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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: Columbus, United States
Timezone:
Latitude:
39.9625
Longitude:
-83.0061

Dumbbell Nebula (M27) Observation Details

M27

M27 Daily Motion

M27 will rise at 22:56, during twilight, and will ascend to 68° by the time twilight ends at 05:14.
M27 will be visible until January, 2, when it will move too close to the Sun. During this time, its proximity to the Sun will cause it to disappear from the night sky, making it unobservable for a while.

M27 Visibility Timetable on May 10

M27 Rise and Set Timetable

TimeElevation
Moon Rise, 93.2% illuminated17:59-27°
Astrosession begin22:22-5°
M27 rise22:56
Astrosession end04:3362°
Moon Set05:0567°
Civil sunrise05:5172°
M27 transit06:1773°
Sunrise06:2273°

Track M27 Position Throughout the Night

← Sat, 10 May 2025 →

Elevation (degrees)
Time
Altitude
Azimuth
Shift the map to change the time and observe M27 changing position in the night sky.

M27 - Dumbbell Nebula

The Dumbbell Nebula (M27) is a planetary nebula located in the constellation Vulpecula. It was discovered by Charles Messier in 1764. M27 is one of the largest and brightest planetary nebulae known.

M27 spans about 3 light-years across and is illuminated by a hot, central white dwarf star. The nebula is approximately 1,360 light-years away from Earth and has an apparent magnitude of 7.5, making it visible with binoculars or a small telescope.

M27 Image Gallery

DSS Blue

M27 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

M27 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

M27 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

M27 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 M27

Double-click to unlock the map.
Object nameM27
Field of view
Limiting magnitude
M27 coordinates19.99344, 22.72103
Center coordinates19.99344, 22.72103

M27 Passage Through Night

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Current position of M27

Time14:26
Latitude39.9625
Longitude-83.0061
M27 elevation-7°
M27 Azimuth52°
Here you can see the current position of the M27 on the map, as well as its positions for rise and set. This tool allows you to track the M27's movement throughout the night, providing you with accurate and up-to-date information.

Annual motion of M27

Time
DateSat, 10 May 2025
Twighlight start22:18
Twighlight end04:28
Twighlight duration6h 10m
Rise22:56
Set13:38
Elevation at transit73°
Transit time06:17
Equatorial coordinatesRA: 19h 59m 36s", Dec: 22° 43' 15s
Magnitude7
ConstellationVulpecula
The graph illustrates the annual visibility pattern of a M27, 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 M27 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.