Stars Scorpius contains many bright stars, including
Antares (α Sco), "rival of Mars," so named because of its distinct reddish hue;
β1 Sco (Graffias or Acrab), a triple star;
δ Sco (
Dschubba, "the forehead");
θ Sco (
Sargas, of Sumerian origin);
ν Sco (Jabbah);
ξ Sco;
π Sco (Fang);
σ Sco (Alniyat); and
τ Sco (Paikauhale). Marking the tip of the scorpion's curved tail are
λ Sco (
Shaula) and
υ Sco (Lesath), whose names both mean "sting." Given their proximity to one another, λ Sco and υ Sco are sometimes referred to as the Cat's Eyes. The constellation's bright stars form a pattern like a
longshoreman's hook. Most of them are massive members of the nearest
OB association:
Scorpius–Centaurus. The star δ Sco, after having been a stable 2.3
magnitude star, flared in July 2000 to 1.9 in a matter of weeks. It has since become a variable star fluctuating between 2.0 and 1.6. This means that at its brightest it is the second brightest star in Scorpius.
U Scorpii is the fastest known
nova, with a period of about 10 years.
AH Scorpii is a
red supergiant star and
one of the largest known stars, being 1,400 times larger than the Sun. It is also a luminous star, 340,000 times brighter than the Sun, although it is too faint to be seen by the naked eye, with a brightness varying from 6.5 to 9.6. The
close pair of stars
ω1 Scorpii and
ω² Scorpii are an
optical double, which can be resolved by the unaided eye. One is a yellow giant, while the other is a blue B-type star in the Scorpius-Centaurus Association. The star once designated γ Sco (despite being well within the boundaries of Libra) is today known as
σ Lib. Moreover, the entire constellation of
Libra was considered to be claws of Scorpius (
Chelae Scorpionis) in
Ancient Greek times, with a set of scales held aloft by
Astraea (represented by adjacent
Virgo) being formed from these westernmost stars during later Greek times. The division into Libra was formalised during Ancient Greek or
Roman times.
Deep-sky objects , with
M4 and
M80 visible near Antares,
M6 and
M7 just below centre,
NGC 6124 at the top of the frame, and
NGC 6334 just above centre. Due to its location straddling the
Milky Way, this constellation contains many
deep-sky objects such as the
open clusters
Messier 6 (the
Butterfly Cluster) and
Messier 7 (the
Ptolemy Cluster),
NGC 6231 (by
ζ² Sco), and the
globular clusters
Messier 4 and
Messier 80.
Messier 80 (NGC 6093) is a globular cluster of magnitude 7.3, 33,000 light-years from Earth. It is a compact Shapley class II cluster; the classification indicates that it is highly concentrated and dense at its nucleus. M80 was discovered in 1781 by
Charles Messier. It was the site of a rare discovery in 1860 when
Arthur von Auwers discovered the nova
T Scorpii.
NGC 6302, also called the Bug Nebula, is a bipolar planetary nebula.
NGC 6334, also known as the Cat's Paw Nebula, is an emission nebula and star-forming region. are illuminated by Antares and the other neighboring stars. == History and mythology ==