Q75073317
long-period variable star in the constellation Puppis
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Q75073317
Summary
Q75073317 is a long-period variable star[1].
Key Facts
- Q75073317's instance of is recorded as long-period variable star[2].
- Q75073317's instance of is recorded as infrared source[3].
- Q75073317's instance of is recorded as near-infrared source[4].
- Q75073317's constellation is recorded as Puppis[5].
- Q75073317's spectral class is recorded as M5:[6].
- Q75073317's catalog code is recorded as GSC 05989-01870[7].
- Q75073317's catalog code is recorded as HD 62982[8].
- Q75073317's catalog code is recorded as IRAS 07437-1902[9].
- Q75073317's catalog code is recorded as PPM 219162[10].
- Q75073317's catalog code is recorded as CQ Pup[11].
- Q75073317's catalog code is recorded as 2MASS J07455713-1910107[12].
- Q75073317's catalog code is recorded as UCAC2 24309766[13].
- Q75073317's catalog code is recorded as Gaia DR1 5716075698261230336[14].
- Q75073317's catalog code is recorded as Gaia DR2 5716075698261230336[15].
- Q75073317's catalog code is recorded as TYC 5989-1870-1[16].
- Q75073317's catalog code is recorded as TIC 140871007[17].
- Q75073317's catalog code is recorded as Gaia DR3 5716075698261230336[18].
- Q75073317's type of variable star is recorded as slow irregular variables of late spectral types[19].
- Q75073317's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.89'}[20].
- Q75073317's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.32'}[21].
- Q75073317's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.584'}[22].
- Q75073317's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.449'}[23].
- Q75073317's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.105'}[24].
- Q75073317's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.502685'}[25].
- Q75073317's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8852'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].