Global Information Lookup Global Information

Chi1 Orionis information


Chi1 Orionis A

Star map of the Bayers Stars in Orion. Chi1 Orionis is indicated.
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 54m 22.98s[1]
Declination +20° 16′ 34.2″[1]
Apparent magnitude (V) 4.38 - 4.41[2]
Characteristics
Spectral type G0 V[3]
U−B color index +0.07[4]
B−V color index +0.59[4]
Variable type RS CVn[2]
Astrometry
Radial velocity (Rv)−15.42[5] km/s
Proper motion (μ) RA: −162.54±0.28[1] mas/yr
Dec.: −99.51±0.16[1] mas/yr
Parallax (π)115.43 ± 0.27 mas[1]
Distance28.26 ± 0.07 ly
(8.66 ± 0.02 pc)
Absolute magnitude (MV)4.82±0.005[6]
Orbit[7]
Period (P)5156.291±2.508 d
Semi-major axis (a)89.662±0.880 Mas
Eccentricity (e)0.452±0.002
Inclination (i)95.937±0.790°
Longitude of the node (Ω)126.360±0.593°
Periastron epoch (T)2451468.2±3.083 JD
Argument of periastron (ω)
(secondary)
111.527±0.230°
Semi-amplitude (K1)
(primary)
1.876±0.003 km/s
Details
primary
Mass1.01[8] M
Radius0.979±0.009[9] R
Luminosity1.081±0.018[9] L
Surface gravity (log g)4.39[8] cgs
Temperature5,955±6.1[10] K
Metallicity [Fe/H]−0.01[11] dex
Rotation5.2 days[11]
Rotational velocity (v sin i)8.7[8] km/s
Age300–400[12] Myr
companion
Mass0.15[8] M
Age70-130[8] Myr
Other designations
54 Ori, Gl 222, HR 2047, BD+20°1162, HD 39587, LTT 11743, GCTP 1354.00, SAO 77705, HIP 27913
Database references
SIMBADdata

Chi1 Orionis1 Ori, χ1 Orionis) is a star about 28 light years away.[1] It is in the constellation Orion, where it can be seen in the tip of the hunter's upraised club.[13]

A light curve for Chi1 Orionis, plotted from TESS data.[14] The 5.5 day period derived by Stępień and Geyer is marked in red.

χ1 Ori is a G0V star.[8] It is listed in the General Catalog of Variable Stars as an RS Canum Venaticorum variable, varying between visual magnitude 4.38 and 4.41.[2] Stępień and Geyer measured its period to be 5.5 days.[15]

χ1 Ori has a faint companion with a mass estimated at 15% of the mass of the Sun, and an orbital period of 14.1 years. The companion orbits an average distance of 6.1 AU from the primary, but has a fairly high orbital eccentricity, ranging from 3.3 AU out to 8.9 AU from the primary. Because of this red dwarf companion, the likelihood of habitable planets in this system is low. It is thought that the companion is a red dwarf still contracting towards the main sequence.[8]

A necessary condition for the existence of a planet in this system are stable zones where the object can remain in orbit for long intervals. For hypothetical planets in a circular orbit around the individual members of this star system, this maximum orbital radius is computed to be 1.01 AU for the primary and 0.41 AU for the secondary. (Note that the orbit of the Earth is 1 AU from the Sun.) A planet orbiting outside of both stars would need to be at least 18.4 AU distant.[16]

χ1 Ori is a candidate stream star member of the Ursa Major Moving Group, although there is some evidence to the contrary.[11]

  1. ^ a b c d e f Cite error: The named reference van Leeuwen2007 was invoked but never defined (see the help page).
  2. ^ a b c Cite error: The named reference gcvs was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference perkins was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference hr was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference dr3 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference park2013 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference Han2002 was invoked but never defined (see the help page).
  8. ^ a b c d e f g Cite error: The named reference konig2015 was invoked but never defined (see the help page).
  9. ^ a b Cite error: The named reference apj746_1_101 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference aaa411_3_559 was invoked but never defined (see the help page).
  11. ^ a b c Cite error: The named reference aaa521_A12 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference apj687 was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference kaler was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference Stepien was invoked but never defined (see the help page).
  16. ^ Cite error: The named reference mnras427_4_2723 was invoked but never defined (see the help page).

and 4 Related for: Chi1 Orionis information

Request time (Page generated in 0.7581 seconds.)

Chi1 Orionis

Last Update:

Chi1 Orionis (χ1 Ori, χ1 Orionis) is a star about 28 light years away. It is in the constellation Orion, where it can be seen in the tip of the hunter's...

Word Count : 842

Chi2 Orionis

Last Update:

above it, 35th.[citation needed] Chi1 Orionis is an unrelated, yellow, main sequence star over two degrees away. χ2 Orionis has a B2 bright supergiant spectrum...

Word Count : 753

Chi Orionis

Last Update:

Chi Orionis (Chi Ori, χ Orionis, χ Ori) is the name of two stars: Chi1 Orionis (54 Orionis, HD 39587) Chi2 Orionis (62 Orionis, HD 41117) All of them were...

Word Count : 102

List of nearest stars by spectral type

Last Update:

; Jayawardhana, R. (2002-11-01). "Direct detection of the companion of Orionis". Astronomy & Astrophysics. 394 (3): L43–L46. doi:10.1051/0004-6361:20021377...

Word Count : 13260

PDF Search Engine © AllGlobal.net