| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Gemini |
| Right ascension | 07h 55m 39.89s |
| Declination | +19° 53′ 02.3″ |
| Apparent magnitude (V) | 5.365±0.009 |
| Characteristics | |
| Evolutionary stage | main-sequence |
| Spectral type | A0Vs |
| Astrometry | |
| Radial velocity (Rv) | 12.3 km/s |
| Proper motion (μ) | RA: -15.114 mas/yr Dec.: -39.83 mas/yr |
| Parallax (π) | 6.4022±0.1333 mas |
| Distance | 510 ± 10 ly (156 ± 3 pc) |
| Details | |
| Mass | 3.29 M☉ |
| Other designations | |
| 85 Gem, BD+20 1946, HD 64648, HIP 38722, HR 3086, SAO 79799, GCRV 5268, 2MASS J07553990+1953024, Gaia DR3 670326064263850624 | |
| Database references | |
| SIMBAD | data |
85 Geminorum (85 Gem) is an A-type main-sequence star located approximately 510 light-years from Earth in the constellation of Gemini. It is a relatively bright star with an apparent visual magnitude of approximately 5.37, making it visible to the naked eye under dark skies.
In 2005, 85 Geminorum was observed by NASA Infrared Telescope Facility and has served as an A0V spectrophotometric standard star in infrared spectroscopy to calibrate spectra of M, L, and T dwarf stars.
In a 2022 survey of visual binaries among intermediate-mass stars, 85 Geminorum was included with an estimated mass of approximately 3.29 M☉, placing it in the A-type stars mass range. Although, no companion stars have been detected.