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Astronomy

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Title: Astronomy


1
Astronomy
This picture was taken by the Hubble Space
Telescope and is provided courtesy of the Space
Telescope Science Institute.
  • What is out there?
  • How big is the universe?
  • Does the universe have an edge?
  • When did the universe begin, and will it end?
  • Is anybody else out there?

2
Astronomy
  • Astronomy is one of the sciences. This class is
    designed to fulfill the science requirement and
    so needs to emphasize what science is (and isnt)
    and how science works, using astronomy as the
    example.
  • Thus the first question to ask is What is a
    Science? (and what is NOT science?)
  • Another question we need to consider while we
    consider the first question is Can Science
    discover the truth ?

3
Science
  • To really answer this question, we need to ask
    What is the Scientific Method?
  • (What are the STEPS in the Scientific Method?)

4
Scientific Method
  • 1. Define the problem what are we trying to
    figure out?
  • 2. Gather data experiment to see what happens.
  • 3. Hypothesize try to explain what we see a
    good theory should a) organize what we know, and
    b) predict new things to look for.
  • 4. Test the hypothesis Go back to step 2
    (gather data) to see if the predictions work.

5
Scientific Theories
  • For a theory to be classified as scientific, it
    must be testable (and hence falsifiable).
  • For data to be considered scientific, it must be
    repeatable.
  • As we go through this course, we will see
    theories that were quite useful in their time but
    were later proved inadequate and were replaced by
    better theories. This process is continuing
    today.

6
Scientific Truth
  • The scientific method as listed on the previous
    slide looks like an infinite loop (it keeps going
    back to step 2!). Do we ever get out of this
    loop - do we ever discover the real truth ?

7
Scientific Truth
  • A related question is can we perform perfect
    experiments - can we make perfect measurements?
    No!
  • If we cannot measure perfectly, there is always
    room for a little doubt!
  • Does this mean that we really dont know anything?

8
Scientific Truth
  • In some cases, we have tested theories, and they
    agree with experiment to a high degree of
    accuracy these theories agree with measurements
    to the best that we can perform the measurements.
    For example, we know that gravity attracts, and
    that the formula for gravity works extremely well!

9
Scientific Uncertainty
  • However, other theories (like weather prediction
    and global warming) are still quite uncertain and
    do not agree all that well with all the data.
    However, we are making good progress in these
    difficult areas.
  • Since science is based on experiment, even
    untrue theories can still be useful in making
    predictions and hence in developing technologies.
    However, we must always be careful in
    believing theories until they have been
    thoroughly tested.

10
Science and Philosophy
  • In some cases we have theories which cannot yet
    be tested. In these cases, choosing between
    competing theories is more a matter of philosophy
    than of science.
  • Later, when the technology allows for tests to be
    made, the theories then can become scientific.

11
Astronomy
  • The first step in the scientific method is
    Define the situation what are we trying to
    explain?
  • The situation is different for the different
    scientific disciplines. So what are we looking
    at in astronomy?

12
Astronomy
  • Astronomy is the science which describes the
    celestial bodies according to their locations,
    sizes, motions, constitutions and evolutions.
  • The first part of the course considers what we
    can find out by using only our unaided eyes. We
    will consider how different people and
    civilizations made sense of these observations.

13
Astronomy course overview
  • In part two we will look at our modern tools
    (mainly the telescope and spectrograph) for
    extending our data gathering.
  • In the remaining parts of the course we consider
    our current best theories about astronomy in
    part 3 we consider the objects in our
    astronomical neighborhood the solar system in
    part 4 we consider stars and in part 5 we
    consider how stars are grouped and how big and
    old the universe is.

14
Gathering Data
  • What are the objects that we see when we look up?
    For each, we need to consider the following
    questions
  • how big does it appear in the sky?
  • (how big an angle does it make with the eye?)
  • how bright does it appear to be?
  • (how do we measure brightness?)
  • where is it located?
  • (how do we indicate location?)
  • how does it appear to move?
  • (is it moving, are we moving, or both?)

15
Gathering Data
  • 1. Sun
  • 2. Moon
  • 3. Stars
  • 4. Planets (how are planets and stars
    different?)

16
Sun
  • How big?
  • (what shape is it?)
  • (how do we measure size for this shape?)
  • (how do we measure size for objects that are far
    away?)

This image was taken by SOHO's EIT
(Extreme-Ultraviolet Imaging Telescope) and is
courtesy of the EIT Consortium.
17
Sun
  • a) How big? A circle (or ball?) in the sky
    with a diameter that forms an angle with the eye
    of about ½ degree. (There are 360 degrees in a
    full circle. Who decided that we break a circle
    into 360 equal parts instead of, say, 100?)

Angle the sun makes is about ½ degree
From horizon to horizon covers 180 degrees
18
Sun
  • The 360 degrees in a circle comes from the
    observed fact that there are 365 days in a year
    (solar cycle). But 365 is an inconvenient number
    since it is odd. The 360 is much better since it
    is divisible by 2, 3, 4, 5 and 6!
  • b) How bright is the sun?

