NGC 1365 is a double barred spiral galaxy that lies about 56 million light years away from Earth.
In the MIRI observations of NGC 1365, clumps of dust and gas in the interstellar medium have absorbed the light from forming stars and emitted it back out in the infrared, lighting up an intricate network of cavernous bubbles and filamentary shells created by young stars releasing energy into the galaxy’s spiral arms.
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Location: The universe
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