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Icarus, 1967
Abstract Lower bounds for the strength of the lunar surface have been derived from the properties necessary to provide stability of the slopes observed in Ranger 7, 8, and 9 imagery. Additional information was obtained from Luna 9 data, from hydrostatic considerations, and from laboratory tests.
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Abstract Lower bounds for the strength of the lunar surface have been derived from the properties necessary to provide stability of the slopes observed in Ranger 7, 8, and 9 imagery. Additional information was obtained from Luna 9 data, from hydrostatic considerations, and from laboratory tests.
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Morphology of the Lunar Surface
1969In the preceding Chapters 13 and 14 we got acquainted with the methods and results of the determination of lunar coordinates, which have provided the basis for lunar mapping described in Chapter 15, and made possible a topographic description of the surface of the Moon with its almost innumerable and diverse features.
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Icarus, 1964
Abstract As a working hypothesis it is proposed that the lunar subsurface is smooth and firm with little or no dust and that it has an overlying cloud of 0.06 mm thickness consisting of ionized accreted interplanetary particles spaced at 8 microns with radius 0.8 microns.
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Abstract As a working hypothesis it is proposed that the lunar subsurface is smooth and firm with little or no dust and that it has an overlying cloud of 0.06 mm thickness consisting of ionized accreted interplanetary particles spaced at 8 microns with radius 0.8 microns.
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Lunar Surface Temperature and Emissivity Retrieval From Diviner Lunar Radiometer Experiment Sensor
Earth and Space Science, 2021Huazhong Ren, Jing Nie, Jiaji Dong
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Payload concepts for investigations of electrostatic dust motion on the lunar surface
Acta Astronautica, 2023Christine M Hartzell +2 more
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Near-field plume-surface interaction and regolith erosion and dispersal during the lunar landing
Acta Astronautica, 2020Amin Rahimi +2 more
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