On A Hertzsprung Russell Diagram Where Would We Find Stars That Have The Largest Radii
Red giant and supergiant stars luminosity classes i through iii occupy the region above the main sequence. A upper right.
B lower right.
On a hertzsprung russell diagram where would we find stars that have the largest radii. On a hertzsprung russell diagram where would we find red giant stars. Study 74 chapter 15 flashcards from james d. They have low surface temperatures and high luminosities which according to the stefan boltzmann law means they also have large radii.
25 on a hertzsprung russell diagram where would we find stars that have the largest radii. B lower right. D a stars absolute magnitude is the apparent magnitude it would have if it were at a distance of 10 parsecs from earth.
B a star with apparent magnitude 1 is brighter than one with apparent magnitude 2. On a hertzsprung russell diagram where would we find stars that are cool and luminous. You will need to determine all of the following except the rotation rate of the star.
On a hertzsprung russell diagram where would we find white dwarfs. C the absolute magnitude of a star is another measure of its luminosity. You observe a star in the disk of a milky way and you want to plot the star on an h r diagram.
C upper left. D lower left. On a hertzsprung russell diagram where would we find stars that have the largest radii.
C upper left. E all of the above are true. On a hertzsprung russell diagram where would we find stars that have the largest radii.
D lower left. Main sequence stars have a morgan keenan luminosity class labelled v. 24 on a hertzsprung russell diagram where would we find stars that are cool and luminous.
B a star with apparent magnitude 1 is brighter than one with apparent magnitude 2. A the magnitude system that we use now is based on a system used by the ancient greeks over 2000 years ago that classified stars by how bright they appeared. A upper right.
Compared to a high luminosity main sequence star stars in the upper right of the h r diagram are.
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