2MASSW J0920122+351742
brown dwarf
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2MASSW J0920122+351742
Summary
2MASSW J0920122+351742 is a brown dwarf[1].
Key Facts
- 2MASSW J0920122+351742's instance of is recorded as brown dwarf[2].
- 2MASSW J0920122+351742's instance of is recorded as binary star[3].
- 2MASSW J0920122+351742's instance of is recorded as spectroscopic binary[4].
- 2MASSW J0920122+351742's instance of is recorded as infrared source[5].
- 2MASSW J0920122+351742's constellation is recorded as Lynx[6].
- 2MASSW J0920122+351742's spectral class is recorded as L5.5:+L9:.[7].
- 2MASSW J0920122+351742's catalog code is recorded as 2MASS J09201223+3517429[8].
- 2MASSW J0920122+351742's catalog code is recorded as WDS J09202+3518AB[9].
- 2MASSW J0920122+351742's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.625'}[10].
- 2MASSW J0920122+351742's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.673'}[11].
- 2MASSW J0920122+351742's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.979'}[12].
- 2MASSW J0920122+351742's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+34.40'}[13].
- 2MASSW J0920122+351742's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+21'}[14].
- 2MASSW J0920122+351742's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+140.051000'}[15].
- 2MASSW J0920122+351742's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+35.295278'}[16].
- 2MASSW J0920122+351742's epoch is recorded as J2000.0[17].
- 2MASSW J0920122+351742's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-200'}[18].
- 2MASSW J0920122+351742's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-167'}[19].
Body
Definition and Type
Recorded instance of include brown dwarf[2], binary star[3], spectroscopic binary[4], and infrared source[5].