WebApr 13, 2024 · When a red supergiant has burnt out most of its fuel it resulst in a gravitational collaps, lowering its volume making the star smaller. When it shrinks the temperature get higher resulting in the start of thermonuclear fusion emiting great force and a giant explosion in the form of a supernova. Answer link WebAccording to Wikipedia, the red giant phase begins when the Hydrogen in the stars center is completely converted to Helium. Hydrogen is then fused to Helium in a shell surrounding the inert Helium core. This occurs a few thousand times faster than the earlier phase, so its lifetime is a few thousand times less than the main sequence phase that ...
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A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses (M☉)) in a late phase of stellar evolution. The outer atmosphere is inflated and tenuous, making the radius large and the surface temperature around 5,000 K (4,700 °C; 8,500 °F) or lower. The appearance of the red giant is … See more A red giant is a star that has exhausted the supply of hydrogen in its core and has begun thermonuclear fusion of hydrogen in a shell surrounding the core. They have radii tens to hundreds of times larger than that of the See more Red giants with known planets: the M-type HD 208527, HD 220074 and, as of February 2014, a few tens of known K-giants including See more The Sun will exit the main sequence in approximately 5 billion years and start to turn into a red giant. As a red giant, the Sun will grow so large (over 200 times its present-day radius) … See more Red giants are evolved from main-sequence stars with masses in the range from about 0.3 M☉ to around 8 M☉. When a star initially See more Many of the well-known bright stars are red giants, because they are luminous and moderately common. The red-giant branch variable star Gamma Crucis is the nearest M-class giant star at 88 light-years. The K1.5 red-giant branch star Arcturus is 36 light-years away. See more Media related to Red giants at Wikimedia Commons See more WebFeb 5, 2024 · 5 February 2024 Astronomy Now. Using the Atacama Large Millimetre/submillimetre Array, astronomers have found a binary star system in which the larger star’s transition from red giant to white dwarf was interrupted by a smaller companion star. Image: ALMA (ESO/NAOJ/NRAO), Olofsson et al. Acknowledgement: Robert Cumming. highwire farms adrian
Star Formation (Stellar Evolution or Life Cycle Of A Star)
WebJan 10, 2024 · Red supergiants look red because of their low surface temperatures. They range from about 3,500 - 4,500 Kelvin. According to Wien's law, the color at which a star radiates most strongly is directly … WebSep 12, 2024 · Red giant Red giants have diameters between 10 and 100 times that of the Sun. They are very bright, although their surface temperature is lower than that of the Sun. A red giant is formed during the … WebJan 13, 2024 · Why do red supergiants appear red? The color of stars depends primarily on the temperature of the surface of the star. ... For red supergiants to form, the mass in the cloud must be between 8 and ... highwire farms adrian mi