| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Lupus |
| Right ascension | 15h47m 08.27687s[1] |
| Declination | −47° 40′ 10.2846″[1] |
| Apparent magnitude (V) | 11.96[2] (14.6 - 16.7)[3] |
| Characteristics | |
| Evolutionary stage | main sequence[4] |
| Spectral type | A2 V + black hole[5] |
| Variable type | XNG[3] |
| Astrometry | |
| Proper motion (μ) | RA: −7.543 mas/yr[1] Dec.: −5.356 mas/yr[1] |
| Parallax (π) | 0.1909 ± 0.0551 mas[1] |
| Distance | approx. 17,000 ly (approx. 5,000 pc) |
| Details | |
| donor star | |
| Mass | 2.45±0.15[6] M☉ |
| Radius | 2.84±0.11[5] R☉ |
| Luminosity | 48±11[5] L☉ |
| Surface gravity (log g) | 3.82[7] cgs |
| Temperature | 9,000±500[5] K |
| Metallicity [Fe/H] | −0.11[8] dex |
| black hole | |
| Mass | 9.4±2.0[9] M☉ |
| Other designations | |
4U 1543-47, IL Lup, TIC 254732447, 2MASS J15470829-4740103[10] | |
| Database references | |
| SIMBAD | data |
4U 1543-475 is a recurrent X-ray transient[11] located in the southern constellation Lupus, the wolf. IL Lupi is its variable star designation. It has an apparent magnitude that fluctuates between 14.6 and 16.7, making it readily visible in large telescopes but not to the naked eye. The object is located relatively far at a distance of approximately 17,000 light years based on Gaia DR3 parallax measurements.
4U 1543-475 was first observed by Uhuru in 1971.[12] In 1976, 4U 1543-475's spectrum was observed. However, its status as a black hole binary had not been confirmed until 1984 by astronomer S. Kiamoto and colleagues.[13] After subsequent observations, it was given the variable star designation IL Lupi in 1995. 4U 1543-475 erupted three times.[citation needed]
