HD210767

Summary

HD210767 is a peculiar star^[1].

Key Facts

• HD210767's instance of is recorded as peculiar star^[2].
• HD210767's instance of is recorded as high proper-motion star^[3].
• HD210767's constellation is recorded as Grus^[4].
• HD210767's spectral class is recorded as F0IV^[5].
• HD210767's catalog code is recorded as HD 210767^[6].
• HD210767's catalog code is recorded as CCDM J22134-3729AB^[7].
• HD210767's catalog code is recorded as CPC 18 11389^[8].
• HD210767's catalog code is recorded as GSC 07502-00104^[9].
• HD210767's catalog code is recorded as IDS 22075-3759 AB^[10].
• HD210767's catalog code is recorded as 2MASS J22132394-3729026^[11].
• HD210767's catalog code is recorded as PPM 302320^[12].
• HD210767's catalog code is recorded as SAO 213645^[13].
• HD210767's catalog code is recorded as TD1 28865^[14].
• HD210767's catalog code is recorded as WDS J22134-3729AB^[15].
• HD210767's catalog code is recorded as TYC 7502-104-1^[16].
• HD210767's catalog code is recorded as Gaia DR2 6574109597341814784^[17].
• HD210767's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.12'}^[18].
• HD210767's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.78'}^[19].
• HD210767's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.7327'}^[20].
• HD210767's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.208'}^[21].
• HD210767's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.095'}^[22].
• HD210767's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.035'}^[23].
• HD210767's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2141'}^[24].
• HD210767's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-25.08'}^[25].
• HD210767's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+333.34973716395230'}^[26].

Body

Definition and Type

Recorded instance of include peculiar star^[2] and high proper-motion star^[3].