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Hubble’s image of NGC 3627 shows a face-on barred spiral galaxy anchored by its central region. It has a bright yellow circular area surrounded by a lighter yellow diagonal 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 spiral arms made of stars, gas, and brown filamentary dust lanes start at the center and extend to the edges, rotating clockwise. The farther the arms are from the central region the easier it is to see bright blue clusters of stars, which appear as pinpricks. The darkest areas of the arms are two large dusty arcs that start at the central region. One to lower left extends toward the top and the second starts at the top-right and extends to the bottom. The background of space beyond the galaxy appears dark gray. There are some fine red points of light toward the bottom half and top right. A triangular area at center-right is black, reflecting where there isn’t any data.

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https://cdn.masto.host/astrodonsocial/media_attachments/files/111/914/896/763/817/097/original/6e063b3cae582bfe.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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