'Roche limit' diaporamas de présentation

EART160 Planetary Sciences

EART160 Planetary Sciences. Francis Nimmo. Last Week. Giant planets primarily composed of H,He with a ~10 M e rock-ice core which accreted first They radiate more energy than they receive due to gravitational contraction (except Uranus!)

482 views • 38 slides

EART160 Planetary Sciences

EART160 Planetary Sciences. Francis Nimmo. Last Week. Giant planets primarily composed of H,He with a ~10 M e rock-ice core which accreted first They radiate more energy than they receive due to gravitational contraction (except Uranus!)

384 views • 38 slides

12b. Saturn

654 views • 34 slides

465 views • 32 slides

Greenhouse Effect

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357 views • 28 slides

Rotation period as fast as Jupiter, as well as differential rotation rates at poles and equator

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Astronomy Picture of the Day

Astronomy Picture of the Day. Question. Jovian planets are composed of fluids, which means: A) They are composed of a liquid interior layer and a gaseous outer layer. B) They have no rocky surface of any kind. C) They can exhibit convection. D) All of the above. Question.

305 views • 22 slides

Roche limit

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ASTR 2310: Chapter 4

ASTR 2310: Chapter 4. Earth-Moon System Precession Tides Limits on Sizes of Orbits Phases of the Moon Rotation of the Moon Eclipses. ASTR 2310: Chapter 4. Precession We talked about this already (equinoxes, Polaris...) ? Now a bit more on why...

296 views • 13 slides

rings

All Jovian planets have rings

655 views • 5 slides