Q77412030

Summary

Q77412030 is a low-mass star^[1].

Key Facts

• Q77412030's instance of is recorded as low-mass star^[2].
• Q77412030's constellation is recorded as Leo^[3].
• Q77412030's spectral class is recorded as M3V^[4].
• Q77412030's catalog code is recorded as SDSS J102520.20+091015.7^[5].
• Q77412030's catalog code is recorded as Gaia DR2 3875978324149667968^[6].
• Q77412030's redshift is recorded as {'unit': '1', 'amount': '+0.00020'}^[7].
• Q77412030's apparent magnitude is recorded as {'unit': '1', 'amount': '+22.097'}^[8].
• Q77412030's apparent magnitude is recorded as {'unit': '1', 'amount': '+21.255'}^[9].
• Q77412030's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.843'}^[10].
• Q77412030's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.883'}^[11].
• Q77412030's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.216'}^[12].
• Q77412030's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.7639'}^[13].
• Q77412030's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8356'}^[14].
• Q77412030's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+21'}^[15].
• Q77412030's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1049.6'}^[16].
• Q77412030's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+156.33418797837600'}^[17].
• Q77412030's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+9.17102506867340'}^[18].
• Q77412030's epoch is recorded as J2000.0^[19].
• Q77412030's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.938'}^[20].
• Q77412030's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.031'}^[21].

Body

Definition and Type

Q77412030's instance of is recorded as low-mass star^[2].