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Title: Origin and implications of non-radial Imbrium Sculpture on the Moon

Journal Article · · Nature (London)
DOI:https://doi.org/10.1038/nature18278· OSTI ID:1321817
 [1];  [2]
  1. Brown Univ., Providence, RI (United States)
  2. Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)

Rimmed grooves, lineations and elongate craters around Mare Imbrium shape much of the nearside Moon. This pattern was coined the Imbrium Sculpture1, and it was originally argued that it must have been formed by a giant oblique (~30°) impact, a conclusion echoed by later studies2. Some investigators, however, noticed that many elements of the Imbrium Sculpture are not radial to Imbrium, thereby implicating an endogenic or structural origin3, 4. Here we use these non-radial trends to conclude that the Imbrium impactor was a proto-planet (half the diameter of Vesta), once part of a population of large proto-planets in the asteroid belt. Such independent constraints on the sizes of the Imbrium and other basin-forming impactors markedly increase estimates for the mass in the asteroid belt before depletion caused by the orbital migration of Jupiter and Saturn5. Furthermore, laboratory impact experiments, shock physics codes and the groove widths indicate that multiple fragments (up to 2% of the initial diameter) from each oblique basin-forming impactor, such as the one that formed Imbrium, should have survived planetary collisions and contributed to the heavy impact bombardment between 4.3 and 3.8 billion years ago.

Research Organization:
Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA), Office of Defense Nuclear Nonproliferation
Grant/Contract Number:
AC04-94AL85000
OSTI ID:
1321817
Report Number(s):
SAND-2016-5142J; 640983
Journal Information:
Nature (London), Vol. 535, Issue 7612; ISSN 0028-0836
Publisher:
Nature Publishing GroupCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 30 works
Citation information provided by
Web of Science

References (19)

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Atmospheric effects on ejecta emplacement and crater formation on Venus from Magellan journal January 1992
An Archaean heavy bombardment from a destabilized extension of the asteroid belt journal April 2012
An Impactor Origin for Lunar Magnetic Anomalies journal March 2012
Structure and evolution of the lunar Procellarum region as revealed by GRAIL gravity data journal October 2014
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Dynamic fault weakening and the formation of large impact craters journal October 2009
Some things we can infer about the Moon from the composition of the Apollo 16 regolith journal July 1997
Modeling damage and deformation in impact simulations journal February 2004
Projectile remnants in central peaks of lunar impact craters journal May 2013
Re-examining the main asteroid belt as the primary source of ancient lunar craters journal February 2015
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Some recent advances in the scaling of impact and explosion cratering journal January 1987
Hydrocode modeling of oblique impacts: The fate of the projectile journal January 2000
Expectations for Crater Size and Photometric Evolution from the Deep Impact Collision journal March 2005
The geologic history of the Moon report January 1987
Estimating transient crater size using the crustal annular bulge: Insights from numerical modeling of lunar basin-scale impacts: ESTIMATING TRANSIENT CRATER SIZE journal September 2012

Cited By (3)

Lunar Orientale Impact Basin Secondary Craters: Spatial Distribution, Size-Frequency Distribution, and Estimation of Fragment Size journal June 2018
Geological Characterization of the Ina Shield Volcano Summit Pit Crater on the Moon: Evidence for Extrusion of Waning‐Stage Lava Lake Magmatic Foams and Anomalously Young Crater Retention Ages journal April 2019
Projectile preservation during oblique hypervelocity impacts journal April 2018

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