Classification of Starsearthtoreilly.com/documents/modern-astronomy/Keynote...Earth Science...
Transcript of Classification of Starsearthtoreilly.com/documents/modern-astronomy/Keynote...Earth Science...
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Classification of StarsHow do we classify the billions of stars that
exist in our galaxy and Universe?
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How Big?
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• Star - sphere of gas held together by gravity that produces tremendous amounts of energy and shines
• Creates energy by nuclear fusion
• Majority of known matter!in the galaxy
Classification of Stars
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•Absolute Magnitude - how bright a star appears to an observer on Earth
• Factors that Affect Absolute Magnitude:
• Temperature
• Size
•Distance
Classification of Stars
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•Absolute Brightness - the actual brightness of stars compared at a distance of 32.6 light years
• Factors that Affect Absolute Brightness:
• Temperature
• Size
Classification of Stars
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• Spectral Class - classification of stars based on analyzing the electromagnetic radiation emitted
•Electromagnetic radiation is split with a prism into the rainbow of colors and spectral lines
Classification of Stars
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Spectral Class
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Spectral Class O28,000 K - 50,000 K
Spectral Class B10,000 K - 28,000 K
Spectral Class A7,500 K - 10,000 K
Spectral Class F6,000 K - 7,500 K
Spectral Class G5,000 K - 6,000 K
Spectral Class K3,500 K - 5,000 K
Spectral Class M2,500 - 3,500 K
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• Luminosity - a measure of the rate of energy output
•Our Sun is the baseline with 1 energy unit
•Graphed on a logarithmic [non-linear] scale
Classification of Stars
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• Logarithmic [non-linear] Scale:
Classification of Stars
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•H-R Diagram - chart used to describe the relationship between a star’s surface temperature and luminosity
•Developed by Ejner Hertzsprung of Denmark and Henry N. Russell of the United States
Classification of Stars
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H-R Diagram
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Earth Science Reference Tables
(Name in italics refers to star represented by a .)
(Stages indicate the general sequence of star development.)
Color
Surface Temperature (K)
0.0001
0.001
0.01
0.1
1
10
100
1,000
10,000
100,000
1,000,000
Lu
min
osi
ty(R
ate
at w
hich
a s
tar
emits
ene
rgy
rela
tive
to th
e S
un)
20,000 10,000 8,000 6,000 4,000 3,000
Blue Blue White White Yellow
2,000
RedOrange
Sirius
Spica
Polaris
Rigel
Deneb Betelgeuse
SUPERGIANTS(Intermediate stage)
(Intermediate stage)GIANTS
Barnard’sStar
ProximaCentauri
Pollux
Alpha Centauri
Aldebaran
Sun
Procyon B SmallStars
MassiveStars
WHITE DWARFS(Late stage)
MAIN SEQUENCE
(Early stage)
40 Eridani B
30,000