.png){kind=icon}
返回
Analytical YORP torques model with an improved temperature distribution function
.png){kind=icon}
OA
AI
DOI：10.1111/j.1365-2966.2009.15781.x.png)
.png){kind=icon}
.png){kind=icon}
分享.png){kind=icon}
收藏
摘要
En 中文
Previous models of the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect relied either on the zero thermal conductivity assumption, or on the solutions of the heat conduction equations assuming an infinite body size. We present the first YORP solution accounting for a finite size and non-radial direction of the surface normal vectors in the temperature distribution. The new thermal model implies the dependence of the YORP effect in rotation rate on asteroids conductivity. It is shown that the effect on small objects does not scale as the inverse square of diameter, but rather as the first power of the inverse.
Keyword:
errata, addenda
radiation mechanisms: thermal
methods: analytical
celestial mechanics
minor planets, asteroids
AI总结
对已上传原文的论文进行重点信息的提取，主要内容包括：简要概述、研究摘要、背景介绍、关键亮点、图文解析、展望与总结。
期刊
IF:
4.8
论文数:
7.1W
被引数:
25.0W
机构
引用论文
.png){kind=icon}
查看更多内容