19
Sun
  • b) How bright is the sun? Very! It overwhelms
    almost everything else in the sky when it is
    visible. (Well set up a scale later.)
  • c) Where is the sun located?

20
Sun
  • c) Where is the sun located? At different
    places in the sky at different times of the day
    and at different places in the sky at the same
    time of day when viewed from different locations
    on the earth. (For instance, the sun may still
    be up on the West Coast when it has already set
    on the East Coast.) This will be further
    analyzed as we answer the next question
  • d) How does the sun move?

21
Sun
  • d) How does the sun move?
  • d1 a DAY is the time from noon on one day to
    noon on the next day. Noon is the time of day
    when the sun is highest in the sky (and shadows
    are the smallest).
  • d2 The sun rises in the East (more or less) and
    sets in the West (more or less). Does the sun
    always rise exactly due East and set exactly due
    West?

22
Sun
  • d2 Does the sun always rise exactly due East
    and set exactly due West?
  • No! The sun rises North of due East and sets
    North of due West in the spring and summer, and
    it rises South of due East and Sets South of due
    West in the fall and winter. It only rises due
    East on the first day of spring and first day of
    fall. This change in the rising and/or setting
    positions of the sun can be used to mark a yearly
    calendar.

23
Sun
  • In the first lab meeting, we will use a star
    chart to investigate the motions of the suna)
    how it rises and sets throughout the yearb)
    how high in the sky it is at noon at different
    days throughout the yearc) how the sun moves
    relative to the stars.
  • There is a separate powerpoint set on the Star
    Charts which you can use to familiarize yourself
    with this useful tool.

24
Moon
  • a How big is the moon?
  • (What shape is it?)
  • (How does the moons size compare to the suns
    size?)

The Galileo spacecraft sent back this image of
the Moon as it headed into the outer solar
system. The distinct bright ray crater at the
bottom of the image is the Tycho impact basin.
25
Moon
  • a) How big is the moon? A circle (or ball?)
    that makes about ½ degree with the eye.This is
    about the same size (in angle) as the sun. This
    will be important when we talk about eclipses in
    Part III. The moon appears to change shape from
    a new moon (which is dark) to a crescent shape to
    a half circle to a gibbous shape to a full circle
    and then back through these shapes to a new moon.
    This cycle takes about a month.
  • b) How bright is the moon?

26
Moon
  • b) How bright is the moon? A full moon is quite
    bright - enough to make it hard to see the dimmer
    stars, but not nearly as bright as the sun. The
    new moon is so dim it is hard to see (also
    because it appears to be so close to the sun).
  • c) Where is the moon located?

27
Moon
  • c) Where is the moon located? At different
    places in the sky at different times of the day
    the phases (shape) of the moon are related to its
    position during the day. New moons are always
    near the sun, and full moons are always opposite
    the sun.
  • d) How does the moon move?

28
Moon
  • d) How does the moon move? It follows a path
    similar to that of the sun rising somewhere in
    the East and setting somewhere in the West. Its
    time of rising and setting changes during the
    month. When the moon is new, it rises and sets
    with the sun when the moon is full, it rises and
    sets opposite the sun.

29
Stars
  • a) How big do the stars appear to be?

Betelgeuse, the brightest star in the
constellation Orion. (Produced with ESA's Faint
Object Camera (FOC), Hubble Space Telescope.)
30
Stars
  • a) How big do the stars appear to be? Each star
    appears to be a point, that is, it makes too
    small an angle to be measured.
  • b) How bright are the stars?

31
Stars
  • b) How bright are the stars? The stars vary in
    brightness - some are so dim that they can only
    be viewed by the most powerful telescopes while
    others are bright enough to be seen in faint
    early dawn or late evening twilight. (Well set
    up a scale later.)
  • c) Where are the stars located?

32
Stars
  • c) Where are the stars located? Like the sun
    and the moon, stars move across the sky however,
    the stars do not move relative to one another -
    that is, we can group them into constellations
    (like the big dipper).
  • d) How do the stars move?

33
Stars
  • d) How do the stars move? Except for the North
    Star, all stars move across the sky. They move
    around the North Star and so most seem to rise in
    the East and set in the West just like the sun
    and moon.
  • In this connection, the sun and the moon do
    change relative position with the stars. The sun
    seems to move along a path through the stars
    called the ecliptic. The moon follows a path
    very close to the ecliptic.

34
Sun and Stars
  • The constellations that are found on the path of
    the sun (the ecliptic) are called the
    constellations of the zodiac. During the year
    the sun moves along the ecliptic spending
    approximately one month in each of the 12
    constellations of the zodiac. The sun moves from
    West to East through these constellations
    (although it moves from East to West across the
    sky), and this causes the sun to rise a little
    later than a particular constellation or star
    each day, and conversely the constellation and
    its stars rise a little earlier each day.

