Back Groot Bombardement Afrikaans قصف شديد متأخر Arabic Gecikən ağır bombardman Azerbaijani Gran bombardeig tardà Catalan Pozdní velké bombardování Czech Det Store Bombardement Danish Spätes schweres Bombardement German Bombardeo intenso tardío Spanish Bonbardaketa Berantiar Handia Basque آخرین بمباران سنگین Persian

Late Heavy Bombardment

Timescale
Artist's impression of the Moon during the Late Heavy Bombardment (above) and today (below)

The Late Heavy Bombardment (LHB), or lunar cataclysm, is a hypothesized astronomical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago,[1] at a time corresponding to the Neohadean and Eoarchean eras on Earth. According to the hypothesis, during this interval, a disproportionately large number of asteroids and comets collided into the terrestrial planets and their natural satellites in the inner Solar System, including Mercury, Venus, Earth (and the Moon) and Mars.[2] These came from both post-accretion and planetary instability-driven populations of impactors.[3] Although it gained widespread credence,[4] definitive evidence remains elusive.[5]

Evidence for the LHB derives from moon rock samples of Lunar craters brought back by the Apollo program astronauts. Isotopic dating showed that the rocks were last molten during impact events in a rather narrow interval of time, suggesting that a large proportion of craters were formed during this period. Several hypotheses attempt to explain this apparent spike in the flux of impactors in the inner Solar System, but no consensus yet exists. The Nice model, popular among planetary scientists, postulates that the giant planets underwent orbital migration, scattering objects from the asteroid belt, Kuiper belt, or both, into eccentric orbits and into the path of the terrestrial planets.[3]

Other researchers doubt the heavy bombardment, arguing for example that the apparent clustering of lunar impact-melt ages is a statistical artifact produced by sampling rocks scattered from a single large impact.[1] A range of evidence suggests that there may instead have been a more extended period of lunar bombardment, lasting from approximately 4.2 billion years ago to 3.5 billion years ago.[6]

  1. ^ a b Cite error: The named reference taylor1 was invoked but never defined (see the help page).
  2. ^ Claeys, Philippe; Morbidelli, Alessandro (1 January 2011). "Late Heavy Bombardment". In Gargaud, Muriel; Amils, Prof Ricardo; Quintanilla, José Cernicharo; Cleaves II, Henderson James (Jim); Irvine, William M.; Pinti, Prof Daniele L.; Viso, Michel (eds.). Encyclopedia of Astrobiology. Springer Berlin Heidelberg. pp. 909–912. doi:10.1007/978-3-642-11274-4_869. ISBN 978-3-642-11271-3.
  3. ^ a b Bottke, William F.; Norman, Marc D. (30 August 2017). "The Late Heavy Bombardment". Annual Review of Earth and Planetary Sciences. 45 (1): 619–647. Bibcode:2017AREPS..45..619B. doi:10.1146/annurev-earth-063016-020131. ISSN 0084-6597. Retrieved 11 August 2022.
  4. ^ Boehnke, Patrick; Harrison, T. Mark (27 September 2016). "Illusory Late Heavy Bombardments". Proceedings of the National Academy of Sciences. 113 (39): 10802–10806. Bibcode:2016PNAS..11310802B. doi:10.1073/pnas.1611535113. ISSN 0027-8424. PMC 5047187. PMID 27621460.
  5. ^ Mann, Adam (2018-01-24). "Bashing holes in the tale of Earth's troubled youth". Nature. 553 (7689): 393–395. Bibcode:2018Natur.553..393M. doi:10.1038/d41586-018-01074-6. PMID 29368708.
  6. ^ Zellner, Nicolle E. B. (September 2017). "Cataclysm No More: New Views on the Timing and Delivery of Lunar Impactors". Origins of Life and Evolution of Biospheres. 47 (3): 261–280. arXiv:1704.06694. Bibcode:2017OLEB...47..261Z. doi:10.1007/s11084-017-9536-3. ISSN 0169-6149. PMC 5602003. PMID 28470374.

Developed by StudentB