Kappa Geminorum
Binary star system with a giant primary used as a spectral anchor.
Kappa Geminorum (κ Geminorum, κ Gem) is a binary star system in the northern zodiac constellation of Gemini. It is visible to the naked eye with an apparent visual magnitude of 3.568 and is located about 141 light years distant from the Sun. The system is notable as a probable astrometric binary and for its primary component, an evolved G-type giant star whose spectrum has served as a stable anchor point for stellar classification since 1943.
- Apparent visual magnitude
- 3.568
- Distance
- 141 light years
- Parallax
- 23.07 mas
- Spectral type (primary)
- G9 III
- Mass (primary)
- 2 solar masses
- Radius (primary)
- 11 solar radii
- Luminosity (primary)
- 69 solar luminosities
- Effective temperature (primary)
- 5,020 K
- Projected rotational velocity (primary)
- 3.3 km/s
- Age (primary)
- 2 billion years
Lore & Background
In Chinese astronomy, Kappa Geminorum is called 積薪 (Jīxīn), meaning 'Pile of Firewood', because the star marks itself and stands alone in the Pile of Firewood asterism within the Well mansion. This name was westernized as Tseih Tsing, though R.H. Allen designated Tseih Tsing for χ Gem and μ Cnc with the meaning 'piled-up fuel'. In Japanese, the star is known as 隆博星 (Takahiro-boshi), meaning 'Esteemed Nobility Star'.
The system is a probable astrometric binary. As of 2014, the components had an angular separation of 7.2 arcseconds along a position angle of 241°. The primary is an evolved G-type giant star with a stellar classification of G9 III. Since 1943, its spectrum has been one of the stable anchor points by which other stars are classified. The primary has double the mass of the Sun but has expanded to 11 times the solar radius, radiating about 69 times the Sun's luminosity from its outer atmosphere at an effective temperature of 5,020 K. It shows a leisurely spin with a projected rotational velocity of 3.3 km/s and is around two billion years old. The secondary component is a magnitude 8.2 star.
Reader's Guide
Kappa Geminorum holds significance as a binary system whose primary component has been a fundamental reference for stellar classification since 1943. Its stable G9 III spectrum serves as an anchor point, meaning that astronomers compare the spectra of other stars against it to determine their types. This role makes the star a cornerstone in the empirical framework of stellar astrophysics. The system's probable astrometric binary nature, with a wide separation of 7.2 arcseconds, allows for direct study of its components, though the secondary is much fainter at magnitude 8.2. The primary's evolved state—a giant star with 11 times the Sun's radius and 69 times its luminosity—provides a clear example of post-main-sequence evolution for a star of about two solar masses. Its leisurely rotation and age of two billion years offer constraints on stellar evolution models. Culturally, the star's Chinese name Jīxīn (Pile of Firewood) and Japanese name Takahiro-boshi (Esteemed Nobility Star) reflect its recognition across different astronomical traditions, though the Chinese name was historically applied to other stars by Western sources. The system's visibility to the naked eye at magnitude 3.568 makes it accessible for amateur observation, while its spectral anchor status ensures its continued importance in professional astronomy.
Did You Know?
- Kappa Geminorum is a probable astrometric binary with components separated by 7.2 arcseconds as of 2014.
- In Chinese astronomy, it is called Jīxīn, meaning 'Pile of Firewood'.
- The primary is an evolved G9 III giant with 11 times the Sun's radius and 69 times its luminosity.
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