A barred spiral galaxy spanning 100,000 light-years, home to hundreds of billions of stars and one of the deepest mysteries in modern science.
March 20268 Sources9 Slides
By the Numbers
100,000
Light-years across — the diameter of the Milky Way's stellar disk
100-400B
Estimated number of stars, most too faint or dust-obscured to count
4.3M
Solar masses of Sagittarius A*, our central supermassive black hole
13.6B
Years old — age of the oldest stars in the galaxy's halo
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Structure & Our Address
A barred spiral with six components: nucleus, central bulge, thin & thick disk, spiral arms, stellar halo, and a massive dark-matter halo
The Sun orbits 26,000 light-years from the centre in the Orion-Cygnus Arm — the galaxy's suburbs
One orbit takes 250 million years at 800,000 km/h. Earth has completed only 18 laps in its lifetime
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Sagittarius A*
First directly imaged in May 2022 by the Event Horizon Telescope — strong magnetic fields spiral from its edge
Currently quiescent, but evidence shows it erupted violently within the last few centuries, creating Fermi Bubbles blasting outward at 2 million mph
Tracking stars around it earned Genzel & Ghez the 2020 Nobel Prize in Physics
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The Dark Matter Mystery
~95% of the Milky Way's mass is dark matter — invisible, detectable only through gravity. Its particle nature remains unknown
A mysterious gamma-ray glow at the galactic centre may be colliding dark matter particles — or thousands of millisecond pulsars (2025, Physical Review Letters)
The galaxy may be missing ~20% of predicted dark matter, challenging cosmological models
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Recent Breakthroughs
Dec 2025: Simulations show the Milky Way's chemical split may not require an ancient collision — overturning a decade of assumption
Jan 2026: A new MWA radio image maps 98,000 sources with 10x sensitivity, revealing hidden supernova remnants and stellar nurseries
Mar 2026: The galaxy sits inside a giant dark-matter "pancake" stretching tens of millions of light-years, solving a 50-year puzzle
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A Cannibal Galaxy
The Milky Way actively devours smaller galaxies — dozens of faint stellar streams are the shredded remains of past victims
The disk is warped and wobbles like a spinning top, possibly from the gravitational tug of the Large Magellanic Cloud
Gaia catalogued 2 billion stars and 3 trillion measurements before retiring in 2025, with final data releases still ahead
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The Andromeda Question
A Milky Way-Andromeda collision was once called inevitable. A 2025 Nature Astronomy study revised the odds to just 50/50 over 10 billion years
Only a 2% chance of a head-on collision in the next 4-5 billion years — the galaxies may simply sail past each other
If they do merge, the result would be "Milkomeda" — a giant elliptical galaxy, but with a relatively mild starburst
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What's Next
Gaia DR4 & DR5 — Final releases (2026, ~2030) will complete the most detailed 3-D map of the galaxy ever made
Cherenkov Telescope Array — May resolve whether the galactic centre glow is dark matter or pulsars
Vera C. Rubin Observatory — Its 10-year survey will uncover faint stellar streams and dwarf galaxy remnants
JWST — Finding Milky Way twins at high redshift, showing us what our galaxy looked like billions of years ago