Arp 107 (MIRI Image) - a photo on Flickriver

Arp 107 (MIRI Image)

            This image of Arp 107, shown by Webb’s MIRI (Mid-Infrared Instrument), reveals the supermassive black hole that lies in the center of the large spiral galaxy to the right. This black hole, which pulls much of the dust into lanes, also display’s Webb’s characteristic diffraction spikes, caused by the light that it emits interacting with the structure of the telescope itself.

Perhaps the defining feature of the region, which MIRI reveals, are the millions of young stars that are forming, highlighted in blue. These stars are surrounded by dusty silicates and soot-like molecules known as polycyclic aromatic hydrocarbons. The small elliptical galaxy to the left, which has already gone through much of its star formation, is composed of many of these organic molecules.

Credit: NASA, ESA, CSA, STScI

Image Description: A pair of interacting galaxies. The larger of the two galaxies is slightly right of center, and is composed of a bright, white center and a ring of blue, gaseous filaments. The center of this galaxy shows Webb’s eight-pronged diffraction pattern. There are three filaments of gas and dust moving from the ring toward the center. At the top left of the ring is a noticeable gap, bordered by two large, blue pockets of dust and gas. The smaller galaxy is made of hazy, light blue gas and dust. Many red, green, blue, and yellow galaxies are spread throughout, with some being hazier in composition and others having more defined spiral patterns.

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Taken on: September 18, 2024

Tags:

jwst

webb

space

telescope

galaxies

interacting

galaxy

merger

mid-infrared

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Sets appears in: • Webb Images/Science 2024

Stats: 71,076 views

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