Rasalnaqa

In the western parts of the constellation of Andromeda, three stars form a clear downward-pointing triangle. These three stars are Psi Andromedae, Udkadua (Lambda Andromedae) and Kaffalmusalsala (Kappa Andromedae). Together they point southward towards a fourth star, faint blue Rasalnaqa or Iota Andromedae. Iota falls close to the Blue Snowball planetary nebula, which lies a little over two degrees to the west.

Rasalnaqa lies far from the Solar System at a distance of almost exactly five hundred light years. It is a young dwarf or main sequence star, and a highly luminous one. Though its apparent magnitude as seen from Earth is a modest +4.3, its absolute magnitude is a brilliant -1.7, and the star emits nearly four hundred times as much light energy as the Sun.

The spectral type of this star is B8V, meaning that it has a similar structure to better-known Algol in Perseus, which is also a B8V star. Unlike Algol, Rasalnaqa has no known binary companion, and so where Algol (which is regularly eclipsed by its own companion star) Rasalnaqa shines steadily with a constant level of brightness.