Wolf 1061

Wolf 1061

Artist's impression of exoplanets orbiting a red dwarf.[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 16h 30m 18.0584s[2]
Declination –12° 39′ 45.325″[2]
Apparent magnitude (V) 10.07[3] (10.05 - 10.10)[4]
Characteristics
Spectral type M3.5V[5]
U−B color index +1.20[6]
B−V color index +1.57[3]
Variable type BY Draconis[4]
Astrometry
Radial velocity (Rv)–21.22[7] km/s
Proper motion (μ) RA: –94.212[2] mas/yr
Dec.: 1,183.679[2] mas/yr
Parallax (π)232.29 ± 0.49[2] mas
Distance14.04 ± 0.03 ly
(4.305 ± 0.009 pc)
Absolute magnitude (MV)11.87[5]
Details
Mass0.294[5] M☉
Radius0.307 (± 0.027)[5] R☉
Luminosity (bolometric)0.0102[5] L☉
Luminosity (visual, LV)0.0015 L☉
Temperature3342 ± 49[5] K
Metallicity [Fe/H]–0.09 ± 0.09[5] dex
Rotation94 ± 1 days[5]
Other designations
BD -12°4523, G 153-058, GCTP 3746.00, GJ 628, HIP 80824, LHS 419, Vys 164.
Database references
SIMBADdata

Wolf 1061 (also known as HIP 80824 and V2306 Ophiuchi) is an M class red dwarf star located about 13.8 light years away in the constellation Ophiuchus. It is the 36th closest known star system to the Sun and has a relatively high proper motion of 1.2 seconds of arc per year. Like many red dwarfs, it most likely has a long rotation period of more than 100 days, although it is difficult to measure accurately. Wolf 1061 does not have any unusual spectroscopic features.[8] The star was first cataloged in 1919 by German astronomer Max Wolf when he published a list of dim stars that had high proper motions. Wolf 1061's name originates from this list.[9] The star has a stellar rotation period of 89.3±1.8~ days. A seven years study found no evidence of photometric transits and confirms the radial velocity signals are not due to stellar activity. The habitable zone estimate for the system lies between approximately 0.1 and 0.2 AU from the star.

Planetary system

In December 2015, a team of astronomers from the University of New South Wales announced the discovery of three planets orbiting Wolf 1061. The planets were detected by analyzing 10 years of observations of the Wolf 1061 system by the HARPS spectrograph at La Silla Observatory in Chile. The team used archive radial velocity measurements of the star's spectrum in the HARPS data and, along with 8 years of photometry from the All Sky Automated Survey, discovered two definite planets with orbital periods of around 4.9 and 17.9 days and a very likely third with a period of 67.3 days.[8]

All three planets have masses low enough that they are likely to be rocky planets similar to the inner planets of the Solar System although their actual sizes and densities are currently unknown. However, this information could be determined if the planets happen to transit in front of Wolf 1061 when viewed from Earth. Because all three planets orbit close to the star and have short orbital periods, there is a chance that this will occur. The University of New South Wales team estimated the chances of a transit at around 14% for planet b, 6% for planet c, and 3% for planet d.[8]

One of the planets, Wolf 1061 c, is a super-Earth located near the inner edge of the star's habitable zone, which conservatively extends from 0.11 to 0.21 AU, or at most from 0.09 to 0.23 AU.[3] It is one of the closest known potentially habitable planets to Earth after Proxima b, Ross 128 b, and Luyten b.[10][11][12] The next planet out, Wolf 1061 d, could be marginally habitable depending on its atmosphere's composition as it orbits just beyond the habitable zone.[8]

In March 2017, another team of astronomers re-analyzed the system using the HARPS spectrograph. They found planets b and c to be quite similar to their originally reported parameters, but found that planet d was more massive and in a larger, more eccentric orbit. The team was also able to find updated parameters for the host star. Their results showed that Wolf 1061 c is slightly smaller, yet closer to the inner edge of the habitable zone.[5]

