Q86490330

Summary

Q86490330 is a star^[1].

Key Facts

• Q86490330's instance of is recorded as star^[2].
• Q86490330's constellation is recorded as Canis Major^[3].
• Q86490330 is part of Messier 41^[4].
• Q86490330's catalog code is recorded as 2MASS J06452735-2055283^[5].
• Q86490330's catalog code is recorded as Cl* NGC 2287 AR 11^[6].
• Q86490330's catalog code is recorded as Cl* NGC 2287 HFMR 90^[7].
• Q86490330's catalog code is recorded as Cl* NGC 2287 UVA 107^[8].
• Q86490330's catalog code is recorded as NGC 2287 90^[9].
• Q86490330's catalog code is recorded as GEN# +2.22870090^[10].
• Q86490330's catalog code is recorded as BD-20 1536^[11].
• Q86490330's catalog code is recorded as UCAC2 23555385^[12].
• Q86490330's catalog code is recorded as GSC 05961-00932^[13].
• Q86490330's catalog code is recorded as TYC 5961-932-1^[14].
• Q86490330's catalog code is recorded as CPD-20 1569^[15].
• Q86490330's catalog code is recorded as Gaia DR1 2926911566731283840^[16].
• Q86490330's catalog code is recorded as Gaia DR2 2926911571033324544^[17].
• Q86490330's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.00'}^[18].
• Q86490330's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.55'}^[19].
• Q86490330's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.924'}^[20].
• Q86490330's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.646'}^[21].
• Q86490330's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.584'}^[22].
• Q86490330's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.8584'}^[23].
• Q86490330's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.0927'}^[24].
• Q86490330's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+9.61'}^[25].
• Q86490330's metallicity is recorded as {'unit': '1', 'amount': '-0.05'}^[26].

Body

Definition and Type

Q86490330's instance of is recorded as star^[2].

Use and Application

Q86490330 is part of Messier 41^[4].