HD 40657
Star in the constellation Orion
From Wikipedia, the free encyclopedia
HD 40657 is a single[12] star in the equatorial constellation of Orion, near the constellation border with Monoceros. It has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.52.[3] The star is located at a distance of approximately 333 light years from the Sun based on parallax.[2] It is drifting further away with a radial velocity of +26 km/s.[6]
 | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Orion[1] |
| Right ascension | 06h 00m 03.34963s[2] |
| Declination | −03° 04′ 27.3305″[2] |
| Apparent magnitude (V) | 4.52[3] |
| Characteristics | |
| Evolutionary stage | red giant branch[2] |
| Spectral type | K1.5III-IIIb CN-1[4] |
| U−B color index | +1.21[3] |
| B−V color index | +1.22[3] |
| Variable type | suspected[5] |
| Astrometry | |
| Radial velocity (Rv) | +25.9±0.9[6] km/s |
| Proper motion (μ) | RA: +10.754[2] mas/yr Dec.: −73.601[2] mas/yr |
| Parallax (π) | 9.7817±0.2473 mas[2] |
| Distance | 333 ± 8 ly (102 ± 3 pc) |
| Absolute magnitude (MV) | −1.00[1] |
| Details | |
| Mass | 1.68[7] M☉ |
| Radius | 22.2[8] R☉ |
| Luminosity | 171[8] L☉ |
| Surface gravity (log g) | 2.42[9] cgs |
| Temperature | 4,435[8] K |
| Metallicity [Fe/H] | −0.48[1] dex |
| Rotational velocity (v sin i) | 2.1[10] km/s |
| Age | 2.27[7] Gyr |
| Other designations | |
| NSV 2770, BD−03°1256, FK5 2457, GC 7587, HD 40657, HIP 28413, HR 2113, SAO 132732[11] | |
| Database references | |
| SIMBAD | data |
This is an aging giant star with a stellar classification of K1.5III-IIIb CN-1,[4] where the suffix notation indicates an underabundance of cyanogen in the spectrum. Having exhausted the supply of hydrogen at its core, this star cooled and expanded off the main sequence. At present it has 22 times the radius of the Sun.[8]
HD 40657 is a suspected variable star with a brightness that has been measured ranging from magnitude 4.54 down to 4.58.[5] It is an estimated 2.27 billion years old with 1.68 times the mass of the Sun[7] and is spinning with a projected rotational velocity of 2.1 km/s.[10] The star is radiating 171 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,536 K.[8]