A mixture of two photographs taken throughout a total solar eclipse in 2009 on the board of the ship in neighborhood of Iwo Jima Island.
Credit score: Marta and Michal Zolnowski
On April 8, 2024, the utmost length of totality anyplace alongside the eclipse path will probably be 4 minutes 28 seconds. For comparability, the utmost size of totality for the final total solar eclipse to cross the continental U.S., which occurred on Aug. 21, 2017, was simply 2 minutes 40 seconds.
Certainly, some eclipse totalities final however a number of seconds. And the longest eclipse totality from 2000 B.C. to A.D. 3000 is 7 minutes 29 seconds. That eclipse will happen July 16, 2186.
What determines the size of a solar eclipse?
So why aren’t all totalities 7½ minutes lengthy?
The reason for this goes approach again to the time of the German astronomer, Johannes Kepler, who lived from 1571 till 1630. Within the fall of 1600, Kepler started working for the Danish astronomer Tycho Brahe, who had for years been accumulating observational information on the planets. Tycho paid Kepler to investigate the info. However in October 1601, Tycho out of the blue died and Kepler grew to become the imperial mathematician, a place he held for 11 years.
Throughout Kepler’s first 4 years, he focused on making an attempt to make the orbit of Mars match Tycho’s observations. He initially assumed a round orbit for the Purple Planet, however that didn’t work. Neither did quite a lot of egg-shaped orbits. Then, in early 1605, he tried an ellipse, and it labored to a excessive diploma of accuracy. He instantly assumed that every one the planets moved this manner and formulated the primary of his three legal guidelines of planetary movement: Planets transfer in elliptical orbits.
As you may guess, astronomers additionally see elliptical orbits once they have a look at moons round planets. None have round orbits; all of them transfer alongside elliptical paths.
The factor a couple of physique in an elliptical orbit is that its distance from the item it orbits is at all times altering. Typically it’s farther from its “main,” and different occasions it’s nearer. Now we begin to perceive why totality might final 1 second, 1 minute, or 7½ minutes. It has to do with each the altering distance of Earth from the Solar and the altering distance of the Moon from Earth.
As our planet orbits the Solar, its distance adjustments from a minimal of 91.4 million miles (147 million kilometers) round Jan. 4, to a most of 94.5 million miles (152 million km) round July 4. That’s a change of three p.c.
Likewise, the Moon’s distance from Earth can range from a minimal of 221,500 miles (356,000 km) to a most of 252,700 miles (407,000 km). And that’s a whopping change of 14 p.c.
The results of combining these numbers is that whereas the Moon’s true dimension doesn’t really change, its obvious diameter — that’s, the disk that we see — can vary from 7 p.c bigger than the Solar to 10 p.c smaller than the Solar.

So, let’s take into consideration the 2 extremes. In a single case, Earth is at its closest level to the Solar whereas the Moon is as far-off from Earth as it might get. In different phrases, the Solar would seem giant whereas the Moon appeared small. On this case, there could be no totality in any respect. Even when the Solar, the Moon, and Earth had been in a straight line, folks alongside the trail would expertise an annular eclipse.
The opposite excessive is far more to our liking. On this case, Earth is at its farthest level from the Solar and the Moon is at its closest strategy to Earth. So, our daytime star would look small whereas our lone pure satellite would look as huge as it might get. That is the mixture that yields a solar eclipse totality lasting 7½ minutes.
So, the precise size of any total solar eclipse’s totality lasts someplace between a fraction of a second and 7½ minutes.
Lengths of totality for 2024 solar eclipse
To complicate issues, the size of totality additionally adjustments alongside every eclipse’s path, primarily as a result of we reside on a round Earth. That will help you plot a potential viewing location, listed below are the durations of totality for numerous cities alongside the trail of the 2024 total solar eclipse. As a result of the eclipse strikes from southwest to northeast, that’s the best way I’ve organized the areas. Additionally, for giant cities, the size is a mean. Components of the metro areas nearer to the eclipse’s middle line can have longer durations, and people farther from it would have shorter ones.
Location | Size of totality |
---|---|
Radar Base, Texas | 4 minutes 27 seconds |
Laughlin Air Drive Base | 3 minutes 41 seconds |
Dabney, Texas | 4 minutes 24 seconds |
Concan, Texas | 4 minutes 24 seconds |
Kerrville, Texas | 4 minutes 24 seconds |
Austin, Texas | 1 minute 46 seconds |
Georgetown, Texas | 3 minutes 15 seconds |
Killeen, Texas | 4 minutes 17 seconds |
Temple, Texas | 3 minutes 47 seconds |
Valley Mills, Texas | 4 minutes 24 seconds |
Waco, Texas | 4 minutes 13 seconds |
Ennis, Texas | 4 minutes 22 seconds |
Fort Value, Texas | 2 minutes 35 seconds |
Dallas, Texas | 3 minutes 49 seconds |
Tyler, Texas | 1 minute 57 seconds |
Sulphur Springs, Texas | 4 minutes 21 seconds |
Mt. Nice, Texas | 3 minutes 55 seconds |
Texarkana, Texas | 2 minutes 28 seconds |
Clarksville, Texas | 4 minutes 20 seconds |
Idabel, Oklahoma | 4 minutes 19 seconds |
Pencil Bluff, Arkansas | 4 minutes 18 seconds |
Sizzling Springs, Arkansas | 3 minutes 39 seconds |
Little Rock, Arkansas | 2 minutes 30 seconds |
Hardy, Arkansas | 4 minutes 12 seconds |
Doniphan, Missouri | 4 minutes 12 seconds |
Cape Girardeau, Missouri | 4 minutes 6 seconds |
Carbondale, Illinois | 4 minutes 9 seconds |
Evansville, Indiana | 3 minutes 2 seconds |
Bloomington, Indiana | 4 minutes 3 seconds |
Indianapolis, Indiana | 3 minutes 47 seconds |
Dayton, Ohio | 2 minutes 44 seconds |
Celina, Ohio | 3 minutes 47 seconds |
Delaware, Ohio | 2 minutes 38 seconds |
Toledo, Ohio | 1 minute 52 seconds |
Norwalk, Ohio | 3 minutes 54 seconds |
Akron, Ohio | 2 minutes 48 seconds |
Cleveland, Ohio | 3 minutes 50 seconds |
Erie, Pennsylvania | 3 minutes 43 seconds |
Buffalo, New York | 3 minutes 45 seconds |
Niagara Falls, New York | 3 minutes 29 seconds |
Rochester, New York | 3 minutes 40 seconds |
Syracuse, New York | 1 minute 29 seconds |
Harrisville, New York | 3 minutes 38 seconds |
Plattsburgh, New York | 3 minutes 34 seconds |
Burlington, Vermont | 3 minutes 15 seconds |
Jackman, Maine | 3 minutes 27 seconds |
Houlton, Maine | 3 minutes 21 seconds |
Understanding precisely how lengthy totality for the 2024 total solar eclipse will probably be in your neck of the woods will assist you to put together for the absolute best viewing expertise. However irrespective of how lengthy totality lasts in your location, belief us, it would nonetheless really feel like a blink of a watch!