Ch. 1
Earth, Moon, and Sun
              This amazing
              Earthrise above
              the moon's
              horizon was seen
              by astronaut
              Michael Collins in
              the Apollo 11
              moon orbiter
              Columbia.
Objectives
Identify the effects of Earth’s
rotation and revolution.
Explain the causes of the
seasons on Earth.
Section 1, Earth in Space

                Why Does
                Earth Have
                Day and
                Night?
Introduction

      Egyptian farmers planted
      their crops after the floods
      every year. They noticed
      that the star Sirius
      became visible before the
      floods. That’s when they
      could start predicting the
      floods.
      The Egyptians were the
      first people to study the
      stars.
Days and Years
        Astronomy is the
        study of the moon,
        stars, and other
        objects in space.
Rotation
           Axis - the
           imaginary line that
           passes through
           Earth’s center and
           the North and
           South poles.
           Rotation - the
           spinning of Earth
           on its axis.
           A point on the
           equator rotates at
           about 1,600 km
           per hour.
Rotation

Earth’s rotation on its axis
causes day and night.
Earth rotates eastward.
It takes 24 hours to rotate
once on its axis. This is called
a day.
Revolution

Earth also travels around the
sun.
Revolution - the movement of
one object around another
object.
Earth’s orbit is an oval shape.
Calendars
The Egyptians counted the number of
days between Sirius stars which was
about 365.
Earth’s orbit around the sun is about
365 1/4 days.
Four years of 365 1/4 days each can
be approx. by taking 3 years of 365
days and a fourth year of 366 days.
This is known as leap year.
On a leap year, one extra day in
February is added for 29 days.
Calendars
Dividing the year into smaller parts
(months) was difficult.
Early people used the moon cycle
which is 29 1/2 days but this only
added up to 354.
The Egyptians had a plan to have 12
months of 30 days and 5 extra days.
The Romans borrowed the calendar
and devised the one that we have
today with 11 months of 30 to 31
days and February with 28 or 29
days.
Seasons on Earth

            Most places
            have four
            seasons:
            winter, spring,
            summer, and
            autumn.
Earth’s Tilted Axis

                 Earth has
                 seasons
                 because its
                 axis is tilted as
                 it moves
                 around the
                 sun.
Earth in June
   The north end of
   Earth’s axis is
   tilted toward the
   sun. It is summer
   in the Northern
   Hemisphere and
   winter in the
   Southern
   Hemisphere.
Earth in December
      The south end
      of Earth’s axis
      is tilted toward
      the sun. It is
      summer in the
      Southern
      Hemisphere
      and winter in
      the Northern
      Hemisphere.
Both in June and
   December
  Summer solstice - longest day
  of the year (June 21).
  Winter solstice - shortest day
  of the year (December 21).
  Both of these are in the
  Northern Hemisphere and the
  opposite in the Southern
  Hemisphere.
Earth in March & September

               Neither
               hemisphere is
               tilted toward or
               away from the
               sun. So the days
               and nights are in
               an equinox which
               is equal.
Earth in March and
    September

   Vernal equinox, or spring
   equinox occurs around March
   21 and is the first day of
   spring.
   Autumnal equinox, or fall
   equinox occurs around
   September 23 and is the first
   day of fall.
Solstices and
Equinoxes
 Solstices occur when the sun
 reaches its greatest distance north
 or south of the equator twice each
 year, each of these days, when the
 sun is the farthest north or south of
 the equator.
 Equinoxes occur twice a year,
 when the noon sun is directly
 overhead at the equator.
Plants and Animals

   Plants and animals are effected by
   the amount of day light hours.
   In the spring and summer, plants
   grow, and animals feed on the
   plants. Insects and animals get
   more food.
   In the winter, animals go dormant
   and birds travel to warmer climates
   to find food.
Reasons for the Seasons
Reasons for the Seasons




