Supriya Ghosh (Editor)

Triangulum II

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Right ascension
  
02 13 17.4

Constellation
  
Triangulum

Declination
  
+36° 10′ 42.4″

Apparent size (V)
  
3.9′

Mass/Light ratio
  
3600 (V) M☉/L☉

Triangulum II tvmaxisciencescomthumbnails6815w620jpg

Distance (comoving)
  
30 ± 2 kpc (97.8 ± 6.5 kly)

Distance
  
97.8 ± 6.5 kly (30 ± 2 kpc)

Similar
  
Hercules, Phoenix Dwarf, Willman 1, Ursa Major II Dwarf, Leo IV

Triangulum II (Tri II or Laevens 2) is a dwarf galaxy close to the Milky Way Galaxy. It contains only 1000 stars, yet is quite massive, having a solar mass to light ratio of 3600. This is an unusually high mass for such a small galaxy.

The distance from the centre of the Milky Way is 26 kpc (85 kly). The luminosity is 450 times that of the Sun. This makes it one of the dimmest known galaxies. The 2D half light radius is 34 pc (110 ly). The galaxy was discovered in images taken by Pan-STARRS by Benjamin P. M. Laevens in 2015.

Triangulum II is a candidate for detecting WIMPs as a source of dark matter.

References

Triangulum II Wikipedia