From Wikipedia, the free encyclopedia
17 Delphini
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Delphinus
Right ascension 20h 55m 36.689s [1]
Declination +13° 43′ 17.531″ [1]
Apparent magnitude (V) 5.18 [2](5.16-5.27) [3]
Characteristics
Spectral type K0 III [4]
U−B color index +0.95 [5]
B−V color index +1.13 [5]
Variable type suspected [3]
Astrometry
Radial velocity (Rv)−10.2±0.9 [6] km/s
Proper motion (μ) RA: +16.457  mas/ yr [1]
Dec.: −11.468  mas/ yr [1]
Parallax (π)6.3132 ± 0.0699  mas [1]
Distance517 ± 6  ly
(158 ± 2  pc)
Absolute magnitude (MV)−0.64 [7]
Details [8]
Mass2.33  M
Radius23.36  R
Luminosity219  L
Surface gravity (log g)2.07  cgs
Temperature4,616  K
Metallicity [Fe/H]−0.19 [9]  dex
Rotational velocity (v sin i)3±1 [10] km/s
Age832  Myr
Other designations
17 Del, AG+13°2209, BD+13°4572, FK5 3669, GC 29201, HD 199253, HIP 103294, HR 8011, SAO 106665
Database references
SIMBAD data

17 Delphini is a solitary [11] star in the equatorial constellation Delphinus. It has an absolute magnitude of −0.64 [7] and apparent magnitude of 5.18, [2] allowing it to be faintly seen with the naked eye. Located 517 light years away, [1] it is approaching the Solar System with a heliocentric radial velocity of −10.2  km/s. [6]

17 Delphini is an orange giant that is most likely on the horizontal branch (84% probability). [8] At present it has 2.33 times the mass of the Sun, but at an age of 832 million years — has expanded to 23.36 times the radius of the Sun. [8] It shines at 219  solar luminosities from its enlarged photosphere at an effective temperature of 4,616 K, [8] giving it an orange glow. 17 Del has an iron abundance 64% that of the Sun [9] and spins modestly with a projected rotational velocity of km/s. [10]

17 Del is suspected to be a variable star of unknown type ranging from 5.16 to 5.27. [3]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H. ISSN  0004-6361.
  3. ^ a b c Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. ISSN  1063-7729. S2CID  255195566.
  4. ^ Griffin, R. F.; Redman, R. O. (1 April 1960). "Photoelectric Measurements of the 4200 A CN Band and the G Band in G8-K5 Spectra". Monthly Notices of the Royal Astronomical Society. 120 (4): 287–316. Bibcode: 1960MNRAS.120..287G. doi: 10.1093/mnras/120.4.287.
  5. ^ a b Gutierrez-Moreno, A. (1966). "A system of photometric standards". Publications of the Department of Astronomy University of Chile. 1: 1. Bibcode: 1966PDAUC...1....1G.
  6. ^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication: 0. Bibcode: 1953GCRV..C......0W.
  7. ^ a b Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. ISSN  1063-7737. S2CID  119257644.
  8. ^ a b c d Stock, Stephan; Reffert, Sabine; Quirrenbach, Andreas (August 2018). "Precise radial velocities of giant stars: X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search". Astronomy & Astrophysics. 616: A33. arXiv: 1805.04094. Bibcode: 2018A&A...616A..33S. doi: 10.1051/0004-6361/201833111. ISSN  0004-6361.
  9. ^ a b Hekker, S.; Meléndez, J. (December 2007). "Precise radial velocities of giant stars: III. Spectroscopic stellar parameters". Astronomy & Astrophysics. 475 (3): 1003–1009. arXiv: 0709.1145. Bibcode: 2007A&A...475.1003H. doi: 10.1051/0004-6361:20078233. ISSN  0004-6361.
  10. ^ a b de Medeiros, J. R.; Mayor, M. (November 1999). "A catalog of rotational and radial velocities for evolved stars". Astronomy and Astrophysics Supplement Series. 139 (3): 433–460. Bibcode: 1999A&AS..139..433D. doi: 10.1051/aas:1999401. ISSN  0365-0138.
  11. ^ 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.
From Wikipedia, the free encyclopedia
17 Delphini
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Delphinus
Right ascension 20h 55m 36.689s [1]
Declination +13° 43′ 17.531″ [1]
Apparent magnitude (V) 5.18 [2](5.16-5.27) [3]
Characteristics
Spectral type K0 III [4]
U−B color index +0.95 [5]
B−V color index +1.13 [5]
Variable type suspected [3]
Astrometry
Radial velocity (Rv)−10.2±0.9 [6] km/s
Proper motion (μ) RA: +16.457  mas/ yr [1]
Dec.: −11.468  mas/ yr [1]
Parallax (π)6.3132 ± 0.0699  mas [1]
Distance517 ± 6  ly
(158 ± 2  pc)
Absolute magnitude (MV)−0.64 [7]
Details [8]
Mass2.33  M
Radius23.36  R
Luminosity219  L
Surface gravity (log g)2.07  cgs
Temperature4,616  K
Metallicity [Fe/H]−0.19 [9]  dex
Rotational velocity (v sin i)3±1 [10] km/s
Age832  Myr
Other designations
17 Del, AG+13°2209, BD+13°4572, FK5 3669, GC 29201, HD 199253, HIP 103294, HR 8011, SAO 106665
Database references
SIMBAD data

