1. The plots luminosity in solar units on an X and Y axis. 2. If an excessive mass transfer from a companion star to a White Dwarf, it can cause a 3. In once helium fusion has occurred, the core will never get hot or dense enough to fuse any additional elements, so the star begins to die.
1. The plots luminosity in solar units on an X and Y axis. 2. If an excessive mass transfer from a companion star to a White Dwarf, it can cause a 3. In once helium fusion has occurred, the core will never get hot or dense enough to fuse any additional elements, so the star begins to die.
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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Transcribed Image Text:Word Bank: average star, Type la supernova, red supergiant, supergiants, dwarfs, red giants, low mass
star, Hertzsprung-Russell, stellar nebula, Absolute Magnitude, Apparent Magnitude, red giant, supernova,
white dwarf, planetary nebula, high mass star, spiral galaxies, lenticular galaxies, elliptical galaxies,
irregular galaxies.
1. The
plots luminosity in solar units on an X and Y axis.
2. If an excessive mass transfer from a companion star to a White Dwarf, it can cause a
3. In
once helium fusion has occurred, the core will never get hot or dense enough
to fuse any additional elements, so the star begins to die.
4. In
the temperature and pressure in the core can reach high enough values that
carbon fusion can begin, and then oxygen fusion can begin and continue to power the star.
5. More than two-thirds of all observed galaxies are
6. The brightest stars are called
7. Star clusters are rich in stars just off the main sequence called
8. Main sequence stars are called
9. The faint, hot stars are called
10.
is the magnitude the star would have if it were placed at a distance of 10
parsecs from the Earth.
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