2012, Vol. 29(1): 19601-019601    DOI: 10.1088/0256-307X/29/1/019601
	An Internal Heating Model to Elucidate the Shape of a Small Planetary Body
	LI Gen, CHEN Chu-Xin**
	School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026
	收稿日期 2011-04-18  修回日期 1900-01-01
	Supporting info
	[1] Herndon J M et al 1973 Nature Phys. Sci. 244 40 [2] Urey H 1955 Proc. Natl. Acad. Sci. U. S.A. 41 127 [3] Lee T et al 1976 Geophys. Res. Lett. 3 41 [4] Russell S S et al 1996 Science 273 757 [5] Kita N T et al 2000 Geochim. Cosmochim. Acta 64 3913 [6] Thomas C Hanks et al 1968 Phys. Earth Planet. Interiors 2 19 [7] Herndon J M 1977 Meteoritic 12 459 [8] Carslaw H S and Jaeger J C 1959 Conduction of Heat in Solids (Oxford: Oxford University) [9] Opeil C P et al 2010 Icarus 208 449 [10] Kleine T et al 2005 Geochimica et Cosmochimica Acta 69 5805 [11] López Gonzáles M J 2005 Planet. Space Sci. 53 1147 [12] Baer J 2010 Recent Asteroid Mass Determinations http://home.earthlink.net/ jimbaer1/astmass.txt [13] JPL Small Body Database Browser http://ssd.jpl.nasa.gov/sbdb.cgi [14] Michałowski T et al 2004 Astron. Astrophys. 416 353 [15] Nugent R 2003 http://www.weblore.com/richard/Asteroid_Profiles.htm#704 Interamnia [16] Schmidt B E et al 2008 39th Lunar and Planetary Science Conference (League City, Texas 10–14 March) 1391 2502 [17] Thomas P C et al 1997 Science 277 1492 [18] Ghosh A et al 2000 Meteoritics Planet. Sci. 35 A59 [19] Merk R 2002 Icarus 159 183