WASP-45

WASP-45 is a K-type main-sequence star about 701 light-years (215 parsecs) away. The star's age cannot be well constrained, but it is probably older than the Sun. Yet, WASP-45 is enriched in heavy elements compared to the Sun, having 240% of the solar abundance.

WASP-45
Observation data
Epoch J2000      Equinox J2000
Constellation Sculptor
Right ascension 00h 20m 56.99413s
Declination −35° 59 53.7466
Apparent magnitude (V) 11.8
Characteristics
Spectral type K2V
Astrometry
Radial velocity (Rv)4.71±0.33 km/s
Proper motion (μ) RA: 52.831 mas/yr
Dec.: −46.940 mas/yr
Parallax (π)4.6520 ± 0.0226 mas
Distance701 ± 3 ly
(215 ± 1 pc)
Details
Mass0.932+0.045
−0.046
 M
Radius0.891±0.013 R
Luminosity0.510±0.013 L
Surface gravity (log g)4.508+0.023
−0.025
 cgs
Temperature5167±29 K
Metallicity [Fe/H]0.388+0.090
−0.10
 dex
Rotational velocity (v sin i)2.3±0.7 km/s
Age5.4+4.7
−3.5
 Gyr
Other designations
TOI-229, TIC 120610833, WASP-45, TYC 6996-583-1, GSC 06996-00583, 2MASS J00205699-3559537
Database references
SIMBADdata

The star has low ultraviolet emission, therefore it is suspected to have a low starspot activity, although chromospheric activity was reported elsewhere.

There is a companion star at a separation of 4.4 arcseconds, corresponding to 929 AU.

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