53 Eridani

53 Eridani (abbreviated 53 Eri), also designated l Eridani (l Eri), is a binary star in the constellation of Eridanus. The system has a combined apparent magnitude of 3.87. Parallax estimates made by the "Hipparcos" spacecraft put it at a distance of about 110 light-years, or 33.7 parsecs, from the Sun.
The two components are designated 53 Eridani A (officially named Sceptrum) and B.
Nomenclature.
"53 Eridani" is the system's Flamsteed designation; "l Eridani" is its Bayer designation. The designations of the two components as "53 Eridani A" and "B" derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).
53 Eridani bore the traditional name ('scepter'), as it was one of the brighter stars, designated "p Sceptri (Brandenburgici)", in the obsolete constellation of Sceptrum Brandenburgicum. The constellation was coined by Gottfried Kirch to honor the Brandenburg province of Prussia, and although it was later used in other atlases by Johann Elert Bode, the constellation fell out of use. In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. It approved the name "Sceptrum" for the component 53 Eridani A on 30 June 2017 and it is now so included in the List of IAU-approved Star Names.
Properties.
53 Eridani is a visual binary, where the orbit of the two stars is calculated from their orbital motions. The primary star, 53 Eridani A, is an evolved red giant with a spectral type of K1III. It is almost ten times as wide as the Sun and slightly more massive than the Sun. The secondary star, 53 Eridani B, has an apparent magnitude of 6.95 and its spectral type is unknown. The two have an orbital period of 77 years and have a quite eccentric orbit at 0.666. The total mass of the system is .