StarTalk Radio
StarTalk Radio

Cosmic Queries Science in Movies and TV

Stay Tuned for… Science! Neil deGrasse Tyson and comic co-host Eugene Mirman answer more of your questions about science in Star Trek, Star Wars, Sliders, Superman, Contact, Mary Poppins and more.

Topics Discussed

Episode Summary

Executive Summary: This StarTalk Cosmic Queries episode uses movie and TV scenes to explain real physics, including relativity, wormholes, angular momentum, binary/trinary star systems, planetary destruction, kites, and cosmological expansion. Tyson and Merman blend humor with corrections to popular science, emphasizing when fiction is plausible, when it breaks known physics, and how scale changes what is possible.

Main Topics: Relativity and the ending of Contact (Priority: 5/5): A listener asks whether the film’s time-dilation portrayal is backwards. Tyson explains that if the traveler moves through a wormhole or other spacetime shortcut, the observed timing can be consistent with the movie’s alien-assisted setup. Wormholes, time dilation, and science fiction plausibility (Priority: 5/5): The hosts discuss Red Dwarf and Star Trek as examples of how wormholes could create large time gaps if travel is relativistic, while noting that synchronized or near-simultaneous trips would not produce huge delays. Atoms, solar systems, and scale (Priority: 5/5): A question compares atoms to solar systems or the Milky Way to a molecule. Tyson explains that atomic and astronomical systems obey different laws: classical physics for large scales and quantum physics for microscopic ones. Tumbling in space and conservation of momentum (Priority: 4/5): The Gravity-inspired question explores whether a person can change rotation or trajectory by twisting their body. Tyson explains that without external interaction or expelled mass, motion continues unchanged; ejecting mass can alter attitude. Multiple stars and planetary stability (Priority: 4/5): The discussion of triple-star systems explains that planets too close to multiple suns face unstable orbits and chaotic climates, while sufficiently distant planets can treat the stars as a single combined gravitational source. Planetary destruction, oxygen in the atmosphere, and kites (Priority: 4/5): Tyson evaluates how to destroy a planet by exceeding its binding energy, warns that extra atmospheric oxygen increases fire risk, and analyzes how kite height is limited by string weight and wind conditions.

Key Arguments: Relativity can make a journey appear instantaneous on one end and prolonged on the other, but fictional setups may alter which frame experiences the time dilation. A wormhole effectively allows faster-than-light traversal through spacetime, which can produce unusual time-ordering effects, including potential time travel. Solar systems are not atom-sized analogs because atomic behavior is governed by quantum mechanics, not the same classical laws that govern planets and stars. A person in free fall cannot change spin or trajectory by body twisting alone unless they expel mass or interact with another object. Stable planetary orbits in multi-star systems require enough distance for the stars to act like a single gravitational source. Destroying a planet requires delivering more energy than its gravitational binding energy; the result is fragmentation, not necessarily radiation. Adding oxygen to Earth’s atmosphere would not fix climate problems and would make fires much more dangerous. Kites rise until string weight and aerodynamic lift balance; very large kites could reach high altitudes but would require extreme engineering. The universe has no center in the usual sense because expansion occurs everywhere, like points on an inflating balloon surface. Pluto is a dwarf planet because it has not cleared its orbital neighborhood, while Kepler-37b qualifies as a planet under the same definition.

Data Points: Time delay in Red Dwarf wormhole example: 557 years - Listener cites a character waiting this long for the others to catch up through a wormhole. Time window for synchronized wormhole travel: about a minute - Tyson says if travelers go through together or nearly together, the delay would be minimal. Atmospheric oxygen remaining after photosynthesis: not a shortage of oxygen; too much carbon dioxide - Tyson argues Earth does not need oxygen brought in from space. Nebula emission wavelength: 5,007 angstroms - Tyson identifies the green nebular line associated with oxygen in rarefied space conditions. Moon reflectivity: about 5% - Tyson says the Moon is a poor reflector compared with Earth. Earth reflectivity relative to Moon: about 10 times more reflective - Tyson contrasts Earth’s surface/clouds with the Moon’s low albedo. Planetary definition year: 2006 - Tyson refers to the IAU definition that demoted Pluto.

Pivotal Quotes: "The laws of physics that describe what goes on in a solar system are different from the laws of physics that describe what goes on in an atom." — Neil deGrasse Tyson: Explaining why solar systems are not analogous to atoms "You calculate what's called the binding energy of the planet." — Neil deGrasse Tyson: Describing how to determine the energy needed to blow up a planet "It is expanding in every direction, therefore there is no center." — Neil deGrasse Tyson: Answering the question of where the Big Bang occurred

Implications: The episode shows how science fiction can teach real physics when listeners distinguish plausible spacetime effects from cinematic shortcuts. It also reinforces core ideas in cosmology, orbital stability, and planetary science that help evaluate future sci-fi claims.

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