Small Sagittarius Star Cloud: Difference between revisions
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Messier described the cloud as "a large nebulosity in which there are many stars of different magnitudes" and gave its dimensions as being some 1.5° across. Some sources, improperly, identify M24 as the small [[open cluster]] [[NGC 6603]].<ref>{{cite web |url=http://www.messier.seds.org/m/m024.html |title=Messier 24 |access-date=21 July 2024 |website=SEDS Messier Catalog}}</ref> The location of the Small Sagittarius Star Cloud is near the [[Omega Nebula]] (also known as M17) and open cluster [[Messier 18]], both north of M24. | Messier described the cloud as "a large nebulosity in which there are many stars of different magnitudes" and gave its dimensions as being some 1.5° across. Some sources, improperly, identify M24 as the small [[open cluster]] [[NGC 6603]].<ref>{{cite web |url=http://www.messier.seds.org/m/m024.html |title=Messier 24 |access-date=21 July 2024 |website=SEDS Messier Catalog}}</ref> The location of the Small Sagittarius Star Cloud is near the [[Omega Nebula]] (also known as M17) and open cluster [[Messier 18]], both north of M24. | ||
Messier 24 is not a distinct [[deep-sky object]], rather an open window through the [[Great Rift (astronomy)|Great Rift]] into deeper regions of the [[Milky Way]] galaxy.<ref name=Harrington>{{Cite journal|last=Harrington|first=Phil|date=Jan 2022|title=The Small Sagittarius Star Cloud |journal=Astronomy |language=English|page=31}}</ref> It fills a space of significant volume to a depth of 10,000 to 15,000 light years away, including stars from the [[Scutum-Centaurus Arm]], the major [[spiral arm]] between | Messier 24 is not a distinct [[deep-sky object]], rather an open window through the [[Great Rift (astronomy)|Great Rift]] into deeper regions of the [[Milky Way]] galaxy.<ref name=Harrington>{{Cite journal|last=Harrington|first=Phil|date=Jan 2022|title=The Small Sagittarius Star Cloud |journal=Astronomy |language=English|page=31}}</ref> It fills a space of significant volume to a depth of 10,000 to 15,000 light years away, including stars from the [[Scutum-Centaurus Arm]], the major [[spiral arm]] between Earth and the [[Galactic Center]].<ref name=French/> The star cloud is the most dense concentration of individual stars visible using [[binoculars]], with around 1,000 stars visible within a single [[field of view]].<ref name=UT/> In [[telescopes]] it is best seen at low magnification, with a field of view of at least 2 degrees.<ref name=":0" /> Described as "a virtual carpet of stellar jewels", M24 is visible to the naked eye whenever the Milky Way itself is visible as well.<ref name=O'Meara/> | ||
The light of M24 is spread out over a large area, which makes estimating its brightness difficult. Older references give the star cloud's magnitude as 4.6, but more recent estimates place it a full two magnitudes brighter, at 2.5.<ref name=O'Meara/><ref name=French/> | The light of M24 is spread out over a large area, which makes estimating its brightness difficult. Older references give the star cloud's magnitude as 4.6, but more recent estimates place it a full two magnitudes brighter, at 2.5.<ref name=O'Meara/><ref name=French/> | ||
Latest revision as of 11:23, 7 June 2025
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The Small Sagittarius Star Cloud (also known as Messier 24 and IC 4715) is a star cloud in the constellation of Sagittarius approximately 600 light years wide, which was catalogued by Charles Messier in 1764. It should not be confused with the nearby Large Sagittarius Star Cloud which lies about 10° to the south.[1]
Messier described the cloud as "a large nebulosity in which there are many stars of different magnitudes" and gave its dimensions as being some 1.5° across. Some sources, improperly, identify M24 as the small open cluster NGC 6603.[2] The location of the Small Sagittarius Star Cloud is near the Omega Nebula (also known as M17) and open cluster Messier 18, both north of M24.
Messier 24 is not a distinct deep-sky object, rather an open window through the Great Rift into deeper regions of the Milky Way galaxy.[3] It fills a space of significant volume to a depth of 10,000 to 15,000 light years away, including stars from the Scutum-Centaurus Arm, the major spiral arm between Earth and the Galactic Center.[4] The star cloud is the most dense concentration of individual stars visible using binoculars, with around 1,000 stars visible within a single field of view.[5] In telescopes it is best seen at low magnification, with a field of view of at least 2 degrees.[6] Described as "a virtual carpet of stellar jewels", M24 is visible to the naked eye whenever the Milky Way itself is visible as well.[7]
The light of M24 is spread out over a large area, which makes estimating its brightness difficult. Older references give the star cloud's magnitude as 4.6, but more recent estimates place it a full two magnitudes brighter, at 2.5.[7][4]
HD 167356 is the brightest star within the Small Sagittarius Star Cloud, a white supergiant with an apparent magnitude of 6.05. This star is an Alpha-2 Canum Venaticorum variable, showing small changes in brightness as it rotates. There are three other stars in M24 with visual magnitudes between 6.5 and 7.0.[6]
The star cloud incorporates two prominent dark nebulae which are vast clouds of dense, obscuring interstellar dust. This dust blocks light from the more distant stars, which keeps them from being seen from Earth. Lying on the northwestern side is Barnard 92, which is the darker of the two. Within the star field, the nebula appears as an immense round hole devoid of stars. American astronomer Edward Emerson Barnard discovered this dark nebula in 1913.[6] Along the northeast side lies Barnard 93, as large as Barnard 92 though less obvious. There are also other dark nebulae within M24, including Barnard 304 and Barnard 307.[4][6]
The Small Sagittarius Star Cloud also contains two planetary nebulae, M 1-43 and NGC 6567. Messier 24 holds some similarities with NGC 206, a bright, large star cloud within the Andromeda Galaxy.[6]
See also
References
External links
- Finder Chart for Messier 24
- Messier 24, SEDS Messier pages
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Template:Sky Template:Messier objects
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