On 31 January, 2018 a total eclipse of the Moon will be visible from eastern Europe, eastern Africa, Asia, Australia, the Pacific Ocean and North America. During this lunar eclipse, the full Moon will pass through the Earth’s shadow (or umbra) lasting around 5 hours and 10 minutes from beginning to end.
Eclipse visibility diagram
Although not the deepest of total lunar eclipses, the total phase of the eclipse of January 2018 will last a fairly respectable 1 hours and 17 minutes. The Moon will pass through the Earth’s shadow (or umbra) just underneath its central line.
The Moon will slowly turn from its familiar pearly white color to a reddish colour then back to its original colour all over a period of around five hours. The shade of red can vary from eclipse to eclipse depending on a few factors including conditions in the Earth’s upper atmosphere and the position of the Moon along its orbit. If there have been any significant volcanic eruptions for example, this can cause the eclipsed Moon to appear a much darker red than of other eclipses. The added amount of volcanic ash and dust in the Earth’s atmosphere can block more of the Sun’s light from refracting around the Earth during the eclipse causing deep, dark red effects. The total lunar eclipse on 28 September, 2015 (photographed above) was considered particularly dark and this was not just down to volcanic eruptions or air pollution. The 2015 eclipse was during a perigee Moon when the Moon is closest to the Earth (coining the phrase ‘Supermoon Eclipse’ at the time). This meant that the Moon was deeper in to the Earth’s umbral shadow. The eclipse on 31 January will also co-inside with a perigee Moon (on 30th) once again making this a ‘supermoon eclipse’. It’s hard to predict with certainty how red the eclipse on January 31, 2018 will be. It’s best to wait and see and enjoy any surprises that this eclipse may reveal. During totality, many more stars can be seen than what could be seen during the full Moon. It’s a good photographic opportunity for a wide field shot of the eclipsed moon complimented by a background of stars.
Lunar Eclipse 31 January 2018 Animation
What causes the ‘Blood Red Moon’
During lunar eclipses, the Moon turns an orange-red colour which is the reason why lunar eclipses are sometimes referred to as a Blood Moon. This effect is caused by something called Rayleigh scattering. This is the same effect that causes the sky to look blue during the day and red during sunrise or sunset. During a normal full Moon, the Moon is simply reflecting back light from the Sun when it is on the opposite side of the Earth from the Sun. During a lunar eclipse, the Earth lies directly between the Sun and the Moon meaning the light should be totally blocked. However, some of this light gets scattered and reflected around the Earth’s atmosphere reaching the Moon. As sunlight passes through our atmosphere, the green to violet portion of the light spectrum is filtered out leaving the primarily red light to reach the Moon and reflect back to us. This is what causes the reddish colour of the Moon during a lunar eclipse.
The next Total Lunar Eclipse?
2018 is a good year for total lunar eclipses as the January eclipse is one of two total lunar eclipses to occur in 2018. The next total lunar eclipse takes place on 27 July 2018. More information on our dedicated page.