33 Piscium

33 Piscium
Observation data Epoch J2000 Equinox J2000
Constellation	Pisces
Right ascension	00^h 05^m 20.14193^s^[1]
Declination	−05° 42′ 27.4279″^[1]
Apparent magnitude (V)	4.61^[1]
Characteristics
Spectral type	K0IIIb^[1]
Apparent magnitude (U)	6.52^[1]
Apparent magnitude (B)	5.65
Apparent magnitude (V)	4.61
Apparent magnitude (R)	3.83
Apparent magnitude (I)	3.29
Apparent magnitude (J)	2.89
Apparent magnitude (H)	2.31
Apparent magnitude (K)	2.21
Astrometry

Radial velocity (R_v)	−6.56 ± 0.23^[1] km/s
Proper motion (μ)	RA: −6.54^[1] mas/yr Dec.: 87.85^[1] mas/yr
Parallax (π)	25.32 ± 0.53^[1] mas
Distance	129 ± 3 ly (39.5 ± 0.8 pc)

Other designations
33 Piscium (Flamsteed), BC Piscium (var.), BD−06° 6357, FK5 1002, GC 59, GCRV 36, GSC 04669-00996, HD 28, HIC 443, HIP 443, HR 3, 2MASS J00052013-0542275, PMC 90-93 649, PPM 181831, SAO 128572
Database references
SIMBAD	data

33 Piscium (33 Psc) is a star in the constellation Pisces. Its apparent magnitude is 4.61.

References

Stars of Pisces

Bayer	α (Alrescha) β (Fum al Samakah) γ δ ε ζ η (Kullat Nunu) θ ι κ λ μ ν ξ ο (Torcularis Septentrionalis) π ρ σ τ υ φ χ ψ¹ ψ² ψ³ ω

Flamsteed	1 2 3 5 7 9 11 12 13 14 15 16 20 21 22 24 25 26 27 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 51 52 53 54 55 57 58 59 60 61 62 64 65 66 67 68 70 72 73 75 76 77 78 80 82 87 88 89 91 92 94 95 96 97 100 101 103 104 105 107 109 112 4 Cet 5 Cet

Variable	R Y RU RV RZ SS SV SZ TX (19) TY UV UZ VY (3 Ari) VZ WW WX WZ XZ AO AQ AR AY AZ BE BK BR BT BU CY DT DV DZ EO FL GU

HR	2 29 67 69 94 107 141 145 161 222 243 259 276 277 303 341 344 356 371 374 397 407 426 450 457 484 527 8730 8734 8735 8738 8751 8776 8785 8897 8983 9015

HD	26 1502 2358 4203 4313 5418 5891 7107 8574 8733 9496 9986 10262 12730 217590 217786 218566 219188 224690

Gliese	GJ 1286 GJ 3076 GJ 3128

Other	Bond's flare star CS 22949-037 Feige 110 G 29-38 2MASS 0036+1821 NGC 33 NGC 46 PG 0014+067 PG 0122+200 PSR J0030+0451 1RXS J232953.9+062814 SIMP J013656.5+093347 van Maanen 2 WASP-28 WASP-32

List

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