DEN 1048−3956
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Antlia |
| Right ascension | 10h 48m 14.640s[1] |
| Declination | −39° 56′ 06.24″[1] |
| Apparent magnitude (V) | 17.4[2] |
| Characteristics | |
| Spectral type | M9 V or L0 |
| Apparent magnitude (J) | 9.5[1] |
| Astrometry | |
| Radial velocity (Rv) | −10.1 ± 0.5[1] km/s |
| Proper motion (μ) | RA: −1198 ± 10[1] mas/yr Dec.: −970 ± 8[1] mas/yr |
| Parallax (π) | 248.08 ± 0.61[3] mas |
| Distance | 13.15 ± 0.03 ly (4.031 ± 0.010 pc) |
| Absolute magnitude (MV) | 19.37[2] |
| Details | |
| Mass | 0.07[2] M☉ |
| Luminosity | 0.00000356 L☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Data sources: | |
| Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) | |
DEN 1048−3956 is a brown dwarf about 13 light years from Earth in the southern constellation of Antlia, among the closest interstellar objects to Earth. This substellar object is very dim with an apparent magnitude of about 17,[2] and will require a telescope with a camera to be seen. It was discovered in 2000 by Xavier Delfosse (Institute of Astrophysics of the Canary Islands, now Observatoire de Grenoble) and Thierry Forveille (Canada–France–Hawaii Telescope Corporation), with the assistance of nine other astronomers.
In 2005 a powerful flare from this object was detected by radio astronomy.[4]
See also
References
- 1 2 3 4 5 6 "2MASSI J1048147-395606 -- Brown Dwarf (M<0.08solMass)". Centre de Données astronomiques de Strasbourg. Retrieved 2009-12-15.
- 1 2 3 4 "The One Hundred Nearest Star Systems". RECONS. Georgia State University. January 1, 2009. Retrieved 2011-12-03.
- ↑ Lurie, John C.; Henry, Todd J.; Jao, Wei-Chun; Quinn, Samuel N.; Winters, Jennifer G.; Ianna, Philip A.; Koerner, David W.; Riedel, Adric R.; Subasavage, John P. (2014). "The Solar Neighborhood. XXXIV. a Search for Planets Orbiting Nearby M Dwarfs Using Astrometry". The Astronomical Journal 148 (5): 91. arXiv:1407.4820. Bibcode:2014AJ....148...91L. doi:10.1088/0004-6256/148/5/91.
- ↑ Adam J. Burgasser1 and Mary E. Putman (June 10, 2005). "Quiescent Radio Emission from Southern Late-Type M Dwarfs and a Spectacular Radio Flare from the M8 Dwarf DENIS 1048−3956". The Astrophysical Journal 626 (1): 486–497. arXiv:astro-ph/0502365. Bibcode:2005ApJ...626..486B. doi:10.1086/429788.
- Deacon, N. R.; Hambly, N. C. (2001). "The trigonometric parallax of DENIS-P J104814.7-395606.1". Astronomy and Astrophysics 380: 148–150. Bibcode:2001A&A...380..148D. doi:10.1051/0004-6361:20011290.
- Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Ianna, Philip A.; Bartlett, Jennifer L.; Costa, Edgardo; Méndez, René A. (2005). "The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with mu >= 1.0" yr-1 (MOTION Sample)". The Astronomical Journal 129 (4): 1954–1967. arXiv:astro-ph/0502167. Bibcode:2005AJ....129.1954J. doi:10.1086/428489.
- Costa, Edgardo; Méndez, René A.; Jao, W.-C.; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Ianna, Philip A.; Bartlett, Jennifer (2005). "The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation-First Results from the 1.5 m Telescope Program". The Astronomical Journal 130 (1): 337–349. Bibcode:2005AJ....130..337C. doi:10.1086/430473.
Notes
External links
- Image Den 1048-3956
- The nearest stars: DEN 1048-3956
- M dwarfs, L dwarfs and T dwarfs
- Parallax Investigation Results
- Infrared Photometry from 2Mass and Denis
- Image 2Mass J10481463-3956062
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