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HD 133981

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Star in the constellation Apus
HD 133981
Observation data
Epoch J2000      Equinox J2000
Constellation Apus
Right ascension 15 12 33.97907
Declination −72° 46′ 14.1634″
Apparent magnitude (V) 6.02±0.01
Characteristics
Spectral type B8 IV
U−B color index −0.24
B−V color index 0.00
Astrometry
Radial velocity (Rv)−13.7±1.3 km/s
Proper motion (μ) RA: −14.107 mas/yr
Dec.: −16.361 mas/yr
Parallax (π)3.8088 ± 0.0418 mas
Distance856 ± 9 ly
(263 ± 3 pc)
Absolute magnitude (MV)−1.34
Details
Mass3.72
−0.05 M
Radius6.35 R
Luminosity364
−14 L
Surface gravity (log g)3.48 cgs
Temperature10,250 K
Metallicity 0.00 dex
Age202
−2 Myr
Other designations
25 G. Apodis[11], CD−72°1096, CPD−72°1714, GC 20391, HD 133981, HIP 74421, HR 5628, SAO 257247
Database references
SIMBADdata

HD 133981, also known as HR 5628, is a solitary, bluish-white hued star located in the southern circumpolar constellation of Apus. It has an apparent magnitude of 6.02, allowing it to be faintly visible to the naked eye in ideal conditions. The object is located relatively far at a distance of 856 light years based on parallax measurements from Gaia DR3 but is approaching the Solar System with a heliocentric radial velocity of −13.7 km/s.

HD 133981 has a stellar classification of B8 IV, indicating that it is a B-type star that is evolving towards the red giant branch. Houk and Cowley (1975) gave a slightly more evolved class of B8/9 III, instead indicating that it is a giant star. Some evolutionary models show that it is a star just reaching the end of the main sequence. Nevertheless, it has 3.72 times the mass of the Sun and 6.35 times its girth. It radiates 364 times the luminosity of the Sun from its photosphere at an effective temperature of 10,250 K. HD 133981 is said to be 202 million years old.

HD 133981 lies in front of the distant faint galaxy LEDA 54288. A debris disk has been detected around the star. It has 22.5 times the mass of the Earth and an equilibrium temperature of 27 K.

The HD 133981 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
circumstellar disc 1,851 AU

References

  1. ^ 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. ^ 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. ^ Abt, Helmut A.; Morrell, Nidia I. (July 1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182. ISSN 0067-0049.
  4. ^ 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.
  5. ^ 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. eISSN 1562-6873. 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. eISSN 1562-6873. ISSN 1063-7737. S2CID 119257644.
  7. ^ 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. eISSN 1538-3881.
  8. Anders, F.; et al. (February 2022). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G = 18.5". Astronomy & Astrophysics. 658: A91. arXiv:2111.01860. Bibcode:2022A&A...658A..91A. doi:10.1051/0004-6361/202142369. eISSN 1432-0746. ISSN 0004-6361.
  9. ^ Liu, Qiong; Wang, Tinggui; Jiang, Peng (23 May 2014). "Bright Debris Disk Candidates Detected with the AKARI/Far-infrared Surveyor". The Astronomical Journal. 148 (1): 3. arXiv:1308.5593. Bibcode:2014AJ....148....3L. doi:10.1088/0004-6256/148/1/3. eISSN 1538-3881. ISSN 0004-6256.
  10. Gontcharov, G. A. (December 2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. ISSN 0320-0108. S2CID 118345778.
  11. 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.
  12. "HD 133981". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved October 9, 2022.
  13. 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.
  14. "LEDA 54288". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2022-09-01.
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