H₂OCO₂CH₄O₂Na

— atmospheric absorption spectrum

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The science of
other worlds.

Essays on exoplanet detection, atmospheric chemistry, orbital mechanics, and the search for life. Written for curious minds, not simplified for casual readers.

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01

The Transit Method

How a shadow reveals a world

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When a planet passes in front of its star, it dims the starlight by a tiny but measurable fraction. This essay explores the mathematics behind transit photometry and how Kepler and TESS turned it into the most prolific planet-finding technique in history.

02

Radial Velocity

The wobble that changed astronomy

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Long before we could see exoplanet shadows, astronomers noticed stars moving. Not through space — but toward and away from us, in tiny rhythmic pulses. This is the story of the Doppler technique and the discovery of 51 Pegasi b.

03

The Habitable Zone

Where liquid water might survive

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Not too hot, not too cold. The habitable zone is the orbital band around a star where surface liquid water is theoretically possible. But the concept is more nuanced — and more contested — than it first appears.

04

Atmospheric Spectroscopy

Reading the chemistry of alien skies

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When starlight filters through a planet's atmosphere during transit, different molecules absorb different wavelengths. The result is a fingerprint. JWST is now reading those fingerprints on worlds dozens of light-years away.

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