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Title: Astronomy 101 The Solar System Tuesday, Thursday 2:30-3:45 pm Hasbrouck 20 Tom Burbine tomburbine@astro.umass.edu


1
Astronomy 101The Solar SystemTuesday,
Thursday230-345 pmHasbrouck 20Tom
Burbinetomburbine_at_astro.umass.edu
2
Course
  • Course Website
  • http//blogs.umass.edu/astron101-tburbine/
  • Textbook
  • Pathways to Astronomy (2nd Edition) by Stephen
    Schneider and Thomas Arny.
  • You also will need a calculator.

3
Office Hours
  • Mine
  • Tuesday, Thursday - 115-215pm
  • Lederle Graduate Research Tower C 632
  • Neil
  • Tuesday, Thursday - 11 am-noon
  • Lederle Graduate Research Tower B 619-O

4
Homework
  • We will use Spark
  • https//spark.oit.umass.edu/webct/logonDisplay.dow
    ebct
  • Homework will be due approximately twice a week

5
Class Averages
  • For people who took all 4 tests
  • Class average is 81
  • Grades range from a 98.5 to a 55.4
  • Scores will go up when the lowest exam grade is
    dropped after the final

6
  • A (92.50 100)
  • A- (89.50 92.49)
  • B (87.50 89.49)
  • B (82.50 87.49)
  • B- (79.50 82.49)
  • C (77.50 79.49)
  • C (72.50 77.49)
  • C- (69.50 72.49)
  • D (59.50 69.49)
  • F (below 59.49)

7
Final
  • Cumulative
  • Monday - 12/14
  • 400 pm
  • Hasbrouck 20
  • Review Session
  • Sunday -12/13
  • 300 pm
  • Hasbrouck 134

8
Formulas you may need to know
  • p2 a3
  • F GMm/r2
  • F ma
  • a GM/r2
  • Escape velocity sqrt(2GM/r)
  • T (K) T (oC) 273.15
  • c f?
  • E hf
  • KE 1/2mv2
  • E mc2
  • Density mass/volume
  • Volume 4/3?r3

9
More Formulas
  • Power emitted per unit surface area sT4
  • ?max (nm) (2,900,000 nmK)/T
  • Apparent brightness Luminosity
  • 4? x
    (distance)2

10
Intelligent Life
  • Intelligent life that we can detect is usually
    defined as life that can build a radio telescope

11
Radio
  • Transmitting information over radio waves is very
    cheap
  • uses equipment that is easy to build
  • has the information-carrying capacity necessary
    for the task
  • The information also travels at the speed of
    light.

12
Fermis Paradox
  • Where are they?

13
Fermis Paradox
  • Why have we not observed alien civilizations even
    though simple arguments would suggest that some
    of these civilizations ought to have spread
    throughout the galaxy by now?

14
Reason for question
  • Straightforward calculations show that a
    technological race capable of interstellar travel
    at (a modest) one tenth the speed of light ought
    to be able to colonize the entire Galaxy within a
    period of one to 10 million years.

15
Explanation
  • Interested in us but do not want us (yet) to be
    aware of their presence (sentinel hypothesis or
    zoo hypothesis)

16
Explanation
  • Not interested in us because they are by nature
    xenophobic or not curious

17
Explanation
  • Not interested in us because they are so much
    further ahead of us

18
Explanation
  • Prone to annihilation before they achieve a
    significant level of interstellar colonization,
    because     (a) they self-destruct     (b) are
    destroyed by external effects, such as
            (i) the collision of an asteroid or
    comet with their home world         (ii) a
    galaxy-wide sterilization phenomenon (e.g. a
    gamma-ray burster       (iii) cultural or
    technological stagnation

19
Explanation
  • Capable of only interplanetary or limited
    interstellar travel because of fundamental
    physical, biological, or economic restraints

20
Fermis paradox
  • The Fermi paradox is the apparent contradiction
    between high estimates of the probability of the
    existence of extraterrestrial civilizations and
    the lack of evidence for, or contact with, such
    civilizations.
  • http//en.wikipedia.org/wiki/Fermi_paradox

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22
Jupiter
  • Largest planet
  • Mass - 1.8991027 kg (317.8 Earths)
  • Jupiter is 2.5 times more massive than all the
    other planets combined
  • Mean density - 1.326 g/cm3
  • Equatorial diameter - 142,984 km (11.209 Earths)

23
Probes to Jupiter
  • Pioneer 10 1973
  • Pioneer 11 - 1974
  • Voyager 1 1979
  • Voyager 2 - 1979
  • Ulysses - 1992
  • Galileo 1995 - Orbiter
  • Cassini - 2000

24
Jupiter
  • Jupiter's atmosphere is composed of
  • 81 hydrogen and 18 helium.
  • Jupiter probably has a core of rocky material
    amounting to something like 10 to 15
    Earth-masses.
  • Above the core lies the main bulk of the planet
    in the form of liquid metallic hydrogen. This
    exotic form of the most common of elements is
    possible only at pressures exceeding 4 million
    bars
  • 1 bar standard atmospheric pressure at sea
    level on Earth.

