Start your day early with an eclipse of the full Moon! Before or during dawn on October 8, 2014, a total lunar eclipse will be visible across most of North America.

Image of red Moon during lunar eclipse April 15, 2014
The total lunar eclipse of April 14-15, 2014, was visible all across North America.
Joel D. Tonyan

We’re approaching the second of four total lunar eclipses that come at half-year intervals in 2014 and 2015: a lunar-eclipse tetrad. All four can be seen from at least parts of North America.

The one before dawn on Wednesday, October 8th, will be visible from nearly all of the Americas. Moreover, the Moon, two days after perigee, will be 5% larger in diameter than it was during the first eclipse of the tetrad on April 14-15 earlier this year.

The map, diagram, and timetable below will tell what to expect at your location and when. If you’re in the central or western parts of the U.S. and Canada, you’ll see the total eclipse high in a dark sky well before sunrise. Easterners will find dawn brightening and the Moon sinking low in the west while the eclipse is in progress — offering particularly interesting photo opportunities. Viewers in Australia and eastern Asia get to view this event on the evening of October 8th local date.

If you're stuck under cloudy skies, at least two webcasts are planned. Weather permitting in Los Angeles, Griffith Observatory plans a 4½-hour-long webcast beginning on October 8th at 1:15 a.m. PDT (8:15 UT). Meanwhile, Gianluca Masi has assembled an international team of photographers for his Virtual Telescope Project webcast at 6:00 a.m. EDT (10:00 UT).

For your location, see if the Moon will set or rise during any stage of the eclipse. Because an eclipsed Moon is always full, the Sun rises or sets at almost the same time on the opposite horizon. This means a lunar-eclipse moonset or moonrise always happens in a bright sky.
For your location, see if the Moon will set or rise during any stage of the eclipse. Because an eclipsed Moon is always full, the Sun rises or sets at almost the same time on the opposite horizon. This means a lunar-eclipse moonset or moonrise always happens in a bright sky.
Sky & Telescope illustration

How to Watch the Lunar Eclipse

Stages of the October 8th lunar eclipse
Phases and timings for the total lunar eclipse on October 8, 2014. For North Americans, all phases of the eclipse take place in the hours after midnight through dawn.
Sky & Telescope illustration

A total lunar eclipse has five stages, with different things to watch during each interval over a roughly 3-hour period.

The first penumbral stage begins when the Moon’s leading edge enters the pale outer fringe of Earth’s shadow, the penumbra. But the shading is so weak that you won’t notice anything until the Moon has intruded about halfway into the penumbra. Watch for a slight darkening to become apparent on the Moon’s celestial eastern side. The penumbral shading becomes stronger as the minutes tick off and the Moon moves deeper in.

The second stage is partial eclipse. This begins much more dramatically when the Moon’s leading (eastern) edge enters the umbra, Earth’s central shadow, where no direct sunlight reaches. With a telescope, you can watch the edge of the umbra slowly engulfing one lunar feature after another, as the entire sky grows darker and darker.

An hour or so into partial eclipse, only a final bright sliver of Moon remains outside the umbra. And the rest is already showing an eerie reddish glow.

The third stage is the total eclipse itself, or totality, beginning when the last rim of Moon slips into the umbra. Although the Sun here is completely hidden, the Moon is sure to glow some shade of orange or red. This red light on the Moon is sunlight skimming and bending through Earth’s atmosphere: it’s the light of all the sunrises and sunsets that ring our world at any given moment. An astronaut standing on the Moon would see the Sun hidden and the dark Earth ringed with sunset- and sunrise-colored brilliance.

On rare occasions the eclipsed Moon does go almost black. Other times it appears as bright as a fresh penny. Sometimes it turns brown like milk chocolate.

Two factors affect an eclipse’s color and brightness. The first is simply how deeply the Moon goes into the umbra; the umbra’s center is much darker than its edges.

The other factor is the state of Earth’s atmosphere along the sunrise-sunset line. If the air is very clear, the eclipse is bright. But if a major volcanic eruption has recently polluted the stratosphere with thin global haze, the eclipse will be dark red, ashen gray, or almost black.

In addition, blue light refracted by Earth’s clear, ozone-rich upper atmosphere can also add to the scene, especially near the umbra’s edge, creating a subtle mix of changing colors. Time-lapse videos might show large “flying shadows” in the umbra, caused by changing cloud-shadowing effects around the sunrise-sunset line as Earth turns.

Totality on October 8th lasts 59 minutes. And then, as the Moon continues eastward along its orbit, events replay in reverse order. The Moon’s leading edge reemerges into sunlight, ending totality and beginning stage four: partial eclipse again.

When the entire Moon escapes the umbra, only the last penumbral shading remains for stage five. This final duskiness slowly fades away, leaving the full Moon as bright as ever.

Eclipse event EDT CDT MDT PDT
Penumbra first visible 4:45 a.m. 3:45 a.m. 2:45 a.m. 1:45 a.m.
Partial eclipse begins 5:15 a.m. 4:15 a.m. 3:15 a.m. 2:15 a.m.
Total eclipse begins 6:25 a.m. 5:25 a.m. 4:25 a.m. 3:35 a.m.
Mid-eclipse 6:55 a.m. 5:55 a.m. 4:55 a.m. 3:55 a.m.
Total eclipse ends 7:24 a.m. 6:24 a.m. 5:24 a.m. 4:24 a.m.
Partial eclipse ends 7:34 a.m. 6:34 a.m. 5:34 a.m.
Penumbra last visible? 7:05 a.m. 6:05 a.m.

