Messier 13

Globular cluster in the constellation Hercules
title: "Messier 13" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["globular-clusters", "hercules-(constellation)", "messier-objects", "milky-way", "ngc-objects", "astronomical-objects-discovered-in-1714"] description: "Globular cluster in the constellation Hercules" topic_path: "general/globular-clusters" source: "https://en.wikipedia.org/wiki/Messier_13" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0
::summary Globular cluster in the constellation Hercules ::
::data[format=table title="Infobox globular cluster"]
| Field | Value |
|---|---|
| name | Messier 13 |
| image | M13-Globular-Cluster.png |
| caption | Globular cluster Messier 13 in Hercules captured with an amateur telescope in 2025. |
| epoch | J2000 |
| class | V |
| constellation | Hercules |
| ra | |
| dec | |
| dist_ly | 24.1 kly |
| appmag_v | 5.8 |
| size_v | 20 arcminutes |
| mass_msol | |
| radius_ly | 84 ly |
| metal_fe | –1.33 |
| absmag_v | –8.5 |
| age | 11.65 Gyr |
| notes | One of the best-known clusters of the Northern Hemisphere |
| names | NGC 6205 |
| :: |
| name=Messier 13 | image=M13-Globular-Cluster.png | caption=Globular cluster Messier 13 in Hercules captured with an amateur telescope in 2025. | credit= | epoch=J2000 | class=V | constellation=Hercules | ra= | dec= | dist_ly=24.1 kly | appmag_v=5.8 | size_v=20 arcminutes | mass_msol= | radius_ly = 84 ly | metal_fe = –1.33 | absmag_v = –8.5 | age = 11.65 Gyr | notes=One of the best-known clusters of the Northern Hemisphere | names=NGC 6205 Messier 13, or M13 (also designated NGC 6205 and sometimes called the Great Globular Cluster in Hercules, the Hercules Globular Cluster, or the Great Hercules Cluster), is a globular cluster of several hundred thousand stars in the constellation of Hercules.
Discovery and visibility
Messier 13 was discovered by Edmond Halley in 1714, It is located at right ascension 16h 41.7m, declination +36° 28'. Messier 13 is often described by astronomers as the most magnificent globular cluster visible to northern observers.
About one third of the way from Vega to Arcturus, four bright stars in Hercules form the Keystone asterism, the broad torso of the hero. M13 can be seen in this asterism of the way north (by west) from Zeta to Eta Herculis. With an apparent magnitude of 5.8, At least four inches of telescope aperture resolves stars in Messier 13's outer extent as small pinpoints of light. However, only larger telescopes resolve stars further into the center of the cluster. The cluster is visible throughout the year from latitudes greater than 36 degrees north, with the longest visibility during Northern Hemisphere spring and summer.
Nearby to Messier 13 is NGC 6207, a 12th-magnitude edge-on galaxy that lies 28 arcminutes directly northeast. A small galaxy, IC 4617, lies halfway between NGC 6207 and M13, north-northeast of the large globular cluster's center. At low powers the cluster is bracketed by two seventh-magnitude stars.
Characteristics
::figure[src="https://upload.wikimedia.org/wikipedia/commons/6/60/Heart_of_M13_Hercules_Globular_Cluster.jpg" caption="access-date=2021-11-22}}"] ::
The stars in this cluster are firmly in the Population II category, markedly lower in metals than Population I stars like the Sun and most other stars in the Sun's close proximity. M13 as a whole has only about 4.6% as much iron as the Sun does.
Single stars in this globular cluster were first resolved in 1779. Compared to the stars in the neighborhood of the Sun, the stars of the M13 population are more than a hundred times more densely packed. They are so close together that they sometimes collide and produce new stars. The newly formed, young stars, known as "blue stragglers", are particularly interesting to astronomers.
The last three variables (V63, V64 and V65) were discovered from Spain in April 2021, March 2022 and January 2024, respectively.
