Zobrazeno 1 - 10
of 133
pro vyhledávání: '"Alexander T. Basilevsky"'
Publikováno v:
Geological Society, London, Special Publications. 541
Geological mapping principles have been applied across planet Earth since William Smith's initial 1815 map. During the Space Age, these principles were applied to smaller moons and planets, appropriately adjusted for remote conditions and data, and r
Autor:
Irina Nadezhdina, Alexander T. Basilevsky, A. E. Zubarev, N. A. Kozlova, V. A. Volov, A. M. Abdrakhimov, M. I. Malenkov
Publikováno v:
Solar System Research. 55:285-308
The paper describes the results of measuring the depth of the track left by the wheels of Lunokhod-1 and -2; the depth was used to estimate the compressive strength of the upper layer of the lunar soil. The measurements were taken at 13 locations alo
Publikováno v:
Solar System Research. 55:83-96
Abstract The geomorphological and geological analysis of the surface of three primary and ten secondary landing ellipses (15 × 30 km) for the Russian Luna-Glob automated scientific station (Luna-25) is presented. The earlier selected landing ellipse
Autor:
Alexander T. Basilevsky, Greg Michael
Publikováno v:
Solar System Research. 55:20-30
We present the results of geological and morphological analysis of LROC NAC images of a small volcanic crater Ina, D-shaped in plan view (2.9 × 1.9 km), and its immediate surroundings. This crater is located at the top of a very gently sloping shiel
Publikováno v:
Solar System Research. 54:361-371
The paper discusses three types of processes of destruction of small lunar craters: (1) destruction by overlapping craters; (2) destruction due to filling with ejecta from neighboring and remote craters; and (3) destruction due to the displacement of
Autor:
Christian Wöhler, Alexander T. Basilevsky, Stephanie Althoff, Minggang Xie, Roberto Bugiolacchi, Yong L. Zou, Thorsten Wilhelm, Lionel Wilson, James W. Head, Feng Zhang
Publikováno v:
Journal of Geophysical Research: Planets. 126
Ring-moat dome structures (RMDSs) are small circular mounds of diameter typically about 200 m and ∼3–4 m in height, surrounded by narrow, shallow moats. They occur in clusters, are widespread in ancient Imbrian-aged mare basalt host units and sho
Publikováno v:
Icarus. 329:24-33
Wrinkle ridges are common landforms widely distributed in the lunar maria. Many young wrinkle ridges were found inside Mare Imbrium using Lunar Reconnaissance Orbiter Camera (LROC) Narrow Angle Camera (NAC) high-resolution images. They represent very
Autor:
S. S. Krasilnikov, Mikhail A. Ivanov, M. I. Malenkov, D. R. Scott, James W. Head, Tiantian Liu, Alexander T. Basilevsky, L. Lark, Gregory Michael
Publikováno v:
Solar System Research. 53:383-398
Polar areas of the Moon are prospective sites for construction of a lunar base due to the near constant illumination conditions and the potential presence of water ice in the regolith of cold traps. The mountain Mons Malapert (MM) near the South pole
Autor:
Alexander T. Basilevsky, E. V. Shalygin, O. S. Shalygina, Wojciech J. Markiewicz, Nataliya V. Bondarenko
Publikováno v:
Icarus. 330:103-122
This work presents a comparative study of microwave properties and 1-μm emissivity for five Venus crater-associated radar-dark parabolas along with neighboring plains and some other geologic units. Craters of interest are Adivar, Bassi, Bathsheba, S
Publikováno v:
Planetary and Space Science. 172:14-21
Boulders larger than 2.2 m were studied on the rims and interior of 15 secondary craters of Copernicus Crater. The age of this Copernicus is 800 Ma, so that the age of its secondaries should be the same. This study continues the earlier work of Basil