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We know mass, radius, distance of Sun and other stars. We also know size, number of stars in our galaxy or others. But, how do scientists measure these parameters ?
The discussion revolves around the methods used by scientists to measure mass, radius, and distance in astronomy, specifically focusing on celestial bodies like the Sun and stars within galaxies. The scope includes conceptual understanding and practical measurement techniques.
Participants express varying levels of familiarity with the topic, and while some encourage self-research, there is no consensus on the specific methods or answers to the original question posed.
The discussion reflects a mix of knowledge levels among participants, with some expressing confidence in their understanding while others seek more detailed explanations. There are no resolved mathematical steps or definitions provided.
Individuals interested in astronomy, particularly those looking to understand measurement techniques in the field, may find this discussion relevant.
It was a mistake. Thanks for noticing : ) : )BvU said:Intermediate level means undergrad -- or did you pick this by accident ?
Can you google "astronomic distance measurement" ?
Any further questions after you've read some of that are welcome, of course.
It's good. But what's answer... : ) : )BvU said:It's PF culture to encourage posters to do some research of their own![]()