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Astro 201: Sept. 6, 2010 • Do on-line practice quiz #2 by 9/14 • Homework #2: posted on web page, due 9/9 • Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6 Today: – Astronomical basis for calendars – Why there are seasons – Tycho, Kepler, Newton – Forces; String Theory – Determinism v. Chaos; Fractals
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Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

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Page 1: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Astro 201: Sept. 6, 2010• Do on-line practice quiz #2 by 9/14• Homework #2: posted on web page, due 9/9• Reading: Hester, Chapters 2-3

Gleiser: Sections 3-6• Today: – Astronomical basis for calendars– Why there are seasons– Tycho, Kepler, Newton– Forces; String Theory– Determinism v. Chaos; Fractals

Page 2: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

The Astronomical Basis for Calendars

The Earth rotates on its axis once a day.The Earth orbits the Sun with a period of about 365.242190 daysThe Moon orbits the Earth, such that the period between new moon and new moon is 29.5305 days

These periods vary a little bit because of the gravitational forces exerted by the other planets and other factors.

Every 4 years, we take into account the .242190 days by added a leap day, February 29.

Otherwise we would keep slipping, and eventually January would be summer in the northern hemisphere, etc.

Now, the thing is that there are NOT an integral number of months (29.5305 days) in one 365.242190 year.

So if for example today is a new moon, next year it will not be.

Page 3: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

SEASONS: Seasons are a result of the tilt of the Earth’s axis with respect to the plane of its orbit. Seasons ARE NOT the result of the Earth being closer to the Sun in summer,and farther in winter – in fact during winter in the northern hemisphere, we are closer to the Sun than we are in the summer.

Page 4: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 5: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 6: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 7: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 8: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 9: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 10: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

The Gregorian Calendar (Christian, one we use)

is based on the motion of the Earth around the Sun.

The length and number of months have no connection to the motion of the Moon

It is based on the Julian Calendar, which was introduced by Julius Caesar in 45 BC.

He made Jan. 1 the start of the Year.

During the middle ages, different groups in Europe adopted different start dates for the new years.

In 1582, Pope Gregory reformed the calendar, which is basically what we use today.

The French recognized a different pope for a while and had a different calendar.

Page 11: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

The Islamic Calendar

is based on the motion of the Moon, with no connection to the motion of the Earth around the Sun.

Hijri Calendar, Based on the Qur'an.

Used in many countries around the Gulf, e.g. Saudi Arabia.

Purely lunar: 12 months, each with 29.53 days.

Therefore the Islamic year has 12x29.53 = 354.36 days

The Islamic year is shorter than the time it takes the Earth to go around the Sun.

Thus, a particular Islamic month falls during different times of the year , e.g. Ramadan.

Years are counted since the Hijra, which is is the time that Mohammed emigrated to Medina in AD 622.

So AD 2009 is Islamic year 1430.

Page 12: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

The Jewish and Chinese Calendars

combine both, so years are linked to the period of the orbit of the Earth around the Sun, AND months are linked to the motion of the Moon around the Earth.

19 x365.24 = an integral number of 29.53 day months.

Jewish Year: A "ordinary" year has 355 days, and 12 months. A "leap" year has 385 days and 13 months.

The length of a particular month varies from year to year by a day, so that if New Year's Day (Rosh HaShannah) is, say, a new moon, then the first day of every month is a new moon.

Years are counted since the creation of the world, taken to be 3761 BC. Thus 1998 is Jewish year 5759.

Page 13: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Mayan Calendar

The ancient Mayans developed a complex and accurate calendar, which wasadopted by other people in meso-america – Aztecs, Tolmec .

Actually had THREE calendars, which they used at the same time:

1.The Haab Civilian calendar

18 months, 20 days each + 5 days to make 365 day years The 5 extra days were considered unlucky, days of mourning Did not count YEARS in the Haab calendar however

2.The Tzolkin Devine calendar, used for divinations

two types of weeks, one with 13 days, the other with 20 days

Each year was 260 days Years were not counted

Page 14: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Mayan Calendars, continued:

3.The Long CountInstead of years, the Mayan used the Long Count calendar system to

keep track of historical events

kin = 1 dayuinal(1 uinal = 20 kin = 20 days)Tun (1 tun = 18 uinal = 360 days = approx. 1 year)katun (1 katun = 20 tun = 7,200 days = approx. 20 years)baktun (1 baktun = 20 katun = 144,000 days = approx. 394 years) pictun = 20 baktun = 2,880,000 days = approx. 7885 yearscalabtun = 20 pictun = 57,600,000 days = approx. 158,000 yearskinchiltun = 20 calabtun = 1,152,000,000 days = approx. 3 million yearsalautun = 20 kinchiltun = 23,040,000,000 days = approx. 63 million years

The Mayan calendar started on our August 11, 3114 BC. With Date: 0.0.0.0.0.

