On the night of September 7th and 8th, Earth passes directly between the sun and the full moon in the second final total lunar eclipse of the year.
For over five hours, the celestial event peaks at an impressive 82-minute overall stage as the giant shadows of the Earth plunge the entire moon into reddish darkness.
Sadly, unlike the previous Blood Moon Lunar Eclipse of the year, held from March 13-14, US viewers will not be invited to the show. By the time Eclipse begins at 11:28am (15:28 UTC), it has already set North and South America, cutting down much of the Western Hemisphere from events, according to Live Science’s sister site Space.com.
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Instead, solar eclipses will be most commonly seen from Asia and Western Australia. In this Western Australia, over 6 billion people (almost 77% of the world’s population) violate the entire total stage of the solar eclipse, depending on the time of the day. Skywatchers in most Europe and Africa can end at least part of the whole with UTC worldwide, and capture most of the substages that follow as the moon moves out of Earth’s shadow.
But North American Skywatchers want to catch the Bloody Moon in real time, but aren’t totally unlucky. A free live stream of the event is set for September 7th courtesy of the Italian Virtual Telescope Project. According to the Eclipse Map tool in Time and Date, the moon is partially covered and reaches the whole after about 45 minutes.
You can view the entire stream via the official Virtual Telescope Project YouTube page or the videos built into below.
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A solar eclipse of the general moon always occurs during a full moon where the moon, the earth and the sun are lined up in succession. When perfectly aligned, the umbrella, the innermost and darkest part of the Earth’s shadow – crosses the visible surface of the moon, extinguishing sunlight.
At this stage, the moon appears red thanks to a phenomenon known as Rayleigh scattering. In Rayleigh scattering, particles in the Earth’s atmosphere preferentially scatter light wavelengths of different wavelengths. As incoming sunlight bends around the globe, particles in the atmosphere scatter short-wavelength blue light, allowing long-wavelength red light to pass through the moon’s surface.
As always on Earth, the solar eclipse continues two weeks after the counterpart of the month. On September 21, partial solar eclipses are visible from New Zealand, Australia and parts of Antarctica, with up to 80% of the solar disk being blocked by the moon during peak hours. Several Pacific islands, including Fiji, Tonga and Samoa, can see slimmer solar eclipses covered less than 30% of the solar disc.
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