Measuring Erosional and Depositional Patterns Across Comet 67P's Imhotep Region

Author:

Jindal A. S.12ORCID,Birch S. P. D.2,Hayes A. G.1,Özyurt F. P.3ORCID,Issah A. B.1ORCID,Moruzzi S. A.4,Barrington M. N.1ORCID,Soderblom J. M.5ORCID,Kirk R. L.6ORCID,Marschall R.7,Vincent J. B.8ORCID

Affiliation:

1. Cornell Center for Astrophysics and Planetary Sciences, Cornell University Ithaca NY USA

2. Department of Earth, Environmental and Planetary Sciences Brown University Providence RI USA

3. Department of Physics Wellesley College Wellesley MA USA

4. Lunar and Planetary Laboratory The University of Arizona Tucson AZ USA

5. Department of Earth Atmospheric and Planetary Sciences, Massachusetts Institute of Technology Cambridge MA USA

6. US Geological Survey Astrogeology Science Center Flagstaff AZ USA

7. CNRS, Observatoire de la Côte d’Azur, Laboratoire J.‐L. Lagrange Nice France

8. Deutsches Zentrum fur Luft‐und Raumfahrt (DLR), Institut für Planetenforschung Berlin Germany

Abstract

AbstractComet 67P/Churyumov‐Gerasimenko displays a pronounced hemispherical dichotomy in surface morphology, where the southern hemisphere exhibits more erosional features than the northern hemisphere due to receiving much greater solar radiation. Consequently, it is generally assumed that particles are ejected from the southern hemisphere through sublimation and a significant fraction eventually descends as airfall, covering the northern terrains. To investigate this south‐to‐north material transfer during the comet's perihelion passage, we used photoclinometry to measure material redistribution within its most extensive smooth terrain deposit around the Imhotep region. However, our findings do not align with this expected trend. Instead, we show that local‐scale processes substantially impact the erosion and accumulation of material, with one area experiencing net erosion while another nearby region, just a few dozen meters away, sees sediment buildup. Our analysis underscores the complex interplay of processes shaping Comet 67P's surface and likely comets more generally.

Funder

Heising-Simons Foundation

Publisher

American Geophysical Union (AGU)

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