
Over the span of three days in January 2016, the Hubble Space Telescope captured detailed images of just that scenario happening to Comet 332P/Ikeya-Murakami, or Comet 332P, located roughly 67 million miles from Earth.
The Hubble observations revealed 25 building-size blocks made of a mixture of ice and dust that broke off from the comet and are now are scattered along a 3,000-mile-long trail, larger than the width of the continental U.S. The icy chunks comprise about 4 percent of the parent comet and range in size from roughly 65 feet wide to 200 feet wide. They are drifting away from the comet and each other at a few miles per hour, about the walking speed of an adult. See animation here.
The Hubble observations also reveal that the comet is much smaller than previously thought, measuring only 1,600 feet across, about the length of five football fields.
According to a NASA statement, these observations provide insight into the volatile behavior of comets as they approach the sun, begin to vaporize, and unleash dynamical forces. Comet 332P was 150 million miles from the sun, slightly beyond the orbit of Mars, when Hubble spotted the breakup.












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