Deep space 2: The Mars Microprobe Mission

被引:56
作者
Smrekar, S
Catling, D
Lorenz, R
Magalhaes, J
Moersch, J
Morgan, P
Murray, B
Presley, M
Yen, A
Zent, A
Blaney, D
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] NASA, Ames Res Ctr, Div Space Sci, Moffett Field, CA 94035 USA
[3] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[4] No Arizona Univ, Dept Geol, Flagstaff, AZ 86011 USA
[5] CALTECH, Dept Geol & Planetary Sci, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[6] Arizona State Univ, Dept Geol, Tempe, AZ 85287 USA
关键词
D O I
10.1029/1999JE001073
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Mars Microprobe Mission will be the second of the New Millennium Program's technology development missions to planetary bodies. The mission consists of two penetrators that weigh 2.4 kg each and are being carried as a piggyback payload on the Mars Polar Lander cruise ring. The spacecraft arrive at Mars on December 3, 1999. The two identical penetrators will impact the surface at similar to 190 m/s and penetrate up to 0.6 m. They will land within 1 to 10 km of each other and similar to 50 km from the Polar Lander on the south polar layered terrain. The primary objective of the mission is to demonstrate technologies that will enable :future science missions and, in particular, network science missions. A secondary goal is to acquire science data. A subsurface evolved water experiment and a thermal conductivity experiment will estimate the water content and thermal properties of the regolith. The atmospheric density, pressure, and temperature will be derived using descent deceleration data. Impact accelerometer data will be used to determine the depth of penetration, the hardness of the regolith, and the presence or absence of 1.0 cm scale layers.
引用
收藏
页码:27013 / 27030
页数:18
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