SCIENCE:
NASA, ESA, CSA, Janice
Lee
(NOIRLab)
IMAGE PROCESSING:
Alyssa
Pagan
(STScI)
This image taken by NASA’s James Webb Space Telescope shows one of a total of 19 galaxies targeted for study by the Physics at High Angular resolution in Nearby Galaxies (PHANGS) collaboration. Nearby barred spiral galaxy NGC 1433 takes on a completely new look when observed by Webb’s Mid-Infrared Instrument (MIRI).
NGC 1433’s spiral arms are littered with evidence of extremely young stars releasing energy and, in some cases, blowing out the gas and dust of the interstellar medium. Areas that appear dark and dim in optical imaging light up under Webb’s infrared eye. This is due to clumps of dust and gas in the interstellar medium absorbing the light from forming stars and emitting it back out in the infrared.
Webb’s image of NGC 1433 is a strong display of how dynamic processes associated with forming stars influence the larger structure of an entire galaxy.
At the center of the galaxy, a tight, bright core featuring a unique double ring structure shines in exquisite detail with Webb’s extreme resolution. In this case, that ‘double ring’ is actually tightly wrapped spiral arms that wind into an oval shape along the galaxy’s bar.
NGC 1433 is a Seyfert galaxy, which are typically relatively close to Earth and has a supermassive black hole at the center eating material at a high rate. The brightness and lack of dust in the MIRI image of NGC 1433 could hint at a recent collision with another galaxy.
NGC 1433 lies over 46 million years away from Earth in the constellation Horologium.
MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) and NASA’s Jet Propulsion Laboratory, in partnership with the University of Arizona.