Outdoor Lighting Report
by Jim Walker
Bernie reported seeing a very bright
light at the Highland Concrete Plant just outside the city on US 90 East.
This light is directly in the eyes of drivers travelling west on the highway.
Another light is aimed to the northeast. I spoke with one of the
owners who was very cooperative. I believe both of these new lights
will soon be readjusted to 20 deg above the horizontal, as the Alpine lighting
ordinance specifies.
Several unshielded wallpacks were
recently installed on the Pete P. Gallego Building, the new multipurpose
building on the Sul Ross Campus. More than a year ago I had a lengthy conversation
with the director of the physical plant about the kinds of lights to be
installed on and around that building. I was assured that all such
lights would be full cutoff fixtures. When I called the director
after observing the new unshielded wallpacks, he said they were supposed
to be FCO fixtures, and he would call the contractor. The contractor, however,
refused to change the lights. I wrote Pete Gallego, pointing out that it
would be unfortunate if the Pete P. Gallego Building were to remain in
violation of HB916 - the state lighting law, which Pete sponsored and successfully
carried through the legislature in 1999 - and also in violation of our
Alpine ordinance. Pete sent a copy of my letter at once to Dr. Vic Morgan,
SR President, and a cover letter of his own expressing the hope that the
situation would be remedied. I believe the lights will be replaced. [At
this writing, the lights have been turned on, all 7 of them, and they are
bright. Have a look.]
When the new acorn lights were
installed as part of the Main Street Program a couple of years ago, several
of the new lights were installed within 6 to 30 feet of existing streetlights
(pole to pole distance). Most of those nearby streetlights were 400-watt
drop lens cobra-heads. Shortly after I gave a list of those redundant street
lights to City Manager Bill Lewis, 5 of the cobras were removed. Eliminating
those very bright lights reduces glare, reduces uplight, and saves the
city more than $1,000.00 a year. Your tax dollars at work!
The new Ft. Davis Post Office
is now under construction. It might be very helpful if some of our members
living nearby would speak to the on-site construction superintendent about
their lighting. There has been a lighting order in effect in Jeff
Davis County for many years, so we can hope that we will see better lighting
installed in Ft. Davis than we have seen at the Alpine Post Office.
Exploring our Solar Origins
by John Bell
Reported by Jim Walker
Before showing a videotape from
the Learning Channel, John asked us to look at the presentation critically,
with respect to its possible use in the schools.
The Sun has been very dependable
in the past, but its future will be violent. Perhaps in a billion years
or so, it will get much hotter, very likely boiling away the earth's oceans,
eventually expanding to engulf Mercury, Venus, Earth, and possibly Mars.
The Hubble Space Telescope has
given us new insights into the history and evolution of stars. From its
orbit 380 miles above the earth, the HST can see about 10 billion years
into the past, into the fairly early days of our solar system. We can observe
regions of active star formation, such as the area dubbed the Pillars of
Creation in the Eagle Nebula.
New stars and perhaps solar systems
are forming out of disks of gas and dust. As in our own solar system, the
heavier elements remain near the center, and the lighter elements are driven
outward.
Is our solar system unique? The
answer is no, at least in several important respects. For example, there
is a disk of gas and dust around the star Beta Pictoris that has many of
the characteristics of the disk of material around our own sun that gave
rise to our own solar system. Today, we can observe similar processes in
the Orion Nebula.
Geoff Marcy and Paul Butler, astronomers
at California State University at San Francisco, have found strong evidence
of large planets orbiting distant stars. An orbiting planet tugs at its
star, causing the image of the star to wobble slightly. If the orbit of
a planet lies roughly in our line of sight, then it will tug its star alternately
toward and away from the earth, causing predictable shifts in the spectrum
of the starlight. [At this writing, more than 50 planets have been
"discovered" outside our solar system. However, no such planet has been
directly observed visually or photographed.]
In our own solar system, the inner
planets are rocky, made of heavier elements. Mercury, Venus, Earth, Mars,
and the Asteroids, are much heavier (in the sense of being more dense)
than the outer planets, the gas giants. With the exception of Venus, all
of the other planets rotate in the same direction, west to east. It is
unclear why Venus should rotate in the opposite direction.
