Zobrazeno 1 - 10
of 297
pro vyhledávání: '"Magnetic field of the Moon"'
Publikováno v:
Nature
Nature, 2023, 479 (7372), pp.215-218. ⟨10.1038/nature10565⟩
Nature, Nature Publishing Group, 2011, 479 (7372), pp.215-218. ⟨10.1038/nature10565⟩
Nature, 2023, 479 (7372), pp.215-218. ⟨10.1038/nature10565⟩
Nature, Nature Publishing Group, 2011, 479 (7372), pp.215-218. ⟨10.1038/nature10565⟩
Recent palaeomagnetic and seismological studies have strengthened the suggestion that the Moon once possessed a core dynamo. Despite its importance as a constraint on lunar evolution, there is currently no consensus on how such a dynamo was driven. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e698b5aca70ec6dd57ce21a53e9124d
https://hal.science/hal-00715312
https://hal.science/hal-00715312
Autor:
Thorsten Kleine, Thomas S. Kruijer
Publikováno v:
Earth and Planetary Science Letters. 475:15-24
The giant impact model of lunar origin predicts that the Moon mainly consists of impactor material. As a result, the Moon is expected to be isotopically distinct from the Earth, but it is not. To account for this unexpected isotopic similarity of the
Autor:
Yuki Harada, Hideo Tsunakawa, Hidetoshi Shibuya, Yoshifumi Saito, Shoichiro Yokota, Hisayoshi Shimizu, Masaki Matsushima, Futoshi Takahashi, Masaki N. Nishino
Publikováno v:
Icarus. 293:45-51
Accepted: 2017-04-05
資料番号: SA1170044000
資料番号: SA1170044000
Autor:
Jafar Arkani-Hamed, Daniel Boutin
Publikováno v:
Journal of Geophysical Research: Planets. 122:1195-1216
The analysis of the Lunar Prospector magnetic data over South Pole Aitken basin reveals two categories of magnetic anomalies with distinctly different polarities. Modeling the anomalies in terms of vertical prism source bodies shows two separate true
Publikováno v:
JETP Letters. 105:635-640
The possibility of the formation of a plasma–dust cloud in the exosphere of the Moon owing to impacts of meteoroids on the lunar surface is discussed. Attention is focused on dust particles at large altitudes of ~10–100 km at which measurements w
Publikováno v:
Icarus. 286:138-152
The lunar surface features diverse impact structures originating from its early bombardment; the largest among them are the lunar basins. Basin-forming impacts delivered large amounts of energy to the target and expelled lots of material that deposit
Publikováno v:
Icarus. 281:90-102
Several new scenarios of the Moon-forming giant impact have been proposed to reconcile the giant impact theory with the recent recognition of the volatile and refractory isotopic similarities between Moon and Earth. Two scenarios leave the post-impac
Publikováno v:
Nature. 539:402-406
In the giant impact hypothesis for lunar origin, the Moon accreted from an equatorial circum-terrestrial disk; however the current lunar orbital inclination of 5 degrees requires a subsequent dynamical process that is still debated. In addition, the
Autor:
E.M.A. Chen, Francis Nimmo
Publikováno v:
Icarus. 275:132-142
The present-day inclination of the Moon reflects the entire history of its thermal and orbital evolution. The Moon likely possessed a global magma ocean following the Moon-forming impact. In this work, we develop a coupled thermal-orbital evolution m
Publikováno v:
Plasma Physics Reports. 42:543-548
Dusty plasma in the region of the lunar terminator is considered. It is shown that, in this region, a structure resembling a plasma sheath forms near the lunar surface. This sheath creates a potential barrier, due to which electrons over the illumina