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Astronomical spectroscopy began with
Isaac Newton's initial observations of the light of the Sun, dispersed
by a prism. He saw a rainbow of color, and may even have seen
absorption lines. These dark bands which appear throughout the solar
spectrum were first described in detail by Joseph von Fraunhofer. Most
stellar spectra share these two dominant features of the Sun's
spectrum: emission at all wavelengths across the optical spectrum (the
continuum) with many discrete absorption lines, resulting from gaps of
radiation.

Astronomical spectroscopy
provides a way to analyze the star’s chemical composition, temperature
and its radial velocity. Spectroscopy is the analysis of star light
dispersed according to its wavelength. This light dispersion is called
a spectrum and it is displayed as white streaks or color streaks in an
image.
A
common example of a spectrum that most people have seen is a
rainbow that is created by the Sun and the rain.
David’s presentation starts with an overview of the basics types
of spectrums.
He will show you how to build a
simple solar spectroscope that shows that the Sun’s photosphere is
composed of hydrogen, sodium and magnesium. A moderate resolution
spectrum of the Moon and planets are analyzed next.
Moving father from Earth an
introduction to spectral classification is covered with examples
of standard spectral type stars taken with a simple grating
filter. Also, the spectrum of stars is compared to a nebula
spectrum.
Finally an image like the one on
the right will be analyzed showing unique objects such a very cool
temperature infrared star and the redshift spectrum of a Quasar
that is 3.269 billion light years away |
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David
Haworth enjoys astronomy, astrophotography and processing images to
bring out details that cannot be seen by visual observing. David
started in astrophotography in 1996 and he has used a variety of
cameras to image the sky.
David wrote "Afocal Photography with
Digital Cameras" chapter in the second edition of "The Art and Science
of CCD Astronomy" book and "Flat Field Calibration using an LCD
Monitor" article in AstroPhoto Insight magazine. David's images have
appeared on a magazine front cover, in magazine articles, a book front
cover, in books, in catalogs, in videos, on posters, on music CD
covers, on T-shirts, on wine bottles and on a variety of web sites.
Recently, David has been using
spectroscopes to analyze the light from celestial objects that range
from the Sun to distant Quasars that are billions of light years from
us.
More information available at
http://www.stargazing.net/david/spectroscopy/index.html
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