Short Answer
For stars on the main sequence, the luminosity can be estimated by the formula L = ____________________.
Correct Answer:

Verified
Correct Answer:
Verified
Related Questions
Q130: The most accurate way to determine the
Q131: Describe two methods that could be used
Q132: Table 8-1<br><img src="https://d2lvgg3v3hfg70.cloudfront.net/TB5757/.jpg" alt="Table 8-1
Q133: To observe a visual binary, we must
Q134: abcPredict the next panel in the spectral
Q136: Doppler-shift observations of a spectroscopic binary star
Q137: Two stars of the same spectral class
Q138: The least massive main-sequence stars have a/an
Q139: What information can we get from eclipsing
Q140: On the H-R diagram, cool and bright