Instruments The
Phobos 2 infrared spectrometer (ISM) obtained 45000 spectra in the near infrared (from ) in the equatorial areas of Mars, with a spatial resolution ranging from , and 400 spectra of Phobos at 700 m resolution. These observations made it possible to generate the first mineralogical maps of the planet and its satellite, and to study the atmosphere of Mars. ISM was developed at
IAS and
DESPA (
Paris Observatory) with support from
CNES. List of instruments: • "VSK" TV imaging system • PROP-F "hopping" lander. • ARS-FP automatic X-ray fluorescence spectrometer • ferroprobe
magnetometer • Kappameter magnetic permeability / susceptibility sensor • gravimeter • temperature sensors • BISIN conductometer / tiltmeter • mechanical sensors (penetrometer, UIU accelerometer, sensors on hopping mechanism) • "DAS" (long-lived autonomous station) lander • TV camera • ALPHA-X Alpha-Proton-X-Ray Spectrometer • LIBRATION
Sun sensor (also known as STENOPEE) • Seismometer • RAZREZ anchor penetrometer • Celestial mechanics experiment • "ISM" thermal infrared spectrometer/radiometer – resolution • near-infrared imaging spectrometer • thermal imaging camera; magnetometers • gamma-ray spectrometers • X-ray telescope • radiation detectors • radar and laser altimeters • Lima-D laser experiment – designed to vaporize material from the Phobos surface for chemical analysis by a mass spectrometer • Automatic Space Plasma Experiment with Rotating Analyzer (ASPERA), an electron spectrometer and ion mass analyzer from the
Swedish Institute of Space Physics. ==Results==