Contributor Post Created with Sketch. Saturday Night Science: Final Totality

 

perimoonOne of the most remarkable celestial coincidences is that the Moon and Sun — as viewed from the Earth — have almost the same apparent size. Depending on its position in orbit, the Moon can appear either larger or smaller than the Sun, resulting in solar eclipses on Earth occurring in two varieties: total, when the Moon is close enough to appear larger than Sun and completely cover it, and annular, where a more distant Moon fails to completely cover the Sun’s photosphere, resulting in a “ring of fire”.

This size coincidence is striking, especially since it hasn’t always been the case, nor will it be the case forever. Billions of years ago, the Moon was much closer to the Earth and total eclipses were far more common, yet less spectacular because the Sun’s corona and prominences wouldn’t have been visible all around the Sun. Eventually, tidal-driven recession of the Moon from the Earth will put an end to total solar eclipses visible from Earth and all subsequent eclipses will be annular. Some have actually argued that the closely comparable apparent sizes of the Sun and Moon have contributed in some way to the evolution of human intelligence, providing an “anthropic” explanation of why we happen to be observing such a marvel at the epoch in geological time when it happens to occur.

apm1In the first week of July, 2004 three completely unrelated celestial phenomena occurred within days of one another: the full Moon, the passage of the Moon through perigee (the moment when it most closely approaches the Earth), and the passage of the Earth through aphelion—its greatest annual distance from the Sun. Thus, the full Moon occurred less than 12 hours after lunar perigee, and only three days later the Earth arrived at aphelion. The coincidence of these events permitted taking photographs of the perigean full Moon and the Sun near aphelion, all with the same camera and optics, to illustrate the difference in the apparent sizes of the Sun and Moon in these circumstances.

Such a close coincidence of all three events is relatively rare. I checked all years between 2000 and 2100 for full moons within 24 hours of perigee occurring in the first ten days of July (aphelion always falls on July 3 through 6). By this definition, perigean full Moons near aphelion occur 5 times in this century, in 2004, 2031, 2058, 2066, and 2093. You can search for such events in other time periods using my Lunar Perigee and Apogee Calculator. The far more rare four-way coincidence of new Moon, perigee, aphelion, and the Moon’s crossing a node of its orbit produces solar eclipses with the longest duration of totality, such as the extraordinary eclipse of July 11, 1991, whose 6 minute 53 second totality will not be exceeded until the eclipse of June 13th, 2132, with two seconds more totality.

Amazingly, there were three solar eclipses in the 20th century with even longer totality: the eclipses of 1937, 1955, and 1973—all comfortably within a single human lifespan—each exceeded seven minutes. To put this into context, the last seven-minute-totality eclipse before 1937 was in the year 1098 (July 1st), and the next won’t occur until June 25th, 2150, the opening act for the Big Show on July 16th, 2186, when there’s an eclipse with 7 minutes and 29 seconds of totality! This is the solar eclipse with longest totality in the entire 8000 year interval from 3000 B.C. to A.D. 5000. Me, I’m signing up for the expedition right away—this one is sure to sell out!

The tables below give the date and time the pictures of the Sun and Moon were taken, and the distance and angular extent of each body at that time.

apm2

apm3

Even though the photo of the Sun was taken two days before aphelion, the appearance of the Sun in an image at this scale is indistinguishable from one shot precisely at the moment of aphelion; Earth takes a whole year to traverse its orbit, which has an eccentricity of only 1.67%, so a couple of days don’t make much difference. The Sun was rather featureless at the time of this photo—we were heading toward the trough in the solar activity cycle, so there weren’t any spectacular naked-eye sunspots, only the modest active region 0639 near the centre of the disc.

Moon Near Apogee, Earth Near Perihelion

apmoon_perisunTwo near-apogean full Moons on either side of the Earth’s perihelion passage on January 2nd, 2005 provided opportunities to photograph the converse case: Moon near apogee and Earth near perihelion. I had originally aimed for the full Moon of December 26th, which is only a little more than 24 hours before lunar apogee and a week before the Earth reaches perihelion. Planning a photo like this six months in advance amounts to daring the sky to do its worst, and the last week in December the sky took the dare and delivered a steady menu of clouds, howling wind, and precipitation.

