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10 Trianguli
Location of 10 Trianguli (circled)
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Triangulum
Right ascension 02h 18m 56.99355s [1]
Declination +28° 38′ 33.6322″ [1]
Apparent magnitude (V) 5.29±0.01 [2]
Characteristics
Evolutionary stage main sequence star [3]
Spectral type A2 V [4] [5]
U−B color index +0.02 [6]
B−V color index +0.04 [6]
Astrometry
Radial velocity (Rv)0.4±0.1 [7] km/s
Proper motion (μ) RA: +7.073  mas/ yr [1]
Dec.: +0.836  mas/ yr [1]
Parallax (π)8.9971 ± 0.0729  mas [1]
Distance363 ± 3  ly
(111.1 ± 0.9  pc)
Absolute magnitude (MV)−0.02 [8]
Details
Mass2.83±0.05 [3]  M☉
Radius3.71±0.19 [9]  R☉
Luminosity108+10
−9 [3]  L☉
Surface gravity (log g)3.73 [10]  cgs
Temperature9,023 [11]  K
Metallicity [Fe/H]+0.33 [12]  dex
Rotational velocity (v sin i)22±2 [13] km/s
Age372±44 [14] [15]  Myr
Other designations
1 H. Trianguli Minus, [16] 10 Tri, AG+28° 262, BD+27°360, GC 2781, HD 14252, HIP 10793, HR 675, SAO 75276
Database references
SIMBAD data

10 Trianguli (HD 14252; HR 675; 1 H. Trianguli Minus), or simply 10 Tri is a solitary star [17] located in the northern constellation Triangulum. It is faintly visible to the naked eye as a white-hued point of light with an apparent magnitude of 5.29. [2] Gaia DR3 parallax measurements imply a distance of 363 light-years [1] and it is slowly receding with a heliocentric radial velocity of 0.4  km/s. [7] At its current distance, 10 Tri's brightness is diminished by an interstellar extinction of 0.11 magnitudes [18] and it has an absolute magnitude of −0.02. [8]

10 Trianguli has a stellar classification of A2 V, [4] [5] indicating that it is an ordinary A-type main-sequence star that is generating energy via hydrogen fusion at its core. It has 2.83 times the mass of the Sun [3] and a slightly enlarged radius 3.71 times that of the Sun. [9] It radiates 108 times the luminosity of the Sun [3] from its photosphere at an effective temperature of 9,023  K. [11] 10 Trianguli is rather evolved for its class, having completed 92.5% of its main sequence lifetime [3] at the age of 372 million years. [14] [15] It is metal enriched with an iron abundance of [Fe/H] = +0.33 or % of the Sun's [12] and unlike most hot stars, it spins modestly with a projected rotational velocity of 22  km/s. [13]

10 Trianguli has a 13th magnitude companion located 58.3" away along a position angle of 205°. [19] It is an unrelated background star that is much more distant than 10 Trianguli. [20] Together with ι Trianguli and 12 Trianguli, it forms part of the obsolete Triangulum Minus.

