The inner solar system cratering record and the evolution of impactor populations

Robert G. Strom, Renu Malhotra, Zhi Yong Xiao, Takashi Ito, Fumi Yoshida, Lillian R. Ostrach

Research output: Contribution to journalArticle

26 Citations (Scopus)

Abstract

We review previously published and newly obtained crater size-frequency distributions in the inner solar system. These data indicate that the Moon and the terrestrial planets have been bombarded by two populations of objects. Population 1, dominating at early times, had nearly the same size distribution as the present-day asteroid belt, and produced heavily cratered surfaces with a complex, multi-sloped crater size-frequency distribution. Population 2, dominating since about 3.8-3.7 Gyr, had the same size distribution as near-Earth objects (NEOs) and a much lower impact flux, and produced a crater size distribution characterized by a differential -3 single-slope power law in the crater diameter range 0.02 km to 100 km. Taken together with the results from a large body of work on age-dating of lunar and meteorite samples and theoretical work in solar system dynamics, a plausible interpretation of these data is as follows. The NEO population is the source of Population 2 and it has been in near-steady state over the past ∼ 3.7-3.8 Gyr; these objects are derived from the main asteroid belt by size-dependent non-gravitational effects that favor the ejection of smaller asteroids. However, Population 1 was composed of main belt asteroids ejected from their source region in a size-independent manner, possibly by means of gravitational resonance sweeping during orbit migration of giant planets; this caused the so-called Late Heavy Bombardment (LHB). The LHB began some time before ∼3.9 Gyr, peaked and declined rapidly over the next ∼ 100 to 300 Myr, and possibly more slowly from about 3.8-3.7 Gyr to ∼2 Gyr. A third crater population (Population S) consisted of secondary impact craters that can dominate the cratering record at small diameters.

Original languageEnglish (US)
Pages (from-to)407-434
Number of pages28
JournalResearch in Astronomy and Astrophysics
Volume15
Issue number3
DOIs
StatePublished - Mar 1 2015

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cratering
impactors
solar system
crater
craters
asteroid
asteroid belts
near Earth objects
frequency distribution
planet
bombardment
meteorite
terrestrial planets
Moon
impactor
power law
meteorites
moon
asteroids
dating

Keywords

  • Earth
  • Minor planets, asteroids
  • Moon
  • Solar system: formation

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The inner solar system cratering record and the evolution of impactor populations. / Strom, Robert G.; Malhotra, Renu; Xiao, Zhi Yong; Ito, Takashi; Yoshida, Fumi; Ostrach, Lillian R.

In: Research in Astronomy and Astrophysics, Vol. 15, No. 3, 01.03.2015, p. 407-434.

Research output: Contribution to journalArticle

Strom, Robert G. ; Malhotra, Renu ; Xiao, Zhi Yong ; Ito, Takashi ; Yoshida, Fumi ; Ostrach, Lillian R. / The inner solar system cratering record and the evolution of impactor populations. In: Research in Astronomy and Astrophysics. 2015 ; Vol. 15, No. 3. pp. 407-434.
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