Mercury, about the size of our
moon, is a barren, pock-marked planet that is too small to have an atmosphere.
Venus, similar in size to the earth, has a dense atmosphere of carbon dioxide,
and sulfuric and hydrochloric acid. The Russian Venera probe and the American
Magellan probe barely survived the 800-deg F temperature long enough to
send a little data back to the earth. Rugged mountains and valleys indicate
a violent past.
Mars and the Earth are thought
to have been more similar about 4 billion years ago. Mars is substantially
smaller than the earth, and has lost much of its water and atmosphere in
the last few billion years. Today, Mars s not a hospitable place - but
we'll go there one day nevertheless.
The Asteroid Belt, between Mars
and Jupiter, may be the material left over from a potential planet that
never developed. Ceres, the largest asteroid, is about 600 miles in diameter,
and the smallest ones are no more than small boulders.
Jupiter, the largest planet and
the first of the gas giants, has no solid surface. All we can see is the
upper atmosphere, with its cloud bands, and the Great Red Spot, a rotating,
hurricane-like storm that has been active for 300 years or so.
Uranus, discovered in 1781, is
the first planet discovered since ancient times. The axis of Uranus is
tilted more that 90 deg out of the plane of the solar system. The planet
has several thin rings in the plane of its equator. The tilt of its axis
and rings suggests that Uranus may have suffered a massive blow from a
large body at some time in the past.
Neptune, the outermost of the
gas giants, shows little surface detail. This planet has the highest winds
measured so far in the solar system, 1,000 miles per hour. Triton, one
of Neptune's moons, is the coldest body in the solar system.
Pluto, the outermost planet, was
not discovered until 1930. Clyde Tombaugh, a Kansas farm boy turned astronomer,
was hired by Lowell Observatory, in Flagstaff, AZ, specifically to look
for the outermost planet. His diligence and skill finally paid off with
the discovery of our last planet. [Before his death a few years ago, Clyde
Tombaugh was a frequent visitor and speaker at the Texas Star Party. There
is an excellent biography entitled Clyde Tombaugh: Discoverer of Planet
Pluto, by David H. Levy, University of Arizona Press, 1991.]
Pluto doesn't fit well with the
other planets. It seems unreasonable to find another solid planet, rocky
or icy, beyond the gas giants. Some astronomers have argued that Pluto
more properly belongs to the Kuiper Belt, or perhaps the Oort Cloud, a
spherical shell of icy bodies that may become comets when they are somehow
deflected into the inner solar system. Planet or not, the last word on
Pluto has not been said.
Although the video is somewhat
dated, as all such presentations must soon become, we thought the program
was fundamentally well done. Anyone showing the video could easily offer
some current information updating, for example, the search for extrasolar
planets.
End of minutes.
Respectfully submitted, Jim
Walker, Secretary
Earth Reaches Aphelion
(NASA Science News, July 3, 2001)
On the 4th of July, Earth reached
its greatest distance from the Sun, the aphelion of our orbit. But don't
expect any sudden relief from the heat. Indeed, our planet is actually
warmer when we're farther from the Sun than at any other time of year.
The varying temperatures of our
seasons are caused by the 23 1/2 degree tilt of the earth's axis with respect
to our orbit. But there are complications. It happens that there
is more land in the northern hemisphere and more water in the southern
hemisphere. The northern land masses absorb more heat than do the southern
oceans, so summers are warmer when the northern hemisphere tilts toward
the sun - even though the earth is about a million miles farther from the
sun at that time. Be glad that our northern summer doesn't occur
at perihelion!
Daytime Fireball Streaks
Over Northeast US
(David Tytell, Sky Publishing, July 24)
Around 6:19 p.m. EDT on the evening
of July 23, a brilliant meteor shot through the skies above the northeastern
United States. Reports of a daytime fireball stretch from North Carolina
all the way to Buffalo, New York, and Bobcaygeon, Ontario (see the map
and other information at http://www.skypub.com).
The meteoroid apparently entered the Earth's atmosphere above North Carolina
and traveled north-northwest to the Canadian border. One observer in Virginia,
described the object as "much brighter than any daytime full moon . . .
[like] a sparkler lit in daytime."