         Lab
         Books, Styrofoam balls
         and flashlights.
Gravity and Motion

    Gravity gives the Universe its
    structure
      It is a universal force that
      causes all objects to pull on all
      other objects everywhere
      It holds objects together
      It is responsible for holding the
      Earth in its orbit around the Sun.
Inertia
                Galileo established the idea of inertia
                   A body at rest tends to remain at rest
                   A body in motion tends to remain in motion
                   Through experiments with inclined planes,
                   Galileo demonstrated the idea of inertia
                   and the importance forces (friction)
                This concept was incorporated in
                Newton’s First Law of Motion :



An object at rest will remain at rest, an object in motion
will remain in motion in a straight line, unless acted on
Bike Accident
For a mass on a string to travel in a circle, a force must act
along the string to overcome inertia. Without that force,

inertia makes the mass move in a straight line.
Phases, Eclipses, and
        Tides
Objectives

Describe the causes of the
moon’s phases.
Explain what causes solar and
lunar eclipses.
Identify the cause of the tides.
Engage/Explore

  When does the moon appear?

   Moon Rise and Set
Discover Activity

  How Does the
  Moon Move?
    Quarter &
    penny
    P. 20
Motions of the Moon

     The moon revolves around
     Earth and rotates on its own
     axis.
     It takes 29.5 days to revolve
     around Earth.
     The same side of the moon
     always faces the Earth.
The same side of the moon always
          faces Earth.
Phases of the Moon

    Phases of the moon are seen by
    the reflection of the sun on the
    moon’s surface.
    The different shapes of the moon
    you see from Earth are called
    phases. The moon goes through
    its whole set of phases each time it
    revolves around the Earth, about
    once a month.
What Causes Phases?

    Phases are caused by
    changes in the relative
    positions of the moon, Earth,
    and the sun.
    The phase of the moon you
    see depends on how much of
    the side of the moon faces
    Earth.
The Cycle of the Phases of the
            Moon
Eclipses
When the moon’s shadow hits
Earth or Earth’s shadow hits
the moon, an eclipse occurs.
Two types of eclipses:
solar and lunar
Solar Eclipses
During a new moon, most of the
time the moon is a little above or
below the sun in the sky.
A solar eclipse occurs when the
moon passes between Earth and
the sun, blocking the sunlight from
reaching Earth.
It is really a new moon that blocks
your view of the sun.
Solar Eclipses
Total Solar Eclipses
               Umbra - the
               darkest part of
               the moon’s
               shadow that is
               cone-shaped.
               The point of
               the cone can
               reach a small
               part of Earth’s
               surface.
Partial Solar
 Eclipses
            Penumbra -
            larger part of the
            shadow which is
            more visible on
            Earth. During a
            partial eclipse,
            part of the sun is
            visible.
            It is not safe to
            look at a partial
            eclipse.
Solar Eclipse

   August 11, 1999
Total Lunar Eclipses

                A lunar eclipse
                occurs at a full
                moon when
                Earth is
                between the
                moon and the
                sun. Earth
                blocks sunlight
                from reaching
                the moon.
Total Lunar Eclipse

                 When the moon
                 is in Earth’s
                 umbra, you see a
                 total lunar
                 eclipse. You are
                 more likely to see
                 a total lunar
                 eclipse than a
                 total solar eclipse.
Partial Lunar Eclipses

             Occurs when the
             moon passes
             partly into the
             umbra of Earth’s
             shadow. The
             edge of the
             shadow appears
             blurry and you
             can watch it pass
             across the moon
             for up to two or
             three hours.
Tides
Two high tides and two low tides occur
daily, over 24 hours.
The water rises for about six hours,
then falls for about six hours, in a
regular cycles.
Tides are caused mainly by differences
in how much the moon ‘s gravity pulls
on different parts of earth.
The Tide cycle is representing the two
points of high tides due to the strength
and weakness of the moon’s gravity on
the earth as a whole at those points
causing the tides keeping between
them the other two low tides.
Gravity and Tides
  Low tides occur                 The moon’s gravity
  between the two                 causes high tide on
  high tides.                     the side closest to the
                                  moon.




