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Sharing The Mystery & Grandeur Of Our Universe
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"NightFall"
, a monthly newsletter for the Huachuca Astronomy Club |
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Two photos taken on the evening of July 17, 2001 during a 'lull' in the summer monsoon. They were taken here in Palominas with a 35mm camera mounted on a telescope so that the camera 'tracked' the stars as the Earth rotated. Each photo is a 15 minute exposure of two different areas of our Milky Way. The top photo is looking south towards Sagittarius (the larger pink region at lower center is the Lagoon Nebula), and the bottom one is part of the constellation Cygnus (the larger pinkish region in this photo shows the North American Nebula). Star Haven Observatory is always looking up! |
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This is a digital image taken on the evening of December 5, 2001 showing a comet with the 'name' of C/2000 WM1 (Linear). At this time, it was in the constellation Cetus, and heading south pretty fast. It briefly became visible with the naked eye. The camera was following the comet, so stars 'trailed'. |
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In this photo, there was no 'star-guiding'. The camera was pointed north, and as the Earth rotates (in this photo, 11 minutes), the stars left this trail of the Earth's movement. The camera did catch a meteor streaking through the north sky. The one star that doesn't appear to rotate is the North Star. |
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Here is another view that shows the Earth's rotation over a 30 minute period. Again, the star near the top that does not show any rotation effect is Polaris, the north star. The observatory is being lit by a soft red light while this exposure was being made. There is considerable light pollution showing up above the observatory because of all the *$%##@** unshielded lights in Sierra Vista and Hereford. What an unnecessary waste of energy, and killing the view of our night sky across the country. |
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One example of our monsoon weather - a
lightning strike and downpour quite close to the observatory. This is a
common occurrence during the summer here in SE Arizona.
More SKY photos are shown on this linked page. |
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Looking northward from slightly above the observatory. In this picture the roof is shown 'rolled' off to the north so that the interior of the observatory is open to the sky. The 20 inch reflecting telescope is in the center and the southern wall 'flap' allows better views to the southern horizon. The observatory is a 20 ft by 25 ft roll-off roof type observatory, and 100 sq. ft of this is designed to be a 'warm room'. The walls are 6 ft. high, and the floor is carpeted concrete. |
Palominas Observatory is located at 110º 08' 27.4" West, +31º 24' 1.6"N, at an elevation of 4,310 feet in the community of Palominas, Arizona (southeastern corner of the state).
For the following series of 'thumbnail' photos, click on the image to view a larger photo.
The observatory was designed by its owner, Doug Snyder, who also assisted in the construction, which was contracted to Stellar Vision in Tucson, Arizona. Construction was started on June 8, 2000, and completed on February 4, 2001. This place is a real blast! The design consideration to use a roll-off roof style building instead of a domed building came about because roll-off's are easier to construct, the view of the sky from inside the observatory is much greater when the roof is opened, and heat dissipation is much faster in most cases compared to using a dome.
The observatory presently houses
three telescopes, the main instrument being a 20 inch reflecting telescope, made
by Obsession Telescopes in Wisconsin. The 20 inch diameter highly polished
mirror, which is about 2" thick, was ground, figured, polished, and coated
in Colorado. This telescope is being used for visual observations, but in the
future will also be used for digital photography.
A second telescope, being of the Schmidt-Cassegrain type, is currently used for
both visual and digital imaging of objects such as galaxies, globular clusters,
planetary nebulae, bright nebulae, and all sorts of neat stuff found in our
skies. This is a 14" (inch) Meade LX200, and the f-ratio is f/10,
although it can be converted to an f/5 system (giving a larger field of
view). Attached to this telescope is a digital camera built for astronomy
(a CCD camera); the light sensitivity of this telescope/camera combination is
such that it captures much more light from distant objects and displays the
object on a computer screen with more detail than can be seen through the human
eyes when looking at the same object in the 20" telescope.
The remaining telescope is an 8" Dobsonian, similar to the 20", but
with far less light gathering power. We don't rate telescopes on how much
they can magnify, but by how much light they can gather. Telescopes with
larger mirrors (reflecting types) or lenses (refracting types) collect more
light than their smaller counterparts. Magnification can be changed
(50x, 100x, 400x, etc) by using different sized 'eyepieces', but the light
gathering capability is fixed by the size of the mirror or lens.
Inside the observatory, there are two rooms - the main observing area, and a smaller insulated room called the 'warm room'. This room includes the library, storage area, and control center for the Meade LX200 10" telescope, which can be operated remotely from a warm environment during cold winter nights. There is also a small refrigerator and microwave, but alas, no indoor plumbing. Two windows in this room allow views to the west and into the observing area.
Have any sky watching or
astronomy questions? Feel free to ask us at info@palominas.com.
Please Remember This: Stars Up, Lights Down (Thank You!)
Doug & Jean Snyder
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For information about, or comments on this website,
please email
starhaven@palominas.com
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