Q80948988
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Q80948988
Summary
Q80948988 is a brown dwarf[1].
Key Facts
- Q80948988's instance of is recorded as brown dwarf[2].
- Q80948988's instance of is recorded as low-mass star[3].
- Q80948988's constellation is recorded as Lepus[4].
- Q80948988's spectral class is recorded as M7.6V[5].
- Q80948988's catalog code is recorded as 2MASSI J0544115-243301[6].
- Q80948988's catalog code is recorded as 2MUCD 10444[7].
- Q80948988's catalog code is recorded as 2MASS J05441150-2433018[8].
- Q80948988's catalog code is recorded as WISEA J054411.66-243309.5[9].
- Q80948988's catalog code is recorded as Gaia DR2 2915187925218983296[10].
- Q80948988's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.532'}[11].
- Q80948988's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.874'}[12].
- Q80948988's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.463'}[13].
- Q80948988's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.9407'}[14].
- Q80948988's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+48.4871'}[15].
- Q80948988's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+21'}[16].
- Q80948988's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+20.6240'}[17].
- Q80948988's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.04801258038560'}[18].
- Q80948988's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-24.55069771281900'}[19].
- Q80948988's epoch is recorded as J2000.0[20].
- Q80948988's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-678.315'}[21].
- Q80948988's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+183.426'}[22].
Body
Definition and Type
Recorded instance of include brown dwarf[2] and low-mass star[3].