Arecibo message
::figure[src="https://upload.wikimedia.org/wikipedia/commons/c/cd/Arecibo_Observatory_Aerial_View.jpg" caption="The Arecibo Observatory radio telescope that transmitted the message."] ::
Main article: Arecibo message
The 1974 Arecibo message, which contained encoded information about the human race, DNA, atomic numbers, Earth's position and other information, was beamed from the Arecibo Observatory radio telescope towards Messier 13. It was meant as a demonstration of human technological achievement, rather than a real attempt to enter into a conversation with extraterrestrials. M13 was chosen because it was a large, relatively close star cluster that was available at the time and place of the ceremony. It will take around 25,000 years for the message to reach the cluster, though it will move through space during the transit time; opinions differ as to whether or not the cluster will be in a position to receive the message by the time that it arrives.
Literary references
- The science fiction novellas "Sucker Bait" by Isaac Asimov and the novel Question and Answer by Poul Anderson take place on Troas, a world within M13.
- In the German science fiction series Perry Rhodan, M13 is the location of Arkon, the homeworld of the race of Arkonides.
- In author James Blish 's Cities In Flight, the alien "Web of Hercules" attacks from this cluster.
- In author Dan Simmons' Hyperion Cantos the Hercules cluster is where a copy of Earth was secretly recreated after the original was destroyed.
- In his novel The Sirens of Titan, Kurt Vonnegut writes "Every passing hour brings the Solar System forty-three thousand miles closer to Globular Cluster M13 in Hercules—and still there are some misfits who insist that there is no such thing as progress."
- Messier 13 is the home of the antagonistic aliens in the 1977 space opera The War in Space, who hail from the third planet of a system orbiting a star called Yomi.
- Deliberately engineering a star in Messier 13 to go nova was part of the Cybermen's complicated plot in the 1968 Doctor Who story The Wheel in Space.
In art
- Messier 13 is featured as part of the interior of the dome of St Anne's Church, Kew in London, based on a photograph by NASA. Halley discovered the galaxy in 1714, the same year that the church was first dedicated.
Gallery
File:Hercules constellation map.png|M13 is in the "armpit" of the constellation Hercules. File:Heart of M13 Hercules Globular Cluster.jpg|Heart of the Hercules Globular Cluster, Hubble image File:Hubble’s Views of M13 (2010) and M3 (2019).jpg|Hubble images comparing M13 and M3 File:Messier 13 (infrared, red, green).jpg|M13 in near infrared and visible light File:The ceiling of the chancel of St Anne's Church, Kew Green - geograph.org.uk - 8110657.jpg|M13 painted on the interior of the dome ceiling of St Anne's Church, Kew. File:Hercules globular cluster m13.jpg|Portrait of Messier 13
References
References
- distance × sin(diameter_angle / 2) = 84 ly radius
- (2016-05-09). "Messier 13 (M13) - The Great Hercules Cluster - Universe Today". Universe Today.
- "How to See the Great Hercules Cluster of Stars". Space.com.
- "M13: Great Cluster in Hercules {{!}} EarthSky.org".
- "NGC 6207".
- "Control Telescope :: Stars & Nebulae".
- "Star Cluster".
- Garner, Rob. (2017-10-06). "Messier 13 (The Hercules Cluster)". NASA.
- (December 1975). "The Arecibo message of November, 1974". Icarus.
- Klaes, Larry. (2005-11-30). "Making Contact". Ithaca Times.
- (1999-11-12). "It's the 25th anniversary of Earth's first attempt to phone E.T.". Cornell News.
- [[David Blomfield. (2014). "St Anne's Kew, 1714–2014". R J L Smith and Associates.
- (December 2010). "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters". The Astronomical Journal.
- (September 2020). "Isochrone fitting of Galactic globular clusters - II. NGC 6205 (M13)". Monthly Notices of the Royal Astronomical Society.
- "M 13".
- (August 1927). "A Classification of Globular Clusters". Harvard College Observatory Bulletin.
- (May 2010). "Accreted versus in situ Milky Way globular clusters". [[Monthly Notices of the Royal Astronomical Society]].
- (1992). "The mass and stellar content of the globular cluster M13". [[Astronomical Journal]].
- (2020). "The 83rd Name-List of Variable Stars. Variables in Globular Clusters and Novae". Peremennye Zvezdy (Variable Stars) 40, No. 8.
- (2007). "Illustrated Guide to Astronomical Wonders: From Novice to Master Observer". O'Reilly Media, Inc.
- O'Meara, Stephen James. (1998). "Deep-Sky Companions: The Messier Objects". Cambridge University Press.
::callout[type=info title="Wikipedia Source"] This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page. ::