6. Figure 1 is an excerpt of the evolution of both components of a binary star (that is, there are missing phases, do not let that distract you). For each phase (A-G), explain what is going on in 1-2 sentences. To do so, focus on the columns that show the evolution time, the masses for each star, the stellar types for each star, the "what's happening?" and the pictorial representation of the binary. Your explanation cannot just a paraphrase of the "what's happening?" column.

Applications and Investigations in Earth Science (9th Edition)
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Chapter1: The Study Of Minerals
Section: Chapter Questions
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6.
A
C
D
E
B 12.1376 15.508
LL
F
Figure 1 is an excerpt of the evolution of both components of a binary star (that is, there are missing
phases, do not let that distract you). For each phase (A-G), explain what is going on in 1-2 sentences. To
do so, focus on the columns that show the evolution time, the masses for each star, the stellar types for
each star, the "what's happening?" and the pictorial representation of the binary. Your explanation cannot
just a paraphrase of the "what's happening?" column.
G
Evolution Star I mass Star 2 mass
Time
(M₂) (Mo)
(Myr)
0.0000
12.1492 15.488
13.3297 5.236
13.3891 1.503
16.000
19.8877 1.503
19.9555 1.503
(uns / ០015o|
5.2
5.1
5.0
4.9
4.8
4.7
4.6
4.5
4.4
4.3
4.2
4.5
12.000
11.935
11.938
12.374
12.465
11.564
1.408
Star I type
Main Sequence
Core Helium
Burning
Core Helium
Burning
Glant Branch
Naked Helium
star
Neutron Star
Neutron Star
Neutron Star
Star 2 type
Main Sequence
Main Sequence 1019.9
Main Sequence
Main Sequence 1020
Main Sequence
Separation
(R)
1000.5
Neutron Star
4.2
41.721
Early Asymptotic 53.104
Giant Branch
-53.104
-53.104
Star I
Period Eccentricity R/R
693.140.00
720.60 0.00
720.93 0.00
7.44 0.00
-1.00
-1.00
-1.00
4.0
log10(Teff0/K)
Star
2 What's happening?
R/R
0.013 0.012 Hydrogen ignition
0.717 0.018 Begin Symbiotic
1.000 0.018 Begin Roche Lobe
Overflow
26.1160.378 Invert Mass Ratio
0.398 Stellar Type Change
Figure 1: Summary of binary evolution
Stellar Type Change
Mers(5)=0.799477
3.8
3.6
4100
24
3.5
Transcribed Image Text:6. A C D E B 12.1376 15.508 LL F Figure 1 is an excerpt of the evolution of both components of a binary star (that is, there are missing phases, do not let that distract you). For each phase (A-G), explain what is going on in 1-2 sentences. To do so, focus on the columns that show the evolution time, the masses for each star, the stellar types for each star, the "what's happening?" and the pictorial representation of the binary. Your explanation cannot just a paraphrase of the "what's happening?" column. G Evolution Star I mass Star 2 mass Time (M₂) (Mo) (Myr) 0.0000 12.1492 15.488 13.3297 5.236 13.3891 1.503 16.000 19.8877 1.503 19.9555 1.503 (uns / ០015o| 5.2 5.1 5.0 4.9 4.8 4.7 4.6 4.5 4.4 4.3 4.2 4.5 12.000 11.935 11.938 12.374 12.465 11.564 1.408 Star I type Main Sequence Core Helium Burning Core Helium Burning Glant Branch Naked Helium star Neutron Star Neutron Star Neutron Star Star 2 type Main Sequence Main Sequence 1019.9 Main Sequence Main Sequence 1020 Main Sequence Separation (R) 1000.5 Neutron Star 4.2 41.721 Early Asymptotic 53.104 Giant Branch -53.104 -53.104 Star I Period Eccentricity R/R 693.140.00 720.60 0.00 720.93 0.00 7.44 0.00 -1.00 -1.00 -1.00 4.0 log10(Teff0/K) Star 2 What's happening? R/R 0.013 0.012 Hydrogen ignition 0.717 0.018 Begin Symbiotic 1.000 0.018 Begin Roche Lobe Overflow 26.1160.378 Invert Mass Ratio 0.398 Stellar Type Change Figure 1: Summary of binary evolution Stellar Type Change Mers(5)=0.799477 3.8 3.6 4100 24 3.5
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