Astronomy:Delta Crateris

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Short description: K-type giant star in the constellation Crater
δ Crateris
Location of δ Crateris (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Crater
Right ascension  11h 19m 20.4473s[1]
Declination −14° 46′ 42.743″[1]
Apparent magnitude (V) 3.56[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type K0 III[2]
B−V color index 1.12[2]
Astrometry
Radial velocity (Rv)−4.94±0.21[4] km/s
Proper motion (μ) RA: −122.958[1] mas/yr
Dec.: +207.083[1] mas/yr
Parallax (π)17.017 ± 0.1617[1] mas
Distance192 ± 2 ly
(58.8 ± 0.6 pc)
Absolute magnitude (MV)−0.321[3]
Details[5]
Mass1.47 ± 0.2 M
Radius20.14±0.48 R
Luminosity154.8±4.9 L
Surface gravity (log g)2.00 ± 0.08 cgs
Temperature4,540 ± 40 K
Metallicity [Fe/H]−0.43±0.10 dex
Age2.89[6] Gyr
Other designations
δ Crt, 12 Crateris, BD−13°3345, FK5 426, HD 98430, HIP 55282, HR 4382, SAO 156605.[7]
Database references
SIMBADdata

Delta Crateris (δ Crt, δ Crateris) is a solitary[8] star in the southern constellation of Crater. With an apparent visual magnitude of 3.56,[2] it is the brightest star[9] in this rather dim constellation. It has an annual parallax shift of 17.017 mas as measured from Earth,[1] indicating Delta Crateris lies at a distance of 192 ly from the Sun.

Characteristics

This is an evolved orange-hued giant star belonging to the spectral class K0 III. Delta Crateris is a member of the so-called red clump, indicating that it is generating energy through the thermonuclear fusion of helium at its core.[3] The star has an estimated 1.47 times the mass of the Sun but has expanded to 20 times the Sun's radius.[5]

It is around 2.89[6] billion years old with a rotation rate that is too small to measure; the projected rotational velocity is 0.0 km/s.[4] Delta Crateris is radiating 171.4±9.0 as much luminosity as the Sun[6] from its outer envelope at an effective temperature of 4,540 K.[5]

This star is occasionally called by the name Labrum, usually in an astrological context.[10]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. 2.0 2.1 2.2 2.3 Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics 352: 495–507, Bibcode1999A&A...352..495M. 
  3. 3.0 3.1 3.2 Soubiran, C. et al. (2008), "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants", Astronomy and Astrophysics 480 (1): 91–101, doi:10.1051/0004-6361:20078788, Bibcode2008A&A...480...91S. 
  4. 4.0 4.1 Massarotti, Alessandro et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal 135 (1): 209–231, doi:10.1088/0004-6256/135/1/209, Bibcode2008AJ....135..209M. 
  5. 5.0 5.1 5.2 Reffert, Sabine; Bergmann, Christoph; Quirrenbach, Andreas; Trifonov, Trifon; Künstler, Andreas (2015-02-01). "Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity". Astronomy and Astrophysics 574: A116. doi:10.1051/0004-6361/201322360. ISSN 0004-6361. Bibcode2015A&A...574A.116R. 
  6. 6.0 6.1 6.2 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal 150 (3): 88, doi:10.1088/0004-6256/150/3/88, Bibcode2015AJ....150...88L. 
  7. "del Crt". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=del+Crt. 
  8. Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode2008MNRAS.389..869E. 
  9. Ridpath, Ian (2012), A Dictionary of Astronomy, OUP Oxford, p. 108, ISBN 978-0199609055, https://books.google.com/books?id=O31j9UJ3U4oC&pg=PA108. 
  10. Robson, Vivian E. (1923). The Fixed Stars And Constellations In Astrology. p. 110. https://archive.org/details/in.ernet.dli.2015.128091/page/n103/mode/2up.