WebRed supergiants ( RSGs) are stars with a supergiant luminosity class ( Yerkes class I) of spectral type K or M. [1] They are the largest stars in the universe in terms of volume, although they are not the most massive or luminous. Betelgeuse and Antares A are the brightest and best known red supergiants (RSGs), indeed the only first magnitude ... WebApr 14, 2024 · It will take approximately 5 billion years for the sun to reach this red giant phase. Now at the speed of earth drifts away, and taken into account the mass loss: By fusion, the sun "burns" about 564 million tons hydrogen …
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WebApr 13, 2024 · When our Sun enters the red giant phase of its life, in about 5 billion years, it will be so big that Mercury will be completely swallowed. Our red giant Sun will still be consuming helium and cranking out carbon. When the helium is gone, the Sun will succumb to gravity again. When the core contracts, it will cause a release of energy and the ... WebAs the red giant loses mass, the star’s gravitational hold on its planets becomes much weaker, so their orbits will expand. In our own solar system, the Sun will throw off about … screen cap on kindle fire hd 10
The Life Cycles of Stars - NASA
WebThe immense growth expected in the Sun when it becomes a red giant will cause its radius to swell from roughly 1 AU to perhaps 2 AU or so. This means that Mercury and Venus … WebMay 7, 2015 · Once a medium size star (such as our Sun) has reached the red giant phase, its outer layers continue to expand, the core contracts inward, and helium atoms in the … WebStellar evolution is the process by which a star changes over the course of time. Depending on the mass of the star, its lifetime can range from a few million years for the most massive to trillions of years for the least … screen cap programs