Eta Andromedae (Eta And / η Andromedae / η And) adalah bintang ganda yang berada di rasi Andromeda. Sistem bintang ini terdiri dari dua bintang sub raksasa tipe G (G-type subgiant)]] dengan periode orbit 115.7 hari dan magnitudo keseluruhan 4.40.[1][2]
^ abcdefghijklmThe spectroscopic binary eta Andromedae: Determination of the orbit by optical interferometry, C. A. Hummel et al., Astronomical Journal106, #6 (December 1993), pp. 2486–2492, Bibcode: 1993AJ....106.2486H, DOI:10.1086/116816.
^ abcHR 271, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line August 23, 2008.
^ abTable 2, Resolved double-lined spectroscopic binaries: A neglected source of hypothesis-free parallaxes and stellar masses, D. Pourbaix, Astronomy and Astrophysics Supplement145 (August 2000), pp. 215–222, Bibcode: 2000A&AS..145..215P.
^A list of nine stars whose velocities in the line of sight are variable, W. W. Campbell and W. H. Wright, Astrophysical Journal12 (November 1900), pp. 254–257, Bibcode: 1900ApJ....12..254C, DOI:10.1086/140765.
^The Spectroscopic Binary η Andromedae, Katherine C. Gordon, Astrophysical Journal103 (January 1946), pp. 13–15, Bibcode: 1946ApJ...103...13G.