NGC 7496 was found on September 5, 1834 by the English astronomer John Herschel.

Otherwise called ESO 291-1, LEDA 70588 and IRAS 23069-4341, this galaxy has to do with 70,000 light-years throughout.

NGC 7496 belongs to the NGC 7582 group, an event of nearly 10 big galaxies.

The galaxy is likewise categorized as a type II Seyfert galaxy with high star development rate.

At the center of NGC 7496 lies an active galactic nucleus, a supermassive great void that delight in gas.

“Hubble initially observed NGC 7496 as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program,” the Hubble astronomers stated in a declaration.

“This program has actually employed the capabilities of a number of effective huge observatories, consisting of the Atacama Large Millimetre/submillimetre Array, ESO’s Very Large Telescope, and the NASA/ESA/CSA James Webb Space Telescope, in addition to the NASA/ESA Hubble Space Telescope.”

“NGC 7496 was the very first galaxy in the PHANGS sample that Webb observed.”

“Each of these observatories uses a various point of view on this well-studied galaxy.”

“With its special ultraviolet abilities and great resolution, Hubble’s view exposes young star clusters breaking with high-energy radiation.”

“Hubble’s observations of NGC 7496 assistance to expose the ages and masses of these young stars, in addition to the degree to which their starlight is obstructed by dust.”

“A previous Hubble picture of NGC 7496 was launched in 2022,” they included.

“Today’s image integrates brand-new information that highlight the galaxy’s star clusters, which are surrounded by radiant red clouds of hydrogen gas.”