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Radar Astronomy — Mapping Asteroids and Venus With Pings

Most astronomy is passive — we collect what stars and planets emit. Radar astronomy is different: we shout at the solar system and listen for the echo. The science it has produced is irreplaceable.

Radar Astronomy — Mapping Asteroids and Venus With Pings
tech · science

Venus through the clouds

Venus is wrapped in sulphuric acid clouds opaque to every visible-light telescope. In the 1960s and 70s, Arecibo and Goldstone pinged it with S-band radar and mapped its surface for the first time. Magellan finished the job from orbit in 1990, but radar got there first.

Asteroid radar imaging

When a near-Earth asteroid passes within a few million km, Goldstone or (until 2020) Arecibo could resolve it down to metres. Shape, spin rate, surface roughness, moons — all recovered from delay-Doppler images. Hundreds of asteroids have been characterised this way.

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Planetary defence

Radar imaging is how we know whether an incoming asteroid is solid rock, rubble pile, or contact binary. Defenders need that data to decide between a kinetic impactor (DART), a nuclear option, or a gravity tractor. Radar provides it years in advance.

After Arecibo

Arecibo's collapse in December 2020 cut radar astronomy roughly in half. The Goldstone Solar System Radar continues. Plans for a new dedicated radar at Green Bank (the ngRADAR concept) would partially replace Arecibo's capability.

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