There are two main types of eclipse namely Solar or Lunar eclipses (eclipses of the Sun and eclipses of the Moon). These eclipses can be broken down further in to various types of partial and total eclipse. Below is an outline of these eclipse types starting with lunar eclipses.
Penumbral Lunar Eclipse
Penumbral lunar eclipses are very subtle and can sometimes go un-noticed depending on how deep they go in to the penumbra. During these eclipses the Moon only ‘brushes’ with the Earth’s outer shadow. Of course these are witnessed as the first stages of a partial or total lunar eclipse as well but sometimes lunar eclipses occur that are only ever penumbral. A very slight darkening of one side of the full Moon is seen which then slowly progresses around the edge of the Moon before a full Moon is restored.
Partial Lunar Eclipse
Partial lunar eclipses can be seen during the build up to a total lunar eclipse or when there is an eclipse of the Moon that will only ever be partial. The Moon enters the penumbra and then part of the Earth’s primary shadow called the umbra but this shadow does not completely cover the Moon. There is an illustration of these two shadows further down the page. Only the Earth’s outer shadow (the Penumbra) covers all of the Moon making the full Moon more dimmer. The side of the Moon in the Umbra will darken quite considerably as shown in the image above.
Total Lunar Eclipse
This is what will be witnessed on 31 January and 27 July 2018. The Moon will first move in to the Earth’s outer shadow (penumbra) then passes right in to the Earth’s central shadow (Umbra). The full Moon will darken considerably once it reaches this phase. The colour of the Moon varies from eclipse to eclipse which is explained further on our eclipse 2018 main page. Below is an illustration showing the two shadows cast by the Earth and how the Moon’s position creates these different types of lunar eclipse.
Partial Solar Eclipses
This type of eclipse is witnessed during the build up to a total solar eclipse, annular solar eclipse or just during an eclipse that will only ever be partial. Often seen from a large area of Earth, these types of solar eclipses are seen more often than any. This is mainly due to the fact that the Moon’s distance from Earth is irrelevant to us on Earth during these events. If a partial eclipse is going to happen, a big chunk of Earth will witness it. Appearing to take a ‘bite’ out of the Sun, the Moon obscures the Sun’s disc. During sunrise or sunset, partial eclipses can be quite picturesque.
As the illustration later below shows, a partial eclipse is observed from Earth when it is in the Moon’s outer shadow or ‘Penumbra’. The ever-so-slight darkening caused by the ‘Penumbral Shadow’ is hardly noticeable. It’s the point between full sunlight and complete shadow from the Moon. The Sun’s light is so brilliant that even when partially obscured, it is difficult to notice a darkening in surrounding light (despite the obvious ‘bite’ of the Sun in the sky). Even when 60% obscured, things can seem normal.
Annular Solar Eclipse
An annular solar eclipse is much more rare than a partial solar eclipse. Even though a partial eclipse is seen by many during these events, the annular phase is only seen in a narrow corridor across the Earth. What causes the ‘ring in the sky’ is down to the elliptical orbit of the Moon. There are times when the new moon is located further away from Earth than at other times. The point at when it is furthest away is called ‘apogee’. If a full eclipse of the sun happens around this time, an annular solar eclipse is witnessed due to the Moon appearing slightly smaller than the Sun. This means that the main shadow of the Moon, the umbra, does not reach the Earth, allowing sunlight to peer around the complete circumference of the Moon.
During these events, a noticeable darkening of the sky can be seen but not to the dramatic extent that a total solar eclipse can.
Total Solar Eclipse
Aa total solar eclipse is the rarest of the three solar eclipse types mentioned. In order for this event to happen, the Moon must be at new phase and not be near apogee in its orbit around the Earth. Much like the annular eclipse, only a select few will be able to witness the event in a narrow corridor which stretches across the Earth from West to East. Most area’s of the Earth will be located outside of this ‘path of totality’. However, a much larger area of Earth will be able to see the partial phase of the eclipse as the illustration below shows.
It’s commonplace to hear that solar eclipses are rare. However, on average there are 2.4 solar eclipses every year visible from somewhere on the Earth. This number includes the 3 types of solar eclipse mentioned above, total, annular and partial. A total solar eclipse is visible from somewhere on Earth approximately every 18 months. It is rare to witness a total solar eclipse as the total phase of the eclipse is only visible from a narrow corridor across the Earth’s surface. Therefore, to witness a total solar eclipse without travelling far to see it is considered rare.
Lunar eclipses are more common and are visible 2 to 4 times a year from somewhere on Earth. Lunar eclipses are also visible from a much larger geographical area of Earth for as long as the Moon is risen in the sky during the time of the eclipse, anyone can witness it, regardless of location (weather permitting). This effectively means around half the planet can witness some part of the eclipse. The total phase of the eclipse lasts much longer by comparison to the few minutes of a total solar eclipse. The total phase of an eclipse of the Moon can often last up to an hour or more with the whole eclipse lasting over 3 hours.