Cannabaceae

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HD 193556
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Delphinus
Right ascension 20h 20m 20.5234s[1]
Declination +14° 34′ 09.3206″[1]
Apparent magnitude (V) 6.17±0.01[2]
Characteristics
Spectral type G8 III[3]
U−B color index +0.67[4]
B−V color index +0.92[4]
Astrometry
Radial velocity (Rv)11.7±0.3[5] km/s
Proper motion (μ) RA: −3.887 mas/yr[1]
Dec.: +5.610 mas/yr[1]
Parallax (π)6.9878 ± 0.0252 mas[1]
Distance467 ± 2 ly
(143.1 ± 0.5 pc)
Absolute magnitude (MV)+0.04[6]
Details
Mass2.65[7] M☉
Radius11.33[8] R☉
Luminosity102[9] L☉
Surface gravity (log g)2.76[10] cgs
Temperature5,104[10] K
Metallicity [Fe/H]+0.03[10] dex
Rotational velocity (v sin i)1.5±1.2[11] km/s
Age490[7] Myr
Other designations
AG+14°2187, BD+14°4263, FK5 3629, GC 28288, HD 193556, HIP 100274, HR 7778, SAO 105988[12]
Database references
SIMBADdata

HD 193556 (HR 7778) is a solitary star in the equatorial constellation Delphinus. It has an apparent magnitude of 6.17,[2] making it visible to the naked eye under ideal conditions. Parallax measurements place the object at a distance of 467 light years[1] and it is currently receding with a heliocentric radial velocity of 11.7 km/s.[5]

HD 193556 has a stellar classification of G8 III,[3] indicating that it is a red giant. It has 2.65 times the mass of the Sun and is currently 490 million years old,[7] having expanded to 11.33 times the radius of the Sun.[8] It shines with a luminosity of 102 L☉[9] from its enlarged photosphere at an effective temperature of 5,104 K,[10] giving it a yellow glow. HD 193556 has an iron abundance around solar level[10] and spins leisurely with a poorly constrained projected rotational velocity of 1.5 km/s.[11]

References[edit]

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
  3. ^ a b Harlan, E. A. (September 1969). "MK classifications for F and G-type stars. I." The Astronomical Journal. 74: 916. Bibcode:1969AJ.....74..916H. doi:10.1086/110881. ISSN 0004-6256.
  4. ^ a b Fernie, J. D. (May 1983). "New UBVRI photometry for 900 supergiants". The Astrophysical Journal Supplement Series. 52: 7. Bibcode:1983ApJS...52....7F. doi:10.1086/190856. eISSN 1538-4365. ISSN 0067-0049.
  5. ^ a b 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. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. ISSN 1063-7737. S2CID 119231169.
  6. ^ 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. ISSN 1063-7737. S2CID 255204555.
  7. ^ a b c Dotter, Aaron; Chaboyer, Brian; Jevremović, Darko; Kostov, Veselin; Baron, E.; Ferguson, Jason W. (September 2008). "The Dartmouth Stellar Evolution Database". The Astrophysical Journal Supplement Series. 178 (1): 89–101. arXiv:0804.4473. Bibcode:2008ApJS..178...89D. doi:10.1086/589654. eISSN 1538-4365. ISSN 0067-0049.
  8. ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256.
  9. ^ a b Luck, R. Earle (25 August 2015). "Abundances in the Local Region. I. G and K Giants". The Astronomical Journal. 150 (3): 88. arXiv:1507.01466. Bibcode:2015AJ....150...88L. doi:10.1088/0004-6256/150/3/88. eISSN 1538-3881. ISSN 0004-6256. S2CID 118505114.
  10. ^ a b c d e Liu, Y. J.; Tan, K. F.; Wang, L.; Zhao, G.; Sato, Bun'ei; Takeda, Y.; Li, H. N. (31 March 2014). "The Lithium Abundances of a Large Sample of Red Giants". The Astrophysical Journal. 785 (2): 94. arXiv:1404.1687. Bibcode:2014ApJ...785...94L. doi:10.1088/0004-637X/785/2/94. eISSN 1538-4357. ISSN 0004-637X.
  11. ^ a b de Medeiros, J. R.; Mayor, M. (November 1999). "A catalog of rotational and radial velocities for evolved stars". Astronomy and Astrophysics Supplement Series. 139 (3): 433–460. Bibcode:1999A&AS..139..433D. doi:10.1051/aas:1999401. ISSN 0365-0138.
  12. ^ "HD 193556". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 20, 2022.
source: https://en.wikipedia.org/wiki/HD_193556

One thought on “Cannabaceae”

  1. Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
    View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction

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