Things You Thought You Knew – Is Everything Light?
Neil deGrasse Tyson hosts this episode of StarTalk exploring three fundamental concepts that shape our understanding of light, space, and observation. The discussion covers albedo (reflectivity measurements), light pollution affecting astronomical observations, and the electromagnetic spectrum.
- 01
The Moon has an albedo of only 0.1, making it nearly as dark as car tire sidewalls - its brightness comes from the Sun's intensity
- 02
Earth appears 50 times brighter from the Moon than the Moon appears from Earth due to size and reflectivity differences
- 03
Leonardo da Vinci first explained earthshine in his Codex Leicester, illustrating how sunlight reflects from Earth to Moon and back
- 04
Light pollution costs money - streetlights visible from airplanes mean you're paying to illuminate the sky unnecessarily
- 05
Radio telescopes face pollution from TV, satellites, and even car key fobs disrupting observations of distant galaxies
- 06
The Vera Rubin Telescope takes movies of the night sky to distinguish between satellites and potentially dangerous asteroids
- 07
Humans can only see a tiny slice of the electromagnetic spectrum - we are 'practically blind' to most light forms
- 08
William Herschel discovered infrared light by measuring temperatures in Newton's spectrum, finding the hottest spot beyond visible red
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