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From the High Desert

A Cultural History of Art Bell

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September 16, 2006: Space Solar Energy & Launch Systems - John C. Mankins

Sep 16, 2006
2h 38m
0:00 / 0:00
Art Bell speaks with John C. Mankins, a 25-year NASA veteran who spent a decade at JPL and 15 years at headquarters overseeing advanced technology programs. Mankins explains how breakthroughs in lightweight thin-film reflectors now make solar power viable even in the outer solar system, challenging NASA's long reliance on plutonium-powered systems for deep space missions.

The conversation expands to space solar power, the concept of collecting energy in orbit where sunlight is constant, then beaming it to Earth via microwave or laser. Mankins describes fail-safe phased arrays that prevent the beam from targeting anything without a ground-based pilot signal. He estimates the technology could become cost-competitive within 10 to 20 years, potentially delivering hundreds of gigawatts to multiple locations from a single satellite.

Art and Mankins discuss the risks of nuclear materials in space, launch economics, and the stalled civilian space program. Mankins advocates for international cooperation modeled on commercial ventures rather than government projects. The program opens with Art sharing observations from a recent Hong Kong trip, a Pravda report about Russian journalists allegedly cooking an egg between two cell phones, and updates on the Lake Superior F-89 Scorpion mystery.

Key Moments

  1. What space solar power actually is: Mankins lays out the core concept: ground solar suffers day/night, weather and seasons, but in space the sun shines almost constantly, so you collect energy in orbit, convert it to a beam, and send it down to Earth.

  2. Retro-directive phased array fail-safe: Mankins explains the Sunstroke disaster cannot happen: a retro-directive phased array, invented by Nobuyuki Kaya, requires a pilot signal from the ground rectenna. Without it, millions of RF transmitters cannot focus and the energy smears harmlessly across space.

  3. Beam intensity is one tenth of midday sunlight: Mankins quantifies the safety case: peak ground sunlight is about 1 kW per square meter, and a power beam would be about 10% of that, only in its center. A square kilometer rectenna at full sun delivers a gigawatt.

  4. Maglev catapult as a virtual first stage: Mankins explains rockets burn ten times more fuel for the first 1,000 fps than the last, so a maglev catapult giving even a small initial push acts as a virtual electric first stage with disproportionate effects on launch economics.

  5. StarTram - magnetically levitated launch tube to space: Mankins describes Jim Powell's StarTram concept: accelerate to orbital velocity on the ground, then coast up through an evacuated tube held aloft by a ground-based electromagnetic field. When the vehicle exits the tube, it is already in space, no rocket required.