Origin of the earth and moon

By R. Canup, K. Righter. 2000

160 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/02c23b1837e4ab9c72e08872de89de169cdb7d88

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Citations in the corpus

THE Hf-W ISOTOPIC SYSTEM AND THE ORIGIN OF THE EARTH AND MOON (2005, background): “See Canup & Righter 2000, pp. 45–62 Harper CL, Jacobsen SB. 1994a. Investigations of the 182Hf-182W systematics.”
Temperatures, Heat, and Energy in the Mantle of the Earth (2007, background): “, Stevenson, 1989; Wetherill, 1990) and two books (e.g., Newsom and Jones, 1990; Canup and Righter, 2000) deal with these issues in detail.”
Constructing the secular architecture of the solar system II: The terrestrial planets (2009, unknown): “For example, in the preferred case of Hahn & Malhotra (1999), in which planet migration is driven by a 50 M⊕ planetesimal disc, it takes more than 30 Myr for the planets to reach their current orbits.”
Evolution of a habitable planet (2003, background): “See Canup & Righter 2000, pp. 113–29 Canup RM, Righter K, eds.”
Protoplanetary Disk Turbulence Driven by the Streaming Instability: Nonlinear Saturation and Particle Concentration (2007, unknown): “…can form by gravitational instability (as originally proposed by Safronov [1969] and Goldreich & Ward [1973]), because the oft-mentioned critical density for gravitational collapse is irrelevant when drag forces are included to transfer angularmomentum from the solids to the gas (Ward 1976, 2000).”
Early life on land and the first terrestrial ecosystems (2013, methodology): “Geological events were compiled from references within Canup and Righter (2000), Eriksson et al. (2004), and Van Kranendonk et al. (2007a, 2007b).”