The force of the
moon’s gravity pulls
Earth toward the
moon, leaving the
water behind
Spring Tides and Neap
        Tides:
        Spring Tides: the
        combined gravity forces
        of the sun and moon
        produce a tide of the
        greatest difference
        between consecutive low
        and high tides, called
        spring tide. It happens
        twice a month, at new
        moon and at full moon.
Neap Tides
    During the moon’s first
    quarter and third
    quarters, the line
    between earth and sun
    is perpendicular on the
    line between earth and
    moon, so the sun’s pull
    at right angles to the
    moon’s pull produces
    the Neap Tides. It
    occurs twice a month.
Section 4, Earth’s Moon
 Maria

            In 1609, The Italian Scientist
              Galileo Galileo succeeded
              to see that the moon has an
              irregular surface with a
              variety of remarkable
              features that are called
              craters (pits), by the help of
              a telescope that built to
    Highlands
              observe distant objects.
The Moon’s Surface
Features on the moon’s surface include Maria, craters,
  and highlands.
  Maria; they are dark, flat areas actually hundred rock
  formed from lava flows from 3 or 4 billion years ago.
  Craters; they were caused by the impacts of
  meteoroids, chunks of rock or dust from space, also
  on Earth, some craters were disappeared due to
  water, wind and other forces for billions of year.
  Highlands; They looked as light-coloured features as
  the peaks of the lunar highlands and the rims of
  craters cast shadows, which Galileo could see by his
  Telescope.
Characteristics of the Moon


       The moon is dry and airless,
       compared to Earth, the moon
       is small and has large
       variations in its surface
       temperature.
Size and Density of the
moon
       Diameter; is 3, 476 km. = ¼
       Earth’s diameter.
       1/8 as much as mass as
       Earth.
       Its average density = density
       of Earth’s outer layers.
       Its core is less denser than
       Earth’s core.
Temperature and Atmosphere

           Temperature on the moon
           vary so much because it has
           no atmosphere.
           It ranges from torrid 130 °C
           in direct sunlight to a frigid
           -180 °C at night.
           The moon surface gravity is
           so weak that gases can
           easily escape into space.
Water

There is evidence that there
may be large patches of ice
near the moon’s poles.
The moon has no liquid water.
Some areas are shielded from
sunlight by crater walls.
The Origin of the Moon

          The moon is formed by “
          Collision- ring theory” that
          says planet-sized objects
          collided with Earth to form
          the moon.
          i.e. materials from the object
          and Earth’s outer layers was
          ejected into orbit around
          Earth, where it is formed a
          ring. Gravity caused these
          materials to combine to form
          the moon.
Ch. 1 Earth, Moon, and Sun

