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    The History and Philosophyof Astronomy

    (Lecture 10: Tycho/Kepler II)

    Instructor: Volker BrommTA: Jarrett Johnson

    The University of Texas at Austin

    Astronomy 350L

    (Fall 2006)

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    Tycho and Kepler meet in Prague (1600-01)

    Tycho needs Kepler:

    - difficult calculations

    to figure out orbit of Mars

    Kepler needs Tycho:

    - precision data to

    figure out true orbitsof the planets

    Together embark onimproved astron. tables

    (Tabulae Rudolphinae)

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    Johannes Kepler: The Great Theorist

    1571 1630

    born into middle-class:- lifelong economic struggles

    completed Copernicus

    agenda

    The last mystic(last scientific astrologer)

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    Kepler: Geography of his Life

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    Europe: Deeply divided into multiple confessions

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    Kepler: Birth and Upbringing in Wuerttemberg

    Born 1571: Weil der Stadt (near Stuttgart)

    middle-class family father: a mercenary, mother: cantankerous

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    University Education at Tuebingen (1589-94)

    Leading Protestant

    University

    Undergrad(7 Liberal Arts)

    (Lutheran) Theology

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    University Education at Tuebingen (1589-94)

    Michael Maestlin, professorof mathematics and astronomy

    taught: Ptolemy and

    Copernicus

    lifelong friendship with

    Kepler

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    Neoplatonism: Search for hidden harmony

    God

    Realm of Ideas Realm of Experience

    (William Blake, 1757-1827)

    Motion of planets

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    Neo-Pythagoreanism: A Universe governed by Numbers

    Divine Tetractys:

    1 + 2 + 3 + 4 = 10

    - symbolizes the universe!

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    Kepler studies Theology and makes Enemies

    Last Supper Controversy:

    - Lutherans: Wine isChrist- Calvinists: Wine only symbolizesChrist

    Kepler, being a Lutheran, supports Calvinist view

    Source of great trouble, professionally and personally

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    Mathematician in Graz (Austria)

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    Mathematician in Graz

    Teacher at Protestant High School

    Styrian estate mathematician: horoscopes

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    Mysterium Cosmographicum

    Why are there exactlysix planets?

    What determines theirdistances from the Sun?

    Cosmographic Mystery(1596)

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    Mysterium Cosmographicum: 5 Platonic Solids

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    Mysterium Cosmographicum

    planetary orbits nested between

    Platonic solids!

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    Kepler and Astrology

    One of his duties: Work out annual calendars, i.e.,

    predict the events of the year ahead!

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    Kepler and Astrology

    Kepler: one of the last scientific astrologers!

    Henceforth, astronomy and astrology part company

    (Keplers nativity)

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    Kepler: Fleeing the Counter Reformation in Graz

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    Kepler: Move to Imperial Prague

    Rudolph II- Emperor (1576-1612)

    Great Patron of Arts and Sciences (Tycho, Kepler)

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    Tychos Assistant in Imperial Prague

    Benatky Castle: Tychos Final Domicile (1599 1601)

    Tycho invites upstart young Johannes Kepler!

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    Kepler: The Inheritor of Tycho

    After Tychos death (1601): Kepler moves quickly

    to get hold of Tychos data

    Emperor Rudolph II appoints Kepler to becomeImperial Mathematician

    Imperial order: Complete Rudolphine Tables

    Keplers main agenda: Win the battle with Mars

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    Keplers ``Warfare with Mars

    Tycho pointed out to Kepler that orbit of Mars

    is particularly difficult to understand! Orbit of Mars shows large deviation from circularity!

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    The New Astronomy: The Orbits of the Planets

    Astronomia Nova(New Astronomy, 1609)

    Keplers 1st and 2nd Law:

    - planets move in elliptic

    orbits with Sun in one focus- law of areas

    Finally: A model that works!

    Introduce Celestial Physics

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    The New Astronomy: The Orbits of the Planets

    Problem: Observe

    (Mars-orbit) from moving

    platform (Earth)!

    But want to figure out

    orbit with respect to Sun!

    A convolved problem!

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    Long Process of Trial-and-Error

    Method: (1) Try given orbital geometry, and

    (2) compare with Tychos data

    All combinations involving circles, can onlygive accuracy of ~ 8 arcmin

    But: Kepler knew that Tychos data have accuracy

    of ~ 4 arcmin

    Thus: Reject circular orbits!

    Eventually: Try elliptic orbits with Sun in one focus!

