Chi Ceti

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Chi Ceti

A light curve for EZ Ceti, plotted from TESS data[1]
Observation data
ICRS
)
Constellation Cetus
HD 11171
Right ascension 01h 49m 35.10316s[2]
Declination −10° 41′ 11.0674″[2]
Apparent magnitude (V) 4.66[3]
HD 11131
Right ascension 01h 49m 23.35579s[2]
Declination −10° 42′ 12.8594″[2]
Apparent magnitude (V) 6.75[3]
Characteristics
HD 11171
Spectral type F3 III[4] or F0 V[5]
U−B color index +0.04[3]
B−V color index +0.33[3]
HD 11131
Spectral type G3 V[5]
U−B color index +0.12[3]
B−V color index +0.61[3]
Variable type BY Dra[6]
Distance
74 ± 5 ly
(23 ± 2 pc)
Absolute magnitude (MV)4.98[9]
Details
HD 11171
Rotational velocity (v sin i)
3.34[11] km/s
HR 531, SAO 148036.[12]
χ Ceti B: EZ Cet, HD 11131, BD−11°351, HIP 8486, SAO 148033.[13]
Database references
SIMBADχ Ceti
χ Ceti A
χ Ceti B

Chi Ceti (χ Ceti), is the

mass.[2]

The primary, component A, is an

F-type main sequence star. It displays an infrared excess at a wavelength of 70 μm and thus is a candidate host of an orbiting debris disk.[15]

The common proper motion companion, component B, is a

References

  1. ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  2. ^
    S2CID 18759600
    .
  3. ^ .
  4. ^ , 88.
  5. ^ .
  6. ^ .
  7. ^ .
  8. , A61.
  9. .
  10. ^ , A124.
  11. .
  12. ^ "chi Cet". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-02-12.{{cite web}}: CS1 maint: postscript (link)
  13. ^ V* EZ Cet.
  14. .
  15. .

External links