3 Piscis Austrini
Star in the constellation Microscopium
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3 Piscis Austrini, also known as HD 201901 or simply 3 PsA, is an astrometric binary[14] (100% chance[15]) located in the southern constellation Microscopium. It was once part of Piscis Austrinus, the southern fish. The system has a combined apparent magnitude of 5.39,[3] making it faintly visible to the naked eye under ideal conditions. Gaia DR3 parallax measurements imply a distance of 404 light years[2] and it is currently approaching the Solar System with a heliocentric radial velocity of −46.2 km/s.[6] At its current distance, 3 PsA's brightness is diminished by 0.12 magnitudes due to extinction from interstellar dust[16] and it has an absolute magnitude of +0.19.[1]
 | |
| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Microscopium[1] |
| Right ascension | 21h 13m 17.32730s[2] |
| Declination | −27° 37′ 09.7106″[2] |
| Apparent magnitude (V) | 5.39±0.01[3] |
| Characteristics | |
| Spectral type | K3 III[4] |
| B−V color index | +1.42[5] |
| Astrometry | |
| Radial velocity (Rv) | −46.2±2.4[6] km/s |
| Proper motion (μ) | RA: +98.513 mas/yr[2] Dec.: −110.906 mas/yr[2] |
| Parallax (π) | 8.0734±0.1733 mas[2] |
| Distance | 404 ± 9 ly (124 ± 3 pc) |
| Absolute magnitude (MV) | +0.19[1] |
| Details | |
| Mass | 1.58[7] M☉ |
| Radius | 31.3±1.6[8] R☉ |
| Luminosity | 184+9 −8[2] L☉ |
| Surface gravity (log g) | 1.86[9] cgs |
| Temperature | 4,225±123[10] K |
| Metallicity [Fe/H] | −0.17[9] dex |
| Rotational velocity (v sin i) | <1[11] km/s |
| Age | 2.59+0.83 −1.90[2] Gyr |
| Other designations | |
| 3 PsA, 58 G. Microscopii[12], CD−28°17178, CPD−28°7411, FK5 1556, GC 29652, HD 201901, HIP 104750, HR 8110, SAO 190129[13] | |
| Database references | |
| SIMBAD | data |
The visible component is an evolved red giant with a stellar classification of K3 III.[4] The interferometry-measured angular diameter of the star, after correcting for limb darkening, is 2.03±0.04 mas,[17] which, at its estimated distance, equates to a physical radius of about 20 times the radius of the Sun.[18] However, its actual empirical radius is 31.3 R☉.[8] It has 1.58 times the mass of the Sun[7] and is radiating 184 times the luminosity of the Sun[2] from its enlarged photosphere at an effective temperature of 4,225 K.[10] 3 PsA is metal deficient with an iron abundance 68% that of the Sun ([Fe/H] = −0.17)[9] and it spins too slowly for its projected rotational velocity to be measured accurately.[11] It is estimated to be 2.59 billion years old based on Gaia DR3 models.[2]
