Gamma Lupi (star)
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| Gamma Lupi A | |
| Spectral | B2 IV |
| Type | Subgiant |
| Multiple | Trinary |
| Luminosity | 5000 LSol |
| Absolute magnitude | -2.4 |
| Mag Terra | 2.77 |
| Temperature | 20,900° K |
| Mass | 9.5 MSol |
| Companion | Gamma Lupi Ab / Gamma Lupi B |
| Gamma Lupi Ab | |
| Spectral | |
| Type | |
| Luminosity | LSol |
| Absolute magnitude | |
| Temperature | ° K |
| Gamma Lupi B | |
| Spectral | |
| Type | |
| Luminosity | LSol |
| Absolute magnitude | |
| Temperature | ° K |
The star Gamma Lupi is a trinary star system.
- It can be resolved into a binary star system in close orbit known as the Gamma Lupi AB system (often abbreviated as γ Lup AB), orbiting each other with a period of about 190 years. Gamma Lupi A is itself a spectroscopic binary (Gamma Lupi Ab) with a period of about 2.81 days.
- It lies in the general region of Arzul Sector, far to coreward-trailing of Sol.
Description (Specifications)[edit]
The Gamma Lupi star system is approximately 129pc from Terra, and is located in a Coretrailing/Trailing direction from Terra at bearing 333.2o Galactic Longitude and +11.9o North Galactic Latitude.
History & Background (Dossier)[edit]
Though it shares a similar name, the star Gamma Lupi has no relationship with the world Gamma Lupus 2/Ilelish (Ilelish 2704).
References & Contributors (Sources)[edit]
| This article has metadata. |
| This page uses content from Wikipedia. The original article was at Gamma_Lupi. The list of authors can be seen in the page history. The text of Wikipedia is available under the Commons Attribution-ShareAlike 3.0 Unported License. |
This list of sources was used by the Traveller Wiki Editorial Team and individual contributors to compose this article. Copyrighted material is used under license from Mongoose Publishing or by permission of the author. The page history lists all of the contributions.
- EXTERNAL LINK: SIMBAD @ University of Strasbourg: [1]
- Author & Contributor: WHULorigan