Q92304758
high proper-motion star in the constellation Virgo
Press Enter · cited answer in seconds
0 sources
Q92304758
Summary
Q92304758 is a high proper-motion star[1].
Key Facts
- Q92304758's instance of is recorded as high proper-motion star[2].
- Q92304758's instance of is recorded as near-infrared source[3].
- Q92304758's constellation is recorded as Virgo[4].
- Q92304758's spectral class is recorded as M2.5[5].
- Q92304758's child astronomical body is recorded as TIC 176963071.01[6].
- Q92304758's catalog code is recorded as 2MASS J13534190-0045586[7].
- Q92304758's catalog code is recorded as Gaia DR2 3659074164939708544[8].
- Q92304758's catalog code is recorded as TIC 176963071[9].
- Q92304758's catalog code is recorded as Gaia DR3 3659074164939708544[10].
- Q92304758's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.684'}[11].
- Q92304758's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.030'}[12].
- Q92304758's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.811'}[13].
- Q92304758's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.255024'}[14].
- Q92304758's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+14.8315'}[15].
- Q92304758's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+67.424'}[16].
- Q92304758's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+208.42452470879'}[17].
- Q92304758's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-0.76631243708'}[18].
- Q92304758's epoch is recorded as J2000.0[19].
- Q92304758's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-86.555'}[20].
- Q92304758's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-128.837'}[21].
Body
Definition and Type
Recorded instance of include high proper-motion star[2] and near-infrared source[3].