Pi 4 Orionis

from Wikipedia, the free encyclopedia
Double star
π 4 Orionis
Orion constellation map.svg
Map pointer.svg
Observation
dates equinoxJ2000.0 , epoch : J2000.0
AladinLite
Constellation Orion
Right ascension 04 h 51 m 12.4 s
declination + 05 ° 36 ′ 18 ″
Apparent brightness  3.68 likes
Astrometry
Radial velocity (+23 ± 4) km / s
parallax (3.10 ± 0.18) mas
distance  (1050 ± 60) ly
((323 ± 19) pc )
Proper movement :
Rec. Share: (−2.21 ± 0.22) mas / a
Dec. portion: (+0.85 ± 0.12) mas / a
orbit 
period 9.52 d
eccentricity 0.033 ± 0.023
Epoch of the periastron JD 2418276
Argument of the periapsis 165 ° ± 40 °
Individual data
Names A; B.
Other names
and catalog entries
Bayer name π 4 Orionis
Flamsteed name 3 Orionis
Bonn survey BD + 5 ° 745
Bright Star Catalog HR 1552 [1]
Henry Draper Catalog HD 30836 [2]
SAO catalog SAO 112142 [3]
Tycho catalog TYC 92-2345-1 [4]
Hipparcos catalog HIP 22549 [5]
Further designations: FK5  179

π 4 Orionis (Pi 4 Orionis / π 4 Ori, also 3 Orionis ) is a spectroscopic double star in the constellation Orion . It is around 1000 light years from Earth. The period of rotation of the system is 9.5 days.

Web links

Individual evidence

  1. a b Hipparcos catalog (ESA 1997)
  2. Pulkovo radial velocities for 35493 HIP stars
  3. ^ Hipparcos, the New Reduction (van Leeuwen, 2007)