Details

Autor(en) / Beteiligte

• Arvidson, R. E.
• Bonitz, R. G.
• Robinson, M. L.
• Carsten, J. L.
• Volpe, R. A.
• Trebi-Ollennu, A.
• Mellon, M. T.
• Chu, P. C.
• Davis, K. R.
• Wilson, J. J.
• Shaw, A. S.
• Greenberger, R. N.
• Siebach, K. L.
• Stein, T. C.
• Cull, S. C.
• Goetz, W.
• Morris, R. V.
• Ming, D. W.
• Keller, H. U.
• Lemmon, M. T.
• Sizemore, H. G.
• Mehta, M.

Titel

Results from the Mars Phoenix Lander Robotic Arm experiment

Ist Teil von

• Journal of Geophysical Research - Planets, 2009-01, Vol.114 (E1), p.E00E02-n/a

Ort / Verlag

American Geophysical Union

Erscheinungsjahr

2009

Quelle

Wiley Online Library

Beschreibungen/Notizen

• The Mars Phoenix Lander was equipped with a 2.4 m Robotic Arm (RA) with an Icy Soil Acquisition Device capable of excavating trenches in soil deposits, grooming hard icy soil surfaces with a scraper blade, and acquiring icy soil samples using a rasp tool. A camera capable of imaging the scoop interior and a thermal and electrical conductivity probe were also included on the RA. A dozen trench complexes were excavated at the northern plains landing site and 31 samples (including water‐ice‐bearing soils) were acquired for delivery to instruments on the Lander during the 152 sol mission. Deliveries included sprinkling material from several centimeters height to break up cloddy soils on impact with instrument portals. Excavations were done on the side of the Humpty Dumpty and the top of the Wonderland polygons, and in nearby troughs. Resistive forces encountered during backhoe operations show that soils above the 3–5 cm deep icy soil interfaces are stronger with increasing depth. Further, soils are similar in appearance and properties to the weakly cohesive crusty and cloddy soils imaged and excavated by the Viking Lander 2, which also landed on the northern plains. Adsorbed H2O is inferred to be responsible for the variable nature and cohesive strength of the soils. Backhoe blade chatter marks on excavated icy soil surfaces, combined with rasp motor currents, are consistent with laboratory experiments using grain‐supported icy soil deposits, as is the relatively rapid decrease in icy soil strength over time as the ice sublimated on Mars.