Mercury's Caloris basin: Continuity between the interior and exterior plains

Author:

Rothery David A.1,Mancinelli Paolo2ORCID,Guzzetta Laura3ORCID,Wright Jack1ORCID

Affiliation:

1. School of Physical Sciences; Open University; Milton Keynes UK

2. Dipartimento di Fisica e Geologia; Università degli Studi di Perugia; Perugia Italy

3. Istituto di Astrofisica e Planetologia Spaziali; INAF; Rome Italy

Funder

UK Space Agency and the Science and Technology Funding Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference43 articles.

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2. Becker , K. J. M. S. Robinson T. L. Becker L. A. Weller K. J. Edmundson G. A. Neumamn M. E. Perry S. C. Solomon 2016 First global digital elevation model of Mercury

3. Mercury's global contraction much greater than earlier estimates;Byrne;Nat. Geosci.,2014

4. Widespread effusive volcanism on Mercury likely ended by about 3.6 Ga;Byrne;Geophys. Res. Lett.,2016

5. A laboratory model of surface crust formation and disruption on lava flows through non-uniform channels;Cashman;Bull. Volcanol.,2006

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