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Great Pegasus Cluster (M15)

globular cluster in Pegasus

M15 is one of the densest globular clusters known. Its core has collapsed into an extremely tight concentration of stars, and it is one of the few globulars known to contain a planetary nebula, Pease 1. It is bright and easy to find in Pegasus, and well placed in the autumn evening sky.

Photograph of Great Pegasus Cluster (M15), a globular cluster in Pegasus
Photo: Credit: NASA, ESA (resized) · CC BY 3.0 · Wikimedia Commons
M15 · 18′10′

Save your telescope or lens on the planner to lay your camera frame over this diagram.

Approximate size and shape, drawn to scale. Not a photograph.

// Key facts

Catalog
M15
Type
globular cluster
Constellation
Pegasus
Size
18′ across
Brightness
Magnitude 6.2
Distance
about 33,600 light-years
Peak month (any location)
Aug
Typical prime months
May to Oct
Difficulty
Beginner
Filter
No filter (broadband)
// For your location

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How to image Great Pegasus Cluster

Framing: what focal length?

M15 is small, so a "60% of the frame" focal length would be impractical. Here is how much of an APS-C frame it covers at common long focal lengths; expect to crop.

Focal lengthShare of the frame width
1,000 mmabout 22%
2,000 mmabout 45%
3,000 mmabout 67%

How high does it climb from your latitude?

The highest point M15 reaches in the sky. Above about 60° is excellent, 30° to 60° is workable, and under 30° you are looking through a lot of air.

LatitudeHighest pointRating
55°N (Scotland, Alaska)47°Workable
45°N (Minneapolis, Milan)57°Workable
35°N (Los Angeles, Tokyo)67°High in the sky
25°N (Miami, Cairo)77°High in the sky
35°S (Sydney, Santiago)43°Workable

Also worth imaging

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