Sierks H, Lamy P, Barbieri C. Images of asteroid 21 Lutetia: A remnantplanetesimal from the early solar system[J]. Science, 2011, 334(6055):487-490.
[5]
Fujiwara A, Kawaguchi J, Yeomans D K, et al. The rubble-pile asteroiditokawa as observed by Hayabusa[J]. Science, 2006, 312(5778): 1330-1334.
[6]
Huang J C, Ji J H, Ye P J, et al. The Ginger-shaped asteroid 4179Toutatis: New observations from a successful flyby of Chang'e-2[J].Scientific Reports, 2013, 3: 3411-3416.
[7]
余亮亮, 季江徽. 小行星热模型研究现状[J]. 天文学进展, 2013, 31(2):185-201.Yu Liangliang, Ji Jianghui. The review of thermal models for asteroids[J].Progess in astronomy, 2013, 31(2): 185-201.
[8]
Lebofsky L A, Sykes M V, Tedesco E F, et al. A refined standard thermalmodel for asteroids based on observations of 1 Ceres and 2 Pallas[J].Icarus, 1986, 68(2): 239-251.
[9]
Lebofsky L A, Spencer J R. Radiometry and thermal modeling of asteroid[C]//Asteroids II. Tucson: University of Arizona Press, 1989, 128-147.
[10]
Harris A W. A thermal model for near-earth asteroids[J]. Icarus, 1998,131(2): 291-301.
[11]
Delbo M, Harris A W. Physical properties of near Earth asteroids fromthermal infrared observations and thermal modeling[J]. Meteoritics &Planetary Science, 2002, 37(12): 1929-1936.
[12]
Lagerros J S V. Thermal physics of asteroids I. Effects of shape, heatconduction and beaming[J]. Astronomy & Astrophysics, 1996, 310:1011-1020.
[13]
Rozitis B, Green S F. Directional characteristics of thermal infraredbeaming from atmosphereless planetary surfaces-a new thermophysicalmodel[J]. Monthly Notices of the Royal Astronomical Society, 2011, 415(3): 2042-2062.
[14]
Lagerros J S V. Thermal physics of asteroids IV. Thermal infraredbeaming[J]. Astronomy & Astrophysics, 1998, 332: 1123-1132.
[15]
Rozitis B, Green S F. The influence of rough surface thermal-infraredbeaming on the Yarkovsky and YORP effects[J]. Monthly Notices of theRoyal Astronomical Society, 2012, 423(1): 367-388.
[16]
Müller T G, Lagerros J S V, Burgdorf M, et al. Fundamental thermalemission parameters of main-belt asteroids derived from ISO[C].Proceedings of the Conference“The Universe as seen by ISO”, Paris,Frances, October 20-23, 1998.
[17]
MüllerTG,SekiguchiT,KaasalainenM,etal.Thermalinfraredobservationsof the Hayabusa spacecraft target asteroid 25143 Itokawa[J]. Astronomy& Astrophysics, 2005, 443(1): 347-355.
[18]
Müller T G, Durech J, Hasegawa S, et al. Thermo-physical properties of162173 (1999 JU3), a potential flyby and rendezvous target forinterplanetary missions[J]. Astronomy & Astrophysics, 2010, 525: A145.
[19]
Müller T G, Rourke L O, Barucci A M, et al. Physical properties ofOSIRIS-REx target asteroid (101955) 1999 RQ36 derived fromHerschel, ESO-VISIR and Spitzer observations[J]. Astronomy &Astrophysics, 2012, 548: A36.
[20]
Emery J P, Fernandez Y R, Kelley M S P, et al. Thermal infraredobservations and thermophysical characterization of OSIRIS-REx targetasteroid (101955) Bennu[J]. Icarus, 2014, 234: 17-25.
[21]
李庆扬, 王能超, 易大义. 数值分析[M]. 第5版. 北京: 清华大学出版社, 2008: 188.Li Qingyang, Wang Nengchao, Yi Dayi. Numerical analysis[M]. 5thEdition. Beijing: Tsinghua University Press, 2008: 188.
[22]
Yu L L, Ji J H, Wang S. Shape, thermal, surface properties determinationof a candidate spacecraft target (175706) 1996 FG3[J]. Monthly Noticesof the Royal Astronomical Society, 2014, 439: 3357-3370.
[23]
Rozitis B, Duddy S R, Green S F, et al. A thermophysical analysis of the(1862) Apollo Yarkovsky and YORP effects[J]. Astronomy & Astrophysics,2013, 555: A20.
