Prime Time Lunar Eclipse
October 2004 :
Note: This article may contain outdated information
This article was published in the October 2004 issue of The Skyscraper and likely contains some information that was pertinent only for that month. It is being provided here for historical reference only.
Do you think you would notice if the Full Moon practically
disappeared one night? Well, we'll have an opportunity to explore that
idea on the night of October 27-28, as the Full Hunter's Moon slides
deep into the Earth's shadow. Yes, we are again fortunate to be ideally
situated to observe another total lunar eclipse in its entirety. Let's
hope for some clear skies, because this is the last total lunar eclipse
until August 28, 2007.
I consider this lunar eclipse a "prime time" event since totality
concludes before midnight. As commuters drive home from work on the
night of October 27, they won't be able to miss the Full Hunter's Moon
rising in the east. Our desolate neighbor will bathe the landscape in
eerie reflected sunlight.
But, if those same folks ventured outside later in the evening would
they wonder what had happened to the bright Full Moon? Well, if you keep
on reading this article you won't be left in the dark as to the Moon's
whereabouts.
To refresh everyone's memory, a total eclipse of the Moon occurs
when the Sun, Earth and Moon are nearly in a straight line. With the
Earth in the middle of this celestial configuration, our planet's shadow
will sweep across the lunar surface. It's like compressing an entire
month's moon phase cycle into one evening.
The eclipse begins at 8:06 pm on the 27th and ends at 2:03 am on
the 28th for a duration of 5 hours and 57 minutes. All times listed are
Eastern Daylight Time (EDT). You don't necessarily have to watch the
entire eclipse to be impressed with the beauty of this event. Don't have
much free time? Just watch through the end of totality. After that it's
anti-climatic anyway. To help you plan your evening, the following
narrative highlights the times when significant phases of the eclipse
will occur.
The Moon enters the Earth's faint shadow called the penumbra at
8:06 pm and the eclipse begins. The penumbra is so dim that the Moon's
"first contact" with it cannot be seen. Only as the Moon slides deeper
into the shadow will a keen-eyed observer see a subtle shading of the
lunar surface. Just prior to the Moon entering the Earth's dark umbral
shadow one should notice that the moonlight looks somewhat subdued.
At 9:14 pm the Moon encounters the dark umbral shadow of the Earth.
The Moon will be moving eastward in our sky when it encounters the
Earth's shadow. Therefore, watch for the shadow to sweep across the
lunar surface from left to right. By the time the Moon is more than
halfway through the umbra we should be able to tell if this is going to
be a dark eclipse or a bright one.
Since there are no major volcanic eruptions spewing copious amounts
of dust into our atmosphere to darken the eclipse, I suspect the Moon
will remain visible even during mid-totality. And since the Moon will be
well within the Earth's dark shadow, it should present a collage of
yellow and orange hues to the observer, but without the bright ring of
light that moved around the edge of the lunar disk in May and November
2003. The umbral shadow completely envelopes the Moon at 10:23 pm.
That's the moment when totality begins.
Totality will last for one hour and twenty-two minutes. That's
almost one hour longer than last November's eclipse. This scenario will
give an observer plenty of time to scan the Moon's colorful surface.
Totality will be so long that I've actually seen folks get bored during
similar eclipses. Even during the darkest eclipses that I've observed, a
telescope will still reveal some rusty browns or reds on our lunar
neighbor. Mid-totality occurs at 11:04 pm. Forty-one minutes later a
sliver of brightness marks the end of totality at 11:45 pm as the Earth
and Moon move out of alignment and sunlight once again strikes the lunar
surface.
The partial phase will last until 12:45 am. At that time the dark
umbral shadow will leave the Moon's surface. Soon thereafter, like the
beginning of the eclipse, the remaining phase will hardly be noticeable
at all as the Moon begins to return to full brightness. For an hour and
eighteen minutes, until 2:03 am when the eclipse ends, the Moon will
remain within the lighter penumbral shadow. Only while the Moon is
still deep within the penumbral shadow will the lunar surface appear in
subdued light.
If you have binoculars or a telescope, this event is the time to put
them to good use. The more optical aid an observer uses, the more detail
one will discern. Even if you don't have access to expensive equipment
don't despair. Mother Nature provided you with a pair of the most
valuable observing tools - your eyes! Use them to follow the progress
of this beautiful event.
Skyscrapers, Inc. cordially invites you to Seagrave Observatory to
observe this total lunar eclipse. All our society's instruments will be
available to watch the progress of this astronomical event. Our members
may also bring their own telescopes and binoculars to share the view
with you. Parking is limited, so plan accordingly. Once the lot is full,
we will have to turn folks away. No parking is permitted on Peeptoad
Road.
If the weather is favorable make every effort to observe this
beautiful celestial show. The next one is more than two and a half years
away, so make the best of this upcoming opportunity.
Good luck, keep your eyes to the skies, and hope to see you at
Seagrave Observatory on the night of October 27-28.
And remember, Seagrave Observatory is also open every Saturday night
for your viewing pleasure, weather permitting of course. Visit us at
http://www.theskyscrapers.org for information.