MORPHOMETRIC PARAMETERS OF FRESH LUNAR CRATERS
Authors:
1.
Sternberg State Astronomical Institute
2.
Sternberg State Astronomical Institute
3.
Sternberg State Astronomical Institute
Type:
Сonference abstract
Pages:
from 541
to 544
Published:
27.12.2024
Subject area:
UDC 52
UDC 523
UDC 53
UDC 520
UDC 521
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.19
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
UDC 523
UDC 53
UDC 520
UDC 521
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.19
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
Language:
English
Keywords:
Moon; craters
Abstract (English):
We study the morphometric parameters of 111 lunar craters with a diameter of 10 km or more, the formation of which, according to some researchers, can be attributed to the Copernican period. These craters were selected by analyzing data from the Diviner spectrometer on board the LRO probe. The purpose of this work is to study the morphometric characteristics of such craters in order to identify their characteristic features. According to the results obtained, the morphometric parameters of the fresh lunar craters are significantly similar to the morphometric parameters of lunar craters of the 1st degree of degradation (well-preserved craters) according to the classification of the SAI MSU.
We study the morphometric parameters of 111 lunar craters with a diameter of 10 km or more, the formation of which, according to some researchers, can be attributed to the Copernican period. These craters were selected by analyzing data from the Diviner spectrometer on board the LRO probe. The purpose of this work is to study the morphometric characteristics of such craters in order to identify their characteristic features. According to the results obtained, the morphometric parameters of the fresh lunar craters are significantly similar to the morphometric parameters of lunar craters of the 1st degree of degradation (well-preserved craters) according to the classification of the SAI MSU.
Keywords:
Moon; craters
Moon; craters
1. Slodarzh N., 2021, Vupusknaya kvalifikatsionnaya rabota bakalavra, p. 271
2. Mazrouei S., Ghent R., Bottke W., et al., 2019, Science, 363, 6424, p. 253
3. Rodionova Zh.F., Karlov A.A., Skobeleva T.P., et al., 1987, Morphological Catalogue of the Craters of the Moon, Moscow University Press
