Paul Sutter

Chandrasekhar and the Limits of Physics, Part 4: Vindication

July 23, 2026

The collapsing stars Eddington swore couldn't exist turned out to be everywhere, and half a century later the world handed Chandrasekhar his Nobel. How the 1.4 solar mass limit became one of the most important numbers in modern astronomy.

Chandrasekhar and the Limits of Physics, Part 3: Exile and Beauty

July 22, 2026

Driven from Europe by the feud, Chandrasekhar rebuilt his life in America and turned mastery-and-move-on into an art form. On his conviction that beautiful physics is true physics, and the two students he drove through blizzards to teach.

Chandrasekhar and the Limits of Physics, Part 2: Humiliation

July 21, 2026

In 1935 the most eminent astronomer alive stood up in a packed room and called Chandrasekhar's discovery "stellar buffoonery." The story of Arthur Eddington's years-long campaign against a result that everyone privately knew was correct.

Chandrasekhar and the Limits of Physics, Part 1: Triumph

July 20, 2026

The story of Subrahmanyan Chandrasekhar, who as a teenager on an ocean voyage worked out that white dwarf stars have a maximum mass of 1.4 Suns. A tour of degeneracy pressure, the relativistic insight everyone else missed, and the number that would define his life.

What's It Like to Travel Near the Speed of Light? Part 4: The Hot View

July 17, 2026

An accelerating observer finds their empty vacuum glowing with real particles, a bizarre effect called Unruh radiation. It's a cousin to Hawking radiation, but with no black hole required, just a rocket and its throttle.

What's It Like to Travel Near the Speed of Light? Part 3: The Limited View

July 17, 2026

Constant acceleration builds a horizon out of nothing but motion, walling off part of the universe forever. Meet Wolfgang Rindler, the coffee date you'll never reach, and the light that can chase you for infinite time without ever catching up.

What's It Like to Travel Near the Speed of Light? Part 2: The Warped View

July 16, 2026

Move fast enough and the entire universe compresses into a searing, blueshifted cone of light aimed at your face. How relativistic aberration and the Doppler effect warp your view of the cosmos as you approach lightspeed.

What's It Like to Travel Near the Speed of Light? Part 1: The Broken View

July 15, 2026

You can't ride alongside a beam of light, and the reason why opens a door onto the strangest parts of relativity. A tour of rest frames, why a photon has no point of view, and how your speed reshapes reality itself.

What Would Happen if the Sun Stopped? Part 4: Black Hole Sun

June 18, 2026

Switch off fusion and, for ten thousand years, nothing happens. Then the Sun begins a slow, strange death: shrinking, briefly brightening, and coasting on gravitational heat for tens of millions of years. And the neutrinos give the whole thing away in just eight minutes.

What Would Happen if the Sun Stopped? Part 3: The Photon Traffic Jam

June 17, 2026

A photon born in the Sun's core takes around 100,000 years to fight its way to the surface, bouncing through a random walk so inefficient that the light on your face is older than human civilization. Why the Sun's surface is a hundred-millennia-delayed broadcast.

What Would Happen if the Sun Stopped? Part 2: Kelvin and Helmholtz at the Ready

June 16, 2026

How can the Sun keep shining with its furnace switched off? Two nineteenth-century aristocrats, Helmholtz and Lord Kelvin, worked out the answer mostly by accident. It comes down to stored heat, gravitational shrinking, and the strange self-regulating thermostat of hydrostatic equilibrium.

What Would Happen if the Sun Stopped? Part 1: The Infernal Reservoir

June 15, 2026

If the Sun's fusion shut off right now, you would not notice for a very long time. The first stop is understanding the Sun itself: a vast pile of gravitating matter where fusion is so absurdly inefficient that, pound for pound, a compost heap beats it.

Why Can't the Universe Be Cyclic? Part 4: When a Good Idea Meets Bad Data

June 09, 2026

The ekpyrotic universe is a beautiful idea that runs headlong into the data. From hand-waved singularities and assumed dark energy to the killer blow from Planck and WMAP measurements of the cosmic microwave background, here is why nature has so far voted against it.

Why Can't the Universe Be Cyclic? Part 3: The Ekpyrotic Universe and Its Bouncing Branes

June 08, 2026

The ekpyrotic theory tries to beat inflation with bouncing higher-dimensional branes, no singularity, and a universe that has always existed. A tour of the prettiest version of the idea and how it claims to handle flatness, dark energy, and the entropy that doomed earlier cyclic models.

Why Can't the Universe Be Cyclic? Part 2: The Awkward Triumph of Inflation

June 07, 2026

Inflation is awkward, possibly not even a proper theory, and it has reigned over cosmology for forty years anyway. Here is what it claims, the flatness, horizon, and monopole problems it solves, the structure-formation prediction it nailed, and the deep problems it still cannot escape.

Why Can't the Universe Be Cyclic? Part 1: The Lure of the Eternal Universe

June 06, 2026

A look at why a cyclic, eternally repeating universe is such an appealing idea, and why the first serious attempt to build one, Richard Tolman's 1930s model of endless big bangs and big crunches, collapsed under the weight of entropy. The Big Bang keeps demanding a beginning.

Is Dust the Best Thing in the Universe? Part 4: We Owe Dust Our Lives

May 22, 2026

No dust, no way to cool a collapsing gas cloud. No way to cool it, no stars. No dust, no first rung on the ladder from grain to pebble to planet. The substance I spent two articles complaining about turns out to be the substance that makes me possible.

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