# Interacting galaxy

Interacting galaxies (colliding galaxies) are galaxies whose gravitational fields result in a disturbance of one another. Major mergers occur between galaxies with similar amounts of mass, whereas minor mergers involve galaxies with masses that vary significantly. An example of a minor interaction is a satellite galaxy disturbing the primary galaxy's spiral arms. An example of a major interaction is a galactic collision, which may lead to a galaxy merger.

## Satellite interaction

A giant galaxy interacting with its satellites is common. A satellite's gravity could attract one of the primary's spiral arms. Alternatively, the secondary satellite can dive into the primary galaxy, as in the Sagittarius Dwarf Elliptical Galaxy diving into the Milky Way. That can possibly trigger a small amount of star formation. Such orphaned clusters of stars were sometimes referred to as "blue blobs" before they were recognized as stars.

## Galaxy collision

Colliding galaxies are common during galaxy evolution. The extremely tenuous distribution of matter in galaxies means these are not collisions in the traditional sense of the word, but rather gravitational interactions. As a result, some galaxy features such as star formation, shape, and size are impacted by interactions with other galaxies.
Colliding may lead to merging if two galaxies collide and do not have enough momentum to continue traveling after the collision. As with other galaxy collisions, the merging of two galaxies may create a starburst region of new stars. This starburst is an example of an increased star formation rate within the merged galaxies. A study conducted in 2024 shows that a key component in determining this change in star formation rate is the masses of the two galaxies involved. It suggests that if the two galaxies are of similar mass to begin with, this increase in star formation rate will be greater. When a starburst region is created, the galaxies fall back into each other and eventually merge into one galaxy after many passes through each other. If one of the colliding galaxies is much larger than the other, it will remain largely intact after the merger. The larger galaxy will look much the same, while the smaller galaxy will be stripped apart and become part of the larger galaxy. When galaxies pass through each other, unlike during mergers, they largely retain their material and shape after the pass.
Galactic collisions are now frequently simulated on computers, which use realistic physics principles, including the simulation of gravitational forces, gas dissipation phenomena, star formation, and feedback. Dynamical friction slows the relative motion of galaxy pairs, which may possibly merge at some point, according to the initial relative energy of the orbits. A library of simulated galaxy collisions can be found at the Paris Observatory website GALMER.

## Gallery

* UGC 2369 taken by HST.
* Close encounter at IRAS 06076-2139.
* Interacting galaxies NGC 4302 and NGC 4298 both located 55 million light-years away.
* Galaxy NGC 6052 merging into a single structure.
* Galaxy pair Zw I 136.
* ESO 576-69 is believed to be the nucleus of a former spiral galaxy.
* The Whirlpool Galaxy with its satellite NGC 5195.
* The Mice Galaxies.
* This simulation follows the collision of two spiral galaxies that harbour giant black holes.
* NGC 3447 comprises a couple of interacting galaxies.
* Barred spiral galaxy NGC 1512 in the process of a lengthy merger with NGC 1510, a dwarf elliptical galaxy.
* ESO 593-8 is an impressive pair of interacting galaxies with a feather-like galaxy crossing a companion galaxy.
* Antennae Galaxies NGC 4038 & NGC 4039 are a pair of interacting galaxies in the constellation Corvus.
* 2MASX J09133888-1019196, an interacting galaxy in the constellation of Hydra located 700 million light-years away. Both galaxies are beginning to merge, with a separation gap of only 130,000 light-years.
* Interacting galaxy pair, ESO 77-14 located in the constellation Indus. These galaxies are currently in a gravitational tug of war with each other, distorting their appendences.

## Galactic cannibalism

Galactic cannibalism is a common phenomenon. It refers to the process in which a large galaxy, through tidal gravitational interactions with a companion, merges with that companion. The most common result of the gravitational merger between two or more galaxies is a larger irregular galaxy, but elliptical galaxies may also result.
It has been suggested that galactic cannibalism is currently occurring between the Milky Way and the Large and Small Magellanic Clouds. Streams of gravitationally-attracted hydrogen arcing from these dwarf galaxies to the Milky Way is taken as evidence for the theory.

## Galaxy harassment

Galaxy harassment is a type of interaction between a low-luminosity galaxy and a brighter one that takes place within rich galaxy clusters, such as Virgo and Coma, where galaxies are moving at high relative speeds and suffering frequent encounters with other systems of the cluster due to the high galactic density.
According to computer simulations, the interactions convert the affected galaxy disks into disturbed barred spiral galaxies and produces starbursts followed by, if more encounters occur, loss of angular momentum and heating of their gas. The result would be the conversion of (late type) low-luminosity spiral galaxies into dwarf spheroidals and dwarf ellipticals.
Evidence for the hypothesis had been claimed by studying early-type dwarf galaxies in the Virgo Cluster and finding structures, such as disks and spiral arms, which suggest they are former disc systems transformed by the above-mentioned interactions. The existence of similar structures in isolated early-type dwarf galaxies, such as LEDA 2108986, has undermined this hypothesis.

## Notable examples

| Name | Type | Distance (million ly) | Magnitude | Notes |
| Milky Way Galaxy, LMC and SMC | SBc/SB(s)m/SB(s)m pec | 0 | | Satellites interacting with their primary |
| Whirlpool Galaxy (M51) | SAc (SB0-a) | 37 | +8.4 | Satellite interacting with its primary |
| NGC 1097 | SB(s)bc (E6) | 45 | +9.5 | Satellite interacting with its primary |
| Butterfly Galaxies NGC 4567/8 | SA(rs)bc / SA(rs)bc | 60 | +10.9 | Early phase of interaction |
| NGC 2207 and IC 2163 | SAc/SAbc | 114 | +11 | Galaxies going through the first phase in galactic collision |
| Mice Galaxies (NGC 4676A and NGC 4676B) | S0/SB(s)ab | 300 | +13.5 | Galaxies going through the second phase in galactic collision |
| Antennae Galaxies (NGC 4038/9) | SAc/SBm | 45 | +10.3 | Galaxies going through the third phase in galactic collision |
| NGC 520 | S | 100 | +11.3 | Galaxies going through the third phase in galactic collision |
| NGC 2936 | Irr | 352 | +12.9 | ? |

## Andromeda–Milky Way collision

Astronomers have estimated the Milky Way Galaxy will collide with the Andromeda Galaxy in about 4.5 billion years. Thanks to the Hubble Space Telescope, astronomers were able to more accurately track Andromeda's movement, leading to the conclusion that the two galaxies will temporarily touch before eventually undergoing an ultimate merging. Some think the two spiral galaxies will eventually merge to become an elliptical galaxy whose gravitational interactions will fling various celestial bodies outward, evicting them from the resulting elliptical galaxy. or perhaps a large disc galaxy.