Q75251855
long-period variable star in the constellation Octans
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Q75251855
Summary
Q75251855 is a long-period variable star[1].
Key Facts
- Q75251855's instance of is recorded as long-period variable star[2].
- Q75251855's instance of is recorded as infrared source[3].
- Q75251855's instance of is recorded as near-infrared source[4].
- Q75251855's constellation is recorded as Octans[5].
- Q75251855's catalog code is recorded as 2MASS J00375288-8237136[6].
- Q75251855's catalog code is recorded as GSC 09490-01842[7].
- Q75251855's catalog code is recorded as IRAS 00367-8253[8].
- Q75251855's catalog code is recorded as NSV 244[9].
- Q75251855's catalog code is recorded as PPM 375964[10].
- Q75251855's catalog code is recorded as DW Oct[11].
- Q75251855's catalog code is recorded as UCAC2 164630[12].
- Q75251855's catalog code is recorded as Gaia DR1 4630122869920541568[13].
- Q75251855's catalog code is recorded as Gaia DR2 4630122874216769920[14].
- Q75251855's catalog code is recorded as TYC 9490-1842-1[15].
- Q75251855's catalog code is recorded as TIC 318608473[16].
- Q75251855's catalog code is recorded as Gaia DR3 4630122874216769920[17].
- Q75251855's type of variable star is recorded as SRb semi-regular variable star[18].
- Q75251855's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.07'}[19].
- Q75251855's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.46'}[20].
- Q75251855's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.230'}[21].
- Q75251855's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.223'}[22].
- Q75251855's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.896'}[23].
- Q75251855's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.653591'}[24].
- Q75251855's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9656'}[25].
- Q75251855's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.41'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].