The Sperling Files:
Overexposures for Discovery and Fame
Norman Sperling
(c) 2002 Norman Sperling. Excerpted with
permission from "What Your Astronomy Textbook Won't Tell
You" (ISBN 0-913399-04-3).
Imaging technology is rapidly improving and
cheapening. From current astrophotography guides, determine
“recommended” exposures for accessible deep-sky objects. Then
take time exposures that are many times longer than the recommended
amount - up to the sky-fogging limit. That should grossly
overexpose the inner parts, but what will you discover beyond
them?
This may reveal new structures, some of which
have different shapes than the brighter components. Some may
show nothing new - itself noteworthy. And all the ones that
do show something new are worth drawing scholarly attention
to. Please send me a copy of any interesting results.
Tony and Daphne Hallas photographed M57,
showing a larger loop of faint old gas beyond the Ring. Their
photo of part of M13 shows gazillions of stars all the way
out to the edge of the photo, and presumably beyond.
Now apply the same technique to elliptical
galaxies. Some galaxies presently catalogued as ellipticals
may actually be the bulges of disc galaxies, whose discs have
not yet been noticed.
I suspect that at least one will reveal a
hint of a Population I disc outside the elliptical (= bulge),
showing that that galaxy is really spiral rather than elliptical.
Important discoveries await serious amateur
astronomers. All it takes is really deep overexposures.
Norm Sperling is editor of The
Journal of Irreproducible Results. Previously he was
assistant editor of Sky & Telescope magazine
and Science Editor at AltaVista.com. Norm teaches astronomy
in universities around San Francisco, wrote the new book "What
Your Astronomy Textbook Won't Tell You," and co-designed Edmund
Scientific's Astroscan telescope. 
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