25
  • Jupiter is composed
  • relatively small rocky core
  • surrounded by metallic hydrogen
  • surrounded by liquid hydrogen
  • surrounded by gaseous hydrogen.

26
Clouds
  • clouds of ammonia (NH3), methane (CH4), ammonia
    hydrosulfide (NH4HS)

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  • zone for the light stripes
  • belt for the dark stripes
  • http//en.wikipedia.org/wiki/Cloud_pattern_on_Jupi
    ter
  • The differences in colors are caused by slight
    differences in chemical composition and
    temperature
  • http//zebu.uoregon.edu/imamura/121/lecture-13/vj
    upitr2.mov

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31
Galileo Probe
32
Great Red Spot
  • A particularly violent storm, about three times
    Earth's diameter, is known as the Great Red Spot,
    and has persisted through more than three
    centuries of human observation.
  • The spot rotates counterclockwise, once every 7
    days.

33
Jupiters Rings
  • Jupiter has a faint planetary ring system
    composed of smoke-like dust particles knocked
    from its moons by meteor impacts.

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35
Jupiter has four rings
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38
Voyager 1 and 2
  • Voyager 2 launched first (1977)
  • Then Voyager 1 (1977)

39
Grand Tour
  • Planetary Grand Tour was an ambitious plan to
    send unmanned probes to the outermost planets of
    the solar system. Conceived by Gary Flandro of
    the Jet Propulsion Laboratory, the Grand Tour
    would have exploited the alignment of Jupiter,
    Saturn, Uranus, Neptune and Pluto

40
Voyager 2
  • Went to Jupiter, Saturn, Uranus, and Neptune

41
Voyager 1
  • Went to Jupiter and Saturn

42
Voyager Golden Record
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44
Pioneer 10 and 11 Plaques (1972)

45
Saturn
46
Saturn
  • Known since prehistoric times
  • Galileo was the first to observe it with a
    telescope in 1610
  • In 1659, Christian Huygens correctly inferred the
    geometry of the rings
  • Saturn is the least dense of the planets its
    density (0.7 g/cc) is less than that of water.

47
Rings
  • Very thin
  • 250,000 km or more in diameter they are less than
    one kilometer thick
  • The ring particles seem to be composed primarily
    of water ice, but they may also include rocky
    particles with icy coatings.

48
Roche Limit
  • Rings are either a satellite torn apart by tidal
    forces or material that was never allowed to
    condense into moons because of the tidal forces

49
  • http//csep10.phys.utk.edu/astr161/lect/saturn/rin
    gs.html

50
Cassini-Huygens
  • Visited Saturn and Titan

51
Uranus
52
Uranus
  • Discovered by William Herschel in 1781
  • In 1977, the first nine rings of Uranus were
    discovered

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Atmosphere
  • The atmosphere of Uranus is composed of 83
    hydrogen, 15 helium, 2 methane and small
    amounts of acetylene and other hydrocarbons.
  • Methane in the upper atmosphere absorbs red
    light, giving Uranus its blue-green color.

55
Unusual
  • Tipped on its side
  • Why?

56
Probably
  • Due to a collision

57
Uranus Satellites
  • Miranda
  • Ariel
  • Umbriel
  • Titania
  • Oberon
  • 2001U3
  • Caliban
  • Stephano
  • Trinculo
  • Sycorax
  • 2003U3
  • Prospero
  • Setebos
  • 2002U2
  • Cordelia
  • Ophelia
  • Bianca
  • Cressida
  • Desdemona
  • Juliet
  • Portia
  • Rosalind
  • 2003U2
  • Belinda
  • 1986U10
  • Puck
  • 2003U1

58
  • Instead of being named after people from
    classical mythology, Uranus' moons take their
    names from the writings of William Shakespeare
    and Alexander Pope.

59
Neptune
60
Neptune
  • After the discovery of Uranus, it was noticed
    that its orbit was not as it should be in
    accordance with Newton's laws.
  • It was therefore predicted that another more
    distant planet must be perturbing Uranus' orbit.
  • Neptune was first observed by Johan Galle and
    Heinrich d'Arrest on 1846 Sept 23 very near to
    the locations predicted from theoretical
    calculations based on the observed positions of
    Jupiter, Saturn, and Uranus.

