DEEP FIELDthe cosmos · ch·11
Chapter 11 · Galaxies & Cosmology

The Cosmos

Three movements outward — from our neighbour galaxies, to the energy budget of everything, to worlds you can turn in your hand.

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The island universes

Ultraviolet image of the Andromeda Galaxy
M31 · Andromeda — our nearest large neighbour, 2.5 million light-years out, shown in ultraviolet where its youngest stars burn brightest.

The claim A century ago astronomers argued in public over whether the "spiral nebulae" were inside the Milky Way. They are not — they're other galaxies, hundreds of billions of them, each a hundred billion suns give or take, colliding, merging and evolving on billion-year clocks.

The Milky Way, from inside

A barred spiral roughly 100,000 light-years across, holding on the order of 100–400 billion stars, with Sagittarius A* anchoring the centre and our Sun orbiting once every ~230 million years, two-thirds of the way out. We've never seen it from outside — every "photo of the Milky Way" is either the band across our sky or another galaxy standing in.

Andromeda is coming

M31 is approaching at ~110 km/s, and for years the standard line was a merger in about 4.5 billion years. Honest update: a 2025 analysis in Nature Astronomy, folding in the tug of satellite galaxies, put the odds of a merger within 10 billion years at roughly a coin flip. Either way — no star-on-star collisions. Galaxies are mostly empty space passing through empty space.

The Whirlpool Galaxy spiral structure
M51 · Whirlpool — a grand-design spiral mid-interaction with a smaller companion.
The Sombrero Galaxy seen edge-on
M104 · Sombrero — seen nearly edge-on, its dust lane cutting the bulge in half.
The colliding Antennae galaxies
Antennae — two galaxies in the act of merging, throwing off tidal streamers.
Infrared view of the Milky Way's central region
Galactic centre — our own core in infrared, cutting through the dust that hides it.
JWST image of a galaxy cluster used to map dark matter
Webb cluster — a foreground cluster lensing the galaxies behind it into arcs.

Lensing, in one sentence Mass bends light, so a foreground cluster acts as a natural telescope — smearing background galaxies into arcs — and the shape of the distortion reveals where the invisible mass sits. It's how the Webb cluster above maps dark matter without ever seeing it.

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The universe, entire

Cosmology asks the biggest possible questions with the plainest possible data: one baby picture, one expansion rate, one energy budget. Here are all three — including the part where the numbers disagree.

All-sky map of the cosmic microwave background
The baby picture — the entire sky, unrolled. It glows at 2.725 K in every direction: the stretched-out flash of the moment the universe first turned transparent. The speckles are temperature differences of a few parts in 100,000, and every galaxy that exists grew from one of them.

The budget of everything

The open argument: Hubble tension

Planck · CMB fit
67.4km/s/Mpc · predicted from the early universe
~8% gap
SH0ES · Cepheids + SNe
~73km/s/Mpc · measured nearby

Why it matters. The two methods should agree, and stubbornly don't — the gap has survived a decade of error-hunting. It may be a subtle systematic. It may be the first crack in the standard model of cosmology. This is what a live scientific controversy looks like, mid-argument. (The Cepheid rung of that ladder was built by Henrietta Leavitt — section 24.)

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Five worlds in four dimensions

Real spacecraft-derived maps wrapped onto spinning globes — three dimensions of shape plus the fourth, time, as each world turns at its true axial tilt. Saturn wears its rings; Uranus rolls by on its side, exactly as it really does. Drag any globe to explore.

Mars

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