HD 34137
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 |
Characteristics | |
Spectral type | K2III C [1] orange giant |
Astrometry | |
Proper motion (μ) | RA: 1.844 mas/yr Dec.: 4.115 mas/yr |
Parallax (π) | 1.42 ± 0.37[2] mas |
Distance | approx. 2,300 ly (approx. 700 pc) |
Absolute magnitude (MV) | -0.174 |
Details | |
Radius | 28 R☉ |
Luminosity | 117 L☉ |
Temperature | 4420 K |
Rotation | 48 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 | |
SIMBAD | data |
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
References[edit]
- ↑ 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
- ↑ 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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