Astronomy:LSR J1835+3259
Coordinates: 
18h 35m 37.902s, +32° 59′ 54.59″
.jpg) Artist's impression of LSR J1835+3259 and its aurorae. Credit: Chuck Carter and Gregg Hallinan/Caltech | |
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Lyra |
| Right ascension | 18h 35m 37.902s[1] |
| Declination | +32° 59′ 54.59″[1] |
| Characteristics | |
| Spectral type | M8.5[2] |
| Apparent magnitude (V (USNO filter system)) | 18.27 ± 0.03[2] |
| Apparent magnitude (I (USNO filter system)) | 13.46 ± 0.02[2] |
| Apparent magnitude (z (USNO filter system)) | 12.63 ± 0.02[2] |
| Apparent magnitude (J (2MASS filter system)) | 10.27 ± 0.03[2] |
| Apparent magnitude (H (2MASS filter system)) | 9.58 ± 0.05[2] |
| Apparent magnitude (Ks (2MASS filter system)) | 9.15 ± 0.04[2] |
| Astrometry | |
| Radial velocity (Rv) | -10 ± 40[3] km/s |
| Proper motion (μ) | RA: −72.650±0.047[4] mas/yr Dec.: −755.146±0.052[4] mas/yr |
| Parallax (π) | 175.7930 ± 0.0468[4] mas |
| Distance | 18.553 ± 0.005 ly (5.689 ± 0.002 pc) |
| Details | |
| Mass | 55 ± 4[5] MJup |
| Radius | 2.1 ± 0.1[5] RJup |
| Surface gravity (log g) | 4.5 ± 0.05[5] cgs |
| Temperature | 2800 ± 30[5] K |
| Age | 22 ± 4[5] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
  LSR J1835+3259 Location of LSR J1835+3259 in the constellation Lyra | |
LSR J1835+3259 is a nearby ultracool dwarf[6] of spectral class M8.5,[2] located in constellation Lyra, the discovery of which was published in 2003.[2][3] Previously it was concluded that this star is a young brown dwarf,[5] but no lithium absorption lines are detected for this object, which is a strong indicator for young brown dwarfs that need 10-100 million years to deplete lithium.[6]
Distance
Trigonometric parallax of this object, measured in 2001–2002 with the USNO 61 inch (1.5 m) reflector under US Naval Observatory (USNO) parallax program, is 0.1765 ± 0.0005 arcsec, corresponding to a distance of 5.67 ± 0.02 pc, or 18.48 ± 0.05 ly.[2]
Characteristics
The first potential extrasolar auroras detected occurred in the atmosphere of LSR J1835+3259. They were found in July 2015 by the Karl G. Jansky Very Large Array in New Mexico by analyzing the emitted radio waves. The potential auroras were probably 1 million times brighter than those ever observed on Earth.[7] The optical emission is mainly red in colour, because the charged particles are interacting with hydrogen in its atmosphere. It is not known what the cause is. Some have speculated that material may be being stripped off the surface of the brown dwarf via stellar winds to produce its own electrons. Another possible explanation is an as-yet-undetected planet or moon around the dwarf, which is throwing off material to light it up, as is the case with Jupiter and its moon Io.[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 "2MASS J18353790+3259545 -- Brown Dwarf (M<0.08solMass)". Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J18353790%2B3259545.
- ↑ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 2.11 Reid, I. Neill; Cruz; Laurie; Liebert; Dahn; Harris; Guetter; Stone et al. (2003). "Meeting the Cool Neighbors. IV. 2MASS 1835+32, a Newly Discovered M8.5 Dwarf within 6 Parsecs of the Sun". The Astronomical Journal 125 (1): 354–358. doi:10.1086/344946. Bibcode: 2003AJ....125..354R.
- ↑ 3.0 3.1 3.2 Lepine, Sebastien; Rich; Shara (2003). "Spectroscopy of New High Proper Motion Stars in the Northern Sky. I. New Nearby Stars, New High-Velocity Stars, and an Enhanced Classification Scheme for M Dwarfs". The Astronomical Journal 125 (3): 1598–1622. doi:10.1086/345972. Bibcode: 2003AJ....125.1598L.
- ↑ 4.0 4.1 4.2 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 5.0 5.1 5.2 5.3 5.4 5.5 Berdyugina, S. V.; Harrington, D. M.; Kuzmychov, O.; Kuhn, J. R.; Hallinan, G.; Kowalski, A. F.; Hawley, S. L. (September 2017). "First Detection of a Strong Magnetic Field on a Bursty Brown Dwarf: Puzzle Solved" (in en). Astrophysical Journal 847 (1): 61. doi:10.3847/1538-4357/aa866b. ISSN 0004-637X. Bibcode: 2017ApJ...847...61B.
- ↑ 6.0 6.1 Saur, Joachim; Fischer, Christian; Wennmacher, Alexandre; Feldman, Paul D.; Roth, Lorenz; Strobel, Darrell F.; Reiners, Ansgar (May 2018). "The UV Spectrum of the Ultracool Dwarf LSR J1835+3259 Observed with the Hubble Space Telescope" (in en). Astrophysical Journal 859 (1): 74. doi:10.3847/1538-4357/aabb55. ISSN 0004-637X. Bibcode: 2018ApJ...859...74S.
- ↑ O'Neill, Ian (July 29, 2015). "Monstrous Aurora Detected Beyond our Solar System". Discovery. http://news.discovery.com/space/alien-life-exoplanets/monstrous-aurora-detected-beyond-our-solar-system-150729.htm.
- ↑ Q. Choi, Charles (July 29, 2015). "First Alien Auroras Found, Are 1 Million Times Brighter Than Any On Earth". http://www.space.com/30087-alien-auroras-found-beyond-solar-system.html.
- Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "Trigonometric Parallaxes for 1507 Nearby Mid-to-late M Dwarfs". The Astrophysical Journal 784 (2): 156. doi:10.1088/0004-637X/784/2/156. Bibcode: 2014ApJ...784..156D. Table with parallaxes.
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