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6/10/20161 Ch. 22: Astronomers Mr. Litaker 6/10/20162 Our Solar System What do we know? Time required for Earth to make one rotation on its axis? 24.

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Presentation on theme: "6/10/20161 Ch. 22: Astronomers Mr. Litaker 6/10/20162 Our Solar System What do we know? Time required for Earth to make one rotation on its axis? 24."— Presentation transcript:

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2 6/10/20161 Ch. 22: Astronomers Mr. Litaker

3 6/10/20162 Our Solar System What do we know? Time required for Earth to make one rotation on its axis? 24 Hours

4 6/10/20163 Revolution Time required for Earth to make one revolution around the sun? 365 ¼ Days

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6 5 Time of Year During what time of the year is the Earth closest to the sun? Winter The northern hemisphere tilted away from sun during winter resulting in less solar heating even though the earth is closer to sun. * During what time of the year is the Earth farthest from the sun? Summer The northern hemisphere tilted towards sun resulting in more solar heating Perihelion Aphelion

7 6/10/20166 Orbit What type of orbit does the Earth have around the sun? elliptical

8 6/10/20167 Early Astronomy Astronomy – is the science that studies the universe. Astronomy deals with the properties of objects in space and the laws under which the universe operates.

9 6/10/20168 Our Solar System The Historical Perspective Aristotle Ptolemy Copernicus Tycho Brahe Kepler Galileo Newton

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11 10 Aristotle Greek philosopher (384- 322 B.C.) Believed that the Earth was the center of the Universe. Geocentric model – Earth Centered ** Thought – the Sun, Stars, and other Planets revolved around the Earth. Concluded the Earth was round because… It always cast a curved shadow on the moon.

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13 6/10/201612 Ptolemy 141 A.D. Much of our knowledge of Greek astronomy comes from Claudius Ptolemy. Supported Geocentric Model Since Ptolemy’s model predicted motions of the planets, his model went unchallenged for nearly 13 centuries.

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15 6/10/201614 Heliocentric Model – (312-230 B.C.) was the 1 st to believe that the sun was the center of the universe. This was referred to as a Aristarchus – (312-230 B.C.) was the 1 st to believe that the sun was the center of the universe. This was referred to as a Heliocentric model. Everything orbits the sun in this model.

16 6/10/201615 Viewpoints Even though Aristarchus provided some evidence of distances and sizes that were not completely accurate --- 2000 years!!! The Geocentric Model dominated western thought for nearly 2000 years!!!

17 6/10/201616 Nicolaus Copernicus Cleric and Astronomer 1473 - 1543 Finally we shall place the Sun himself at the center of the Universe. All this is suggested by the systematic procession of events and the harmony of the whole Universe, if only we face the facts, as they say, 'with both eyes open'.

18 6/10/201617 Nicolas Copernicus “Copernican Revolution” Polish astronomer (1473-1543) Believed that the sun was the center of the solar system. Heliocentric Model – Sun Centered The 1 st Great Astronomer To emerge In the Middle Ages!

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20 6/10/201619 Tycho Brahe Tycho Brahe Danish Astronomer (1546 – 1601) Built an observatory financed by the king of Denmark. Made detailed observations and records of the planets. Assisted by mathematician Johannes Kepler

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22 6/10/201621 Johannes Kepler German astronomer (1571- 1630) Used the planet data of Tycho Brache and developed Kepler’s: Three Laws of Planetary Motion. Used the planet data of Tycho Brache and developed Kepler’s: Three Laws of Planetary Motion. Look in the book and copy his 3 laws. 618

23 6/10/201622 First Law The First Law: Planets move in ellipses with the Sun at one focus. Circular and Elliptical Orbits Having the Same Period and Focus

24 6/10/201623 2 nd Law The radius vector describes equal areas in equal times. (The Second Law) For a circle the motion is uniform as shown above, but in order for an object along an elliptical orbit to sweep out the area at a uniform rate, the object moves quickly when the radius vector is short and the object moves slowly when the radius vector is long.

25 6/10/201624 3 rd Law The Third Law: The squares of the periodic times are to each other as the cubes of the mean distances. This law he published in 1619 in his Harmonices Mundi. It was this law, not an apple, that lead Newton to his law of gravitation. Kepler can truly be called the founder of celestial mechanics.

26 6/10/201625 Galileo Galilei

27 6/10/201626 Galileo Galilei Italian Mathematician (1564 – 1642) Invented the telescope in 1608 and observed… ? Look in the book on page 619 and list the 5 discoveries Galileo made with his telescope.

28 6/10/201627 Galileo Galileo quickly discovered that our Moon had craters, that Jupiter had it's own moons, that the Sun has spots, and that Venus has phases like our Moon. Galileo, who lived from 1564 to 1642, made many more discoveries. Galileo claimed that his observations only made sense if all the planets revolved around the Sun, as championed by Aristarchus and Copernicus, not the Earth, as was commonly believed then. The powerful Inquisition made Galileo publicly recant this conclusion, but today we know he was correct.

29 6/10/201628 Newton

30 6/10/201629 Isaac Newton English Scientist 1643 to 1727 Recognized as the greatest Scientific intellect of all time. Best known for his laws of motion and universal gravitation formula. What does the Law of Universal Gravitation state ?

31 6/10/201630 Play CD: Discover Astronomy Section II

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33 6/10/201632 Earth – Moon Relationships

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35 6/10/201634 Sidereal Day vs. Solar Day Solar Day – 24 Rotation using the Sun as our reference. Sidereal Day – 23 hours 56 minutes for one complete rotation using a star other than the sun. There is a loss of 4 minutes or 1 0. Power Line Example: At Night

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40 6/10/201639 What season is the Northern Hemisphere experiencing? Summer Where is the most direct rays striking? Tropic of Cancer

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