Messier Objects Tonight
Messier objects are a set of 110 astronomical objects cataloged by the French astronomer Charles Messier in the 18th century. These objects include a variety of celestial phenomena such as star clusters, nebulae, and galaxies. The catalog was created to help astronomers distinguish between permanent and transient objects in the night sky. Some of the most famous Messier objects include the Andromeda Galaxy (M31), the Orion Nebula (M42), and the Pleiades star cluster (M45). The Messier Catalog remains a popular reference for amateur and professional astronomers alike.Sky Map
Celestial bearing and elevation at 21:29
This interactive sky map shows the positions of the brightest celestial objects from your location. Move it horizontally to follow how their positions change through the night.
M44
Open Cluster
The Beehive Cluster, an open star cluster containing over 1,000 stars, located approximately 577 light-years away in the constellation Cancer.
Orion Nebula (M42)
Star cluster + Nebula
The Orion Nebula, a bright emission nebula and star-forming region, containing over 700 stars, located approximately 1,344 light-years away in the constellation Orion.
M39
Open Cluster
An open star cluster containing approximately 30 stars, located approximately 800 light-years away in the constellation Cygnus.
M35
Open Cluster
An open star cluster containing over 1200 stars, located approximately 2,800 light-years away in the constellation Gemini.
M34
Open Cluster
An open star cluster containing over 400 stars, located approximately 1,400 light-years away in the constellation Perseus.
M37
Open Cluster
A rich open star cluster containing over 500 stars, located approximately 4,500 light-years away in the constellation Auriga.
M48
Open Cluster
An open star cluster containing over 200 stars, located approximately 1,500 light-years away in the constellation Hydra.
M50
Open Cluster
An open star cluster containing over 200 stars, located approximately 3,000 light-years away in the constellation Monoceros.
M36
Open Cluster
An open star cluster containing over 60 stars, visible to the naked eye under dark skies, located approximately 4,100 light-years away in the constellation Auriga.
M71
Globular Cluster
A loose globular cluster containing tens of thousands of stars, located approximately 12,000 light-years away in the constellation Sagitta.
M2
Globular Cluster
A globular cluster containing hundreds of thousands of stars, located approximately 55,000 light-years away.
M15
Globular Cluster
A dense globular cluster containing hundreds of thousands of stars, located in the constellation Pegasus, approximately 33,600 light-years away.
M38
Open Cluster
An open star cluster containing over 100 stars, located approximately 4,200 light-years away in the constellation Auriga.
M92
Globular Cluster
Globular cluster one of the oldest clusters known, contains high metallicity stars.
M29
Open Cluster
An open star cluster containing over 400 stars, part of the Cygnus OB1 association, located approximately 4,000 light-years away.
M67
Open Cluster
An open star cluster containing over 500 stars, located approximately 2,800 light-years away in the constellation Cancer.
M52
Open Cluster
An open star cluster containing over 200 stars, located approximately 5,000 light-years away in the constellation Cassiopeia.
M103
Open Cluster
M103 is an open cluster with apparent magnitude 7.40 in the constellation Cassiopeia, spanning approximately 4.5 arcseconds in the sky.
M56
Globular Cluster
A globular cluster containing tens of thousands of stars, located approximately 32,900 light-years away in the constellation Lyra.
M73
Association of stars
An asterism consisting of four stars, located approximately 2,500 light-years away in the constellation Aquarius.
Data Credits
The deep-sky information on this page comes from the OpenNGC project developed by Matteo Verga. OpenNGC provides detailed catalog data for nebulae, galaxies, clusters and other deep-sky objects.
For details or contributions, visit the official repository: OpenNGC GitHub.



















