This image shows WR 140 and its nebula with JWST Mid-Infrared Instrument, taken in July 2022. The nebula is formed by the binary and only the innermost shells were previously imaged with Keck in 1999/2001.[1] | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cygnus |
Right ascension | 20h 20m 27.97608s[2] |
Declination | +43° 51′ 16.2802″[2] |
Apparent magnitude (V) | 6.85[3] |
Characteristics | |
Spectral type | WC7p + O5[4] |
Apparent magnitude (J) | 5.547[5] |
Apparent magnitude (K) | 5.037[6] |
U−B color index | −0.35[3] |
B−V color index | +0.40[3] |
Variable type | WR[7] |
Astrometry | |
Radial velocity (Rv) | 3.10[8] km/s |
Proper motion (μ) | RA: −4.653[9] mas/yr Dec.: −2.047[9] mas/yr |
Parallax (π) | 0.5815 ± 0.0286 mas[9] |
Distance | 5,600 ± 300 ly (1,720 ± 80 pc) |
Absolute magnitude (MV) | WR: −6.6 to −4.8 O: −6.11 to −5.94[10] |
Orbit[11] | |
Primary | O |
Companion | WR |
Period (P) | 7.9241+0.0037 −0.0035 yr |
Semi-major axis (a) | 8.30+0.22 −0.23″ |
Eccentricity (e) | 0.9012±0.0034 |
Inclination (i) | 119.4+3.7 −3.4° |
Longitude of the node (Ω) | 349.1±2.5° |
Periastron epoch (T) | MJD 1993.1825+0.0036 −0.0039 |
Argument of periastron (ω) (primary) | 42.31+0.70 −0.68° |
Semi-amplitude (K1) (primary) | 29.3±1.8 km/s |
Semi-amplitude (K2) (secondary) | 68.5+1.2 −1.1 km/s |
Details | |
WR | |
Mass | 8.4[11] M☉ |
Luminosity | 537,000[12] L☉ |
Temperature | 70,000[12] K |
O | |
Mass | 20.5[11] M☉ |
Radius | 35[12] R☉ |
Luminosity | 1,600,000[12] L☉ |
Temperature | 35,000[12] K |
Other designations | |
Database references | |
SIMBAD | data |
WR 140 is a visually moderately bright Wolf–Rayet star placed within the spectroscopic binary star, SBC9 1232,[8] whose primary star is an evolved spectral class O4–5 star.[8] It is located in the constellation of Cygnus, lying in the sky at the centre of the triangle formed by Deneb, γ Cygni and δ Cygni.
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