Hi Doug
I guess 2 main reasons for the sub length:
1. KAF8300 has relatively lowish well depth, and with the Newt it starts to saturate bright star within 2-3 mins (and there are some very bright stars in this field and nearby). 8" at F5 is a lot different to say F7 in a 4" refractor as you'd know.
2. Maths and object visibility - this was back in April and I only had an hour or two before Orion set, so I roughly tried split my time 50:50 Lum and RGB then get enough of each filter to have at least 4 images (less than that and you don't get effect noise control during sub integration regardless of sub length I find).
Hopefully I'll soon be able to get back into imaging Orion in more detail if work and weather conspire correctly