Forming the lunar farside highlands by accretion of a companion moon View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2011-08-03

AUTHORS

M. Jutzi, E. Asphaug

ABSTRACT

By the light of the moonsThe Moon is a satellite of two distinct halves. The nearside that faces us all the time is low in altitude, flat and dark in colour, whereas the farside is mountainous and deeply cratered. Martin Jutzi and Erik Asphaug propose that this lunar dichotomy might be the consequence of the late accretion of a companion moon. Companion moons are a common outcome of giant impact and protolunar disk simulations. The new calculations suggest that a collision with a companion at subsonic impact velocity leads to an accretionary pile rather than a crater, resulting in a hemispheric layer consistent with the dimensions and crustal structure of the topography of the farside highlands. More... »

PAGES

69-72

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature10289

DOI

http://dx.doi.org/10.1038/nature10289

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1034018719

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/21814278


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