References

  1. ^ a b c d e 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. ^ 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. S2CID  17128864.
  3. ^ a b c d e f Zorec, J.; Royer, F. (January 2012). "Rotational velocities of A-type stars IV: Evolution of rotational velocities". Astronomy & Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. eISSN  1432-0746. ISSN  0004-6361. S2CID  55586789.
  4. ^ a b Osawa, Kiyoteru (July 1959). "Spectral Classification of 533 B8-A2 Stars and the Mean Absolute Magnitude of A0 V Stars". The Astrophysical Journal. 130. American Astronomical Society: 159. Bibcode: 1959ApJ...130..159O. doi: 10.1086/146706. ISSN  0004-637X. S2CID  120004061.
  5. ^ a b Cowley, A.; Cowley, C.; Jaschek, M.; Jaschek, C. (April 1969). "A study of the bright stars. I. A catalogue of spectral classifications". The Astronomical Journal. 74: 375. Bibcode: 1969AJ.....74..375C. doi: 10.1086/110819. ISSN  0004-6256. S2CID  121555804.
  6. ^ a b Osawa, K.; Hata, S. (1960). "Three colour photometry of B8-A2 stars". Annals of the Tokyo Astronomical Observatory. 6: 148. Bibcode: 1960AnTok...6..148O.
  7. ^ 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. eISSN  1562-6873. ISSN  1063-7737. S2CID  119231169.
  8. ^ a b 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.
  9. ^ a b Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (April 8, 2004). "The angular sizes of dwarf stars and subgiants: Surface brightness relations calibrated by interferometry". Astronomy & Astrophysics. 426 (1): 297–307. arXiv: astro-ph/0404180. Bibcode: 2004A&A...426..297K. doi: 10.1051/0004-6361:20035930. eISSN  1432-0746. ISSN  0004-6361. S2CID  6077801.
  10. ^ Philip, A. G. D.; Egret, D. (May 1980). "An analysis of the Hauck-Mermillod catalogue of homogeneous four-color data. II". Astronomy and Astrophysics Supplement Series. 40: 199–205. Bibcode: 1980A&AS...40..199P. ISSN  0365-0138.
  11. ^ a b Takeda, Yoichi; Han, Inwoo; Kang, Dong-Il; Lee, Byeong-Cheol; Kim, Kang-Min (May 1, 2019). "Compositional differences between the component stars of eclipsing close binary systems showing chemical peculiarities". Monthly Notices of the Royal Astronomical Society. 485 (1): 1067–1084. arXiv: 1902.04766. Bibcode: 2019MNRAS.485.1067T. doi: 10.1093/mnras/stz449. ISSN  0035-8711. S2CID  119421663.
  12. ^ a b Gebran, M.; Farah, W.; Paletou, F.; Monier, R.; Watson, V. (18 April 2016). "A new method for the inversion of atmospheric parameters of A/Am stars". Astronomy & Astrophysics. 589: A83. arXiv: 1603.01146. Bibcode: 2016A&A...589A..83G. doi: 10.1051/0004-6361/201528052. eISSN  1432-0746. ISSN  0004-6361. S2CID  118549566.
  13. ^ a b Royer, F.; Grenier, S.; Baylac, M.-O.; Gómez, A. E.; Zorec, J. (October 2002). "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i". Astronomy & Astrophysics. 393 (3): 897–911. arXiv: astro-ph/0205255. Bibcode: 2002A&A...393..897R. doi: 10.1051/0004-6361:20020943. eISSN  1432-0746. ISSN  0004-6361.
  14. ^ a b Gontcharov, G. A. (November 2012). "Spatial distribution and kinematics of OB stars". Astronomy Letters. 38 (11): 694–706. arXiv: 1606.09028. Bibcode: 2012AstL...38..694G. doi: 10.1134/S1063773712110035. eISSN  1562-6873. ISSN  1063-7737. S2CID  255202762.
  15. ^ a b 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. eISSN  1562-6873. ISSN  1063-7737. S2CID  118345778.
  16. ^ Verbunt, F.; van Gent, R. H. (June 2010). "The star catalogue of Hevelius: Machine-readable version and comparison with the modern Hipparcos Catalogue". Astronomy and Astrophysics. 516: A29. Bibcode: 2010A&A...516A..29V. doi: 10.1051/0004-6361/201014003. eISSN  1432-0746. ISSN  0004-6361. S2CID  54171435.
  17. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. S2CID  14878976.
  18. ^ 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.
  19. ^ 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. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. ISSN  0004-6256. S2CID  119533755.
  20. ^ 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.
Retrieved from " https://en.wikipedia.org/?title=10_Trianguli&oldid=1189379391"
From Wikipedia, the free encyclopedia
10 Trianguli
Location of 10 Trianguli (circled)
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Triangulum
Right ascension 02h 18m 56.99355s [1]
Declination +28° 38′ 33.6322″ [1]
Apparent magnitude (V) 5.29±0.01 [2]
Characteristics
Evolutionary stage main sequence star [3]
Spectral type A2 V [4] [5]
U−B color index +0.02 [6]
B−V color index +0.04 [6]
Astrometry
Radial velocity (Rv)0.4±0.1 [7] km/s
Proper motion (μ) RA: +7.073  mas/ yr [1]
Dec.: +0.836  mas/ yr [1]
Parallax (π)8.9971 ± 0.0729  mas [1]
Distance363 ± 3  ly
(111.1 ± 0.9  pc)
Absolute magnitude (MV)−0.02 [8]
Details
Mass2.83±0.05 [3]  M☉
Radius3.71±0.19 [9]  R☉
Luminosity108+10
−9 [3]  L☉
Surface gravity (log g)3.73 [10]  cgs
Temperature9,023 [11]  K
Metallicity [Fe/H]+0.33 [12]  dex
Rotational velocity (v sin i)22±2 [13] km/s
Age372±44 [14] [15]  Myr
Other designations
1 H. Trianguli Minus, [16] 10 Tri, AG+28° 262, BD+27°360, GC 2781, HD 14252, HIP 10793, HR 675, SAO 75276
Database references
SIMBAD data

10 Trianguli (HD 14252; HR 675; 1 H. Trianguli Minus), or simply 10 Tri is a solitary star [17] located in the northern constellation Triangulum. It is faintly visible to the naked eye as a white-hued point of light with an apparent magnitude of 5.29. [2] Gaia DR3 parallax measurements imply a distance of 363 light-years [1] and it is slowly receding with a heliocentric radial velocity of 0.4  km/s. [7] At its current distance, 10 Tri's brightness is diminished by an interstellar extinction of 0.11 magnitudes [18] and it has an absolute magnitude of −0.02. [8]

10 Trianguli has a stellar classification of A2 V, [4] [5] indicating that it is an ordinary A-type main-sequence star that is generating energy via hydrogen fusion at its core. It has 2.83 times the mass of the Sun [3] and a slightly enlarged radius 3.71 times that of the Sun. [9] It radiates 108 times the luminosity of the Sun [3] from its photosphere at an effective temperature of 9,023  K. [11] 10 Trianguli is rather evolved for its class, having completed 92.5% of its main sequence lifetime [3] at the age of 372 million years. [14] [15] It is metal enriched with an iron abundance of [Fe/H] = +0.33 or % of the Sun's [12] and unlike most hot stars, it spins modestly with a projected rotational velocity of 22  km/s. [13]

10 Trianguli has a 13th magnitude companion located 58.3" away along a position angle of 205°. [19] It is an unrelated background star that is much more distant than 10 Trianguli. [20] Together with ι Trianguli and 12 Trianguli, it forms part of the obsolete Triangulum Minus.

