OUTCOME QUESTION(S): S1-4-04: How was the process of science important in showing the Sun is the centre of our solar system? S1-4-05: How does the position.

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Presentation transcript:

OUTCOME QUESTION(S): S1-4-04: How was the process of science important in showing the Sun is the centre of our solar system? S1-4-05: How does the position and motion of Earth produce day/night, the phases of the moon, and the seasons? Vocabulary & People PtolemyCopernicusGalileo KeplerRetrogradeGeocentric HeliocentricSolsticeEquinox

Ptolemy (100 AD) Hypothesized “epicycles” to explain observations and knowledge of that time Earth was centre of the universe - Geocentric In good with the Church Observation: Some planets seem to move backwards in orbits: “Retrograde motion” Planet is Greek for “wanderer”

Ptolemy GEOCENTRIC Ptolemy’s proposed mini-loop “epicycles” solved the retrograde motion puzzle

Copernicus (1473) Produced mathematical evidence for a Sun- centered system – heliocentric Much simpler explanation for retrograde motion Hypothesized Earth rotated on axis once daily and revolved around Sun once yearly Not in good with Church Called the “Founder of modern astronomy”

Copernicus HELIOCENTRIC

First optical telescope made in Netherlands (1608): The first one was a simple refracting telescope Uses curved optical elements Gathers and collects light to a focal point Increase apparent size and apparent brightness

Telescopes are classified by the energy detected: Optical – visible light Infrared – heat energy Ultraviolet, X-ray Different energies provide astronomers with different information a Refracting telescope - lenses focus an image b Reflecting telescope - mirrors focus an image

Galileo (1564) Perfected the telescope (built a few years earlier) First to state and use the scientific method Discovered moons around Jupiter 1 Proof that not all objects traveled around Earth Venus had phases (day/night) like Earth/moon 2 Proof that it traveled around the Sun Not in good with the Church

Galileo’s drawings and scientific records of his observations

Would not recant his work as a mistake and spent entire life under house arrest Galileo published his evidence confirming Copernicus’ mathematics, and was accused of heresy by the Church. By the way, Pope John Paul II made a public apology and exonerated Galileo in 1992

Kepler (1571) Brahe built one of the best observatories in the world Worked as assistant for astronomer, Tycho Brahe Brahe’s goal was to prove Copernicus incorrect Measured positions of 777 stars and five planets that were known at that time He received loads of money from the Church in hopes he could prove the Earth-centred view…he failed

Kepler used Brahe’s data after his death to describe three laws of planetary motion: 1. Planets orbit the Sun in ellipses (not circles) 2. Planets move faster close to Sun, slower farther away 3. Planets farther away have a longer orbital period

What do we know today?

The Earth rotates on its axis once a day. At any time - half of Earth is in “day” and half in “night.” Earth rotates towards the East The Earth revolves around the Sun once a year. At any time - half of Earth is in “winter” and half in “summer.” summer winter

Our axis is tilted at 23.5 o (degrees) This tilt and the curvature of the Earth is responsible for the variations in the Sun’s energy – and creates our seasons.

Summer “direct” energy Winter “indirect” energy Summer: not only more “direct” but also more hours of the Sun’s energy Summer Solstice (June 21) Longest Day Winter Solstice (Dec 21) Shortest Day Fall Equinox (Sept 22) 12h and 12h Spring Equinox (Mar 21) 12h and 12h

Moon completes 1 rotation on its axis in the same time as it completes 1 revolution around the Earth (synchronous) We always see the same side facing the Earth Orbit is elliptical Tilted 5° Mean Distance: 384,400 km Moon Rotation That’s why there is a “dark side” of the Moon

Phases of the Moon Shines only by reflected sunlight Depends on fraction of sunlit half visible to us

CAN YOU ANSWER THESE QUESTIONS? S1-4-04: How was the process of science important in showing the Sun is the centre of our solar system? S1-4-05: How does the position and motion of Earth produce day/night, the phases of the moon, and the seasons? Vocabulary & People PtolemyCopernicusGalileo KeplerRetrogradeGeocentric HeliocentricSolsticeEquinox