesting to the Hubble telescope's ability to reveal
fine detail on the planet's surface. To the south of Syrtis is a large
circular feature called Hellas. Viking and more recently Mars Global
Surveyor have revealed that Hellas is a large and deep impact crater.
These Hubble telescope pictures show it to be filled with surface frost
and water ice clouds. Along the right limb, late afternoon clouds have
formed around the volcano Elysium.

Shown here are color composites generated from data using three filters:
blue (410 nanometers), green (502 nanometers), and red (673 nanometers).
A total of 12 color filters, spanning ultraviolet to near-infrared
wavelengths, were used in the observation.

Photo credits: Steve Lee (University of Colorado), Jim Bell (Cornell
University), Mike Wolff (Space Science Institute), and NASA

Other researchers involved in the collection and analysis of these
Hubble telescope data are R. Todd Clancy (Space Science Institute),
Philip James (University of Toledo), and Michael Ravine (Malin Space
Science Systems, Inc.).

NOTE TO EDITORS:

For additional information, please contact Jim Bell at
jimbo@marswatch.tn.cornell.edu.

Image files are available on the Internet at:
http://oposite.stsci.edu/pubinfo/pr/1999/27 or via links in
http://oposite.stsci.edu/pubinfo/latest.html and
http://oposite.stsci.edu/pubinfo/pictures.html

Higher resolution digital versions (300 dpi JPEG and TIFF) of the
release photo are available at:
http://oposite.stsci.edu/pubinfo/pr/1999/27/extra-photos.html

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