Re: M27 and filters: It's the colors, Dumbbell!
Howard Ritter
The way to see a faint DSO the way you’d see it from much closer in space is to use an eyepiece that gives, with a given telescope, an exit pupil that matches your own fully dilated pupil, say 6 mm. If you look at the Orion Nebula through a 12” f/5 Dob with a 31mm TermiNagler eyepiece, the exit pupil will be 31mm/5 or ~6 mm and the magnification ~50x. Since its distance is ~1350 LY, it would appear in the EP as big as it would appear from 50 times closer, as it were, or ~27 LY. And because the exit pupil of the EP matches the entrance pupil of your eye, it appears to have exactly the same surface brightness in both situations – or, indeed, the same as it appears to your dark-adapted eye in a dark-sky location. Getting closer doesn’t make it look brighter, and neither does looking at it with optical aid. They both only make it look bigger, which exactly reciprocates the increase in total light gathered. No optical system can increase the perceived areal brightness of the scene it’s focused on compared to the naked-eye view. Pity!
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When people look at a closeup view of the Moon through a large scope with a large exit pupil and exclaim that it’s blindingly bright, remind them that it’s actually less bright than a beach scene on Earth, because of the lower albedo of moondust than of beach sand. It’s just that their eyes are dark-adapted and the Moon’s brightness is overwhelming under the circumstances. I think it’s fair to speak of the true color of DSOs, since their spectrum does indeed correspond to an actual perceived color, as we would see if it were many times brighter, like the way a piece of colored clothing appears to go from grey in the moonlight to blue when you go back in the house. If the multiple variables applying to a sensor and a monitor or a printer are selected to yield a depiction of the piece of clothing that we perceive to be true-color, then the same will yield a true-color depiction of a DSO. —howard
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