Procyon B Polaris Vega It is fusing hydrogen at its core. It has lost its outer shell and retained only a hot core that is slowly losing its brightness. Its temperature has decreased, but it is shining brighter than before.
Procyon B Polaris Vega It is fusing hydrogen at its core. It has lost its outer shell and retained only a hot core that is slowly losing its brightness. Its temperature has decreased, but it is shining brighter than before.
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:idreas e
Drag the tiles to the boxes to form correct pairs.
Use the Hertzsprung-Russell diagram to determine which condition describes each star. Use the arrows to help you locate the stars.
Solar Rad
10 60 M
30 M
10 Solar Rad
Deneb
Centaur
105
Rgel
SUPERGIANTS
Betegese
Spica
10 M
Litetime
10' yrs
Canopus
Artares
10
Belax
Polaris
M
Achemar
SEQUENCE
10
MAIN
GIANTS
Lifetime
ctrus
Aldebaran
102
10 yrs
Pollux
Sius
Vega
10
Atar
Lifetime
10 yrs
aCentaun A
Sun
Centaurn B
dar
61 Cygni A
ei Cyoni B
Lacae 9052
0.3 M
Ce
Litetime
1010 yrs
01
Giese 725 A
Glese 725 B
0.1 M
Ross 128
Sinus B
WHITE
DWARFS
10
Barnard's Star
Lifetime
1011 yrs
Wolf 359
Proxma Centau
DX Canon
109
Procyon B-
104
105
A F G
км
10.000
6.000
3,000
30.000
decreasng
increasing
surface temperature (Kelvin)
temperature
temperature
s reserved.
NOV
33,806
luminosity (solar units)

Transcribed Image Text:Wolf 359
Proena Centu
Procyon B
DX Canos
A FG
30 000
10.000
6.000
3,000
noasng
temperature
surface temperature (Kelvin)
docreasing
temperature
Procyon B
Polaris
Vega
It is fusing hydrogen at its core.
It has lost its outer shell and retained only a hot core that is slowly losing its
brightness.
Its temperature has decreased, but it is shining brighter than before.
Reset
Next
33,806
NOV
15
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