Q85247188
long period variable
Press Enter · cited answer in seconds
0 sources
Q85247188
Summary
Q85247188 is a long-period variable star[1].
Key Facts
- Q85247188's instance of is recorded as long-period variable star[2].
- Q85247188's instance of is recorded as infrared source[3].
- Q85247188's instance of is recorded as near-infrared source[4].
- Q85247188's constellation is recorded as Vela[5].
- Q85247188's spectral class is recorded as M6[6].
- Q85247188's catalog code is recorded as CF 5757[7].
- Q85247188's catalog code is recorded as GSC 08170-00918[8].
- Q85247188's catalog code is recorded as HD 79669[9].
- Q85247188's catalog code is recorded as IRAS 09120-4826[10].
- Q85247188's catalog code is recorded as PPM 756505[11].
- Q85247188's catalog code is recorded as 2MASS J09134394-4839051[12].
- Q85247188's catalog code is recorded as Gaia DR1 5326043602076609152[13].
- Q85247188's catalog code is recorded as Gaia DR2 5326043606376335104[14].
- Q85247188's catalog code is recorded as GH Vel[15].
- Q85247188's catalog code is recorded as TYC 8170-918-1[16].
- Q85247188's catalog code is recorded as TIC 356079977[17].
- Q85247188's catalog code is recorded as Gaia DR3 5326043606376335104[18].
- Q85247188's type of variable star is recorded as SRb semi-regular variable star[19].
- Q85247188's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.26'}[20].
- Q85247188's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.59'}[21].
- Q85247188's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.258'}[22].
- Q85247188's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.936'}[23].
- Q85247188's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.271'}[24].
- Q85247188's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.440137'}[25].
- Q85247188's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.7068'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].