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Interiors of Worlds and Heat loss. Differentiation -materials separate into layers. How do we learn about planetary interiors?. Measure moment of inertia & average density Observe seismic events Study planetary magnetic fields.
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How do we learn about planetary interiors? • Measure moment of inertia & average density • Observe seismic events • Study planetary magnetic fields
waves travel in straight lines unless diverted by the material they travel through. • refract due to density changes. • refract due to composition changes • reflect dues to boundary changes
Interiors and Magnetic Fields We can deduce that any world with a global magnetic field has 2 things: • It has an electrically conducting material within it. • The material is a moving, circulating liquid. (movement usually caused by the rapid rotation of a planet)
Interiors and Magnetic Fields Terrestrial Worlds like Earth have a 3rd • It has an electrically conducting material within it. • The material is a moving, circulating liquid. • It has two internal layers composed of a solid layer inside a liquid one.
Main Worlds with Active Magnetic Fields Strength Order: Sun, Gas giants, Earth, Mercury, Mars (remnant)
Interior of Gas Giant Worlds The magnetic fields of gas giants indicate that there are large amounts of circulating, electrically-conducting materials. Metallic hydrogen or water
Planets gain their initial internal heat energy by 3 main methods:- Kinetic Gravitational Radioactivity
Planet spend the rest of their lives losing internal energy to space
3 Types of Heat loss • Conduction -atoms vibrate strongly causing atoms next them to pick up energy • Convection- heat causes fluids to move, the hot fluid rises, the cold fluid sinks. • Radiation- photons of electromagnetic light carry energy away from the object
Which Forms of Heat Loss Work Where? • All worlds conduct inside. • All worlds radiate out to space (the only heat transfer that works in a vacuum!). • Larger worlds convect inside. • Largest worlds radiate inside.
Dominant Form of Internal Heat Loss Conduction -all small bodies: asteroids, comets, small only moons, Mercury, Moon, modern Mars Convection cells break the crust causing the surface to move with the convection -Earth Solid Convection cells heat the crust causing melting and volcanism Convection- Venus, early-middle Mars,earliest Moon and Mercury Gas-Sun(outer layers), gas giant planets all wavelengths -internal layer deep in theSun Radiation weakly at IR and longer for other worlds
Radiation inside Worlds • The hotter the world, the stronger the black-body curve and the more and shorter-wavelength radiation it emits. • Sun: hottest, visible light • Gas giants : IR • Rocky: some reflected radiation (not a black-body), some IR, some microwave and radio.
Radiation inside Worlds • The Sun has an internal zone where electro-magnetic radiation is emitted.