跳转到内容

恒星光谱

出自维基百科,自由个百科全书

天文学恒星分类是拿恒星依照光球个温度分门别类,伴随着个是光谱特性、搭子随后衍生个各种性质。根据维恩定律可以用温度来测量物体表面个温度,但对距离遥远个恒星是非常困难个。恒星光谱学提供了解决个方法,可以根据光谱个吸收谱线来分类:因为拉一定个温度范围内,只有特定个谱线会被吸收,所以检视光谱中被吸收个谱线,就可以确定恒星个温度。

pFad - Phonifier reborn

Pfad - The Proxy pFad of © 2024 Garber Painting. All rights reserved.

Note: This service is not intended for secure transactions such as banking, social media, email, or purchasing. Use at your own risk. We assume no liability whatsoever for broken pages.


Alternative Proxies:

Alternative Proxy

pFad Proxy

pFad v3 Proxy

pFad v4 Proxy