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Earth and its Moon

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Equinox. Twice a year neither hemisphere is tilted toward the sun. ... Autumn begins on September 22 or 23, the autumnal equinox. A Magnet in Space ... – PowerPoint PPT presentation

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Title: Earth and its Moon


1
Earth and its Moon
2
The Earth in Space
  • The Earth revolves around the sun.
  • The Earth rotates on its axis.
  • These two combined movements affect both day and
    night and the seasons on Earth.

3
Day and Night
  • The Earths rotation causes day and night every
    24 hours.
  • The Earth rotates in a counterclockwise pattern (
    west to east) causing the sun to appear to rise
    in the east and set in the west.
  • Since the Earths axis is tilted when the North
    Pole is leaning toward the sun, the South Pole is
    leaning away.
  • The hemisphere that leans toward the sun has long
    days and short nights.

4
A Year on Earth
  • The Earth takes 365.25 days to complete the
    revolution around the sun.
  • An extra day is added to the calendar every four
    years in February.
  • This is called a leap year.

5
Seasons on Earth
  • The Earth has four seasons winter, spring,
    summer and autumn.
  • Five of the other planets, Mars, Saturn, Uranus,
    Neptune and possibly Pluto.
  • The other planets, Mercury, Venus and Jupiter, do
    not have seasons since they are not tilted on
    their axis.

6
Seasons
  • When the Northern Hemisphere is tilted toward the
    sun, that part of the Earth has summer since the
    suns rays are more direct and the days are
    longer.
  • At the same time, the Southern Hemisphere is
    tilted away and has winter.
  • Summer and winter are not affected by the
    distance from the sun.

7
Solstices
  • Summer begins in the Northern Hemisphere on June
    20 or 21.
  • The summer solstice is the longest day of the
    year.
  • The winter solstice is the shortest day of the
    year.
  • When the Northern Hemisphere has the longest day,
    the Southern Hemisphere has the shortest day.

8
Equinox
  • Twice a year neither hemisphere is tilted toward
    the sun. These times are known as equinoxes.
  • Spring begins on March 20 or 21, the vernal
    equinox.
  • Autumn begins on September 22 or 23, the autumnal
    equinox.

9
A Magnet in Space
  • The Earths magnetism is probably the result of
    movement of the materials in the Earths inner
    core, which is made mainly of iron and nickel.
  • The Earth is surrounded by lines of force.
  • The magnetic poles are not in the same location
    as the geographic poles.

10
Magnetosphere
  • The Earths magnetic field is called the
    magnetosphere.
  • The magnetic field starts at an altitude of 1000
    km and extends to an altitude of 64,000 km on
    the side facing the sun.
  • On the side facing away from the sun, the
    magnetosphere extends in a long tail caused by
    solar winds blowing away from the sun.

11
Van Allen Radiation Belts
  • Two doughnut shaped regions of charged particles
    are formed as the magnetosphere traps some of the
    particles in the solar wind.
  • The outer belt contains mostly electrons, or
    negatively charged particles.
  • The inner belt contains mainly protons, or
    positively charged particles.

12
Auroras
  • Charged particles that are trapped by the Van
    Allen belt travel along line of force to the
    Earths poles.
  • Here they collide with particles of the upper
    atmosphere and produce an aurora.
  • The aurora borealis is located at the North Pole
    and the aurora australis is at the South Pole.

13
The Earths Moon
  • Neil Armstrong was the first man to step on the
    moon.
  • Buzz Aldrin and Armstrong landed on the moon in
    the lunar module, the Eagle.
  • Michael Collins, stayed in the command module,
    the Columbia.
  • By 1973, 12 Americans had explored the moons
    surface.

14
The Moons Characteristics
  • The moons diameter is 1/4 of the Earth.
  • The moons gravity is 1/6 of the Earth.
  • The moon is 384,403 km from the Earth.
  • The moon does not have an atmosphere or weather.
  • The temperature is extreme from 100 degrees
    Celsius to 175 degrees.

15
Composition of the Moon
  • Instruments have measured moonquakes.
  • The crust is 60 km thick.
  • Beyond the crust is a dense layer of rock that is
    800 km thick.
  • The central core is made of melted iron.

16
Features of the Moon
  • In 1609, Galileo looked at the moon with a
    telescope. He called the lowlands, Maria.The
    highlands reach to a height of 8 km.
  • Most of the craters are in the highlands. One of
    the largest is Copernicus, which is 91 km in
    diameter.
  • Most craters were formed by meteorites.
  • Rilles, evidence of volcanic activity, crisscross
    the surface.

