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The Taylor Moon

The Taylor Moon
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摘要 The formation of the Moon remains obscure after*400 years since Galileo saw that the Moon was mountainous in 1609.The current hypothesis is that the Moon formed through a low-angle collision between the Earth and Mar-size impactor,which is known as the Giant Impact model(e.g.Benz et al.1989).The giant impact should be sufficiently The formation of the Moon remains obscure after*400 years since Galileo saw that the Moon was mountainous in 1609.The current hypothesis is that the Moon formed through a low-angle collision between the Earth and Mar-size impactor,which is known as the Giant Impact model(e.g.Benz et al.1989).The giant impact should be
作者 Wei-dong Sun
出处 《Acta Geochimica》 EI CAS CSCD 2016年第1期14-14,共1页 地球化学学报(英文)
关键词 Galileo collision obscure Giant hypothesis mountainous sufficiently giant likely volatile 月亮 泰勒 碰撞模型 伽利略 月球 地球
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参考文献6

  • 1Albarede F (2009) Volatile accretion history of the terrestrial planets and dynamic implications. Nature 461:1227-1233. doi: 10.1038/ nature08477.
  • 2Asphaug E (2014) Impact origin of the Moon. Ann Rev Earth Planet Sci 42:551-578.
  • 3Benz W, Caneron AGW, Melosh HJ (1989) The origin of the Moon and the single impact hypothesis. Icarus 81:113-131.
  • 4Stevenson DJ, Halliday AN (2014) Origin of the Moon. Phil Trans A Roy Soc London 372:20140289.
  • 5Taylor SR (2016) The Moon. Acta Geochim.
  • 6Yin QZ et al (2002) A short timescale for terrestrial planet formation from Hf-W chronometry of meteorites. Nature 418:949-952.

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