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Our neighbours: Andromeda and the Local Group

The light from the Andromeda galaxy left it about 2.5 million years ago.

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An irregular galaxy, the type of the Large Magellanic Cloud, which orbits the Milky Way. Switch to "Barred spiral" for the shape shared by the Milky Way and Andromeda.

A small group of galaxies

Galaxies are not scattered evenly. NASA explains that they gather into groups of about 100 or fewer members held together by their own gravity, while larger clusters may contain thousands. The Milky Way belongs to the Local Group, which NASA's galaxies page says holds more than 50 galaxies; an older NASA Hubble page says more than 20, a reminder that the count keeps rising as faint dwarf galaxies are found. Most members are dwarfs with up to a few billion stars. Only a few are large, and the biggest is the Andromeda galaxy, our nearest large neighbour.

Zoom out further and the Local Group sits just off the edge of the Virgo cluster and is part of a much larger structure, the Laniakea supercluster. NASA notes that superclusters are not held together by gravity as a whole. Together with empty voids and long walls of galaxies they make up the cosmic web, the largest pattern of matter in the universe.

The Magellanic Clouds

From the Southern Hemisphere two fuzzy patches are visible to the naked eye: the Large and Small Magellanic Clouds, dwarf galaxies that orbit the Milky Way. JPL gives the Large Magellanic Cloud a distance of about 160,000 light-years and a width about one third of the Milky Way's; if it could be seen in full it would cover as much sky as about 480 full Moons. It is full of star-forming regions, including the Tarantula Nebula. These two clouds also changed astronomy: studying variable stars there, Henrietta Swan Leavitt found that a Cepheid's pulsing period is tied to its true brightness, which made Cepheids a way to measure distances.

How Andromeda became a galaxy

BackgroundA century ago many astronomers thought the Milky Way was the whole universe, and that fuzzy spirals such as the "Andromeda Nebula" were clouds inside it. In 1923 Edwin Hubble, using the 100-inch Hooker Telescope at Mount Wilson Observatory, then the largest in the world, found a Cepheid variable star in Andromeda on a glass plate dated 6 October 1923. He first marked it as a nova, then crossed that out and wrote "VAR!" when he saw it vary. Using Leavitt's period rule he worked out a distance far beyond the edge of the Milky Way. Andromeda was a separate galaxy, and the universe was suddenly far larger. The star, called V1, is still watched today.

NASA gives Andromeda's distance as about 2.5 million light-years, or 0.8 megaparsecs. That makes it about 25 Milky Way diameters away, and it is the most distant object most people can see with the naked eye. Its light left it about 2.5 million years ago. Like the Milky Way it is a barred spiral, and it is somewhat larger.

Will we collide?

Andromeda is moving towards us. In 2012 an analysis of Hubble observations by Roeland van der Marel and Tony Sohn suggested a direct hit within about 5 billion years. In 2025 a team led by Till Sawala combined newer Hubble data with ESA's Gaia mission, tested 22 uncertain quantities, and ran 100,000 simulations. They found only about a 50% chance that the two galaxies merge within the next 10 billion years, and about a 2% chance of a head-on collision in just 4 to 5 billion years. The Large Magellanic Cloud pulls the Milky Way off course, making a merger a little less likely, while Andromeda's companion M33 pulls the other way. As ESA points out, the Sun will likely burn out in about 5 billion years anyway.