The fall-back opportunity was the full Moon of January 25th, which occurred less than two days after apogee on the 23rd. This isn’t as close to perihelion as the December opportunity would have been—about three weeks away from perihelion instead of one, but for practical purposes it’s close enough; at the time of lunar apogee on the 23rd, the Earth would be only 156,000 kilometers further from the Sun than at perihelion, which is just 3% of the distance from perihelion to aphelion. The difference in apparent size of the Sun would barely be perceptible.

The weather didn’t look very promising in the run-up to the January 23–25 opportunity either, but shortly before sunset on the 23rd, the snow stopped and the Sun popped out between the clouds. I grabbed the camera and lens, already mounted on the tripod in the hope of exploiting such an opportunity, dashed outside, planted the tripod in the snow, and shot a sequence of pictures of the Sun through the solar filter. The two visible sunspot groups (NOAA Active Region 0726 near the centre of the disc and 0725 near the solar limb) helped in focusing. From the extensively bracketed sequence of images, I chose one taken at 1/80 second with sensitivity set to ISO 200. The Sun looks somewhat “lumpy” due to refraction through the turbulent atmosphere so near to sunset.

apm6

After shooting the Sun, I turned to the Moon, which was rising in a pellucid sky in the East. While the Moon wouldn’t be full until 10:33 UTC on January 25th, it was already 97% full, and only three hours before perigee (18:55 UTC). I whipped off the solar filter, centred the Moon, and shot a sequence of exposures at various shutter speeds. The image I chose from the set was taken at 1/500 second with ISO 200 sensitivity.

apm7

apm8

Final Totality

totalNothing lasts forever. After some date in the distant future, there will be no more total solar eclipses—only annular eclipses where the Moon fails to completely cover the Sun. Our distant earthbound descendants will be forever deprived of one of nature’s greatest spectacles. Why? Because of the tides in the ocean.

Really! As the Moon raises tides in the ocean (and to a lesser extent in the solid Earth), and the tides wash up on the shores of the continents, Earth’s rotation gradually slows, transferring its rotational angular momentum to the orbit of the Moon, which in turn causes the Moon to steadily recede from the Earth. The gradual slowing of the Earth’s rotation was discovered by Edmond Halley in the 18th century by noting discrepancies between the location of solar eclipses recorded in history and predictions based on the assumption of an unchanging length of day.

In 1754, Immanuel Kant correctly identified tidal friction as the cause of the lengthening day, and further predicted lunar recession as a consequence. Lunar recession was subsequently confirmed by precision measurement of the Moon’s orbit. The Apollo 11, 14, and 15 lunar landing missions in 1969 and 1971, and the Soviet Lunokhod 2 robotic rover in 1973 placed retro-reflectors at various sites on the Moon which permit Lunar Laser Ranging with a precision of a few centimeters. This has permitted the present-day lunar recession rate to be measured as 3.82±0.07 centimetres per year.[1] If you’re fifty years old, the moon is about two metres farther away than when you were born.

annularPaleontologists have been able to estimate length of the day in the distant past through the effect of tides on the formation of beds of sandstone. In the Neoproterozoic era (620 million years ago, well before the Cambrian Explosion of metazoan life), Earth’s day was only 21.9±0.4 hours long, and over the entire period from then until the present, the Moon’s average rate of recession was 2.17±0.31 cm/year—a little more than half the current rate.[2]

It’s no surprise that the average recession is slower than today’s, since the present configuration of continents and oceans is almost optimal to maximise tidal friction: two large pole-to-pole oceans separated by two landmasses which span most of the latitude range, including the equator where tidal forces are the greatest. When continental drift causes the continents to aggregate into a single landmass, or opens up a world-girdling equatorial ocean, or an ice age reduces sea level and freezes out the tides in northern and southern latitudes, tidal braking and hence lunar recession occur at a reduced rate. All of these circumstances have occurred in the 620 million years since the Neoproterozoic, averaging out to about 2 cm/year.

As the Moon recedes from the Earth, its apparent size diminishes. Already, when the Moon is near apogee, its angular size is always less than the Sun’s even at aphelion, so a total solar eclipse cannot occur near lunar apogee. The recession of the Moon increases both perigee and apogee, so eventually even the perigee will be sufficiently distant so the Moon doesn’t cover the Sun, and from that point unto eternity, no total solar eclipse will ever been seen from Earth. At some point before that date, when the Moon is near perigee and the Earth near aphelion, final totality will occur—the last total eclipse of the Sun visible from Earth. It will be extremely short, just a fraction of a second, and total only within a tiny spot near the Earth’s equator, but any being lucky enough to see it will have glimpsed something never, ever to be seen again from the Earth. How long will it be until that last-ever total solar eclipse?

