![]() Throughout human culture, lunar eclipses have been viewed with awe and sometimes fear. If you have questions about this eclipse, you will have an opportunity to ask experts at NASA’s Marshall Space Flight Center in Huntsville, Alabama! The table below lists eclipse timing details. CDT.Īll of the Americas are well placed to see this eclipse. If observing close to the Greenwich Meridian in the U.K., the eclipse begins just after midnight, in the morning of Sept. This eclipse will straddle midnight on Sept. 27, we will be treated to a lunar eclipse with its beautiful orange and red colors, a prelude to the fall color of leaves in Earth’s Northern Hemisphere. This lunar eclipse is related to two annular solar eclipses of solar saros 144.In the Americas on Sunday night, Sept. Because of the date shift, Earth's shadow will be about 11 degrees west in sequential events.Ī lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). The lunar year series repeats after 12 lunations, or 354 days (shifting back about 10 days in sequential years). The eclipse was one of four lunar eclipses in a short-lived series at the descending node of the Moon's orbit. A partial solar eclipse on 13 September.Contact points relative to Earth's umbral and penumbral shadows, here with the Moon near its descending node * The penumbral phase of the eclipse changes the appearance of the Moon only slightly and is generally not noticeable. † The Moon was not visible during this part of the eclipse in this time zone. Simulated appearance of Earth and atmospheric ring of sunlight View of Earth from Moon at greatest eclipse The eclipse was visible over Europe, the Middle East, Africa, and America. The northern portion of the Moon was closest to the center of the shadow, making it darkest, and most red in appearance. The Moon's brightness is exaggerated within the umbral shadow. The following simulation shows the approximate appearance of the Moon passing through Earth's shadow. The Moon appears to be reddish because of Rayleigh scattering (the same effect that causes sunsets to appear reddish) and the refraction of that light by Earth's atmosphere into its umbra. Then, the shadow begins to "cover" part of the Moon, turning it a dark red-brown color (typically – the color can vary based on atmospheric conditions). As the eclipse begins, Earth's shadow first darkens the Moon slightly. Main article: Lunar eclipse This animated video explains the September 2015 supermoon lunar eclipse.Ī lunar eclipse occurs when the Moon passes within Earth's umbra (shadow). The total lunar eclipse was darker than expected, possibly due to ash left behind from eruptions of the Calbuco volcano in April 2015. The Moon's apparent diameter was larger than 34' viewed straight overhead, just off the coast of northeast Brazil. ![]() The Moon appeared larger than normal, because the Moon was just 1 hour past its closest approach to Earth in 2015 at mid-eclipse, sometimes called a supermoon. Other eclipses in the tetrad are those of 15 April 2014, 8 October 2014, and 4 April 2015. It was the latter of two total lunar eclipses in 2015, and the final in a tetrad (four total lunar eclipses in series). It was seen on Sunday evening, 27 September, in the Americas while in Europe, Africa, and the Middle East, it was seen in the early hours of Monday morning, 28 September. ![]() Uranus, at magnitude 5.7, can be seen in binoculars 16 degrees east of the total eclipsed Moon.Ī total lunar eclipse took place between 27 and 28 September 2015. The Moon crosses Earth's shadow in Pisces, passing west to east (right to left) as shown here in hourly movements. The Moon passes right to left (west to east) through Earth's shadow ![]()
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