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Crab Nebula (M1)

supernova remnant in Taurus

The Crab Nebula is the remains of a star that exploded in the year 1054, recorded by astronomers in China and elsewhere. At its center sits a pulsar spinning about thirty times a second. The nebula is small but bright, with a network of fine filaments around a smooth blue glow.

Photograph of Crab Nebula (M1), a supernova remnant in Taurus
Photo: NASA , ESA , J. Hester and A. Loll (Arizona State University) · Public domain · Wikimedia Commons
M1 · 6′2′

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
M1
Type
supernova remnant
Constellation
Taurus
Size
6′ across
Brightness
Magnitude 8.4
Distance
about 6,500 light-years
Peak month (any location)
Dec
Typical prime months
Sep to Feb
Difficulty
Intermediate
Filter
OIII + Ha narrowband, or a UHC filter
// For your location

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How to image Crab Nebula

Framing: what focal length?

M1 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 7%
2,000 mmabout 15%
3,000 mmabout 22%

How high does it climb from your latitude?

The highest point M1 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)57°Workable
45°N (Minneapolis, Milan)67°High in the sky
35°N (Los Angeles, Tokyo)77°High in the sky
25°N (Miami, Cairo)87°High in the sky
35°S (Sydney, Santiago)33°Workable

Also worth imaging

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