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Delta Crateris

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.

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
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]
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

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. ^ a b c d e 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.
  2. ^ a b c d e f g Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics, 352: 495–507, Bibcode:1999A&A...352..495M.
  3. ^ a b c 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. ^ 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.
  5. ^ 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.
  6. ^ a b c d e f 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.
  7. ^ a b c 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.
  8. ^ "del Crt". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-03-02.{{cite web}}: CS1 maint: postscript (link)
  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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  10. ^ Ridpath, Ian (2012), A Dictionary of Astronomy, OUP Oxford, p. 108, ISBN 978-0199609055.

External links

  • Kaler, James B., "Delta Crateris", Stars, University of Illinois

delta, crateris, crateris, traditional, name, labrum, solitary, star, southern, constellation, crater, with, apparent, visual, magnitude, brightest, star, this, rather, constellation, annual, parallax, shift, measured, from, earth, indicating, lies, distance, . Delta Crateris d Crt d 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 d CraterisLocation of d Crateris circled Observation dataEpoch J2000 0 Equinox J2000 0 ICRS Constellation CraterRight ascension 11h 19m 20 44756s 1 Declination 14 46 42 7413 1 Apparent magnitude V 3 56 2 CharacteristicsSpectral type K0 III 2 B V color index 1 12 2 AstrometryRadial velocity Rv 4 94 0 21 3 km sProper motion m RA 124 67 1 mas yr Dec 207 59 1 mas yrParallax p 20 0507 0 5308 mas 4 Distance163 4 ly 50 1 pc Absolute magnitude MV 0 321 5 DetailsMass1 56 6 M Radius22 44 0 28 7 R Luminosity171 4 9 0 7 L Surface gravity log g 2 59 2 cgsTemperature4 510 15 6 KMetallicity Fe H 0 48 2 dexRotational velocity v sin i 0 0 3 km sAge2 89 6 GyrOther designationsd Crt 12 Crateris BD 13 3345 FK5 426 HD 98430 HIP 55282 HR 4382 SAO 156605 8 Database referencesSIMBADdataThis 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 Edit a b c d e van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 a b c d e f g Mallik Sushma V December 1999 Lithium abundance and mass Astronomy and Astrophysics 352 495 507 Bibcode 1999A amp A 352 495M a b c 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 Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR 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 amp A 480 91S doi 10 1051 0004 6361 20078788 S2CID 16602121 a b c d e f 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 a b c Berio P et al November 2011 Chromosphere of K giant stars Geometrical extent and spatial structure detection Astronomy amp Astrophysics 535 A59 arXiv 1109 5476 Bibcode 2011A amp A 535A 59B doi 10 1051 0004 6361 201117479 S2CID 17171848 del Crt SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2017 03 02 a href Template Cite web html title Template Cite web cite web a 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 EditKaler James B Delta Crateris Stars University of Illinois Retrieved from https en wikipedia org w index php title Delta Crateris amp oldid 1141268717, wikipedia, wiki, book, books, library,

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