M101

 Posted: Jan 25th, 2026
Technical Info
Telescope/Lens: Sky-Watcher 150/750
Camera: ZWO ASI533MC Pro
Mount: Juwei 17
Guide Scope: ZWO OAG
Guide Camera: ZWO ASI220MM
Software: Siril
Accessories: Baader MPCC
Exposure:
134 x 90" ISO/Gain: 101 - SVBONY UV/IR Cut
White, Bortle 8/9 zone:
 Tokyo, Japan
 Jan 25th, 2026
3 h 21 m
95
Resolution: 2817x2848 px
Scale: 4585 KB
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Comments

Are 90-second sub-exposures too long for this level of light pollution?
26 Jan, 2026 Reply
Ananas Replied to Yas
It's hard to say. For bright objects, like Orion or Andromeda, 60 is definitely the upper limit. For fainter ones, like this, it looks optimal.
27 Jan, 2026 Reply
Yas Replied to Ananas
The issue isn't overexposure of bright objects, but rather that under such conditions the sky background will be very high, causing faint objects to be lost.
27 Jan, 2026 Reply
Ananas Replied to Yas
Makes sense, I'll have to experiment with it.
27 Jan, 2026 Reply
Yas Replied to Ananas
If you use NINA, you can immediately determine the maximum exposure time for your conditions.
27 Jan, 2026 Reply
Ananas Replied to Yas
I checked the histogram of the raw frames: in the evening, the exposure was clearly too long, yes. But by midnight, it already looks reasonable—10–15% from the left edge.
27 Jan, 2026 Reply
Yas Replied to Ananas
The histogram doesn't tell you much. If you're comfortable with math, check out https://forums.sharpcap.co.uk/viewtopic.php?t=456. If not, here's a quick summary: you need to know: 1. The average bias for your camera settings, 2. The average background level for a given sub-exposure, 3. The camera read noise, 4. The conversion factor for your camera settings in e-/ADU. Recommended Exposure Time = 10 × (read noise)² / light pollution rate where light pollution rate is defined as: (median ADU of a subframe − median bias) × electrons per ADU / exposure length
27 Jan, 2026 Reply

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