54 Piscium

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54 Piscium
Observation data
Epoch J2000
Constellation
(pronunciation)
Pisces
Right ascension 00h 39m 21.8s
Declination +21° 15′ 01.7″
Apparent magnitude (V) 5.80
Characteristics
Spectral type K0 V
U-B color index 0.57
B-V color index 0.85
Variable type Suspected
Astrometry
Radial velocity (Rv) −34.2 km/s
Proper motion (μ) RA: −461.09 mas/yr
Dec.: −370.90 mas/yr
Parallax (π) 90.03 ± 0.72 mas
Distance 36.2 ± 0.3 ly
(11.11 ± 0.09 pc)
Absolute magnitude (MV) 5.65
Details
Mass 0.78 M
Radius 0.86 R
Luminosity 0.48 L
Metallicity 110%
Planet
Companion
b
Mass (MJ)
>0.227
Orbital period (days)
62.206
Semimajor axis (AU)
0.296
Eccentricity
0.618


Other designations
GJ 27, HR 166, BD +20°85, HD 3651, LHS 1116, LTT 10224, GCTP 110.00, SAO 74175, LFT 59, NSV 245, HIP 3093.

54 Piscium (abbreviated 54 Psc) is a 6th magnitude star in the constellation of Pisces. It is classified as an orange dwarf star (spectral class K0 V) and is somewhat less massive and luminous than our Sun. The star is relatively nearby, distance being only 36 light years. It is visible to the unaided eye under very good conditions. The planet 54 Piscium b was found orbiting the star in 2003.[1] The star is also suspected to be variable in brightness.


Contents

[edit] 54 Piscium B

54 Piscium B
Observation data
Epoch 2000
Constellation
(pronunciation)
Pisces
Right ascension 0h 39m 32s
Declination +21° 15' 15"
Distance 36.2 ± 0.3 ly
(11.11 ± 0.09 pc)
Spectral type T
Other designations
BD+20°85B

54 Piscium has a companion which was classified as a T class brown dwarf with mass 50 times the mass of Jupiter. It was imaged by Spitzer Space Telescope. It's orbit has a 500AU radius and orbital period of more than a thousand years.[2]


[edit] References

  1. ^ Fischer et al. (2003). "A Sub-Saturn Mass Planet Orbiting HD 3651". The Astrophysical Journal 590 (2): 1081 – 1087. doi:10.1086/375027. 
  2. ^ SPACE.com - Distorted Solar System Discovered

[edit] See also

[edit] External links