Zobrazeno 1 - 10
of 16 844
pro vyhledávání: '"impact crater"'
Publikováno v:
Frontiers in Earth Science, Vol 12 (2024)
Geophysical methods may provide crucial information for the characterization of buried impact structures. In this study, we report and comment on the results of the geophysical survey of an elliptical-shaped structure near Mahout at Oman’s central
Externí odkaz:
https://doaj.org/article/af8ba6ca7ede42f794d2d1caf6c01257
Publikováno v:
AGU Advances, Vol 5, Iss 5, Pp n/a-n/a (2024)
Abstract Earth's terrestrial surfaces commonly exhibit topographic roughness at the scale of meters to tens of meters. In soil‐ and sediment‐mantled settings topographic roughness may be framed as a competition between roughening and smoothing pr
Externí odkaz:
https://doaj.org/article/cef335cac6744c3b848946e532a68767
Publikováno v:
Scientific Reports, Vol 14, Iss 1, Pp 1-13 (2024)
Abstract Identifying lithologies in meteorite impact craters is an important task to unlock processes that have shaped the evolution of planetary bodies. Traditional methods for lithology identification rely on time-consuming manual analysis, which i
Externí odkaz:
https://doaj.org/article/28484b4e7b9d4685837ef17f41820a4c
Publikováno v:
Earth, Planets and Space, Vol 76, Iss 1, Pp 1-19 (2024)
Abstract The Zhurong rover of the Tianwen-1 mission successfully landed in the southern part of the Utopian Planitia and the northern region of the dichotomy boundary. Craters within a ~ 134 km2 region surrounding the Zhurong rover were identified an
Externí odkaz:
https://doaj.org/article/7c408a71f7d94c6cb9fdb02f32da29b5
Autor:
Losiak Anna
Publikováno v:
Miscellanea Geographica: Regional Studies on Development, Vol 27, Iss 4, Pp 165-171 (2023)
Impact craters are formed by collisions of cosmic bodies moving with hypervelocity. The formation of these features is not restricted to the distant geological past; new structures are constantly being created and at least 13 confirmed impact craters
Externí odkaz:
https://doaj.org/article/71dfca41fa0b49d7aca76dad9d9a2d07
Autor:
DIEGO D. GARCIA, EMILSON P. LEITE, MARCOS ALBERTO R. VASCONCELOS, EVANGELOS CHRISTOU, ALVARO P. CRÓSTA
Publikováno v:
Anais da Academia Brasileira de Ciências, Vol 96, Iss 1 (2024)
Abstract Large meteorite impacts release kinetic energy that induces rock deformation, high temperatures and fluid circulation during the cratering process. To understand the correlation between rock deformation and fluid circulation, it is relevant
Externí odkaz:
https://doaj.org/article/56ce3849030f4c18860cb3a28893bf9b
Publikováno v:
Scientific African, Vol 21, Iss , Pp e01893- (2023)
Impact cratering is an important aspect of planetary evolution. Geophysics plays a complementary role in identifying impact craters on Earth given the non-unique geological characteristics associated with such craters. The Bosumtwi impact crater in G
Externí odkaz:
https://doaj.org/article/590cfe86ba334f9ebbd63361fd596773
Autor:
Yanshuang Liu, Jialong Lai, Minggang Xie, Jiannan Zhao, Chen Zou, Chaofei Liu, Yiqing Qian, Jiahao Deng
Publikováno v:
Remote Sensing, Vol 16, Iss 2, p 344 (2024)
Impact craters are extensively researched geological features that contribute to various aspects of lunar science, such as evaluating the model age, regolith thickness, etc. The method for identifying impact craters has gradually transitioned from ma
Externí odkaz:
https://doaj.org/article/7c0d0084b3e7442ab0cfb91146d4439e
Publikováno v:
Remote Sensing, Vol 16, Iss 2, p 371 (2024)
Water ice has been found in the permanently shadowed regions of impact craters around the lunar South Pole, which makes them ideal areas for in situ exploration missions. However, near the rim of impact craters, construction and exploration activitie
Externí odkaz:
https://doaj.org/article/9d9e79e663cf4aa28e2efdcaf08e93ab
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