| 词条 | HD 213429 |
| 释义 |
| name=HD 213429 }}{{Starbox observe | epoch=J2000 | ra={{RA|22|31|18.31271}} | dec={{DEC|−06|33|18.5437}} | appmag_v=6.160[3] | constell=Aquarius }}{{Starbox character | class=F8V[4] | b-v=+0.55[5] | u-b=+0.03[5] | variable= }}{{Starbox astrometry | radial_v={{val|−9.9|6.3}}[3] | prop_mo_ra=+161.61 | prop_mo_dec=−108.40 | parallax=39.35 | p_error=0.70 | parallax_footnote= | absmag_v=4.13[3] }}{{Starbox detail | component1=HD 213429 A | mass=1.18[12] | radius= | luminosity= | temperature=6,001[4] | gravity=4.10[4] | metal_fe=−0.23[4] | rotational_velocity=6[16] | age_gyr=3.7[3] | component2=HD 213429 B | mass2=0.78[12] }}{{Starbox catalog | names=BD-07° 5797, HD 213429, HIP 111170, HR 8581, LTT 9053, SAO 146135. }}{{Starbox reference | Simbad=HD+213429 }}{{starbox sources|HIP|CCDM|HR}}{{Starbox end}}HD 213429 is a spectroscopic binary[12] system in the equatorial constellation of Aquarius. It has a combined apparent magnitude of 6.16 and is located around 83 light years away. The pair orbit each other with a period of 631 days,[12] at an average separation of 1.74 AU and an eccentricity of 0.38.[21] References1. ^1 2 3 4 {{citation | display-authors=1 | last1=Gray | first1=R. O. | last2=Corbally | first2=C. J. | last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T. | last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E. | last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R. | title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | journal=The Astronomical Journal | volume=132 | issue=1 | pages=161–170 | date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770}} [1][2][3][4][5][6]2. ^1 2 3 4 {{citation | display-authors=1 | last1=Nordström | first1=B. | last2=Mayor | first2=M. | last3=Andersen | first3=J. | last4=Holmberg | first4=J. | last5=Pont | first5=F. | last6=Jørgensen | first6=B. R. | last7=Olsen | first7=E. H. | last8=Udry | first8=S. | last9=Mowlavi | first9=N. | title=The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs | journal=Astronomy and Astrophysics | volume=418 | pages=989–1019 | date=May 2014 | doi=10.1051/0004-6361:20035959 | bibcode=2004A&A...418..989N |arxiv = astro-ph/0405198}} 3. ^1 {{citation | last1=Uesugi | first1=Akira | last2=Fukuda | first2=Ichiro | title=Catalogue of rotational velocities of the stars | journal=Contributions from the Institute of Astrophysics and Kwasan Observatory | date=1970 | publisher=University of Kyoto | bibcode=1970crvs.book.....U}} 4. ^1 2 {{citation | last1=Mermilliod | first1=J.-C. | title=Compilation of Eggen's UBV data, transformed to UBV (unpublished) | journal=Catalogue of Eggen's UBV data. SIMBAD | date=1986 | bibcode=1986EgUBV........0M}} 5. ^1 2 3 4 {{citation | last1=Tokovinin | first1=Andrei | title=From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs | journal=The Astronomical Journal | volume=147 | issue=4 | id=87 | pages=14 | date=April 2014 | doi=10.1088/0004-6256/147/4/87 | bibcode=2014AJ....147...87T |arxiv = 1401.6827 }} 6. ^1 {{citation | display-authors=1 | last1=Jaime | first1=Luisa G. | last2=Aguilar | first2=Luis | last3=Pichardo | first3=Barbara | title=Habitable zones with stable orbits for planets around binary systems | journal=Monthly Notices of the Royal Astronomical Society | volume=443 | issue=1 | pages=260–274 | date=September 2014 | doi=10.1093/mnras/stu1052 | bibcode=2014MNRAS.443..260J|arxiv = 1401.1006 }} }} External links
8 : Aquarius (constellation)|Henry Draper Catalogue objects|F-type main-sequence stars|HR objects|Spectroscopic binaries|Durchmusterung objects|Hipparcos objects|Gliese and GJ objects |
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