Literature DB >> 21814278

Forming the lunar farside highlands by accretion of a companion moon.

M Jutzi1, E Asphaug.   

Abstract

The most striking geological feature of the Moon is the terrain and elevation dichotomy between the hemispheres: the nearside is low and flat, dominated by volcanic maria, whereas the farside is mountainous and deeply cratered. Associated with this geological dichotomy is a compositional and thermal variation, with the nearside Procellarum KREEP (potassium/rare-earth element/phosphorus) Terrane and environs interpreted as having thin, compositionally evolved crust in comparison with the massive feldspathic highlands. The lunar dichotomy may have been caused by internal effects (for example spatial variations in tidal heating, asymmetric convective processes or asymmetric crystallization of the magma ocean) or external effects (such as the event that formed the South Pole/Aitken basin or asymmetric cratering). Here we consider its origin as a late carapace added by the accretion of a companion moon. Companion moons are a common outcome of simulations of Moon formation from a protolunar disk resulting from a giant impact, and although most coplanar configurations are unstable, a ∼1,200-km-diameter moon located at one of the Trojan points could be dynamically stable for tens of millions of years after the giant impact. Most of the Moon's magma ocean would solidify on this timescale, whereas the companion moon would evolve more quickly into a crust and a solid mantle derived from similar disk material, and would presumably have little or no core. Its likely fate would be to collide with the Moon at ∼2-3 km s(-1), well below the speed of sound in silicates. According to our simulations, a large moon/Moon size ratio (∼0.3) and a subsonic impact velocity lead to an accretionary pile rather than a crater, contributing a hemispheric layer of extent and thickness consistent with the dimensions of the farside highlands and in agreement with the degree-two crustal thickness profile. The collision furthermore displaces the KREEP-rich layer to the opposite hemisphere, explaining the observed concentration.

Entities:  

Year:  2011        PMID: 21814278     DOI: 10.1038/nature10289

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


  6 in total

1.  Origin of the Moon in a giant impact near the end of the Earth's formation.

Authors:  R M Canup; E Asphaug
Journal:  Nature       Date:  2001-08-16       Impact factor: 49.962

2.  The origin of the moon and the single-impact hypothesis III.

Authors:  W Benz; A G Cameron; H J Melosh
Journal:  Icarus       Date:  1989       Impact factor: 3.508

3.  Structure and formation of the lunar farside highlands.

Authors:  Ian Garrick-Bethell; Francis Nimmo; Mark A Wieczorek
Journal:  Science       Date:  2010-11-12       Impact factor: 47.728

4.  A constitutive law for dense granular flows.

Authors:  Pierre Jop; Yoël Forterre; Olivier Pouliquen
Journal:  Nature       Date:  2006-06-08       Impact factor: 49.962

5.  Global elemental maps of the moon: the Lunar Prospector gamma-Ray spectrometer.

Authors:  D J Lawrence; W C Feldman; B L Barraclough; A B Binder; R C Elphic; S Maurice; D R Thomsen
Journal:  Science       Date:  1998-09-04       Impact factor: 47.728

6.  The shape and internal structure of the moon from the clementine mission.

Authors:  M T Zuber; D E Smith; F G Lemoine; G A Neumann
Journal:  Science       Date:  1994-12-16       Impact factor: 47.728

  6 in total
  3 in total

1.  Planetary science: Making mountains out of a moon.

Authors:  Maria T Zuber
Journal:  Nature       Date:  2011-08-03       Impact factor: 49.962

2.  The tidal-rotational shape of the Moon and evidence for polar wander.

Authors:  Ian Garrick-Bethell; Viranga Perera; Francis Nimmo; Maria T Zuber
Journal:  Nature       Date:  2014-07-30       Impact factor: 49.962

3.  Near/Far Side Asymmetry in the Tidally Heated Moon.

Authors:  Alice C Quillen; Larkin Martini; Miki Nakajima
Journal:  Icarus       Date:  2019-04-15       Impact factor: 3.508

  3 in total

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