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NGC 1398 is a spiral galaxy in the Fornax constellation, around 65 million light years from earth.
A striking feature of this galaxy is the ring structure around its core region. It's likely a density wave that's expanding. In plain English, think of it as a region that's slightly denser than its surroundings; making it stand out.
If you're interested in learning how and why this phenomenon manifests itself; I recommend giving the following link a read (which in my eyes explains it perfectly in terms that should be understandable to anyone).
astronomy.swin.edu.au/cosmos/D/density+wave+model
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Today's story and sketch by me #1398, Is a tragic tale about the two medical patients from the Planet Woomou, which is located in a dimension unknown to any of our very knowledgeable deputies. Deputy Cosmo only learned about the Planet Woomou, after we removed the patient from the nearly dead ancient oak tree. The patient named Roscoe had his medical chart attached to the end of his Gurnee, which only read Roscoe was getting a hair transplant procedure, an the bed and all of the equipment were property of the Planet Woomou Sasquatch Hair Institute. Please do not remove equipment from these premises. We are guessing the Dude in the wheelchair, was also at the institute when the two, and the ancient oak were snatched by a Big Blue Dimension Dust Devil and dropped here on this Lovely Tropical Volcanic Planet we call Budahunga. It will surely be an interesting tale when we interrogate these two, but those will have to be stories for another time, until then Tata the Rod Blog.
matrixspirt.blogspot.com/2026/01/ms-1398.html
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This week’s picture shows spectacular ribbons of gas and dust wrapping around the pearly centre of the barred spiral galaxy NGC 1398. This galaxy is located in the constellation of Fornax (The Furnace), approximately 65 million light-years away. Rather than beginning at the very middle of the galaxy and swirling outwards, NGC 1398’s graceful spiral arms stem from a straight bar, formed of stars, that cuts through the galaxy’s central region. Most spiral galaxies — around two thirds — are observed to have this feature, but it’s not yet clear whether or how these bars affect a galaxy’s behaviour and development. This image comprises data gathered by the FOcal Reducer/low dispersion Spectrograph 2 (FORS2) instrument, mounted on ESO’s Very Large Telescope (VLT) at Paranal Observatory, Chile. It shows NGC 1398 in striking detail, from the dark lanes of dust mottling its spiral arms, through to the pink-hued star-forming regions sprinkled throughout its outer regions. This image was created as part of the ESO Cosmic Gems programme, an outreach initiative to produce images of interesting, intriguing or visually attractive objects using ESO telescopes, for the purposes of education and public outreach. The programme makes use of telescope time that cannot be used for science observations. All data collected may also be suitable for scientific purposes, and are made available to astronomers through ESO’s science archive.
Credit: ESO
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