Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Serpens |
Right ascension | 15h 44m 42.1323s [1] |
Declination | +17° 15′ 51.197″ [1] |
Apparent magnitude (V) | 6.144 [1] |
Characteristics | |
Spectral type | A0V [1] |
U−B color index | −0.03 [2] |
B−V color index | 0.00 [2] |
Astrometry | |
Radial velocity (Rv) | −5.2 ± 5 [1] km/s |
Proper motion (μ) |
RA: −30.44
[1]
mas/
yr Dec.: 6.59 [1] mas/ yr |
Parallax (π) | 10.16 ± 0.79 mas [1] |
Distance | 320 ± 20
ly (98 ± 8 pc) |
Absolute magnitude (MV) | 0.88 [3] |
Details | |
Radius | 2.0 [4] R☉ |
Rotational velocity (v sin i) | 76 [2] km/s |
Other designations | |
τ8 Ser, Tau8 Ser,
26 Serpentis,
BD+17° 2906,
GC 21164,
HD 140729,
HIP 77111,
HR 5858,
SAO 101712,
PPM 131656
[1] | |
Database references | |
SIMBAD | data |
Tau8 Serpentis, Latinized from τ8 Serpentis, is an A-type main sequence star in the constellation of Serpens, approximately 320 light-years from the Earth. [1] It has an apparent visual magnitude of approximately 6.144. [1] Although it was observed to be binary by speckle interferometry in 1985, subsequent observations show no sign of binarity, and the detection appears to have been spurious. [5]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Serpens |
Right ascension | 15h 44m 42.1323s [1] |
Declination | +17° 15′ 51.197″ [1] |
Apparent magnitude (V) | 6.144 [1] |
Characteristics | |
Spectral type | A0V [1] |
U−B color index | −0.03 [2] |
B−V color index | 0.00 [2] |
Astrometry | |
Radial velocity (Rv) | −5.2 ± 5 [1] km/s |
Proper motion (μ) |
RA: −30.44
[1]
mas/
yr Dec.: 6.59 [1] mas/ yr |
Parallax (π) | 10.16 ± 0.79 mas [1] |
Distance | 320 ± 20
ly (98 ± 8 pc) |
Absolute magnitude (MV) | 0.88 [3] |
Details | |
Radius | 2.0 [4] R☉ |
Rotational velocity (v sin i) | 76 [2] km/s |
Other designations | |
τ8 Ser, Tau8 Ser,
26 Serpentis,
BD+17° 2906,
GC 21164,
HD 140729,
HIP 77111,
HR 5858,
SAO 101712,
PPM 131656
[1] | |
Database references | |
SIMBAD | data |
Tau8 Serpentis, Latinized from τ8 Serpentis, is an A-type main sequence star in the constellation of Serpens, approximately 320 light-years from the Earth. [1] It has an apparent visual magnitude of approximately 6.144. [1] Although it was observed to be binary by speckle interferometry in 1985, subsequent observations show no sign of binarity, and the detection appears to have been spurious. [5]