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Big Bend Astronomical Society, Inc. August/September, 1999 Jim Walker, Editor |
Please Note
THIS NEWSLETTER covers the months of August and September. Because I was away most of August, I couldn’t do a regular Newsletter for that month, hence the present coverage of two months. Once again I thank Bernie Zelazny for taking the minutes at the August meeting.
Jim Walker, Secretary
| Minutes of the 11 August 1999 BBAS Meeting |
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The meeting was called to order by President Bill Baker at 19:36:49 CDT.
The minutes from the previous meeting were accepted by acclamation.
| Treasurer
Betty Grimm presented the following written report:
Working balance June 30, 1999
$194.66
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Opened 09/25/98 Savings balance June 30, 1999
$1,071.82
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CD 1/19/99
$935.32
CD 5/18/99
$2,952.79
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Old Business: The Meteor Shower party was discussed. No one in attendance indicated that they planned to go to Double Diamond Pavilion to view the meteor shower.
Star Party Report by Bill Baker: The 19 August 1999 Star Party for SRSU Student Government attracted 20-25 participants. The event was held in the parking area behind the Outdoor Amphitheatre at Kokernot Park.
New Business: Bill Baker suggested we determine a set fee for future Student Group Star Parties. After a brief discussion Terry Eakens made a motion to charge $2.50 per person. Zelazny seconded. The motion passed unanimously.
Bernie Zelazny suggested that BBAS earmark all funds collected from Star Parties for the Murray Newman fund. After a brief discussion, Zelazny made a motion to earmark 50% of such receipts for the Murray Newman fund and the balance for the BBAS General Fund. Betty Grimm seconded the motion. The motion passed with 4 yeas, 2 nays and 1 abstention.
Bill Baker asked for volunteers to serve on the Nomination Committee. Judith Brueske-Plimmer volunteered with the understanding that she would not be the only person on the committee. No one else in attendance who was eligible came forward. Several possible members for the committee were discussed. Bill Baker would contact potential Committee members.
The meeting adjourned at 20:09 CDT.
Respectfully submitted,
Bernie Zelazny, VP and Secretary Pro Tem
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The president appointed an Election Committee consisting of Judy Brueske-Plimmer and Bernie Zelazny, Chair. A third member of the committee is yet to be appointed.
Bill reported that a star party held for participants in the Sul Ross Pass Program for incoming freshmen has yielded $50.00 for the BBAS, and another for the Student Advisory Board Delegates has yielded $62.50. Checks will be forthcoming.
Our program was a presentation by Doug McCombs gave on the General Principles of Telescopes (see below).
Respectfully submitted,
Jim Walker, Secretary
| Treasurer
Betty Grimm presented the following written report:
Working balance July 31, 1999
$144.66
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Opened 09/25/98 Savings balance August 31, 1999 $771.82 |
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CD 1/19/99 $945.87 CD 5/18/99
$2,952.79
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Another Example of Combination Optics:
The Mersenne Telescope
This note is
a review of a major article in the September issue of Sky & Telescope,
pp. 130-133, by Clyde Bone, a BBAS member since our inception. The
article is well illustrated with photos by the author and a diagram of
the optics. Unfortunately for us, Clyde lives in San Angelo, so we
have not seen him as often as we would like. In any case, congratulations,
Clyde! (By the way, Doug McCombs is another BBASer with an S &
T article, published a few years ago on his 10-inch binocular scope.)
Marin Mersenne,
a French mathematician first proposed this design for a reflecting telescope
in 1636. The design uses a concave parabolic primary mirror and a
convex parabolic secondary. [Because of the difficulty of grinding these
surfaces, no such telescope was ever made until long after Newtonian reflectors
became common.] Clyde has made two Mersenne scopes, a 20-inch and
a 30-inch. In addition to the reflective optics, the 20-inch uses
a 4-inch refractor at the eyepiece end of the scope, and the 30-inch uses
a 5.5-inch refractor. A principal advantage of the Mersenne design is the
fact that the eyepiece remains at a constant, comfortable height for a
seated observer independent of where the scope is pointing. Anyone
who has ever climbed a tall ladder in the dark at the Texas Star Party
to look through a 30-inch monster Dob, or larger, can surely appreciate
the accessibility of the eyepiece in Clyde’s design.
Barbara and
I watched the last total solar eclipse of this millennium from a point
near Lizard Head, the southernmost point in England. The line of
totality came ashore from the Atlantic near Land’s End, the extreme southwest
of England, near the city of Penzance. The path of totality swept
across southern Cornwall, leaving the coast south of Plymouth, crossing
the English Channel, and then crossing central Europe into the Black Sea,
Turkey, and continuing across India.
The weather
outlook was not good. Before we left, we knew the climatologic history
gave us only a 45% chance of seeing the eclipse where we were headed.
But we were going to Great Britain anyway, so we took our chances.
We camped
out the night before the eclipse. The night was mostly clear, offering
good views of the sky. We even saw a few Perseids. After years
of looking at Polaris 30 deg above the horizon at home, it was fascinating
to see it up nearly 50 deg. All of England is north of the 49th parallel,
which is the north line of the US. Even so, the climate is mild enough
for palm trees to grow along the coast in the south of Cornwall, thanks
to the Gulf Stream.
It was cloudy
the morning of August 11, the day of the eclipse. We considered driving
somewhere else, but decided to stay put. Good thing, because two
or three minutes before totality, a hole in the clouds opened up.
We were able to see all of totality, a little over two minutes in our area.
We could see the corona very well, and even some solar prominences.
But our hole in the clouds was too small to show us Mercury and Venus,
about 10 and 15 deg away from the sun. Oh well, we saw those
planets plus Jupiter during the longer eclipse last year in the Pacific.
We were among
the merest handful of people in Great Britain who saw totality. The
weather was clear in northern Scotland, but totality was confined to southern
England.
As we drove
northward across England, Wales, and Scotland, we saw more and more of
the northern sky. The latitude at the little town of John o’Groats
on the northern tip of Scotland is about 58.5 deg, so Polaris is nearly
twice as high as at home – and it looks even higher.
We drove 3,400
miles in three weeks, touching all the geographic extremes on the mainland
of Great Britain, plus ferry trips to the Orkney Islands and the Outer
Hebrides. We found the northwest coast of Scotland especially delightful
– great scenery, great salmon and trout, and a thinly populated countryside.
REGULAR MEETING:
Wednesday, October 13, at 7:30 PM.
Doug McCombs will give the 2nd half of his presentation
on telescopes on
Grinding and Polishing Mirrors in
Room 204 of the ACR Center.
STAR PARTY
Saturday October 9, 7:45 PM
(sun sets at 7:52)
at Jim & Barbara Walker’s,
364-2467. No potluck until next month.
ALTERNATE STAR PARTY DATE
Sunday, October 10
Please note: There will be no potluck suppers until November.
Please call or e-mail Bernie Zelazny at 837-1717 if you need further information.
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It's that time of year again. Dues for 1999 are now payable. If you have not yet paid your dues
for this year please send a check to
Our dues are still $20.00 per year
payable on a calendar-year basis,
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