Final totality will occur when the Moon, at a very close perigee, subtends an angle, as seen from the closest point on Earth, just sufficient to cover the disc of the Sun near apogee. Let’s put some numbers on these items, bearing in mind that we’re only making a rough estimate. There are so many uncertainties which could affect the Moon’s recession rate over the intervals involved that seeking great precision in other quantities is unwarranted.

The Sun-Earth distance at aphelion varies slightly from year to year depending on the relative positions of the Sun, Earth, and Moon, and the location of the solar system barycentre (centre of mass), which is affected by the positions of all the planets, principally Jupiter and Saturn. The most distant aphelion in the period 1960–2005 was 1.016759 astronomical units,[3] which we’ll round off to 1.017 AU. (An astronomical unit is the mean distance from the Earth to the Sun, equal to 149,597,870.691 kilometers.) Since the Sun is not a solid body and rotates, it isn’t a sphere, but rather an ellipsoid flattened at the poles with an equatorial bulge. For a total solar eclipse to occur, every part of the Sun’s disc must be covered, so we’ll use the equatorial radius of 695,000 km as the size of the Sun. From the radius and distance, a little trigonometry tells us that at an extreme aphelion, the broadest part of the Sun’s disc subtends about 0.5236 degrees.

Next, we need to calculate how far from the Earth the Moon must be to subtend that angle in the sky. The Moon’s mean radius is 1737.5 km, and once more pounding the problem with the hammer of trigonometry, we find that the Moon subtends the same angle as the Sun at apogee when the Moon is 380,376 km from the observer (note that since present-day apogees of the Moon are in excess of 406,000 km, no total solar eclipse can occur at lunar apogee.) Total solar eclipses will cease forever when lunar recession elevates the perigee to 380,376 km and above.

Before calculating how long that will take, there’s one more detail to attend to. The distance at which the Moon appears the same size as the Sun is the distance from the Moon to the observer, not the centre of the Earth, from which perigee is measured. You can’t see the Moon from the centre of the Earth (and, besides, it’s awfully hot there), so observers will be on the Earth’s surface which, at the point where the vector from the centre of the Earth to the centre of the Moon intersects the Earth’s surface, will be one Earth radius closer, which at the equator is 6378 km. Since we’re looking for the final total eclipse, we’ll take maximum advantage of the Earth’s equatorial radius and consider an eclipse which is only total for a moment at the equator, which permits the perigee to be as high as 386,754 km while keeping the observer to Moon distance at 380,376 km.

The Earth-Moon distance at perigee varies depending on the relative positions of the Sun, Earth, and Moon. The closest perigee in the A.D. 1500–2500 period occurs on January 1st, 2257 at 356,371 km, so we’ll take that as the present-day minimum.[4] The difference between this figure and the 386,754 km perigee which just permits an equatorial observer to see the Moon as big as the Sun: 30,383 km, is how far the orbit of the Moon will have been raised at the time of final totality. Using the mean recession rate over the last 620 million years of 2.17 cm/year as an estimate of the average rate over comparably long periods in the future, we find that it will take about 1.4 billion years before solar eclipses cease to be visible from Earth. Eclipse tour operators thus have no need to worry about near-term business prospects!

Over deep time like this, many factors can strongly influence the actual outcome. Over the next billion years, the Sun will continue to get brighter and brighter (as it has over all of Earth’s history), and may consequently appear somewhat larger than today. In any case, solar brightening will result in extreme changes in the Earth’s climate. The Earth may exhaust its inventory of carbon accessible to the biosphere, resulting in photosynthesis shutting down and the collapse of the plant and animal biosphere. A runaway greenhouse effect may result in the loss of the oceans, which would dramatically reduce tidal braking and the rate of lunar recession. And, of course, all of these events may result in the only observers present at the final solar eclipse being single-celled bacteria.[5] Not to worry; descendants of humanity will have moved on to more hospitable climes, but will no doubt arrange a Galaxy Wide Webcast of the event.

