Class G — G-type (Yellow)

G-type stars are yellow main-sequence stars with surface temperatures of 5,200 to 6,000 K. The Sun (G2V) is the most famous G-type star, making this class of particular importance for astrobiology. G-type stars comprise about 7.6% of main-sequence stars. Their spectra are dominated by calcium and iron absorption lines. Other notable G-type stars include Alpha Centauri A (G2V) and Tau Ceti (G8.5V). They have lifetimes of roughly 10 billion years.

G-type stars are yellow stars with surface temperatures between 5,200 and 6,000 K. They comprise about 7.6% of main-sequence stars, and their most famous member is our own Sun (G2V). G-type stars are central to the search for habitable exoplanets because they combine long lifetimes (7-15 billion years on the main sequence) with sufficient luminosity to maintain liquid water at moderate orbital distances — making them prime targets for missions like Kepler, TESS, and the upcoming PLATO.

Characteristics

G-type spectra are characterized by prominent ionized calcium (Ca II) H and K lines, neutral metal lines (especially iron), and the G-band — a molecular absorption feature near 430 nm caused by CH molecules that gives the spectral class its name. G stars have deep convective envelopes that drive magnetic dynamos, producing sunspot cycles, chromospheric activity, coronae, and stellar winds. Their masses range from 0.8 to 1.04 solar masses. G-type giants and supergiants exist at higher luminosities as evolved stars that have left the main sequence.

Notable Examples

The Sun (G2V) is the defining member, the only star whose surface features — granulation, sunspots, prominences — can be studied in exquisite detail. Alpha Centauri A (G2V) is a solar twin and the brightest component of our nearest stellar neighbor at 4.37 light-years. Tau Ceti (G8.5V) is one of the nearest Sun-like stars and has been a target of SETI programs since 1960's Project Ozma. Capella (Alpha Aurigae) is a binary of two G-type giants, the sixth-brightest star system in the sky.

HIP 108074HIP 108088HIP 108090HIP 108095HIP 108099HIP 108103HIP 108111HIP 108116HIP 108118HIP 108121HIP 10813HIP 108132HIP 108136HIP 108137HIP 108146HIP 108158HIP 108169HIP 108178HIP 10818HIP 108181HIP 108184HIP 108185HIP 108193HIP 10820HIP 108201HIP 108204HIP 108207HIP 108209HIP 10821HIP 108221HIP 108225HIP 108228HIP 108229HIP 108231HIP 108242HIP 108247HIP 10825HIP 108252HIP 108255HIP 108256HIP 108259HIP 108265HIP 108268HIP 108269HIP 10827HIP 108285HIP 108288HIP 108290

Frequently Asked Questions

What is a class G star?
Class G (G-type (Yellow)) stars are yellow stars. G-type stars are yellow main-sequence stars with surface temperatures of 5,200 to 6,000 K. The Sun (G2V) is the most famous G-type star, making this class of particular importance for astrobiology. G-
How hot are class G stars?
Class G stars have surface temperatures between 5,200 K and 6,000 K.
What color are class G stars?
Class G stars appear yellow.
How many class G stars are in the StarFYI database?
StarFYI currently catalogs 22,793 class G stars.
How luminous are class G stars?
Solar-like, 0.6-1.5 solar luminosities