North America Favored for This Week’s Deep Partial Lunar Eclipse
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Contacts:
Diana Hannikainen, Observing Editor, Sky & Telescope
+1 617-500-6793 x22100, diana@skyandtelescope.org
Gary Seronik, Consulting Editor, Sky & Telescope
gseronik@skyandtelescope.org
Susanna Kohler, Communications Manager and Press Officer, American Astronomical Society
+1 202-328-2010 x127, susanna.kohler@aas.org
Note to Editors/Producers: This release is accompanied by high-quality graphics; see the end of this release for the images and links to download.
Very late Friday night and early Saturday morning, you have a chance to watch the Moon darken and turn a reddish hue as it slips into Earth’s shadow. However, unlike the total lunar eclipse on May 26th this year, the November 18–19 event is a partial eclipse. But it’s a very deep one: About 97% of the Moon’s disk will pass through the umbra — the dark inner part of Earth’s shadow — leaving a tiny, silvery sliver of the Moon’s southern edge peeking out.
Weather permitting, viewers across almost all of North America will witness the entirety of the event. November’s eclipse favors night owls and early risers, because the full Moon passes through the umbra after midnight on November 19th for the four main U.S. time zones, and mid-eclipse occurs in the wee hours of the morning (at 4:03 a.m. EST and 1:03 a.m. PST). For Hawai’i and Alaska, the event starts to unfold before midnight.
Northeasternmost Asia will also see the entire event. In South America the eclipse happens as dawn is brightening, while for most of Australia the Moon will already be eclipsed as it rises. Much of western Europe should see the early penumbral stages before the Moon dips below the horizon.
What to Look For
The partial eclipse is predicted to last longer than usual, nearly 3½ hours. In fact, not only will it be the longest partial lunar eclipse this century, it’s also the longest partial lunar eclipse between February 18, 1440, and February 8, 2669. It happens 1.7 days before the Moon reaches its apogee, or the farthest point from Earth, in its orbit. This means that the Moon’s orbital motion will be slower, thereby increasing the duration of the event.
“The Moon will be in Taurus and pleasingly placed some 6° — approximately the width of three fingers held together at arm’s length — lower left of the pretty Pleiades open star cluster at the time of maximum eclipse,” says Diana Hannikainen (pronounced HUHN-ih-KY-nen), observing editor at Sky & Telescope. “This should provide great opportunities for some fun photos.”
The stages of the eclipse occur simultaneously for everyone who can see the Moon, but the actual clock times depend on your time zone. See the table below and diagrams at the end for times of key events for the lunar eclipse:
| Eclipse Event | UT | AST | EST | CST | MST | PST | AKST | HST |
| Penumbra first visible | 6:00 | 2:00 a.m. | 1:00 a.m. | 12:00 a.m. | *11:00 p.m. | *10:00 p.m. | *9:00 p.m. | *8:00 p.m. |
| Partial eclipse begins | 7:18 | 3:18 a.m. | 2:18 a.m. | 1:18 a.m. | 12:18 a.m. | *11:18 p.m. | *10:18 p.m. | *9:18 p.m. |
| Maximum eclipse | 9:03 | 5:03 a.m. | 4:03 a.m. | 3:03 a.m. | 2:03 a.m. | 1:03 a.m. | 12:03 a.m. | *11:03 p.m. |
| Partial eclipse ends | 10:47 | 6:47 a.m. | 5:47 a.m. | 4:47 a.m. | 3:47 a.m. | 2:47 a.m. | 1:47 a.m. | 12:47 a.m. |
| Penumbra last visible | 12:06 | — | 7:06 a.m. | 6:06 a.m. | 5:06 a.m. | 4:06 a.m. | 3:06 a.m. | 2:06 a.m. |
Mechanics of a Lunar Eclipse
A lunar eclipse happens when the Sun, Earth, and a full Moon form a near-perfect lineup in space, in what is known as syzygy. The Moon gradually glides into Earth’s shadow, until most of the lunar disk turns from silvery grey to an eerie dim orange or red. Then events unfold in reverse order, until the Moon returns to full brilliance.