Exercises for the Reader

Using similar reasoning, estimate how far in the past the first-ever annular eclipse occurred on Earth. Calculate what fraction of the era in which both total and annular eclipses occur has elapsed so far. Decide whether the creepy-crawlers of the Burgess Shale could have witnessed an annular eclipse.

References

  1. Dickey, J.O. et al. “Lunar Laser Ranging: A Continuing Legacy of the Apollo Program,” Science 265, 486 (1994).
  2. Williams, G. “Geological constraints on the Precambrian history of Earth’s rotation and the Moon’s orbit”. Reviews of Geophysics 38, 37 (2000).
  3. Meeus, Jean. Astronomical Tables of the Sun, Moon, and Planets . 2nd. ed. Richmond: Willmann-Bell, 1995. ISBN 0-943396-45-X.
  4. Meeus, Jean. Mathematical Astronomy Morsels . Richmond: Willmann-Bell, 1997. ISBN 0-943396-51-4.
  5. Ward, Peter D. and Donald Brownlee. The Life and Death of Planet Earth. New York: Owl Books, 2003. ISBN 0-8050-7512-7.

Videos

Here is a video of the 2006 total solar eclipse viewed from Egypt.

This is a video of 2012 annular solar eclipse, as seen from Albuquerque, New Mexico.

Eclipse Photography

Images from Fourmilab eclipse expeditions:

There are 34 comments.

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  1. Yeah...ok. Inactive

    Exercises for the Reader

    [CoC][CoC][CoC] John gave us homework! I suppose it is back to school time…

    If I, sometimes, skip down to the videos and don’t actually READ the entire post, can I earn full credit by maybe clapping erasers or cleaning the blackboard?

    • #1
    • August 16, 2014, at 2:23 PM PDT
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  2. John Walker Contributor
    John Walker

    Yeah…ok.: If I, sometimes, skip down to the videos and don’t actually READ the entire post, can I earn full credit by maybe clapping erasers or cleaning the blackboard?

    Certainly! Got me through high school.

    • #2
    • August 16, 2014, at 2:25 PM PDT
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  3. Carey J. Inactive

    John Walker: Earth’s day was only 21.9±0.4 hours long, and over the entire period from then until the present, the Moon’s average rate of recession was 2.17±0.31 cm/year—a little more than half the current rate.[2]

     It has always seemed to me that the days went by quicker when I was a kid. Now I know why. Thanks, John.

    • #3
    • August 16, 2014, at 2:44 PM PDT
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  4. ParisParamus Member
    ParisParamus Joined in the first year of Ricochet Ricochet Charter Member

    So… just what is the consensus view on the origin of the moon?

    • #4
    • August 16, 2014, at 4:17 PM PDT
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  5. John Walker Contributor
    John Walker

    ParisParamus:

    So… just what is the consensus view on the origin of the moon?

    The most widely accepted theory is that the Moon was formed by an impact on the early Earth by a Mars-sized impactor which ejected a portion of the Earth’s crust which then condensed into the Moon. The primordial Moon would have been much closer to the Earth, but would have receded over time due to tidal recession, as discussed in the post.

    Evidence for this is that the composition of the Moon is much the same as that of the Earth’s crust with few of the elements in the Earth’s core. If the Earth and Moon had condensed independently from the protoplanetary disc, you’d expect their compositions to be similar. Also, there is evidence of a heavy bombardment during the early history of the solar system as objects coalesced into planetary bodies.

    It would be supererogatory to call this a consensus. We have so little hard data that other theories remain viable.

    • #5
    • August 16, 2014, at 4:45 PM PDT
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  6. Yeah...ok. Inactive

    John Walker:

    Yeah…ok.: If I, sometimes, skip down to the videos and don’t actually READ the entire post, can I earn full credit by maybe clapping erasers or cleaning the blackboard?

    Certainly! Got me through high school.

     Always the Suck-Up, I put an apple on your desk in Simon T‘s fine RM:AC post.

    • #6
    • August 16, 2014, at 5:18 PM PDT
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  7. John Walker Contributor
    John Walker

    Yeah…ok.: Always the Suck-Up, I put an apple on your desk in Simon T‘s fine RM:AC post.

    Heh.

    • #7
    • August 16, 2014, at 5:30 PM PDT
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  8. ParisParamus Member
    ParisParamus Joined in the first year of Ricochet Ricochet Charter Member

    John Walker:

    ParisParamus:

    So… just what is the consensus view on the origin of the moon?

