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M77
spiral galaxy in Cetus
M77 is a barred spiral in Cetus with a very bright, active nucleus, making it a Seyfert galaxy. Its bright core shines even through some light pollution, and the tightly wound arms surround it.

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// Key facts
- Catalog
- M77
- Type
- spiral galaxy
- Constellation
- Cetus
- Size
- 7′ across
- Brightness
- Magnitude 8.9
- Distance
- about 47 million light-years
- Peak month (any location)
- Oct
- Typical prime months
- Aug to Jan
- Difficulty
- Intermediate
- Filter
- No filter (broadband); a light-pollution filter is optional
Pick a saved location or share your device location. Your coordinates are used only to calculate tonight and are not stored. To save locations, use the planner.
How to image M77
- At 7 arcminutes, use 1,200 to 2,000 mm.
- The bright core can clip, so blend in short exposures to preserve detail.
- It is best in autumn and early winter evenings.
Framing: what focal length?
M77 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 length | Share of the frame width |
|---|---|
| 1,000 mm | about 9% |
| 2,000 mm | about 17% |
| 3,000 mm | about 26% |
How high does it climb from your latitude?
The highest point M77 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.
| Latitude | Highest point | Rating |
|---|---|---|
| 55°N (Scotland, Alaska) | 35° | Workable |
| 45°N (Minneapolis, Milan) | 45° | Workable |
| 35°N (Los Angeles, Tokyo) | 55° | Workable |
| 25°N (Miami, Cairo) | 65° | High in the sky |
| 35°S (Sydney, Santiago) | 55° | Workable |
Also worth imaging
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