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Webb’s image of NGC 3627 shows a face-on barred spiral galaxy anchored by its central region, which has a bright blue central dot surrounded by a lighter diagonal blue bar structure made of a haze of stars, which forms an angled oval toward the top. The central core and bar fill about a third of the image. Two distinct spiny spiral arms made of stars, gas, and dust also start at the center, appearing brown or greenish within the blue bar, and extending to the edges, rotating clockwise in bright oranges. The brightest areas of the arms are two large arcs that start at the central region. The one at left stretches up to the top in a long arc and another at right extends toward the bottom. Scattered across the packed scene are bright blue pinpoints of light, which are stars spread throughout the galaxy. In areas where there is less orange, it is darker. A triangular area at bottom right is largely the black background of space.

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https://cdn.masto.host/astrodonsocial/media_attachments/files/111/914/896/986/250/614/original/fc530cfde879c2aa.png

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  1. Kelly Lepo (kellylepo@astrodon.social)'s status on Sunday, 11-Feb-2024 22:37:01 UTC Kelly Lepo Kelly Lepo

    Next in our 19 days of #PHANGS galaxies series is the barred spiral galaxy NGC 3627, as seen by #Hubble and #JWST.

    NGC 3627, also known as M66, is about 37 million light-years (11.3 Mpc) away.

    It was discovered by Charles Messier on 1 March 1780, object 66 in his catalog of “fuzzy things in the night sky that are not comets”. He described it as "very long and very faint."
    📷 https://webbtelescope.org/contents/media/images/2024/105/01HMA6P3V363GW0EA0347CR6HV
    1/

    In conversation Sunday, 11-Feb-2024 22:37:01 UTC from astrodon.social permalink
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