61
Galileo
  • Galileo's astronomical drawings show that he had
    first observed Neptune on December 27, 1612, and
    again on January 27, 1613
  • on both occasions Galileo had mistaken Neptune
    for a fixed star

62
  • Neptune's blue color is largely the result of
    absorption of red light by methane in the
    atmosphere

63
Great Dark Spot
  • Thought to be a hole

Scooter
Small dark spot
64
Great Dark Spot has disappeared
65
Neptunes Rings
66
Shoemaker-Levy 9
  • Comet that hit Jupiter
  • Discovered in 1993
  • Hit Jupiter in 1994

67
Roche Limit
  • The smallest distance at which a natural
    satellite can orbit a celestial body without
    being torn apart by the larger body's
    gravitational force. The distance depends on the
    densities of the two bodies and the orbit of the
    satellite.
  • If a planet and a satellite have identical
    densities, then the Roche limit is 2.446 times
    the radius of the planet.
  • Jupiter's moon Metis and Saturn's moon Pan are
    examples of natural satellites that survive
    despite being within their Roche limits

68
Why is the Roche Limit important?
  • Comet Shoemaker-Levy 9's decaying orbit around
    Jupiter passed within its Roche limit in July,
    1992, causing it to break into a number of
    smaller pieces.
  • All known planetary rings are located within the
    Roche limit

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  • The first impact occurred at 2015 UTC on July
    16, 1994
  • Fragment A of the nucleus slammed into Jupiter's
    southern hemisphere at a speed of about 60 km/s.
  • Instruments on Galileo detected a fireball which
    reached a peak temperature of about 24,000 K,
    compared to the typical Jovian cloudtop
    temperature of about 130 K, before expanding and
    cooling rapidly to about 1500 K after 40 s.

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72
Has this happened before?Ganymede
73
Ganymede-Europa
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76
Satellites
  • Jupiter has 63 known satellites
  • The four large Galilean moons plus many more
    small ones some of which have not yet been named

77
Simon Marius (1573-1624)
  • In 1614, Marius published his work Mundus
    Iovialis describing how he had discovered
    Jupiters Moons some days before Galileo did
  • The names by which these satellites are known
    today (Io, Europa, Ganymede and Callisto) are
    those given them by Marius.
  • But untile the middle of the 20th century, these
    satellited were known as "Jupiter I," "Jupiter
    II," "Jupiter III," and "Jupiter IV"
  • Gan De, a Chinese astronomer, may have discovered
    the moons in 362 BC

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Galileo
80
Galileo spacecraft
  • Launched in 1989
  • It arrived at Jupiter on December 7, 1995
  • On September 21, 2003, Galileo's mission ended by
    crashing into Jupiter's atmosphere to avoid any
    chance of it contaminating the Galilean moons
    with bacteria from Earth.

81
Sagans Criteria for Life(From measurements of
Earth by Galileo)
  • Strong absorption of light at the red end of the
    visible spectrum, caused by absorption by
    chlorophyll in photosynthesizing plants
  • Absorption bands due to molecular oxygen (O2),
    which is also a result of plant activity (O2 in
    our atmosphere is many orders of magnitude
    greater than is found on any other planet in the
    Solar System)
  • Infrared absorption bands caused by methane (CH4)
    (about 1 part per million in Earth's atmosphere),
    a gas which must be replenished by either
    volcanic or biological activity)
  • Modulated narrowband radio wave transmissions
    uncharacteristic of any known natural source.

82
Densities
  • Io - 3.53 g/cm3
  • Europa - 3.01 g/cm3
  • Ganymede 1.94 g/cm3
  • Callisto (JIV) 1.83 g/cm3

83
Io
84
Io
  • Io has almost no craters as first seen by Voyager
    I (1979)
  • What does that mean?

85
  • It is geologically active
  • Voyager I saw 9 active volcanos

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  • The energy for this activity probably derives
    from tidal interactions among Io, Jupiter, and
    two other moons of Jupiter, Europa, and Ganymede.

89
Europa
90
Europa
  • Very smooth surface
  • Its albedo is one of the highest of all moons
  • Lack of craters indicates a young and active
    surface

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  • Symmetric ridges in the dark bands suggest that
    the surface crust was separated and filled with
    darker material, somewhat analogous to spreading
    centers in the ocean basins of Earth.

94
  • Spectroscopy suggests that the dark reddish
    streaks and features on Europa's surface may be
    rich in salts such as magnesium sulfate (Epsom
    salt), deposited by evaporating water that
    emerged from within.

95
Europa
  • It is thought that under the surface there is a
    layer of liquid water kept warm by tidally
    generated heat.

96
Ganymede
97
Ganymede
  • Largest Moon of Jupiter
  • Largest Moon in the solar system

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  • Surface is a mix of two types of terrain
  • very old, highly cratered dark regions
  • somewhat younger (but still ancient) lighter
    regions marked with an extensive array of grooves
    and ridges.

100
Galileo Regio
101
Callisto
102
Callisto
  • One of the most heavily cratered objects in the
    solar system
  • No large mountains

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