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Article #41Math/Science Experiment for Public Education by Lakewood, Ohio H.S.
From: G_HOLBERTRL
Date: Fri, 16 Sep 1994 14:43
Date: Fri, 16 Sep 1994 14:43
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7242 bytes
Date: Thu, 15 Sep 1994 22:42:18 -0400
From: aj860@cleveland.Freenet.Edu (James D. Meinke)
ATTENTION - SEPTEMBER 24, 1994 IS THE EQUINOX
A WORLDWIDE SCIENCE AND MATH EXPERIMENT
ERATOSTHENES EXPERIMENT
Eratosthenes, a Greek geographer (about 276 to 194 B.C.), made a
surprisingly accurate estimate of the earth's circumference. In
the great library in Alexandria he read that a deep vertical well
near Syene, in southern Egypt, was entirely lit up by the sun at
noon once a year. Eratosthenes reasoned that at this time sun
must be directly overhead, with its rays shining directly into
the well. In Alexandria, almost due north of Syene, he knew that
the sun was not directly overhead at noon on the same day because
a vertical object cast a shadow. Eratosthenes could now measure
the circumference of the earth (sorry Columbus) by making two
assumptions - that the earth is round and that the sun's rays are
essentially parallel. He set up a vertical post at Alexandria
and measured the angle of its shadow when the well at Syene was
completely sunlit. Eratosthenes knew from geometry that the size
of the measured angle equaled the size of the angle at the
earth's center between Syene and Alexandria. Knowing also that
the arc of an angle this size was 1/50 of a circle, and that the
distance between Syene and Alexandria was 5000 stadia, he multi-
plied 5000 by 50 to find the earth's circumference. His result,
250,000 stadia (about 46,250 km) is quite close to modern meas-
urements. Investigating the Earth, AGI, l970, Chapter 3, p. 66.
The formula Eratosthenes used is:
D A d=distance between Syene and Alexandria
_____ = _____ A=360 degrees assumption of round earth
a=shadow angle of vertical stick
d a D=to be determined (circumference)
----------------------------------------------------------------
Are you interested in participating?
All you need to do is place a vertical stick (shaft) into the
ground at your school and when the sun reaches it's highest
vertical assent for the day (solar noon therefore the shadow
length will be the shortest), measure the angle of the shadow of
the stick (a).
-\
- \
stick -> - \
- a \ a=shadow angle
- \
- \
ground___________________-______\shadow_______________________
By doing this experiment on the equinox we all know that the
vertical rays of the sun are directly over the equator, like the
well at Syene. Using a globe or an atlas the distance between
your location and the equator ( d in equation) can be determined
and the circumference can be calculated.
*****************************************************************
But how about sharing your shadow angle measurement with others
around the real globe.
******************************************************************
Send your measurement of the shadow angle____________degrees
Send your location city ____________________________________
Send your location country _________________________________
Send your latitude _________________________________________
Send your longitude ________________________________________
To Lakewood High School Earth Science Class, Lakewood, Ohio
bd765@cleveland.freenet.edu
We will compile all the data and send you a copy to use in your
classroom to compare the various locations and angles.
If your interested send us your data. We will compile and return
it to you by September 30, 1994. Chances are your lesson plans
will not be able to fit this in on Friday, September 24, l994
(the equinox). Most any day plus or minus 2-4 days of the equi-
nox will give fairly good data (like Wednesday through Friday or
Monday or Tuesday).
Jim Meinke - Lakewood High School bd765@cleveland.freenet.edu
******************************************************************
INTERESTED IN A NEW WORLDWIDE EXPERIMENT
MAPPING THE EARTH'S MAGNETIC FIELD (ISOGONIC)
This experiment can involve many classrooms around the globe in:
communications
measurement
mapping skills
calculations
It would involve a minimum of equipment at each school (or home)
to conduct the experiment.
world map
compass(es)
night observation of Polaris (North Star), Southern Cross
for our southern neighbors
The experiment would involve many schools or homes involved in
gathering the data from their latitude and longitude. How far off
is your magnetic data from true north or south in your location?
This data would be transmitted to us here at Lakewood High School
and we would send out a summary so that you could construct a
worldwide magnetic map in your classroom. This would also lead
to discussions on the locations of the magnetic poles as well as
how to draw iso or (equal) lines. It might also lead to discus-
sions of night sky movements around the constellations or how the
magnetic field is thought to be created.
ARE YOU INTERESTED?
If you are interested in trying such an experiment, drop me a
quick note at the address below.
Jim Meinke - Lakewood High School
bd765@cleveland.freenet.edu
or
personal account - aj860@cleveland.freenet.edu
personal account - meinke@freenet.lorain.oberlin.edu
********************************************************************************
Richard Lee Holbert '85 g_holbertrl@titan.sfasu.edu
210 West Austin, #204 rlh@tenet.edu
Nacogdoches, Texas 75961 rholbert@cap.gwu.edu
AGGIE '85, Cooking/Eating, Genealogy, Alternative Medicine/Health Care
K-12 Computing/Networking, INTERNET Surfing, and other stuff
"If you think Education is Expensive, consider the Alternative "
- cannot remember author -
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From: G_HOLBERTRL@TITAN.SFASU.EDU
Subject: Math/Science Experiment for Public Education by Lakewood,
Ohio H.S.
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