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Earth in Space

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Earth in Space Astronomy; Science Explorer, Prentice Hall Why does the Earth have day and night? Astronomy: the study of the moon, stars, and other objects in space ... – PowerPoint PPT presentation

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Title: Earth in Space


1
Earth in Space
  • Astronomy Science Explorer, Prentice Hall

2
Why does the Earth have day and night?
  • Astronomy the study of the moon, stars, and
    other objects in space
  • Axis the imaginary line that passes through the
    Earths center and the North and South poles at
    an angle of 23.5º Polaris is the North Star.
  • Rotation Earths spinning on its axis A point
    on the equator spin at 1600 km/hr
  • Earths rotation causes day and night

3
Whats in a day?
  • In what cardinal direction does Earth rotate?
  • Where does the sun appear to set?
  • How many hours does one rotation take?
  • How are daytime and nighttime defined?
  • Think about it Why do the sun and moon appear to
    move each day?

4
3rd Rock From the Sun
  • In addition to rotating on its axis, Earth
    travels around the sun, our closest star.
  • Revolution the movement of one object around
    another object
  • Orbit the elliptical (or oval) path of
    revolution around the sun
  • Think about it How long does one trip around the
    sun take?

5
The Calendar
  • 1500 B.C., British Isles
  • Stonehenge build by ancient people
  • Giant stones mark directions in which the sun
    rises and sets on the longest day of the year

6
The Calendar
  • 1300 B.C., China
  • During the Shang dynasty, Chinese astronomers
    calculated the length of a year is 365.25 days.
  • 300 B.C., Egypt
  • Egyptian astronomers counted the numbers of days
    between the first appearance of the star Sirius.
    Sirius appeared before the Niles spring floods.
    There were about 365 days.

7
The Calendar
Chichen Itza El Caracol (Mayan Observatory)
  • 900 A.D., Mexico
  • Mayan astronomers studied the sun, moon, and
    Venus. Their calendar had 365 days.
  • The Mayans were also able to predict astronomical
    events 3000 years in the future.

8
The Calendar
  • A.D. 1450, Wyoming, USA
  • Big Horn Medicine Wheel built by Native
    Americans. Individual stones are aligned with
    rising and setting of sun and stars. Used to
    determine migration times.

9
The Calendar
  • Earths orbit around the sun takes slightly more
    that 365 days 365 ¼ days
  • Leap year was created to compensate. Every four
    years the years has 366 days.
  • The time between two full moons is about 29 ½
    days. Hence the month (moonth).
  • Romans altered Egyptian calendar of 12 30-day
    months (360 5 days) to the one currently used.

10
Seasons on Earth
11
Seasons on Earth
  • The Earth is warmer at the equator and cooler at
    the poles. The equator receives the most direct
    sunlight. The poles receive sunlight at an
    angle.

12
Seasons on Earth
  • Earth has seasons due to the 23.5 degree tilt of
    its axis as Earth moves around the sun.
  • When does the Northern Hemisphere have summer?
    Winter?
  • Why do the Northern and Southern Hemispheres have
    opposite seasons?
  • Which areas on Earth do not experience a change
    of season?

13
Seasons Vocabulary
  • Latitude measurement of distance from the
    equator, expressed in degrees north or south
    (equator 0º, North Pole 90º)
  • Summer Hemisphere has more direct sunlight and
    more hours of daylight winter is the opposite.
  • Solstice The two days each year when the noon
    sun is overhead at 23.5º south (winter) or 23.5º
    north (summer). For the Northern Hemisphere,
    summer solstice is June 21 and winter solstice is
    Dec. 21.
  • Southern Hemisphere?

14
Seasons Vocabulary
  • Equinox Halfway between the solstices, the noon
    sun is directly over the equator for one day.
    Means equal night. Day and night are the same
    length.
  • Vernal equinox (spring) Around March 21 for the
    Northern Hemisphere.
  • Autumnal equinox (fall) Around Sept. 23 for the
    Northern Hemisphere.

