Astronomy 100 The Solar System Tuesday, Wednesday, Thursday. Tom Burbine

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1 Astronomy 100 The Solar System Tuesday, Wednesday, Thursday Tom Burbine

2 HW #2 Due day after next clear night Go to Use interactive sky chart Print pdf out for particular time, date, and location Circle what objects you can see in the sky

3 What is a galaxy?

4 What is a galaxy? Is a massive, gravitationally bound system consisting of stars, gas and dust, and dark matter. Galaxies can contain between ten million and a trillion stars Dark matter is matter that does not emit or reflect enough radiation to be seen, but whose gravitation effects can be felt

5 When we are looking at stars or galaxies We are looking into the past Light-year is the distance light travels in a year.

6 Milky Way Galaxy Milky Way is 100,000 light years in diameter There are ~200 billion stars in the Milky Way (estimates from billions stars)

7 What is the Universe?

8 What is the Universe? Sum total of all matter and energy all galaxies and everything between them Observable universe portion of the universe that can be seen from Earth, probably only tiny portion of the whole universe ~93 billion Light-years wide

9 What causes seasons? The tilt of the Earth s axis relative to the ecliptic

10 Seasons

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12 Solstices Summer Solstice June 21 Northern Hemisphere receives its most direct sunlight Winter Solstice December 21 Northern Hemisphere receives its least direct sunlight

13 Equinoxes Sun shines equally on both hemispheres Spring Equinox March 21 Northern Hemisphere goes from slightly tipped away from the Sun to slightly tipped towards Fall Equinox September 21 - Northern Hemisphere goes from slightly tipped toward from the Sun to slightly tipped away

14 Why does the orbital difference not matter?

15 Reasons There is only a 3% difference in the distance from the Earth to the Sun at its farthest and closest point The Earth is actually closer to the Sun in the winter than in the summer

16 Angular size We measure distances in the sky using angles 180 o in the observable sky

17 More precise distances 1 degree = 60 arcminutes (symbol ) 1 arcminute = 60 arcseconds (symbol ) So something that is 2 degrees, 10 arcminutes, 22 arcseconds would be written as 2 o 10 22

18 Terminology for looking at the sky

19 Celestial Sphere an imaginary sphere of infinite extent on which all celestial objects appear to lie

20 Celestial Sphere

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22 What is a constellation?

23 Constellations People refer to constellations as a pattern of stars Astronomers refer to constellations as specific regions of the sky In 1928, the IAU (International Astronomical Union) decided there were 88 constellations Many of the constellation names go back thousands of years

24 Constellations The constellations are totally imaginary things that poets, farmers and astronomers have made up over the past 6,000 years (and probably even more!). The real purpose for the constellations is to help us tell which stars are which, nothing more.

25 What is this constellation?

26 Orion Bigger the star, the brighter it is

27 Orion was the son of the god of the sea, Poseidon and a great hunter. One story is that he made an enemy of Hera who sent a scorpion to sting him. Orion was restored to health by Ophiuchus, the first doctor of medicine. Another story is that Artemis was tricked by by Apollo to shoot an arrow at Orion. When he died, Poseidon asked Zeus to put him among the stars.

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32 Ursa Major Ursa Major, the Great Bear, was identified with a bear by native American Indians of the Northeastern United States and the ancient Greeks. The name common in Britain, the Plough,seems to have a medieval origin, Another common name among northern European cultures is the Wain, a shortened form of wagon

33 What are the constellations named after 14 men and women 9 birds 2 insects 19 land animals 10 water creatures 2 centaurs one head of hair a serpent a dragon a flying horse a river 29 inanimate objects

34 Originally considered part of Leo s tail

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36 Named after Queen Berenice II of Egypt, wife of Ptolemy III Euergetes (246 BC BC) Around 243 BC, the king undertook a dangerous expedition against the Syrians, who had murdered his sister. Berenice swore to the goddess Aphrodite to sacrifice her famous long hair if her husband returned safely. He did, she had her hair cut, and placed it in the goddess' temple. By the next morning, the hair had disappeared. To appease the furious king and queen (and save the lives of the temple priests), the court astronomer, Conon, announced that the offering had so pleased the goddess that she had placed it in the sky. He indicated a cluster of stars that at the time were identified as Leo's tail, but now have been called Berenice's Hair.

37 Zodiac The zodiac is an imaginary belt in the heavens extending approximately 8 degrees on either side of the Sun's apparent path (the ecliptic), that includes the apparent paths of the Moon and the planets Mercury, Venus, Mars, Jupiter, Saturn, Uranus, and Neptune.

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41 Question: Why do all the planets seem to follow the same path?

42 Answer: The planets, the Earth, and the Sun all tend to fall in the same plane called the ecliptic

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45 Why don t all the constellations have ancient names?

46 Ancient cultures such as the Greeks and Egyptians could not see the constellations in the Southern Hemisphere

47 Question: Why is the path of the constellations on the zodiac not on the celestial equator?

48 Answer: The rotation axis of the Earth is inclined with respect to the ecliptic

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51 Polaris is called the North Star Brightest star in the constellation Ursa Minor. 48th brightest star in the night sky It is very close to the north celestial pole, making it the current northern pole star. Polaris' altitude, or height above the horizon, is equal to an observer's latitude.

52 Long Term Changes

53 Precession Earth precesses like a top Precession - phenomenon by which the axis of a spinning object (e.g. a part of a gyroscope) "wobbles" when a torque is applied to it

54 Forces For a top, the force is gravity, which is trying to pull the top down For the Earth, the forces are due to the pull of the Sun and Moon, which is trying to align the Earth s axis with the ecliptic

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56 Because of precession The position of a star that corresponds to the North Celestial Pole changes

57 Models When you have a model of how something works, you should be able to predict what will happen If observations do not fit the model, either the observations or the model is wrong The ancient astronomers wanted to predict the positions of planets in the sky

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59 What did the ancients think That the Earth was the center of the universe That the celestial sphere was rotating around the Earth However, there was two observations that caused problems with this idea Apparent retrograde motion Inability to detect stellar parallax

60 Greek model

61 Apparent Retrograde Motion = backward motion

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63 Retrograde Motion

64 Retrograde Planet appears to go backwards in its orbit

65 Stellar Parallax Stellar Parallax The apparent shift in the position of a nearby star (relative to distant objects) that occurs as we view the star from different positions in the Earth s orbit of the Sun each year

66 The distance the star moves is greatly exaggerated in this figure. Stellar parallax can only be seen by a telescope.

67 Ancient astronomers could not detect stellar parallax If Earth orbited the Sun, ancient astronomers believed that they would see differences in angular separation of stars as the Earth rotated around the Sun Since they saw no changes in angular separation of the stars, they assumed the Earth was the center of the universe They could not fathom that stars are so far away that stellar parallax is undetectable by the human eye

68 Ptolemy s ( AD) Model of the Universe

69 Nicholas Copernicus ( ) Copernicus came up with a model that the Earth revolves around the Sun Similar to what Aristarchus ( BC) thought 2000 years before However, Copernicus models did not match observations since he wanted everything to arouind in perfect circles

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71 Any Questions?