Wikipedia
SCR 1845−6357
SCR 1845−6357 is a binary system, about 13 light-years away in the constellation Pavo. The primary is a faint red dwarf. It has a brown dwarf companion. The primary red dwarf was discovered in 2004 by Hambly et al., while the secondary brown dwarf was later discovered in 2006.
Three-colour image of SCR1845−6357AB generated from the SDI filter images (blue=1.575 μm, green=1.600 μm, red=1.625 μm). Because the T-dwarf fades away towards the longer wavelengths, it appears quite blue in this image. It is roughly 50 times fainter than the star and is separated from it by an angle of 1.17″ on the sky (4.5 times the Earth-Sun distance). | |
| 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) | 249.6651 ± 0.1330 mas[4] |
| Distance | 13.064 ± 0.007 ly (4.005 ± 0.002 pc) |
| Details | |
| Mass | 0.07[5] M☉ |
| Radius | 0.096 R☉ |
| Luminosity | 0.0004 L☉ |
| Temperature | 2600–2700[3] K |
| Other designations | |
| Database references | |
| SIMBAD | The system |
| A | |
SCR 1845−6357 Location of SCR 1845−6357 in the constellation Pavo | |
System Edit
The primary, SCR 1845−6357A, is a faint (apparent magnitude 17.4)[2] ultra-cool red dwarf with a mass of about 7% of the Sun's. However, the measurements are still preliminary and are subject to change.[5]
| 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 [7] |
| Characteristics | |
| Spectral type | T6[3] |
| Apparent magnitude (J) | 13.26[8] |
| 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 | |
| Database references | |
| SIMBAD | B |
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][7] The brown dwarf has a near-IR J-band magnitude of 13.26.[8]
See also Edit
References Edit
- ^ a b 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" (PDF). The Astronomical Journal. 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233. S2CID 15002841.
- ^ a b c d e "DENIS-P J184504.9-635747". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h i j k l 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.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b "THE ONE HUNDRED NEAREST STAR SYSTEMS". Research Consortium On Nearby Stars. Georgia State University. January 1, 2008. Retrieved June 17, 2008.
- ^ Golovin, Alex; Reffert, Sabine; Just, Andreas; Jordan, Stefan; Vani, Akash; Jahreiß, Hartmut (November 2022). "The Fifth Catalogue of Nearby Stars (CNS5)". Astronomy & Astrophysics. 670: A19. arXiv:2211.01449. Bibcode:2023A&A...670A..19G. doi:10.1051/0004-6361/202244250. S2CID 253264922. Catalogue can be accessed here.
- ^ a b Observed projected distance computed from parallax and observed angular distance.
- ^ a b Chris Gelino; Davy Kirkpatrick; Adam Burgasser. . caltech.edu. Archived from the original on 2013-11-13. Retrieved 2012-06-10. (main page) 2019-05-11 at the Wayback Machine
- ^ SCR J1845−6357B, entry, SIMBAD. Accessed on line June 17, 2008.
- 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. S2CID 9586813.
- 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.
External links Edit
- New Objects within 20 light-years at SolStation.
- SCR 1845−6357