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Dodgers pitcher Clayton Kershaw finds himself in a familiar spot, selected to the All-Star team for the 11th time in 18 seasons. Kershaw missed the first 45 games of the season on the injured list as ...
RALEIGH, NC.-For the third time in his NHL career (2019, 2022), Sebastian Aho is an All-Star. Touting 43 points in 35 games, he ranks third among all Metropolitan Division skaters in scoring. With ...
Its total mass mainly determines its evolution and eventual fate. A star shines for most of its active life due to the thermonuclear fusion of hydrogen into helium in its core. This process releases energy that traverses the star's interior and radiates into outer space.
A star that consumes hydrogen to form helium is called a "main-sequence" star for all the time it is a hydrogen-fusing object. When it uses up all its fuel, the core contracts because the outward radiation pressure is no longer enough to balance the gravitational force.
When a high-mass star runs out of hydrogen, it begins converting carbon into other elements such as oxygen, magnesium, and neon. These new elements become the star’s fuel, which prevents the star from collapsing for longer. This entire process generally lasts a few million years.
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