The Moon will pass in front of the Sun, creating a solar eclipse. However, the alignment will not be very exact, so the Moon will only partially cover the Sun, and nowhere on Earth will see a total eclipse.
The path of the eclipse will pass through numerous countries, including:
|Country||Extent of eclipse|
|Finland||Sun 61% covered|
|Norway||Sun 61% covered|
|Russia||Sun 61% covered|
|Sweden||Sun 61% covered|
|Estonia||Sun 59% covered|
|Aland Islands||Sun 59% covered|
|Latvia||Sun 58% covered|
From United States, no eclipse will be visible. To see information about the times when the eclipse will be visible elsewhere in the world, select a different location.
Solar eclipses occur when the Sun, Moon and Earth are aligned in an almost exact straight line, with the Moon in the middle, such that the Moon passes in front of the Sun.
The Moon passes close to the Sun in the sky every month, at new moon, but because the Moon's orbit is tipped up by 5° relative to the Earth's orbit around the Sun, the alignment usually isn't exact. As a result, the Moon usually passes a few degrees to the side of the Sun.
Even when eclipses do occur, they are not visible from the whole world at once. The Moon casts a circular shadow onto the Earth, but because the Moon is much smaller than the Earth, the shadow doesn't cover the whole planet. Over time, the shadow sweeps across the Earth, so that different places see the eclipse at different times.
The simulation to the right shows the path of the Moon's shadow across the Earth.
The red line shows the edge of the Moon's shadow: all places inside the red circle will see the Moon covering some part of the Sun's disk. The white contours within this show where the Moon appears to cover 20%, 40%, 60% and 80% of the Sun.
The white spot in the centre of the Moon's shadow traces out where you would need to be in space to see a total eclipse. Because this is only a partial eclipse, it does not cross the Earth's surface at any point.
Below, the path of the Moon's shadow is reprojected onto a flat map of the world. As before, the red contour shows the edge of the Moon's shadow, and encloses everywhere where the eclipse can be seen. The white contours show where the Sun is 20%, 40%, 60% and 80% covered.
The map below shows a still image mapping the maximum extent of the eclipse across the world. The red contour encloses all places in which any part of the eclipse is visible.
Observing the Sun can be very dangerous if it is not done with the right equipment. The Sun is the brightest object in the sky, and looking directly at it can cause permanent eye damage within seconds. Viewing it through any optical instrument – even a pair of binoculars or the finderscope on the side of your telescope – can cause instant and permanent blindness.
If you have any doubts about whether your equipment is safe, it is best not to risk using it. By far the safest thing to do is to go along to a public observing event. Many astronomical societies are likely to be hosting observing events on the day, and they'll be sure to welcome newcomers. You may meet some new people at the same time as seeing the transit.
Many astronomy suppliers sell special special filters which are made for safe solar viewing. These include aluminised mylar filters, or black polymer filters, identified as suitable for direct viewing of the Sun. Check that the filter has a CE mark, and a statement that it conforms to European Community Directive 89/686/EEC. Alternatively, you can use a welder's glass rated at No. 14 or higher. Always read the manufacturer's instructions carefully.
Never attempt to make your own filter. In addition to visible light, the Sun also produces prodigious amounts of infrared and ultraviolet radiation which cannot be seen yet can still damage your eye. Even if a homebrew filter appears adequate, it may allow this unseen radiation to pass.
Projecting an image of the Sun
Another safe way to view solar eclipses is to buy a purpose-built solar projection box.
These typically consist of a cardboard box with a small lens on one side. They project an enlarged image of the Sun onto a white cardboard sheet inside the box. Once the transit is over, they're also great for observing sunspots. They are safe to use, quick to set up, and ideal for use with children and groups.
This eclipse is a member of Saros series 122. The position of the Sun at the moment of greatest eclipse will be:
|Object||Right Ascension||Declination||Constellation||Angular Size|
The coordinates above are given in J2000.0.
|The sky on 17 March 2018|
All times shown in EDT.
Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.
The simulations above were derived from the DE405 ephemeris published by the Jet Propulsion Laboratory (JPL). The position of the Moon's shadow is superimposed on maps of the world taken from the NASA Visible Earth project.
The list of countries from which the eclipse is visible was computed on the basis of shape files available from DIVA-GIS.
Additional information was taken from:
Espanak, F., & Meeus, J., Five Millennium Canon of Solar Eclipses: -1999 to +3000, NASA Technical Publication TP-2006-214141 (2006)
You may embed the animations and images above in your own website. They are licensed under the Creative Commons Attribution 3.0 Unported license, which allows you to copy and/or modify them, so long as you credit In-The-Sky.org.
|16 Jan 2037, 04:36 EST||– New Moon|
|24 Jan 2037, 09:57 EST||– Moon at First Quarter|
|31 Jan 2037, 09:05 EST||– Full Moon|
|07 Feb 2037, 00:45 EST||– Moon at Last Quarter|
© Jerry Kickhart, Los Osos, California.