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Elsevier, Earth and Planetary Science Letters, (430), p. 542-550, 2015

DOI: 10.1016/j.epsl.2015.08.003

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Knob heights within circum-Caloris geologic units on Mercury: Interpretations of the geologic history of the region

Journal article published in 2015 by S. E. Ackiss ORCID, D. L. Buczkowski ORCID, C. M. Ernst, J. A. McBeck, K. D. Seelos
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

The circum-Caloris geologic units show morphology consistent with ejecta-derived formation, however crater counts suggest the units formed after the basin. To determine if the surrounding units are directly related to basin formation or products of later volcanic resurfacing events, we measured the heights and densities of knobs in 22 study regions to the east of the Caloris basin in three geologic units circumferential to the basin: the Odin Formation, the Van Eyck Formation, and the Smooth Plains Formation. In these study regions the size and concentration of ejecta blocks generally decrease away from the crater rim. The morphology that superposes the knobs and the distribution of knob heights within each study region suggests that the knobs were deposited as ejecta and later embayed by one or multiple volcanic events. The distribution of knob height and concentration indicates that the knobs within the circum-Caloris units are related to the formation of the basin.