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δ Crateris
Location of δ Crateris (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Crater
Right ascension 11h 19m 20.4473s [1]
Declination −14° 46′ 42.7434″
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: −122.958 [1]  mas/ yr
Dec.: +207.083 [1]  mas/ yr
Parallax (π)17.017 ± 0.1617  mas [1]
Distance192 ± 2  ly
(58.8 ± 0.6  pc) [1]
Absolute magnitude (MV)−0.321 [4]
Details [5]
Mass1.468±0.165  M
Radius16.2±0.6  R
Luminosity171.4±9.0 [6]  L
Surface gravity (log g)2.46±0.09  cgs
Temperature4,605±33  K
Metallicity [Fe/H]−0.04±0.02  dex
Age2.424±0.879  Gyr
Other designations
δ Crt, 12 Crateris, BD−13° 3345, FK5 426, HD 98430, HIP 55282, HR 4382, SAO 156605. [7]
Database references
SIMBAD data

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. [4] The star has an estimated 1.47 times the mass of the Sun but has expanded to 16.2 times the Sun's radius. [5]

The metallicity of the star – what astronomers term the abundance of elements other than hydrogen and helium – is only 40% that of the Sun. [5] [a] It is around 2.89 [10] 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 [10] from its outer envelope at an effective temperature of 4,605 K. [5]

Notes

  1. ^ The abundance is estimated by taking [Fe/H] to the power of ten:
              10[Fe/H] = 10-0.4 = 0.4

References

  1. ^ a b c d e f 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. ^ a b c d Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics, 352: 495–507, Bibcode: 1999A&A...352..495M.
  3. ^ a b 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, Bibcode: 2008AJ....135..209M, doi: 10.1088/0004-6256/135/1/209, S2CID  121883397.
  4. ^ a b 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, arXiv: 0712.1370, Bibcode: 2008A&A...480...91S, doi: 10.1051/0004-6361:20078788, S2CID  16602121.
  5. ^ a b c d Gomes da Silva, J.; Santos, N. C.; Adibekyan, V.; Sousa, S. G.; Campante, T. L.; Figueira, P.; Bossini, D.; Delgado-Mena, E.; Monteiro, M. J. P. F. G.; de Laverny, P.; Recio-Blanco, A.; Lovis, C. (2021-02-01). "Stellar chromospheric activity of 1674 FGK stars from the AMBRE-HARPS sample. I. A catalogue of homogeneous chromospheric activity". Astronomy and Astrophysics. 646: A77. arXiv: 2012.10199. doi: 10.1051/0004-6361/202039765. ISSN  0004-6361. Delta Crateris' database entry at VizieR.
  6. ^ Berio, P.; et al. (November 2011), "Chromosphere of K giant stars. Geometrical extent and spatial structure detection", Astronomy & Astrophysics, 535: A59, arXiv: 1109.5476, Bibcode: 2011A&A...535A..59B, doi: 10.1051/0004-6361/201117479, S2CID  17171848.
  7. ^ "del Crt". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-03-02.{{ cite web}}: CS1 maint: postscript ( link)
  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, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID  14878976.
  9. ^ Ridpath, Ian (2012), A Dictionary of Astronomy, OUP Oxford, p. 108, ISBN  978-0199609055.
  10. ^ a b Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3), 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID  118505114.

External links