Qatar-4

From Wikipedia, the free encyclopedia

Qatar-4
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Andromeda[1]
Right ascension 00h 19m 26.22s[2]
Declination +44° 01 39.5[2]
Apparent magnitude (V) 13.60[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type K1V[3]
Variable type planetary transit
Astrometry
Proper motion (μ) RA: 0.923±0.011 mas/yr[2]
Dec.: −8.921±0.009 mas/yr[2]
Parallax (π)3.0567±0.0158 mas[2]
Distance1,067 ± 6 ly
(327 ± 2 pc)
Details
Mass0.856+0.029
0.030
[4] M
Radius0.800+0.015
0.014
[4] R
Luminosity0.481[3] L
Surface gravity (log g)4.565+0.018
0.020
[4] cgs
Temperature5174+33
35
[4] K
Metallicity [Fe/H]0.095+0.076
0.088
[4] dex
Rotational velocity (v sin i)7.1±0.5[3] km/s
Age170±0.1[3] Myr
Other designations
Gaia DR3 385697172809355392, Qatar 4, UCAC3 269-3518
Database references
SIMBADdata
Exoplanet Archivedata

Qatar-4 is a faint K-dwarf star that hosts a planet in the constellation Andromeda. With an apparent magnitude of 13.60, it is impossible to detect with the naked eye, but can be detected with a powerful telescope. Qatar-4 is currently located 1,083 light years away based on parallax.

This star is a relatively young star with an age of only 170 million years. At this age, it is still on the main sequence. Qatar-4 has 89.6% the mass of the Sun, and 84.9% the latter's radius. Despite all of this, it only has 48.1% of the Sun's luminosity, which corresponds to an effective temperature of 5,120 K. Qatar-4 has a similar metallicity to the Sun, and rotates at a rate of 7.1 km/s.

Planetary system

See also

References

Related Articles

Wikiwand AI