    The most widely accepted theory is that the Moon was formed by an impact on the early Earth by a Mars-sized impactor which ejected a portion of the Earth’s crust which then condensed into the Moon. The primordial Moon would have been much closer to the Earth, but would have receded over time due to tidal recession, as discussed in the post.

    Evidence for this is that the composition of the Moon is much the same as that of the Earth’s crust with few of the elements in the Earth’s core. If the Earth and Moon had condensed independently from the protoplanetary disc, you’d expect their compositions to be similar. Also, there is evidence of a heavy bombardment during the early history of the solar system as objects coalesced into planetary bodies.

    It would be supererogatory to call this a consensus. We have so little hard data that other theories remain viable.

     Well, I’m glad I wasn’t around to witness that! Also, which level of Ricochet membership is required to use the word “supererogatory”?

    • #8
    • August 16, 2014, at 5:35 PM PDT
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  9. John Walker Contributor
    John Walker

    ParisParamus: Well, I’m glad I wasn’t around to witness that! Also, which level of Ricochet membership is required to use the word “supererogatory”?

    I would think that president Coolidge, the last to write his own speeches and able to read and write Greek and Latin as easily as English, would have endorsed the use of this word by members at the level bearing his name.

    • #9
    • August 16, 2014, at 5:44 PM PDT
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  10. Eeyore Member
    Eeyore Joined in the first year of Ricochet Ricochet Charter Member

    Okay, so much for the short view. When will the moon just say adieu cuz we don’t give it enough gravity to care? I suspect this could be deduced from the above information, but it’s been so long since I took math, I used to ride a stegosaurus home from class. 
    [I know. It was a special saddle. But they were really loyal. Anybody tried to mess with you, they got a face full of tail spikes]
    Calculable, or just useless, since the sun will already have done its supernova flashy thing?

    • #10
    • August 16, 2014, at 5:48 PM PDT
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  11. ParisParamus Member
    ParisParamus Joined in the first year of Ricochet Ricochet Charter Member

    Here’s a an almost related question: if “this space thing” every takes off in a big way, do we need to be concerned about Earth mass increases or decreases from removing a large amount of material from Earth, or delivering large amounts materials to Earth from other planets, asteroids, the moon, etc?

    • #11
    • August 16, 2014, at 5:52 PM PDT
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  12. John Walker Contributor
    John Walker

    Eeyore: Okay, so much for the short view. When will the moon just say adieu cuz we don’t give it enough gravity to care?

    This will probably not happen before the Earth and Moon are swallowed up by the Sun as it expands into a red giant. Once the Sun begins to expand, the oceans will be boiled off the Earth and tidal braking will be much reduced. Hence it is probable the Moon will still in be in an orbit (albeit more distant) when both are swallowed up by the Sun.

    • #12
    • August 16, 2014, at 5:53 PM PDT
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  13. John Walker Contributor
    John Walker

    ParisParamus: Here’s a an almost related question: if “this space thing” every takes off in a big way, do we need to be concerned about Earth mass increases or decreases from removing a large amount of material from Earth, or delivering large amounts materials to Earth from other planets, asteroids, the moon, etc?

    In a word, no. The mass of the Earth is 5.97×10^24 kilograms. The mass of all of the asteroids combined is about 1.7×10^21 kilograms, which is a hundred times smaller than the mass of the Earth and far less than the mass of the Moon (7.35^22 kg).

    • #13
    • August 16, 2014, at 6:01 PM PDT
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  14. Bob W Member

    I was on the sea of Cortez to watch the solar eclipse in 1991, one of the longest. It was a quite an experience. We here in the US will be able to experience a rare and not to be repeated anytime soon total eclipse Aug 21, 2017. A quick search will show the times and path. I can assure that making plans to be in the path should be on your “bucket list”. I will make every effort to see this one, it will be the last that can be easily viewed in our lifetimes.

    • #14
    • August 16, 2014, at 8:10 PM PDT
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  15. John Walker Contributor
    John Walker

    Bob W: We here in the US will be able to experience a rare and not to be repeated anytime soon total eclipse Aug 21, 2017.

    Here are details of this eclipse. Astronomers visualise solar eclipses with an orthographic map. In planning an eclipse expedition, the weather is a prime consideration. This page provides an early look at expected weather conditions along the eclipse track.