How To Photograph the Lunar Eclipse

With the prospect of the Moon changing from bright to dull red-orange and back again, don't overlook the possibility of recording this dramatic celestial event with your still or video camera! Photographing a total lunar eclipse isn't difficult — but it does take a little preparation.

Total lunar eclipse of April 14-15, 2014
Alberto Levy captured last April's total lunar eclipse over a period of 3½ hours from his backyard in San Diego. He used a 4-inch f/8 refractor and exposures ranging from 11200 to 2 seconds at ISO 400.

Most importantly, you'll need a telescope or telephoto lens that enlarges the Moon to a good size. The minimum focal length for getting a good-looking Moon is about 300 mm. You'll also need a tripod to keep your camera rock-steady, or you can piggyback your camera on a tracking telescope mount.

Because the coloration and brightness of eclipsed Moon is different every time it plunges through the umbra — and even during totality itself — the best advice for photographing a lunar eclipse is to take lots of pictures at many different exposures. Count on using times of ½ second or longer during totality, so make sure your camera is able to make exposures that long, preferably in "manual" mode. Use a remote control (or the self-timer function) to minimize vibration during the exposures.

S&T's imaging experts offer more great tips on how to photograph a lunar eclipse elsewhere on this website.

Uranus Too!

Finding Uranus during October's lunar eclipse
During October's lunar eclipse, the planet Uranus will be nearby. The Moon’s position might vary a bit; it’s plotted here for an observer in the middle of North America at the start of totality. Click on the image for a large, black-on-white version for use outside.
Sky & Telescope illustration

By quite a coincidence the planet Uranus, just one day past opposition and thus shining its brightest at magnitude 5.7, will appear only about 1° from the Moon during totality. Spot it in binoculars using the finder chart at right.

The actual position of the eclipsed Moon against the starry background in Pisces will depend slightly on where you are and the stage of the eclipse. The Moon on the chart is positioned for the middle of North America at the start of totality, but elsewhere the difference won't be more than a couple of Moon diameters at most. You should have no trouble finding the 4½-magnitude stars Epsilon (ε) and Delta (δ) Piscium north of the Moon. Identify Uranus by the shape of the triangle it makes with those two stars.

Can you see anything of Uranus's aquamarine blue-green tint? Color contrast with the vivid orange-red Moon might make this more apparent. In a telescope, Uranus is a tiny disk 3.7 arcseconds wide. It's 2.6 light-hours from Earth, compared to the Moon's distance of 1.2 light-seconds.

Want to know more about the Moon? Look to the Sky & Telescope Moon Globe for all the details!


Image of Glenn


September 26, 2014 at 6:14 pm

The position of the moon against the starry background varies by a maximum of over 4 lunar diameters - that's 2 degrees. This will be quite noticeable in all the pix that will show Luna close to Uranus. A combination of the latitude of the observer and the time during the eclipse when the photo is taken will give a variety of separations between the two bodies. Indeed the planet will be occulted as seen from NE Asia, northern Greenland and the Arctic Ocean. Anyone able to take a pic of the Uranian disc half covered by the edge of the moon? .... G

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Image of Glenn


September 26, 2014 at 6:28 pm

Note to Eds. Downunder totality is on the evening of 8th October. There are a couple of glitches in the text above saying the 14th.

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Image of Alan MacRobert

Alan MacRobert

October 2, 2014 at 11:06 am

> ...glitches in the text above saying the 14th.
--Alan MacRobert

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Image of Graham-Wolf


October 8, 2014 at 6:38 pm

Partially successful last night from Hutt Valley, New Zealand. Afocal photos were undertaken at 170x, Danjon estimates made, and crater shadows timed. Local conditions frequently alternated between light haze and total overcast!

11:00 2.6
11:12 2.8
11:16 2.4
11:20 3.6
11:23 3.2
11:24 2.8

At Danjon max, the eclipsed moon took on the wonderful appearance of bright orange glowing coals... similar to what one would see in the firebox of a grand old steam train!

Regards to all from NZ.

Graham W. Wolf
Barber Grove Observatory (BGO)

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Image of Robert Victor

Robert Victor

October 5, 2014 at 8:45 pm


In the timetable for the total lunar eclipse, in the column for Pacific Daylight Time,
the start of totality is given as 3:35 a.m. PDT. It should be 3:25 a.m. PDT, or
1 hour 10 minutes after the Moon enters the umbra, consistent with the
data given for other time zones.

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October 8, 2014 at 8:54 am

October 8, 2014 (Dallas, TX)
Danjon Scale of Lunar Eclipse Brightness
Luminosity of Total Lunar Eclipse as observed today.
L = 1 Dark Eclipse, brownish in coloration. Moon details distinguishable only with dificulty.

William Mach

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Image of neil


October 9, 2014 at 5:15 am

I was interested to know how does the visibility change with elevation. I am in a location where moon rises with leaving umbra but I managed to clicked this from flight from my flight

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