Astronomy
Eccentricity and Motions of the Earth
Summative part 2
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Johannes Kepler
Kepler found flaws in the Heliocentric model of the solar system.
Continue
Johannes Kepler
The planets could NOT be traveling in perfect circles around the Sun.
Continue
Johannes Kepler
He developed three laws known as Kepler’s Laws of Planetary Motion
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Kepplers Laws
Third Law
Second Law
First Law
(Law of Areas) As a planet moves around the Sun in its orbit, it covers equal areas in equal time. (changes speed)
(Law of Orbits) The orbit of each planet around the Sun is an ellipse. The Sun is at one focus.
(Law of Periods) The time it takes a planet to complete one orbit around the Sun is related to its average distance from the Sun. (p2 = a3, p = time, a = dist. from sun)
Continue
Eccentricity
Eccentricity is how flat or circular an ellipse is.
It ranges from 0 – 1
0 = circle
1 = line
Earth’s orbit has an eccentricity value of 0.017. This tells us that Earth’s orbit is nearly circular.
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EdPuzzle Time
Axial Tilt
The Earth’s axis of rotation is now tilted 23.5˚.
These changes in the axial tilt is believed to be the cause for Ice Ages.
Over 41,000 years the tilt varies from 22.1˚ to 24.5˚
Continue
Google Classroom Complete the Activity
Motions of Earth
Rotation – spinning of a body on its axis
Causes day and night 24 hour period (time zones)
Continue
Motions of Earth
Revolution – object traveling along a path around some point in space
365.25 days
Continue
Motions of Earth
Perihelion – when the earth is closest to the sun (Jan. 3)
Aphelion – when the earth is furthest from the sun (July 4)
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Motions of Earth
Ecliptic – The apparent annual path of the Sun against the backdrop of the celestial sphere
Continue
Google Classroom Complete the Activity
Continue
Astronomy
Solstice and Equinox
Summative part 2
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Equinox
Solstice
Autumnal Equinox – Sep. 23
- Night and day are same length
- First day of fall
Spring Equinox - March 21
- Night and day are same length
- First day of spring
Winter Solstice – Dec. 21
- The Sun is the lowest in the sky
- Shortest day of the year
- First day of winter
- Tropic of capricorn (23.5°S)
Summer Solstice – June 21 –
- The Sun is the highest in the sky (N.H)
- longest day of the year
- First day of summer
- Tropic of cancer (23.5° N) – Sun directly overhead (zenith)
Continue
Continue
Continue
Precession
The Earth wobbles like a spinning top.
This wobbling is called precession.
This is caused by the gravitational pull of the Moon and the Sun
It takes 25,725 years for the Earth to wobble through one complete cycle.
Continue
Continue
Orbital Precession
The Earth’s orbit is revolving around the Sun.
This is called the orbital precession.
Continue
Combined Effects
The combined effects of the axial and orbital precessions will make our seasons as we know them today more extreme.
Winters will be colder
Summers will be hotter.
Continue
Inclination
Orbital plane – the first 8 planets are all fixed in the same plane.
Pluto however is tilted 17.1˚ from the rest of the planets.
This tilt is called inclination.
Continue
Continue
Google Classroom Complete the Activity Goal = 80%
Continue
Astronomy
Summative
Summative part 2
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Astronomy summative 2
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Transcript
Astronomy
Eccentricity and Motions of the Earth
Summative part 2
Let's go!
Johannes Kepler
Kepler found flaws in the Heliocentric model of the solar system.
Continue
Johannes Kepler
The planets could NOT be traveling in perfect circles around the Sun.
Continue
Johannes Kepler
He developed three laws known as Kepler’s Laws of Planetary Motion
Continue
Kepplers Laws
Third Law
Second Law
First Law
(Law of Areas) As a planet moves around the Sun in its orbit, it covers equal areas in equal time. (changes speed)
(Law of Orbits) The orbit of each planet around the Sun is an ellipse. The Sun is at one focus.
(Law of Periods) The time it takes a planet to complete one orbit around the Sun is related to its average distance from the Sun. (p2 = a3, p = time, a = dist. from sun)
Continue
Eccentricity
Eccentricity is how flat or circular an ellipse is.
It ranges from 0 – 1 0 = circle 1 = line Earth’s orbit has an eccentricity value of 0.017. This tells us that Earth’s orbit is nearly circular.
Continue
EdPuzzle Time
Axial Tilt
The Earth’s axis of rotation is now tilted 23.5˚.
These changes in the axial tilt is believed to be the cause for Ice Ages.
Over 41,000 years the tilt varies from 22.1˚ to 24.5˚
Continue
Google Classroom Complete the Activity
Motions of Earth
Rotation – spinning of a body on its axis
Causes day and night 24 hour period (time zones)
Continue
Motions of Earth
Revolution – object traveling along a path around some point in space
365.25 days
Continue
Motions of Earth
Perihelion – when the earth is closest to the sun (Jan. 3)
Aphelion – when the earth is furthest from the sun (July 4)
Continue
Motions of Earth
Ecliptic – The apparent annual path of the Sun against the backdrop of the celestial sphere
Continue
Google Classroom Complete the Activity
Continue
Astronomy
Solstice and Equinox
Summative part 2
Let's go!
Equinox
Solstice
Autumnal Equinox – Sep. 23
Spring Equinox - March 21
Winter Solstice – Dec. 21
Summer Solstice – June 21 –
Continue
Continue
Continue
Precession
The Earth wobbles like a spinning top.
This wobbling is called precession.
This is caused by the gravitational pull of the Moon and the Sun
It takes 25,725 years for the Earth to wobble through one complete cycle.
Continue
Continue
Orbital Precession
The Earth’s orbit is revolving around the Sun.
This is called the orbital precession.
Continue
Combined Effects
The combined effects of the axial and orbital precessions will make our seasons as we know them today more extreme.
Winters will be colder
Summers will be hotter.
Continue
Inclination
Orbital plane – the first 8 planets are all fixed in the same plane.
Pluto however is tilted 17.1˚ from the rest of the planets.
This tilt is called inclination.
Continue
Continue
Google Classroom Complete the Activity Goal = 80%
Continue
Astronomy
Summative
Summative part 2
Let's go!