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Published November 25, 1999 | Published
Journal Article Open

Deep Space 2: The Mars Microprobe Mission

Abstract

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 ∼190 m/s and penetrate up to 0.6 m. They will land within 1 to 10 km of each other and ∼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 10 cm scale layers.

Additional Information

© 1999 American Geophysical Union. Received April 22, 1999; revised August1 7, 1999. The Mars Microprobe Project, and in particular, Sarah Gavit, George Powell, Randy Blue, and Kari Lewis, deserves acknowledgment for accomplishing a task that was not infrequently viewed as impossible by some outside the project. Suzanne Smrekar is the project scientist; Diana Blaney is also on the DS2 project staff. Other authors constitute the science team. This paper was substantially improved due to reviews by Jim Bell and an anonymous reviewer.

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Created:
August 19, 2023
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October 26, 2023