A NOT-SO-SPOOKY
ECLIPSE
by Dr. Terry Goforth
Associate Professor of Physics, SWOSU
Saturday, November 8, skywatchers have a chance to observe the second
lunar eclipse of 2003. Once again, the full moon will pass through
Earth’s shadow and, for a brief time, appear much dimmer and possibly in shades
of red, orange, or copper instead of its usual bright white.
The moonlight we see is simply sunlight that has reflected off the moon’s
surface. When the moon is in the umbra, there is (almost) no sunlight
to reflect, so the moon appears dark. What little sunlight leaks into
the umbra is light that has been deflected by Earth’s atmosphere. This
deflection primarily scatters red and orange light, causing the moon to
take on the characteristic “angry” colors associated with a fully eclipsed
moon. (This same color selection is what causes sunsets and sunrises
to appear red or orange.)
The Earth’s umbra (the darkest part of its shadow) is shaped like an cone
(with Earth at the fat end) and extends over a million miles into space.
The moon, a mere 240 thousand miles away, fits easily into this shadow.
If the moon passes through the center of the shadow, totality can last over
an hour and a half. This time, the moon will simply graze the umbra
near its south side, so the total portion of the eclipse will be relatively
short, lasting only about 25 minutes. This proximity to the edge of
the umbra also means the moon will likely be darker near its northern side
and somewhat lighter near the southern edge. The exact color of the
moon during totality depends on the amount of dust and moisture in Earth’s
atmosphere at the time of the eclipse.
For viewers in Weatherford, moonrise will occur at 5:29 p.m. on Saturday.
The partial phase of the eclipse (when only part of the moon is in the umbra)
begins at 5:32 p.m. (8 Nov, 23:32 UT*), when the moon is still very low on
the east-northeastern horizon. The moon will continue moving into the
umbra as it rises. Totality (when the moon is completely inside the
umbra) begins at 7:06 p.m. (9 Nov, 01:06 UT) At this time, the moon
will be about 20° above the eastern horizon. Totality will end
at 7:31 p.m. (9 Nov, 01:31 UT) as the moon begins to emerge from the umbra.
The second partial phase of the eclipse (as the moon moves out of the umbra)
will continue until 9:04 p.m. (9 Nov, 03:04 UT), by which time the moon
will be about half-way up in the east-southeastern sky. (If you don’t
live near Weatherford, the time of moonrise may be slightly different, but
the eclipse times will be the same.)
Lunar eclipses are easy to observe. No special equipment is needed,
and they happen right on time. All you’ll need are clear skies and
a view of the eastern horizon. If you have binoculars or a telescope,
it’s worth a look to see some details on the moon. There’s no danger
in looking directly at the moon with your eyes, binoculars, or through telescopes.
Unlike observing solar eclipses, the light is not bright enough to cause
any damage. So take a look. Weather permitting, it will be a good
show.
More information: There are many web sites and publications
with information on this event. Try the the November 2003 issue of Sky
& Telescope (skyandtelescope.com)
or the November 2003 issue of Astronomy magazine (www.astronomy.com). NASA information
and links can be found at science.nasa.gov/headlines/y2003/04nov_lunareclipse2.htm.