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An ongoing satellite–ring cycle of Mars and the origins of Phobos and Deimos

An ongoing satellite–ring cycle of Mars and the origins of Phobos and Deimos

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1891875267

An ongoing satellite–ring cycle of Mars and the origins of Phobos and Deimos

About this item

Full title

An ongoing satellite–ring cycle of Mars and the origins of Phobos and Deimos

Publisher

London: Nature Publishing Group UK

Journal title

Nature geoscience, 2017-04, Vol.10 (4), p.266-269

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

The Martian moons Phobos and Deimos may have accreted from a ring of impact debris, but explaining their origin from a single giant impact has proven difficult. One clue may lie in the orbit of Phobos that is slowly decaying as the satellite undergoes tidal interactions with Mars. In about 70 million years, Phobos is predicted to reach the location...

Alternative Titles

Full title

An ongoing satellite–ring cycle of Mars and the origins of Phobos and Deimos

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1891875267

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1891875267

Other Identifiers

ISSN

1752-0894

E-ISSN

1752-0908

DOI

10.1038/ngeo2916

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