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Unit 2: Earth in Space

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Terminology Frame of Reference: a fixed background which we can measure motions against P.O.V. Polaris: the North Star directly above Earth s North Pole/axis of ... – PowerPoint PPT presentation

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Title: Unit 2: Earth in Space


1
Unit 2 Earth in Space
  • Terminology
  • Frame of Reference a fixed background which we
    can measure motions against
  • P.O.V.
  • Polaris the North Star directly above Earths
    North Pole/axis of rotation
  • Celestial Object an object outside of Earths
    atmosphere
  • Stars, our Sun, Valenti in a space suit orbiting
    earth, other planets

2
  • a) Angular Diameter how large a celestial
    object appears to be to an observer
  • It depends on
  • The objects actual size
  • How far it is from the observer
  • Earths Motions in Space
  • Rotation Earth spins on its axis once every 24
    hours
  • Earth turns 15o/hour from west to east-
  • -how do we know?
  • Day and night- either the sun actually rises
    and sets or Earth rotates

3
  • Revolution (orbit) Earth moves around the sun
    in a nearly circular orbit
  • Earth orbits the sun in 365.25 days-
  • -how do we know?
  • Star Shift- constellations appear to change
    position each night (slightly)
  • This is why we see different constellations
    during different seasons we see different views
    or snapshots at different times

Sun
4
  • Seasons and Earth-Sun Relationships
  • The Seasons are a result of 3 factors
  • Tilted axis of rotation- 23.5o
  • Revolution around the sun
  • Parallelism- earths axis always point to the
    same place in space
  • It points at the North Star (Polaris)

Polaris
5
  • Season Characteristics
  • September 21- Autumnal/Fall Equinox
  • Direct rays of the sun hit the Equator (0o)
  • Because of where we are in space, tilt is neither
    towards or away from sun
  • Everywhere on Earth has 12 hours of
    daylight/night
  • EQUAL on an EQUInox

0o
6
  • December 21- Winter Solsitice
  • Direct rays of the sun hit the Tropic of
    Capricorn (23.5o S latitude)
  • Because of where we are in space, Northern
    Hemisphere is tilted AWAY from the sun
  • In NYS, we have 8 hours of daylight/16 hours of
    night
  • Shortest day of the year
  • Travel north towards the North Pole you approach
    locations of 24 hours of night (Artic Circle to
    the North Pole)

7
  • March 21- Vernal/Spring Equinox
  • With the exception of the date and name, its the
    same as its twin the Autumnal Equinox!

0o
8
  • June 21- Summer Solstice
  • Direct rays of the sun hit the Tropic of Cancer
    (23.5o N latitude)
  • Because of where we are in space, Northern
    Hemisphere is tilted TOWARD the sun
  • In NYS, we have 16 hours of daylight/8 hours of
    night
  • Longest day of the year
  • Travel north towards the North Pole you approach
    locations of 24 hours of daylight (Artic Circle
    to the North Pole)

9
  • Observing our Moon
  • It takes the moon about one month (29.5 days) to
    go through a complete cycle of phases
  • The moons period of rotation and revolution are
    the same
  • We always see the same side of the moon facing
    the Earth
  • Moon Phases- the amount of lit surface as seen
    from Earth
  • Phases are caused by the moons revolution
  • The angle and set up of SUN, EARTH and MOON
    determines what phase we see

10
  • Phases repeat every month in a cyclic manner
  • Waxing/1st/New Phases- to see more of the moon
    each night
  • when the light is on the right, the moon is
    getting bright
  • New Moon to Full Moon
  • Waning /3rd/Old Phases- to see less of the moon
    each night
  • Waning Fading away
  • Getting dark on the right, the moon is getting
    erased


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15
  • Moons Affect on Earth
  • The moons gravity affects our hydrosphere
  • Tides are created by the pull of the moon on
    the oceans
  • There are 4 changes in tides in 24 hours
  • 2 high tides
  • 2 low tides
  • This means every 6 hours the level of the oceans
    change (from high to low OR from low to high)
  • Special Tides
  • Spring Tides (Severe high and low tides)
  • Happens when the moon is Full or New
  • Moon and Sun work together to pull on the
    oceans making height of tides more extreme

16
The Moons Gravity Causes a change in our tidal
levels throughout the day
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18
  • Eclipses
  • Lunar Eclipse- Earths shadow is cast on the
    surface of a Full Moon
  • Sun, Earth and moon align exactly in this order
  • Happens during a FULL MOON ONLY
  • Relatively common (about every 18 months)
  • Safe to view
  • Visible to everyone on the nighttime side of
    Earth
  • Solar Eclipse- Moons shadow is cast on the
    surface of the Earth
  • Sun, Moon and Earth align exactly in this order
  • Happens during a NEW MOON ONLY
  • Rare (about 1 every 7 to 10 years)
  • Dangerous to view (burns your retinal nerve in
    your eyes (youd go blind)
  • Visible to only certain locations/latitudes on
    Earth (you must be located at the right spot on
    the daytime side of Earth to experience a solar
    eclipse)

19
Lunar Eclipse How do the Sun, Earth and moon
align to create this common celestial phenomenon?
20
Solar Eclipse How do the Sun, Earth and Moon
align to create this more rare phenomenon?
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