15
Phases, Eclipses, and Tides
16
Motions of the Moon
  • The moon revolves around Earth in 29.5 days.
  • The moon also completes one rotation in 29.5
    days.
  • The moon day is the same length as the moon year
    and is approximately one month on Earth.
  • The moon has an elliptical orbit.

17
Phases of the Moon
  • Why can you observe the moon in the sky at night?
  • The moon takes many shapes round circle, thin
    sliver, crescent shape.
  • Phases Different shapes of the moon
  • The moon goes through all of its phases each
    month (1 revolution).

18
What Causes the Phases?
  • Because the sun lights the moon, half of the moon
    is almost always in sunlight.
  • However, the half of the moon facing the Earth is
    not always the half that is reflecting sunlight.
  • The phase of the moon depends on how much of the
    sunlit side of the moon faces Earth.

19
Phases of the Moon
20
The Eight Phases
  • New Moon (dark)
  • Waxing Crescent
  • First Quarter (half lighted)
  • Waxing Gibbous
  • Full Moon (fully lighted)
  • Waning Gibbous
  • Third Quarter (half lighted)
  • Waning Crescent
  • About 29.5 days later New Moon again

21
1999, Salzburg - Austria
22
Eclipses
  • What causes an Eclipse?
  • Eclipse an object (moon) in space comes between
    the sun and a third object (Earth), casting a
    shadow on the third object.
  • Solar and Lunar Eclipses
  • Why are eclipses rare?
  • The moons orbit is slightly tilted with respect
    to the Earths orbit around the sun. The moons
    shadow rarely hits Earth and Earths shadow
    rarely covers the moon.

23
(No Transcript)
24
Solar Eclipses
  • Solar Eclipse the new moon passes between the
    Earth and the sun blocking the sunlight (during
    the day)
  • Umbra Darkest part of moons shadow cone-shaped
  • Small part of Earth experiences a total solar
    eclipse
  • Penumbra Lighter part of moons shadow part of
    sun is visible
  • Larger part of Earth experiences a partial solar
    eclipse (Do not look directly at a partial solar
    eclipse.)

25
Lunar Eclipse sequence from 28th August 2007
taken with SkyWatcher ED100 refractor and Canon
PowerShot compact camera.by Steve Massey
26
(No Transcript)
27
Lunar Eclipses
  • Lunar Eclipse during a full moon the Earth
    passes directly between the moon and the sun
    Earths shadow blocks sunlight from hitting the
    moon
  • Umbra total lunar eclipse occurs
  • Penumbra partial lunar eclipse occurs
  • A lunar eclipse can be observed from anywhere on
    Earth (unlike a solar eclipse)

28
The Tides
  • Tides The rise and fall of the water
    approximately every 12.5 hours The water rises
    for 6 hours and then falls for 6 hours twice a
    day, in a regular cycle.
  • Tides occur because of differences in the force
    of gravity between the moon and different parts
    of Earth
  • Force of Gravity Depends on the mass and
    distance between two objects

29
A The moons gravity pulls the oceans more
strongly than the Earth. The oceans are drawn
towards the moon creating high tide.
C
A
B
B The moons gravity pulls the Earth more
strongly than the oceans. The oceans are left
behind creating a second high tide.
C D Water flowing towards the high tides and
away from points C and D creates low tides.
D
30
The Tide Cycle
  • There are always two high tides and two low tides
    occurring on Earth.
  • Why does Ocean City Beach experience two high
    tides in one day?

31
Spring and Neap Tides
  • Spring Tides The highest high tide The tide
    with the greatest difference between high and low
    occurs when the sun, moon, and Earth line up.
    The gravitational pull of the sun and moon
    combine forces.
  • Neap Tides The tide with the least difference
    between high and low occurs when the
    gravitational pull of the sun and moon are at
    right angles.
  • How many times a month do Spring and Neap Tides
    occur? During which phases?

32
Spring and Neap Tides
33
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