Then date 13.0.0.0.0 is our December 21, 2012, or 12/21/2012.

Page 15: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

This coincidence has caused some people to claim that the Mayan Calendar predicts the end of the world on December 21, 2012.

But the Long Count calendar doesn’t end on 13.0.0.0.

Page 16: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 17: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Tycho Brahe (1546-1601) Danish noblemanGot drunk as a college student, lost his nose in a duel

Built an observatory, Uraniborg,financed by King Frederic II

Made extremely accurate Observations of the planets

Page 18: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Astronomiæ Instauratæ Mechanica: Tycho’s book about his instrumentation

Page 19: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 20: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Tycho made observations of the positions of the stars and planets that were 15x more accurate than what others had made

He “beat down the errors” by repeating a particular measurement many times and averaging the result

Page 21: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Tycho’s cosmology

Tycho found no parallax for the stars and concluded they are very far awayHe made measurements which neither the Ptolemaic model, nor the simple Copernicus model could explain.

Earth stationary in centerSun and moon orbit the EarthOther planets orbit the SunStars orbit the Earth

Page 22: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Johannes Kepler (1564-1630)

Worked as Tycho’s assistantTook Tycho’s observations when Tycho died and spent the next 29 years analyzing them

First, he wrote “Mysterium Cosmographicum”The orbits of the 6 known planets were described By 5 “Pythagorian” polyhedra in spheres:

Page 23: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 24: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Eventually abandoned this model and came up with

Kepler’s Three Laws of Planetary Motion

1. Planets move in elliptical orbits (not circles), with the Sun at one focus.

Page 25: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

2. An imaginary line connecting the Sun to any planet sweeps out equal areas in equal time..

Area 2

Area 1

Planets move faster when near Sun

Page 26: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 27: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

3. The square of a planet’s orbital period is proportional to the cube of its semi-major axis.

P2 (years) = A3 (astronomical units)

1 Astronomical Unit = The Earth-Sun Distance

The farther out a planet is in the solar system, the longer it takes for it to go around the Sun.

Page 28: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 29: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Kepler’s Laws are empirical descriptions of the data.

The don’t explain WHYthe planets move as they do.

Page 30: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Isaac Newton (1642-1727)

Bubonic Plague 1665:

While home for 2 years with nothing to do he figured out

Laws of motion

Gravity

Page 31: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

“Philosophiae Naturalis Principia Mathematica”The laws explained not only why planets move as they do, but why objects in general move as they do.

Newton's First Law of Motion:Every object in a state of uniform motion tends to remain in that state of motion unless an external force is applied to it.

speed: how many miles per hour velocity: speed and direction of motion acceleration: change in velocity, i.e. change in speed and/or change in direction of motion An object at rest stays at rest; an object in motion at a constant velocity stays moving at that velocity unless a force is exerted on it.

Objects with mass have INERTIA.

Page 32: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Newton's Second Law of Motion:

F = m a a = acceleration, change of velocity with time m = mass F = force

Newton's third Law of Motion:

For every action there is an equal and opposite reaction.

Page 33: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Law of Gravitation: Fg = Force of Gravity

Page 34: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

From kepler.nasa.gov

Page 35: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Forces of Nature:

Gravity: very weak, but very long range. always attractive. always acts between any two masses

Electro-Magnetism: Electric & Magnetic fields; light Result of charged particles, or magnets Long range

Weak responsible for radioactive decay,

e.g. beta decay -- n --> p + e + anti-neutrino the interaction of neutrinos

Strong extremely strong on very short distance scales: only really important on scales of 10-13 cm holds neutrons and protons in the nuclei of atoms together

Page 36: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

James Maxwell (1831-1879)

“Unified” Electricity and Magnetism Electro-magnetic field, light

Maxwell’s equations:

Page 37: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Glashow, Weinberg and Salaam got the Nobel Prize in Physics in 1979

for "unifying” Weak & EM forces and coming up with one theory

which describes the "Electroweak Force"

Grand Unified Theories: attempt to unify Electroweak and Strong forces

Theory of Everything: one theory to describe all 4 forces Plus quantum mechanics

Page 38: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

STRING THEORY

everything is ultimately made of strings(sub-sub-sub atomic particles)

How big are strings?

Smaller than a Planck length,

which is about 10-33 centimeters

or about a millionth of a billionth of a billionth of a billionth of a centimeter.

