SCR 1845-6357
SCR 1845-6357 is a binary system, about 12.6 light-years away in the constellation Pavo. The primary is a faint red dwarf. It has a brown dwarf companion.
SCR 1845-6357 A
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Pavo |
Right ascension | 18h 45m 05.26s[1] |
Declination | −63° 57′ 47.8″[1] |
Apparent magnitude (V) | 17.4[2] |
Characteristics | |
Spectral type | M8.5[3] |
Astrometry | |
Proper motion (μ) | RA: 2444[2] mas/yr Dec.: 696[2] mas/yr |
Parallax (π) | 259.45 ± 1.11[1] mas |
Distance | 12.57 ± 0.05 ly (3.85 ± 0.02 pc) |
Details | |
Mass | 0.07 [4] M☉ |
Radius | 0.096 R☉ |
Luminosity | 0.0004 L☉ |
Temperature | 2600–2700[3] K |
Other designations | |
The primary, SCR 1845-6357A, is a faint (apparent magnitude 17.4)[2] red dwarf star with a mass of about 7% of the Sun's. However, the measurements are still preliminary and are subject to change.[4]
SCR 1845-6357 B
Position (relative to A) | |
---|---|
Epoch of observation | J2006.3 |
Angular distance | 1.064 ± 0.004″ [3] |
Position angle | 177.2 ± 0.06° [3] |
Observed separation (projected) | 4.10 ± 0.04 AU [5] |
Characteristics | |
Spectral type | T6 [3] |
Apparent magnitude (J) | 13.26[6] |
Details | |
Mass | 0.04 to 0.05 [3] M☉ |
Surface gravity (log g) | 5.1 [3] cgs |
Temperature | 950 [3] K |
Age | 1.8·109 to 3.1·109 [3] years |
Other designations | |
This star has been found to possess a brown dwarf companion, designated SCR 1845-6357B. The companion, classified as a T-dwarf, has an observed projected distance of 4.1 AU, an estimated mass between 40 and 50 times the mass of Jupiter, and an estimated effective temperature of 950 K.[3][5] The brown dwarf has a near-IR J band magnitude of 13.26.[6]
Distance
SCR 1845-6357 distance estimates
Source | Parallax, mas | Distance, pc | Distance, ly | Distance, Pm | Ref. |
---|---|---|---|---|---|
Deacon et al. (2005) | 282±23 | 3.55+0.31 −0.27 |
11.6+1 −0.9 |
109.4+9.7 −8.3 |
[8] |
Henry et al. (2006) | 259.45±1.11 | 3.854+0.017 −0.016 |
12.57±0.05 | 118.9±0.5 | [1][9] |
RECONS TOP100 (2012) | 259.50±1.11[note 1] | 3.854+0.017 −0.016 |
12.57±0.05 | 118.9±0.5 | [10] |
Non-trigonometric distance estimates are marked in italic. The most precise estimate is marked in bold.
References
- ↑ 1.0 1.1 1.2 1.3 Henry, T. J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample". The Astronomical Journal 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233.
- ↑ 2.0 2.1 2.2 2.3 2.4 DENIS-P J184504.9-635747, entry, SIMBAD. Accessed on line June 17, 2008.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 3.9 3.10 3.11 The very nearby M/T dwarf binary SCR 1845-6357, Markus Kasper, Beth A. Biller, Adam Burrows, Wolfgang Brandner, Jano Budaj, and Laird M. Close, Astronomy and Astrophysics 471, #2 (August 2007), pp.655–659. Bibcode: 2007A&A...471..655K. doi:10.1051/0004-6361:20077881.
- ↑ 4.0 4.1 Research Consortium On Nearby Stars, Georgia State University (January 1, 2008). "THE ONE HUNDRED NEAREST STAR SYSTEMS". RECONS. Retrieved June 17, 2008.
- ↑ 5.0 5.1 Observed projected distance computed from parallax and observed angular distance.
- ↑ 6.0 6.1 Chris Gelino, Davy Kirkpatrick, Adam Burgasser. "DwarfArchives.org: Photometry, spectroscopy, and astrometry of M, L, and T dwarfs". caltech.edu. Retrieved 2012-06-10. (main page)
- ↑ SCR J1845-6357B, entry, SIMBAD. Accessed on line June 17, 2008.
- ↑ Deacon, Niall R.; Hambly, Nigel C.; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Jao, Wei-Chun (2005). "The Solar Neighborhood. XI. The Trigonometric Parallax of SCR 1845-6357". The Astronomical Journal 129 (1): 409–412. arXiv:astro-ph/0409582. Bibcode:2005AJ....129..409D. doi:10.1086/426330.
- ↑ Faherty, Jacqueline K.; Burgasser, Adam J.; Walter, Frederick M.; Van der Bliek, Nicole; Shara, Michael M.; Cruz, Kelle L.; West, Andrew A.; Vrba, Frederick J.; Anglada-Escud, Guillem (2012). "The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 Ultracool Dwarfs". The Astrophysical Journal 752 (1): 56. arXiv:1203.5543. Bibcode:2012ApJ...752...56F. doi:10.1088/0004-637X/752/1/56.
- ↑ "RECONS TOP100". THE ONE HUNDRED NEAREST STAR SYSTEMS brought to you by RECONS (Research Consortium On Nearby Stars). 2012. Retrieved 2014-10-22.
- Hambly, Nigel C.; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Jao, Wei-Chun (2004). "The Solar Neighborhood. VIII. Discovery of New High Proper Motion Nearby Stars Using the SuperCOSMOS Sky Survey". The Astronomical Journal 128 (1): 437–447. arXiv:astro-ph/0404265. Bibcode:2004AJ....128..437H. doi:10.1086/421748.
- B.A. Biller et al., 2006, "Discovery of a Brown Dwarf Very Close to the Sun: A Methane-rich Brown Dwarf Companion to the Low-Mass Star SCR 1845-6357", Astrophysical Journal Letters.
Notes
- ↑ Weighted parallax based on parallaxes from Deacon et al. (2005) and Henry et al. (2006).
External links
- New Objects within 20 light-years at SolStation.
- SCR 1845-6357
See also
- OTS 44
- Cha 110913-773444
- List of nearest stars
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