GQ Lupi

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

GQ Lupi
File:GQLupLightCurve.png
A visual band light curve for GQ Lupi. The main plot (from ASAS data[1]), shows the long-term variability, and the inset plot (adapted from Broeg et al.[2]) shows the short-term periodic brightness variation.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lupus
Right ascension Template:RA[3]
Declination Template:DEC[3]
Apparent magnitude (V) 11.40[4]
Characteristics
A
Evolutionary stage T Tauri star[5]
Spectral type K7V[4]
B−V Template:Engvar 0.96[4]
Variable type T Tauri variable[5]
C (2MASS J15491331)Template:Efn
Evolutionary stage Red dwarf
Spectral type M4[6]
Astrometry
Proper motion (μ) RA: Script error: No such module "val".[3] mas/yr
Dec.: Script error: No such module "val".[3] mas/yr
Parallax (π)6.5868±0.0473 mas[3]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)~5[7]
Orbit
PrimaryGQ Lupi A
CompanionGQ Lupi C (2MASS J15491331)Template:Efn
Semi-major axis (a)Script error: No such module "val".[6]
Details
A
Mass0.7[8] Template:Solar mass
Age<2 million[8] years
C (2MASS J15491331)Template:Efn
Mass~0.15[6] Template:Solar mass
Radius0.21[6] Template:Solar radius
Temperature3190 K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
CD−35°10525, GQ Lup[4]
Database references
SIMBADdata

Script error: No such module "Check for unknown parameters".

GQ Lupi is a T Tauri variable star approximately 495 light-years away[3] in the constellation of Lupus.[5] The star is young and has about 70% of the Sun's mass.[8]

Stellar system

In 2020, another low-mass companion of GQ Lupi was discovered at a separation distance of about 16 arcseconds, or 2400 AU. Designated 2MASS J15491331-3539118 under the 2MASS catalogue, it is likely a young stellar object that is gravitationally bound to its primary star. It is estimated to be approximately 15% the Sun's mass and 21% the Sun's radius. It has an effective temperature of about 3190 K, indicating that it is a red dwarf with the spectral type M4.[6]

Possible planetary system

File:The Sub-Stellar Companion to GQ Lupi.jpg
VLT NACO image, taken in the Ks-band, of GQ Lupi. The feeble point of light to the right of the star is the newly found cold companion. It is 250 times fainter than the star itself and it located 0.73 arc second west. At the distance of GQ Lupi, this corresponds to a distance of roughly 100 AU. North is up and East is to the left.

In 2005, Ralph Neuhäuser and his colleagues reported a substellar object, GQ Lupi b, orbiting the star. Along with 2M1207b, this was one of the first extrasolar planet candidates to be directly imaged. The image was made with the VLT telescope at Paranal Observatory, Chile, on June 25, 2004. Depending on its mass and the definition of a planet, GQ Lupi b may or may not be considered a planet.[9] As of 2006, the International Astronomical Union Working Group on Extrasolar Planets described GQ Lupi b as a "possible planetary-mass companion to a young star".[10] GQ Lupi b is listed as "confirmed planet" as in 2020.[11]

Template:OrbitboxPlanet short

Notes

Template:Notelist

References

<templatestyles src="Reflist/styles.css" />

  1. Script error: No such module "citation/CS1".
  2. Script error: No such module "Citation/CS1".
  3. a b c d e f Template:Cite Gaia DR2
  4. a b c d Template:Cite simbad
  5. a b c Astrometric and photometric monitoring of GQ Lupi and its sub-stellar companion, Ralph Neuhaeuser, Markus Mugrauer, Andreas Seifahrt, Tobias Schmidt, and Nikolaus Vogt, Astronomy and Astrophysics 484, #1 (2008), pp. 281–291. Script error: No such module "CS1 identifiers".. Bibcode:2008A&A...484..281NScript error: No such module "check bibcode".
  6. a b c d e Script error: No such module "Citation/CS1".
  7. From parallax and apparent magnitude.
  8. a b c First image of exoplanet orbiting Sun-like star, Kelly Young, April 4, 2005, NewScientist.com news service. Accessed on line June 13, 2008.
  9. Is this a Brown Dwarf or an Exoplanet? New Young Sub-stellar Companion Imaged with the VLT Script error: No such module "webarchive"., ESO Press Release 09/05, April 7, 2005. Accessed on line June 13, 2008.
  10. Lists of Extrasolar Planets Script error: No such module "webarchive"., IAU Working Group on Extrasolar Planets, August 28, 2006. Accessed on line June 13, 2008.
  11. openexoplanetcatalogue.com GQ Lup

Script error: No such module "Check for unknown parameters".

External links

  • The low-mass companion of GQ Lup, E.W. Guenther, R. Neuhaeuser, G. Wuchterl, M. Mugrauer, A. Bedalov, and P.H. Hauschildt, Astronomische Nachrichten 326, #10 (December 2005), pp. 958–963. Script error: No such module "CS1 identifiers".. Bibcode:2005AN....326..958GScript error: No such module "check bibcode".
  • R. Neuhaeuser (2005). "Homogeneous comparison of directly detected planet candidates: GQ Lup, 2M1207, AB Pic". arXiv:astro-ph/0509906v1.
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".
  • Script error: No such module "citation/CS1".

Template:Stars of Lupus