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HD 34137

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HD 34989
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Orion
Right ascension  05h 15m 11,8777s
Declination +01° 33′ 22,136″
Apparent magnitude (V) +7.24
Spectral type K2III C [1] orange giant
Proper motion (μ) RA: 1.844 mas/yr
Dec.: 4.115 mas/yr
Parallax (π)1.42 ± 0.37[2] mas
Distanceapprox. 2,300 ly
(approx. 700 pc)
Absolute magnitude (MV)-0.174
Radius28 R
Luminosity117 L
Temperature4420 K
Rotation48 days
Other designations
HIP 24482 GSC 00100-01653 2MASS J05151186+0133220 SRS 6261 AG+01 545 HD 34137 PPM 148670 TYC 100-1653-1 AGKR 4672 HIC 24482 SAO 112568 YZ 1 1632 BD+01 945 IRAS 05126+0130 SKY# 8285
Database references

HD 34137 is star of spectral type K2III in the constellation of Orion. It is about 2,300 light-years from the solar system and its apparent magnitude is +7.24. Its classification puts it in the category of orange giants.

Distance and local setting[edit]

HD 34137 appears to us weak due to its distance, of 2,300 light-years with a 26% error margin, as recorded by the first data release of the Gaia spacecraft.  The supergiant can be viewed using a small pair of binoculars.

External links[edit]

  • "HD 34137". SIMBAD Astronomical Database.
  • [dead link] wolframalpha.com


  1. SIMBAD (cited below) citing Michigan Spectral Survey, Ann Arbor, Dep. Astron., Univ. Michigan, 5, 0 (1999): Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5
  2. SIMBAD University of Strasbourg (Unistra) and CNRS, retrieved 2018.06.17-18:00:36 citing Astronomy and Astrophysics, volume 595A, 2-2 (2016/11-1) Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties.

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