17 Delphini is a solitary [11] star in the equatorial constellation Delphinus. It has an absolute magnitude of −0.64 [7] and apparent magnitude of 5.18, [2] allowing it to be faintly seen with the naked eye. Located 517 light years away, [1] it is approaching the Solar System with a heliocentric radial velocity of −10.2  km/s. [6]

17 Delphini is an orange giant that is most likely on the horizontal branch (84% probability). [8] At present it has 2.33 times the mass of the Sun, but at an age of 832 million years — has expanded to 23.36 times the radius of the Sun. [8] It shines at 219  solar luminosities from its enlarged photosphere at an effective temperature of 4,616 K, [8] giving it an orange glow. 17 Del has an iron abundance 64% that of the Sun [9] and spins modestly with a projected rotational velocity of km/s. [10]

17 Del is suspected to be a variable star of unknown type ranging from 5.16 to 5.27. [3]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H. ISSN  0004-6361.
  3. ^ a b c Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. ISSN  1063-7729. S2CID  255195566.
  4. ^ Griffin, R. F.; Redman, R. O. (1 April 1960). "Photoelectric Measurements of the 4200 A CN Band and the G Band in G8-K5 Spectra". Monthly Notices of the Royal Astronomical Society. 120 (4): 287–316. Bibcode: 1960MNRAS.120..287G. doi: 10.1093/mnras/120.4.287.
  5. ^ a b Gutierrez-Moreno, A. (1966). "A system of photometric standards". Publications of the Department of Astronomy University of Chile. 1: 1. Bibcode: 1966PDAUC...1....1G.
  6. ^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication: 0. Bibcode: 1953GCRV..C......0W.
  7. ^ a b Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. ISSN  1063-7737. S2CID  119257644.
  8. ^ a b c d Stock, Stephan; Reffert, Sabine; Quirrenbach, Andreas (August 2018). "Precise radial velocities of giant stars: X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search". Astronomy & Astrophysics. 616: A33. arXiv: 1805.04094. Bibcode: 2018A&A...616A..33S. doi: 10.1051/0004-6361/201833111. ISSN  0004-6361.
  9. ^ a b Hekker, S.; Meléndez, J. (December 2007). "Precise radial velocities of giant stars: III. Spectroscopic stellar parameters". Astronomy & Astrophysics. 475 (3): 1003–1009. arXiv: 0709.1145. Bibcode: 2007A&A...475.1003H. doi: 10.1051/0004-6361:20078233. ISSN  0004-6361.
  10. ^ a b de Medeiros, J. R.; Mayor, M. (November 1999). "A catalog of rotational and radial velocities for evolved stars". Astronomy and Astrophysics Supplement Series. 139 (3): 433–460. Bibcode: 1999A&AS..139..433D. doi: 10.1051/aas:1999401. ISSN  0365-0138.
  11. ^ 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.

Videos

Youtube | Vimeo | Bing

Websites

Google | Yahoo | Bing

Encyclopedia

Google | Yahoo | Bing

Facebook