35
Constellations of the Zodiac
  • The months below refer to when the sun appears to
    be in the constellation
  • Constellation Month Constellation Month
  • Aquarius March Leo September
  • Pisces April Virgo October
  • Aries May Libra November
  • Taurus June Scorpius December
  • Gemini July Sagittarius January
  • Cancer August Capricornus February
  • Note The months are approximate

36
Heliacal Rising
  • Since the stars appear to rise a little earlier
    each day than the sun, for each star there is one
    day each year that the star can first be seen
    before sunrise (assuming clear skies). After
    that, the star can be seen earlier and earlier.
    This first day is called the heliacal rising of
    that star. Some cultures based their calendars
    on such heliacal risings of certain bright stars.

37
Moon, Sun and Stars
  • The moon also moves along a path very close to
    the one the sun moves on (the ecliptic). It
    makes a complete cycle around the path through
    the constellations of the zodiac once a month
    (rather than once a year like the sun). It also
    moves East along its path through the stars (but
    moves West through the sky as we see it), so it
    also rises a little later each day than the
    stars, and since the moon moves faster than the
    sun, the moon rises a little later (relative to
    the sun) each day.

38
Planets
  • Although the stars do notappear to move
    relativeto one another (and hence we can make
    constellations out of them),there are five
    visible exceptions to this(besides the sun and
    moon which makes the total seven).These the
    Greeks named wandering stars which today we call
    planets. The five planets visible to the naked
    eye are Mercury, Venus, Mars, Jupiter and
    Saturn.

Voyager 2 captured this image of Neptune in 1989.
39
Planets
  • Although without a telescope the planets do not
    appear to have a measurable size, with a modest
    telescope they do!
  • Do the planets wander all over the place, or do
    they have definite paths (like the sun and moon
    along the ecliptic)?

40
Planets
  • Do the planets wander all over the place, or do
    they have definite paths (like the sun and moon
    along the ecliptic)?
  • All the planets have definite paths through the
    stars, and all these paths are very close to the
    ecliptic.

41
Planets
  • Like the sun, moon and stars, the planets move
    across the sky from East to West but do the
    planets move across the ecliptic from West to
    East like the sun and moon?

42
Planets
  • Like the sun, moon and stars, the planets move
    across the sky from East to West but do the
    planets move across the ecliptic from West to
    East like the sun and moon? All the planets do
    move from West to East along the ecliptic MOST OF
    THE TIME, but occasionally each goes backward
    (from East to West). This is called RETROGRADE
    motion.

43
Planets
  • Another interesting piece of data Mercury and
    Venus are always close to the sun in the sky.
    You never see Mercury or Venus at midnight - only
    a little before dawn or a little after sunset.
    The other three Mars, Jupiter and Saturn can
    sometimes be seen close to the sun but can also
    be seen far from the sun (you can sometimes see
    these at midnight).

44
Positions in the sky
  • To locate a position on the earth, we can tell
    where it is in relation to other landmarks, or we
    can give its latitude and longitude.
  • In the same way in the sky, we can tell where
    something is near to something else, e.g., which
    constellation it is in or near, or we can give
    its declination and right ascension.

45
Declination
  • Declination is like latitude it gives the
    north-south position. The North Star is directly
    above the North Pole. So we give the North Star
    a declination of 90o (just like the North pole
    has a latitude of 90o North). The positions of
    the sky directly over the equator have a
    declination of 0o just like the equator has a
    latitude of 0o. Anything that is directly above
    places South of the Equator (latitude of xo
    South) is given a declination of -xo .

46
Right Ascension
  • Right Ascension is like longitude. It describes
    the East-West position. Just like longitude has
    to have some starting place (on Earth, we assign
    the North-South line through Greenwich, England
    as having 0o longitude), so right ascension needs
    some line to call 0. This line is the
    North-South line from the North Star through the
    location of where the sun is on March 21 (equal
    day and night equinox). Instead of degrees we
    use hours there are 24 hours in the complete
    circle.

47
Star Charts and locations
  • On one type of star chart the celestial equator
    (0o declination) is marked with a solid white
    line. On the other, the one used in the Star
    Chart powerpoint set, the celestial equator is
    the pink circle added to the slide. The North
    Star is the brass ring (since it is the one place
    that does not move). The ecliptic (path of sun,
    moon and planets) is marked with a dotted white
    line. On the other type, it is marked as the
    railroad tracks. Note that the dotted white
    line crosses the solid white line in two places
    the sun is at one place on March 21 and on the
    other on September 21 (the date of the two
    equinoxes).

48
Constellations of the Zodiac
  • The months below refer to when the sun appears to
    be in the constellation
  • Constellation Month RA Dec Constellation Month
    RA Dec
  • Aquarius March 23 0 Leo Sept. 11 0
  • Pisces April 1 0 Virgo Oct. 13
    0
  • Aries May 3 Libra Nov. 15 -
  • Taurus June 5 Scorpius Dec. 17
    -
  • Gemini July 7 Sagittarius Jan.
    19 -
  • Cancer August 9 Capricornus Feb. 21
    -
  • Note The months and Right Ascension are
    approximate
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