Andromeda distance (NASA)About 2.5 million light-years
Large Magellanic Cloud distance (JPL)About 160,000 light-years
Who proved Andromeda is a galaxyEdwin Hubble, 1923, with the Cepheid V1
Cepheid period ruleHenrietta Swan Leavitt
Chance of merging within 10 billion years (2025)About 50%
  1. What is the Local Group?
    • The small group of galaxies that includes the Milky Way
    • The planets near the Sun
    • The stars of Orion
    • A cluster of thousands of galaxies in Virgo
  2. Andromeda is about 2.5 million light-years away and the Milky Way about 100,000 light-years wide. How many Milky Way widths is that?
  3. What kind of star let Hubble measure the distance to Andromeda?
    • A Cepheid variable
    • A white dwarf
    • A red dwarf
    • A neutron star
  4. Before 1923, what did many astronomers think the "Andromeda Nebula" was?
    • A cloud inside the Milky Way
    • A planet
    • A comet
    • The Sun's twin
  5. Who discovered the link between a Cepheid's period and its brightness?
    • Henrietta Swan Leavitt
    • Galileo Galilei
    • Annie Jump Cannon
    • Tycho Brahe
  6. The 2025 study found about a 2% chance of a head-on collision within 4 to 5 billion years. Out of 100,000 simulations, about how many?
  7. What did the 2025 Hubble and Gaia study conclude?
    • About a 50% chance of a merger within 10 billion years
    • A collision is certain in 4.5 billion years
    • Andromeda is moving away
    • The galaxies already merged
  8. Which galaxy pulls the Milky Way off course and makes a merger a little less likely?
    • The Large Magellanic Cloud
    • M33
    • Andromeda
    • M87
  9. The Large Magellanic Cloud is about 160,000 light-years away. How many years ago did the light we see from it leave?
  10. Is the Laniakea supercluster held together by gravity as a whole?
    • No, NASA says superclusters are not bound
    • Yes, like a single galaxy
    • Yes, by a black hole at its centre
    • It is part of the Milky Way
Key points
  • The Milky Way belongs to the Local Group, more than 50 galaxies, mostly dwarfs.
  • Andromeda: about 2.5 million light-years, the largest neighbour, a barred spiral.
  • Large Magellanic Cloud: about 160,000 light-years, an irregular dwarf.
  • Hubble's 1923 Cepheid V1 showed Andromeda is a separate galaxy.
  • 2025: about a 50% chance of merging within 10 billion years.
Sources for this course (17)
  • NASA Galaxies (science.nasa.gov/universe/galaxies)
  • NASA Galaxy types (science.nasa.gov/universe/galaxies/types)
  • NASA Hubble's Galaxies (science.nasa.gov/mission/hubble/science/universe-uncovered/hubble-galaxies)
  • ESA/Hubble tuning fork (esahubble.org/images/heic9902o)
  • NASA Sun facts (science.nasa.gov/sun/facts)
  • NASA Stars (science.nasa.gov/universe/stars)
  • NASA/JPL Milky Way spiral arms (science.nasa.gov/resource/the-milky-way-galaxy)
  • JPL Large Magellanic Cloud (jpl.nasa.gov/images/pia07137-whats-old-is-new-in-the-large-magellanic-cloud)
  • NASA APOD Magellanic Clouds and Leavitt, NASA Hubble V1 asset (science.nasa.gov/asset/hubble/cepheid-variable-star-v1-in-andromeda-galaxy)
  • NASA Edwin Hubble (science.nasa.gov/people/edwin-hubble)
  • NASA Hubble 100 years (science.nasa.gov/missions/hubble/nasa-celebrates-edwin-hubbles-discovery-of-a-new-universe)
  • NASA and ESA Andromeda collision 2025 (science.nasa.gov/missions/hubble/apocalypse-when-hubble-casts-doubt-on-certainty-of-galactic-collision, esahubble.org/news/heic2508)
  • JPL Event Horizon Telescope Sagittarius A* (jpl.nasa.gov/edu/resources/teachable-moment/telescopes-get-extraordinary-view-of-milky-ways-black-hole)
  • NASA Hubble Deep Fields (science.nasa.gov/mission/hubble/science/universe-uncovered/hubble-deep-fields)
  • NASA 2016 galaxy census (science.nasa.gov/missions/hubble/hubble-reveals-observable-universe-contains-10-times-more-galaxies-than-previously-thought)
  • NASA New Horizons cosmic background with correction (science.nasa.gov/missions/hubble/new-horizons-spacecraft-answers-question-how-dark-is-space)
  • CERN Courier Hubble tension (cerncourier.com/a/the-hubble-tension).

Checked: 2026-10-17