Galaxy time: the 230-million-year year
On the scale of the galaxy, a year is a lap of the Milky Way. Watch your journey tick up live, and meet the three spiral galaxies of our Local Group.
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around the centre of the Milky Way, at about 230 km/s.
- …and since 1 January—
- Milky Way and Andromeda closer by0 km
- Our motion against the Big Bang's afterglow0 km
The galactic year
The Sun, with everything orbiting it, travels around the centre of the Milky Way at roughly 230 km per second. Even at that speed one lap takes about 230 million years — a galactic year (estimates run from 225 to 250 million, depending on the speed and radius assumed).
That gives a strange calendar. The Sun and Earth are about 20 galactic years old. The last time the Solar System was at this point in its orbit, the first dinosaurs were appearing in the Triassic. All of recorded human history fits inside the last 1/45,000th of one galactic year.
| In galactic time… | Earth time | Galactic years |
|---|---|---|
| One full orbit of the Milky Way | ≈ 230 million years | 1 |
| Age of the Sun | 4.6 billion years | ≈ 20 |
| Since the dinosaurs died out | 66 million years | ≈ 0.29 |
| Since Homo sapiens appeared | 300,000 years | ≈ 0.0013 |
| Since writing was invented | 5,200 years | ≈ 0.000023 |
| A human lifetime of 80 years | 80 years | ≈ 0.00000035 |
Where the galaxies are in your sky right now
Five of our galactic neighbours can be seen without a telescope, though not all from the same place. Andromeda and Triangulum are northern-sky objects; the two Magellanic Clouds — small satellite galaxies of the Milky Way — never rise for most of the northern hemisphere and hang high in the southern sky. The chart below draws the real sky over your city and marks each one.
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Times are shown in your device's own time zone.
How to read it: the centre is straight overhead and the rim is the horizon. Hold it above your head with N towards north — east and west are swapped compared with a map because you're looking up, not down.
Your cosmic address
Writing an address from the inside out, the way you would on a letter:
- Earththird planet from the Sun
- Solar Systemthe Sun's bubble of solar wind, whose edge Voyager 1 crossed in 2012, about 17 light-hours out
- Local Interstellar Clouda thin cloud of gas, about 30 light-years across, the Sun is passing through
- Orion–Cygnus Arma minor spiral arm of the Milky Way, about 26,700 light-years from the centre
- Milky Way Galaxya barred spiral of 100–400 billion stars
- Local Groupmore than 80 galaxies in about 10 million light-years, dominated by the Milky Way and Andromeda
- Virgo Superclusterthe Local Group's neighbourhood, centred on the Virgo Cluster 54 million light-years away
- Laniakea Superclusterabout 100,000 galaxies flowing towards a common centre, mapped in 2014; the name means "immense heaven" in Hawaiian
The three spirals of the Local Group
Of the Local Group's galaxies, only three are big spirals. Each has its own page with live sky positions and viewing seasons.
| Milky Way | Andromeda (M31) | Triangulum (M33) | |
|---|---|---|---|
| Type | Barred spiral | Spiral | Spiral (loosely wound) |
| Distance | We're inside it | ≈ 2.5 million ly | ≈ 2.73 million ly |
| Disk diameter | ≈ 100,000 ly | ≈ 150,000–220,000 ly | ≈ 60,000 ly |
| Stars | 100–400 billion | ≈ 1 trillion | ≈ 40 billion |
| Central black hole | Sagittarius A*, 4.3 million Suns | ≈ 100 million Suns | None detected |
| Seen with the naked eye | As a band across dark skies | Easily, as a fuzzy oval | Only under very dark skies |
How fast are you moving, really?
Sitting still is a matter of opinion. Each speed below is measured against a different reference point, and they add up in different directions.
| Motion | Speed | Measured against |
|---|---|---|
| Earth's spin (at the equator) | 0.47 km/s | Earth's axis |
| Earth around the Sun | 29.8 km/s | The Sun |
| Sun around the Milky Way | ≈ 230 km/s | The galaxy's centre |
| Andromeda towards the Milky Way | ≈ 110 km/s | The Milky Way |
| Sun relative to the cosmic microwave background | ≈ 370 km/s | The Big Bang's afterglow — the closest thing to an absolute rest frame |
Galaxy shapes: Hubble's tuning fork
In 1926 Edwin Hubble sorted galaxies by shape, and his diagram — later drawn as a tuning fork — is still the starting point. Ellipticals (E0 round to E7 flattened) are smooth balls of old stars with little gas left to make new ones. Spirals have a disc, arms and ongoing star birth; Sa have big bulges and tight arms, Sc small bulges and loose arms. About two-thirds of spirals, including ours, have a bar of stars across the middle (SBa–SBc). Lenticulars (S0) sit at the fork: a disc but no arms. Irregulars, like the Magellanic Clouds, fit nowhere.
Hubble thought galaxies might evolve along the diagram from left to right. They don't — but the shapes do record history. Big ellipticals are mostly the products of galaxies merging, which is the likely fate of the Milky Way and Andromeda. In modern notation the Milky Way is an SBbc, Andromeda an SA(s)b and Triangulum an SA(s)cd.
How many galaxies are there?
In December 1995 the Hubble Space Telescope stared for ten days at a tiny patch of apparently empty sky in Ursa Major — about as big as a tennis ball seen from 100 metres away. The Hubble Deep Field revealed around 3,000 galaxies. The Ultra Deep Field of 2004 found about 10,000 in a similar patch. Scaling up gives an answer in the hundreds of billions for the observable universe.
A 2016 study suggested two trillion, counting faint galaxies too dim to see. But in 2021 NASA's New Horizons probe, far beyond Pluto where the sky is darker than anywhere near Earth, measured the total background glow and found no room for that many hidden galaxies — pointing back to a few hundred billion. JWST is now counting the earliest ones directly.
How we learned there are other galaxies
- 1610
Galileo turns a telescope on the Milky Way and finds it is made of countless faint stars.
- 1755
Immanuel Kant suggests the faint elliptical nebulae are 'island universes' — whole star systems like ours.
- 1785
William Herschel counts stars in different directions to map the Milky Way as a flattened disc.
- 1845
Lord Rosse's giant telescope in Ireland reveals spiral structure in the Whirlpool Galaxy (M51).
- 1912
Henrietta Swan Leavitt finds that a Cepheid star's period reveals its true brightness — a cosmic measuring stick.
- 26 April 1920
The 'Great Debate' in Washington: Harlow Shapley and Heber Curtis argue whether spirals are inside the Milky Way.
- 1 January 1925
Hubble's Cepheid distances to Andromeda and Triangulum are announced, settling it: they are separate galaxies.
- 1929
Hubble shows galaxies are moving away from us faster the farther they are — the universe is expanding.
- 1995 →
Hubble's deep fields, then JWST, reveal galaxies back to within a few hundred million years of the Big Bang.
Frequently asked questions
What is a galactic year?
The time the Sun takes to orbit the centre of the Milky Way once: about 230 million years, with estimates from 225 to 250 million. It is also called a cosmic year.
How many times has the Sun orbited the galaxy?
About 20 times in its 4.6-billion-year life.
How many galaxies are in the Local Group?
More than 80 known members, almost all small dwarf galaxies. Only the Milky Way, Andromeda and Triangulum are large spirals.
How fast is the Solar System moving through the galaxy?
About 230 km/s, or roughly 828,000 km per hour, around the galactic centre.