Q89318237

Summary

Q89318237 is a high proper-motion star^[1].

Key Facts

• Q89318237's instance of is recorded as high proper-motion star^[2].
• Q89318237's instance of is recorded as near-infrared source^[3].
• Q89318237's instance of is recorded as rotating variable star^[4].
• Q89318237's instance of is recorded as astrophysical X-ray source^[5].
• Q89318237's constellation is recorded as Pictor^[6].
• Q89318237's child astronomical body is recorded as TOI-540 b^[7].
• Q89318237's catalog code is recorded as 2MASS J05051443-4756154^[8].
• Q89318237's catalog code is recorded as UCAC4 211-005570^[9].
• Q89318237's catalog code is recorded as Gaia DR2 4785886941312921344^[10].
• Q89318237's catalog code is recorded as 1RXS J050514.2-475625^[11].
• Q89318237's catalog code is recorded as TOI-540^[12].
• Q89318237's catalog code is recorded as Gaia DR3 4785886941312921344^[13].
• Q89318237's catalog code is recorded as TIC 200322593^[14].
• Q89318237's type of variable star is recorded as rotating variable star^[15].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.755'}^[16].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.170'}^[17].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.900'}^[18].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.873695'}^[19].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.126'}^[20].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.748'}^[21].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.076'}^[22].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.365'}^[23].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.96'}^[24].
• Q89318237's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.157'}^[25].
• Q89318237's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.159'}^[26].

Body

Definition and Type

Recorded instance of include high proper-motion star^[2], near-infrared source^[3], rotating variable star^[4], and astrophysical X-ray source^[5].