Q88207802
eclipsing binary star
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Q88207802
Summary
Q88207802 is an eclipsing binary star[1].
Key Facts
- Q88207802's instance of is recorded as eclipsing binary star[2].
- Q88207802's instance of is recorded as eclipsing binary candidate[3].
- Q88207802's instance of is recorded as near-infrared source[4].
- Q88207802's instance of is recorded as astrophysical X-ray source[5].
- Q88207802's constellation is recorded as Leo Minor[6].
- Q88207802's spectral class is recorded as F7V[7].
- Q88207802's catalog code is recorded as UCAC2 43789664[8].
- Q88207802's catalog code is recorded as SBC9 1993[9].
- Q88207802's catalog code is recorded as GSC 02505-00412[10].
- Q88207802's catalog code is recorded as RX J094947.8+342733[11].
- Q88207802's catalog code is recorded as 2MASS J09494831+3427154[12].
- Q88207802's catalog code is recorded as CRTS J094948.3+342715[13].
- Q88207802's catalog code is recorded as Gaia DR2 796029174219793536[14].
- Q88207802's catalog code is recorded as RT LMi[15].
- Q88207802's catalog code is recorded as TYC 2505-412-1[16].
- Q88207802's catalog code is recorded as TIC 4892291[17].
- Q88207802's catalog code is recorded as Gaia DR3 796029174219793536[18].
- Q88207802's type of variable star is recorded as W Ursae Majoris variable[19].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.35'}[20].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.11'}[21].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.433'}[22].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.382'}[23].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.44999'}[24].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.084'}[25].
- Q88207802's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.781'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], eclipsing binary candidate[3], near-infrared source[4], and astrophysical X-ray source[5].