Van Maanen's Star (star)

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Van Maanen's Star
Traveller Imperial Science Societies Sunburst logo.svg
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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