释义 |
- References
{{Starbox begin | name=Iota Antliae }}{{Starbox image | image = | caption = Location of ι Antliae (circled) }}{{Starbox observe | epoch = J2000 | ra = {{RA|10|56|43.05206}} | dec = {{DEC|–37|08|15.9552}} | appmag_v = +4.60[3] | constell = Antlia }}{{Starbox character | class = K1 III[4] | b-v = +1.03[3] | u-b = +0.84[3] | variable = }}{{Starbox astrometry | radial_v = –0.2[7] | prop_mo_ra = {{Val|+74.303|0.221}}[8] | prop_mo_dec = {{Val|−125.185|0.259}}[8] | parallax = 16.1823 | p_error = 0.1882 | parallax_footnote = [1] | absmag_v = +0.77[11] }}{{Starbox detail | mass = 1.55[12] | radius = | luminosity = 60[11] | temperature = {{Val|4786|22|fmt=commas}} | gravity = | rotational_velocity = | age_gyr = 3.32[12] }}{{Starbox catalog | names=CD–36° 6808, FK5 414, HD 94890, HIP 53502, HR 4273, SAO 201927.[15] }}{{Starbox reference |Simbad=iot+Ant }}{{Starbox end}}Iota Antliae (ι Ant, ι Antliae) is the Bayer designation for a star in the southern constellation of Antlia. It has an apparent visual magnitude of +4.60,[3] making it a faint naked eye star. From parallax measurements, the distance to this star can be estimated as {{Convert|202 ± 2|ly|pc|abbr=off|lk=on}}.[1] The spectrum of Iota Antliae matches a stellar classification of K1 III,[4] indicating that this is an evolved star that is now in its giant phase. It is a core helium fusing star that is classified as a member of the red clump evolutionary branch.[19]References1. ^1 2 3 {{cite DR2|5394951821153092864}} 2. ^1 2 {{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | postscript=. }} 3. ^1 2 {{citation | title=Abundances in the Local Region. I. G and K Giants | last1=Luck | first1=R. Earle | journal=Astronomical Journal | postscript=. | volume=150 | issue=3 | at=88 | year=2015 | bibcode=2015AJ....150...88L | doi=10.1088/0004-6256/150/3/88 |arxiv = 1507.01466 }} 4. ^1 2 {{citation | title=Michigan catalogue of two-dimensional spectral types for the HD stars | volume=3 | last1=Houk | first1=Nancy | publication-place=Ann Arbor, Michigan | publisher=Dept. of Astronomy, University of Michigan | year=1979 | bibcode=1982mcts.book.....H | postscript=. }} 5. ^1 {{citation | display-authors=1 | title=Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions | last1=Wielen | first1=R. | last2=Schwan | first2=H. | last3=Dettbarn | first3=C. | last4=Lenhardt | first4=H. | last5=Jahreiß | first5=H. | last6=Jährling | first6=R. | publisher=Astronomisches Rechen-Institut Heidelberg | issue=35 | year=1999 | bibcode=1999VeARI..35....1W | postscript=. }} 6. ^1 2 3 4 {{citation | display-authors=1 | last1=Johnson | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966 | bibcode=1966CoLPL...4...99J | postscript=. }} 7. ^1 {{citation | title=iot Ant -- Star | work=SIMBAD Astronomical Object Database | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Iota+Antliae | accessdate=2012-06-29 | postscript=. }} 8. ^1 {{citation | display-authors=1 | last1=Kubiak | first1=M. | last2=McWilliam | first2=A. | last3=Udalski | first3=A. | last4=Gorski | first4=K. | title=Metal Abundance of Red Clump Stars in Baade's Window | journal=Acta Astronomica | volume=52 | pages=159–175 |date=June 2002 | bibcode=2002AcA....52..159K | postscript=. }}
[2][3][4][5][6][7][8] }}{{Stars of Antlia}}{{giant-star-stub}} 8 : K-type giants|Horizontal-branch stars|Antlia|Bayer objects|Durchmusterung objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects |