Zobrazeno 1 - 10
of 69
pro vyhledávání: '"Nadine G. Barlow"'
Publikováno v:
Geophysical Research Letters. 46:13355-13362
Autor:
Elizabeth A. Silber, Michelle R. Kirchoff, Angela Stickle, Stuart J. Robbins, Clark R. Chapman, Simone Marchi, Nadine G. Barlow
Publikováno v:
Bulletin of the AAS. 53
Autor:
M. F. Zeilnhofer, Nadine G. Barlow
Publikováno v:
Icarus. 368:114586
Polygonal impact craters (PICs) are supposed to form as a result of impacts into structure systems within the target. The structure systems are an umbrella term which encompass faults, joints, fractures, lithographic boundaries, and other planes of w
Publikováno v:
Meteoritics & Planetary Science. 52:1371-1387
We report on the first results of a large-scale comparison study of central pit craters throughout the solar system, focused on Mars, Mercury, Ganymede, Rhea, Dione, and Tethys. We have identified 10 more central pit craters on Rhea, Dione, and Tethy
Autor:
S. E. Braden, Nadine G. Barlow, Clark R. Chapman, Simone Marchi, Zhiyong Xiao, Maria E. Banks, Caleb I. Fassett
Publikováno v:
Journal of Geophysical Research: Planets. 122:1010-1020
Following an approach similar to that used for the Moon, Mercury's surface units were subdivided into five time-stratigraphic systems based on geologic mapping using Mariner 10 images. The absolute time scale originally suggested for the time periods
Autor:
Nadine G. Barlow
Publikováno v:
Lecture Notes in Geoinformation and Cartography ISBN: 9783319628486
Impact crater databases are one of the first data products produced from images acquired by planetary spacecraft missions and are used in a variety of studies investigating the formation ages and geologic histories of surface units. Martian crater da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::196831790af51ca8e70d363d75bc5c8f
https://doi.org/10.1007/978-3-319-62849-3_15
https://doi.org/10.1007/978-3-319-62849-3_15
The Martian obliquity cycle is predominately influenced by Solar and Jovian tidal forces. The present-day axial tilt of Mars (25 degrees) is predicted to cycle between 0 degrees and 60 degrees (Mischna & Richardson 2005) with excursions up to 80 degr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab84656f77847d1248571b6dad914fef
http://arxiv.org/abs/1807.09716
http://arxiv.org/abs/1807.09716
Autor:
Nadine G. Barlow
Publikováno v:
Geological Society of America Abstracts with Programs.
Autor:
Nadine G. Barlow
Publikováno v:
Geomorphology. 240:18-33
Impact cratering is the one geologic process which is common to all solar system objects. Impact craters form by the resulting explosion between a solar system body and hypervelocity objects. Comparison with craters formed by chemical and nuclear exp