Solar and Lunar Eclipses in 2018

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Two total lunar eclipses occur this year, the first since late 2015, in January and July. Meanwhile, three solar eclipses take place in 2018 — all of them only partial cover-ups.

By Kelly Beatty

If you’re one of the estimated 154 million U.S. adults who watched the solar eclipse on August 21, 2017 — and that’s most of us! — you know how incredible such events can be. So when will the ones in 2018 occur? Read on to find out!

Up to seven eclipses of the Sun and Moon can take place in one year, though the last time that happened was 1982, and the fewest possible is four. This year we’ll get three solar eclipses (alas, all partial events) and two total lunar eclipses spaced six months apart.

Why Do Eclipses Happen?

Eclipses of the Sun or Moon can only occur when the Moon crosses the plane of Earth’s orbit (orange circle) very close to the time of new or full Moon. [Jay Anderson]

A solar eclipse, such as the one in August 2017, occurs only at new Moon, when the lunar disk passes directly between us and the Sun and the Moon’s shadow falls somewhere on Earth’s surface.

Conversely, a lunar eclipse takes place during full Moon, when our satellite passes through Earth’s shadow.

These alignments don’t happen at every new and full Moon because the lunar orbit is tipped about 5° to Earth’s orbital plane — only occasionally do the Sun, Earth, and Moon line up exactly enough for an eclipse to occur. (The technical name for that, by the way, is syzygy.)

Three types of lunar eclipse are possible (total, partial, and penumbral) depending on how deeply the full Moon plunges into or near the umbra, our planet’s dark, central shadow.

A long-exposure image captured red hues on the portion of the Moon inside the umbra during the lunar eclipse on October 8, 2014. [Johnny Horne]

If it goes all the way in, we see a total lunar eclipse that’s preceded and followed by partial phases. That was the case during the widely viewed event in September 2015, which marked the conclusion of a series of four consecutive total lunar eclipses in 2014–15! Such eclipse tetrads are not common — the last one occurred during 2003–04, but the next won’t begin until 2032.

If the Moon skims part way into the umbra, as shown at right, only the partial phases occur — you’ll see part of the Moon in nearly full sunlight, and part of it steeped in the deep, red-tinged umbral shadow.

And if its disk passes just outside the umbra, it still encounters the weak penumbral shadow cast by Earth. A sharp-eyed observer will notice that one side of the full Moon’s disk looks a little dusky.

Fortunately, every lunar eclipse is observable anywhere on Earth where the Moon is above the horizon. (But there’s still an element of luck involved — after all, the sky has to be clear!)

However, solar eclipses more tightly restrict where you can see them because the Moon casts a smaller shadow than Earth does.

If the Moon completely hides the Sun, the eclipse is considered total. With its brilliant disk completely covered, the Sun’s ghostly white outer atmosphere is momentarily revealed for durations from seconds to several minutes. In November 2013, for example, planeloads of eclipse-chasers converged in a remote portion of northern Kenya to watch just 11 seconds of totality.

Here’s how the corona looked during the total solar eclipse seen across the U.S. on August 21, 2017.
[Sky & Telescope / Kelly Beatty]

A completely eclipsed Sun can be viewed only from a narrow track or path on Earth’s surface that’s typically just 100 miles (160 km) wide. Outside of that path, about half of the daylit hemisphere of Earth is able to watch a partialeclipse as the Moon obscures a portion of the Sun.

Occasionally the Moon passes directly in front of the Sun but doesn’t completely cover it. When that occurs, it’s usually because the Moon is farther from Earth than its average distance. (The Moon’s orbit isn’t perfectly circular; its eccentricity is about 5%.)

This geometric circumstance is known as an annular eclipse, so-called because you can see a ring, or annulus, of sunlight surrounding the lunar disk. Annular eclipses of the Sun occur about as often as the total ones do, and an annular’s path is likewise narrow. Outside of it observers see only a partial cover-up.

The Five Eclipses in 2018

Below are brief descriptions of this eclipses in 2018 of the Sun and Moon. You’ll find more details Sky & Telescope magazine as the date of each draws near. Times are in Universal Time (UT) except as noted. Adjust these to get those for your time zone (e.g. PST = UT – 8, EST = UT – 5).

January 31: Total Lunar Eclipse

This plot shows key events in the total lunar eclipse on January 31, 2018. [S&T / Leah Tiscione]

It’s been more than two years since we’ve experienced a total lunar eclipse — the last one was September 27–28, 2015— and skygazers are ready for another! As the graphic at right shows, the eclipse will last almost 3½ hours from the beginning of the partial phase at 11:48 UT until it ends at 15:12 UT. Totality lasts a generous 77 minutes, from 12:51 to 14:08 UT.

