HD 18438

HD 18438
Location of HD 18438 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cepheus
HD 18438
Right ascension 03h 06m 07.84053s
Declination +79° 25 06.7270
Apparent magnitude (V) +5.49
TYC 4516-2148-1
Right ascension 03h 06m 06.49835s
Declination +79° 25 03.7722
Apparent magnitude (V) +9.08
Characteristics
HD 18438
Evolutionary stage AGB
Spectral type M2.5 III
B−V color index +1.569
Variable type suspected
TYC 4516-2148-1
Evolutionary stage subgiant
Spectral type F7 IV
B−V color index +0.61
Astrometry
HD 18438
Radial velocity (Rv)−37.6 km/s
Proper motion (μ) RA: −35.523 mas/yr
Dec.: +10.383 mas/yr
Parallax (π)4.2470±0.0776 mas
Distance770 ± 10 ly
(235 ± 4 pc)
Absolute magnitude (MV)-1.0
TYC 4516-2148-1
Proper motion (μ) RA: −35.639 mas/yr
Dec.: +10.069 mas/yr
Parallax (π)4.3427 ± 0.0176 mas
Distance751 ± 3 ly
(230.3 ± 0.9 pc)
Absolute magnitude (MV)2.5
Orbit
PrimaryHD 18438
CompanionTYC 4516-2148-1
Semi-major axis (a)4.7"
(1100 AU)
Details
HD 18438
Mass1.84±0.09 M
Radius88.475±4.424 R
Luminosity929±41 L
Surface gravity (log g)0.9±0.1 cgs
Temperature3860±100 K
Metallicity [Fe/H]−0.4±0.1 dex
Rotation637 d
Rotational velocity (v sin i)5.5±0.2 km/s
Age5.5±2.4 Gyr
TYC 4516-2148-1
Mass1.174±0.184 M
Radius2.554±0.182 R
Luminosity7.558±0.095 L
Surface gravity (log g)3.7±0.1 cgs
Temperature6164±211 K
Other designations
ADS 2294, CCDM J03061+7925, WDS J03061+7925
HD 18438: AG+79°95, BD+78°103, FK5 105, GC 3638, HD 18438, HIP 14417, HR 881, SAO 4810, PPM 5183, TIC 297820335, TYC 4516-2147-1, 2MASS J03060788+7925066
TYC 4516-2148-1: TYC 4516-2148-1
Database references
SIMBADHD 18438
TYC 4516-2148-1

HD 18438 is a red giant star in the deep northern constellation of Cepheus, located about 730 light-years (220 parsecs) from Earth. With an apparent magnitude of 5.49, it is visible by the naked eye under dark skies as a red-hued dot of light about 10 degrees away from the celestial north pole. It is part of a wide binary system with an F-type subgiant star. In 2023, HD 18438 was discovered to be orbited by a 21 MJ substellar object, potentially making it the largest host star to an exoplanet ever found as of September 2024.