Numerical Calculation and Analytic Formulas of Yarkovsky Effect Parameter of Circumsolar Asteroids

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY
T. Yu. Galushina, D. L. Bashaev, O. N. Letner, O. M. Syusina
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引用次数: 0

Abstract

The paper deals with two problems. The main problem is the parameter calculation for the Yarkovsky effect using analytic formulas and their comparison with that obtained through its inclusion in the number of parameters to be detected. Unknown physical parameters of asteroids are varied to obtain the boundary values from analytic formulas. Numerical calculations imply that acceleration driven by the Yarkovsky effect, is inversely proportional to the degree of the heliocentric distance. It is shown that numerical calculations for objects with a well-defined orbit are in good agreement with analytic boundaries. The second problem concerns the numerical calculation of the best degree value for the distance to the Sun. It is demonstrated that the best results are obtained at the degree value of 2.

环极小行星雅尔科夫斯基效应参数的数值计算和解析公式
本文涉及两个问题。主要问题是使用解析公式计算雅尔科夫斯基效应的参数,并将其与通过将其纳入待检测参数数量而获得的参数进行比较。通过改变小行星的未知物理参数,从解析公式中获得边界值。数值计算表明,雅尔科夫斯基效应驱动的加速度与日心距离的程度成反比。结果表明,对具有明确轨道的物体进行的数值计算与解析边界十分吻合。第二个问题涉及到到太阳距离最佳度值的数值计算。结果表明,最佳度值为 2 时结果最佳。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Russian Physics Journal
Russian Physics Journal PHYSICS, MULTIDISCIPLINARY-
CiteScore
1.00
自引率
50.00%
发文量
208
审稿时长
3-6 weeks
期刊介绍: Russian Physics Journal covers the broad spectrum of specialized research in applied physics, with emphasis on work with practical applications in solid-state physics, optics, and magnetism. Particularly interesting results are reported in connection with: electroluminescence and crystal phospors; semiconductors; phase transformations in solids; superconductivity; properties of thin films; and magnetomechanical phenomena.
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