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    Orbit of the Planets: Keplers 1st Law

    1st Law: Planets move in ellipses with the Sun in

    one focus!

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    Orbit of the Planets: Keplers 1st Law

    Ellipse is one of the three conic sections,

    and the circle is a special case!(Conic sections described by Apollonius of Perga in 200 BC)

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    Speed of the Planets: Keplers 2nd Law

    Start with Sun-centered version of Ptolemys equant!

    Earth

    Sun

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    Speed of the Planets: Keplers 2nd Law

    Kepler realizes: Pseudo-equant is almost equivalent

    to equal area in equal times as seen from Sun!

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    Speed of the Planets: Keplers 2nd Law

    2nd Law: A line drawn from the Sun to a planet

    sweeps out equal areas in equal times!

    A=B=C

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    Finally solving the Problem of the Planets

    One unified framework valid for allplanets!

    - No ad-hoc fixes allowed!

    For each planet, 2 free quantities (parameters)to choose: semi-major axis a, and eccentricity e

    It could not have been done without Tychos data!

    C dE i P (1611)

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    Coup-dEtat in Prague (1611)

    Emperor Rudolph deposed by his brother

    Rudolph II Matthias

    Kepler has to leave Prague

    M t Li (U A t i )

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    Move to Linz (Upper Austria)

    M th ti i i Li (1612 28)

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    Mathematician in Linz (1612-28)

    Teacher at Protestant High School

    Upper-Austrian estate mathematician: horoscopes

    Th H r f th W rld

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    The Harmony of the Worlds

    Harmonices Mundi(Harmony of the Worlds, 1619)

    Keplers 3rd Law:

    - P2

    =a3

    full of mystical speculation

    The Harmony of the Worlds

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    The Harmony of the Worlds

    Keplers 3rd Law:

    - P2

    =a3

    The Harmony of the Worlds

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    The Harmony of the Worlds

    The Music of the Spheres

    recall: Pythagoras

    Rudolphine Tables (Tabulae Rudolphinae)

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    Rudolphine Tables (Tabulae Rudolphinae)

    improve Reinholds old (1551)

    Prutenic Tables

    based on Copernicus

    De Revolutionibus

    limited accuracy in light ofTychos observations

    Kepler has promised Tycho

    on deathbed to complete this

    Rudolphine Tables (Tabulae Rudolphinae)

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    Rudolphine Tables (Tabulae Rudolphinae)

    Tabulae Rudolphinae(1627)

    based on Keplers newlaws of planetary motion

    unprecedented accuracy

    (after all: Keplers is thecorrect model)

    Astronomers adopt tables first,

    before the theoretical works

    Rudolphine Tables

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    Rudolphine Tables

    Tables: non-glamorous, but very useful!

    Rudolphine Tables: The Frontispiece

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    Rudolphine Tables: The Frontispiece

    Allegory of Astronomy

    Witchcraft Trial of Keplers Mother (1620-21)

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    Witchcraft Trial of Kepler s Mother (1620 21)

    Water Trial

    Kepler (successfully) defended his old mother

    Kepler: Pact with the Devil (1628-30)

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    Kepler: Pact with the Devil (1628 30)

    Entered the employ

    of generalissimo

    Wallenstein

    Wallenstein was firm

    believer in astrology

    Moved to Sagan

    Wallenstein, Supreme

    Commander of Imperial TroopsIn Thirty Years War

    Journeys End: Death in Regensburg (1630)

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    Journey s End: Death in Regensburg (1630)

    Keplers Epitaph:

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    p p p

    I measured the skies, now

    the shadows I measure.Skybound was the mind,

    eartbound the body rests

    Keplers role in the Scientific Revolution

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    ep e s o e t e Sc e t c e o ut o

    Newton (1642-1727)- dynamics

    - law of gravity

    Kepler (1571-1630)- celestial motion

    - 3rd Law

    Galileo (1564-1642)- laws of free-fall

    - principle of inertia

    Standing on theshoulders of giants

    Tycho/Kepler (part 2): Johannes Kepler

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    y p p p

    Johannes Kepler:- finally solves the problem of the planets

    - break free from the old dogma of uniform circular motion

    - completes Copernican Revolution

    Keplers Laws of Planetary Motion

    - 1

    st

    Law: Planets move in ellipses with the Sun in one focus- 2nd Law: A line from the Sun to a planet sweeps over equalareas in equal time (Law of Areas)

    - 3rd Law: P2 = a3

    Kepler calculates Rudolphine Tables

    - New standard of precision