    • #15
    • August 17, 2014, at 2:57 AM PDT
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  16. Profile Photo Member

    Was it tried in a comment? (If you want to flip a disk, ask a dime. :-))

    perimoon_apsun_l

    • #16
    • August 17, 2014, at 4:32 AM PDT
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  17. Profile Photo Member

    Off topic.

    There is now a bug in the system that puts the date stamp of the most recent edit and puts your post at the top of the Member Feed. I did wonder when they tried to fix the “Draft Bug” if they would test for this. Of course only a rookie programmer would make this mistake. I am beginning to think the developer is in Junior High but I am optimistic.

    • #17
    • August 17, 2014, at 5:11 AM PDT
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  18. Michael Collins Member

    Bob W:

    We here in the US will be able to experience a rare and not to be repeated anytime soon total eclipse Aug 21, 2017. A quick search will show the times and path. I can assure that making plans to be in the path should be on your “bucket list”. 

    As a life-long Nebraskan I have been looking forward to this for a few years. I have read that the eclipse will last for a few seconds longer at one end of the Memorial Stadium football field in Lincoln than it will at the other end. I plan to drive a few miles to the south to some location that lies directly on the center line of the eclipse, so as to make my view last as long as possible. I will pray for good weather, but if the forecasts are poor I may drive to a neighboring state where the viewing will be better. It is a once in a lifetime opportunity, not to be missed.

    • #18
    • August 17, 2014, at 2:45 PM PDT
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  19. John Walker Contributor
    John Walker

    Michael Collins: I will pray for good weather, but if the forecasts are poor I may drive to a neighboring state where the viewing will be better. It is a once in a lifetime opportunity, not to be missed.

    Mobility is the key. If it’s partly cloudy you may be able to dash for a hole in the clouds and rescue an otherwise missed opportunity. Around the time of solar eclipses, beware of drivers looking out the window at the Sun instead of oncoming traffic.

    • #19
    • August 17, 2014, at 2:52 PM PDT
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  20. Michael Collins Member

    John Walker:

    Mobility is the key. If it’s partly cloudy you may be able to dash for a hole in the clouds and rescue an otherwise missed opportunity. Around the time of solar eclipses, beware of drivers looking out the window at the Sun instead of oncoming traffic.

     Yes, mobility is the key. Back in the early 1990’s after checking the forecasts for that “hole in the clouds” I drove to Columbia, MO with a #14 arc welders filter to see an annular eclipse of the sun. I avoided the inattentive drivers problem by leaving Lincoln the day before the eclipse. The night before I asked the clerks at my hotel if they knew of a place where amateur astronomers would be setting up their telescopes to allow people to share their view of the eclipse. By good fortune I found that the hotel was two blocks from the Columbia public library, where the local astronomers club was planning to hold just such an exhibit. The next day I found the place quite easily. There were several people setting up reflector telescopes with a white screen mounted on the side a few inches from the eyepiece. (cont).

    • #20
    • August 17, 2014, at 3:25 PM PDT
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  21. Michael Collins Member

    (Continued). For those who haven’t seen an eclipse the image of the sun is projected through an eyepiece to the screens which are mounted at a 90 degree angle from the telescope. It works kind of like a movie projector, so the entire audience can see the eclipse in real time (and of course is not subjected to having their eyes burned out by looking directly at the sun through a large telescope). I asked the amateur nearest to me what time the eclipse would begin, and made my standard eclipse joke of expressing hope that the eclipse would begin on time!
    One strange thing always happens at an eclipse while I am looking at one of the telescope screens: About 30 seconds or so before the eclipse begins something goes “click” in my head and I know the eclipse is about to begin. I can point directly to the exact spot on the screen where the moon will begin eating up the sun. My guess is that I am sensitive to some part of the infrared spectrum. Sure enough the moon made contact exactly where I thought it would. (continued).

    • #21
    • August 17, 2014, at 3:40 PM PDT
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  22. Edward Smith Inactive

    Which song would go best with this Post?

    This one?

    • #22
    • August 17, 2014, at 3:54 PM PDT
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  23. Edward Smith Inactive

    Or this one?

    • #23
    • August 17, 2014, at 3:57 PM PDT
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  24. Edward Smith Inactive

    I thought I’d leave You’re So Far Away out of the mix. It’s a mawkish sort of song.

