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Black holes at the centres of galaxies

Sagittarius A*, at the centre of the Milky Way, has about 4 million times the Sun's mass.

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A black hole with a glowing disk of infalling gas, from the end of a very massive star's life. The supermassive black holes in galaxy centres look similar in outline but are millions to billions of times heavier. Change the stage to see how a stellar black hole forms.

A dark mass at the centre

NASA says most large galaxies have supermassive black holes at their centres, some with billions of times the Sun's mass. A black hole is a region where matter is packed so tightly that nothing, not even light, can escape from inside a boundary called the event horizon. The radius of that boundary grows in step with mass. For one solar mass it is about 3 km. For the Milky Way's central black hole, Sagittarius A* (said "Sagittarius A-star"), with about 4 million solar masses, it works out at about 12 million km, roughly 17 times the Sun's radius and well inside Mercury's orbit.

How can anyone weigh something that gives off no light? By watching what moves around it. For decades, two research groups, one in Germany and one in the United States, followed individual stars orbiting very close to the galactic centre in infrared light, which passes through the dust. One star, called S2, swings round the centre in about 16 years. Applying Kepler's laws to those orbits gives the mass packed inside them, about 4 million Suns in a region too small to be anything except a black hole. That work was recognised with the 2020 Nobel Prize in Physics.

Pictures of shadows

Black holes themselves are dark, but hot gas swirling around them glows. The Event Horizon Telescope links radio dishes across the world into a virtual telescope the size of Earth. In 2019 it released the first image of a black hole's silhouette, the one at the centre of the giant elliptical galaxy M87, about 53 million light-years away according to JPL. In 2022 it released an image of Sagittarius A*, which JPL describes as more than 26,000 light-years away with the mass of 4 million Suns. Both pictures show a dark centre inside a bright ring. The Sagittarius A* image spans only about 50 microarcseconds, which JPL compares to about 1/13th of a billionth of the whole sky.

Distances to the galactic centre are quoted as about 26,000 or about 27,000 light-years on different NASA pages. Both are rounded versions of measurements near 26,000 to 27,000; the difference is within the precision of the round numbers.

Quiet and active

Sagittarius A* is quiet today: little gas is falling in, so it is faint. NASA notes that the Milky Way is not currently an active galaxy, although it likely had a burst of activity in the past few million years. In active galaxies, a central black hole is swallowing plenty of gas, which heats up in a disk and can outshine all the galaxy's stars. The most luminous are quasars. NASA says more than a million quasars have been identified; the nearest, Markarian 231, is about 600 million light-years away, and the farthest known lies about 13 billion light-years away. Because light takes time to arrive, distant quasars show black holes as they were billions of years ago.

Milky Way's central black holeSagittarius A*, about 4 million solar masses
Event horizonBoundary inside which not even light escapes
First black hole image (2019)M87*, in a giant elliptical about 53 million light-years away
Sagittarius A* imageReleased in 2022 by the Event Horizon Telescope
QuasarThe most luminous kind of active galaxy
  1. What do most large galaxies have at their centres?
    • A supermassive black hole
    • A giant star
    • Nothing at all
    • A planet
  2. The event horizon radius is about 2.95 km per solar mass. For 4 million solar masses, how many million km? (one decimal)
  3. How many Sun radii (695,700 km) is 11.8 million km? (whole number)
  4. How was the mass of Sagittarius A* measured?
    • From the orbits of stars close to it
    • By weighing light from it
    • By sending a probe
    • From its colour
  5. Why did astronomers track stars near the centre in infrared light?
    • Infrared passes through the dust that hides the centre
    • The stars give off only infrared
    • Infrared is faster than light
    • Visible light telescopes do not exist
  6. Which black hole was the first to be imaged, in 2019?
    • M87*, in the galaxy M87
    • Sagittarius A*
    • The one in Andromeda
    • One in the Large Magellanic Cloud
  7. What makes the bright ring in black hole images?
    • Hot gas swirling close to the black hole
    • Light from the black hole itself
    • A ring of planets
    • Reflected sunlight
  8. NASA says the nearest quasar, Markarian 231, is about 600 million light-years away. How many times the distance to Andromeda (2.5 million) is that?
  9. Is the Milky Way an active galaxy today?
    • No, but it likely had a burst of activity in the past few million years
    • Yes, it is a quasar
    • Yes, it is the brightest galaxy known
    • No, it has no black hole
  10. Looking at a quasar 13 billion light-years away shows a black hole ...
    • as it was about 13 billion years ago
    • as it is right now
    • as it will be in the future
    • as seen from inside it
Key points
  • Most large galaxies have a supermassive black hole at the centre.
  • Sagittarius A*: about 4 million solar masses; event horizon about 12 million km.
  • Its mass comes from the orbits of nearby stars such as S2.
  • Event Horizon Telescope images: M87* (2019) and Sagittarius A* (2022).
  • Active galaxies and quasars are lit by gas falling into the central black hole.
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