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Lecture 6

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Earth and The Solar System
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Earth and Space Earth and Space
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Page 1: Lecture 6

Earth and SpaceEarth and Space

Page 2: Lecture 6

Earth’s Vital StatisticsEarth’s Vital Statistics

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 3: Lecture 6

Locating Places on the EarthLocating Places on the Earth

Reference lines (imaginary lines) Equator – line that equally divides the earth into upper and lower hemispheres

Latitude –horizontal line drawn with respect to the equator Adams and Lambert. Earth Science: An Illustrated Guide To

Science, 2006. NY: Chelsea House

Page 4: Lecture 6

Locating Places on the EarthLocating Places on the Earth

Reference lines (imaginary lines) Prime Meridian – line that equally divides the earth into left and right hemispheres

Longitude –vertical line drawn with respect to the prime meridian

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 5: Lecture 6

How to tell direction?How to tell direction?

Example: Manila: 14o N; 120oE

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 6: Lecture 6

Key Latitudes and LongitudeKey Latitudes and Longitude

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 7: Lecture 6

Earth’s RotationEarth’s Rotation

Counterclockwise (East to West) Results to day and night

One complete rotation = 24 hours

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 8: Lecture 6

Standard Time ZoneStandard Time Zone

Divides the globe into 24 time zones 180o WEST and EAST of the prime meridian (0o) Each time zone covers 15o longitudes a 1 time zone = 1 hour Important consideration: West or East

ExampleManila: 120o East

Page 9: Lecture 6

Standard Time ZoneStandard Time Zone

http://www.mapsofworld.com/time-zone-map/maps/world-time-zone.jpg

Page 10: Lecture 6

Standard Time ZoneStandard Time Zone

International date line Passing thorough this lineprompts addition/subtraction of 24 hours exactly opposite of the prime meridian (0o longitude) @ 180o)

http://upload.wikimedia.org/wikipedia/

commons/6/61/International_Date_Line.png

Page 11: Lecture 6

Solar SystemSolar System

is composed of one star (Sun), planets and their natural satellites (moons), and other heavenly objects

they ALL revolve around the sun Sun is the center of the solar system

Page 12: Lecture 6

Solar System Solar System

http://www.infoplease.com/spot/solar-system.html

Page 13: Lecture 6

SunSun

It is a star The closest star from the earth or other objects in the solar system

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 14: Lecture 6

Energy of the sunEnergy of the sun

• Comes from the fusion of Hydrogen gas to helium

• Occurs in the sun’s core

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 15: Lecture 6

PlanetsPlanets

IAU (Aug. 24, 2006) criteria: The object must be in orbit around the sun It must be the only object that “use” its orbit Spherical in shape due to gravity

Page 16: Lecture 6

Solar System Solar System

http://www.infoplease.com/spot/solar-system.html

Page 17: Lecture 6

Why was Pluto demoted?Why was Pluto demoted?

IAU (Aug. 24, 2006) criteria: The object must be in orbit around the sun It must be the only object that use its orbit Spherical in shape due to gravity

Page 18: Lecture 6

Planetary MotionsPlanetary Motions

Rotation on its axis Revolution around the sun

Page 19: Lecture 6

RevolutionRevolution

One complete revolution around the sun = 1 year

Follows a track = railway = orbit Each planet has their own orbit

Page 20: Lecture 6

Earth’s OrbitEarth’s Orbit

Gravity pull of the sunKeeps the earth from straying away from its Orbit.

gravity vs. inertia

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 21: Lecture 6

Earth’s OrbitEarth’s Orbit

elliptical in shape

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 22: Lecture 6

Moons in the solar systemMoons in the solar system

Planet No. of MoonsMercury 0

Venus 0

Earth 1

Mars 2

Jupiter 62

Saturn 33

Uranus 27

Neptune 13

http://www.spacetoday.org/SolSys/Moons/MoonsSolSys.html

Page 23: Lecture 6

Earth’s MoonEarth’s Moon

Rotates on its axis No light of its own

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 24: Lecture 6

EclipsesEclipses

When shadow of a heavenly body falls on another

Solar/Lunar eclipse Partial/Total Eclipse

Page 25: Lecture 6

Solar EclipseSolar Eclipse

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 26: Lecture 6

Solar EclipseSolar Eclipse

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 27: Lecture 6

Lunar EclipseLunar Eclipse

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 28: Lecture 6

Lunar EclipseLunar Eclipse

Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

Page 29: Lecture 6

Other heavenly objectsOther heavenly objects

Asteroids belt – found between Mars and Jupiter

Comets Meteoroids Meteor Meteorite

Page 30: Lecture 6

Beyond solar systemBeyond solar system

Solar system is part of the Milky way galaxy Galaxy = billions of stars that move around

through space as one unit

Page 31: Lecture 6

StarsStars

Huge ball of flaming gas Has a life cycle constellations

http://www.tepapa.govt.nz/space/Images/star_constellations3.gif

Page 32: Lecture 6

ReferencesReferences

• Adams and Lambert. Earth Science: An Illustrated Guide To Science, 2006. NY: Chelsea House

• Rabago, Lilia M., et al. Dynamic Science. 2003. QC: vibal Publishing House


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