The events that happen during a total lunar eclipse are more complex and interesting than many people realize. The eclipse occurs in five stages, each with different things to watch.
(1) The Moon’s leading edge enters the pale outer fringe of Earth’s shadow: the penumbra. You probably won’t notice anything until the Moon is about halfway across the penumbra. Watch for a slight darkening on the Moon’s leading edge. The penumbral shading becomes stronger as the Moon moves deeper in.
The penumbra is the region where an astronaut standing on the Moon would see Earth covering only part of the Sun’s disk.
(2) The Moon’s leading edge enters the umbra, the cone of Earth’s shadow within which the Sun’s completely hidden. You should notice a dramatic darkening on the upper left edge of the lunar disk as seen from North America. With a telescope, you can watch the edge of the umbra slowly engulfing one lunar feature after another, as the entire sky begins to grow darker.
(3) The trailing edge of the Moon slips into the umbra for the beginning of maximum eclipse. The Moon will glow some shade of coppery red or burnt orange.
Why is this? The Earth’s atmosphere scatters and bends (refracts) sunlight that skims its edges, diverting some of it onto the eclipsed Moon. It’s the same effect that happens at sunset. If you were on the Moon during a lunar eclipse, you’d see the Sun hidden by a dark Earth rimmed with the reddish light of all the sunrises and sunsets ringing the world at that moment.
The red umbral glow can be quite different from one eclipse to the next. Two main factors affect its brightness and hue. The first is simply how deeply the Moon goes into the umbra as it passes through; the center of the umbra is darker than its edges. The other factor is the state of Earth’s atmosphere. If a major volcanic eruption has recently polluted the stratosphere with thin global haze, a lunar eclipse can be dark red, ashen brown, or occasionally almost black.
In addition, blue light is refracted through Earth’s clear, ozone-rich upper atmosphere, above the thicker layers that produce the red sunrise-sunset colors. This ozone-blue light tints the Moon also, especially near the umbra’s edge, but you’ll need binoculars or a telescope to see this effect.
During this deep partial, a sliver of the southern edge of the Moon’s disk will shine brightly even at mid-eclipse.
(4) As the Moon continues moving along its orbit, events replay in reverse order. The sliver of light will grow and expand upwards along the Moon’s leading edge.
(5) When all of the Moon escapes the umbra, only the last, penumbral shading is left. Some time later, nothing unusual will remain visible.
“You only need your eyes to see the drama unfold, but if you have binoculars or a backyard telescope, they’ll give a much-enhanced view,” says Hannikainen.
Read more on this eclipse in the November 2021 issue of Sky & Telescope and on S&T‘s website: A Near-Miss Total Lunar Eclipse.
If it’s cloudy where you are, you can follow a live stream of the eclipse on the Virtual Telescope website starting at 7:00 UT on November 19th.
Sky & Telescope is making the illustrations below available to editors and producers. Permission is granted for nonexclusive use in print and broadcast media, as long as appropriate credits (as noted) are included. Web publication must include a link to skyandtelescope.org.
Gregg Dinderman / Sky & Telescope; Source: USNO
Gregg Dinderman / Sky & Telescope; Source: USNO
Sky & Telescope
Sky & Telescope
Bob King
For skywatching information and astronomy news, visit SkyandTelescope.org or pick up Sky & Telescope magazine, the essential guide to astronomy since 1941. Sky & Telescope and SkyandTelescope.org are published by the American Astronomical Society, along with SkyWatch (an annual beginner’s guide to the night sky) as well as books, star atlases, posters, prints, globes, apps, and other products for astronomy enthusiasts.
The American Astronomical Society (AAS), established in 1899, is a major international organization of professional astronomers, astronomy educators, and amateur astronomers. Its membership of approximately 8,000 also includes physicists, geologists, engineers, and others whose interests lie within the broad spectrum of subjects now comprising the astronomical sciences. The mission of the AAS is to enhance and share humanity’s scientific understanding of the universe as a diverse and inclusive astronomical community, which it achieves through publishing, meetings, science advocacy, education and outreach, and training and professional development.
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