Chicagohenge – an equinox sunset.
For a few days around and during the autumnal and vernal equinoxes, the sun puts on a spectacular show as it seemingly rises and sets between the soaring skyscrapers of Chicago’s east/west streets. Since the first time I captured the phenomenon back in 2013, I’ve tried to take unique images every year thereafter. Since then, I’ve shot it from various streets, a helicopter, and from an L platform. I’ve even shot the ‘Reverse Chicagohenge’ in which I captured the sun’s reflection on the west side of the skyline. Check out my photo gallery at the bottom of this post for more images.
During the Equinox, the tilt of the Earth’s axis is inclined neither away from, nor towards the sun, so the center of the sun is in the same plane as the Earth’s equator. For our purposes, the important part is that the the sun sets at 270° – exactly due west. But there’s a twist. It turns out that Chicago’s street grid is off by a fraction of a degree. So when looking down the ‘concrete canyon’ you’re actually pointing ever so slightly southwest. This matters because ‘optimum’ Chicagohenge conditions vary based on which part of the year you shoot it.
Long story short, there are varying degrees of “Chicagohengey-ness” in the few days before and after each equinox that make each occurrence unique. In spring, the ‘henge sunset becomes visible a day or two before the equinox as the sun marches north (the opposite is true for sunrise). Conversely, Chicagohenge may peak a day or two after the fall equinox as the sun moves southward. The equinox varies by a few days from year-to-year (here’s why), so the exact sunset times and angles vary as well, making certainties tough to pin down. What was ‘perfect’ one year may be off by a few hours or degrees the next. Your best bet is to get out there and witness it for yourself.
Shooting directly into the sun is tricky so here are some numbers to help you out. I photographed the feature image on 9/22/2013. The settings were 1/8000, f/5.6, ISO 320, at 200mm. The image directly above was taken on 9/25/2013 – just three days later – at 1/125, f/5.6, ISO 200, at 200mm. I point this out because it’s pretty spectacular to see just how much the sun moved in three short days. Additionally, I use PhotoPills to help me judge sunset times and the sun’s actual angle.