Ch. 1 Earth, Moon, and Sun

  • 2.
    Ch. 1 Earth, Moon,and Sun This amazing Earthrise above the moon's horizon was seen by astronaut Michael Collins in the Apollo 11 moon orbiter Columbia.
  • 3.
    Objectives Identify the effectsof Earth’s rotation and revolution. Explain the causes of the seasons on Earth.
  • 4.
    Section 1, Earthin Space Why Does Earth Have Day and Night?
  • 5.
    Introduction Egyptian farmers planted their crops after the floods every year. They noticed that the star Sirius became visible before the floods. That’s when they could start predicting the floods. The Egyptians were the first people to study the stars.
  • 6.
    Days and Years Astronomy is the study of the moon, stars, and other objects in space.
  • 7.
    Rotation Axis - the imaginary line that passes through Earth’s center and the North and South poles. Rotation - the spinning of Earth on its axis. A point on the equator rotates at about 1,600 km per hour.
  • 8.
    Rotation Earth’s rotation onits axis causes day and night. Earth rotates eastward. It takes 24 hours to rotate once on its axis. This is called a day.
  • 9.
    Revolution Earth also travelsaround the sun. Revolution - the movement of one object around another object. Earth’s orbit is an oval shape.
  • 10.
    Calendars The Egyptians countedthe number of days between Sirius stars which was about 365. Earth’s orbit around the sun is about 365 1/4 days. Four years of 365 1/4 days each can be approx. by taking 3 years of 365 days and a fourth year of 366 days. This is known as leap year. On a leap year, one extra day in February is added for 29 days.
  • 11.
    Calendars Dividing the yearinto smaller parts (months) was difficult. Early people used the moon cycle which is 29 1/2 days but this only added up to 354. The Egyptians had a plan to have 12 months of 30 days and 5 extra days. The Romans borrowed the calendar and devised the one that we have today with 11 months of 30 to 31 days and February with 28 or 29 days.
  • 12.
    Seasons on Earth Most places have four seasons: winter, spring, summer, and autumn.
  • 13.
    Earth’s Tilted Axis Earth has seasons because its axis is tilted as it moves around the sun.
  • 14.
    Earth in June The north end of Earth’s axis is tilted toward the sun. It is summer in the Northern Hemisphere and winter in the Southern Hemisphere.
  • 15.
    Earth in December The south end of Earth’s axis is tilted toward the sun. It is summer in the Southern Hemisphere and winter in the Northern Hemisphere.
  • 16.
    Both in Juneand December Summer solstice - longest day of the year (June 21). Winter solstice - shortest day of the year (December 21). Both of these are in the Northern Hemisphere and the opposite in the Southern Hemisphere.
  • 17.
    Earth in March& September Neither hemisphere is tilted toward or away from the sun. So the days and nights are in an equinox which is equal.
  • 18.
    Earth in Marchand September Vernal equinox, or spring equinox occurs around March 21 and is the first day of spring. Autumnal equinox, or fall equinox occurs around September 23 and is the first day of fall.
  • 19.
    Solstices and Equinoxes Solsticesoccur when the sun reaches its greatest distance north or south of the equator twice each year, each of these days, when the sun is the farthest north or south of the equator. Equinoxes occur twice a year, when the noon sun is directly overhead at the equator.
  • 20.
    Plants and Animals Plants and animals are effected by the amount of day light hours. In the spring and summer, plants grow, and animals feed on the plants. Insects and animals get more food. In the winter, animals go dormant and birds travel to warmer climates to find food.
  • 21.
  • 22.
    Reasons for theSeasons Lab Books, Styrofoam balls and flashlights.
  • 23.
    Gravity and Motion Gravity gives the Universe its structure It is a universal force that causes all objects to pull on all other objects everywhere It holds objects together It is responsible for holding the Earth in its orbit around the Sun.
  • 24.
    Inertia Galileo established the idea of inertia A body at rest tends to remain at rest A body in motion tends to remain in motion Through experiments with inclined planes, Galileo demonstrated the idea of inertia and the importance forces (friction) This concept was incorporated in Newton’s First Law of Motion : An object at rest will remain at rest, an object in motion will remain in motion in a straight line, unless acted on
  • 25.
  • 27.
    For a masson a string to travel in a circle, a force must act along the string to overcome inertia. Without that force, inertia makes the mass move in a straight line.
  • 28.
  • 29.
    Objectives Describe the causesof the moon’s phases. Explain what causes solar and lunar eclipses. Identify the cause of the tides.
  • 30.
    Engage/Explore Whendoes the moon appear? Moon Rise and Set
  • 31.
    Discover Activity How Does the Moon Move? Quarter & penny P. 20
  • 32.
    Motions of theMoon The moon revolves around Earth and rotates on its own axis. It takes 29.5 days to revolve around Earth. The same side of the moon always faces the Earth.
  • 33.
