Here is the Eclipse time table provided by Fred Espenak on the Astroleague of the Philippines site:
Eclipse Phases | Time (PST) | Altitude | Azimuth |
Moon enters Penumbra | 07:33:32 pm | 30 deg | 72 deg E |
Moon enters Umbra | 08:45:42 pm | 47 deg | 72 deg E |
Moon enters Totality | 10:06:16 pm | 64 deg | 67 deg E |
Maximum Totality | 10:31:48 pm | 70 deg | 63 deg NE |
Moon exits Totality | 10:57:24 pm | 75 deg | 55 deg NE |
Moon exits Umbra | 12:17:58 am | 80 deg | 325 deg NW |
Moon exits Penumbra | 01:30:00 am | 65 deg | 294 deg NW |
The reddening effect of the moon during the total lunar eclipse happens when the Moon enters the umbra, or the darker shadow of the Earth. When this happens, light from the Sun reaching the moon is blocked completely by the Earth, however the atmosphere of Earth acts as a lens which bends light into its component parts (spectra). The light that is bent most is the red part of the spectrum, which also explains the red-orange hue of the sky during sunrise and sunset. In contrast, blue wavelengths are the easiest component of light that is scattered - hence the blue colored sky as particles in the air scatter the blue light.
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