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ASTRONOMY 161 Introduction to Solar System Astronomy

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Title: ASTRONOMY 161 Introduction to Solar System Astronomy


1
ASTRONOMY 161Introduction to Solar System
Astronomy
Class 6
2
Tycho, Kepler, GalileoMonday, October 5
  • E pur si muove! It still moves!
  • - Galileo

3
Astronomical movies
  • The Phases of Venus
  • http//antwrp.gsfc.nasa.gov/apod/ap060110.html
  • When Moons and Shadows Dance (Jupiter)
  • http//antwrp.gsfc.nasa.gov/apod/ap030227.html
  • Large Sunspot Group (Sun)
  • http//antwrp.gsfc.nasa.gov/apod/ap010411.html

4
Tycho, Kepler, Galileo Key Concepts
  • (1) Tycho Brahe made accurate measurements of
    planetary motion.
  • (2) Planetary orbits are ellipses with the Sun at
    one focus.
  • (3) A line between planet Sun sweeps out equal
    areas in equal times.
  • (4) The square of a planets orbital period is
    proportional to the cube of its average distance
    from the Sun.
  • (5) Galileo made telescopic observations
    supporting the heliocentric model.

5
(1) Tycho Brahe made accurate measurements of
planetary motion.
  • Tycho Brahe (1546-1601) Danish astronomer

6
Tychos contributions to astronomy
  • Tycho discovered new star, or nova, upsetting
    ancient notion of perfect, unchanging heavens.
  • Made very accurate measurements of planetary
    positions.

7
  • Copernican system

8
  • Tychos system

9
Johannes Kepler (1571-1630) German
  • Was Tychos assistant.
  • Used Tychos data to discover
  • Three Laws of Planetary Motion.

10
(2) Keplers First Law
of planetary motion
  • The orbits of planets around the Sun are ellipses
    with the Sun at one focus.

11
Ellipse an oval built around two points, called
focuses (or foci).
  • SIZE of ellipse
  • Major axis longest diameter of ellipse.
  • Semimajor axis half the major axis.

12
SHAPE of ellipse
  • Eccentricity distance between foci divided by
    major axis.
  • Foci close together ellipse nearly circular,
    eccentricity close to zero.
  • Foci far apart ellipse very flattened,
    eccentricity close to one.

13
Example Mars
  • Semimajor axis 1.524 A.U.
  • Eccentricity 0.093 (much smaller than one)

14
Ellipse comes from the family of Conic Sections
15
(3) Keplers
Second Law of planetary motion
  • A line
    from the Sun to a planet
    sweeps out equal areas
    in equal time intervals.

16
Consequences of Keplers Second Law
  • Planets move fastest when closest to the Sun.
  • Example Mars
  • Perihelion 206,600,000 km (1.381 A.U.)
  • Max. Orbital Speed 26.5 km/s
  • Aphelion 249,200,000 km (1.666 A.U.)
  • Min. Orbital Speed 22.0 km/s

17
(4) Keplers Third Law of
planetary motion
  • The square of a planets orbital period is
    proportional to the cube of its average distance
    from the Sun
  • A planets average distance from the Sun is
    equal to the semimajor axis of its orbit.

18
Keplers Third Law in mathematical form
  • P orbital period (in years)
  • a semimajor axis (in A.U.)
  • Example The orbit of Mars

19
(5) Galileo made telescopic observations
supporting the heliocentric model.
  • Galileo Galilei (1564-1642) Italian
  • Galileo was among the first to observe the sky
    with a telescope (1609).

20
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21
Flashback to Class 1 What is Science?
  • The SYSTEMATIC study of the Universe
  • Gather facts
  • Modify hypothesis Guess an
    explanation
  • (Guesshypothesis)
  • Test hypothesis

22
1) Mountains on the Moon
  • Aristotle Ptolemy said the Moon is a perfect,
    smooth sphere.
  • In fact, the Moon is no more perfect than the
    Earth.

23
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24
2) The Sun has spots on its surface.
  • The Sun is not perfect.
  • Motion of sunspots indicates that the Sun is
    rotating.
  • If the Sun rotates, why not the Earth?

25
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26
3) The planet Jupiter has moons of its own.
  • Four Galilean moons of Jupiter Io, Europa,
    Ganymede, Callisto.
  • The Earth is NOT the center of all orbits in the
    universe.

27
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29
4) Venus shows phases
like those of the Moon.
  • Venus goes through all phases looks big when
    nearly new, looks small when full.
  • Results consistent with Copernicus, inconsistent
    with Ptolemy.

30
Phases of Venus in the
geocentric model of Ptolemy.
  • Only new and crescent phases.

31
Phases of Venus in the
heliocentric model.
  • All phases smaller angular size
    when full than when new.

32
Few closing questions
  • 1) Do the inner planets show retrograde motions?
    (again)
  • 2) See picture on the right. What is it?
  • 3) Does Mercury show phases? Mars? Jupiter?

33
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34
Few closing questions continued
  • 4) If the Sun is at one focus of the ellipse,
    what is at the other focus?
  • 5) See picture on the right. What is it? Is it
    real?
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