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Unveiling Io's Thermal Mysteries: Heat Loss Analysis from Jupiter's Volcanic Moon

Discover the fascinating relationship between Io's volcanic activity and its thermal properties through blackbody analysis. By modeling Io's surface as a blackbody, we aim to determine temperature variations on this dynamic moon.

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Unveiling Io's Thermal Mysteries: Heat Loss Analysis from Jupiter's Volcanic Moon

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Presentation Transcript

  1. Heat Loss from Io

  2. What’s an Io? • Io is one of Jupiter’s largest moons • Most volcanically active body in the solar system • Reshapes itself at least every 8 years =>

  3. What’s a Blackbody? • Technically, refers to light in a thermodynamic equilibrium (???) but for us: • Anything governed by the following laws: • Let’s look at a picture…

  4. A Blackbody Curve

  5. WTH does this have to do with Io? • The surface of Io can be modeled as a blackbody! • We can use those laws to figure out how hot this moon 598 392 000 kilometers away is! Our goal for today: determine the temperature of different regions of Io using blackbody laws

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