DEN 1048-3956
From Infogalactic: the planetary knowledge core
| 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]:{{{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]
Contents
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found.
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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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