From interstellar gas to the Earth-Moon system

Meteoritics and Planetary Science

Volumn 36, Issue 1, 2001, Pages 9-22

  Cameron, A G W ^a  

^a UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EARLY EARTH; FORMATION MECHANISM; HYDRODYNAMICS; MOON; PLANETARY EVOLUTION;

EID: 0035071281     PISSN: 10869379     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1945-5100.2001.tb01806.x     Document Type: Article

References (28)

1. The origin of the moon and the single impact hypothesis I
2. The origin of the moon and the single impact hypothesis II
3. The origin of the moon and the single impact hypothesis III
4. Formation of the prelunar accretion disk
5. The first ten million years in the solar nebula
6. The origin of the Moon and the single impact hypothesis V
7. Extinct radioactivities, core collapse supernovas, jets, and the R-process
8. The origin of the moon and the single impact hypothesis IV
9. The origin of the moon (abstract)
10. Some aspects of triggered star formation
11. A scaling relationship for satellite-forming impacts
12. Extinct radionuclides and the origin of the solar system
13. Satellite-sized planetesimals and lunar origin
14. Nucleosynthesis in neutrino-driven winds. II. Implications for heavy element synthesis
15. Compaction as the origin of the unusual craters on the asteroid Mathilde
16. Age and origin of the moon
17. Deuterium in the Galactic Centre as a result of recent infall of low-metallicity gas
18. 10Be in a Calcium-Aluminum-Rich Inclusion from the Allende meteorite
19. Magnetic braking, ambipolar diffusion, cloud cores, and star formation-natural length scales and protostellar masses
20. Origin of the moon: The collision hypothesis
21. Two-phase gravitational instabilities in thin disks with application to the origin of the Moon (abstract)
22. Gravitational instability in two-phase disks and the origin of the moon
23. Poynting jets from accretion disks: Magnetohydrodynamic simulations
24. Injection of radioactivities into the presolar cloud: Convergence testing
25. Numerical simulations of triggered star formation. I. Collapse of dense moleclar cloud cores
26. Disk evolution within the Roche limit (abstract)
27. The evolution and explosion of massive stars. II. Explosive hydrodynamics and nucleosynthesis