2MASS J04414489+2301513
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Taurus |
| 2MASS J04414489+2301513 | |
| Right ascension | 04h 41m 44.898s[1] |
| Declination | +23° 01′ 51.39″[1] |
| Apparent magnitude (V) | |
| 2MASS J04414565+2301580 | |
| Right ascension | 04h 41m 45.652s[1] |
| Declination | +23° 01′ 58.07″[1] |
| Apparent magnitude (V) | 15.20[2] |
| Characteristics | |
| Spectral type | M8.5[3] |
| Astrometry | |
| Distance | 470 ± 50 ly (145 ± 15[4] pc) |
| 2MASS J04414565+2301580 | |
| Proper motion (μ) | RA: 5.6[2] mas/yr Dec.: −22.1[2] mas/yr |
| Details | |
| 2MASS J04414489+2301513 | |
| Mass | 19 ± 3 / 9.8 ± 1.8[4] MJup |
| Luminosity | 0.00347 / 0.00093[4] L☉ |
| Temperature | 2100 / 1800[4] K |
| Age | 1[3] Myr |
| 2MASS J04414565+2301580 | |
| Mass | 0.20+1.0 −0.05 M☉ / 35 ± 5[4] MJup |
| Luminosity | 0.14 / 0.00741[4] L☉ |
| Temperature | 3400 / 2800[4] K |
| Age | 1[3] Myr |
| Other designations | |
WDS J04417+2302AB | |
| Database references | |
| SIMBAD | 2M J044144 |
| 2M J044145 | |
2MASS J04414489+2301513 (often abbreviated as 2M J044144) is a young brown dwarf approximately 470 light years (145 parsecs) away with an orbiting companion about 5–10 times the mass of Jupiter.[5] The mass of the primary brown dwarf is roughly 20 times the mass of Jupiter and its age is roughly one million years.[3]
It is not clear whether this companion object is a sub-brown dwarf or a planet. The companion is very large with respect to its parent brown dwarf, and must have formed within 1 million years or so. This seems to be too big and too fast to form like a regular planet from a disk around the central object.[3]
| Companion | Mass | Observed separation (AU) | Discovery year |
| b | 7.5 ± 2.5 MJ | 15 ± 0.6 | 2010 |
2MASS J04414489+2301513 has another companion, 2MASS J04414565+2301580 (abbreviated as 2M J044145), which is another binary star. At a separation of 0.23 arcseconds to the northeast, it has a similar proper motion to 2M J044144 and is likely physically associated with the system.[6] The primary component has a spectral type of M4.5 and a red apparent magnitude of 14.2.[4] Both components seem to be accreting mass from their stellar disks, as shown by their emission lines.[4] The four stars have a total mass of only 26% of the Sun, making it the quadruple star system with the lowest mass known.[4]
See also
References
- 1 2 3 4 Cutri, R. M.; et al. (2003). "2MASS All-Sky Catalog of Point Sources". VizieR On-line Data Catalog. 2246. Bibcode:2003yCat.2246....0C.
- 1 2 3 Zacharias, N. (2012). "The fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". VizieR On-line Data Catalog. 1322. Bibcode:2012yCat.1322....0Z.
- 1 2 3 4 5 Todorov, K.; Luhman, K. L.; McLeod, K. K. (2010). "Discovery of a Planetary-Mass Companion to a Brown Dwarf in Taurus". The Astrophysical Journal. 714: L84. arXiv:1004.0539
. doi:10.1088/2041-8205/714/1/L84. - 1 2 3 4 5 6 7 8 9 10 Bowler, Brendan P.; Hillenbrand, Lynne A. (2015). "Near-infrared Spectroscopy of 2M0441+2301 AabBab: A Quadruple System Spanning the Stellar to Planetary Mass Regimes". The Astrophysical Journal. 811 (2): L30. Bibcode:2015ApJ...811L..30B. arXiv:1509.01658 . doi:10.1088/2041-8205/811/2/L30.
- ↑ "Hubble spots giant planet orbiting tiny star". USA Today. 2010-04-07. Retrieved 2013-02-24.
- ↑ Todorov, K. O.; Luhman, K. L.; Konopacky, Q. M.; McLeod, K. K.; Apai, D.; Ghez, A. M.; Pascucci, I.; Robberto, M. (2014). "A Search for Companions to Brown Dwarfs in the Taurus and Chamaeleon Star-Forming Regions". The Astrophysical Journal. 788: 40. Bibcode:2014ApJ...788...40T. arXiv:1404.0213 . doi:10.1088/0004-637X/788/1/40.
- Jean Schneider (2011). "Notes for star 2M J044144". Extrasolar Planets Encyclopaedia. Archived from the original on 19 January 2012. Retrieved 30 September 2011.