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Qatar-2 is a K-type main-sequence star about 595 light-years away in the constellation of Virgo. The star is much older than Sun, and has a concentration of heavy elements similar to solar abundance. The star features a numerous and long-lived starspots, and belongs to a peculiar variety of inflated K-dwarfs with strong magnetic activity inhibiting internal convection.

Wikidata facts

Constellation
Virgo
Distance from Earth
182.319
Radius
0.78
Mass
0.74
Show 15 more facts
catalog code
EPIC 212756297
effective temperature
4645
parallax
5.4823
apparent magnitude
13.015017
radial velocity
-27.7
epoch
J2000.0
spectral class
K
metallicity
0.02
surface gravity
40000
luminosity
0.18497734
right ascension component of proper motion
-88.171
declination component of proper motion
-15.187
age estimated by a dating method
5.0
right ascension
207.65587513609998
declination
-6.80400599279

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Encyclopedic overview

2 sections
Contents
  • Planetary system
  • References

Qatar-2 is a K-type main-sequence star about 595 light-years away in the constellation of Virgo. The star is much older than Sun, and has a concentration of heavy elements similar to solar abundance. The star features a numerous and long-lived starspots, and belongs to a peculiar variety of inflated K-dwarfs with strong magnetic activity inhibiting internal convection.

==Planetary system== In 2011 a transiting superjovian planet Qatar-2b was detected by the Qatar Exoplanet Survey. The planet has a large measured temperature difference between dayside and nightside . The planetary orbit is well aligned with the equatorial plane of the star, misalignment angle equal to . No orbital decay was detected. The color of planetary atmosphere is blue due to Rayleigh scattering of light, and albedo is very low, being below 0.06.

Excerpted from Wikipedia’s “Qatar 2” article, available under the CC BY-SA 4.0 licence.

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