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A comparison of rayed craters on the Moon and Mercury

Author
NEISH, C. D1 ; BLEWETT, D. T2 ; HARMON, J. K3 ; COMAN, E. I4 ; CAHILL, J. T. S2 ; ERNST, C. M2
[1] Department of Physics and Space Sciences, Florida Institute of Technology, Melbourne, Florida, United States
[2] Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, United States
[3] National Astronomy and Ionosphere Center, Arecibo Observatory, Arecibo, Puerto Rico
[4] Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri, United States
Source

Journal of geophysical research. Planets (Print). 2013, Vol 118, Num 10, pp 2247-2261, 15 p ; ref : 1 p.1/4

ISSN
2169-9097
Scientific domain
Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
Publisher
Wiley, Hoboken, NJ
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Age Claste Comparaison planète Concentration Cratère météoritique Dimension Imagerie Longueur onde Lune Méthode radar Planète Mercure Cratère secondaire
Keyword (en)
age clasts interplanetary comparison concentration meteorite craters dimensions imagery wavelength Moon radar methods Mercury Planet
Keyword (es)
Edad Clasto Comparación planeta Concentración Dimensión Imaginería Luna Radar Planeta Mercurio
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences / 001E01D Cosmochemistry. Extraterrestrial geology / 001E01D01 Extraterrestrial geology

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
27977697

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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