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Galaxy Details and Mergers

Galaxies evolve through gravitational interaction with their neighbors, creating a menagerie of forms.

Comma shaped curved cloud of gases in bright white edged with bright-pink star forming regions, and threaded with rusty-brown tendrils of dust at center and throughout the comma shaped merger. All set against the black of deep space.

Astronomer Edwin Hubble pioneered the study of galaxies based simply on their appearance and categorized them according to three basic shapes: spiral, elliptical, and irregular. Some 60 years later, the sharp vision of the space telescope named in his honor began seeing unprecedented details in galaxies, revealing intricate, dark dust lanes and glowing knots of star formation. Hubble observations showed galaxies often interact, that mergers are common, and that galaxies grow and evolve by merging.

The Antennae Galaxies, officially designated as NGC 4038 and NGC 4039, present a celestial ballet within the vast cosmic theater. Located approximately 68 million light-years away in the Corvus constellation, these interacting galaxies are entangled in a cosmic dance, their long tidal tails resembling the antennae of an insect, hence their name. In this video, Dr. Jennifer Wiseman explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe. Credit: NASA’s Goddard Space Flight Center; Producer, Director & Editor: James Leigh

  • The Hubble telescope captured merging galaxies that look like a “Great Pumpkin,” a “Space Triangle,” “Antennae,” and “Mice.” For all their violence, galactic collisions take place at a snail’s pace – over timescales that span several hundred million years. Hubble captures a mere snapshot of these mergers.

    Galaxy Collision Creates ‘Space Triangle’ in New Hubble Image

    Two galaxies one right one on the left. right galaxy has a blue-white triangular star forming region surrounding it.
    The collision of galaxies NGC 2445 (right) and NGC 2444 fueled a frenzy of star birth that produced this unusual triangle of young, blue stars.
    NASA, ESA, STScI, Julianne Dalcanton (Center for Computational Astrophysics / Flatiron Inst. and University of Washington)
  • Hubble images of the “tadpole-like” Antennae and Mice galaxies reveal the gravitational turbulence these galaxies endure. The interacting duo called Arp 143 (the “Space Triangle”) holds a pair of distorted, star-forming spiral galaxies. Astronomers think the pair passed through each other, igniting a triangular firestorm of new stars.
    Mergers like this preview the coming collision between our own Milky Way and the neighboring Andromeda galaxy 4 billion years from now.

    Hubble Images of Galaxies with Tidal Tails

    Two galaxies interacting that look like mice with tails.
    The Mice or NGC 4676, they will eventually merge into a single giant galaxy.
    NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M. Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA
This computer simulation depicts the colliding galaxies that form “The Mice.”
Josh Barnes (University of Hawaii) and John Hibbard (National Radio Astronomy Observatory)

Hubble Science Highlights

Discover the breadth and depth of Hubble's exciting discoveries!

Hubble image left to right: Jupiter, Uranus, Saturn, Neptune

Studying the Planets and Moons

Hubble’s systematic observations chart the ever-changing environments of our solar system’s planets and their moons. 

animation of a binary asteroid with a shifting tail

Tracking Evolution in the Asteroid Belt

These conglomerates of rock and ice may hold clues to the early solar system.

Three views of Pluto. Three mottled circles in colors of yellow, grey, rusty-orange, and black.

Uncovering Icy Objects in the Kuiper Belt

Hubble’s discoveries helped NASA plan the New Horizon spacecraft’s flyby of Pluto and beyond.

The Mystic Mountain is seen as a chaotic pillar of colorful gas and dust, narrowing toward the top of the image. The dust and gas is mostly yellow, brown, and orange, all jutting against a hazy purple and blue background with a few pink stars.

Exploring the Birth of Stars

Seeing ultraviolet, visible, and near-infrared light helps Hubble uncover the mysteries of star formation.

Hubble image of the Crab Nebula

The Death Throes of Stars

When stars die, they throw off their outer layers, creating the clouds that birth new stars.

Thirty proplyds in a 6 by 5 grid. Each one is unique. Some look like tadpoles, others like bright points in a cloudy disk.

Finding Planetary Construction Zones

Hubble’s sensitivity uncovers the seeds of planets in enormous disks of gas and dust around stars.

Artist's impression of the ten hot Jupiter exoplanets. Two rows of exoplanet illustrations. There are 5 planets of varying sizes, colors, and atmospheric features in each row.

Recognizing Worlds Beyond Our Sun

Hubble can detect and measure the basic organic components for life on planets orbiting other stars.

Hubble view of an expanding halo of light around star v838 monocerotis

Seeing Light Echoes

Like ripples on a pond, pulses of light reverberate through cosmic clouds forming echoes of light.

Hubble Ultra Deep Field image

Tracing the Growth of Galaxies

Hubble’s Deep Field observations are instrumental in tracing the growth of galaxies.

Computer simulation of a supermassive black hole at the core of a galaxy. Center is a black circle. Surrounding the black circle are arcs of red, blue, orange, and white. Further out from the circle are blotches of red, blue, orange, and white representing celestial objects.

Monster Black Holes are Everywhere

Supermassive black holes lie at the heart of nearly every galaxy.

Six Hubble images in a grid of three across and two down. Each is a gamma-ray burst in a host galaxy. The images are orange-red and white with hints of yellow.

Homing in on Cosmic Explosions

Hubble helps astronomers better understand and define some of the largest explosions in the universe.

Cepheid star in Andromeda galaxy (Hubble observations)

Discovering the Runaway Universe

Our cosmos is growing, and that expansion rate is accelerating.

A field of galaxies along with the curved arcs of gravitationally lensed galaxies.

Focusing in on Gravitational Lenses

Gravitational lenses are ‘Nature’s Boost’, expanding our view deeper into space and farther back in time.

A cluster of galaxies fills the frame. A purple glow around the largest concentrations of galaxies indicates the distribution of dark matter.

Shining a Light on Dark Matter

The gravitational pull of dark matter guides the formation of everything we can see in the universe.

Top: Three views going back in time show slices of the cosmos. Bottom: A computer simulated, 3-D map of the distribution of dark matter.

Mapping the Cosmic Web

Filaments and sheets of matter create an interconnected web that forms the large-scale structure of the universe.