Big groups of stars can meet.
They crash into each other. This makes many new stars. It is a big, busy event. We can see them far away. Do you like looking at the stars?
Big groups of stars can meet.
These groups are called galaxies. Sometimes, two galaxies crash into each other. This is called a merger.
When they hit, clouds of gas crash too. This makes many new stars. Most of the gas gets used up. Soon, the new galaxy has very few young stars. Our own home galaxy will hit another one soon.
It will happen in a long time.
Sometimes, big groups of stars meet. These groups are called galaxies. A galaxy merger happens when two or more galaxies collide.
This is a very violent event.
During a merger, gravity pulls the galaxies together. This changes how the stars move. In disk galaxies, stars usually move in an orderly way. During a merger, this motion becomes random. This change is called violent relaxation. The stars end up in a messy network of paths. This often makes a new elliptical galaxy.
Mergers also make many new stars. Giant clouds of gas crash into each other. These crashes make new stars grow very fast. A major merger can make thousands of new stars each year. Our own Milky Way only makes a few stars a year.
Most of the gas gets used up during the crash. This means the new galaxy will have few young stars left. Some mergers are minor. This is when a big galaxy eats a small one. Our Milky Way is doing this now. It is absorbing small galaxies.
In 4.5 billion years, we will hit the Andromeda galaxy.
A galaxy merger is a massive event in space. It happens when two or more galaxies collide. These collisions are the most violent types of interaction between galaxies. Scientists study them to understand how galaxies grow over long periods of time. By looking at mergers, we can learn how galaxies reach their current forms. The merger rate helps astronomers measure how galaxies change through evolution.
Gravity is the main force that drives these huge collisions. As galaxies approach each other, their gravity pulls on the stars and dark matter. In disk galaxies, stars usually move in an orderly, rotating way. During a merger, this orderly motion turns into random energy. This process is called violent relaxation. The stars lose their old paths and move in a complicated, random network. This often results in a new shape called an elliptical galaxy.
Mergers are also famous for making many new stars. Large clouds of gas, called molecular clouds, rush toward the center of the merging galaxies. These clouds crash into each other and create new stars. A major merger can create thousands of solar masses of new stars every year. This is much faster than our Milky Way, which makes only about two new stars each year. However, these mergers also use up most of the available gas. This means the new galaxy will eventually have very few young stars left.
Computers help us see these events through simulations. One famous simulation shows what will happen to our Milky Way and the Andromeda galaxy. In about 4.5 billion years, these two galaxies will collide. Scientists believe they will fuse into one giant elliptical galaxy. Researchers like Jennifer Lotz have used the Hubble Space Telescope to study these events. Her team created 57 different merger scenarios to understand different ways galaxies might join.
We can group mergers by how many galaxies are involved. A binary merger involves two galaxies, while a multiple merger involves three or more. There are also minor mergers where a large galaxy "eats" a smaller one. This is sometimes called galactic cannibalism. Our Milky Way is actually doing this right now with the Canis Major Dwarf Galaxy. Some mergers are "wet" because the galaxies have lots of gas. Others are "dry" if the galaxies have very little gas left to use.
A galaxy merger is a massive cosmic event where two or more galaxies collide. These interactions are considered the most violent types of movement in the universe. Astronomers study these mergers because they act as a fundamental measurement of galaxy evolution. By observing these collisions, scientists gain clues about how galaxies grew into their current shapes over billions of years. The merger rate helps us understand the long-term history of the cosmos.
Gravity is the primary engine behind these massive collisions. As galaxies approach one another, their gravitational pull begins to affect the stars and dark matter within each system. In many galaxies, stars follow an orderly rotation within flat disks. However, as the merger progresses, the gravitational potential changes very quickly. This causes a process called violent relaxation, where star orbits are greatly altered. The stars lose their original paths and move in a complicated, random network. This transformation of ordered motion into random energy is why many mergers result in elliptical galaxies.
Mergers also act as intense factories for new stars. During a major merger, giant molecular clouds rush toward the center of the colliding systems. When these clouds collide with one another, they condense into new stars. The star formation rate (SFR) during a major merger can reach thousands of solar masses per year. This is a massive increase compared to our own Milky Way, which produces only about two new stars each year. However, this process is also self-limiting. The intense activity uses up most of the available gas, leaving very little for future star formation.
Because they use up so much gas, merged galaxies often enter a phase called the post-starburst (PSB) phase. In this stage, the galaxy has very few young stars left because the gas has been depleted. This is a common characteristic of elliptical galaxies seen in the local universe. Scientists believe many elliptical galaxies are the end products of major mergers that occurred 1 to 10 billion years ago. These ancient mergers were more pronounced because galaxies contained much more gas and molecular clouds back then. A major merger can quench star formation more rapidly than almost any other phenomenon in the universe.
Astronomers classify mergers in several different ways. They can be grouped by the number of galaxies involved, such as a binary merger of two galaxies or a multiple merger of three or more. They can also be classified by size. A minor merger occurs when one galaxy is significantly larger than the others. The larger galaxy often "eats" the smaller one in a process called galactic cannibalism. In contrast, a major merger involves two galaxies of similar size. Our own Milky Way is currently experiencing minor mergers with the Canis Major Dwarf Galaxy and possibly the Magellanic Clouds.
Another way to classify mergers is by their gas richness. A wet merger happens between gas-rich "blue" galaxies and typically triggers massive star formation and quasar activity. A dry merger involves gas-poor "red" galaxies and mainly serves to increase stellar mass without much new star formation. There are also damp mergers, which involve one blue and one red galaxy with enough gas to fuel some star formation. Mixed mergers occur when gas-rich and gas-poor galaxies combine. These different types of collisions lead to very different types of resulting galaxies.
To understand these complex events, scientists use advanced computer simulations. Researchers like Jennifer Lotz have used these tools to interpret images from the Hubble Space Telescope. Her team studied 57 different merger scenarios, looking at different orbits, impact angles, and orientations. Other researchers use deep learning and convolutional neural networks to predict the timescales of these events. For example, simulations can predict how long it takes for galaxies to reach maximum separation or to fully fuse. One famous prediction involves our own neighborhood: the Milky Way and Andromeda are expected to collide in about 4.5 billion years. This major merger will likely transform both spiral galaxies into one giant elliptical galaxy.
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