Van Maanen's Star (star)
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| Van Maanen's Star | |
| Spectral | DZ8 |
| Type | White Dwarf (Degenerate Dwarf) |
| Luminosity | 0.00017 LSol |
| Absolute magnitude | 14.23 |
| Mag Terra | 12.374 |
| Temperature | 6220° K |
| Mass | 0.68 MSol |
| Radius | 0.011 RSol |
The star Van Maanen's Star (otherwise known as Van Maanen 2 or Wolf 28) is a white degenerate dwarf stellar core remnant that is the closest solitary degenerate dwarf to the Sol star system.
Description (Specifications)[edit]
As a degenerate dwarf, the composition of the star is largely composed of collapsed atomic matter quantum mechanically supported by electron gas in a degenerate state due to the Pauli Exclusion Principle. Though not currently undergoing nuclear fusion, the star radiates electromagnetic radiation at a high temperature due to trapped heat within the remnant as it slowly cools.
- Despite the star's evolutionary history, there is a circumstellar ring of planetary matter in orbit about Van Maanen's Star.
- The Van Maanen's Star star system lies approximately 4.26pc from Terra, and is located in a Spinward direction from Terra at bearing 121.9o Galactic Longitude and -57.5o South Galactic Latitude.
History & Background (Dossier)[edit]
No information currently available.
References & Contributors (Sources)[edit]
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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]
- Traveller Wiki Editorial Team
- Author & Contributor: WHULorigan
- Author & Contributor: Lord (Marquis) and Master of Sophontology Maksim-Smelchak of the Ministry of Science