KOI-152

Summary

KOI-152 is a star^[1].

Key Facts

• KOI-152's instance of is recorded as star^[2].
• KOI-152's instance of is recorded as rotating variable star^[3].
• KOI-152's instance of is recorded as near-infrared source^[4].
• KOI-152's instance of is recorded as eruptive variable star^[5].
• KOI-152's constellation is recorded as Cygnus^[6].
• KOI-152's spectral class is recorded as F5^[7].
• KOI-152's part of is recorded as Q1348576^[8].
• KOI-152's child astronomical body is recorded as Q21030196^[9].
• KOI-152's child astronomical body is recorded as Q21030211^[10].
• KOI-152's child astronomical body is recorded as Q21030216^[11].
• KOI-152's child astronomical body is recorded as Q24954159^[12].
• KOI-152's catalog code is recorded as UCAC4 672-080422^[13].
• KOI-152's catalog code is recorded as UCAC3 269-182620^[14].
• KOI-152's catalog code is recorded as 2MASS J20020411+4422536^[15].
• KOI-152's catalog code is recorded as GSC2 N030222158999^[16].
• KOI-152's catalog code is recorded as KIC 8394721^[17].
• KOI-152's catalog code is recorded as Gaia DR2 2076085318570299136^[18].
• KOI-152's catalog code is recorded as KOI-152^[19].
• KOI-152's catalog code is recorded as Kepler-79^[20].
• KOI-152's catalog code is recorded as Gaia DR3 2076085318570299136^[21].
• KOI-152's catalog code is recorded as TIC 239306681^[22].
• KOI-152's catalog code is recorded as SPOCS 3800^[23].
• KOI-152's catalog code is recorded as SPOCS 3801^[24].
• KOI-152's type of variable star is recorded as rotating variable star^[25].
• KOI-152's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.55'}^[26].

Body

Geography

KOI-152's part of is recorded as Q1348576^[8].

Designation and Status

Recorded instance of include star^[2], rotating variable star^[3], near-infrared source^[4], and eruptive variable star^[5].

History and Context

Catalog codes include UCAC4 672-080422^[13], UCAC3 269-182620^[14], 2MASS J20020411+4422536^[15], GSC2 N030222158999^[16], KIC 8394721^[17], and Gaia DR2 2076085318570299136^[18].