Astrophysics (Index)About

G-type star

(G, G-class star)
(stars spectrally similar to the Sun)

A G-type star is a star within the G-class, a spectral class for stars with metal and weak hydrogen absorption lines, a yellow color and a surface temperature in the range of 5300-6000 K. The spectral energy distribution (SED) peak is within the visible range. The Sun is a main sequence star within this class. Such main sequence stars (aka yellow dwarfs or G dwarfs) burn their hydrogen in on the order of ten billion years. Characteristics of G-type main sequence stars:

0.96-1.15radius(solar)
0.8-1.04mass(solar)
+4.3 to +5.3absolute magnitude(bolometric)
0.6-1.5bolometric luminosity(solar)
9-18 billion yearsmain-sequence lifetime
7.5%abundance

Some example G-type stars are Alpha Centauri and T Tauri (a pre-main-sequence star). Giant stars can also fall in the G-class (yellow giants), including supergiants (yellow supergiants) and hypergiants (yellow hypergiants).


(star type,spectral class)
Further reading:
https://en.wikipedia.org/wiki/Stellar_classification#Class_G
https://en.wikipedia.org/wiki/G-type_main-sequence_star
https://en.wikipedia.org/wiki/Giant_star#Yellow_giants
https://en.wikipedia.org/wiki/Yellow_supergiant
https://chview.nova.org/solcom/stars3/100-gs.htm
https://lweb.cfa.harvard.edu/~pberlind/atlas/htmls/gstars.html
WaveLFreqPhoton
Energy
  
387nm775THz3.3eVbeginG-type star
527nm569THz2.4eVendG-type star

Referenced by pages:
16 Cygni (16 Cyg)
51 Pegasi b (51 Peg b)
barium star (Ba star)
calcium (Ca)
carbon star (C)
Earth analog
FGK star
G band (G)
G-dwarf problem
HD 133131
HD 209458 b
HD 80606 b
Kepler Telescope
Kepler-1625b
Kepler-452b
M-type star (M)
Malmquist bias
Morgan classification
multiplicity fraction
RR Lyrae variable (RRL)
solar mass (MSun)
spectral class
Spectroscopic Properties of Cool Stars (SPOCS)
Sun
Transiting Exoplanet Survey Satellite (TESS)
WASP-12b
Wilson-Bappu effect

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