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How can the sun have much mass if it's just a bunch of gasses? And also what keeps the sun in a circlular shape? I've always wondered.
The discussion revolves around the mass and shape of the Sun, exploring questions about its composition, density, gravitational effects, and the implications of its gaseous nature. Participants engage in both conceptual and technical explanations related to astrophysics.
Participants express differing views on the Sun's density, gravitational effects at its center, and the efficiency of its mass loss. There is no consensus on these points, indicating ongoing debate and exploration of the topic.
Some claims about the Sun's density and gravitational effects depend on specific definitions and assumptions that are not fully resolved in the discussion.
Actually, the sun's average density is about 1.4 grams per cubic centimeter, about 40% denser than water.Originally posted by Loren Booda
The Sun has, on average, density slightly less than that of water
Originally posted by Loren Booda
90 times greater at its center since its mass, thus gravitation, is so great, thereby maintaining fusion
A ton of feathers still has a mass of one ton.How can the sun have much mass if it's just a bunch of gasses?
It loses far less than 0.01% of its mass yearly.Originally posted by Decker
Isn't the sun something like 99.99% efficient per year? As in, each year it would have 99.99% of its mass that it had last year at the same time?