Wolf 1061c

Wolf 1061c
Exoplanet List of exoplanets

Artist's impression of the planetary system around Wolf 1061.
Parent star
Star Wolf 1061
Constellation Ophiuchus
Right ascension (α) 16h 30m 18.1s
Declination (δ) –12° 39′ 45″
Distance13.8 ly
(4.29 pc)
Spectral type M3V[1]
Mass (m) 0.25[2][3] M☉
Radius (r) 0.26[2] R☉
Temperature (T) 3380 ± 20 K
Metallicity [Fe/H] −0.02 ± 0.17
Age 3–4 Gyr
Physical characteristics
Radius(r)1.6[4] R⊕
Stellar flux(F⊙)0.60[4] ⊕
Temperature (T) 223 K (−50 °C; −58 °F)[4]
Orbital elements
Semi-major axis(a) 0.08427 (± 0.00004)[1] AU
Eccentricity (e) 0.19 (± 0.13)[1]
Orbital period(P) 17.9 d
Discovery information
Discovery date 17 December 2015
Discoverer(s) University of New South Wales, Australia
Discovery method Radial velocity
Discovery site European Southern Observatory
Discovery status Submitted
Database references
Extrasolar Planets
Encyclopaedia		data
SIMBADdata
Exoplanet Archivedata
Open Exoplanet Cataloguedata

Wolf 1061c or WL 1061c is an exoplanet orbiting within the habitable zone of the red dwarf star Wolf 1061 in the constellation Ophiuchus, about 13.8 light years from Earth, making it the second-closest known potentially habitable exoplanet to Earth, after Proxima Centauri b.[5][6] It is the second planet in order from its host star in a triple planetary system, and has an orbital period of 17.9 days. Wolf 1061c is classified as a super-Earth exoplanet as its estimated radius is greater than 1.5 R⊕.

Characteristics

Mass, radius and temperature

Wolf 1061c is thought to be a rocky planet estimated to be a super-Earth exoplanet as its mass is about 4.3 times that of Earth and radius is over 1.5 which would give it a density either near or possibly higher than Earth.[7] It has an estimated surface gravity of 1.6 times that on Earth.[8]

In astronomical terms, the Wolf 1061 system is relatively close to Earth, at only 13.8 light years away. This makes it the third closest known, potentially habitable, and confirmed planet to Earth (first being Mars and second being Proxima Centauri b), yielding interest from astronomers.[5][6]

The discovery was announced on 17 December 2015, following a study that used 10 years of archival spectra of the star Wolf 1061 using the HARPS spectrograph attached to the ESO 3.6 m Telescope at the European Southern Observatory at La Silla, Chile.[5][8]

The planet has an equilibrium temperature of 223 K (−50 °C; −58 °F), slightly higher than that of Mars.[4]

Host star

The planet orbits a (M-type) star named Wolf 1061, orbited by a total of three planets. The star has a mass of 0.25 M☉ and a radius of 0.26 R☉. It has a temperature of 3380 K. The age is poorly constrained/unknown, but estimates would place it around a few billion years. In comparison, the Sun is 4.6 billion years old[9] and has a surface temperature of 5778 K.[10]

The star's apparent magnitude, or how bright it appears from Earth's perspective, is 10.1. Therefore, it is too dim to be seen with the naked eye.

Orbit

Wolf 1061c orbits its host star with less than 1% of the Sun's luminosity every 17.9 days at a distance of 0.08 AU (compared to Mercury which orbits at a distance of 0.38 AU).[8]

Habitability

The planet's orbital distance of 0.084 AU (assuming mild eccentricity) lies at the inner edge of its star's habitable zone, which extends from approximately 0.073 to 0.190 AU (for comparison, the habitable zone of the Sun is approximated at 0.5 to 3.0 AU for its different energy emission). Its host star is a red dwarf, with about a quarter as much mass as the Sun. As a result, stars like Wolf 1061 have the ability to burn up to 400–500 billion years, 40–50 times longer than the Sun will.[11]

Because it is so close to the star, it is likely to be tidally locked, meaning one side permanently faces the star and the other side permanently faces away. Although this scenario could result in extreme temperature differences on the planet, the terminator line that separates the illuminated side and the dark side could potentially be habitable, as the temperature there could be suitable for liquid water to exist.[12] Additionally, a much larger portion of the planet could also be habitable if it has a thick enough atmosphere to facilitate heat transfer away from the side facing the star.[6]

See also

References

  1. 1 2 3 "Wolf 1061 c". Retrieved 24 July 2016.
  2. 1 2 Wright, D.J; Wittenmyer, R.A.; Bentley, C.G.; Riedel, J.S.; Jinglin, Zhao (17 December 2015). "Three planets orbiting Wolf 1061". arXiv:1512.05154v1 Freely accessible [astro-ph.EP].
  3. ↑ Rojas-Ayala, Bárbara; et al. (April 2012). "Metallicity and Temperature Indicators in M Dwarf K-band Spectra: Testing New and Updated Calibrations with Observations of 133 Solar Neighborhood M Dwarfs". The Astrophysical Journal. 748 (2): 93. Bibcode:2012ApJ...748...93R. arXiv:1112.4567 Freely accessible. doi:10.1088/0004-637X/748/2/93.
  4. 1 2 3 4 http://phl.upr.edu/projects/habitable-exoplanets-catalog
  5. 1 2 3 "Astronomers discover closest potentially habitable planet: Wolf 1061c". ScienceAlert.com. 17 December 2015. Retrieved 17 December 2015.
  6. 1 2 3 Marcus Strom (17 December 2015). "Wolf 1061c: closest planet found orbiting in a star's habitable zone 14 light years from Earth". Smh.com.au. Retrieved 17 December 2015.
  7. ↑ "HEC: Exoplanets Calculator - Planetary Habitability Laboratory @ UPR Arecibo". phl.upr.edu. Retrieved 2016-01-27.
  8. 1 2 3 "Three planets orbiting Wolf 1061" (PDF). Newt.phys.unsw.edu.au. Retrieved 17 December 2015.
  9. ↑ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
  10. ↑ Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
  11. ↑ Adams, F. C.; P. Bodenheimer; G. Laughlin (2005). "M dwarfs: planet formation and long term evolution". Astronomische Nachrichten. 326 (10): 913–919. Bibcode:2005AN....326..913A. doi:10.1002/asna.200510440.
  12. ↑ Griffiths, Sarah. "Super-Earth Wolf 1061c is the closest 'habitable' planet outside our solar system". Daily Mail. Retrieved 17 December 2015.

Coordinates: 16h 30m 18.1s, −12° 39′ 45″

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.