intro to the solar system. scaling often one is interested in how quantities change when an object...
TRANSCRIPT
Intro to the Solar System
Scaling
• Often one is interested in how quantities change when an object or a system is enlarged or shortened
• Different quantities will change by different factors!
• Typical example: how does the circumference, surface, volume of a sphere change when its radius changes?
How does it scale?
• Properties of objects scale like the perimeter, the area or the volume– Mass scales like the volume (“more of the same
stuff”)– A roof will collect rain water proportional to its
surface area
Example: Newton’s Law of Gravity
Note that in order to compute a "factor of change" you can ask: by what factor do I have to multiply the original quantity in order to get the desired quantity? Example: Q: By what factor does the circumference of a circle change, if its diameter is halved? A: It changes by a factor 1/2 = 0.5, i.e. (new circumference) = 0.5 * (original circumference), regardless of the value of the original circumference.
•If the mass of the Sun was bigger by a factor 2.7, by what factor would the force of gravity change? scales linear with mass same factor
• If the mass of the Earth was bigger by a factor 2.2, by what factor would the force of gravity change? scales linear with mass same factor
•If the distance between the Earth and the Sun was bigger by a factor 1.2, by what factor would the force of gravity change? falls off like the area factor 1/ f 2 = 1/1.44 = 0.694
From Phrase to Equation
• Important skill: translate a relation into an equation, and vice versa
• Most people have problems with this arithmetical reasoning
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
Sun: Jupiter: Earth: Moon =110:11:1:1/4
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
Venus
Earth
Mars
The Jovian Planets
• Large, made out of gas, and low density
Jupiter
Uranus
Saturn
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 Giacobini-Zinner (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 – caused by comets
Radiant DurationQuadrantids (QUA) Dec. 28-Jan. 7Lyrids (LYR) Apr. 16-25Eta Aquarids Apr. 21-May 12Beta Taurids June 30Delta Aquarids July 25-31Perseids (PER) Aug. 10-14Draconids Oct. 6-10Orionids (ORI) Oct. 15-29Taurids Oct.12- Dec 2Leonids (LEO) Nov. 14-20Geminids (GEM)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
Meteorites – the Remains of Meteors
Impact Craters
• Quebec's Manicouagan Reservoir. Large meteorite landed about 200 million years ago. The lake, 45 miles in diameter, now fills the ring.
• Barringer Crater, AZ 0.8 mi diameter, 200 yd deep; produced by impact about 25,000 years ago
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
Cleaning up the Solar System
• Small objects are forced out of the inner Solar System by gravitational pull of bigger planets
• Small planetesimals collide and form planets
-- or are thrown out!