## ＜学術雑誌論文＞An iterative method for obtaining a nonlinear solution for the temperature distribution of a rotating spherical body revolving in a circular orbit around a star

作成者 著者識別子 作成者名 作成者別名 所属機関 所属機関名 Department of Earth and Planetary Sciences, Faculty of Sciences, Kyushu University : Professor 九州大学大学院理学研究院地球惑星科学部門 : 教授 作成者名 作成者別名 所属機関 所属機関名 Graduate School of Science, Kyushu University 九州大学大学院理学府 英語 Elsevier Pergamon Press 2013-07-05 84 112 121 Accepted Manuscript open access http://www.journals.elsevier.com/planetary-and-space-science http://www.sci.kyushu-u.ac.jp/ http://www.journals.elsevier.com/planetary-and-space-science http://www.sci.kyushu-u.ac.jp/ http://www.journals.elsevier.com/planetary-and-space-science http://www.sci.kyushu-u.ac.jp/ We developed an iterative method for determining the time-dependent three-dimensional temperature distribution in a spherical body with smooth surface that is irradiated by a star. In the method devel...oped in our previous paper (Sekiya et al., 2012), only the rotational motion is taken into account and the effect due to the revolution around the star is ignored. The present work includes both the effects of the rotation and the revolution. We take into account the cooling due to the surface radiation that is proportional to the fourth power of the temperature; this is the difference in the present work from Vokrouhlicky (1999) that employs the linear approximation for the radiative cooling. It is assumed that material parameters such as the thermal conductivity and the thermometric conductivity are constant throughout the spherical body. We obtain a general solution for the temperature distribution inside a body by using the spherical harmonics and the spherical Bessel functions for space and the Fourier series for the time. The term in the boundary condition that represents the heating due to the star is also expanded into the spherical harmonics and the Fourier series. The coefficients of the general solution are fitted to satisfy the surface boundary condition by using an iterative method. We obtained solutions that satisfy the nonlinear boundary condition within 0.1% accuracy. The temperature distribution determined according to the iterative method is different from that according to the linear approximation; both the maximum and minimum temperatures at a given time after the summer solstice for an iterative solution are lower than those for a linear solution. The maximum difference between rate of change of the semimajor axis due to the Yarkovsky effect according to the iterative solution and that according to the linear solution is about 20%. Therefore, current understanding of the Yarkovsky effect based on linear solutions is fairly good.続きを見る

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Sekiya_Shimoda2013 pdf 306 KB 499

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レコードID 1448921 査読有 temperature radiation asteroids small bodies meteorites 0032-0633 10.1016/j.pss.2013.05.015 2014.07.07 2021.12.13