{{Starbox observe 2s
| epoch = J2000
| constell = 寶瓶座
| component1 = 寶瓶座ζA
| ra1 = 。換言之， (, .)。
性質
軌道
這兩顆恆星的軌道週期約為587年。半長軸為3.8 角秒，其軌道離心率為0.40。軌道平面與天空平面傾角138.2°
延伸閱讀
Heintz, Wulff-Dieter (1984). [https://ui.adsabs.harvard.edu/abs/1984ApJ...284..806H/abstract The Triple Star Zeta Aquarii]. The Astrophysical Journal*. 284: pp. 806-9. (This is Heintz's 1984 article, mentioned above as the one that established Zeta Aquarii Ab as being connected to Zeta Aquarii Aa; it was not used as a reference for this article.)
Strand, Kaj Aage Gunnar (1942). [https://ui.adsabs.harvard.edu/abs/1942AJ.....49..165S/abstract The Orbital Motion of the Triple System Zeta Aquarii]. The Astrophysical Journal*. 49 (18): pp. 165-72. (This is Strand's 1942 article, mentioned above as the one that established Zeta Aquarii as a triple system; it was not used as a reference for this article.)
外部連結
- [https://web.archive.org/web/20051212204932/http://www.prairieastronomyclub.org/dblstar4.htm Double Stars to Follow, Part IV: Zeta Aquarii and Mu Cygni.] by Martin Gaskell, Prairie Astronomy Club Home Page.
- [https://web.archive.org/web/20050628090714/http://www.asnsw.com/universe/1997/tmds-1197.htm "This Month's Double Stars"] by Richard Jaworski.
- [http://aladin.u-strasbg.fr/AladinPreview?-c=NLTT+53956&ident=NLTT+53956&submit=Aladin+previewer Image ζ Aquarii]
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