Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Telescopium |
Right ascension | 19h 29m 52.61028s[1] |
Declination | −55° 26′ 30.3051″[1] |
Apparent magnitude (V) | 6.13±0.01[2] |
Characteristics | |
Spectral type | K0/1 III[3] |
U−B color index | +0.81[4] |
B−V color index | +0.98[4] |
Astrometry | |
Radial velocity (Rv) | −27.1±0.4[5] km/s |
Proper motion (μ) | RA: +23.472 mas/yr[1] Dec.: −65.581 mas/yr[1] |
Parallax (π) | 9.9485 ± 0.0394 mas[1] |
Distance | 328 ± 1 ly (100.5 ± 0.4 pc) |
Absolute magnitude (MV) | +1.23[6] |
Details[7] | |
Mass | 2.42±0.04 M☉ |
Radius | 8.08±0.16 R☉ |
Luminosity | 36.9±0.8 L☉ |
Surface gravity (log g) | 2.94±0.08 cgs |
Temperature | 5,006±41 K |
Metallicity [Fe/H] | +0.16±0.03 dex |
Rotational velocity (v sin i) | 1.4±1.2[8] km/s |
Age | 761±9[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 182893, also known as HR 7388 or rarely 60 G. Telescopii, is a solitary, yellowish-orange hued star located in the southern constellation Telescopium. It has an apparent magnitude of 6.13,[2] making it barely visible to the naked eye even under ideal conditions. Based on Gaia DR3 parallax measurements, the object is estimated to be 328 light years away.[1] However, it is approaching the Solar System with a heliocentric radial velocity of −27 km/s.[5] At its current distance, HD 182893's brightness is diminished by 0.19 magnitudes due to interstellar dust.[12] It has an absolute magnitude of +1.23.[6]
HD 182893 has a stellar classification of K0/1 III,[3] indicating that it is an evolved K-type star with the characteristics of a K0 and K1 giant star. It has 2.42 times the mass of the Sun[7] but at the age of 761 million years,[9] it has expanded to 8.08 times the radius of the Sun. It radiates 36.9 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,006 K.[7] HD 182893 is particularly metal enriched with an iron abundance 145% that of the Sun's ([Fe/H] = +0.16).[7] Like most giant stars it spins slowly, having a projected rotational velocity of 1.4 km/s.[8]