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Overview of the Solar System

Delve into the fascinating realm of our solar system, from the blazing Sun to the distant icy worlds. Learn about the composition, characteristics, and unique traits of the major planets, asteroids, comets, and interplanetary dust. Discover how everything, from the gravitational dance of the planets to the icy cometary nuclei, plays a role in shaping the cosmic landscape. Unravel the mysteries of accretion and witness the fossilized memories that tell the story of our celestial neighborhood.

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Overview of the Solar System

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  1. Overview of the Solar System • Solar system contents – one star, several planets, lots of debris.

  2. Most of it is the Sun! • 99.8% of the mass of the Solar System resides in the Sun. • A hot ball of mostly hydrogen and helium held together by gravity. • In bulk composition it resembles an unbiased scoop of galactic material.

  3. Most of it is the Sun! • 99.8% of the mass of the Solar System resides in the Sun. • A hot ball of mostly hydrogen and helium gas held together by gravity. • In bulk composition it resembles an unbiased scoop of galactic material. 3/4 Hydrogen 1/4 Helium 1% other elements

  4. Eight Major Planets • Maybe one or two more depending on semantics and future discoveries.

  5. Four Jovian Worlds • Jupiter, Saturn, Uranus and Neptune • “Gasballs” constituting 99.9% of the planetary mass

  6. Four Jovian Worlds • Jupiter, Saturn, Uranus and Neptune • Hydrogen and helium, under high pressure, become dense liquids – more appropriately these are spinning liquid droplets.

  7. Four Terrestrial Worlds • Mercury, Venus, Earth, and Mars • Small rocky/metallic worlds hugging the Sun with thin or non-existent atmospheres.

  8. Jovian vs. Terrestrial Characteristics • Terrestrial: Mercury, Venus, Earth, and Mars • Small relatively speaking • Solid rocky cratered surfaces with significant iron cores • Three satellites between them all

  9. Jovian vs. Terrestrial Characteristics • Jovian: Jupiter, Saturn, Uranus, Neptune – The “Gas Giants” • about 10 times bigger than the terrestrial worlds • Gaseous with no solid surface, resembling the Sun in composition (mainly Hydrogen and Helium) . • Clouds of Methane, Water, Ammonia, and other molecules provide an apparent “surface” • More than one hundred satellites – most made mainly of water/ice.

  10. Jovian vs. Terrestrial Characteristics • Jovian: Interiors of compressed liquified gas

  11. Jovian vs. Terrestrial Characteristics • Jovian: Cloudtop “surfaces”

  12. Jovian vs. Terrestrial Characteristics • Jovian: Many satellites

  13. Jovian vs. Terrestrial Characteristics • Jovian: Icy satellites

  14. Jovian vs. Terrestrial Characteristics • Jovian: Satellites as big as planets, some with atmospheres.

  15. Minor Constituents: Asteroids, Comets, and Dust • Asteroids: Millions of small rocky objects mostly between the orbits of Mars and Jupiter

  16. Minor Constituents: Asteroids, Comets, and Dust • Asteroids: Millions of small rocky objects mostly between the orbits of Mars and Jupiter http://www.daviddarling.info/encyclopedia/A/asteroid.html

  17. Minor Constituents: Asteroids, Comets, and Dust • Asteroids: Millions of small rocky objects mostly between the orbits of Mars and Jupiter

  18. An Outer Icy Asteroid Belt • Another group of asteroid-sized bodies orbit beyond Neptune in the “Kuiper Belt” • Pluto is one of the largest of these.

  19. A Cloud of Cometary Nuclei • Trillions of small iceballs, most only a kilometer in size, orbit as far out as ½ way to the nearest star. • only a small fraction make it into the inner solar system to be heated by the Sun to become a comet.

  20. A Cloud of Cometary Nuclei • Trillions of small iceballs, most only a kilometer in size, orbit as far out as ½ way to the nearest star. • only a small fraction make it into the inner solar system to be heated by the Sun to become a comet.

  21. Interplanetary Dust • The grinding of asteroids and evaporation of comets populates the inner solar system with fine dust. http://www.astrophoto.com/images.htm

  22. Interplanetary Dust • The grinding of asteroids and evaporation of comets populates the inner solar system with fine dust.

  23. Interplanetary Dust • The grinding of asteroids and evaporation of comets populates the inner solar system with fine dust.

  24. Regular Features of the Solar System See orbits • All of the planets orbit the Sun in the same plane • All planetary orbits are nearly circular • All planets orbit the Sun in the same “direction” • Most planets rotate in the same sense as the orbit.

  25. Regular Features of the Solar System • The Jovian and Terrestrial planets are well sorted in terms of distance from the Sun. • rocky worlds close – gaseous/icy worlds far away

  26. Regular Features of the Solar System See orbits • All of the planets orbit the Sun in the same plane • All planetary orbits are nearly circular • All planets orbit the Sun in the same “direction” • Most planets rotate in the same sense as the orbit.

  27. Regular Features of the Solar System • The Giant Planet satellite systems resemble the Solar System

  28. Regular Features of the Solar System • Exposed solid surfaces are heavily cratered throughout the Solar System. • The process was messy and produced lots of leftovers.

  29. Regular Features of the Solar System • Exposed solid surfaces are heavily cratered throughout the Solar System. • The process was messy and produced lots of leftovers.

  30. Building a Solar System through “Accretion” • These regular features are “fossilized” memory of the conditions that gave rise to the Solar System. • In sum, they suggest the planets grew within a rotating flattened disk and, today, their orbits reflect the structure of that disk.

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