Astronomy:HD 195019

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Short description: Binary star in the constellation Delphinus
HD 195019
Observation data
{{#ifeq:J2000|J2000.0 (ICRS)|Epoch J2000.0      Equinox J2000.0 (ICRS)| Epoch J2000      [[Astronomy:Equinox (celestial coordinates)|Equinox J2000}}
Constellation Delphinus[1]
A
Right ascension  20h 28m 18.6367s[2]
Declination +18° 46′ 10.180″[2]
Apparent magnitude (V) 6.97[3]
B
Right ascension  20h 28m 18.5185s[4]
Declination +18° 46′ 13.365″[4]
Apparent magnitude (V) 10.60[3]
Characteristics
Spectral type G1V[5] + K3:[6]
B−V color index 0.662±0.007[1]
Astrometry
Absolute magnitude (MV)+4.01[1]
A
Radial velocity (Rv)−91.290±0.0039[7] km/s
Proper motion (μ) RA: +349.620(16)[2] mas/yr
Dec.: −56.618(19)[2] mas/yr
Parallax (π)26.6465 ± 0.0225[2] mas
Distance122.4 ± 0.1 ly
(37.53 ± 0.03 pc)
B
Proper motion (μ) RA: +361.063(18) mas/yr
Dec.: −65.735(23) mas/yr
Parallax (π)26.6192 ± 0.0251[4] mas
Distance122.5 ± 0.1 ly
(37.57 ± 0.04 pc)
Details
HD 195019 A
Mass1.08±0.01[8] M
Radius1.47±0.04[8] R
Luminosity2.23±0.02[8] L
Surface gravity (log g)4.13±0.02[8] cgs
Temperature5,825±56[8] K
Metallicity [Fe/H]0.068±0.030[9] dex
Rotation25 days[10]
Rotational velocity (v sin i)2.47±0.50[9] km/s
Age7.7±0.7[8] Gyr
HD 195019 B
Mass0.7[11] M
Radius0.62[12] R
Luminosity0.10[12] L
Surface gravity (log g)4.46[13] cgs
Temperature4,652[13] K
Rotational velocity (v sin i)1.71[13] km/s
Other designations
BD+18°4505, HD 195019, HIP 100970, SAO 106138, WDS J20283+1846, LTT 15981, NLTT 49312, 2MASS J20281860+1846103[14]
Database references
SIMBADdata

HD 195019 is a binary star system in the northern constellation of Delphinus. The brighter star has a close orbiting exoplanet companion. This system is located at a distance of 122 light years from the Sun based on parallax measurements,[2] but it is drifting closer with a radial velocity of −91.3 km/s.[7] Although it has an absolute magnitude of 4.01,[1] at that distance the system is considered too faint to be viewed with the naked eye, having a combined apparent visual magnitude of 6.87.[1] However, it should be readily visible with a pair of binoculars or a small telescope.[15]

The spectrum of the primary member, designated component A, presents as a G-type main-sequence star with a stellar classification of G1V.[5] An older stellar classification of G3 V/IV[16] suggested it may be near the end of its main sequence lifespan and is evolving into a subgiant star.[15] This is an older star with an estimated age of nearly 8[8] billion years and a low level of magnetic activity in its chromosphere.[8] The abundance of iron is near solar.[9] The star has a mass similar to the Sun but a larger radius. It is radiating 2.23 times the luminosity of the Sun from its photosphere at an effective temperature of 5,825 K.[8]

The co-moving companion, component B, was first reported by G. W. Hough in 1881. As of 2016, it is located at an angular separation of 3.40 along a position angle of 334° relative to the primary.[3] This corresponds to a projected separation of 131 astronomical unit|AU. This is a K-type star with 70% of the mass of the Sun[11] and is magnitude 10.60.[3]

Planetary system

In 1998, a planet was discovered at Lick Observatory utilizing a radial velocity method, orbiting around Star HD 195019 A.[16] A search of astrometric observations from Hipparcos suggested this may be a stellar object in a near polar orbit.[17][18][15] However, interferometric observations ruled out a stellar companion in this orbit with high likelihood.[19]

The HD 195019 planetary system[9]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >3.69 ± 0.30 MJ 0.1388 ± 0.0080 18.20132 ± 0.00039 0.0138 ± 0.0044