Page 39: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Strings vibrate

Closed string

Open string

Page 40: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

In many string theories the Universe is 10 dimensional,

with the "extra" dimensions COMPACTIFIED.

All HS math geeks read a book called FLATLAND: A Romance of Many Dimensions,by Edwin A. Abbott (1884)

FLATLAND: a "first person" account of life of a 2-dimensional society

a radical named Arthur Square figures out that space is really 3 dimensional.

Page 41: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 42: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

So what the string theorists say is that in ordinary life we think we live in 3 dimensions, and

we have to think of ways to detect the other 7.

The extra-dimensions in string theory are Calabi-Yau figures:

Page 43: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 44: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 45: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Knitted Calabi-Yau Figures

Page 46: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.
Page 47: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

• Kepler: Empirical description of the motion of the planets

• Newton: Law of Gravity. • Developed Calculus, derived orbits of the planets• Solved the “Two-body” problem: Sun + one planet• Couldn’t solve the “Three-body” problem

Mechanical Universe: In Newtonian physics, objects move in perfectly determined ways

Page 48: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

OrreryMechanical models of planetary motions in the solar system

But is the real solar system accuratelydescribed by an orrery?

Page 49: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

"We may regard the present state of the universe as the effect of its past and the cause of its future. An intellect which at any given moment knew all of the forces that animate nature and the mutual positions of the beings that compose it, if this intellect were vast enough to submit the data to analysis, could condense into a single formula the movement of the greatest bodies of the universe and that of the lightest atom; for such an intellect nothing could be uncertain and the future just like the past would be present before its eyes."

— Marquis Pierre Simon de Laplace (1749-1827)

Page 50: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

The Equations

Many thanksTo Scott Tremaine’sNotes fromApril 2006

Page 51: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

• King Oscar II of Sweden (1829- 1907)- Prize: How stable is the

universe?

• Jules Henri Poincaré (1854-1912)– Sun (large) plus one planet (circular

orbit)• Stable

– Added 3rd body • Strange behavior

– Not periodic

Page 52: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

• Modern approach:Solve many-body problem with computer

calculations– Take a distribution of mass– Figure out the gravitational force on each part– F=ma gives you the acceleration on each part– Compute velocity of each part– Move the parts a little– Repeat

Page 53: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Kuiper belt objectsPlutinos (3:2)Centaurscomets

as of March 8 2006 (Minor Planet Center)

Page 54: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Sensitivity to Initial Conditions"A very small cause which escapes our notice determines a

considerable effect that we cannot fail to see, and then we say that the effect is due to chance. If we knew exactly the laws of nature and the situation of the universe at the initial moment, we could predict exactly the situation of the same universe at a succeeding moment. But even if it were the case that the natural laws had no longer any secret for us, we could still know the situation approximately. If that enabled us to predict the succeeding situation with the same approximation, that is all we require, and we should say that the phenomenon had been predicted, that it is governed by the laws. But is not always so; it may happen that small differences in the initial conditions produce very great ones in the final phenomena. A small error in the former will produce an enormous error in the latter. Prediction becomes impossible...". (Poincaré)

Page 55: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Can we predict the motion of a single planet

a billion years from now?

• Laplace and Newton – Yes• Poincare’ – No

• Lorenz – 1963 – “Butterfly Effect” If a butterfly flaps its wings in Brazil, does it result in a tornado in Kansas?

Page 56: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Two kinds of dynamical systems

Regular • highly predictable, “well-

behaved”• e.g. baseball, golf, simple

pendulum, all problems in mechanics textbooks, planetary orbits on short timescales

Chaotic• difficult to predict, “erratic”• appears regular on timescales

short compared to Liapunov time

• e.g. roulette, dice, pinball, weather, billiards, double pendulum

• The Solar System

Page 57: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Double Pendulum: a chaotic system

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Consequences of chaos

• Positions of planets are not predictable on timescales longer than 100 Myr

• the solar system is a poor example of a deterministic universe• The solar system is “Chaotic”

Page 59: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Fractals• Geometric forms • Define by a recursive rule• Same on all scales

Benoit Mandelbrot

Page 60: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.

Serpinski Triangle

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Von Koch Snowflake

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Fractals are “Self-Similar”:

same when you zoom in

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The Julia Set

Gaston Julia, French mathematician

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The Mandelbrot Set

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Fractals in Nature

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Page 69: Astro 201: Sept. 6, 2010 Do on-line practice quiz #2 by 9/14 Homework #2: posted on web page, due 9/9 Reading: Hester, Chapters 2-3 Gleiser: Sections 3-6.