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Cosmic Queries – Space Volcanoes: Fire and Ice with Natalie Starkey

What’s a supervolcano? Neil deGrasse Tyson and comic co-host Matt Kirshen discover all types of volcanoes in the solar system with cosmochemist and author of Fire and Ice: The Volcanoes of the Solar System, Natalie Starkey. Is there such a thing as an ice volcano? Originally Aired October 5, 2021.

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Episode Summary

Executive Summary: Neil deGrasse Tyson and Matt Kirshen interview geologist-turned-science communicator Natalie Starkey about her book Fire and Ice, exploring volcanism across the solar system. They compare Earth volcanoes with cryovolcanoes on icy moons, explain magma/lava, tidal heating, Venus’s hidden activity, Mars’s giant Olympus Mons, and how volcanism links to planetary cooling, magnetic fields, and astrobiology.

Main Topics: Volcanoes beyond Earth (Priority: 5/5): The conversation broadens the definition of a volcano from Earth’s cone-shaped mountains to material erupting from interiors on many worlds, including icy moons and dwarf planets. Cryovolcanism and icy moons (Priority: 5/5): Starkey explains that many outer-solar-system bodies have ‘ice volcanoes’ driven by internal heat, especially Enceladus and Europa-like worlds, where plumes can sample subsurface oceans. Venus, Mars, and planetary activity (Priority: 4/5): The hosts discuss active or recently active volcanism on Venus and Mars, including Venus’s hidden lava-covered surface and Mars’s enormous Olympus Mons formed without plate tectonics. How eruptions work (Priority: 4/5): Starkey details magma rising due to buoyancy and gas pressure, plus tidal heating on bodies like Enceladus that creates cracks and plumes rather than Earth-like cones. Volcanoes, cooling, and magnetic fields (Priority: 4/5): Volcanism is framed as part of planetary cooling; Earth’s internal heat and radioactive decay sustain the mantle, while a molten core powers the magnetic field that protects the atmosphere. Hazards and benefits of volcanism (Priority: 3/5): The episode covers supervolcano risks, volcanic ash as fertile soil, and why people live near volcanoes despite danger, emphasizing both devastation and agricultural advantages. Astrobiology and mission science (Priority: 4/5): Plumes from icy worlds are presented as promising targets for future missions because they may contain salts, silica, and organic molecules that could hint at life.

Key Arguments: Volcanoes are not limited to conical mountains on Earth; any process that expels material from an interior onto a surface can count as volcanic activity. Many outer-solar-system bodies are more volcanically active than Earth in terms of cryovolcanic plumes, because tidal heating keeps their interiors warm. Enceladus’s plumes are likely sourced from a salty subsurface ocean, making them scientifically valuable for searching for organic chemistry and possible life. Venus is likely still volcanically active, but its dense CO2 atmosphere hides surface changes; radar observations reveal widespread lava flows. Mars hosts Olympus Mons because low gravity and the lack of plate tectonics let a mantle plume erupt through the same spot for a very long time. Earth’s volcanoes are part of the planet’s cooling process, while radioactive decay still provides roughly half of Earth’s internal heat. The molten outer core is essential for Earth’s magnetic field, which protects the atmosphere and living organisms from solar wind and radiation. Supervolcanoes are dangerous, but scientists would likely see warning signs before a catastrophic eruption, making apocalyptic media narratives overstated.

Data Points: Venus surface temperature: 450°C - Natalie Starkey notes Venus is hot enough to melt lead and is inhospitable to humans. Venus surface age: ~500 million years old - Used to illustrate that Venus’s surface is relatively young in solar-system terms and likely resurfaced by volcanism. Mars major active volcanism: ~3 billion years ago - Tyson and Starkey reference Mars as being volcanically active in the ancient past. Jupiter moons: about 79 - Starkey cites the large number of moons around Jupiter when discussing icy volcanic worlds. Volcanic inactivity threshold: 10,000 years - She mentions this as a rough rule of thumb for deciding whether a volcano is still active. Earth’s heat from radioactive decay: about half - Starkey explains that roughly half of Earth’s current internal heat is produced by radioactive decay. Enceladus plume height: 200 kilometers - Used to show that icy-world eruptions can send material very high into space. Iceland electricity use per capita: highest in the world - Mentioned in the discussion of geothermal energy and Iceland’s reliance on volcanic heat. Olympus Mons height comparison: about 3x Mount Everest - Starkey notes Olympus Mons is vastly taller than Everest due to Mars’s low gravity and stagnant lid tectonics.

Pivotal Quotes: "most of the volcanoes out in the solar system, particularly when we go past the asteroid belt out to Jupiter and beyond, most of the bodies out there are actually ice volcanoes." — Natalie Starkey: Starkey explains the title Fire and Ice and the prevalence of cryovolcanism in the outer solar system. "volcanoes are basically just a manifestation of a planet cooling itself down." — Natalie Starkey: She answers whether Earth’s volcanism affects long-term cooling and internal evolution. "if we just got a normal mountain ... those mountains and you know, Mount Everest are not volcanic, they never will be." — Natalie Starkey: She clarifies that mountains formed by plate collision do not become volcanoes later.

Implications: Listeners gain a broader, science-based view of volcanism as a planetary process, not just an Earth hazard. The episode highlights icy moons as prime astrobiology targets and shows why upcoming Venus, Mars, and outer-solar-system missions matter.

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