A solar eclipse is scheduled for Friday the 13th, but most skywatchers will be out of luck without doing a bit of traveling.
Truth be told, not many people will see this partial eclipse, thanks to its location: The moon’s shadow will mostly fall over the open ocean waters that lie between Australia and Antarctica — the region where the Indian and Pacific oceans merge. The people who will get a chance to see the moon take a small nibble out of the sun include those living in Australia, in a portion of the territories of South Australia and Victoria as well as those living on the island of Tasmania; watchers in New Zealand, on the southern tip of South Island as well as on Stewart Island; and observers located on a slice of East Antarctica. Hobart, Tasmania, will see about 10 percent of the sun’s diameter eclipsed, while Melbourne, Australia, will see barely a nick in the sun’s disk, amounting to just 2.5 percent eclipsed! (Note that the eclipse occurs Thursday, July 12 EDT, but Friday local time and GMT.)
In fact, the greatest eclipse — where only about one-third of the sun’s diameter will be eclipsed by the passing new moon — will occur on Antarctica, near Peterson Bank, where an emperor penguin colony currently exists (although it may not in the future; the colony’s exact location continually changes, due to changing ice conditions). [Solar Eclipse Guide 2018: When, Where & How to See Them]
So, perhaps more penguins than people will witness this eclipse.
We are now into our second eclipse season of 2018. The eclipse seasons are actually less than six months apart, by about 19 days, so they keep falling back that much earlier each year. Last year, periods when eclipses could occur fell in February and August; this year, they have shifted to January and February, and July and August. Next year, they will have shifted back again, so that one will come in January and the second in July. Near the end of the year (Christmas Day), one eclipse will squeeze in to make a third eclipse season.
What is an eclipse season?
It is a span of about a month, during which eclipses are possible at the new and full moons, because the line of the nodes of the moon’s orbit is pointing near enough to the sun. The moon’s orbit is tilted toward Earth’s at an angle of just over 5 degrees, and the nodes are the two points at which the planes intersect — that is, at which the moon passes down or up through the plane that Earth revolves around the sun on, called the ecliptic plane.
Picture the moon’s orbit as a coin held at a slope and remaining in the same orientation as it is carried all the way around the sun. Earth is at the center of the coin; the nodes are the two points on the coin’s rim that are on the same ecliptic plane as Earth. If the moon is anywhere else on the rim, it is too high or too low to cast its shadow on Earth.
The middle of this summer’s eclipse season coincides with a total eclipse of the moon on July 27, and it is so central (the moon will pass almost straight through the middle of Earth’s shadow) that we can also have two «marginal» solar eclipses — the first comes two weeks before the lunar one and the other solar eclipse comes two weeks after.
A small shadow zone
Interestingly, the moon will also be very close to Earth during these celestial events; lunar perigee occurs just over 5 hours after new moon. This actually makes Friday’s solar eclipse cover a yet smaller area of Earth’s surface than it otherwise would, since the penumbra of the moon’s shadow (its outer shadow), unlike the umbra, grows broader, the farther it is from the moon. Meanwhile, the moon’s umbra, from where the great spectacle of a total eclipse would be seen, passes far beyond Earth, but misses the planet by more than one-third of Earth’s radius — for an observer in the Antarctic, that part of the shadow is 1,400 miles (2,200 kilometers) aloft.