See also

References

  1. 1.0 1.1 1.2 1.3 1.4 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode2012AstL...38..331A  XHIP record for this object at VizieR.
  2. 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. 3.0 3.1 3.2 3.3 Mason, Brian D. et al. (December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal 122 (6): 3466–3471. doi:10.1086/323920. ISSN 0004-6256. Bibcode2001AJ....122.3466M. 
  4. 4.0 4.1 4.2 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  5. 5.0 5.1 Gray, R. O. et al. (April 2001). "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars". The Astronomical Journal 121 (4): 2148–2158. doi:10.1086/319956. ISSN 0004-6256. Bibcode2001AJ....121.2148G. 
  6. Bidelman, W. P. (October 1985). "G. P. Kuiper's spectral classifications of proper-motion stars". Astrophysical Journal Supplement Series 59: 197–227. doi:10.1086/191069. Bibcode1985ApJS...59..197B. 
  7. 7.0 7.1 Soubiran, C. et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars". Astronomy and Astrophysics 616: A7. doi:10.1051/0004-6361/201832795. Bibcode2018A&A...616A...7S. 
  8. 8.0 8.1 8.2 8.3 8.4 8.5 8.6 8.7 8.8 Bonfanti, A. et al. (2016). "Age consistency between exoplanet hosts and field stars". Astronomy & Astrophysics 585: 14. doi:10.1051/0004-6361/201527297. A5. Bibcode2016A&A...585A...5B. 
  9. 9.0 9.1 9.2 9.3 Butler, R. P. et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. doi:10.1086/504701. Bibcode2006ApJ...646..505B. 
  10. Llorente De Andrés, F.; de la Reza, R.; Cruz, P.; Cuenda-Muñoz, D.; Alfaro, E. J.; Chavero, C.; Cifuentes, C. (2024). "The evolution of lithium in FGK dwarf stars. Influence of planets and Galactic migration". Astronomy and Astrophysics 684. doi:10.1051/0004-6361/202346744. Bibcode2024A&A...684A..28L. 
  11. 11.0 11.1 Quarles, Billy et al. (2020). "Orbital stability of circumstellar planets in binary systems". The Astronomical Journal 159 (3): 80. doi:10.3847/1538-3881/ab64fa. Bibcode2020AJ....159...80Q. 
  12. 12.0 12.1 Hardegree-Ullman, Kevin K.; Apai, Dániel; Bergsten, Galen J.; Pascucci, Ilaria; López-Morales, Mercedes (2023). "Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets". The Astronomical Journal 165 (6): 267. doi:10.3847/1538-3881/acd1ec. Bibcode2023AJ....165..267H. 
  13. 13.0 13.1 13.2 Rice, Malena; Brewer, John M. (August 2020). "Stellar Characterization of Keck HIRES Spectra with The Cannon". The Astrophysical Journal 898 (2): 119. doi:10.3847/1538-4357/ab9f96. 119. Bibcode2020ApJ...898..119R. 
  14. "HD 195019". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+195019. 
  15. 15.0 15.1 15.2 "HD 195019 Delphini". The Planet Project. http://stars.astro.illinois.edu/sow/hd195019.html. 
  16. 16.0 16.1 Fischer, Debra A. et al. (1999). "Planetary Companions around Two Solar-Type Stars: HD 195019 and HD 217107". Publications of the Astronomical Society of the Pacific 111 (755): 50–56. doi:10.1086/316304. Bibcode1999PASP..111...50F. 
  17. Han, Inwoo et al. (February 2001). "Preliminary Astrometric Masses for Proposed Extrasolar Planetary Companions". The Astrophysical Journal 548 (1): L57–L60. doi:10.1086/318927. Bibcode2001ApJ...548L..57H. 
  18. Sahlmann, J. et al. (April 2011). "HD 5388 b is a 69 MJup companion instead of a planet". Astronomy & Astrophysics 528: L8. doi:10.1051/0004-6361/201116533. L8. Bibcode2011A&A...528L...8S. 
  19. Koresko, C. D. et al. (December 2002). "Long baseline interferometric observations of HD 195019: no K dwarf companion detected". Bulletin of the American Astronomical Society 34: 1177. Bibcode2002AAS...201.4613K. 

Coordinates: Sky map 20h 28m 18.6363s, +18° 46′ 10.188″