A Geostratigraphic Map of the Rachmaninoff Basin Area: Integrating Morphostratigraphic and Spectral Units on Mercury

Author:

Wright Jack12ORCID,Zambon Francesca3ORCID,Carli Cristian3ORCID,Altieri Francesca3ORCID,Pöhler Claudia M.4,Rothery David A.2ORCID,van der Bogert Carolyn H.4ORCID,Rossi Angelo Pio5ORCID,Massironi Matteo6ORCID,Balme Matthew R.2ORCID,Conway Susan J.7ORCID

Affiliation:

1. European Space Agency (ESA) European Space Astronomy Centre (ESAC) Villanueva de la Cañada Madrid Spain

2. School of Physical Sciences The Open University Milton Keynes UK

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

4. Institut für Planetologie Universität Münster Münster Germany

5. School of Science Constructor University Bremen Germany

6. Dipartimento di Geoscienze Università degli Studi di Padova Padova Italy

7. Laboratoire de Planétologie et Géosciences CNRS UMR 6112 Nantes Université Université d’Angers Le Mans Université Nantes France

Abstract

AbstractGeological maps of Earth typically incorporate field observations of rock lithology, structure, composition, and more. In contrast, conventional planetary geological maps are often made using primarily qualitative morphostratigraphic remote sensing observations of planetary surfaces. However, it is possible to define independent quantitative spectral units (SUs) of planetary surfaces, which potentially contain information about surface composition, grain size, and space weathering exposure. Here, we demonstrate a generic method to combine independently derived geomorphic and SUs, using the Rachmaninoff basin, Mercury, as an example to create a new geostratigraphic map. From this geostratigraphic map, we can infer some compositional differences within geomorphic units, which clarifies and elaborates on the geological evolution of the region.

Funder

Horizon 2020 Framework Programme

Publisher

American Geophysical Union (AGU)

Reference117 articles.

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