| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Antlia [1] |
| Right ascension | 10h 42m 43.1844s [2] |
| Declination | −32° 42′ 56.413″ [2] |
| Apparent magnitude (V) | 5.62±0.01 [3] |
| Characteristics | |
| Evolutionary stage | subgiant [4] |
| Spectral type | A0 V [5] |
| B−V color index | +0.00 [6] |
| Astrometry | |
| Radial velocity (Rv) | 4.5±0.5 [7] km/s |
| Proper motion (μ) | RA: −28.903 mas/yr [2] Dec.: +1.262 mas/yr [2] |
| Parallax (π) | 4.1113±0.2655 mas [2] |
| Distance | 790 ± 50 ly (240 ± 20 pc) |
| Absolute magnitude (MV) | −0.67 [1] |
| Details | |
| Mass | 3.1±0.1 [4] M☉ |
| Radius | 5.31 [8] R☉ |
| Luminosity | 206+72 −53 [4] L☉ |
| Surface gravity (log g) | 3.5 [9] cgs |
| Temperature | 9,376±109 [8] K |
| Metallicity [Fe/H] | 0.00 [10] dex |
| Rotational velocity (v sin i) | 81±3 [11] km/s |
| Age | 282±34 [12] Myr |
| Other designations | |
| 78 G. Antilae [13] , CD−32°7572, CPD−32°2953, FK5 1277, GC 14732, HIP 52407, HR 4194, SAO 201665, WDS J10427-3243A [14] | |
| Database references | |
| SIMBAD | data |
HD 92845 (HR 4194) is a probable astrometric binary [15] in the southern constellation Antlia. It has an apparent magnitude of 5.62, allowing it to be faintly seen with the naked eye. Parallax measurements place the system at a distance of 790 light years and it is currently receding with a heliocentric radial velocity of 4.5 km/s .
HD 92845 has a stellar classification of A0 V, [5] indicating that it is an ordinary A-type main-sequence star. However, stellar evolution models from Zorec and Royer reveal it to be a subgiant that has just left the main sequence. [4] It has 3.1 times the mass of the Sun [4] but has expanded to an enlarged radius of 5.31 R☉ . [8] It radiates with a luminosity 206 times greater than the Sun [4] from its photosphere at an effective temperature of 9,376 K , [8] giving a white hue. At an age of 282 million years, [12] HD 92845 spins quickly with a projected rotational velocity of 81 km/s . [11]
There is an optical companion 17″ away along a position angle of 214° as of 1999. [16]