Q81162137
long period variable
Press Enter · cited answer in seconds
0 sources
Q81162137
Summary
Q81162137 is a long-period variable star[1].
Key Facts
- Q81162137's instance of is recorded as long-period variable star[2].
- Q81162137's constellation is recorded as Crater[3].
- Q81162137's spectral class is recorded as M4III[4].
- Q81162137's catalog code is recorded as BD-08 3081[5].
- Q81162137's catalog code is recorded as GSC 05501-00305[6].
- Q81162137's catalog code is recorded as HD 96297[7].
- Q81162137's catalog code is recorded as IRAS 11034-0853[8].
- Q81162137's catalog code is recorded as IRC -10248[9].
- Q81162137's catalog code is recorded as PPM 194112[10].
- Q81162137's catalog code is recorded as SAO 137985[11].
- Q81162137's catalog code is recorded as TYC 5501-305-1[12].
- Q81162137's catalog code is recorded as YZ 98 4188[13].
- Q81162137's catalog code is recorded as 2MASS J11055840-0909159[14].
- Q81162137's catalog code is recorded as Gaia DR1 3759235821643760768[15].
- Q81162137's catalog code is recorded as Gaia DR2 3759235825939969408[16].
- Q81162137's catalog code is recorded as RW Crt[17].
- Q81162137's type of variable star is recorded as SRb semi-regular variable star[18].
- Q81162137's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.26'}[19].
- Q81162137's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.85'}[20].
- Q81162137's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.830'}[21].
- Q81162137's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.798'}[22].
- Q81162137's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.492'}[23].
- Q81162137's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.0437'}[24].
- Q81162137's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3195'}[25].
- Q81162137's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+757.8628'}[26].
Body
Definition and Type
Q81162137's instance of is recorded as long-period variable star[2].