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24 Cancri

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Triple star system in the constellation Cancer
24 Cancri
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
24 Cnc A
Right ascension 08 26 39.791
Declination +24° 32′ 03.02″
Apparent magnitude (V) 6.89
24 Cnc BC
Right ascension 08 26 40.068
Declination +24° 32′ 05.33″
Apparent magnitude (V) 7.47
Characteristics
Spectral type F0V / F7V
U−B color index +0.06
B−V color index +0.30
Astrometry
Radial velocity (Rv)15.4±3.0 km/s
24 Cnc A
Proper motion (μ) RA: −43.008 mas/yr
Dec.: −78.521 mas/yr
Parallax (π)14.4288 ± 0.0238 mas
Distance226.0 ± 0.4 ly
(69.3 ± 0.1 pc)
Orbit
Period (P)21.78±0.20 yr
Semi-major axis (a)0.149±0.001″
Eccentricity (e)0.079±0.009
Inclination (i)19.1±1.0°
Longitude of the node (Ω)153.6±5.0°
Periastron epoch (T)B 1998.42±0.30
Argument of periastron (ω)
(secondary)
51.0±10.0°
Details
24 Cnc A
Mass1.5 M
Radius1.6 R
Luminosity6.3 L
Surface gravity (log g)4.17 cgs
Temperature7,331 K
Metallicity −0.49 dex
Age770 Myr
Other designations
24 Cnc, BD+25°1920, HIP 41389, ADS 6811 AB, CCDM J08267+2432AB
24 Cnc A: HD 71152, HR 3312, SAO 80184
24 Cnc B: HD 71153, HR 3313, SAO 80185
Database references
SIMBAD24 Cnc
24 Cnc A
24 Cnc B

24 Cancri (abbreviated to 24 Cnc) is a triple star system in the constellation Cancer. The system is located about 226 light-years (69 parsecs) away, based on its parallax. The system has a combined apparent magnitude of 6.5, and the two components A and B are separated by 5.7.

The primary component in the star system is designated 24 Cancri A. It is a F-type main sequence star.

The secondary component, designated 24 Cancri B, is also a F-type main-sequence star and is itself a binary with an orbital period of about 22 years. The stars are identical, with apparent magnitudes of 8.6 and masses of 1.1 M, and they are separated by 0.15″.

References

  1. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27 – L30. Bibcode:2000A&A...355L..27H.
  3. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  4. Abt, H. A. (1981). "Visual multiples. VII - MK classifications". The Astrophysical Journal Supplement Series. 45: 437. Bibcode:1981ApJS...45..437A. doi:10.1086/190719.
  5. ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
  6. Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  7. ^ Docobo, J. A.; Ling, J. F. (2009). "Binary Stars with Components of Solar Type: 25 Orbits and System Masses". The Astronomical Journal. 138 (4): 1159. Bibcode:2009AJ....138.1159D. doi:10.1088/0004-6256/138/4/1159.
  8. EAS (1997). "The HIPPARCOS and TYCHO catalogues". Astrometric and Photometric Star Catalogues Derived from the ESA Hipparcos Space Astrometry Mission. ESA SP Series. 1200. Noordwijk, Netherlands: ESA Publications Division. Bibcode:1997ESASP1200.....E. ISBN 9290923997.
  9. ^ Tokovinin, Andrei (2018-03-01). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series. 235 (1): 6. arXiv:1712.04750. Bibcode:2018ApJS..235....6T. doi:10.3847/1538-4365/aaa1a5. ISSN 0067-0049. S2CID 119047709.
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