We did not get to see it as this reference shows but what a sight it must have been.
The eclipsed moon in infrared.
Why it looks like this.
During a total eclipse the Moon
shines with a orange reddish glow.
Without Earth's atmosphere, the Moon would disappear completely once immersed in the umbra. Longer wavelengths of light penetrate Earth's atmosphere better than shorter wavelengths, which is why the rising or setting sun looks reddish. In essence, the ruddy tint of a totally eclipsed moon comes from the ring of atmosphere around Earth's limb that scatters a sunset-like glow into the umbra.
The hue actually changes from one eclipse to another, ranging from a bright coppery orange to brownish. The Moon may darken so much that it becomes all but invisible to the unaided eye. These very dark lunar eclipses often occur after exceptional volcanic eruptions.
Totality will end at 1:31 UT, when the moon's leading edge exits the umbra. The moon will leave the umbra completely at 3:05 UT, and the eclipse will end at 4:22 UT when the moon makes its last contact with the penumbra.
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