Astronomy:HD 161988
Observation data Epoch J2000.0 Equinox (celestial coordinates) | |
---|---|
Constellation | Apus |
Right ascension | 17h 57m 41.686s[1] |
Declination | −76° 10′ 40.62″[1] |
Apparent magnitude (V) | 6.07±0.01[2] |
Characteristics | |
Evolutionary stage | red giant branch[3] |
Spectral type | K2 III[4] |
U−B color index | +1.28[5] |
B−V color index | +1.20[5] |
Astrometry | |
Radial velocity (Rv) | +36.8±0.4[6] km/s |
Proper motion (μ) | RA: +2.464[1] mas/yr Dec.: −1.867[1] mas/yr |
Parallax (π) | 5.2546 ± 0.022[1] mas |
Distance | 621 ± 3 ly (190.3 ± 0.8 pc) |
Absolute magnitude (MV) | −0.26[7] |
Details | |
Mass | 3.05[8] M☉ |
Radius | 20.8[9] R☉ |
Luminosity | 185[10] L☉ |
Surface gravity (log g) | 2.04±0.02[3] cgs |
Temperature | 4,498[10] K |
Metallicity [Fe/H] | −0.13[11] dex |
Rotational velocity (v sin i) | 2.1±1.3[12] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 161988, also known as HR 6635, is a solitary, orange hued star located in the southern circumpolar constellation Apus. It has an apparent magnitude of 6.07,[2] allowing it to be faintly visible to the naked eye. Parallax measurements place it at a distance of 621 light years,[1] and it is currently receding with a heliocentric radial velocity of 36.8 km/s.[6]
The object has a stellar classification of K2 III,[4] indicating that it is a red giant. Gaia Data Release 3 models place it on the red giant branch. At present it has 3.05 times the mass of the Sun[8] and an enlarged radius of 20.8 R☉.[9] It shines at 185 times the luminosity of the Sun from its photosphere at an effective temperature of 4,498 K.[10] HD 161988 has an iron abundance 74% that of the Sun,[11] making it slightly metal deficient. Like most giants, it spins modestly with a projected rotational velocity of 2.1 km/s.[12]
HD 161988 has a 14th magnitude optical companion located 26.4 arcseconds away along a position angle of 122°.[14]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 2.0 2.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H.
- ↑ 3.0 3.1 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.
- ↑ 4.0 4.1 Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations −90° to −53°. Bibcode: 1975mcts.book.....H.
- ↑ 5.0 5.1 Johnson, H. L. et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory 4 (99): 99. Bibcode: 1966CoLPL...4...99J.
- ↑ 6.0 6.1 Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G.
- ↑ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A.
- ↑ 8.0 8.1 Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics 657: A7. doi:10.1051/0004-6361/202142146. ISSN 0004-6361. Bibcode: 2022A&A...657A...7K.
- ↑ 9.0 9.1 Stassun, Keivan G. et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S.
- ↑ 10.0 10.1 10.2 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (21 November 2012). "Fundamental parameters and infrared excesses of Hipparcos stars: Parameters and IR excesses from Hipparcos". Monthly Notices of the Royal Astronomical Society 427 (1): 343–357. doi:10.1111/j.1365-2966.2012.21873.x. ISSN 0035-8711. Bibcode: 2012MNRAS.427..343M.
- ↑ 11.0 11.1 Anders, F. et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics 628: A94. doi:10.1051/0004-6361/201935765. ISSN 0004-6361. Bibcode: 2019A&A...628A..94A.
- ↑ 12.0 12.1 De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics 561: A126. doi:10.1051/0004-6361/201220762. ISSN 0004-6361. Bibcode: 2014A&A...561A.126D.
- ↑ "HR 6635". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HR+6635.
- ↑ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (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. Bibcode: 2001AJ....122.3466M.
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is not used in prior text.External links
Original source: https://en.wikipedia.org/wiki/HD 161988.
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