HD 148427

Source: Wikipedia, the free encyclopedia.
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
Distance
193 ± 7 ly
(59 ± 2 pc)
Absolute magnitude (MV)3.039
Inclination
(i)
0.5120+0.1635
−0.1082
°
Details
HD 148427
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
Exoplanet Archive
data

HD 148427, formally named Timir,

. 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.

Brown dwarf/red dwarf companion

In August 2009, it was found to have a companion in orbit (HD 148427 b or Tondra) with a

inclination was measured, revealing its true mass to be between 27 and 345 MJ. This makes it either a brown dwarf or a low-mass red dwarf star.[4]

Naming

HD 148427, and HD 148427 b (thought at the time to be an exoplanet), were chosen as part of the 2019 NameExoWorlds campaign organised by the International Astronomical Union, which assigned each country a star and planet to be named. HD 148427 was assigned to Bangladesh. The winning name for the star was Timir meaning darkness in the Bengali language, alluding to the star being far away in the darkness of space. The winning name for the companion was Tondra meaning nap in the Bengali language, alluding to the symbolic notion that the object was asleep until discovered.[5]

See also

  • List of extrasolar planets

References

  1. ^
  2. ^ "Naming of exoplanets". IAU. International Astronomical Union. Retrieved 26 January 2022.
  3. S2CID 15524804
    .
  4. .
  5. ^ "Naming of Exoplanets". IAU. International Astronomical Union. Retrieved 26 January 2022.