Stars Capricornus is a faint constellation, with only one star above magnitude 3; its
alpha star has a magnitude of only 3.6. The brightest star in Capricornus is
δ Capricorni, also called Deneb Algedi, with a magnitude of 2.9, located 39 light-years from Earth. Like several other stars such as
Denebola and
Deneb, it is named from the Arabic word for "tail" (
deneb) and “young goat / kid” (al-gedi), meaning "the tail of the goat". Deneb Algedi is a
Beta Lyrae variable star (a type of
eclipsing binary). It ranges by about 0.2 magnitudes with a period of 24.5 hours. The other bright stars in Capricornus range in magnitude from 3.1 to 5.1.
α Capricorni is a multiple star. The primary (
α2 Cap), 109 light-years from Earth, is a yellow-hued giant star of magnitude 3.6; the secondary (
α1 Cap), 690 light-years from Earth, is a yellow-hued supergiant star of magnitude 4.3. The two stars are distinguishable by the naked eye, and both are themselves multiple stars. α1 Capricorni is accompanied by a star of magnitude 9.2; α2 Capricorni is accompanied by a star of magnitude 11.0; this faint star is itself a binary star with two components of magnitude 11. Also called Algedi or Giedi, the traditional names of α Capricorni come from the Arabic word for "the kid", which references the constellation's mythology.
β Capricorni is a
double star also known as Dabih. It is a yellow-hued giant star of magnitude 3.1, 340 light-years from Earth. The secondary is a blue-white hued star of magnitude 6.1. The two stars are distinguishable in binoculars. β Capricorni's traditional name comes from the Arabic phrase for "the lucky stars of the slaughterer," a reference to ritual sacrifices performed by ancient Arabs at the
heliacal rising of Capricornus. Another star visible to the naked eye is
γ Capricorni, sometimes called Nashira ("bringing good tidings"); it is a white-hued giant star of magnitude 3.7, 139 light-years from Earth.
π Capricorni is a double star with a blue-white hued primary of magnitude 5.1 and a white-hued secondary of magnitude 8.3. It is 670 light-years from Earth and the components are distinguishable in a small telescope.
Deep-sky objects Several galaxies and star clusters are contained within Capricornus.
Messier 30 is a globular cluster located 1 degree south of the galaxy group that contains
NGC 7103. The constellation also harbors the wide spiral galaxy
NGC 6907. Messier 30 (NGC 7099) is a centrally-condensed globular cluster of magnitude 7.5 . At a distance of 30,000 light-years, it has chains of stars extending to the north that are resolvable in small amateur telescopes. One
galaxy group located in Capricornus is
HCG 87, a group of at least three galaxies located 400 million
light-years from Earth (
redshift 0.0296). It contains a large
elliptical galaxy, a face-on
spiral galaxy, and an edge-on spiral galaxy. The face-on spiral galaxy is experiencing abnormally high rates of
star formation, indicating that it is
interacting with one or both members of the group. Furthermore, the large elliptical galaxy and the edge-on spiral galaxy, both of which have
active nuclei, are connected by a stream of stars and dust, indicating that they too are interacting. Astronomers predict that the three galaxies may
merge millions of years in the future to form a giant elliptical galaxy. ==History ==