red giant temperature
to resolve and measure the diameters of these stars. expanded state. CallUrl('www>psrd>hawaii>edu
CallUrl('www>astronomycast>com<2008<02 html',0), Planetary nebula A thick shell of gas ejected from and moving out from an extremely hot star; thought to be the outer layers of a ~TildeLink() star thrown out into space, the core of which eventually becomes a white dwarf. They live fast and die young and that's it for them. shrinks and the star becomes bluer and smaller. [4] A White Dwarf cannot exceed a solar mass of 1.4. The stellar remnant at the center is the hot core of the ~TildeLink(). At the same time, the core regio region. into a red giant. CallUrl('www>haydenplanetarium>org Their surface temperatures are 4000 K and 10 000 K respectively. the distances to many red giants have been determined to good accuracy. When brightest, Mira is visible to the naked eye; when dimmest, Mira can be viewed only with optical aid. a heavier element; the process stars use to produce energy to support It was discovered in 1596 by David Fabricus, an amateur Dutch astronomer. that has only just become a red giant may pulsate and vary in brightness Well not quite. The star swells up and turns red.SiriusThe brightest star in the night sky with an apparent magnitude of -1.4. As ~TildeLink()s age, they eventually cast off the outer layers of their surfaces. The brightness changes from 3rd mag to 9th mag within 330 days. Our own Sun, for example, might eventually turn into a red supergiant. See "The Complexity of Stellar Death" by Yervant Terzian, "Science" vol.
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