    • #24
    • August 17, 2014, at 3:58 PM PDT
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  25. Michael Collins Member

    (Continued). That day began as a hot day, but it became much cooler. When the moon occludes even a small portion of the sun’s surface, it intercepts a lot of heat and light. People began asking to borrow the arc welders filter. From that time on I spent most of my time passing that filter around. Eclipses are only fun if you share them. The telescopes were great, but there is nothing like seeing an eclipse with your own eyes. The sunlight began to change. It was still broad daylight, but the daylight had a “silvery” character to it. Eventually I saw what I had come to see. For about 7 minutes there was a big burning basketball hoop in the sky (of course people were still borrowing my filter). Then A TV camera crew asked to borrow the filter. They put it in front of their camera before pointing the camera at the sun. (I’m afraid I never saw their broadcast, and I don’t know whether they even used the footage.) All in all it was one of the best days in my life.

    • #25
    • August 17, 2014, at 4:04 PM PDT
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  26. Trink Coolidge
    Trink Joined in the first year of Ricochet Ricochet Charter Member

    Excellent post . . . 
    Having watched a Great Courses series . . I’d heard this account of tidal friction and the moon’s drifting away.
    It’s all so fascinating. We actually went to Aruba with our astronomer planetary scientist son to see a total eclipse of the sun in ’98. Very stirring.

    • #26
    • August 17, 2014, at 5:49 PM PDT
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  27. Bob W Member

    Michael, the annular eclipse you saw was just a partial here on the west coast. It was late in the day and as usual the fog started to move in. The fog provided the “filter” for this shot out side our shop in Carmel.

    There are several ways to view an eclipse. An easy way, which most people can do, is the projection method using regular binoculars and a white paper. Point the binoculars at the sun projecting it on the paper. It can be focused by moving the paper back and forth. No, it will not burn the paper or harm the binoculars. When the event is near I”m sure there will be many “eclipse viewers” on the market which will consist of a mylar film mounted in a cardboard holder. Also available are metalized filters that mount on telescopes, they are usually used to view sunspots. Just make sure any thing you plan to use doesn’t have a hole in it!

    • #27
    • August 18, 2014, at 2:11 PM PDT
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  28. John Walker Contributor
    John Walker

    Bob W: Also available are metalized filters that mount on telescopes, they are usually used to view sunspots. Just make sure any thing you plan to use doesn’t have a hole in it!

    Solar filters are fixed to the objective end of the telescope, so that they reduce the intensity of light before it enters the telescope. Be sure the filter is securely fixed to the front of the telescope—if it were to fall off while you were observing, your vision would be destroyed before the blink reflex could activate. Also, if your telescope has a viewfinder, make sure its objective lens cap is in place (or if it doesn’t have a lens cap, block the objective by wrapping it in aluminium foil. Otherwise, you could inadvertently set your hair on fire (or, in my case, singe the scalp) by sunlight concentrated through the finder while you’re observing the partial phase through the telescope.

    After the last bit of the photosphere is covered (the end of the initial “diamond ring” phase), you’ll want to remove the filter to observe or photograph the corona. But you must be careful to start a timer which will warn you of the end of totality so you can replace the filter before the photosphere is again exposed.

    All of the eclipse photography linked above was made using an Orion metal-on-glass solar filter.

    • #28
    • August 18, 2014, at 2:30 PM PDT
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  29. Bob W Member

    I’ll try again

    See post above…

    • #29
    • August 18, 2014, at 4:19 PM PDT
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  30. Michael Collins Member

    Bob W: There are several ways to view an eclipse. An easy way, which most people can do, is the projection method using regular binoculars and a white paper. Point the binoculars at the sun projecting it on the paper

     Yes, that is basically the same as the telescope method I described (you explained it better). When I was a kid an amateur that I knew made a two piece cardboard disk which he mounted on the front end of his 6 inch reflector. That way he could limit the amount of sunlight entering his eyepiece to the area covered by a small slit. That, combined with a prism that split 90% of the remaining sunlight off from the eyepiece made a dark filter on the eyepiece safe to use, at least for his camera. I don’t remember for sure whether he used this arrangement to view the sun directly. For now I think I’ll stick to my #14 arc welders filter provided I can find it again. I found it a few months ago after losing track of it for several years, but now I’ve forgotten where I put it again.

    • #30
    • August 18, 2014, at 4:43 PM PDT
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