A total lunar eclipse occurs when the Moon passes completely through the Earth’s dark shadow, or umbra. During this type of eclipse, the Moon will gradually get darker and then take on a rusty or blood red color. The eclipse will be visible throughout eastern Russia, Japan, Australia, the Pacific Ocean, and parts of western and central North America. (NASA Map and Eclipse Information)
On Wednesday, Oct. 8th, there will be a unique spectacle in the sky: a lunar eclipse.
Let’s take a look at how lunar eclipses occur, why the moon appears to turn red, and the best way to photograph it for ourselves.
On Friday, 18 October, this month’s full moon occurs and with it, weather permitting, we’ll see a penumbral lunar eclipse – so called because only the full moon passes through the outer bright rim of the Earth’s shadow, or penumbra, as it rises in the east at sunset. Unlike total eclipses, in which Earth’s umbra — the central region of its shadow — darkens the moon entirely, a penumbral lunar eclipse involves only a slight dimming. Still, sky watchers should expect to see a much more subtle sight with a maximum shadowing on the lower half of the full moon occurring at 6.50 pm. CDT. Sky watchers should start observing the moon at sunset. Best place for observing this Friday’s eclipse is in Europe, Africa and the Middle East where it will be visible as a total eclipse. From Baton Rouge however, this penumbral eclipse should last about 45-minutes. The next lunar eclipse to be seen from our area will be Tuesday, 15 April 2014. Mark your calendars!