Small Sagittarius Star Cloud
| Messier 24 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Right ascension | 18h 17m |
| Declination | −18° 29′ |
| Distance | ~10 kly (3070 Pc) |
| Apparent magnitude (V) | 4.6 |
| Apparent dimensions (V) | 90′ |
| Physical characteristics | |
| Radius | ~300 |
| Estimated age | 220 million years[citation needed] |
| Other designations | Delle Caustiche, IC 4715 |
| Associations | |
| Constellation | Sagittarius |
The Sagittarius Star Cloud (also known as Delle Caustiche, Messier 24, IC 4715) is a star cloud in the constellation of Sagittarius, approximately 600 light years wide, which was discovered by Charles Messier in 1764. It is sometimes known as the Small Sagittarius Star Cloud to distinguish it from the Great Sagittarius Star Cloud located to the north of Gamma Sagittarii and Delta Sagittarii.[1]
The stars, clusters and other objects comprising M24 are part of the Sagittarius or Sagittarius-Carina arms of the Milky Way galaxy. Messier described M24 as a "large nebulosity containing many stars" and gave its dimensions as being some 1.5° across. Some sources, improperly, identify M24 as the faint cluster NGC 6603.
M24 fills a space of significant volume to a depth of 10,000 to 16,000 light-years. This is the most dense concentration of individual stars visible using binoculars, with around 1,000 stars visible within a single field of view.
See also
References
- ^ Crossen, Craig; Rhemann, Gerald (2004). Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes. Springer. ISBN 3211008519Template:Inconsistent citations
{{cite book}}: CS1 maint: postscript (link)
External links
- Messier 24, SEDS Messier pages
- Merrifield, Michael. "M24 – Sagittarius Star Cloud". Deep Sky Videos. Brady Haran.
- The Sagittarius Star Cloud on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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