HD 148427

HD 148427
Timir
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ophiuchus
Right ascension 16h 28m 28.151s[1]
Declination –13° 23′ 58.69″[1]
Apparent magnitude (V) 6.903
Characteristics
Spectral type K0IV
Apparent magnitude (B) 7.839
Apparent magnitude (J) 5.299
Apparent magnitude (H) 4.875
Apparent magnitude (K) 4.682
B−V color index 0.936
Astrometry
Proper motion (μ) RA: –37.74 ± 0.76[1] mas/yr
Dec.: 2.81 ± 0.51[1] mas/yr
Parallax (π)16.94 ± 0.60 mas[1]
Distance193 ± 7 ly
(59 ± 2 pc)
Absolute magnitude (MV)3.039
Orbit
PrimaryHD 148427
CompanionHD 148427 b
Period (P)331.5 ± 3.0 d
(0.9076 yr)
Semi-major axis (a)0.93 ± 0.01 AU
Eccentricity (e)0.16 ± 0.08
Inclination (i)0.5120+0.1635
−0.1082
°
Details
HD 148427
Mass1.45 ± 0.06 M
Radius3.22 ± 0.2 R
Luminosity6.06 L
Surface gravity (log g)3.75 cgs
Temperature5052 ± 44 K
Metallicity [Fe/H]0.154 ± 0.04 dex
Age2.5 Gyr
HD 148427 b
Mass136.5+37.2
−33.7
 MJup
Other designations
BD–13°4437, HIP 80687, PPM 231736, SAO 159932
HD 148427: Timir
HD 148427 b: Tondra
Database references
SIMBADdata
Exoplanet Archivedata

HD 148427, formally named Timir,[2] is a 7th-magnitude K-type subgiant star approximately 193 light years away in the constellation Ophiuchus. Its mass is 45% greater than the Sun, and it is three times the size and six times more luminous, although its age is 2½ billion years.

  1. ^ a b c d e Cite error: The named reference van Leeuwen2007 was invoked but never defined (see the help page).
  2. ^ "Naming of exoplanets". IAU. International Astronomical Union. Retrieved 26 January 2022.

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