HD 177565

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HD 177565
Corona Australis constellation map.svg
Red circle.svg
Location of HD 177565 (circled)
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Corona Australis
Right ascension 19h 06m 52.46439s [1]
Declination −37° 48′ 38.3734″ [1]
Apparent magnitude  (V)6.16 [2]
Characteristics
Spectral type G6 V [3]
U−B color index +0.27 [4]
B−V color index +0.70 [4]
Astrometry
Radial velocity (Rv)60.9±0.8 [5] km/s
Proper motion (μ)RA: −187.700 mas/yr [1]
Dec.: −367.009 mas/yr [1]
Parallax (π)58.9860±0.0376  mas [1]
Distance 55.29 ± 0.04  ly
(16.95 ± 0.01  pc)
Absolute magnitude  (MV)+5.00 [6]
Details
Mass 0.99+0.03
−0.04 [7]   M☉
Radius 0.985±0.022 [8]   R☉
Luminosity 0.851±0.005 [1]   L☉
Surface gravity (log g)4.44±0.03 [9]   cgs
Temperature 5,627±19 [10]   K
Metallicity [Fe/H]0.08±0.01 [10]   dex
Rotational velocity (v sin i)3 [11]  km/s
Age 4.58±1.51 [12]   Gyr
Other designations
42 G. Coronae Australis [13] , CD−37°13049, CPD−37°8466, GC 26283, GJ 744, HD 177565, HIP 93858, HR 7232, SAO 210937, LTT 7569 [14]
Database references
SIMBAD data

HD 177565 (HR 7232; LTT 7569; Gliese 744) is a yellow-hued star located in the southern constellation Corona Australis. It has an apparent magnitude of 6.16, [2] placing it near the limit for naked eye visibility, even under ideal conditions. The object is located relatively close at a distance of 55.3 light-years based on Gaia DR3 parallax measurements, [1] but it is receding rapidly with a heliocentric radial velocity of 60.9  km/s . [5] At its current distance, HD 177565's brightness is diminished by interstellar extinction of 0.07 magnitudes [15] and it as an absolute magnitude of +5.00. [6] A 2017 multiplicity survey failed to detect any stellar companions around the star. [16]

HD 177565 has a stellar classification of G6 V, [3] indicating that it is an ordinary G-type main-sequence star like the Sun. The object has also be given a later class of G8 V (Houk 1982) [17] and one source lists it as a G5 subgiant. [18] It has 99% the mass of the Sun [7] and 98.5% the Sun's radius. [8] It radiates 85.1% the luminosity of the Sun [1] from its photosphere at an effective temperature of 5,627  K , [10] making it slightly cooler than the Sun. HD 177565 is slightly metal enriched with an iron abundance at [Fe/H] = +0.08 (120% solar) [10] and it is estimated to be 4.58 billion years old. [12] HD 177565 spins slightly faster than the Sun with a projected rotational velocity of 3  km/s [11] compared to the Sun's rotational velocity of 2 km/s.

Planetary system

In 2017, an exoplanet was discovered orbiting the star after observations of HARPS data. HD 177565 b is a hot Neptune that takes 44.5 days to revolve around its host star in a relatively circular orbit. [19]

The HD 177565 planetary system [19]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b ≥15.10+6.40
−6.05  M🜨 		0.246±0.01944.5+0.6
−0.3		0.059+0.172
−0.058		—~4.1 [20]   R🜨
Size comparison of the planet HD 177565 b (artistic concept) with Earth and Neptune HD 177565 b.jpg
Size comparison of the planet HD 177565 b (artistic concept) with Earth and Neptune

