Astronomy:38 Cancri
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Cancer |
| Right ascension | 08h 39m 42.65445s[2] |
| Declination | +19° 46′ 42.4386″[2] |
| Apparent magnitude (V) | 6.65[3] |
| Characteristics | |
| Evolutionary stage | subgiant |
| Spectral type | F0 IV[4] |
| B−V color index | 0.248±0.010[3] |
| Variable type | δ Sct[5] |
| Astrometry | |
| Radial velocity (Rv) | +32.0±2.0[6] km/s |
| Proper motion (μ) | RA: −36.879[2] mas/yr Dec.: −13.103[2] mas/yr |
| Parallax (π) | 5.3700 ± 0.0705[2] mas |
| Distance | 607 ± 8 ly (186 ± 2 pc) |
| Absolute magnitude (MV) | 0.36[3] |
| Details | |
| Mass | 1.786[7] M☉ |
| Radius | 1.834[7] R☉ |
| Luminosity | 59.31[3] L☉ |
| Surface gravity (log g) | 2.92±0.20[8] cgs |
| Temperature | 7300±200[8] K |
| Metallicity [Fe/H] | −0.16±0.10[8] dex |
| Rotation | 0.670 d[7] |
| Rotational velocity (v sin i) | 138.5[7] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
38 Cancri is a variable star in the zodiac constellation Cancer, located around 607 light years from the Sun. This object has the variable star designation BT Cancri; 38 Cancri is the Flamsteed designation. It is a member of the Praesepe cluster[10] but is a challenge to view with the naked eye, having an apparent visual magnitude of 6.65.[3] The star is moving closer to the Earth with a heliocentric radial velocity of +32 km/s.[6]
This is an evolving subgiant star with a stellar classification of F0 IV.[4] It was found to be a pulsating variable by Michel Breger in 1970[11] and is classed as a Delta Scuti variable. The star displays a pattern of variation showing up to 22 different frequencies, with three being dominant.[12] The brightness varies by up to 0.07 in magnitude.[5] The star has a magnetic field with a computed longitudinal field strength of −215±149 G.[8] It has 1.8[7] times the mass of the Sun and 1.8[7] times the Sun's radius. The star is radiating 59[3] times the Sun's luminosity from its photosphere at an effective temperature of around 7,300 K.[8]
References
- ↑ Gupta, S. K. (September 1979). "Light Variation of the Delta Scuti Star 38 CNC". Bulletin of the Astronomical Society of India 7: 72–77. Bibcode: 1979BASI....7...72G. https://ui.adsabs.harvard.edu/abs/1979BASI....7...72G. Retrieved 11 November 2021.
- ↑ 2.0 2.1 2.2 2.3 2.4 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 4.0 4.1 Gray, R. O. et al. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal 121 (4): 2148–2158, doi:10.1086/319956, Bibcode: 2001AJ....121.2148G.
- ↑ 5.0 5.1 Samus, N. N. et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1 61 (1): 80–88, doi:10.1134/S1063772917010085, Bibcode: 2017ARep...61...80S.
- ↑ 6.0 6.1 de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics 546: 14, doi:10.1051/0004-6361/201219219, A61, Bibcode: 2012A&A...546A..61D.
- ↑ 7.0 7.1 7.2 7.3 7.4 7.5 van Saders, Jennifer L.; Pinsonneault, Marc H. (October 2013), "Fast Star, Slow Star; Old Star, Young Star: Subgiant Rotation as a Population and Stellar Physics Diagnostic", The Astrophysical Journal 776 (2): 20, doi:10.1088/0004-637X/776/2/67, 67, Bibcode: 2013ApJ...776...67V.
- ↑ 8.0 8.1 8.2 8.3 8.4 Fossati, L. et al. (December 2007), "Late stages of the evolution of A-type stars on the main sequence: comparison between observed chemical abundances and diffusion models for 8 Am stars of the Praesepe cluster", Astronomy and Astrophysics 476 (2): 911–925, doi:10.1051/0004-6361:20078320, Bibcode: 2007A&A...476..911F.
- ↑ "38 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=38+Cnc.
- ↑ Michel, E. et al. (February 1999), "Seismology of delta Scuti stars in the Praesepe cluster. I. Ranges of unstable modes as predicted by linear analysis versus observations", Astronomy and Astrophysics 342: 153–166, Bibcode: 1999A&A...342..153M.
- ↑ Breger, Michel (November 1970), "Metallic-Line a Stars and Pulsation", Astrophysical Journal 162: 597, doi:10.1086/150691, Bibcode: 1970ApJ...162..597B
- ↑ Breger, M. et al. (February 2012), "Delta Scuti stars in the Praesepe cluster observed by the MOST satellite", Astronomische Nachrichten 333 (2): 131, doi:10.1002/asna.201111640, Bibcode: 2012AN....333..131B.
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