Lambda Aurigae
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Lambda Aurigae is a Sun-like[10] star in the northern constellation of Auriga.[14] Its name is a Bayer designation that is Latinized from λ Aurigae, and abbreviated Lambda Aur or λ Aur. This star is visible to the naked eye with an apparent visual magnitude of 4.71.[2] Based upon parallax measurements, it is Template:Convert distant from the Earth.[1] The star is drifting further away with a high radial velocity of +66.5 km/s,[5] having come to within Template:Convert some 117,300 years ago.[15] It has a high proper motion, traversing the celestial sphere at the rate of Template:Val per year.[16]
Properties
This is a G-type main sequence star with a stellar classification of G1 V.[3] It is sometimes listed with a class of G1.5 IV-V Fe-1,[4] which indicates the spectrum is showing some features of a more evolved subgiant star along with a noticeable underabundance of iron. In terms of composition it is similar to the Sun, while the mass and radius are slightly larger.[7] It is 73% more luminous than the Sun[3] and radiates this energy from its outer atmosphere at an effective temperature of Template:Val.[9] At this heat, the star glows with the yellow hue of a G-type star.[17] It has a low level of magnetic activity and is a candidate Maunder minimum analog.[18]
Lambda Aurigae has been examined for the presence of excess infrared emission that may indicate the presence of a circumstellar disk of dust, but no significant surplus has been observed.[10] It is a possible member of the Epsilon Indi Moving Group of stars that share a common motion through space. The space velocity components of this star are [U, V, W] = [+76, –39, –6] km/s.[19]
Name
This star may have been called by the name Al Hurr, meaning the fawn in Arabic.[20] Lambda Aurigae, along with μ Aur and σ Aur, were Kazwini's Al Ḣibāʽ (ألحباع), the Tent.[20] According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Ḣibāʽ were the title for three stars : λ Aur as Al Ḣibāʽ I, μ Aur as Al Ḣibāʽ II and σ Aur as Al Ḣibāʽ III.[21]
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Pool of Harmony, refers to an asterism consisting of λ Aurigae, ρ Aurigae and HD 36041.[22] Consequently, the Chinese name for λ Aurigae itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[23]
Observation
From Earth, Lambda Aurigae has an apparent magnitude of 4.71. The closest large neighboring star to Lambda Aurigae is Capella, located Template:Convert away.[24] Hypothetically viewed from Lambda Aurigae, Capella's quadruple star system would have an apparent magnitude of approximately -5.48,[25] about 40 times brighter than Sirius can be seen at maximum brightness from Earth.[26]
References
External links
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- Pages with script errors
- G-type main-sequence stars
- G-type subgiants
- Solar-type stars
- Maunder Minimum
- Auriga
- Bayer objects
- Bright Star Catalogue objects
- Durchmusterung objects
- Flamsteed objects
- Gliese and GJ objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Stars with proper names
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