Total eclipse of the data
August 21st, 2017 is set to be a historic day: The entire continental U.S. will experience a partial eclipse (making our blog headline slightly misleading), with the path of totality sweeping from Oregon to South Carolina. “Totality” refers to when the moon completely blocks the sun.
It’s been hundreds of years since an eclipse only made landfall in the U.S., and this one is notable for being so accessible. Plus, because the eclipse will be total along its entire accessible path and visible as a partial eclipse for the entire continental U.S., this event is getting a ton of attention.
Digging into the data
But is it really that special, on an astronomical scale? I wanted to find out, so I went to the source: NASA. There, I found a Five Millennium Catalog of Hybrid Solar Eclipses.
Turns out, there are a lot of solar eclipses. There’s also a lot more that goes into tracking and describing an eclipse than I realized! Thank goodness there was a key to the data set.
To start with, I learned how many solar eclipses there were in the data set: 11,898. That’s just over two eclipses per year:
Almost 27% of solar eclipses are total. Others are (1) partial, where the moon doesn’t fully mask the sun; (2) annular, where the moon is directly over the sun but too far away (i.e. appearing too small) to fully block out the sun; or (3) hybrid, a combination of total and annular.
While poking around, I noticed some cool things, like the pronounced seasonality for total eclipses:
But things got really exciting when I started exploring Saros numbers. According to NASA, “The periodicity and recurrence of eclipses is governed by the Saros cycle, a period of approximately 6,585.3 days (18 years 11 days 8 hours).” That definition got me wondering if I could visualize this pattern, and sure enough, I quickly made some fantastic vizzes displaying these finite recurrences.
Here, we can see the lifespan of Saros series. As the moon and sun align, we get a string of partial eclipses. Once in alignment, there’s a run of total/annular/hybrid eclipses. After 12-15 centuries, the moon and sun shift out of alignment and the Saros series ends, again with a number of partial eclipses.
And not all Saros series are created equal—there’s some serious patterning happening here, too:
As it happens, the eclipse on August 21st is in Saros 145. The last eclipse in Saros 145 was a total eclipse on August 11th, 1999, and the next will be a total eclipse on September 2nd, 2035.
I wound up creating a story (explore it below!) showcasing some of the more fun things I noticed, but there’s tons of information to be unpacked from this data set—what can you find?
Note: The original data set has a complex field for Eclipse Type. I used the following calculation in Tableau to simplify it:
IF CONTAINS([Eclipse Type], "P") = TRUE THEN "Partial Eclipse"
ELSEIF CONTAINS([Eclipse Type], "A") = TRUE THEN "Annular Eclipse"
ELSEIF CONTAINS([Eclipse Type], "T") = TRUE THEN "Total Eclipse"
ELSEIF CONTAINS([Eclipse Type], "H") = TRUE THEN "Hybrid or Annular/Total Eclipse"
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