spectral classification of stars jph 01/29/10 o b a f g k m hottest to coldest (temperature...
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![Page 1: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/1.jpg)
Spectral Classification of Stars
JPH 01/29/10
O B A F G K M
Hottest to Coldest (Temperature sequence)
Classification scheme due to Annie Jump Cannon (Harvard) (non-alphabetic ordering merely an historical accident)
Within each letter class also a numerical class 0-9 (Hot to Cold) for further refinement. Then a Roman Numeral (e.g., I, II, V) for luminosity class
Sun = G2V
A0 – A9Early to late A-type
![Page 2: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/2.jpg)
Spectral Classification of Stars
JPH 01/29/10
Luminosity classes (LC)Second parameter (pressure-dependent)• Super-supergiants 0 0-Ia Ia-0• Supergiants: Ia Iab Ib • Bright giants: IIa IIab IIb• Normal giants: IIIa IIIab IIIb• Subgiants IVa IVab IVb• Main Sequence V (also “dwarfs”)
a,ab,b: subclasses (in decreasing luminosity order)Transition classes (Ib-II also used)
![Page 3: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/3.jpg)
Spectral Classification of Stars
JPH 01/29/10
![Page 4: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/4.jpg)
Spectral Classification of Stars
JPH 01/29/10
O stars
• Atmospheric temperature: > 33,000 K• Hydrogen Balmer lines: weak• Other spectral features: Ionized Helium (He+) features
sometimes in emission, strong UV continuum • Parameters (in solar units)
– Mass 20-60
– Radius 9-15
– Luminosity 90,000 – 800,000
• Lifetime (M.S.): 10-1 Myr
![Page 5: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/5.jpg)
Spectral Classification of Stars
JPH 01/29/10
B stars
• Atmospheric temperature: 10,500-30,000 K • Hydrogen Balmer lines: medium• Other spectral features: Neutral He absorption • Parameters (in solar units):
– Mass 3-18
– Radius 3.0-8.4
– Luminosity 95-52,000
• Lifetime (M.S.): 400-11 Myr
![Page 6: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/6.jpg)
Spectral Classification of Stars
JPH 01/29/10
A stars
• Atmospheric temperature: 7,500-10,000 K• Hydrogen Balmer lines: strong• Other spectral features: H features maximum at A0,
some features of heavy elements, eg Ca+ • Parameters (in solar units):
– Mass 2.0-3.0
– Radius 1.7-2.7
– Luminosity 8-55
• Lifetime (M.S.): 3 Gyr – 440 Myr
![Page 7: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/7.jpg)
Spectral Classification of Stars
JPH 01/29/10
F stars
• Atmospheric temperature: 6,000-7,200 K • Hydrogen Balmer lines: medium• Other spectral features: Ca+ lines continue to increase
as Balmer lines weaken thru class (from 0 to 9)• Parameters (in solar units):
– Mass 1.1-1.6
– Radius 1.2-1.6
– Luminosity 2.0-6.5
• Lifetime (M.S.): 7-3 Gyr
![Page 8: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/8.jpg)
Spectral Classification of Stars
JPH 01/29/10
G stars
• Atmospheric temperature: 5,500-6,000 K • Hydrogen Balmer lines: weak• Other spectral features: Ca+ H&K, Na "D"
Sun is G2V • Parameters (in solar units):
– Mass 0.9-1.05
– Radius 0.85-1.1
– Luminosity 0.66-1.5
• Lifetime (M.S.): 15-8 Gyr
![Page 9: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/9.jpg)
Spectral Classification of Stars
JPH 01/29/10
K stars
• Atmospheric temperature: 4,000-5,250 K • Hydrogen Balmer lines: very weak• Other spectral features: Ca+, Fe,
strong molecules, eg CH, CN • Parameters (in solar units):
– Mass 0.6-0.8
– Radius 0.65-0.8
– Luminosity 0.10-0.42
• Lifetime (M.S.): 17 Gyr
![Page 10: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/10.jpg)
Spectral Classification of Stars
JPH 01/29/10
M stars
• Atmospheric temperature: 2,600-3,850 K • Hydrogen Balmer lines: very weak• Other spectral features: Molecules, eg TiO ,
very red continuum • Parameters (in solar units):
– Mass 0.08-0.5
– Radius 0.17-0.63
– Luminosity 0.001-0.08
• Lifetime (M.S.): 56 Gyr
![Page 11: Spectral Classification of Stars JPH 01/29/10 O B A F G K M Hottest to Coldest (Temperature sequence) Classification scheme due to Annie Jump Cannon (Harvard)](https://reader036.vdocuments.mx/reader036/viewer/2022082713/5697bffc1a28abf838cc1755/html5/thumbnails/11.jpg)
Spectral Classification of Stars
JPH 01/29/10
Other stars
• W = Wolf-Rayet (WR) stars – very massive – earlier than O-type – losing mass at high rate– WN = nitrogen rich– WC = carbon rich
• L = “stars” redder than M. May not be true stars (i.e., H burning) – brown dwarfs.
• "R", "N", "S" stars are cool stars with particular types of molecular bands.