相关实验视频
Updated: May 25, 2025

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
星座29P/Schwassmann-Wachmann 1及其近核环境从一个恒星遮蔽
C L Pereira1,2, F Braga-Ribas2,3, B Sicardy4
1Observatório Nacional (ON/MCTI), Rio de Janeiro, RJ, Brazil.
彗星29P/Schwassmann-Wachmann 1的恒星遮蔽揭示了它的固体核和局部的尘埃云. 这项研究提供了对彗星组成和太阳系早期状况的新见解.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 彗星科学 彗星科学
背景情况:
- 彗星提供了关于太阳系早期的关键信息.
- 恒星遮蔽是研究彗星核被昏迷所掩盖的关键.
- 了解彗星核附近的尘埃不透明度至关重要.
研究的目的:
- 介绍第一个对彗星29P/Schwassmann-Wachmann 1的恒星遮蔽观测.
- 为未来的隐蔽研究完善轨道预测.
- 为了研究彗星29P的物理特征和尘埃环境.
主要方法:
- 观测彗星29P的恒星遮蔽事件.
- 对光曲线的分析,以确定核的大小和特征.
- 测量尘埃不透明度和同等宽度.
主要成果:
- 一个固体检测相当于约54公里的弦长,为核半径提供了一个下限.
- 核周围的特征的识别,并确定不透明度的上限.
- 检测核附近的局部尘埃云/喷射,光学深度约为[公式:参见文本].
结论:
- 该研究提供了彗星29P半径的下限.
- 一个局部的尘埃云的证据表明表面有活跃的过程.
- 这项研究有助于理解彗星演变和太阳系历史.
更多相关视频
08:48High-Resolution Neutron Spectroscopy to Study Picosecond-Nanosecond Dynamics of Proteins and Hydration Water
Published on: April 28, 2022
11:27Studying Soft-matter and Biological Systems over a Wide Length-scale from Nanometer and Micrometer Sizes at the Small-angle Neutron Diffractometer KWS-2
Published on: December 8, 2016
相关概念视频
Schwarzschild Radius and Event Horizon
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
Atomic Nuclei: Larmor Precession Frequency
Atomic Emission Spectroscopy: Interference
Gravitation Between Spherically Symmetric Masses
Atomic Emission Spectroscopy: Overview
Atomic Emission Spectroscopy: Instrumentation