HD 195019

HD 195019
Observation data
Epoch J2000      Equinox ICRS
Constellation Delphinus
A
Right ascension 20h 28m 18.6367s
Declination +18° 46′ 10.180″
Apparent magnitude (V) 6.97
B
Right ascension 20h 28m 18.5185s
Declination +18° 46′ 13.365″
Apparent magnitude (V) 10.60
Characteristics
Spectral type G1V + K3:
B−V color index 0.662±0.007
Astrometry
Absolute magnitude (MV)+4.01
A
Radial velocity (Rv)−91.290±0.0039 km/s
Proper motion (μ) RA: +349.620(16) mas/yr
Dec.: −56.618(19) mas/yr
Parallax (π)26.6465±0.0225 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 mas
Distance122.5 ± 0.1 ly
(37.57 ± 0.04 pc)
Details
HD 195019 A
Mass1.08±0.01 M☉
Radius1.47±0.04 R☉
Luminosity2.23±0.02 L☉
Surface gravity (log g)4.13±0.02 cgs
Temperature5,825±56 K
Metallicity [Fe/H]0.068±0.030 dex
Rotation25 days
Rotational velocity (v sin i)2.47±0.50 km/s
Age7.7±0.7 Gyr
HD 195019 B
Mass0.7 M☉
Radius0.62 R☉
Luminosity0.10 L☉
Surface gravity (log g)4.46 cgs
Temperature4,652 K
Rotational velocity (v sin i)1.71 km/s
Other designations
BD+18°4505, HD 195019, HIP 100970, SAO 106138, WDS J20283+1846, LTT 15981, NLTT 49312, GCRV 12790, 2MASS J20281860+1846103
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, but it is drifting closer with a radial velocity of −91.3 km/s. Although it has an absolute magnitude of 4.01, 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. However, it should be readily visible with a pair of binoculars or a small telescope.

The spectrum of the primary member, designated component A, presents as a G-type main-sequence star with a stellar classification of G1V. An older stellar classification of G3 V/IV suggested it may be near the end of its main sequence lifespan and is evolving into a subgiant star. This is an older star with an estimated age of nearly 8 billion years and a low level of magnetic activity in its chromosphere. The abundance of iron is near solar. 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.

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. This corresponds to a projected separation of 131 AU. This is a K-type star with 70% of the mass of the Sun and is magnitude 10.60.

Planetary system

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

The HD 195019 planetary system
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 2 3 4 5 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
  2. 1 2 3 4 5 6 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.
  3. 1 2 3 4 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. Bibcode:2001AJ....122.3466M. doi:10.1086/323920. ISSN 0004-6256. S2CID 119533755.
  4. 1 2 3 4 5 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.
  5. 1 2 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. Bibcode:2001AJ....121.2148G. doi:10.1086/319956. ISSN 0004-6256. S2CID 117076031.
  6. ↑ Bidelman, W. P. (October 1985). "G. P. Kuiper's spectral classifications of proper-motion stars". Astrophysical Journal Supplement Series. 59: 197–227. Bibcode:1985ApJS...59..197B. doi:10.1086/191069.
  7. 1 2 Soubiran, C.; et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars". Astronomy and Astrophysics. 616: A7. arXiv:1804.09370. Bibcode:2018A&A...616A...7S. doi:10.1051/0004-6361/201832795. S2CID 52952408.
  8. 1 2 3 4 5 6 7 8 9 Bonfanti, A.; et al. (2016). "Age consistency between exoplanet hosts and field stars". Astronomy & Astrophysics. 585: 14. arXiv:1511.01744. Bibcode:2016A&A...585A...5B. doi:10.1051/0004-6361/201527297. S2CID 53971692. A5.
  9. 1 2 3 4 Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701. S2CID 119067572.
  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. arXiv:2402.01315. Bibcode:2024A&A...684A..28L. doi:10.1051/0004-6361/202346744.
  11. 1 2 Quarles, Billy; et al. (2020). "Orbital stability of circumstellar planets in binary systems". The Astronomical Journal. 159 (3): 80. arXiv:1912.11019. Bibcode:2020AJ....159...80Q. doi:10.3847/1538-3881/ab64fa. S2CID 209444271.
  12. 1 2 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. arXiv:2304.12490. Bibcode:2023AJ....165..267H. doi:10.3847/1538-3881/acd1ec.
  13. 1 2 3 Rice, Malena; Brewer, John M. (August 2020). "Stellar Characterization of Keck HIRES Spectra with The Cannon". The Astrophysical Journal. 898 (2): 119. arXiv:2007.02942. Bibcode:2020ApJ...898..119R. doi:10.3847/1538-4357/ab9f96. 119.
  14. ↑ "HD 195019". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-01-03.
  15. 1 2 3 Kaler, James. "HD 195019 Delphini". The Planet Project. Retrieved 2024-01-03.
  16. 1 2 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. arXiv:astro-ph/9810420. Bibcode:1999PASP..111...50F. doi:10.1086/316304. S2CID 17980987.
  17. ↑ Han, Inwoo; et al. (February 2001). "Preliminary Astrometric Masses for Proposed Extrasolar Planetary Companions". The Astrophysical Journal. 548 (1): L57–L60. Bibcode:2001ApJ...548L..57H. doi:10.1086/318927. S2CID 120952927.
  18. ↑ Sahlmann, J.; et al. (April 2011). "HD 5388 b is a 69 MJup companion instead of a planet". Astronomy & Astrophysics. 528: L8. arXiv:1102.3372. Bibcode:2011A&A...528L...8S. doi:10.1051/0004-6361/201116533. S2CID 55566004. L8.
  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. Bibcode:2002AAS...201.4613K.