Q79175473
Press Enter · cited answer in seconds
0 sources
Q79175473
Summary
Q79175473 is a S-type star[1].
Key Facts
- Q79175473's instance of is recorded as S-type star[2].
- Q79175473's instance of is recorded as infrared source[3].
- Q79175473's instance of is recorded as long-period variable star[4].
- Q79175473's instance of is recorded as near-infrared source[5].
- Q79175473's constellation is recorded as Orion[6].
- Q79175473's spectral class is recorded as S[7].
- Q79175473's catalog code is recorded as 2MASS J05522785+0620530[8].
- Q79175473's catalog code is recorded as GSC 00128-01121[9].
- Q79175473's catalog code is recorded as IRAS 05497+0620[10].
- Q79175473's catalog code is recorded as Gaia DR2 3321104116131835904[11].
- Q79175473's catalog code is recorded as V1623 Ori[12].
- Q79175473's catalog code is recorded as TIC 80836366[13].
- Q79175473's catalog code is recorded as Gaia DR3 3321104116131835904[14].
- Q79175473's type of variable star is recorded as SRa semi-regular variable star[15].
- Q79175473's type of variable star is recorded as long-period variable star[16].
- Q79175473's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.968'}[17].
- Q79175473's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.952'}[18].
- Q79175473's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.609'}[19].
- Q79175473's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.150414'}[20].
- Q79175473's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1733'}[21].
- Q79175473's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+59.07'}[22].
- Q79175473's SIMBAD ID is recorded as V* V1623 Ori[23].
- Q79175473's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+88.11609802659'}[24].
- Q79175473's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+6.3480735359'}[25].
- Q79175473's epoch is recorded as J2000.0[26].