Zobrazeno 1 - 10
of 102
pro vyhledávání: '"Robert G. Strom"'
Autor:
Caleb I. Fassett, Lillian R. Ostrach, William J. Merline, Clark R. Chapman, Robert G. Strom, Olivier S. Barnouin, Louise M. Prockter, Simone Marchi, David M.H. Baker
Publikováno v:
Mercury
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2b0f055eb31933360b03a1ea62bca2f7
https://doi.org/10.1017/9781316650684.010
https://doi.org/10.1017/9781316650684.010
Autor:
Zhiyong Xiao, Clark R. Chapman, Christian Klimczak, Thomas R. Watters, Paul K. Byrne, Maria E. Banks, Sean C. Solomon, S. E. Braden, Robert G. Strom
Publikováno v:
Journal of Geophysical Research: Planets. 120:1751-1762
Lobate scarps, landforms interpreted as the surface manifestation of thrust faults, are widely distributed across Mercury and preserve a record of its history of crustal deformation. Their formation is primarily attributed to the accommodation of hor
Autor:
Robert G. Strom, James W. Head, Mark S. Robinson, Sean C. Solomon, Jennifer L. Whitten, Caleb I. Fassett, Lillian R. Ostrach
Publikováno v:
Icarus. 250:602-622
MESSENGER orbital images show that the north polar region of Mercury contains smooth plains that occupy ~7% of the planetary surface area. Within the northern smooth plains (NSP) we identify two crater populations, those superposed on the NSP (“pos
Autor:
David T. Blewett, Jörn Helbert, Zhiyong Xiao, Deborah L. Domingue, Paul K. Byrne, Sean C. Solomon, Ann L. Sprague, Scott L. Murchie, Robert G. Strom
Publikováno v:
Journal of Geophysical Research: Planets. 118:1752-1765
[1] Orbital images acquired by the MErcury, Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft reveal a distinctive low-reflectance material on the surface of Mercury. Such material occurs in small, isolated, and thin surfic
Autor:
Zhiyong Xiao, Robert G. Strom
Publikováno v:
Icarus. 220:254-267
The small crater populations (diameter smaller than 1 km) are widely used to date planetary surfaces. The reliability of small crater counts is tested by counting small craters at several young and old lunar surfaces, including Mare Nubium and crater
Autor:
William J. Merline, Louise M. Prockter, Caleb I. Fassett, Clark R. Chapman, Sean C. Solomon, Maria E. Banks, Jeffrey A. Forde, Robert G. Strom, James W. Head
Publikováno v:
Planetary and Space Science. 59:1960-1967
The primary crater population on Mercury has been modified by volcanism and secondary craters. Two phases of volcanism are recognized. One volcanic episode that produced widespread intercrater plains occurred during the period of the Late Heavy Bomba
Autor:
Sean C. Solomon, Brett W. Denevi, Scott L. Murchie, Samuel C. Schon, Louise M. Prockter, Carolyn M. Ernst, David M.H. Baker, Robert G. Strom, James W. Head
Publikováno v:
Planetary and Space Science. 59:1932-1948
The study of peak-ring basins and other impact crater morphologies transitional between complex craters and multi-ring basins is important to our understanding of the mechanisms for basin formation on the terrestrial planets. Mercury has the largest
Autor:
Renu Malhotra, Robert G. Strom
Publikováno v:
Icarus. 216:359-362
Cuk et al. (Cuk, M., Gladman, B.J., Stewart, S.T. [2010]. Icarus 207, 590–594) argue that the projectiles bombarding the Moon at the time of the so-called lunar cataclysm could not have been mainbelt asteroids ejected by purely gravitational means,
Autor:
D. M. Hurwitz, Jeffrey J. Gillis-Davis, Nancy L. Chabot, William J. Merline, Sean C. Solomon, David T. Blewett, Clark R. Chapman, Louise M. Prockter, Thomas R. Watters, Caleb I. Fassett, Lillian R. Ostrach, James L. Dickson, Larry R. Nittler, Scott L. Murchie, Jennifer L. Whitten, Robert G. Strom, Zhiyong Xiao, James W. Head, Christian Klimczak, Brett W. Denevi, David M.H. Baker, Carolyn M. Ernst, Jürgen Oberst, Laura Kerber, Paul K. Byrne, Timothy A. Goudge
Publikováno v:
Science. 333:1853-1856
MESSENGER observations from Mercury orbit reveal that a large contiguous expanse of smooth plains covers much of Mercury's high northern latitudes and occupies more than 6% of the planet's surface area. These plains are smooth, embay other landforms,