Gliese 581 e

From Wikipedia, the free encyclopedia
Gliese 581 e
Extrasolar planet List of extrasolar planets

Size comparison of Gliese 581 e with Earth.
(Based on selected hypothetical modeled compositions)
Parent star
Star Gliese 581
Constellation Libra
Right ascension (α) 15h 19m 26s
Declination (δ) −07° 43 20
Apparent magnitude (mV) 10.55
Distance20.3 ± 0.3 ly
(6.2 ± 0.1 pc)
Spectral type M3V
Mass (m) 0.31 M
Radius (r) 0.29 R
Temperature (T) 3480 ± 48 K
Metallicity [Fe/H] −0.33 ± 0.12
Age 7–11 Gyr
Orbital elements
Epoch JD 2451409.762[1]
Semimajor axis(a) 0.0284533 ± 0.0000023[1] AU
Eccentricity (e) 0[1]
Orbital period(P) 3.14867 ± 0.00039[1] d
(0.0086 y)
    (75.57 h)
Mean anomaly (M) 267 ± 40[1]°
Semi-amplitude (K) 1.66 ± 0.19[1] m/s
Physical characteristics
Minimum mass(m sin i)1.7 ± 0.2[1] M
Discovery information
Discovery date 21 April 2009
Discoverer(s) Mayor et al.
Discovery method Radial velocity
Discovery site La Silla Observatory, Chile
Discovery status Published[2]
Database references
Extrasolar Planets
Encyclopaedia
data
SIMBADdata

Gliese 581 e /ˈɡlzə/ or Gl 581 e is an extrasolar planet found around Gliese 581, an M3V red dwarf star approximately 20.5 light-years away from Earth in the constellation of Libra. It is the fourth planet discovered in the system and the first in order from the star.

The planet was discovered by an Observatory of Geneva team led by Michel Mayor, using the HARPS instrument on the European Southern Observatory 3.6 m (140 in) telescope in La Silla, Chile. The discovery was announced on 21 April 2009. Mayor's team employed the radial velocity technique, in which the orbit size and mass of a planet are determined based on the small perturbations it induces in its parent star's orbit via gravity.[2]

Artist concept of Gliese 581 e

At a minimum mass of 1.7 Earth masses,[1] it is one of the least-massive extrasolar planet discovered around a normal star, and relatively close in mass to Earth. At an orbital distance of just 0.03 AU from its parent star, however, it orbits further in than the habitable zone. It is unlikely to possess an atmosphere due to its high temperature and strong radiation from the star. Although scientists think it probably has a rocky surface similar to Earth, it is also likely to experience intense tidal heating similar to (and likely more intense than) that affecting Jupiter's moon Io.[3] Gliese 581 e completes an orbit of its sun in approximately 3.15 days.[2][4][5]

See also

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 Vogt, S. S.; et al. (2010). "The Lick-Carnegie Exoplanet Survey: A 3.1 M_Earth Planet in the Habitable Zone of the Nearby M3V Star Gliese 581". arXiv:1009.5733 [astro-ph.EP].
  2. 2.0 2.1 2.2 Mayor, M.; Bonfils, X.; Forveille, T.; Delfosse, X.; Udry, S.; Bertaux, J.-L.; Beust, H.; Bouchy, F. et al. (2009). "The HARPS search for southern extra-solar planets, XVIII. An Earth-mass planet in the GJ 581 planetary system". Astronomy and Astrophysics 507 (1): 487–494. arXiv:0906.2780. Bibcode:2009A&A...507..487M. doi:10.1051/0004-6361/200912172. 
  3. Barnes, Rory; Jackson, Brian; Greenberg, Richard; Raymond, Sean N. (2009-06-09). "Tidal Limits to Planetary Habitability". The Astrophysical Journal 700: L30–L33. arXiv:0906.1785v1. Bibcode:2009ApJ...700L..30B. doi:10.1088/0004-637X/700/1/L30. 
  4. Rincon, Paul; Amos, Jonathan (2009-04-21). "Lightest exoplanet is discovered". BBC. Retrieved 2009-04-21. 
  5. Overbye, Dennis (April 21, 2009). "Astronomers Find Planet Closer to Size of Earth". New York Times. 

External links

Media related to Gliese 581 e at Wikimedia Commons News related to Discovery of smallest exoplanet yields 'extraordinary' find at Wikinews

Coordinates: 15h 19m 26s, −07° 43′ 20″

This article is issued from Wikipedia. The text is available under the Creative Commons Attribution/Share Alike; additional terms may apply for the media files.