17
Movements of the Moon
  • Perigee is the point of the moons orbit
    closest to the Earth. The apogee is the point of
    the moons orbit farthest from the Earth.
  • The moons period of rotation is the same as the
    period of revolution so the same side of the moon
    always faces the Earth.

18
Origin of the Moon
  • One theory states that the moon was formed
    millions of kilometers from the Earth and
    captured by its gravity.
  • The moon may have been formed in the nebular
    cloud in which the Earth formed.
  • The moon may have been born when a giant
    asteroid struck the Earth and tore a huge chunk
    away, leaving a hole.

19
The Earth, the Moon and the Sun
  • As the Earth moves in its yearly revolution
    around the sun, the moon moves in a monthly
    revolution around the Earth.At the same time both
    rotate.
  • The motion of these three result in the changing
    appearance of the moon as seen from the Earth and
    the blocking of light.

20
Phases of the Moon
  • The moon goes through all of its phases every
    29.5 days. The moon reflects sunlight toward the
    Earth.
  • The moon has 8 phases.
  • The moon is said to be waxing when the lighted
    area grows larger and waning when the lighted
    area appears to grow smaller.

21
New and Waxing Moon
  • A new moon occurs when the moon comes between the
    sun and Earth and the side of the moon facing
    Earth is in darkness.One week later at First
    quarter moon, ½ of the moon appears lighted.
  • Two weeks after the new moon, a full moon is
    visible and the Earth is between the moon and the
    sun.

22
Waning and New Moon
  • The moon takes another two weeks to go through
    the waning-gibbous, last quarter and waning
    crescent phases.
  • The moon then stars all over again as a new moon.

23
Solar Eclipse
  • A solar eclipse occurs when the new moon comes
    directly between the sun and the Earth.
  • The people in the umbra of the shadow see a total
    solar eclipse.
  • The people in the penumbra, the larger outer
    shadow, see a partial solar eclipse.

24
Lunar Eclipse
  • A lunar eclipse occurs when the moon passes
    through the Earths shadow.
  • When the moon moves through the umbra, a total
    lunar eclipse occurs.
  • When the moon moves through the penumbra, a
    partial lunar eclipse occurs.

25
Moon Earth
  • As a result of the Earths gravitational pull on
    the moon, the side that faces Earth has a bulge.
  • The moons gravitational pull on Earth results in
    the rise and fall of the oceans, known as the
    tides.

26
Tides
  • The moons gravity causes the oceans to bulge in
    two places, the side facing the moon and the side
    facing away. This results in high tide.
  • Low tides occur between the two bulges.
  • There are two high tides and two low tides every
    24 hours.

27
Spring Tides
  • During the full moon and the new moon phases, the
    high tides are higher than at other times. These
    are called spring tides.
  • Spring tides occur because the sun and the moon
    are in a direct line with the Earth.

28
Neap Tides
  • When the moon is at the first and last quarter
    phases, its gravitational pull on the oceans is
    partially cancelled by the suns gravitational
    pull. This results is lower high tides called
    neap tides.
  • The varying distance between the Earth and moon
    due to the moons orbit also affects the tides. A
    perigee will cause extremely high tides.

29
The Space Age
  • On October 4, 1957 Sputnik I was the first
    artificial satellite to orbit the Earth.
  • Vanguard (Stayputnik), the United States first
    attempt was not successful.

30
Artificial Satellites
  • Communications
  • Weather
  • Navigation
  • Scientific

31
Communication Satellites
  • Communication satellites bean television
    programs, radio messages, and telephone
    conversations.
  • The satellites receives a signal from a
    transmitting station on Earth and relays it to a
    receiving station in another location on Earth.
    They are often in geosynchronous orbit with the
    Earth.

32
Weather Satellites
  • Weather satellites have made prediction more
    accurate.

33
Navigation Satellites
  • Navigation satellites can tell the exact position
    of ships, airplanes and cars within seconds.

34
Scientific Satellites
  • The Explorer I, the first United States
    satellite, discovered the Van Allen radiation
    belt.
  • The Infrared Astronomy Satellites (IRAS) found
    evidence of a black hole in the Milky Way galaxy
    as well as planetary systems forming around
    distant stars.
  • The Upper Atmosphere Research Satellite (URAS)
    studies the ozone layer.

35
Laboratories in Space
  • In 1973, the United States launched Skylab, and
    later Space Lab.
  • In 1986, the Soviets launched Mir.
  • Today we have the International Space Station.

36
Space Technology Spin-offs
  • Heart pacemakers
  • Lightweight tennis rackets
  • Fabric that can withstand extreme temperatures
    and still be flexible
  • Gel packs to draw excess heat away from humans
  • Monitoring devices for vital statistics
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