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Total lunar eclipse on October 8th
, 2014
Joe Cali



On Wednesday October 8th,  a total lunar eclipse will be visible across Australia during the first half of the night.  A lunar eclipse occurs at some full moons when the Moon passes through the Earth's orbital plane at full moon. The Earth's shadow is cast a long way out into space. When the Moon passes through this shadow, we see a lunar eclipse.  A lunar eclipse is perfectly safe to watch. There is no danger to your eyes.




At full moon, the Moon rises as the sun sets.



This map shows visibility of the total lunar eclipse across the continent.  I have broken the continent into three broad regions, east, central and west.  




The altitudes given in this article are only approximate.  Australia is a big place and altitude of the Moon obviously varies with location.

Eastern States

On the eastern side of the continent, the whole eclipse can be observed in relative darkness.  The penumbral eclipse begins as the Moon rises and the sun sets. Twilight interferes with the penumbral eclipse, which is practically invisible to the untrained observer and barely perceptible to an expert observer.  The partial eclipse begins as twilight ends with the Moon approximately 10-15o above the horizon. Totality begins with the Moon in the northeast about 25o above the horizon and finishes with the Moon 35o above the horizon still in the northeast.

Central Australia
In the central states, the penumbral eclipse occurs before Moonrise and the partial eclipse begins with the Moon near the horizon. Totality begins near the end of twilight with the Moon 13o above the horizon. and ends with the Moon 25 degrees above the northeast horizon.

Western Australia
In Perth, totality is in progress as the Moon rises at sunset. A totally eclipsed moon will probably not be visible at sunset but as twilight sets in, the coppery red moon will progressively become more visible against the deep blue sky on the eastern horizon. The total eclipse ends as twilight is coming to an end.



Whilst not ideal for astronomical observations, eclipses like this are aesthetically beautiful to watch as the coppery Moon magically appears out of the darkening twilight sky.  Lunar eclipses vary in brightness. This is usually related to how deep into the umbra the Moon passes during the eclipse.  As can be seen in the umbral passage diagram below, the limb of the moon does not go through the center of the umbra. One limb of the Moon is always near the edge of the  and so this should be a relatively bright eclipse.

 




Eclipse Contacts

P1 = 04:53:37 UT  [Penumbral eclipse begins]
U1 = 05:58:19 UT  [Partial eclipse begins]
U2 = 07:06:47 UT  [Total eclipse begins]
U3 = 08:24:35 UT  [Total eclipse ends]
U4 = 09:33:04 UT  [Partial eclipse ends]
P4 = 10:37:37 UT   [Penumbral eclipse ends]
Totality Duration     01h17m48s

The above diagram from the NASA Lunar Eclipse Home Page shows the passage of the Moon through the Earth's umbral shadow.  Contacts listed in light grey are not visible from eastern Australia [Moon is below the horizon].  


Taking photographs - basic guide
 


In the west, as the totally eclipsed Moon appears out of the twilight sky, you can use automatic exposure because the red Moon and the deep blue sky will be of similar luminosity values.
You camera will try to give "correct" exposure making it look like the picture is taken in daylight.  To overcome this, use the exposure compensation function.
When the eclipsed moon first becomes visible, turn the compensation to -1eV.  As twilight fades, turn it to -1.5eV then -2eV. Bracket, these exposures.

From the east coast, the eclipse will be seen in darkness.  Camera metering will not work unless the Moon's image is large enough to fill the frame.

Set camera ISO to 200  
 
Event Shutter Speed Aperture
Full Moon
Penumbral Eclipse
Moon 1/4 eclipsed
Moon 1/2 eclipsed
Moon 3/4 eclipsed
Small crescent
Totality
Totality
Totality(ISO800)
1/1000
1/500
1/250
1/125
1/60
1/8
1s-15s*
1/4-4s*
1/15-1s
f8
f8
f8
f8
f8
f8
f8
f4
f4

* Moon's image may move due to Earth's rotation at these exosure times. If using telephoto and tripod without tracking, use the ISO800 recommendation.

References
Map graphics produced with Google Earth
Umbra diagram and eclipse timings from NASA Eclipse Home Page http://sunearth.gsfc.nasa.gov/eclipse/eclipse.html
Sunset and twilight from Geoscience Australia sunrise/sunset program http://ga.gov.au
Some caclulations made with Starry Night Pro
Photographs © Joseph Cali