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The Solar System Contents of the Solar System • Sun • Planets – 9 known (now: 8) – Mercury, Venus, Earth, Mars (“Terrestrials”) – Jupiter, Saturn, Uranus, Neptune (“Jovians”) – Pluto (a Kuiper Belt object?) • Natural satellites (moons) – over a hundred • Asteroids and Meteoroids – 6 known that are larger than 300 km across – Largest, Ceres, is about 940 km in diameter • Comets • Rings • Dust Size matters: radii of the Planets The Astronomical Unit • A convenient unit of length for discussing the solar system is the Astronomical Unit (A.U.) • One A.U. is the average distance between the Earth and Sun – About 1.5 108 km or 8 light-minutes • Entire solar system is about 80 A.U. across The Terrestrial Planets • Small, dense and rocky Mercury Mars Venus Earth The Jovian Planets • Large, made out of gas, and low density Saturn Jupiter Uranus Neptune Asteroids, Comets and Meteors Debris in the Solar System Asteroids Asteroid Discovery • First (and largest) Asteroid Ceres discovered New Year’s 1801 by G. Piazzi, fitting exactly into Bode’s law: a=2.8 A.U. • Today more than 100,000 asteroids known • Largest diameter 960 km, smallest: few km • Most of them are named • about 20 of them are visible with binoculars Comets - Traveling Dirty Snowballs • Small icy bodies, “dirty snowballs” • Develops a “tail” as it approaches the Sun Comet Anatomy • Tail may be up to 1 A.U. long Comet Tail • Two kinds of tails: • Dust • Ion (charged particles) Shapes Comet GiacobiniZinner (1959) • Ion tail 500,000 km long • Coma: 70,000 km across Comet Hale-Bopp (1997) • Tail 40° long as seen from earth Halley’s Comet – a typical Comet Meteor Showers Radiant Quadrantids (QUA) Lyrids (LYR) Eta Aquarids Beta Taurids Delta Aquarids Perseids (PER) Draconids Orionids (ORI) Taurids Leonids (LEO) Geminids (GEM) Duration Dec. 28-Jan. 7 Apr. 16-25 Apr. 21-May 12 June 30 July 25-31 Aug. 10-14 Oct. 6-10 Oct. 15-29 Oct.12- Dec 2 Nov. 14-20 Dec. 6-19 Meteors, Meteroids and Meteorites • A Meteor is a sudden strike of light in the night sky • A Meteoroid is a small asteroid, less than 100 m in diameter • A Meteorite is any piece of interplanetary matter that survives the passage through Earth’s atmosphere and lands on Earth’s surface Meteors and Meteorites • Small particles that strike the atmosphere • Come from fragments of asteroids, Moon, Mars, comets • Strike the earth all the time (“meteorites”) – High speed means lots of energy released on impact Impact Craters • Barringer Crater, AZ 0.8 mi diameter, 200 yd deep; produced by impact about 25,000 years ago • Quebec's Manicouagan Reservoir. Large meteorite landed about 200 million years ago. The lake, 45 miles in diameter, now fills the ring. Tunguska • ~30 m body struck Siberia in 1908 • Energy equal to that of a 10 Megaton bomb! • Detonation above ground; several craters Frequency of Impact Events Formation of the Solar System • Features to explain: – – – – – – – – – planets are far apart, not bunched together orbits of planets are nearly circular orbits of planets lie mostly in a single plane directions of revolution of planets about Sun is the same, and is the same as the direction of the Sun's rotation directions of rotation of planets about their axes is also mostly in the same direction as the Sun's (exceptions: Venus, Uranus, Pluto) most moons revolve around their planets in the same direction as the rotation of the planets differentiation between inner (terrestrial) and outer (Jovian) planets existence and properties of the asteroids existence and properties of the comets Formation of the Solar System • Condenses from a rotating cloud of gas and dust – Conservation of angular momentum flattens it • Dust helps cool the nebula and acts as seeds for the clumping of matter Formation of Planets • Orbiting dust – planitesimals • Planitesimals collide • Different elements form in different regions due to temperature • Asteroids • Remaining gas Structure of the Planets explained Temperature and density of materials drop with distance to sun