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Mars Pathfinder surpasses expectations
By DIANE AINSWORTH and MARK WHALEN
It keeps going and going and going ...
That familiar slogan associated with the pink Energizer
Bunny was one of the many ways the Mars Pathfinder rover
Sojourner was described at a press briefing this week, three
weeks after the mission's historic July 4 landing in an ancient
outflow channel known as Ares Vallis.
In fact, the Mars Pathfinder rover and lander have surpassed
the flight team's greatest expectations. With a primary lifetime
of seven days, the rover continues to operate nearly flawlessly,
traversing short distances to specific rocks each day, making
measurements of their composition, then turning to head for the
next rock a few meters away. Although it is hard to predict how
long the rover will last, the flight team thinks the hearty robot
could last much longer.
Data from the lander camera -- affectionately called the
"IMP," for Imager for Mars Pathfinder -- and several other
experiments continue to be returned in record volume. During the
last week, more than 300 megabits of data were returned, said
Pathfinder Project Scientist Dr. Matthew Golombek.
(As a point of reference, 300 megabits is approximately
equal to 37.5 megabytes, exceeding that of a computer with 32
megabytes of memory. It's roughly equivalent to more than 18,000
typewritten pages.)
Meanwhile, science data are beginning to reveal more about
weather and dust patterns on Mars, the magnetic characteristics
of Martian soil and the origin and composition of rocks in Ares
Vallis.
Rover surface operations were officially under way after
Sojourner safely crawled off its ramp on July 5. Within three
days of its exit, the rover had placed its spectrometer on
Barnacle Bill, the first rock ever to be analyzed on the surface
of another planet.
The rock turned out to be unusually rich in silicon, which
puts Barnacle Bill in one of the most common categories of
volcanic rocks on Earth, known as "andesites," said Dr. Rudolph
Rieder of Germany's Max Planck Institute for Chemistry, who is
principal investigator on the Alpha Proton X-Ray Spectrometer
(APXS) team. This was completely unexpected for Mars, as high
silica rocks require differentiation beyond that expected in
primitive planets.
Weather on Mars has become the topic of another team's
studies. Using data from the Atmospheric Science
Instrument/Meteorology Package (ASI/MET), the weather team led by
Dr. John "Tim" Schofield has reported each day's weather
forecast. Because it is currently summer in Mars' northern
hemisphere, the variations are minimal (for Mars). Generally, the
temperatures are dropping to about -73 degrees Celsius
(-100 degrees Fahrenheit), while rising to approximately -15 to -13
degrees Celsius (5 to 8 degrees Fahrenheit) during the day,
similar to the temperatures recorded by the Viking landers of the
mid-1970s.
"Future astronauts on Mars won't have much to talk about as
far as weather goes," said Dr. Julio Magalhaes, a member of the
ASI/MET team from NASA Ames Research Center in Mountain View,
Calif. "Northern summer in the subtropics on Mars is pretty much
the same from day to day. Fifty or 60 days from now, we'll start
to see dramatic changes with fall," said Dr. Jeffrey Barnes of
Oregon State University, who is a member of the
atmospheric/meteorological experiment. The winds are fairly weak,
blowing up to about 26 kilometers per hour (16 mph) during the
day. However, scientists expect the winds to increase and begin
kicking up dust as the Martian fall approaches this September.
Atmospheric opacity -- or how clear the sky is, according to
Pathfinder's atmospheric experiment -- showed that Mars is
moderately dusty up to about 40 kilometers (25 miles) above the
surface. The dust appears to be uniformly distributed, and is
expected to rise as Mars approaches its dusty season in the fall,
Barnes said. The visibility on Mars was estimated to be about 32
kilometers (20 miles) or more, roughly equivalent to a moderately
smoggy day in Los Angeles.
Worldwide interest in the mission has peaked with all of the
new science being reported. On July 22, more than 400 million
hits had been reported on the 20 Pathfinder mirror sites built
specially for the mission. Kirk Goodall, Mars Pathfinder Web
engineer, along with David Dubov, Mars Pathfinder Webmaster,
reported the most hits ever recorded in a day on a Web site -- 46
million -- which occurred on July 8.
"That's more than double the number of hits received in a
single day during the 1996 Olympic Games in Atlanta," Goodall
said.
"The Mars landing has excited and inspired the public like
very few activities today," Mission Manager Richard Cook noted.
"It shows the rest of the world that we can achieve a
technological marvel like this."
Speaking of technologies, another popular science tool being
used in this mission is three-dimensional modeling, which
recreates the surface of Mars based on stereo images of the
planet's surface. Three-D modeling has been useful in visualizing
otherwise unnoticed geologic features, such as the overhang on
the back side of a large boulder named Yogi. Dr. Carol Stoker, a
participating scientist from Ames, said the images were shipped
to Ames, where they were processed and later returned to JPL. The
3-D imagery was also used to measure distances and sizes of
objects.
One of the few problems encountered by the flight team so
far was a communications glitch, which occurred over the July 19-
20 weekend. The problem was associated with ground operations,
rather than with faulty hardware on the spacecraft, Cook
explained during a recent briefing.
Unlike on other deep space missions, the DSN is required to
reconfigure its equipment and software on a daily basis and to
establish the communications links only during short periods of
time when the lander's transmitter is on. By the middle of this
week, the team felt confident that the problem was fully
understood and would not interrupt surface operations.
Other recent science studies include soil abrasion
experiments performed by Sojourner's wheel tracks, asking it to
perform soil abrasion experiments and measuring the material
properties of the dust and soil by interacting with it by the
rover. Dr. Henry Moore, a rover scientist with the U.S.
Geological Survey in Menlo Park, Calif., likened the Martian soil
to a very fine-grained silt that could be found in Nebraska,
finer than talcum powder.
Dr. Peter Smith of the University of Arizona, who is
principal investigator of the lander camera, described more about
the Martian landscape, pointing out a shallow riverbed crossing
through the landing site and rocks in the distance that were
washed into this outflow channel from the Martian highlands.
Science activities for July 23 were set to take the rover
through the "cabbage patch," an area of soil and small rocks in
between Scooby Doo and the rock named Lamb. The rover will
conduct a soil experiment, then turn and move toward Lamb.
Scientists will take measurements of the dark soil near that rock
before moving on towards the rocks Cradle and Souffle.
For the latest mission updates, check Pathfinder's Web site
at http://www.jpl.nasa.gov/marsnews. An audio update on
Pathfinder's status can be heard by calling (800) 391-6654.
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