相关实验视频
Updated: May 25, 2025

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
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雅尔科夫斯基和YORP效果模拟在3200 Phaethon上进行
Hiroki Senshu1, Hirotomo Noda2,3, Fumi Yoshida1,4
1Planetary Exploration Research Center, Chiba Institute of Technology, 2-17-1 Tsudanuma, Narashino, Chiba 275-0016, Japan.
概括
小行星3200法顿
科学领域:
- * 星球科学 星球科学
- * 太阳系动力学
背景情况:
- *小行星3200 Phaethon是双子座流星雨的母体.
- * 费顿表现出一个极其奇特的轨道与一个小的周日点距离.
研究的目的:
- *以数值研究小行星3200 Phaethon的热行为.
- *精确评估热辐射对法的轨道和旋转运动的影响.
主要方法:
- * 数值建模一个轨道周期的热变化.
- *分析旋转轴与太阳相对方向的影响.
主要成果:
- *热效应对轨道和旋转运动的变化信号在周日点附近.
- *对于热诱导的动量而言,正规表达式不适用于法伊.
- * 轨道平均热效应与观测和先前估计一致.
结论:
- * 费顿独特的轨道特征导致复杂的热效应.
- *这项研究提升了我们对小物体非引力作用的理解.
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