References

  1. ^ a b c d e 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. ^ 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. S2CID  17128864.
  3. ^ a b c d e f Zorec, J.; Royer, F. (January 2012). "Rotational velocities of A-type stars IV: Evolution of rotational velocities". Astronomy & Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. eISSN  1432-0746. ISSN  0004-6361. S2CID  55586789.
  4. ^ a b Osawa, Kiyoteru (July 1959). "Spectral Classification of 533 B8-A2 Stars and the Mean Absolute Magnitude of A0 V Stars". The Astrophysical Journal. 130. American Astronomical Society: 159. Bibcode: 1959ApJ...130..159O. doi: 10.1086/146706. ISSN  0004-637X. S2CID  120004061.
  5. ^ a b Cowley, A.; Cowley, C.; Jaschek, M.; Jaschek, C. (April 1969). "A study of the bright stars. I. A catalogue of spectral classifications". The Astronomical Journal. 74: 375. Bibcode: 1969AJ.....74..375C. doi: 10.1086/110819. ISSN  0004-6256. S2CID  121555804.
  6. ^ a b Osawa, K.; Hata, S. (1960). "Three colour photometry of B8-A2 stars". Annals of the Tokyo Astronomical Observatory. 6: 148. Bibcode: 1960AnTok...6..148O.
  7. ^ 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. eISSN  1562-6873. ISSN  1063-7737. S2CID  119231169.
  8. ^ a b 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.
  9. ^ a b Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (April 8, 2004). "The angular sizes of dwarf stars and subgiants: Surface brightness relations calibrated by interferometry". Astronomy & Astrophysics. 426 (1): 297–307. arXiv: astro-ph/0404180. Bibcode: 2004A&A...426..297K. doi: 10.1051/0004-6361:20035930. eISSN  1432-0746. ISSN  0004-6361. S2CID  6077801.
  10. ^ Philip, A. G. D.; Egret, D. (May 1980). "An analysis of the Hauck-Mermillod catalogue of homogeneous four-color data. II". Astronomy and Astrophysics Supplement Series. 40: 199–205. Bibcode: 1980A&AS...40..199P. ISSN  0365-0138.
  11. ^ a b Takeda, Yoichi; Han, Inwoo; Kang, Dong-Il; Lee, Byeong-Cheol; Kim, Kang-Min (May 1, 2019). "Compositional differences between the component stars of eclipsing close binary systems showing chemical peculiarities". Monthly Notices of the Royal Astronomical Society. 485 (1): 1067–1084. arXiv: 1902.04766. Bibcode: 2019MNRAS.485.1067T. doi: 10.1093/mnras/stz449. ISSN  0035-8711. S2CID  119421663.
  12. ^ a b Gebran, M.; Farah, W.; Paletou, F.; Monier, R.; Watson, V. (18 April 2016). "A new method for the inversion of atmospheric parameters of A/Am stars". Astronomy & Astrophysics. 589: A83. arXiv: 1603.01146. Bibcode: 2016A&A...589A..83G. doi: 10.1051/0004-6361/201528052. eISSN  1432-0746. ISSN  0004-6361. S2CID  118549566.
  13. ^ a b Royer, F.; Grenier, S.; Baylac, M.-O.; Gómez, A. E.; Zorec, J. (October 2002). "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i". Astronomy & Astrophysics. 393 (3): 897–911. arXiv: astro-ph/0205255. Bibcode: 2002A&A...393..897R. doi: 10.1051/0004-6361:20020943. eISSN  1432-0746. ISSN  0004-6361.
  14. ^ a b Gontcharov, G. A. (November 2012). "Spatial distribution and kinematics of OB stars". Astronomy Letters. 38 (11): 694–706. arXiv: 1606.09028. Bibcode: 2012AstL...38..694G. doi: 10.1134/S1063773712110035. eISSN  1562-6873. ISSN  1063-7737. S2CID  255202762.
  15. ^ a b 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. eISSN  1562-6873. ISSN  1063-7737. S2CID  118345778.
  16. ^ Verbunt, F.; van Gent, R. H. (June 2010). "The star catalogue of Hevelius: Machine-readable version and comparison with the modern Hipparcos Catalogue". Astronomy and Astrophysics. 516: A29. Bibcode: 2010A&A...516A..29V. doi: 10.1051/0004-6361/201014003. eISSN  1432-0746. ISSN  0004-6361. S2CID  54171435.
  17. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. S2CID  14878976.
  18. ^ 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.
  19. ^ 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. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. ISSN  0004-6256. S2CID  119533755.
  20. ^ 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.
Retrieved from " https://en.wikipedia.org/?title=10_Trianguli&oldid=1189379391"

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