Newsletter of the
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
by Bernie Zelazny
Eleven folks attended the meeting at the SRSU Planetarium. The group was comprised of 10 BBAS members and 1 non-member.

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
July receipts                    300.00
July Disbursements               350.00
Working balance July 31, 1999    $144.66

First National Bank in Alpine Savings Account
Opened 09/25/98

Savings balance June 30, 1999   $1,071.82
July Disbursements                 300.00
Savings balance July 31, 1999     $771.82

Newman Fund CDs

CD 1/19/99                $935.32
July interest               10.55
                          $945.87

CD 5/18/99              $2,952.79
                        =========
Balance July 31, 1999   $3,898.66

Bernie Zelazny gave a brief BBAS web site report (see Bernie for a copy).

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


Minutes of the September 8, 1999, Meeting
by Jim Walker
The meeting was called to order at 7:30 PM by President Bill Baker.  There were 14 people present.

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
August receipts                        0
August disbursements                   0
Working balance August 31, 1999  $144.66

First National Bank in Alpine Savings Account
Opened 09/25/98

Savings balance August 31, 1999  $771.82

Newman Fund CDs

CD 1/19/99                  $945.87

CD 5/18/99                $2,952.79
Interest 8/18/99              32.93
                          $2,985.72
                           ========
Balance August 31, 1999   $3,931.59


¡News Flash!
        It’s now officially Fall.  The autumnal equinox occurred September 23 at 6:13 AM CDT.  The equinox is the instant when the center of the sun crosses the celestial equator, in this case moving from the northern to the southern hemisphere in the sky.  That movement has great earthly consequences.  The days grow shorter in the northern hemisphere and sunlight strikes the earth more obliquely, eventually bringing on the cold of winter at all northern latitudes outside the tropics – including our own latitude.  So get ready!


General Principles of Telescopes
        Our program for the September meeting was a presentation by Doug McCombs on the above topic.  Doug noted the three major types of telescopes: refractors, which work by bending light rays through lenses; reflectors, which form images by using mirrors; and combination optics, which use lenses in conjunction with mirrors.  Those three types of telescopes are arranged in chronological order of their development.
        Refractors.  The first refractor was made in 1608 by Jan Lippershey, a Dutch spectacle maker.  Galileo soon made a small refractor of his own and was the first person to make observations of the sky, discovering the four largest moons of Jupiter early in 1610, and making astronomical history with many other observations.  Galileo’s scope was about 1 inch in aperture and magnified about ten times.
        Reflectors.  The ability to see dim objects (the light-gathering ability of a scope) depends on the diameter, or aperture, of the lens.  But larger lenses are very difficult and expensive to make, so telescope makers turned to mirrors, which were easier to grind in large diameters.  Gregory proposed a reflecting telescope using mirrors in 1663, but his design was impractical.  Isaac Newton built a highly successful small reflector in 1672, which Cassegrain slightly modified that same year.  To this day, Newtonian and Cassegrain scopes are still with us.
        The large primary mirror of a reflector is mounted at the rear of the telescope tube.  The primary mirror reflects the light to a small secondary mirror mounted near the front of the scope.  In a Newtonian, the secondary then reflects the light at right angles through the side of the tube to the eyepiece.  In a Cassegrain, the secondary mirror reflects the light rearward through a hole in the primary mirror and then to the eyepiece.
        Combination Optics.  Scopes using lenses in combination with mirrors were developed in the present century.  The Schmidt camera has been used extensively in large-scale sky surveys.  The light passes through a thin corrector plate at the front of the camera and is then reflected onto the film by a spherical mirror at the rear.
        The Schmidt-Cassegrain scope has a thin corrector plate at the front and a spherical primary mirror at the rear of the scope.  The primary reflects the light to a secondary mirror mounted on the corrector plate, which then reflects the light to the eyepiece through a hole in the primary mirror.  Thus, the light traverses the length of the telescope tube three times – in the incoming, outgoing, and again in the incoming direction.  [If you’ve ever wondered how an 8-inch Schmidt-Cass could fit a 2,000 mm (79 inches) effective focal length into three traverses of a 16-inch tube and an inch or two of eyepiece, Doug is your man.]
        The Schmidt-Newtonian design uses a front corrector plate with a spherical mirror at the rear.  A flat secondary mirror mounted diagonally reflects the light into the eyepiece on the side of the tube.
        The Maksutov-Cassegrain uses a deeply curved thick corrector plate at the front and a spherical primary mirror.  The secondary mirror is a silvered spot on the rear of the corrector plate.  The reflective spot is smaller than the secondary in a Schmidt-Cass, so the Maksutov offers higher contrast because of lower diffraction at the smaller perimeter of the secondary reflective spot.
        All of the scopes with combination optics are variations on a theme that has been with us for over 300 years.  It is still true today that reflectors and scopes with combination optics are less expensive than refractors, inch for inch of aperture.  Some things never seem to change.


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.


The Last Eclipse

        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.


More on the Monahans Meteorite from NASA
        It is not quite manna from heaven, but NASA scientists on Thursday announced the first discovery of liquid water in an object from space.
        The water was trapped, like a fly in amber, in salt crystals on a meteorite that thudded to earth last year in Monahans, TX.  The meteorite is four and a half billion years old, so analysis of the water may provide clues to the solar nebula, the swirling cloud of gas and dust that gave rise to the Sun and the planets.
        "These are the first direct water samples ever found in a meteorite," said Michael E. Zolensky, space scientist at NASA's Johnson Space Center in Houston and lead author of a paper describing the study, [now] published in the journal Science. "It's a look back at the earliest days of the solar system."
        For further information see the website: http://www.nytimes.com/yr/mo/day/news/national/science/sci-meteor-water.html


¡COMING EVENTS!

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.

Go to Schedule Page for more info


¡1999 Dues Now Payable!

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
Betty Grimm, BBAS Treasurer.

Our dues are still $20.00 per year payable on a calendar-year basis,
the same as for 1996, our first full year of the society.


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