Hubble Telescope Discovers Cosmic Bridge Between Colliding Galaxies

hubble telescope discovers cosmic bridge between colliding galaxies.jpg Science

In a stunning revelation from the cosmos, the Hubble Space Telescope has captured a captivating image of two colliding galaxies, known as the Arp 107 system, delicately linked by a faint "bridge" of gas. Hovering about 465 million light-years away from Earth, the two galaxies, in the midst of their merging process, are tethered together by a fragile stream of dust and gas. This cosmic spectacle is a testament to the Hubble’s Advanced Camera for Surveys, a collaboration between NASA and the European Space Agency, which has offered a new perspective into the intriguing dynamics of the Arp 107 system.

The larger of the two galaxies, a Seyfert galaxy, is a fascinating sight with its singular, large spiral arm encircling the galactic core. Seyfert galaxies are renowned for their unique composition where despite the core’s immense brightness, radiation from the entire galaxy can still be observed. This is vividly illustrated in the Hubble’s image, where the spiraling swirls of the entire galaxy are distinctly visible. The larger galaxy’s luminescent spiral arm, speckled with brilliant budding stars, is a testament to the stellar births fuelled by the abundant material siphoned from its smaller companion galaxy.

A Cosmic Dance: Hubble Witnesses Merging Galaxies

In a recent image from the Hubble Space Telescope, two galaxies in the process of merging are connected by a faint "bridge" of gas, providing a striking view of this cosmic dance. The Arp 107 system, which incorporates these partnering galaxies, is located approximately 465 million light-years from Earth. The image, captured by Hubble’s Advanced Camera for Surveys, showcases an intriguing intergalactic linkage formed by the delicate stream of dust and gas.

The Seyfert Galaxy: A Luminous Spectacle

At the heart of the image on the left is a large galaxy known as a Seyfert galaxy, characterized by an active galactic nucleus. Despite the intense luminosity of the core, radiation from the entire galaxy can be observed, as evident in the image where the spiraling whorls of the whole galaxy are readily visible. The activity of galactic nuclei is associated with the intense glow provoked by material falling into the supermassive black hole at the center of the galaxy. Such is the intensity of this radiation that it can outshine the combined light of every single star in its host galaxy.

Stellar Births in the Galactic Arm

Adding further charm to this cosmic spectacle, the Seyfert galaxy’s bright spiral arm is dotted with luminous budding stars. These stellar births are fuelled by the copious material being drawn from the smaller companion galaxy seen to the lower right of the image.

The Smaller Galaxy: A Fading Light

The smaller galaxy, though featuring a bright core, displays relatively faint spiral arms as it is gradually absorbed into the larger galaxy. This process of cosmic assimilation is highlighted by the stream of material that delicately connects the merging galaxies observed in the new Hubble visual released by the European Space Agency (ESA) on Sept. 18.

Arp 107: A Member of the Peculiar Galaxies

Arp 107 is part of the Atlas of Peculiar Galaxies, a collection compiled by Halton Arp in 1966. The recent Hubble photo is an initiative to observe lesser-studied members of the Arp catalog, with the intention of providing the public with images of these spectacular and not-easily-defined galaxies.


This celestial spectacle presented by the Hubble Space Telescope unravels another layer of the cosmic mystery, offering a mesmerizing view of the merging galaxies. It showcases the dynamic nature of our universe and the continual processes of creation and assimilation. It also underscores the value of ongoing space missions like Hubble and how they contribute to our understanding of the universe. The captivating visuals serve as a reminder of the infinite beauty and complexity of the cosmos, sparking curiosity and inspiring further exploration.

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