Near Williamsport, Pennsylvania,
windows were rattled by a loud crashing noise, described by many as a deafening
thunderclap. Some thought the bolide was a falling airplane and county
emergency services received over 300 calls to 911 switchboards from concerned
citizens. An Emergency Management Coordinator for Lycoming County, described
a burnt patch of a cornfield in Salladasburg, Pennsylvania, near Williamsport.
Several cornstalks were blown over and leaves appeared curled from heat.
However, no meteorite was found. Sky & Telescope will be following
this story as more information becomes available.
The Annual Perseids
You may remember that we had a
good display of meteors at our Perseid watch a while back. Some of the
meteors we saw were bright enough to light up the ground and cast shadows,
and some of their trails lasted for 5 minutes or more. The best time to
watch this year will be the predawn hours of August 12, even though the
peak occurs later during daylight. Unfortunately, the 3rd-quarter
moon rises just after midnight and will wash out all but the brighter meteors.
But it's worth a look if you have a decent viewing site near by.
The following is edited from Mark
Davis and Cathy Hall, North American Meteor Network (see their website
at http://web.infoave.net~meteorobs/)
The Perseids are fast meteors, at about 59 km per second, and often leave
trains behind them. There are many bright Perseids, so even from a less
than perfect sky location, an observer will see a respectable number of
meteors. For the best effect though, try to get out into the country, away
from the light pollution of streetlights.
The Perseid meteor shower has
been observed for about 2000 years, with the first known information on
these meteors coming from the far east. In early Europe, the Perseids came
to be known as the "tears of St. Lawrence." Mark Littmann has a wonderful
article on the history of the Perseids on the Sky and Telescope website
http://www.skypub.com.
Because the orbit of the Perseid
meteoroid particles is tilted so much in relation to the plane of our own
solar system, the Perseids have stayed fairly similar in characteristics
since ancient times, and have not been changed much by the influence of
our large planets such as Jupiter. It was Schiaparelli, the astronomer
most noted for observing so-called "canali" on Mars, who discovered that
the Perseid meteors were related to Comet 1862 III, also known as 109/P
Swift-Tuttle. This was the first proven association between a comet and
a meteor shower.
The parent comet itself, 109/P
Swift-Tuttle, was discovered in July of 1862 by both Lewis Swift of Marathon,
New York and Horace Tuttle of Harvard Observatory, Massachusetts. It was
about magnitude 7.5 at discovery and brightened to about magnitude 2 by
early September, which is about the same brightness as the stars in the
Big Dipper. It sported a tail of between 25 and 30 degrees long, and was
quite impressive! By length comparison, the pointer stars of the Big Dipper
are about 5 degrees apart. The comet comes around to our part of the solar
system about every 120 years and was seen most recently in the mid 1990's.
In November of 1992, it brightened to about magnitude 5.0.
¡Y2K+1 Dues Now Payable:
Still only $20.00!
If we have not yet received your dues, then please use the convenient
envelope addressed to our treasurer that is included with this copy of
your Newsletter.
Betty Lou Grimm, Treasurer
Big Bend Astronomical Society, Inc
1001 N 2nd Street, Apt F-22
Alpine, TX 79830
¡COMING
EVENTS!
***
REGULAR MEETING ***
7:30 PM Wednesday, August 8, 300 Lawrence Hall, Sul
Ross Campus,
Jim Walker Presents:
Understanding the Seasons:
Why Is It Summer in the Northern Hemisphere When
We're Farther from the Sun?
This and other mysteries revealed...and explained!
Star Party & Potluck Supper
Jim & Barbara Walkers'
9:00 PM, Saturday, August 11,
(Sunset 8:25 PM)
HARDY SOULS are welcome to stay
late and watch the PERSEIDS
(See the Star
Chart for more info on these meteors)
Among other celestial wonders, we can offer a good view of Comet LINEAR2
with our scope,
and maybe even with your naked eye! Seen any comets lately???
Alternative date: Sunday, August
12
No potluck suppers until the
Fall.
We will resume having our suppers
when we can meet earlier
after we go off daylight saving
time.
Please e-mail or call Bernie
Zelazny at 837-1717 if you need further information.
Visit
the Schedule Page for more info.
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