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Sky-Tonight.com / Nebulae / M37
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Observation Settings

Or select it on the map:
This Earth map fragment is intended to illustrate celestial motion across the sky, emphasizing both bearing and elevational perspectives. The map's center point corresponds to the transit, showcasing celestial objects at their highest point, while elevation gradually decreases towards the map edges. This dynamic representation offers insights into the changing positions of celestial bodies with a focus on their bearing and elevational trajectories.
Your location:
Timezone:
Latitude:
37.751
Longitude:
-97.822

M37 Observation Details

M37

M37 Daily Motion


M37 will become visible in August, 3. After being too close to the Sun to observe, it will reappear in the night sky. Starting from August, 3, M37 can be seen again, providing a good opportunity for observation.

M37 Visibility Timetable on May 09

M37 Rise and Set Timetable

TimeElevation
M37 transit16:1585°
Moon Rise, 87.7% illuminated17:0079°
Sunset20:2739°
Civil sunset20:5733°
Astrosession begin22:1020°
M37 set00:12
Astrosession end04:44-19°
Moon Set04:47-19°
M37 rise08:14

Track M37 Position Throughout the Night

← Fri, 9 May 2025 →

Elevation (degrees)
Time
Altitude
Azimuth
Shift the map to change the time and observe M37 changing position in the night sky.

M37 - Open Cluster

M37 is an open cluster located in the constellation Auriga. It was discovered by Giovanni Battista Hodierna before 1654 and independently by Charles Messier in 1764. The cluster is the richest and brightest of the three open clusters in Auriga (M36, M37, and M38).

M37 spans about 20 light-years across and contains around 500 stars. The cluster is approximately 4,500 light-years away from Earth and has an apparent magnitude of 6.2, making it visible with binoculars or a small telescope.

M37 Image Gallery

DSS Blue

M37 photo taken with blue filter
These images are valuable for highlighting the presence of younger, hotter stars, which emit more light in the blue wavelengths.

DSS Red

M37 photo taken with red filter
These images are excellent for detecting older, cooler stars, as well as emission nebulae, which glow primarily in the red due to hydrogen alpha emissions.

DSS Near-Infrared

M37 photo taken with Near-Infrared filter
These images can penetrate dust clouds that obscure visible light, revealing structures and objects hidden within.

DSS Composite image

M37 color image
DSS Color images are composite images created by combining the blue, red, and often near-infrared images to produce a full-color representation.

The photos are taken from the Digitized Sky Survey 2 (DSS2), which was produced at the Space Telescope Science Institute (STScI) under NASA contract, using data from the UK Science and Technology Facilities Council (STFC), the European Southern Observatory (ESO), and the National Geographic Society-Palomar Observatory Sky Survey (POSS II).

Special thanks to the National Optical Astronomy Observatory (NOAO), the Royal Observatory, Edinburgh, and the California Institute of Technology for their significant contributions.

Finder Chart for M37

Double-click to unlock the map.
Object nameM37
Field of view
Limiting magnitude
M37 coordinates5.87176, 32.553
Center coordinates5.87176, 32.553

M37 Passage Through Night

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Current position of M37

Time06:16
Latitude37.751
Longitude-97.822
M37 elevation-14°
M37 Azimuth-26°
Here you can see the current position of the M37 on the map, as well as its positions for rise and set. This tool allows you to track the M37's movement throughout the night, providing you with accurate and up-to-date information.

Annual motion of M37

Time
DateSat, 10 May 2025
Twighlight start22:07
Twighlight end04:38
Twighlight duration7h 31m
Rise08:10
Set00:05
Elevation at transit85°
Transit time16:07
Equatorial coordinatesRA: 05h 52m 18s", Dec: 32° 33' 10s
Magnitude6
ConstellationAuriga
The graph illustrates the annual visibility pattern of a M37, providing a comprehensive overview of its daily appearances and transit times throughout the year.
The graph is structured with the vertical axis showing the hours of the day, ranging from 12 AM to 12 AM the next day, while the horizontal axis spans each day of the year.
The reddish shaded area indicates the periods when the M37 is above the horizon, visible to observers. The white line marks the times when the celestial object reaches its highest point in the sky each day, known as the transit.

Data Credits

The nebulae information on this page is sourced from the OpenNGC project, developed by Matteo Verga. OpenNGC provides detailed data on the NGC catalog, which is a valuable resource for exploring deep-sky objects such as nebulae.

For more details or to contribute to OpenNGC, visit the official GitHub repository: OpenNGC on GitHub.