Close-up: Spiral Galaxy Messier 77 in Cetus (2025 version) | Hubble Space Telescope
The designation Messier 77 comes from the galaxy’s place in the famous catalog compiled by the French astronomer Charles Messier. Another French astronomer, Pierre Méchain, discovered the galaxy in 1780. Messier and Méchain were comet hunters. They cataloged nebulous objects that could be mistaken for comets.
Messier, Méchain, and other astronomers of their time mistook the Squid Galaxy for either a spiral nebula or a star cluster. This mischaracterization is not surprising. More than a century would pass between the discovery of the Squid Galaxy and the realization that the ‘spiral nebulae’ scattered across the sky were not part of our galaxy and were in fact separate galaxies millions of light-years away. The Squid Galaxy’s appearance through a small telescope—an intensely bright center surrounded by a fuzzy cloud—closely resembles one or more stars wreathed in a nebula.
The name ‘Squid Galaxy’ only came about recently. This name comes from the extended, filamentary structure that curls around the galaxy’s disc like the tentacles of a squid. The Squid Galaxy is a great example of how advances in technology and scientific understanding can completely change our perception of an astronomical object—and even what we call it!
A Hubble image of the Squid Galaxy was previously released in 2013. This new version incorporates recent observations made with new filters and updated image processing techniques.
Image Description: A close-up of a spiral galaxy, seen face-on. Its center glows brightly. From the sides of the galaxy’s core emerge spiral arms that wind through the round disc of the galaxy, filled with shining pink spots where stars are forming and more dark-red dust. Faint stars can be seen around the galaxy, as well as a particularly bright star in the lower left of the image.
Release Date: April 14, 2025
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