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4hv.org :: Forums :: General Science and Electronics
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Total lunar eclipse

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Proud Mary
Wed Dec 22 2010, 09:41AM
Proud Mary Registered Member #543 Joined: Tue Feb 20 2007, 04:26PM
Location: UK
Posts: 4992
I'd hadn't thought much about the reddish hues of the eclipsing moon, but apparently it's the light of the sunsets and sunrises on Earth, according to an atronomer on Radio 4.
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ScotchTapeLord
Wed Dec 22 2010, 12:23PM
ScotchTapeLord Registered Member #1875 Joined: Sun Dec 21 2008, 06:36PM
Location:
Posts: 635
It was cold but clear where I was, so I managed to catch it perfectly. Awesome sight! I caught the last 20 minutes of it or so and it didn't appear to have completely eclipsed by the team it was supposed to have (it seemed very white and bright on one side, but I don't know much about these things) but I couldn't stand the windchill anymore.
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Nicko
Wed Dec 22 2010, 01:30PM
Nicko Registered Member #1334 Joined: Tue Feb 19 2008, 04:37PM
Location: Nr. London, UK
Posts: 615
Proud Mary wrote ...

I'd hadn't thought much about the reddish hues of the eclipsing moon, but apparently it's the light of the sunsets and sunrises on Earth, according to an atronomer on Radio 4.
From eclipse.org Link2 :
"the umbral shadow had engulfed the Moon and the majority of its visible hemisphere had taken on a coppery-red colour generated by sunlight filtered and refracted through the Earth's atmosphere"

From Wikipedia Link2 :
"The Moon does not completely disappear as it passes through the umbra because of the refraction of sunlight by the Earth’s atmosphere into the shadow cone; if the Earth had no atmosphere, the Moon would be completely dark during an eclipse. The red coloring arises because sunlight reaching the Moon must pass through a long and dense layer of the Earth’s atmosphere, where it is scattered. Shorter wavelengths are more likely to be scattered by the air molecules and the small particles, and so by the time the light has passed through the atmosphere, the longer wavelengths dominate. This resulting light we perceive as red. This is the same effect that causes sunsets and sunrises to turn the sky a reddish color; an alternative way of considering the problem is to realize that, as viewed from the Moon, the Sun would appear to be setting (or rising) behind the Earth.

The amount of refracted light depends on the amount of dust or clouds in the atmosphere; this also controls how much light is scattered. In general, the dustier the atmosphere, the more that other wavelengths of light will be removed (compared to red light), leaving the resulting light a deeper red color. This causes the resulting coppery-red hue of the Moon to vary from one eclipse to the next. Volcanoes are notable for expelling large quantities of dust into the atmosphere, and a large eruption shortly before an eclipse can have a large effect on the resulting color."
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