3) indicate which locations in the H-R diagram correspond to places where the evolution is slow. Answers should be in the order they occur in the star. For example, if, in order, E, I and A are locations where there is a long time between changes, then enter EIA. (HINT: There are exactly three of them Hint: Hint: Our sun will be stable for another 4 billion years and white dwarfs last a long time because they are small. Really good additional hint: There are 3 places where the evolution is slow. Info below is what each of the labels are.  1) red giant, helium flash A 2) white dwarf F 3) red giant with helium burning shell B 4) hydrogen fusion in shell around core I 5) helium fusion in core D 6) envelope ejected, planetary nebula H 7) main-sequence star C 8) helium used up, core collapses G 9) hydrogen used up, core collapses E

College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...
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 3) indicate which locations in the H-R diagram correspond to places where the evolution is slow. Answers should be in the order they occur in the star. For example, if, in order, E, I and A are locations where there is a long time between changes, then enter EIA. (HINT: There are exactly three of them

Hint: Hint: Our sun will be stable for another 4 billion years and white dwarfs last a long time because they are small. Really good additional hint: There are 3 places where the evolution is slow.

Info below is what each of the labels are. 

1) red giant, helium flash A
2) white dwarf F
3) red giant with helium burning shell B
4) hydrogen fusion in shell around core I
5) helium fusion in core D
6) envelope ejected, planetary nebula H
7) main-sequence star C
8) helium used up, core collapses G
9) hydrogen used up, core collapses E

10
10
10'
10
H.
G.
D
10
E
0.1
10*
10
C
F
10*
main sequence
10*
10,000
5000
Surface Temperature (kelvin)
3000
Solar Luminosity
Transcribed Image Text:10 10 10' 10 H. G. D 10 E 0.1 10* 10 C F 10* main sequence 10* 10,000 5000 Surface Temperature (kelvin) 3000 Solar Luminosity
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