References

  1. 1 2 3 4 5 6 7 8 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.
  2. 1 2 Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
  3. 1 2 Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (2 June 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 . eISSN   1538-3881. ISSN   0004-6256. S2CID   250741593.
  4. 1 2 Cousins, A. W. J. (January 1973). "UBV Photometry of Some Southern Stars (Second List)". Monthly Notes of the Astronomical Society of South Africa. 32: 11. Bibcode:1973MNSSA..32...11C. ISSN   0024-8266.
  5. 1 2 Valenti, Jeff A.; Fischer, Debra A. (July 2005). "Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs". The Astrophysical Journal Supplement Series. 159 (1): 141–166. Bibcode:2005ApJS..159..141V. doi: 10.1086/430500 . eISSN   1538-4365. ISSN   0067-0049. S2CID   121398064.
  6. 1 2 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. eISSN   1562-6873. ISSN   1063-7737. S2CID   119257644.
  7. 1 2 Ramírez, I.; Fish, J. R.; Lambert, D. L.; Allende Prieto, C. (13 August 2012). "Lithium Abundances in nearby FGK Dwarf and Subgiant Stars: Internal Destruction, Galactic Chemical Evolution, and Exoplanets". The Astrophysical Journal. 756 (1): 46. arXiv: 1207.0499 . Bibcode:2012ApJ...756...46R. doi: 10.1088/0004-637X/756/1/46 . eISSN   1538-4357. ISSN   0004-637X. S2CID   119199829.
  8. 1 2 Masana, E.; Jordi, C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746. arXiv: astro-ph/0601049 . Bibcode:2006A&A...450..735M. doi: 10.1051/0004-6361:20054021 . eISSN   1432-0746. ISSN   0004-6361.
  9. ↑ Aguilera-Gómez, Claudia; Ramírez, Iván; Chanamé, Julio (June 2018). "Lithium abundance patterns of late-F stars: an in-depth analysis of the lithium desert". Astronomy & Astrophysics. 614: A55. arXiv: 1803.05922 . Bibcode:2018A&A...614A..55A. doi: 10.1051/0004-6361/201732209 . eISSN   1432-0746. ISSN   0004-6361. S2CID   62799777.
  10. 1 2 3 4 Sousa, S. G.; Santos, N. C.; Mayor, M.; Udry, S.; Casagrande, L.; Israelian, G.; Pepe, F.; Queloz, D.; Monteiro, M. J. P. F. G. (4 June 2008). "Spectroscopic parameters for 451 stars in the HARPS GTO planet search program". Astronomy & Astrophysics. 487 (1): 373–381. arXiv: 0805.4826 . Bibcode:2008A&A...487..373S. doi: 10.1051/0004-6361:200809698 . eISSN   1432-0746. ISSN   0004-6361. S2CID   18173201.
  11. 1 2 Nordström, B.; Mayor, M.; Andersen, J.; Holmberg, J.; Pont, F.; Jørgensen, B. R.; Olsen, E. H.; Udry, S.; Mowlavi, N. (16 April 2004). "The Geneva-Copenhagen survey of the Solar neighbourhood". Astronomy & Astrophysics. 418 (3): 989–1019. arXiv: astro-ph/0405198 . Bibcode:2004A&A...418..989N. doi: 10.1051/0004-6361:20035959 . eISSN   1432-0746. ISSN   0004-6361. S2CID   11027621.
  12. 1 2 Gomes da Silva, J.; Santos, N. C.; Adibekyan, V.; Sousa, S. G.; Campante, T. L.; Figueira, P.; Bossini, D.; Delgado-Mena, E.; Monteiro, M. J. P. F. G.; de Laverny, P.; Recio-Blanco, A.; Lovis, C. (February 2021). "Stellar chromospheric activity of 1674 FGK stars from the AMBRE-HARPS sample. I. A catalogue of homogeneous chromospheric activity". Astronomy & Astrophysics. 646: A77. arXiv: 2012.10199 . Bibcode:2021A&A...646A..77G. doi: 10.1051/0004-6361/202039765 . eISSN   1432-0746. ISSN   0004-6361. S2CID   229331727.
  13. ↑ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode:1879RNAO....1.....G.
  14. ↑ "HD 177565". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved June 7, 2023.
  15. ↑ Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017). "Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars". Monthly Notices of the Royal Astronomical Society. 472 (4): 3805–3820. arXiv: 1709.01160 . Bibcode:2017MNRAS.472.3805G. doi: 10.1093/mnras/stx2219 . eISSN   1365-2966. ISSN   0035-8711. S2CID   118879856.
  16. ↑ Fuhrmann, K.; Chini, R.; Kaderhandt, L.; Chen, Z. (February 14, 2017). "Multiplicity among Solar-type Stars". The Astrophysical Journal. 836 (1). American Astronomical Society: 139. Bibcode:2017ApJ...836..139F. doi: 10.3847/1538-4357/836/1/139 . ISSN   1538-4357. S2CID   125253901.
  17. ↑ Houk, N. (1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Declinations −40° to −26°. Vol. 3. Bibcode:1982mcts.book.....H.
  18. ↑ Evans, D. S.; Menzies, A.; Stoy, R. H. (1 December 1959). "Fundamental Data for Southern Stars (Second List)". Monthly Notices of the Royal Astronomical Society. 119 (6): 638–647. Bibcode:1959MNRAS.119..638E. doi: 10.1093/mnras/119.6.638 . eISSN   1365-2966. ISSN   0035-8711.
  19. 1 2 Feng, F.; Tuomi, M.; Jones, H. R. A. (May 16, 2017). "Agatha: disentangling periodic signals from correlated noise in a periodogram framework". Monthly Notices of the Royal Astronomical Society. 470 (4). Oxford University Press (OUP): 4794–4814. arXiv: 1705.03089 . Bibcode:2017MNRAS.470.4794F. doi: 10.1093/mnras/stx1126 . ISSN   0035-8711. S2CID   73635720.
  20. ↑ Foster, G.; Poppenhaeger, K.; Ilic, N.; Schwope, A. (2022). "Exoplanet X-ray irradiation and evaporation rates with eROSITA". Astronomy & Astrophysics. 661. EDP Sciences: A23. arXiv: 2106.14550 . Bibcode:2022A&A...661A..23F. doi: 10.1051/0004-6361/202141097 . ISSN   0004-6361.
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