Community hub
Recent from talks
Contribute something to knowledge base
Content stats: 0 posts, 0 articles, 0 media, 0 notes
Members stats: 0 subscribers, 0 contributors, 0 moderators, 0 supporters
Subscribers
Supporters
Contributors
Moderators
Hub AI
Mu1 Gruis AI simulator
(@Mu1 Gruis_simulator)
Hub AI
Mu1 Gruis AI simulator
(@Mu1 Gruis_simulator)
Mu1 Gruis
Mu1 Gruis, Latinized from μ1 Gruis, is a binary star system in the southern constellation of Grus. It is visible to the naked eye with a combined apparent visual magnitude of 4.79. The distance to this system, as determined using an annual parallax shift of 11.44 mas as seen from the Earth, is around 275 light years. It is drifting closer with a heliocentric radial velocity of −5 km/s.
The pair orbit each other with a period of 19 years and an eccentricity of 0.56. The yellow-hued primary component is an evolved giant star with stellar classification of G III and visual magnitude 5.20. With the supply of hydrogen at its core exhausted, it cooled and expanded; at present it has nine times the girth of the Sun. The star is radiating 67 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,422 K.
The secondary component is magnitude 6.68 and classed as a G-type star, although its color index and absolute magnitude suggest it is of type A6.
Mu1 Gruis
Mu1 Gruis, Latinized from μ1 Gruis, is a binary star system in the southern constellation of Grus. It is visible to the naked eye with a combined apparent visual magnitude of 4.79. The distance to this system, as determined using an annual parallax shift of 11.44 mas as seen from the Earth, is around 275 light years. It is drifting closer with a heliocentric radial velocity of −5 km/s.
The pair orbit each other with a period of 19 years and an eccentricity of 0.56. The yellow-hued primary component is an evolved giant star with stellar classification of G III and visual magnitude 5.20. With the supply of hydrogen at its core exhausted, it cooled and expanded; at present it has nine times the girth of the Sun. The star is radiating 67 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,422 K.
The secondary component is magnitude 6.68 and classed as a G-type star, although its color index and absolute magnitude suggest it is of type A6.