TV Camera

Objective

    Acquire TV panoramas of the surface to study processes that occur at impact sites, such as aeolian activity, fluvial effects on the surface, volcanism, etc. Surveys made in different seasons will yield information about the dynamics of these processes.

Method

    TV imaging of the martian surface. Panorama is taken with a camera built around band-selective CCD line-arrays, by the optical and mechanical package of the camera rotating around the vertical axis of the penetrator.

Main Characteristics

	Height above ground		1 m
	Number of pixels		2048
	IFOV				0.5 mrad
	Field of Regard			60°  X 360° 
	Spectral ranges
		blue band		0.44 to 0.46 µ m
		green band		0.54 to 0.56 µ m
		red band		0.69 to 0.75 µ m
		near-IR	band		0.96 to 1.02 µ m
	Data capacity			26 Mbit (2.6 Mbit w/ compression)
	Power consumption		2.0 W
	Mass				1.0 kg
	Session time			~0.3 hour

MECOM - Meteoset Meteorological Instrumentation

Objective

    in-situ measurements of meteorological parameters on the surface of Mars.

Method

    Measurements of temperature, pressure, wind direction, wind speed, and humidity of the atmosphere.

Main Characteristics

	Temperature		140° to 300° K (accuracy 1%)
	Pressure		3 to 10 mbar (accuracy 1%)
	Wind velocity		1 to 50 m/s (accuracy 5%)
	Humidity		10 to 1000 ppm (accuracy 10%)
	Data capacity		< 16 kbit/day (waiting mode 1.6 kbit/day)
	Power consumption	< 1 W (mean)
	Mass			0.4 kg
	Session time		first day continuous, then periodically

PEGAS - Gamma Ray Spectrometer

Objective

    Measure the elemental composition of martian rocks. The gamma radiation recorded by the instrument permits H, Na, Mg, Al, Si, K, Cl, Ca, Ti, Mn, Fe, Th, U abundances to be determined in rocks.

Method

    Recording of gamma-rays from natural radionuclides K, Th, U, and of the gamma radiation due to the nuclear interaction of cosmic rays with elements of Martian rocks.

Main Characteristics

	Gamma-radiation energy range		0.3 to 0.8 MeV
	Energy resolution for Ev = 0.661 MeV	better than 8%
	Measurement accuracy
	    for major rock-forming elements	better than 10%
	    for minor elements			better than 20%
	Data capacity				10 kbit/hour
	Power consumption			1.2 W
	Mass					0.8 kg
	Session time				10 hours

ANGSTREM - X-Ray Spectrometer

Objective

    Determine the elemental composition of subsurface rocks, including the abundance of rock-forming elements (Mg, Al, Si, Ca, Ti, Fe), volatiles (S, Cl) and minor elements

Method

    Excitation of the X-ray fluorescent radiation of a rock sample using the radioactive sources Fe55 and Cd109.

Main Characteristics

	Energy range		1.0 to 24 keV
	Data capacity		10 kbit/10 min
	Power consumption	0.9 W
	Mass			0.4 kg
	Session time		0.5 hr

ALPHA - Alpha/Proton Spectrometer

Objective

    Measure the elemental composition of. rocks, including the abundance of light elements (C. N. F) and major rock-forming elements (O, Na, Mg. Al. Si, S, K, Ca, Fe) in a small-size soil sample.

Method

    Irradiation of a martian soil sample with alpha-particles of a Cm244 isotope source (60-80 mCurie). The instrument records alpha-particle scattering spectra and secondary proton spectra.

Main Characteristics

	Energy range			0.8 to 6.3 MeV
	Resolution			7%
	Sensitivity			0.1 to 0.5 wt. %
	Data capacity			10 kbit/5 hours
	Power consumption		0.5 W
	Mass				0.32 kg
	Session time			10 hours

NEUTRON-P - Neutron Spectrometer

Objective

    soil humidity content and its variations
    depth variation of rock density

Method

    Recording of neutrons scattered on nuclei of rock elements. The humidity content is determined in ~0.3 m3 volume of a rock sample.

Main Characteristics

	Energy range				0.001 eV to 1 MeV
	Minimum detectable water content	0.1 wt. %
	Data capacity				300 bit/2.5 hours
	Power consumption			0.25 W
	Mass					0.2 kg
	Session time				2.5 hours

GRUNT - Accelerometers

Objective

    To measure the mechanical characteristics of surface rocks. The following characteristics are to be estimated:

      resistance force/time ratio
      velocity/time profile
      penetration profile and depth

Method

    Measurement of three overload components during the probe penetration into the surface.

Main Characteristics

	Instrument sensor		piezocrystal
	Wave range			3 to 100 kHz
	Force measurement accuracy	0.25 g
	Data capacity			1.2 kbit during penetration period
	Power consumption		0. 1 W
	Mass				0.1 kg
	Session time			< 1 min.

TERMOZOND - Temperature Probes

Objective

    Thermal physics of the surface soil layer:

      heat capacity
      heat conductivity
      thermal diffusivity
      diurnal and seasonal propagation of a thermal wave
      thermal flows from the planet's interior

Method

    Measurements of time and spatial profiles of rock temperature.

Main Characteristics

	Sensors					platinum thermocouples
	Accuracy of heat conductivity
	  and heat capacity measurements	5%
	Accuracy of absolute temperature
	  measurements				1° K
	Measurement cycle			5 min
	Data capacity, waiting mode		5 kbit/cycle
	Power consumption			4 W
	Mass					0.3 kg
	Session time				first day continuous, then
						  periodically

KAMERTON - Seismometer

Objective

    Study of the structure of the planetary crust, its stratification and inhomogeneities. Measurements of seismic noise and natural oscillations of the planet will provide the data on its inner structure and dynamics.

METHOD

    Recording of seismic noise of the planet.

Main Characteristics

	Frequency range			10 to 100 Hz
	Data capacity
		in waiting mode		16 bit/hour
		in the event mode	10 kbit/event
	Power consumption		0.02 W
	Mass				0.3 kg
	Session time			continuous

IMAP-6 - Magnetometer

Objective

    Measure the magnetic field of Mars, the magnetic properties of rocks and their paleomagnetism, and possible stratification of layers using magnetometric data.

Method

    Recording of three components of the magnetic field on the martian surface and a vertical component at the penetration depth.

Main Characteristics

	Resolution			0.5 nT
	Data capacity:
		first day		36 bit/min
		in the waiting mode	36 bit/4 hours
	Power consumption		1 W
	Mass				0.25 kg
	Session time:			first day continuous, then
					  periodically

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