Predicting whether a star will eventually fuse oxygen into a heavier element, is a process that helps to determine the mass of the star.
A star refers to a giant celestial or astronomical object that is made up of a luminous sphere of plasma, which is mainly bounded together by its own gravitational force.
Generally, a star is typically comprises two (2) main hot gases and these are:
I. Hydrogen (H).
II. Helium (He).
Some examples of a star include the following;
In Astronomy, you can determine the mass of a star by predicting whether a star will eventually fuse oxygen into a heavier element.
In conclusion, the mass of a star is a fundamental characteristic that determines how two or more stars differ from each other.
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