Manhattanhenge

Manhattanhenge – sometimes referred to as the Manhattan Solstice – is a semiannual occurrence in which the setting sun aligns with the east–west streets of the main street grid in the borough of Manhattan in New York City. The term is derived from Stonehenge, at which the sun aligns with the stones on the solstices. It was popularized in 2002 by Neil deGrasse Tyson, an astrophysicist at the American Museum of Natural History. It applies to those streets that follow the Commissioners' Plan of 1811, which are laid out in a grid offset 29.0 degrees from true east–west. (The 29.0 degrees should be added to true east and west, making the western bearing approximately 299.0 degrees.) During Manhattanhenge, an observer on one of the gridded east-west streets will see the sun setting over New Jersey directly opposite from the street, along its centerline.

The dates of Manhattanhenge are usually around May 28 and July 12 or July 13 – spaced evenly around summer solstice. In 2011, Manhattanhenge occurred on May 31 at 8:17 p.m., and on July 12 (full sun) and 13 (half sun), both at 8:25 p.m.

The two corresponding mornings of sunrise right on the center lines of the Manhattan grid are approximately December 5 and January 8 – spaced evenly around winter solstice. As with the solstices and equinoxes, the dates vary somewhat from year to year.

The same phenomenon occurs in other cities with a uniform street grid. In Chicago, Illinois, for instance, the setting sun lines up with the grid system on September 25, a phenomenon known similarly as Chicagohenge. In Toronto, Ontario, Canada, the setting sun lines up with the east–west streets on October 25 and February 16, a phenomenon known locally as Torontohenge. In Montreal, Quebec, Canada, there may be a Montrealhenge each year on July 12.