Triangulum II
Appearance
Coordinates: 02h 13m 17.4s, +36° 10′ 42.4″
Triangulum II | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Triangulum |
Right ascension | 02h 13m 17.4s[1] |
Declination | +36° 10′ 42.4″[1] |
Distance | 97.8 ± 6.5 kly (30 ± 2 kpc)[1] |
Characteristics | |
Mass/Light ratio | 3600 (V)[1] M☉/L☉ |
Apparent size (V) | 3.9′[1] |
Other designations | |
Triangulum II, Tri II, Laevens 2, Lae 2 |
Triangulum II (Tri II or Laevens 2) is a
Milky Way Galaxy. Like other dwarf spheroidal galaxies, its stellar population is very old: the galaxy was quenched before 11.5 billion years ago.[2] It contains only 1000 stars, yet is quite massive, having a solar mass to light ratio of 3600.[3] This is an unusually high mass for such a small galaxy.[4]
The distance from the centre of the Milky Way is 26 kpc (85 kly). The luminosity is 450 times that of the Sun.[3] This makes it one of the dimmest known galaxies.[3] 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.[1][3]
Triangulum II is a candidate for detecting
WIMPs as a source of dark matter.[4]
References
- ^ a b c d e f
Laevens, Benjamin P. M.; Martin, Nicolas F.; Ibata, Rodrigo A.; Rix, Hans-Walter; Bernard, Edouard J.; Bell, Eric F.; Sesar, Branimir; Ferguson, Annette M. N.; Schlafly, Edward F.; Slater, Colin T.; et al. (31 March 2015). "A New Faint Milky Way Satellite Discovered in the PAN-STARRS1 3π Survey" (PDF). The Astrophysical Journal. 802 (2): L18. S2CID 54179272.
- S2CID 236965965.
- ^ a b c d
Kirby, Evan N.; S2CID 13600560.
- ^ a b
Dajose, Lori (18 November 2015). "Dark matter dominates in nearby dwarf galaxy". Phys.org. Retrieved 19 November 2015.; Lori Dajose (November 18, 2015). "Dark Matter Dominates in Nearby Dwarf Galaxy". Caltech. Retrieved December 16, 2015.