Astronomy:Delta Crateris

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Short description: K-type giant star in the constellation Crater
δ Crateris
Crater constellation map.svg
Red circle.svg
Location of δ Crateris (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Crater
Right ascension  11h 19m 20.44756s[1]
Declination −14° 46′ 42.7413″[1]
Apparent magnitude (V) 3.56[2]
Characteristics
Spectral type K0 III[2]
B−V color index 1.12[2]
Astrometry
Radial velocity (Rv)−4.94±0.21[3] km/s
Proper motion (μ) RA: −124.67[1] mas/yr
Dec.: +207.59[1] mas/yr
Parallax (π)20.0507 ± 0.5308[4] mas
Distance163 ± 4 ly
(50 ± 1 pc)
Absolute magnitude (MV)−0.321[5]
Details
Mass1.56[6] M
Radius22.44±0.28[7] R
Luminosity171.4±9.0[7] L
Surface gravity (log g)2.59[2] cgs
Temperature4,510±15[6] K
Metallicity [Fe/H]−0.48[2] dex
Rotational velocity (v sin i)0.0[3] km/s
Age2.89[6] Gyr
Other designations
δ Crt, 12 Crateris, BD−13° 3345, FK5 426, HD 98430, HIP 55282, HR 4382, SAO 156605.[8]
Database references
SIMBADdata

Delta Crateris (δ Crt, δ Crateris; traditional name: Labrum) is a solitary[9] star in the southern constellation of Crater. With an apparent visual magnitude of 3.56,[2] it is the brightest star[10] in this rather dim constellation. It has an annual parallax shift of 17.56[1] mas as measured from Earth, indicating Delta Crateris lies at a distance of 163 ± 4 light years from the Sun.

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.[5] The star has an estimated 1.56[6] times the mass of the Sun but has expanded to 22.44±0.28[7] times the Sun's radius.

The metallicity of the star – what astronomers term the abundance of elements other than hydrogen and helium – is only 33% that of the Sun.[2] 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.[3] Delta Crateris is radiating 171.4±9.0 as much luminosity as the Sun from its outer envelope at an effective temperature of 4,510±15 K.[6]

References

  1. 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode2007A&A...474..653V. 
  2. 2.0 2.1 2.2 2.3 2.4 2.5 2.6 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 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. 
  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. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  5. 5.0 5.1 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. 
  6. 6.0 6.1 6.2 6.3 6.4 6.5 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. 7.0 7.1 7.2 Berio, P. et al. (November 2011), "Chromosphere of K giant stars. Geometrical extent and spatial structure detection", Astronomy & Astrophysics 535: A59, doi:10.1051/0004-6361/201117479, Bibcode2011A&A...535A..59B. 
  8. "del Crt". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=del+Crt. 
  9. 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. 
  10. Ridpath, Ian (2012), A Dictionary of Astronomy, OUP Oxford, p. 108, ISBN 978-0199609055, https://books.google.com/books?id=O31j9UJ3U4oC&pg=PA108. 

External links