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Solar Mass
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Summary
Solar Mass
is a standard
Unit of mass
in astronomy that is used to express the
Mass of stars
and other
Large celestial bodies
, equivalent to approximately 1.989 × 10^30 kilograms. It provides a
Convenient scale
for comparing the
Masses of different astronomical objects
within and
Beyond our galaxy
.
Concepts
Astronomical Unit
Stellar Mass
Gravitational Binding Energy
Main Sequence Stars
Mass-luminosity Relation
Chandrasekhar Limit
Binary Star Systems
Black Hole Formation
Supernova
Galactic Dynamics
Relevant Degrees
Astronomical Instruments and Techniques 100%
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