Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1 Trianguli

From Wikipedia, the free encyclopedia
Star in the constellation Triangulum
1 Trianguli
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationTriangulum
Right ascension01h 42m 05.92475s[1]
Declination+29° 30′ 21.8431″[1]
Apparent magnitude (V)7.52±0.01[2]
Characteristics
Evolutionary stagemain sequence star[1]
Spectral typeA2 V[3]
B−Vcolor index+0.06[2]
Astrometry
Radial velocity (Rv)7±4.5[4] km/s
Proper motion (μ)RA: −10.545mas/yr[1]
Dec.: −0.288mas/yr[1]
Parallax (π)4.5114±0.0515 mas[1]
Distance723 ± 8 ly
(222 ± 3 pc)
Absolute magnitude (MV)+0.78[5]
Details
Mass2.36+0.34
−0.30
[6] M
Radius2.69±0.14[7] R
Luminosity52+1.5
−2.2
[1] L
Surface gravity (log g)3.90[8] cgs
Temperature9,305+145
−192
[6] K
Metallicity[Fe/H]−0.02[8] dex
Age371±23[9][10] Myr
Other designations
1 Trianguli,AG+29°220,BD+28°282,GC 2068,HD 10407,HIP 7948,SAO 74880,GSC 01762-00704[11]
Database references
SIMBADdata

1 Trianguli, also known asHD 10407, is astar located in the northernconstellationTriangulum. It has anapparent magnitude of 7.52,[2] making it readily visible inbinoculars but not to thenaked eye.Gaia DR3parallax measurements imply a distance of 723light years[1] and it is currently receding with a heliocentricradial velocity ofkm/s.[4] At its current distance 1 Trianguli's brightness is diminished by a quarter of amagnitudes due tointerstellar dust[12] and it has anabsolute magnitude of +0.78.[5] Even though it has aFlamsteed designation, 1 Trianguli is one of the 220 Flamsteed stars that are not in theYale Bright Star Catalogue.[13]

1 Trianguli has astellar classification of A2 V,[3] indicating that it is an ordinaryA-type main-sequence star. It has 2.36 times themass of the Sun[6] and 2.69 times theSun's radius.[7] It radiates 52 times theluminosity of the Sun[1] from itsphotosphere at aneffective temperature of9,305 K,[6] giving it a white hue. It has a near solarmetallicity at [Fe/H] = −0.02[8] and 1 Trianguli is estimated to be 371million years old.[9][10]

References

[edit]
  1. ^abcdefghVallenari, 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 atVizieR.
  2. ^abcHog, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000-03-01). "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. ^abClausen, J. V.; Jensen, K. S. (1979). "Classification Based on 102/A/Mm Objective Prism Spectra".IAU Colloq. 47: Spectral Classification of the Future.9: 479.Bibcode:1979RA......9..479C.
  4. ^abGontcharov, 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.
  5. ^abAnderson, 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.
  6. ^abcdStassun, Keivan G.; et al. (9 September 2019)."The RevisedTESS 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.hdl:1721.1/124721.S2CID 166227927.
  7. ^abKervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 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.
  8. ^abcAnders, F.; et al. (February 2022)."Photo-astrometric distances, extinctions, and astrophysical parameters forGaia EDR3 stars brighter thanG = 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. ^abGontcharov, 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.
  10. ^abGontcharov, 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.
  11. ^"*1 Tri".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedMarch 29, 2021.
  12. ^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.
  13. ^Bidelman, W. P. (December 1990). "Flamsteed stars not contained in the Yale "Catalogue of Bright Stars"".Bulletin d'Information du Centre de Donnees Stellaires.38: 13.Bibcode:1990BICDS..38...13B.ISSN 1169-8837.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Nebulae
NGC
Galaxies
NGC
Numbered
Other
Retrieved from "https://en.wikipedia.org/w/index.php?title=1_Trianguli&oldid=1266528308"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp