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Modification of Caloris ejecta blocks by long-lived mass-wasting: A volatile-driven process?The Caloris basin is the largest well-preserved impact basin on Mercury. As such, Caloris ejecta afford us an opportunity to study material from Mercury's deep interior with remote sensing. We have made observations of the geomorphology, colour, distribution, and flank slopes of the circum-Caloris knobs. Our observations suggest that these circum-Caloris knobs are modified ejecta blocks from the Caloris impact. High-resolution MESSENGER images show that knobs are conical and relatively uncratered compared with the surrounding plains, which implies the knobs have undergone resurfacing. We have observed material that has sloughed off knobs superposing impact craters that demonstrably postdate the Caloris impact, which requires some knob modification to have been more recent. We have observed hollows, depressions in Mercury's surface generally believed to have been caused by volatile-loss, on and closely associated with several knobs, which indicates that many knobs contain volatile material and that knob modification could extend into Mercury's recent past. Our measurements show that knob flanks typically have slopes of ∼21°, which is steep for a mound of unconsolidated material that was originally emplaced ∼3.8 Ga. The conical shape of knobs, their steep slopes, the dearth of superposed craters on knobs, and knob superposition relationships with other landforms suggest that Caloris ejecta blocks of arbitrary original shape were modified into their present shapes by long-lived mass-wasting. Mass-wasting must have dominated over impact gardening, which would have produced domal morphologies only. We suggest that mass-wasting was probably driven by volatile-loss, in a manner analogous to terrestrial landforms called ‘molards’. If the circum-Caloris knobs are analogous to molards, then they represent a landform and a process hitherto undocumented on Mercury, with implications for the volatile content of the planet's interior. These knobs therefore are prime targets for BepiColombo, which could search for fresh failures and volatile exposures in the knobs.
Document ID
20205006132
Acquisition Source
Marshall Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Jack Wright ORCID
(Open University, Milton Keynes)
Susan Conway ORCID
(Laboratoire de Planétologie et Géodynamique de Nantes Nantes, France)
Costanza Morino ORCID
(Université Savoie Mont Blanc Chambéry, Rhône-Alpes, France)
David A. Rothery
(Open University, Milton Keynes)
Matthew R. Balme ORCID
(Open University, Milton Keynes)
Caleb I. Fassett
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Date Acquired
August 10, 2020
Publication Date
August 25, 2020
Publication Information
Publication: Earth and Planetary Science Letters
Publisher: Elsevier
Volume: 549
Issue Publication Date: November 1, 2020
ISSN: 0012-821X
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
WBS: 231402.02.02.03.59
CONTRACT_GRANT: ST/N50421X/1
CONTRACT_GRANT: EUH 2020 776276
CONTRACT_GRANT: NE/L002493/1
CONTRACT_GRANT: GA/14S/024, Ref: 284
PROJECT: GeoPlaNet 2016-10982
PROJECT: ANR-19-CE01-0010 PERMOLARDS
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
Mercury; Caloris basin; impact ejecta; volatiles; molards
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