The evolution of a star depends on its size. If a star is sufficiently large, the gravity forces holding it together may be large enough to collapse it into a very dense object composed mostly of neutrons. The density of such a neutron star is about 1014 times that of the earth. Suppose that a star initially had a radius about that of our sun, 7 × 108 km, and that it rotated once every 26 days, as our sun does. What would be the period of rotation (the time for 1 rev) if the star collapsed to a radius of 15 km?
The evolution of a star depends on its size. If a star is sufficiently large, the gravity forces holding it together may be large enough to collapse it into a very dense object composed mostly of neutrons. The density of such a neutron star is about 1014 times that of the earth. Suppose that a star initially had a radius about that of our sun, 7 × 108 km, and that it rotated once every 26 days, as our sun does. What would be the period of rotation (the time for 1 rev) if the star collapsed to a radius of 15 km?
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The evolution of a star depends on its size. If a star is sufficiently large, the gravity forces
holding it together may be large enough to collapse it into a very dense object composed mostly
of neutrons. The density of such a neutron star is about 1014 times that of the earth. Suppose that
a star initially had a radius about that of our sun, 7 × 108 km, and that it rotated once every 26 days,
as our sun does. What would be the period of rotation (the time for 1 rev) if the star collapsed to a
radius of 15 km?
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