Stars Hercules has no
first or second magnitude stars. However, it does have several stars above magnitude 4.
Alpha Herculis, traditionally called Rasalgethi, is a
triple star system, partly resolvable in small amateur telescopes, 359 light-years from Earth. Its common name means "the kneeler's head". The primary is an irregular
variable star; it is a
bright giant with a minimum magnitude of 4 and a maximum magnitude of 3. It has a diameter of roughly 400
solar diameters. The secondary, a
spectroscopic binary that orbits the primary every 3600 years, is a blue-green hued star of magnitude 5.6. Five degrees east-south-east of Rasalgethi lies
Rasalhague, the brightest star in
Ophiuchus. These stars may be among the closest-lying pair of alpha stars in the entire sky. Despite the star designated as "alpha", it is actually the 5th brightest star in Hercules.
Beta Herculis, also called Kornephoros, is the brightest star in Hercules. It is a
yellow giant of magnitude 2.8, 148 light-years from Earth; kornephoros means club-bearer.
Delta Herculis A is a double star divisible in small amateur telescopes. The primary is a blue-white star of magnitude 3.1, and is 78 light-years from Earth. The optical companion is of magnitude 8.2.
Gamma Herculis is also a double star divisible in small amateur telescopes. The primary is a
white giant of magnitude 3.8, 195 light-years from Earth. The optical companion, widely separated, is 10th magnitude.
Zeta Herculis is a binary star that is becoming divisible in medium-aperture amateur telescopes, as the components widen to their peak in 2025. The system, 35 light-years from Earth, has a period of 34.5 years. The primary is a yellow-tinged star of magnitude 2.9 and the secondary is an orange star of magnitude 5.7. Hercules hosts further quite bright double stars and binary stars.
Kappa Herculis is a double star divisible in small amateur telescopes. The primary is a yellow giant of magnitude 5.0, 388 light-years from Earth; the secondary is an
orange giant of magnitude 6.3, 470 light-years from Earth.
Rho Herculis is a binary star 402 light-years from Earth, divisible in small amateur telescopes. Both components are blue-green giant stars; the primary is magnitude 4.5 and the secondary is magnitude 5.5.
95 Herculis is a binary star divisible in small telescopes, 470 light-years from Earth. The primary is a silvery giant of magnitude 4.9, and the secondary is an old, reddish giant star of magnitude 5.2. The star HD164669 near the primary may be an optical double.
100 Herculis is a double star easily divisible in small amateur telescopes. Both components are magnitude 5.8 blue-white stars; they are 165 and 230 light-years from Earth. between Hercules' left elbow (near
Omicron Herculis) and
Vega (in neighboring
Lyra).
Planetary systems Fifteen stars in Hercules are known to be orbited by
extrasolar planets. •
14 Herculis has two planets. The planet
14 Herculis b had the longest period (4.9 years) and widest orbit (2.8
AU) at the time of discovery. The planet
14 Herculis c orbits much further out with very low eccentricity. It was discovered in 2005 but was only confirmed in 2021. •
HD 149026 has a
transiting hot Jupiter planet. •
HD 154345 has the planet
HD 154345 b, a long period (9.095 years) and wide orbit (4.18 AU). •
HD 164922 has the first long period Saturn-like
planet discovered. The
mass is 0.36 MJ and
semimajor axis of 2.11 AU. More planets have been discovered since. The mass is 8.65 MJ. •
HD 155358 has two planets around the lowest
metallicity planet-harboring star (21% Sun). Both planets orbit in mild eccentricities. •
GSC 03089-00929 has a short transiting planet
TrES-3b. The
period was 31 hours. •
Gliese 649 has a
saturnian planet around the red dwarf star. •
HD 156668 has an
Earth mass planet with a minimum mass of four Earth masses. •
HD 164595 is a G-type star with one known planet,
HD 164595 b. •
TOI-561 has four, or possibly five planets. The innermost of which,
TOI-561 b, is notable because it is an
ultra-short period planet.
Deep-sky objects Hercules contains two bright
globular clusters:
M13, the brightest globular cluster in the northern hemisphere, and
M92. It also contains the nearly spherical
planetary nebula Abell 39. M13 lies between the stars
η Her and
ζ Her; it is dim, but may be detected by the unaided eye on a very clear night. M13, visible to both the naked eye and binoculars, is a globular cluster of the 6th magnitude that contains more than 300,000 stars and is 25,200 light-years from Earth. It is also very large, with an apparent diameter of over 0.25 degrees, half the size of the
full moon; its physical diameter is more than 100 light-years. Individual stars in M13 are resolvable in a small amateur telescope. M92 is visible as a fuzzy star in binoculars, like M13; it is denser and smaller than the more celebrated cluster. The oldest globular cluster known at 14 billion years, its stars are resolvable in a medium-aperture amateur telescope.
NGC 6210 is a
planetary nebula of the 9th magnitude, 4000 light-years from Earth visible as a blue-green elliptical disk in amateur telescopes larger than 75 mm in aperture. As of 22 June 2018, this
astronomical event has generated a very large amount of interest among astronomers throughout the world and may be, as of 22 June 2018, considered a supernova tentatively named
Supernova 2018cow. The
Hercules Cluster (Abell 2151) is a cluster of galaxies in Hercules. The brightest radio source in the constellation is
Hercules A, an
elliptical galaxy located 2.1 billion light years away with a
supermassive black hole with a mass of 2.5-billion-solar-mass that has
radio jets that extend for one-and-a-half million light-years. Another bright radio source in Hercules is the
quasar 3C 345 which has a
jet that appears to
move faster than the speed of light. The
Hercules–Corona Borealis Great Wall, the largest structure in the universe, is in Hercules. ==Visualizations==