Mars Surveyor '01
Mars Surveyor '01 is the third set of orbiter/lander missions.
Mars Surveyor
'01 Orbiter
The '01 Orbiter is scheduled to launch March 7, 2001 and to enter Mars
orbit on December 10, 2001. The uniqueness of the orbiter is characterized
by its aerocaputure method. Within a week of arriving at Mars, the craft
will be in mapping orbit. The orbiter will also relay information from
the lander.
Science Instruments
THEMIS (Thermal Emission Imaging System) has a camera
and a thermal infrared imaging spectrometer. They will identify the morphology
and mineralogy of the surface.
GRS (Gamma Ray Spectrometer) will discover the elemental
composition and detect hydrogen in the shallow Martian subsurface.
MARIE (Martian Radiation Environment Experiment) will
detect radiation in the environment.
ACIP (Aerocapture Instrumentation Package) will find
the pressure and temperature of the
backshell during aerocapture.
Mars Surveyor
'01 Lander
This lander will bring a second rover, similar to Sojourner,
to Mars. Along with that, a CCD disk will be included on the lander which
holds all the names submitted for the mission. The lander will launch
on April 3, 2001 and will land on January 27, 2002.
Science Instruments
MECA (Mars Environmental Compatibility Assessment)
will analyze soil and dust to find any hazards to future astronauts.
MARDI (Mars Descent Imager) is similar to Surveyor '98's
imager.
MARIE (Martian Radiation Environment Experiment) will
find radiation in the environment.
MIP (Mars In Situ Propellant Production) is a package designed
to produce propellant from the Martian soil. Surveyor will not return
to Earth, but this experiment will help future missions. If it is successful,
propellant for the return trip to Earth will not be needed to be brought
to Mars.
APEX (Athena Precursor Experiment) contains the set of experiments
that the 2003 Athena rover will carry. All the instruments, except for
the APXS will the housed on the lander.
- The Pancam are 2 high-resolution color
stereo cameras which will take pictures around the rover.
- Mini-TES (Mini Thermal Emission Spectrometer) will
use thermal infrared wavelengths to measure mineral composition (water,
atmosphere, thermophysical properties).
- The Mössbauer Spectrometer is similar to the APXS,
but it specifically looks for iron minerals and magnetic properties.
- The APXS (Alpha Proton X-Ray Spectrometer), the instrument
on the rover, will find the elemental composition of the surface.
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