    The same sideof the moon always faces Earth.
  • 34.
    Phases of theMoon Phases of the moon are seen by the reflection of the sun on the moon’s surface. The different shapes of the moon you see from Earth are called phases. The moon goes through its whole set of phases each time it revolves around the Earth, about once a month.
  • 35.
    What Causes Phases? Phases are caused by changes in the relative positions of the moon, Earth, and the sun. The phase of the moon you see depends on how much of the side of the moon faces Earth.
  • 36.
    The Cycle ofthe Phases of the Moon
  • 37.
    Eclipses When the moon’sshadow hits Earth or Earth’s shadow hits the moon, an eclipse occurs. Two types of eclipses: solar and lunar
  • 38.
    Solar Eclipses During anew moon, most of the time the moon is a little above or below the sun in the sky. A solar eclipse occurs when the moon passes between Earth and the sun, blocking the sunlight from reaching Earth. It is really a new moon that blocks your view of the sun.
  • 39.
  • 40.
    Total Solar Eclipses Umbra - the darkest part of the moon’s shadow that is cone-shaped. The point of the cone can reach a small part of Earth’s surface.
  • 41.
    Partial Solar Eclipses Penumbra - larger part of the shadow which is more visible on Earth. During a partial eclipse, part of the sun is visible. It is not safe to look at a partial eclipse.
  • 42.
    Solar Eclipse August 11, 1999
  • 43.
    Total Lunar Eclipses A lunar eclipse occurs at a full moon when Earth is between the moon and the sun. Earth blocks sunlight from reaching the moon.
  • 44.
    Total Lunar Eclipse When the moon is in Earth’s umbra, you see a total lunar eclipse. You are more likely to see a total lunar eclipse than a total solar eclipse.
  • 45.
    Partial Lunar Eclipses Occurs when the moon passes partly into the umbra of Earth’s shadow. The edge of the shadow appears blurry and you can watch it pass across the moon for up to two or three hours.
  • 46.
    Tides Two high tidesand two low tides occur daily, over 24 hours. The water rises for about six hours, then falls for about six hours, in a regular cycles. Tides are caused mainly by differences in how much the moon ‘s gravity pulls on different parts of earth. The Tide cycle is representing the two points of high tides due to the strength and weakness of the moon’s gravity on the earth as a whole at those points causing the tides keeping between them the other two low tides.
  • 47.
    Gravity and Tides Low tides occur The moon’s gravity between the two causes high tide on high tides. the side closest to the moon. The force of the moon’s gravity pulls Earth toward the moon, leaving the water behind
  • 48.
    Spring Tides andNeap Tides: Spring Tides: the combined gravity forces of the sun and moon produce a tide of the greatest difference between consecutive low and high tides, called spring tide. It happens twice a month, at new moon and at full moon.
  • 49.
    Neap Tides During the moon’s first quarter and third quarters, the line between earth and sun is perpendicular on the line between earth and moon, so the sun’s pull at right angles to the moon’s pull produces the Neap Tides. It occurs twice a month.
  • 50.
    Section 4, Earth’sMoon Maria In 1609, The Italian Scientist Galileo Galileo succeeded to see that the moon has an irregular surface with a variety of remarkable features that are called craters (pits), by the help of a telescope that built to Highlands observe distant objects.
  • 51.
    The Moon’s Surface Featureson the moon’s surface include Maria, craters, and highlands. Maria; they are dark, flat areas actually hundred rock formed from lava flows from 3 or 4 billion years ago. Craters; they were caused by the impacts of meteoroids, chunks of rock or dust from space, also on Earth, some craters were disappeared due to water, wind and other forces for billions of year. Highlands; They looked as light-coloured features as the peaks of the lunar highlands and the rims of craters cast shadows, which Galileo could see by his Telescope.
  • 52.
    Characteristics of theMoon The moon is dry and airless, compared to Earth, the moon is small and has large variations in its surface temperature.
  • 53.
    Size and Densityof the moon Diameter; is 3, 476 km. = ¼ Earth’s diameter. 1/8 as much as mass as Earth. Its average density = density of Earth’s outer layers. Its core is less denser than Earth’s core.
  • 54.
    Temperature and Atmosphere Temperature on the moon vary so much because it has no atmosphere. It ranges from torrid 130 °C in direct sunlight to a frigid -180 °C at night. The moon surface gravity is so weak that gases can easily escape into space.
  • 55.
    Water There is evidencethat there may be large patches of ice near the moon’s poles. The moon has no liquid water. Some areas are shielded from sunlight by crater walls.
  • 56.
    The Origin ofthe Moon The moon is formed by “ Collision- ring theory” that says planet-sized objects collided with Earth to form the moon. i.e. materials from the object and Earth’s outer layers was ejected into orbit around Earth, where it is formed a ring. Gravity caused these materials to combine to form the moon.