Let's learn how galaxies collide and merge in a cosmic dance, reshaping the universe and revealing the secrets of galaxy evolution.

Join us for an exciting new monthly astronomy series, hosted by RTL contributor Adriano Anfuso. Every first Sunday of the month, we’ll delve into a fascinating topic. This month, we'll explore the mesmerizing cosmic dance of galaxies – witnessing how they collide, merge, and reshape the universe.

Galactic cannibalism: the violent mergers of galaxies

In the vast expanse of the universe, galaxies aren't just isolated islands of stars – they are dynamic entities engaged in a cosmic dance. Sometimes, this dance takes a violent turn, leading to galactic cannibalism, where larger galaxies devour smaller ones. These colossal collisions, though destructive, play a vital role in shaping the cosmos and provide a fascinating glimpse into the processes of galaxy formation and evolution.

The dance of destruction: understanding galactic mergers

Galactic mergers occur when two or more galaxies pass close enough to each other that their mutual gravitational forces cause them to interact. This interaction can distort their shapes, trigger bursts of star formation, and, eventually, lead to a full merger where the galaxies combine into a single, larger galaxy.

These cosmic collisions are not quick or clean. They unfold over millions or even billions of years, with the galaxies stretching, warping, and ultimately blending into one another. The resulting galaxy often bears little resemblance to its original form, sometimes becoming an elliptical galaxy after the chaos subsides.

Implications for galaxy evolution

Such mergers help to explain the variety of galaxy shapes we observe in the universe. Elliptical galaxies, for example, are often the end products of such mergers, formed when two or more spiral galaxies collide and become one. The result is a galaxy with little remaining structure, just a smooth, featureless ellipsoid of stars.

Moreover, galactic mergers can have profound effects on the central supermassive black holes that reside in most galaxies. When two galaxies merge, their central black holes may eventually coalesce into an even more massive black hole, releasing enormous amounts of energy in the process.

While the term “galactic cannibalism” might sound menacing, these mergers are also a form of cosmic recycling. The collisions redistribute gas and dust, sparking new waves of star formation and breathing new life into old galaxies. This process ensures that even in destruction, the cosmos is continually renewing itself.

Evidence of cosmic collisions: the Antennae Galaxies

One of the most stunning examples of galactic cannibalism is the Antennae Galaxies, located about 45 million light-years away in the constellation Corvus. Named for their long, antenna-like tidal tails, these galaxies are in the midst of a dramatic collision. As their stars and gas clouds collide, they trigger intense regions of star formation, creating thousands of new stars in what astronomers refer to as “starburst” regions.

The Antennae Galaxies give us a vivid snapshot of what happens when galaxies collide. The bright knots of new stars, the twisted, elongated shapes, and the chaotic mixture of gas and dust all tell the story of a violent yet beautiful cosmic encounter. This example provides crucial insights into how galaxies grow and evolve over time.

The fate of our Milky Way

Galactic cannibalism is not just an occasional cosmic accident; it’s a fundamental process in galaxy evolution. Through these mergers, galaxies grow in size and complexity. Our own Milky Way is no stranger to this phenomenon—it has cannibalized several smaller galaxies in the past and is on a collision course with the Andromeda Galaxy, with a merger predicted to occur in about 4.5 billion years.

Currently about 2.5 million light-years away, Andromeda is in fact on a direct collision course with the Milky Way, travelling towards us at a speed of around 110 kilometres per second. This colossal event is expected to occur in approximately 4.5 billion years. As Andromeda approaches, the gravitational forces between the two galaxies will begin to distort their shapes, pulling stars and gas into elongated streams.

Eventually, these galaxies will merge, forming a new, larger galaxy that scientists like to call "Milkomeda". The collision will likely trigger bursts of star formation as gas clouds within both galaxies compress and ignite new stars. Despite the violent nature of this merger, the vast distances between stars mean that individual star collisions will be rare. However, the supermassive black holes at the centres of both galaxies are expected to eventually merge, creating an even more massive black one, and releasing an enormous amount of energy. This dramatic event will reshape the night sky and mark a new chapter in the history of our cosmic neighbour.

Galactic mergers are a testament to the dynamic and ever-changing nature of the universe. They show us that even on the grandest scales, the cosmos is a place of creation and destruction, of violence and beauty. As we observe these cosmic feasts, we gain a deeper understanding of the forces that shape galaxies and, by extension, the universe itself.

Adriano Anfuso is a photographer and digital creator who is passionate about capturing the awe-inspiring beauty of the cosmos and Earth's wonders. You can check out his work here.

This article was created in collaboration and features authentic images from ShaRa astrophotography project.