Spiral Galaxy 50 Million Light-Years Away Delivers Stellar Light Show

Written by News One November 8, 2024

A spectacular image of a spiral galaxy with a bright, glowing center and swirling arms dotted with pink and blue. Stars and distant galaxies speckle the background, creating a cosmic scene of vivid colors and depth. — NGC 1672, as seen by the Hubble Space Telescope

The NASA/ESA Hubble Space Telescope continues to churn out fantastic space images. The latest captured by the 34-year-old telescope shows barred spiral galaxy NGC 1672 in all its luminous glory.

NGC 1672 is about 49 million light-years from Earth in the constellation Dorado. Like other spiral galaxies, NGC 1672 features large, distinct arms extending from its galactic core. In NGC 1672’s case, the two large arms shine due to hydrogen gas illuminated by radiation created by infant stars nestled in the interstellar gas and dust, shrouded from view.

These newly formed stars emit extremely powerful X-ray radiation, which has been previously observed by NASA’s Chandra Observatory. The new James Webb Space Telescope has also peered at NGC 1672 as part of its ongoing Physics at High Angular Resolution in Nearby Galaxies (PHANGS) program.

A bright spiral galaxy with glowing pink and purple hues radiates against a dark space backdrop. The galaxy's core is luminous, and numerous stars and other celestial objects surround it, creating a captivating cosmic scene. — NGC 1672 composite created using data from the Chandra X-ray observatory, Spitzer telescope, the Hubble Space Telescope, and the James Webb Space Telescope

Image of a spiral galaxy with a bright core and swirling arms, filled with stars and interstellar dust. The galaxy's structure is highlighted by deep red and blue hues, set against the dark backdrop of space. — The James Webb Space Telescope’s view of NGC 1672, captured as part of the PHANGS collaboration

Near NGC 1672’s center, Hubble spots the active galactic nucleus. “This X-ray powerhouse makes NGC 1672 a Seyfert galaxy,” NASA explains. “It forms as a result of heated matter swirling in the accretion disk around NGC 1672’s supermassive black hole.”

Side-by-side image of a galaxy. The left half shows an infrared view with fiery, swirling patterns and bright stars, while the right half reveals a visible light view with bright stars, dust lanes, and spiral arms. — ‘Hubble (right) and Webb (left) observations complement each other well, providing astronomers with a wide spectrum of light to study. Hubble’s observations showcase visible and ultraviolet light, while Webb’s combine near- and mid-infrared light. Dust absorbs ultraviolet and visible light, and then re-emits it in the infrared. In Hubble’s image, dark dust lanes are where starlight is absorbed. In Webb’s image, we see that dust glowing in infrared light,” NASA explains. In Hubble’s image, young stars appear blue and purple and fill the frame. In Webb’s images, newly-formed stars appear blue, but the orange stars are still forming and are cocooned in gas and dust.

This makes Hubble’s new image spectacular enough, but something else is happening in the image: a fleeting cosmic view of a supernova. Of the six images Hubble captured to create the final composite above, one included a supernova, SN 2017GAX. This was a Type I supernova “caused by the core-collapse and subsequent explosion of a giant star that went from invisible to a new light in the sky in just a matter of days.”

A detailed view of the barred spiral galaxy NGC 1672, showcasing bright clusters of stars and swirling dust lanes. The galaxy's core emits a bright light, surrounded by extended spiral arms with pink and blue hues. Stars are scattered across the scene. — The arrow is pointing at the supernova, SN 2017GAX, captured in one of Hubble’s six images used to create the final composite

The supernova may appear small in the image above, but it is a massive deal to scientists. These transient events are challenging to spot and of significant interest to astronomers and physicists.

Image credits: Hubble images: ESA/Hubble & NASA, O. Fox, L. Jenkins, S. Van Dyk, A. Filippenko, J. Lee and the PHANGS-HST Team, D. de Martin (ESA/Hubble), M. Zamani (ESA/Hubble). | Webb image: NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team. | Chandra image: X-ray: Chandra: NASA/CXC/SAO, XMM: ESA/XMM-Newton; IR: JWST: NASA/ESA/CSA/STScI, Spitzer: NASA/JPL/CalTech; Optical: Hubble: NASA/ESA/STScI, ESO; Image Processing: L. Frattare, J. Major, and K. Arcand.

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