astro.wikisort.org - StarDelta 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.
Star in the constellation Crater
δ Crateris
Location of δ Crateris (circled) |
Observation data Epoch J2000.0 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 |
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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 mas[4] |
Distance | 163 ± 4 ly (50 ± 1 pc) |
Absolute magnitude (MV) | −0.321[5] |
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Details |
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Mass | 1.56[6] M☉ |
Radius | 22.44±0.28[7] R☉ |
Luminosity | 171.4±9.0[7] L☉ |
Surface gravity (log g) | 2.59[2] cgs |
Temperature | 4,510±15[6] K |
Metallicity [Fe/H] | −0.48[2] dex |
Rotational velocity (v sin i) | 0.0[3] km/s |
Age | 2.89[6] Gyr |
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Other designations |
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Database references |
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SIMBAD | data |
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
- van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
- Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics, 352: 495–507, Bibcode:1999A&A...352..495M.
- 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.
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- 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.
- 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.
- 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.
- "del Crt". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-03-02.
{{cite web}}
: CS1 maint: postscript (link) - 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.
- Ridpath, Ian (2012), A Dictionary of Astronomy, OUP Oxford, p. 108, ISBN 978-0199609055.
External links
Constellation of Crater |
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На других языках
[de] Delta Crateris
Delta Crateris (δ Crt, δ Crateris) ist ein Stern des Sternbilds Becher. Delta Crateris ist ein Riesenstern von oranger Farbe, sein Radius beträgt (22.44 ± 0.28) Sonnenradien. Seine Spektralklasse ist K0 und seine scheinbare Helligkeit beträgt 3.56 Magnituden; damit ist er der scheinbar hellste Stern des Sternbilds.
- [en] Delta Crateris
[es] Labrum
Labrum es el nombre tradicional de la estrella δ Crateris (δ Crt / 12 Crt), la más brillante de la constelación de Crater, la copa, con magnitud aparente +3,56. Su nombre proviene del latín y se refiere al Santo Grial, cáliz utilizado por Jesús y los Apóstoles en la Última Cena, también utilizado por José de Arimatea para recoger la sangre de Jesucristo en la Cruz.[1]
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