By A. Treves, L. Maraschi, M. Abramowicz
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Extra resources for Accretion: A collection of influential papers
Also see Whang (1977) and Russell, Elphic and Slavin (1980) for Mercury and Venus, respectively. The surface temperature and pressure of Venus are from Avduevsky et al. (1971), while those for Mars are summarized by Carr (1981). 3. 14 'Equatorial radii and polar radii are at the one-bar pressure level; from Lindal et al. (1987) for Jupiter, Saturn and Uranus. Pluto's radius and mass density are given by Mc Kinnon and Mueller (1988). Reciprocal masses, M 0 /M p , are from the Jet Propulsion Laboratory ephemeris, courtesy of J.
Adopted from Burns, Showalter and Morfill (1984). 0001 O? O? 1 (0) (0) (0) (11) O? O? 9 (1) Q f3 '1 'Y 6 1986U1R e: • Ru = 25,559 km. 1 1 1 22 to to to to 4 9 2 93 (2) 4 Adapted from Lane et a1. (1986) and Stone and Miner (1986). 1 *RN = 24,764 km. Courtesy of Joseph A. Burns and Philip D. Nicholson, Cornell University. All rings have low albedo, no detectable eccentricity or inclination, no measurable thickness and are quite dusty. 1 Physical Parameters and Motions of the Moon Size Mean Radius: It".
7 150 ± 70 1840 ± 150 < 30 60 0N 118°W 49°N lOoE 15°S 134°E 47°N 81°W 44°N 1100E 71 72 73 74 75 Tenoumer, Mauritania Vepriaj, Lith. 5 50 0N 95°W 47°N 35°E 49°N 61°E • After Grieve (1979) and Wasson (1974). 94 ·These mean orbital elements are good for any epoch from 1950 to 2000 at their given accuracy. Greater accuracy for 1950 and any epoch thereafter may be obtained by using the formula in Seidelmann, Doggett and De Luccia (1974); they also give the relations for the mean longitudes of the planets.
Accretion: A collection of influential papers by A. Treves, L. Maraschi, M. Abramowicz