Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
59 And A | |
Right ascension | 02h 10m 52.82451s[1] |
Declination | +39° 02′ 22.3597″[1] |
Apparent magnitude (V) | 6.09[2] |
59 And B | |
Right ascension | 02h 10m 53.65687s[1] |
Declination | +39° 02′ 35.9164″[1] |
Apparent magnitude (V) | 6.82[2] |
Characteristics | |
59 And A | |
Spectral type | B9 V[3] |
B−V color index | −0.054±0.006[2] |
59 And B | |
Spectral type | A1 Vn[3] |
B−V color index | +0.081±0.005[2] |
Astrometry | |
59 And A | |
Radial velocity (Rv) | −1.00±3.4[4] km/s |
Proper motion (μ) | RA: −13.506[1] mas/yr Dec.: −14.981[1] mas/yr |
Parallax (π) | 7.1469 ± 0.1007 mas[1] |
Distance | 456 ± 6 ly (140 ± 2 pc) |
59 And B | |
Radial velocity (Rv) | 6.0±4.6[4] km/s |
Proper motion (μ) | RA: −9.166[1] mas/yr Dec.: −17.208[1] mas/yr |
Parallax (π) | 7.4166 ± 0.0619 mas[1] |
Distance | 440 ± 4 ly (135 ± 1 pc) |
Details | |
59 And A | |
Radius | 2.73[5] R☉ |
Luminosity | 83.97[6] L☉ |
Temperature | 10,870[6] K |
Rotational velocity (v sin i) | 176[3] km/s |
59 And B | |
Mass | 2.23±0.09[7] M☉ |
Radius | 2.59[5] R☉ |
Luminosity | 30.4+7.6 −6.1[7] L☉ |
Temperature | 9,498[6] K |
Rotational velocity (v sin i) | 233[3] km/s |
Other designations | |
59 And A: GC 2600, HD 13294, HIP 10176, HR 628, SAO 55330, PPM 67045[9] | |
59 And B: GC 2602, HD 13295, HIP 10180, HR 629, SAO 55331, PPM 67046[10] | |
Database references | |
SIMBAD | data |
SIMBAD | data |
59 Andromedae, abbreviated 59 And, is a sixth-magnitude binary star system in the northern constellation of Andromeda. 59 Andromedae is the Flamsteed designation. As of 2017, the pair had an angular separation of 16.60″ along a position angle (PA) of 36°. Compare this to a separation of 15.3″ along a PA of 35°, as measured in 1783.[11] The two stars have an estimated physical separation of 1,370 AU.[5]
The magnitude 6.09[2] primary component is a B-type main-sequence star with a stellar classification of B9 V.[3] It has 2.73[5] times the Sun's radius and is radiating 84 times the Sun's luminosity from its photosphere at an effective temperature of 10,870 K.[6] It is spinning with a projected rotational velocity of 176 km/s.[3]
The secondary is a magnitude 6.82[2] A-type main-sequence star with a class of A1 Vn,[3] where the 'n' suffix indicates "nebulous" lines due to rapid rotation. It is spinning with a high projected rotational velocity of 233 km/s.[3] The star has 2.23[7] times the Sun's mass and 2.59[5] times the Sun's radius. It is radiating 30[7] times the luminosity of the Sun and has an effective temperature of 9,498 K.[6]
GaiaDR2
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Royer2007
was invoked but never defined (see the help page).deBruijne2012
was invoked but never defined (see the help page).Howe2009
was invoked but never defined (see the help page).McDonald2012
was invoked but never defined (see the help page).Zorec2012
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).SIMBAD_A
was invoked but never defined (see the help page).SIMBAD_B
was invoked but never defined (see the help page).WDSC2011
was invoked but never defined (see the help page).