Q92801615
Press Enter · cited answer in seconds
0 sources
Q92801615
Summary
Q92801615 is an eruptive variable star[1].
Key Facts
- Q92801615's instance of is recorded as eruptive variable star[2].
- Q92801615's constellation is recorded as Taurus[3].
- Q92801615's spectral class is recorded as K7[4].
- Q92801615 is part of Pleiades[5].
- Q92801615's catalog code is recorded as 2MASS J03485896+2506142[6].
- Q92801615's catalog code is recorded as UCAC4 576-009149[7].
- Q92801615's catalog code is recorded as Gaia DR2 66925902692325504[8].
- Q92801615's catalog code is recorded as Cl* Melotte 22 LLP 67[9].
- Q92801615's catalog code is recorded as CSV 6056[10].
- Q92801615's catalog code is recorded as GEN# +5.20222082[11].
- Q92801615's catalog code is recorded as UBV M 41138[12].
- Q92801615's catalog code is recorded as Cl Melotte 22 2082[13].
- Q92801615's catalog code is recorded as Cl* Melotte 22 HII 2082[14].
- Q92801615's catalog code is recorded as Cl* Melotte 22 SRS 52001[15].
- Q92801615's catalog code is recorded as V354 Tau[16].
- Q92801615's type of variable star is recorded as flare star[17].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.571'}[18].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.745'}[19].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.406'}[20].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.85'}[21].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.39'}[22].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.66'}[23].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.01'}[24].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.35'}[25].
- Q92801615's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.46'}[26].
Body
Definition and Type
Q92801615's instance of is recorded as eruptive variable star[2].
Use and Application
Q92801615 is part of Pleiades[5].