Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Copernican period"'
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef813e8e65e124327bbb9db296396928
https://doi.org/10.1029/2021je006880
https://doi.org/10.1029/2021je006880
Autor:
Sergei I. Ipatov, E. A. Feoktistova
We present a study on the relationship between the ratio of the depth of a crater to its diameter and the diameter for lunar craters both on the maria and on the highlands. We consider craters younger than 1.1 billion years in age, i.e. of Copernican
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ad9bdfbc69477486f83e1a649a54100
http://arxiv.org/abs/2103.00291
http://arxiv.org/abs/2103.00291
Central peaks of lunar complex craters of Copernican period provide best examples to study morphologies of impact melts and exposed subsurface as they are better preserved and less affected by the ...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1ec0e0bbdcd16df2f5f3c74f3400a012
https://doi.org/10.1002/essoar.10502631.1
https://doi.org/10.1002/essoar.10502631.1
Autor:
Tanu Singh, Neeraj Srivastava
Publikováno v:
Icarus. 351:113921
The Grimaldi Basin, centered at (5.2° S, 68.6° W), is a ~400 km diameter highly degraded, Pre-Nectarian double-ring impact structure on the Moon located near the western edge of the Oceanus Procellarum. Hyperspectral data from Moon Mineralogy Mappe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3611548b99bc72a9868437c22fae1ff3
https://doi.org/10.1016/j.icarus.2020.113921
https://doi.org/10.1016/j.icarus.2020.113921
Autor:
Caleb I. Fassett, Masatoshi Hirabayashi, Y. H. Huang, David A. Minton, Nicolle E. B. Zellner, James E. Richardson
Publikováno v:
Geological Society of America Abstracts with Programs.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fbc5300b2caaec2747e000e8572dda8d
https://doi.org/10.1130/abs/2017am-306683
https://doi.org/10.1130/abs/2017am-306683
Autor:
Daket, Yuko, Yamaji, Atsushi, Sato, Katsushi, Haruyama, Junichi, Morota, Tomokatsu, Ohtake, Makiko, Matsunaga, Tsuneo
Publikováno v:
Earth, Planets and Space. 68
Accepted: 2016-08-30
資料番号: SA1160150000
資料番号: SA1160150000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::095eff5aa7200500823a9a69bea6e718
http://id.nii.ac.jp/1696/00029167/
http://id.nii.ac.jp/1696/00029167/
Autor:
Charles J. Byrne
Publikováno v:
The Moon's Largest Craters and Basins ISBN: 9783319220314
This period includes the youngest features in the Catalog, younger than the Orientale Basin. The next period of younger features of the Moon is the Eratosthenian Period, illustrated by the Eratosthenes crater. The Copernican Period is illustrated by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::edf71e9931f86ad1376516f8b74d30d6
https://doi.org/10.1007/978-3-319-22032-1_9
https://doi.org/10.1007/978-3-319-22032-1_9
Autor:
Paul G. Lucey, James F. Bell, David T. Blewett, Bruce A. Campbell, Mark S. Robinson, G. A. Smith, B. Ray Hawke
Publikováno v:
Icarus. 170:1-16
Lunar rays are filamentous, high-albedo deposits occurring radial or subradial to impact craters. The nature and origin of lunar rays have long been the subjects of major controversies. We have determined the origin of selected lunar ray segments uti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fb7d9c62c929d54a106177d9cd6069ac
https://doi.org/10.1016/j.icarus.2004.02.013
https://doi.org/10.1016/j.icarus.2004.02.013
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Publikováno v:
Journal of Geophysical Research: Planets. 102:9231-9242
The relatively recent (< 1 b.y.) flux of asteroids and comets forming large craters on the Earth and Moon may be accurately recorded by craters with bright rays on the Moon's farside. Many previously unknown farside rayed craters are clearly distingu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6a7c7f6eac567c3ae2f1fc155d791d0
https://doi.org/10.1029/97je00114
https://doi.org/10.1029/97je00114