O stars

An Introduction to Physical Science
14th Edition
ISBN:9781305079137
Author:James Shipman, Jerry D. Wilson, Charles A. Higgins, Omar Torres
Publisher:James Shipman, Jerry D. Wilson, Charles A. Higgins, Omar Torres
Chapter18: The Universe
Section: Chapter Questions
Problem 2AYK
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In the H-R diagram we see that stellar masses__________ downward along the main sequence. At the upper end of the main sequence, the hot, luminous O stars can have masses as high as _________ or more times that of the Sun. On the lower end, cool, dim M stars may have as little as __________ times the mass of the Sun. Many more stars fall on the lower end of the main sequence than on the upper end, which tells us that _________stars are much more common than __________ stars.

luminosity (solar units)
106
105
104
10³
10²
10
-
0.1
10-²
10-3
10-4
10-5
-60M Sun
-30M Sun
Lifetime
107 yrs
O
10M Sun
Lifetime
108 yrs
30,000
B
6M Sun
Lifetime
10⁹ yrs
3M Sun
Sun-
Lifetime
1010 yrs
1.5M Sun
Lifetime
10¹1 yrs
A
F G
10,000 6000
surface temperature (K)
1M Sun
K M
0.3M Sun
0.1M Sun
3000
Transcribed Image Text:luminosity (solar units) 106 105 104 10³ 10² 10 - 0.1 10-² 10-3 10-4 10-5 -60M Sun -30M Sun Lifetime 107 yrs O 10M Sun Lifetime 108 yrs 30,000 B 6M Sun Lifetime 10⁹ yrs 3M Sun Sun- Lifetime 1010 yrs 1.5M Sun Lifetime 10¹1 yrs A F G 10,000 6000 surface temperature (K) 1M Sun K M 0.3M Sun 0.1M Sun 3000
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