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Hubble’s Observation of Galaxy NGC 5427

The NASA Hubble Space Telescope has captured a stunning image of the galaxy NGC 5427. This galaxy is part of a pair called Arp 271, with its companion NGC 5426 situated below and outside the frame of the image. However, the gravitational attraction between the two galaxies is evident in the distorted shape of NGC 5427 and the bridge of stars seen in the lower-right region of the image.

Back in 1785, British astronomer William Herschel discovered this interacting pair, which will remain in this state for millions of years. It is still uncertain whether they will eventually collide and merge, but their mutual gravitational pull has already led to the formation of numerous new stars.

The galaxy NGC 5427 shines in the large image from Hubble, with ground-based observations showing its companion galaxy NGC 5426. Together, this pair is known as Arp 271. Credit: Ground-based image: DECam Victor M. Blanco/CTIO; Hubble image: NASA, ESA, and R. Foley (University of California – Santa Cruz); Processing: Gladys Kober (NASA/Catholic University of America)

These young stars can be observed in the faint bridge that connects the two galaxies at the bottom of the image. This bridge serves as a pathway for the exchange of gas and dust, which in turn gives rise to the creation of new stars.

Scientists view Arp 271 as a valuable model for understanding future interactions between our own Milky Way galaxy and our neighboring Andromeda galaxy. This anticipated event is predicted to occur approximately 4 billion years from now.

This article is republished from PhysORG under a Creative Commons license. Read the original article.

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