When to photograph M 50
M 50 is an open cluster in Monoceros, 14′ across at magnitude 5.9. Also listed as NGC 2323.
When to photograph it
From 45° N the best months are November to February, with up to 4.0 hours of astronomical darkness above 30° in January. It reaches 37° at its highest.
From 35° S the best months are December and January, with up to 6.3 hours of astronomical darkness above 30° in January. It reaches 63° at its highest.
Framing
Its long axis is 14′. It fills 35 to 80% of the short side of an APS-C sensor at about 1330 to 3040 mm, and of a full-frame sensor at about 2050 to 4680 mm.
Filters and the moon
Clusters are broadband targets, but bright ones tolerate some moonlight and light pollution. Short subs keep the brightest stars from clipping. The dark sky calendar shows which nights this month are moon-free where you are.
Plan it for tonight
Dates and times depend on your exact location. The imaging planner shows M 50's altitude through tonight, its transit time and its distance from the moon. For sub length, use the exposure calculator.
Nearby targets
- IC 2177 Seagull Nebula 2.2° away
- NGC 2359 Thor's Helmet 6.2° away
- NGC 2360 Caroline's Cluster 8.2° away
- M 47 10.3° away
- M 46 11.5° away
- M 41 13.0° away
Gear that suits M 50
M 50 is 14′ along its long axis. These frame it on an APS-C sensor with room to crop.
- Celestron C8 OTA 2032 mm f/10: fills 53% of an APS-C frame's short side View at High Point Scientific
- Celestron EdgeHD 8 OTA 2032 mm f/10: fills 53% of an APS-C frame's short side View at High Point Scientific
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