There is a new view from the James Webb Space Telescope. Judy was an amateur image editor who took the raw data from the Mid-Infrared Instrument and teased out a view of a distant galaxy. Not a lot of stars can be seen because the arms are full of dust.

The physics of star formation is intertwined with the amount of dust and gas in the universe. The small central nucleus of NGC 1566 is very bright, which is a sign that it is part of the Seyfert class. The centers of the galaxies are very active, emitting strong bursts of radiation and could be home to many millions of black holes.

The constellation of Dorado is 40 million light years away. The shape of this intermediate spiral galaxy is similar to a barred spiral galaxy and a regular spiral galaxy.

Happy Friday, everyone. Here's a new view from JWST's MIRI of spiral galaxy NGC 1566. The colors in this image come from the emission of dust. Hardly any stars are visible. The reddish areas correspond with star formation, though.

Data via Proposal GO 2107 / @janiceleeastro pic.twitter.com/td6nocJvUF