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1 Planetary system  





2 References  














HD 164604






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Coordinates: Sky map18h03m06.95s, 28° 33 38.3
 

From Wikipedia, the free encyclopedia
 


HD 164604 / Pincoya
Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 18h03m 06.93314s[1]
Declination –28° 33′ 38.3576″[1]
Apparent magnitude (V) 9.62[2]
Characteristics
Spectral type K3.5V(k)[3]
Apparent magnitude (B) 11.016[2]
Apparent magnitude (J) 7.784±0.024[2]
Apparent magnitude (H) 7.306±0.038[2]
Apparent magnitude (K) 7.169±0.020[2]
B−V color index 1.396±0.491[2]
Astrometry
Radial velocity (Rv)7.30±0.16[4] km/s
Proper motion (μ) RA: −34.658±0.036[4] mas/yr
Dec.: −42.253±0.025[4] mas/yr
Parallax (π)24.9867 ± 0.0351 mas[4]
Distance130.5 ± 0.2 ly
(40.02 ± 0.06 pc)
Absolute magnitude (MV)6.57[2]
Details
Mass0.77±0.04[5] M
Radius0.77+0.01
−0.04
[1] R
Luminosity0.258±0.001[1] L
Surface gravity (log g)4.41[3] cgs
Temperature4,684+135
−37
[5] K
Metallicity [Fe/H]0.09±0.08[2] dex
Age7.24±4.72[6] Gyr
Other designations

CD–28° 14058, HD 164604, HIP 88414, SAO 186165, PPM 267742[7]

Database references
SIMBADdata
Exoplanet Archivedata

HD 164604 is a single star in the southern constellationofSagittarius constellation. It has the proper name Pincoya, as selected in the NameExoWorlds campaign by Chile, during the 100th anniversary of the IAU. Pincoya is a female water spirit from southern Chilean mythology who is said to bring drowned sailors to the Caleuche so that they can live in the afterlife.[8][9] A 2015 survey ruled out the existence of any additional stellar companions at projected distances from 13 to 340 astronomical units.[10] It is known to host a single super-Jupiter exoplanet.[11]

This star is invisible to the naked eye with an apparent visual magnitude of 9.62.[2] It is located at a distance of 128.5 light years from the Sun based on parallax,[1] and is drifting further away with a radial velocity of +6 km/s.[12] The stellar classification of HD 164604 is K3.5V(k), which indicates this is a K-type main-sequence star. The chromosphere is considered very inactive.[3] It is roughly seven[6] billion years old with 77% of the mass[5] and radius[1] of the Sun. The star is radiating 26%[1] of the luminosity of the Sun from its photosphere at an effective temperature of 4,684 K.[5]

Planetary system

[edit]

A single super-Jupiter exoplanet was detected by the Magellan Planet Search Program in 2010 based on radial velocity variations of the host star.[11] The orbit of this body does not preclude a hypothetical Earth-mass exoplanet from occupying a dynamically stable orbit within the habitable zone of this star.[13]Anastrometric measurement of the planet's inclination and true mass was published in 2022 as part of Gaia DR3.[14]

The HD 164604 planetary system[5][14]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b / Caleuche 14.3±5.5 MJ 1.331 ± 0.0029 641.47 ± 10.13 0.35 ± 0.1 29±19°

References

[edit]
  1. ^ a b c d e f g 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 sourceatVizieR.
  • ^ a b c d e f g h i 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. S2CID 119257644.
  • ^ a b c Gray, R. O.; et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. Bibcode:2006AJ....132..161G. doi:10.1086/504637. S2CID 119476992.
  • ^ a b c d 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 sourceatVizieR.
  • ^ a b c d e Feng, Fabo; et al. (June 2019). "Search for Nearby Earth Analogs. I. 15 Planet Candidates Found in PFS Data". The Astrophysical Journal Supplement Series. 242 (2): 31. arXiv:1904.08567. Bibcode:2019ApJS..242...25F. doi:10.3847/1538-4365/ab1b16. S2CID 121128472. 25.
  • ^ a b Pace, G. (March 2013), "Chromospheric activity as age indicator. An L-shaped chromospheric-activity versus age diagram", Astronomy & Astrophysics, 551: 4, arXiv:1301.5651, Bibcode:2013A&A...551L...8P, doi:10.1051/0004-6361/201220364, S2CID 56420519, L8.
  • ^ "HD 164604". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 5 February 2018.
  • ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
  • ^ "Name Exo Worlds". www.iau.org. International Astronomical Union | IAU. Retrieved 2020-01-02.
  • ^ Mugrauer, M.; Ginski, C. (12 May 2015). "High-contrast imaging search for stellar and substellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society. 450 (3): 3127–3136. Bibcode:2015MNRAS.450.3127M. doi:10.1093/mnras/stv771. hdl:1887/49340. Retrieved 19 June 2020.
  • ^ a b Arriagada, Pamela; et al. (2010). "Five Long-period Extrasolar Planets in Eccentric orbits from the Magellan Planet Search Program". The Astrophysical Journal. 711 (2): 1229–35. arXiv:1001.4093. Bibcode:2010ApJ...711.1229A. doi:10.1088/0004-637X/711/2/1229. S2CID 118682009.
  • ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  • ^ Agnew, Matthew T.; et al. (November 2017). "Stable habitable zones of single Jovian planet systems". Monthly Notices of the Royal Astronomical Society. 471 (4): 4494–4507. arXiv:1706.05805. Bibcode:2017MNRAS.471.4494A. doi:10.1093/mnras/stx1449.
  • ^ a b Gaia Collaboration; et al. (2023). "Gaia Data Release 3". Astronomy & Astrophysics. 674: A34. arXiv:2206.05595. doi:10.1051/0004-6361/202243782. S2CID 249626026.


  • Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_164604&oldid=1235165168"

    Categories: 
    K-type main-sequence stars
    Planetary systems with one confirmed planet
    Sagittarius (constellation)
    Durchmusterung objects
    Henry Draper Catalogue objects
    Hipparcos objects
    Hidden categories: 
    Articles with short description
    Short description matches Wikidata
     



    This page was last edited on 18 July 2024, at 00:10 (UTC).

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