HD 200466
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HD 200466
Summary
HD 200466 is a binary star[1].
Key Facts
- HD 200466's instance of is recorded as binary star[2].
- HD 200466's instance of is recorded as double star[3].
- HD 200466's instance of is recorded as star[4].
- HD 200466's constellation is recorded as Cygnus[5].
- HD 200466's spectral class is recorded as K0V+K0V[6].
- HD 200466's has part is recorded as Q73983083[7].
- HD 200466's has part is recorded as Q83614472[8].
- HD 200466's catalog code is recorded as AG+37 2065[9].
- HD 200466's catalog code is recorded as BD+37 4153[10].
- HD 200466's catalog code is recorded as HD 200466[11].
- HD 200466's catalog code is recorded as HIC 103824[12].
- HD 200466's catalog code is recorded as HIP 103824[13].
- HD 200466's catalog code is recorded as PPM 85906[14].
- HD 200466's catalog code is recorded as SAO 70816[15].
- HD 200466's catalog code is recorded as WDS J21024+3739AB[16].
- HD 200466's catalog code is recorded as uvby98 100200466[17].
- HD 200466's catalog code is recorded as IDS 20585+3716 AB[18].
- HD 200466's catalog code is recorded as GC 29376[19].
- HD 200466's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+22.53'}[20].
- HD 200466's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-8.3'}[21].
- HD 200466's SIMBAD ID is recorded as HD 200466[22].
- HD 200466's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+315.591270883'}[23].
- HD 200466's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.653871491'}[24].
- HD 200466's epoch is recorded as J2000.0[25].
- HD 200466's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5641'}[26].
Body
Designation and Status
Recorded instance of include binary star[2], double star[3], and star[4].
History and Context
Catalog codes include AG+37 2065[9], BD+37 4153[10], HD 200466[11], HIC 103824[12], HIP 103824[13], and PPM 85906[14].