Messier objects, taken and compiled by an amateur astronomer
|Survey type||astronomical catalog|
|Target||nebula, planetary nebula, open cluster, globular cluster, galaxy|
|Named after||Charles Messier|
|Related media on Wikimedia Commons|
The Messier objects are a set of over 100 astronomical objects first listed by French astronomer Charles Messier in 1771. Messier was a comet hunter, and was frustrated by objects which resembled but were not comets, so he compiled a list of them, in collaboration with his assistant Pierre Méchain, to avoid wasting time on them. The number of objects in the lists he published reached 103, but a few more thought to have been observed by Messier have been added by other astronomers over the years.
Lists and editions
The first edition covered 45 objects numbered M1 to M45. The total list published by Messier finally contained 103 objects, but the list was expanded through successive additions by other astronomers, motivated by notes in Messier’s and Mechain’s texts indicating that at least one of them knew of the additional objects. The first such addition came from Nicolas Camille Flammarion in 1921, who added Messier 104 after finding a note Messier made in a copy of the 1781 edition of the catalogue. M105 to M107 were added by Helen Sawyer Hogg in 1947, M108 and M109 by Owen Gingerich in 1960, and M110 by Kenneth Glyn Jones in 1967. M102 was observed by Méchain, who communicated his notes to Messier. Méchain later concluded that this object was simply a re-observation of M101, though some sources suggest that the object Méchain observed was the galaxy NGC 5866 and identify that as M102.
Messier lived and did his astronomical work at the Hôtel de Cluny (now the Musée national du Moyen Âge), in France. The list he compiled contains only objects found in the sky area he could observe: from the north celestial pole to a celestial latitude of about −35.7°. He did not observe or list objects visible only from farther south, such as the Large and Small Magellanic Clouds.
The Messier catalogue comprises nearly all the most spectacular examples of the five types of deep sky object – diffuse nebulae, planetary nebulae, open clusters, globular clusters, and galaxies – visible from European latitudes. Furthermore, almost all of the Messier objects are among the closest to our planet in their respective classes, which makes them heavily studied with professional class instruments that today can resolve very small and visually spectacular details in them. A summary of the astrophysics of each Messier object can be found in the Concise Catalog of Deep-sky Objects.
Since these objects could be observed visually with the relatively small-aperture refracting telescope (approximately 100 mm, or four inches) used by Messier to study the sky, they are among the brightest and therefore most attractive astronomical objects (popularly called "deep sky objects") observable from Earth, and are popular targets for visual study and photography available to modern amateur astronomers using larger aperture equipment. In early spring, astronomers sometimes gather for "Messier marathons", when all of the objects can be viewed over a single night.
- List of Messier objects
- Category:Messier objects
- Deep sky object
- New General Catalogue
- Herschel 400 Catalogue
- Caldwell catalogue
- "Charles Messier's Catalog of Nebulae and Star Clusters". SEDS. 12 August 2011. Retrieved 2014-05-17.
- "The Messier Catalog". SEDS Messier Database. SEDS. 25 February 2008. Retrieved 2010-05-08.
- Birthday of a star cluster, Astronomy Now, January 2011, page 20.
- Patrick Moore (1979). The Guinness Book of Astronomy. Guinness Superlatives. ISBN 0-900424-76-1.
- Charles Messier (1781). "Catalogue des Nébuleuses & des amas d'Étoiles". Connaissance des Temps for 1784. pp. 227–267.
- "Original Messier Catalog of 1781". Original Messier Catalog of 1781. SEDS. Retrieved 2014-05-17.
- W.H. Finlay (2003). Concise Catalog of Deep-sky Objects: Astrophysical Information for 500 Galaxies. Springer. ISBN 1-85233-691-9.
- "The Messier Marathon". SEDS. 19 March 2013. Retrieved 2014-05-17.