The timing of this one, with mid-eclipse at 13:30 UT, favors locations around the Pacific Rim: not long after sunset for eastern Asia and Australia; around midnight for Hawaii; and and before dawn for western North America. This animation by Larry Koehn shows how the event plays out for the principal North American time zones, plus Hawaii.

But not all of the U.S. will enjoy the show. As the map below shows, totality occurs in the hours before dawn for those on the West Coast, but it happens after moonset (and sunrise) for those east of the Mississippi River. In fact, those as far east as Boston won’t get to see more than a small umbral nibble on the lunar disk. More information about this eclipse.

January’s lunar eclipse is observable from a wide area surrounding the Pacific Ocean. However, for those in the U.S. situated roughly east of the Mississippi River, the Moon sets before totality begins.
[S&T / Leah Tiscione]

February 15: Partial Solar Eclipse

All three of this year’s partial solar eclipses occur deep in the Southern Hemisphere. The first one is ideal if you’re a penguin — the maximum (60% of the Sun’s diameter covered) occurs at 20:51 UT along the coast of Queen Maud Land abutting the South Atlantic Ocean. Most Chileans and Argentinians will see up to 40% of the Sun covered. Those of you at the South pole will see the Moon cover 51% of the solar disk’s area. More information about this eclipse.

Note that solar-eclipse predictors compute the Sun’s blockage during partial eclipses in two ways. Magnituderefers to the fraction of the solar disk’s diameter that is covered by Moon, whereas obscuration corresponds to the fraction of the disk’s area that’s covered. So, for example, at this eclipse’s maximum as seen from Buenos Aires, the magnitude is 17% but the obscuration is only 8%.

July 13: Partial Solar Eclipse

The viewing prospects are even worse for this partial solar eclipse, because the Moon’s shadow clips Earth between the the coasts of Australia and Antarctica. France’s Dumont d’Urville scientific station on the Antarctic coast should enjoy this event’s “greatest eclipse,” when a third of the Sun’s diameter is covered at 3:01 UT. Residents of Hobart, Tasmania, will see their biggest small bite in the Sun at 3:35 UT. More information about this eclipse.

July 27: Total Lunar Eclipse

The total lunar eclipse, on July 27, 2018, is timed perfectly for those in the Eastern Hemisphere — but won’t be seen from North America.
[Fred Espenak / eclipsewise.com]

Two weeks after the new Moon involved in a July 13th’s partial solar eclipse, the full Moon takes a deep dive through Earth’s umbra for the second time this year. Mid-eclipse on July 27th comes at 20:22 UT, which unfortunately is in the midst of daylight across North America.

But it will be a grand show across Europe, Africa, Asia, and Australia. The partial phases run from 18:24 to 22:19 UT, nearly 4 full hours, which results from two factors. First, the Moon passes directly through the heart of Earth’s umbral shadow, just 6 arcminutes from its center. Second, the Moon is very nearly its most distant from Earth, near the apogee of its orbit, resulting in a slightly diminished orbital velocity. Totality lasts a generous 1¾ hours, from 19:30 to 21:13 UT. More information about this eclipse.

August 11: Partial Solar Eclipse

Two weeks later, with the Moon having moved halfway around its orbit and once again new, another partial solar eclipse takes place — the third and final one in 2018. This time the geometry shifts from extreme southern latitudes to extreme northern ones. Greatest eclipse, at 9:46 UT, takes place off the northern coast of Siberia at a latitude of 70.4° north, well above the Arctic Circle. From that location one could see 74% of the Sun’s diameter covered.

Much of Scandinavia, Russia, and eastern Asia enjoy a partial eclipse that day. The maximum obscuration is 30% in Ulaanbatar, Mongolia; 23% in Beijing and Novosibirsk; and just 1% in Stockholm. More information about this eclipse.

Looking Ahead to 2019

The mix of events gets more interesting next year, with three different flavors of solar eclipse — one each of partial, annular, and total — and partial and total lunar eclipses. The Moon’s deep umbral dive on January 21, 2019, will offer ringside seats for skywatchers in North and South America.

J. Kelly Beatty, S&T’s Senior Editor, joined the staff of Sky Publishing in 1974 and specializes in planetary science and space exploration. Learn more about him here.

This article (Solar and Lunar Eclipses in 2018) was originally published on Sky & Telescope and syndicated by The Event Chronicle

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