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- Q426726 subject Q7009495.
- Q426726 subject Q7465898.
- Q426726 subject Q7465903.
- Q426726 subject Q7724325.
- Q426726 subject Q8293947.
- Q426726 subject Q8759509.
- Q426726 abstract "Lambda Aurigae (λ Aur, λ Aurigae) is the Bayer designation for a solar analog star in the northern constellation of Auriga. It has the traditional name Al Hurr and is visible to the naked eye with an apparent visual magnitude of 4.71. Based upon parallax measurements made during the Hipparcos mission, it is approximately 41.2 light-years (12.6 parsecs) distant from the Earth.This is a G-type main sequence star with a stellar classification of G1 V. In terms of composition it is similar to the Sun, while the mass and radius are slightly larger. It is 73% more luminous than the Sun and radiates this energy from its outer atmosphere at an effective temperature of 7003589000000000000♠5890 K. At this heat, the star glows with the yellow hue of a G-type star. It has a low level of surface activity and is a candidate Maunder minimum analog.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. 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.".
- Q426726 thumbnail Auriga_IAU.svg?width=300.
- Q426726 wikiPageExternalLink AladinPreview?-c=05+19+08.4745%2B40+05+56.586&ident=LHS++1753&submit=Aladin+previewer.
- Q426726 wikiPageWikiLink Q1045111.
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- Q426726 wikiPageWikiLink Q1326555.
- Q426726 wikiPageWikiLink Q15705.
- Q426726 wikiPageWikiLink Q165074.
- Q426726 wikiPageWikiLink Q1748548.
- Q426726 wikiPageWikiLink Q179600.
- Q426726 wikiPageWikiLink Q2143996.
- Q426726 wikiPageWikiLink Q2402973.
- Q426726 wikiPageWikiLink Q3232710.
- Q426726 wikiPageWikiLink Q499138.
- Q426726 wikiPageWikiLink Q523.
- Q426726 wikiPageWikiLink Q525.
- Q426726 wikiPageWikiLink Q555846.
- Q426726 wikiPageWikiLink Q5864.
- Q426726 wikiPageWikiLink Q6311.
- Q426726 wikiPageWikiLink Q6440.
- Q426726 wikiPageWikiLink Q7009495.
- Q426726 wikiPageWikiLink Q7465898.
- Q426726 wikiPageWikiLink Q7465903.
- Q426726 wikiPageWikiLink Q7724325.
- Q426726 wikiPageWikiLink Q7850.
- Q426726 wikiPageWikiLink Q827568.
- Q426726 wikiPageWikiLink Q8293947.
- Q426726 wikiPageWikiLink Q845735.
- Q426726 wikiPageWikiLink Q850950.
- Q426726 wikiPageWikiLink Q854050.
- Q426726 wikiPageWikiLink Q8759509.
- Q426726 wikiPageWikiLink Q8928.
- Q426726 wikiPageWikiLink Q984158.
- Q426726 type Place.
- Q426726 type CelestialBody.
- Q426726 type Location.
- Q426726 type Place.
- Q426726 type Star.
- Q426726 type Thing.
- Q426726 comment "Lambda Aurigae (λ Aur, λ Aurigae) is the Bayer designation for a solar analog star in the northern constellation of Auriga. It has the traditional name Al Hurr and is visible to the naked eye with an apparent visual magnitude of 4.71. Based upon parallax measurements made during the Hipparcos mission, it is approximately 41.2 light-years (12.6 parsecs) distant from the Earth.This is a G-type main sequence star with a stellar classification of G1 V.".
- Q426726 label "Lambda Aurigae".
- Q426726 depiction Auriga_IAU.svg.
- Q426726 name "Lambda Aurigae".