The Magazine About Learning and Teaching Astronomy


Join others around the world in measuring the Moon's distance and size.  An educational, collaborative experience...and experiment!  Which of two methods gets the more accurate measures?


The ancient Greeks measured the Moon's distance using the size of the Earth's umbral shadow as revealed by the Moon going through it during a total (or deep partial) lunar eclipse.  They knew but could not do, a measurement of lunar parallax, the shift in the sky the Moon would make when seen from two very far away places.  Today we can do both and compare the results.  

The Shadow technique can be done anyplace where the Moon can be watched through the beginning partial, total, and end partial phases of the eclipse.  It can be recorded by drawing or photography.

The Parallax technique is done with two observers sufficiently far apart (we estimate at least 2000 miles (3200 kilometers).  The Moon must be recorded with photographs taken at the exact same time, with a field of view wide enough (4-8 degrees) such that the neighboring stars can be recorded at the same time on both photographs.  Overlaying the photographs, a comparison will show the shift of the stars (or Moon) as seen from the two places.  The larger the shift, the closer the Moon. See the photo below of the shift observed during the June 2011 total lunar eclipse. 

As an example, the following map shows a large area (in pink tones) that can use the umbral, Shadow-cross-section technique, and the striped zones that form the farthest places where the lunar parallax can be accomplished while still being dark enough to show stars (base map courtesy Jet Propulsion Laboratory).



For the December 2011 total lunar eclipse, The Classroom Astronomer magazine sponsored the International Measure The Moon Night, to encourage world-wide total lunar eclipse observations. Shall we do it again for the next eclipse? Would you join us?



To do your measuring, in a future total lunar eclipse, choose the link below for the Method (Shadow or Parallax) you plan to use!!

Shadow
Parallax


Some General Lunar Eclipse Materials and Information

Next Eclipse and Times (UT = Greenwich Time)
April 15, 2014

Moon enters Umbra (partial phases begin):  5:58
Totality begins: 7:06
Totality ends: 8:24
Partial phases end (Moon leaves Umbra):
9:33


You must add or subtract how many time zones you are from London to get local times, and take into account if Summer Hours (Daylight Saving Time) is in effect in your area..

For example: Los Angeles is -7 hours from London (normally -8 but it is on DST then) so totality begins 9:58PM APRIL 14th(!).

Future Total Eclipses

October 8, 2014 --1 hour of totality, Asia, Australia, Pacific, Americas.
April 4, 2015 - 5 minutes(!) of totality, a good Shadow Passage eclipse!, Asia, Australia , Pacific, America.
September 28, 2015 - E. Pacific, Americas, Europe, Africa, W. Asia
No more until 2018.


How to take Lunar Eclipse Photographs--by the three photographers on these Web Pages, in Italy, Turkey and China.


Articles on Lunar Eclipses from The Classroom Astronomer magazine:

The Lunar Parallax and December's International Measure The Moon Night (Fall 2011, Issue 9)
Illuminating Science Through Darkness 1 - Shadow Cones (Fall  2010, Issue 5)
Illuminating Science Through Darkness 2 - In Earth's Shadow
(Fall  2010, Issue 5)
Illuminating Science Through Darkness 3 - Caught! Shadow Reveals Moon's Size and Distance (Fall  2010, Issue 5)