The Wolf 1061 planetary system[8][5]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b ≥1.91 ± 0.25 M⊕ 0.0375 ± 0.0012 4.8869 ± 0.0005 0.15 +0.13
−0.10		 — 1.2 (estimated) R⊕
c ≥3.41 +0.43
−0.41 M⊕		 0.0890 ± 0.003 17.8719 ± 0.0059 0.11 +0.10
−0.07		 — 1.45 (estimated) R⊕
d ≥7.7 +1.12
−1.06 M⊕		 0.470 ± 0.016 217.21 +0.55
−0.52		 0.55 +0.08
−0.09		 — 2.2 (estimated) R⊕

See also

References

  1. ↑ "Astronomers discover closest potentially habitable planet: Wolf 1061c". ScienceAlert.com. 17 December 2015. Retrieved 17 December 2015.
  2. 1 2 3 4 5 Gaia Collaboration; Brown, A. G. A; Vallenari, A; Prusti, T; De Bruijne, J. H. J; Mignard, F; Drimmel, R; Babusiaux, C; Bailer-Jones, C. A. L; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy & Astrophysics. 595: A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512.
  3. 1 2 3 Kane, Stephen R.; et al. (February 2017), "Characterization of the Wolf 1061 Planetary System", The Astrophysical Journal, 835 (2): 9, arXiv:1612.09324, Bibcode:2017ApJ...835..200K, doi:10.3847/1538-4357/835/2/200, 200.
  4. 1 2 Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  5. 1 2 3 4 5 6 7 8 9 10 Astudillo-Defru, N; Forveille, T; Bonfils, X; Ségransan, D; Bouchy, F; Delfosse, X; Lovis, C; Mayor, M; Murgas, F; Pepe, F; Santos, N. C; Udry, S; Wünsche, A (2017). "The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293". Astronomy & Astrophysics. 602: A88. arXiv:1703.05386. Bibcode:2017A&A...602A..88A. doi:10.1051/0004-6361/201630153.
  6. ↑ Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data. SIMBAD, Bibcode:1986EgUBV........0M.
  7. ↑ Nidever, David L.; et al. (August 2002), "Radial Velocities for 889 Late-Type Stars", The Astrophysical Journal Supplement Series, 141 (2): 503–522, arXiv:astro-ph/0112477, Bibcode:2002ApJS..141..503N, doi:10.1086/340570.
  8. 1 2 3 4 5 Wright, D. J; Wittenmyer, R. A; Tinney, C. G; Bentley, J. S; Zhao, Jinglin (2016). "Three Planets Orbiting Wolf 1061". The Astrophysical Journal Letters. 817 (2): L20. arXiv:1512.05154. Bibcode:2016ApJ...817L..20W. doi:10.3847/2041-8205/817/2/L20.
  9. ↑ Wolf, M. (June 1919). "Katalog von 1053 staerker bewegten Fixsternen (Catalog of 1053 moving fixed stars)". Veroeffentlichungen der Badischen Sternwarte zu Heidelberg (in German). 7 (10): 195–219. Bibcode:1919VeHei...7..195W.
  10. ↑ Davison, Cassy L.; White, Russel J.; Henry, Todd J.; Riedel, Adric R.; Jao, Wei-Chun; Bailey III, John I.; Quinn, Samuel N.; Justin R., Cantrell; John P., Subasavage; Jen G., Winters (2015). "A 3D Search for Companions to 12 Nearby M-Dwarfs". The Astronomical Journal. 149 (3): 106. arXiv:1501.05012 [astro-ph.SR]. Bibcode:2015AJ....149..106D. doi:10.1088/0004-6256/149/3/106. Cite uses deprecated parameter |class= (help)
  11. ↑ Sarah Griffiths (17 December 2015). "'Super-Earth' is spotted just 14 light years away: Wolf 1061c is the closest 'habitable' planet outside our solar system ever found". Daily Mail.
  12. ↑ Stuart Gary (17 December 2015). "Potentially habitable super-Earth discovered orbiting star 14 light years from Earth". ABC News (Australia).
  • "Wolf 1061". SIMBAD. Centre de données astronomiques de Strasbourg.
  • Simulated view of the Wolf 1061 system created by the University of New South Wales
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.