Welcome This is Phys 1040 and Astro 1040 Please pick up one each of the papers on the table up front. twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction My e-mail By far the best way to contact me is by e-mail. twlee2016@gmail.com twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction My Web Page http://www.astro1010-lee.com/ Syllabus Copies of my Slides Lecture Notes Links twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction Text There is no Text, only the Slides and Lecture Notes Tests 5 unit tests NO comprehensive final Must be taken on the day scheduled (I can change the date but you can NOT) Absolutely no late tests May be taken early I DROP YOUR LOWEST TEST SCORE twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction ASTROLAB (SEE LINK) •You need to attend one • Dr. Powell offers only a finite number • I recommend that you go to an early one twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction Term Papers Select from the list of Subjects that t provide. These are designed to be associated with the lectures. If you email them to me on the designated day you will get full credit, anytime after that is half credit. twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Introduction The purpose of this exercise is for the student to determine the circumference of the Earth using a variation of the Erotosthenes method twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Exercise 1 Requires Protractor Thread Tape Weight Find the North Star Measure the angle from the Horizon to the North Star twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Exercise 1 This is how your protractor should look after you get it ready twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Exercise 1 NCP NCP θ1 θ2 twlee2016@gmail.com Astro1010-lee.com Survey of Astronomy Exercise 1 Survey of Astronomy Astro1010-lee.com twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 twlee2016@gmail.com BEGINNINGS twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Astronomy -- Study of the Universe Universe -- everything that exists Galaxy The Milky Way is our Galaxy Stars Open Star Clusters Globular Star Clusters Nebulae Sun Solar System Solar System Planets Moons Asteroids Comets Other debris Earth/Moon System twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Subtend When an object just fills an angle it subtends that angle. twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Angular Units Degree (of arc) = 1/360 Circle Minute (of arc) = 1/60 of a Degree Second (of arc) = 1/60 of a Minute Hour (of arc) = 360/24 = 15 degrees twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Distance Measure in Space twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 OUR CODE The Earth and the entire Universe obey a single set of Laws twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Scientific Theory and the Scientific Method Scientific theories: must be testable must be continually tested astro1010-lee.com Survey of Astronomy Chapter 1 Scientific theories can be proven wrong, but they can never be proven right with 100% certainty should be simple should be elegant twlee2016@gmail.com Scientific Theory and the Scientific Method •Observation leads to theory explaining it • Theory leads to predictions consistent with previous observations • Predictions of new phenomena are observed. If the observations agree with the prediction, more predictions can be made. If not, a new theory can be made. twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Early Discoveries Pre-historic Historic Sun Moon Stars Constellations Planets Movement of the Sky Path of the Sun Movement of the Moon Cyclic nature of the Universe ….. led to calendars Explanation of the phases of the Moon NCP Celestial Equator Explanation of the seasons twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Earth’s Orbital Motion Daily cycle, noon to noon, is diurnal motion – solar day Stars aren’t in quite the same place 24 hours later, though, due to Earth’s revolution around Sun; when they are, one sidereal day has passed twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 From season to season the stars that we see change. This is because of the motion of the Earth in it orbit. The ancients thought it was because the Sun moved around the Earth twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 The 12 constellations that the Sun appears to move through during the year are called the zodiac; the apparent path is the ecliptic twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 The Earth revolves around the Sun once each year causing the Sun to appear to move around the sky twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 •Time from one vernal equinox to next is tropical year •Combination of day length and sunlight angle gives seasons twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Precession: rotation of Earth’s axis itself; makes one complete circle in about 26,000 years twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 The Terrestrial Coordinate System Latitude is measured north and south from the equator Longitude is measured east and west from the prime meridian twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Zenith is the point directly overhead Meridian is the line from the north point through the zenith and on to the south point. Horizon is the line on the sky made by the plane that is perpendicular to the vertical line from you to the zenith twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 The Celestial Coordinate System Reference points and planes on Celestial Sphere twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 The Celestial Coordinate System Right Ascension (RA) or Hour Angle is measured from the point on the sky where the Sun is at the Spring Equinox Declination (δ) is measured north or south from the Celestial Equator twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1 Go to Chapter 2 twlee2016@gmail.com astro1010-lee.com Survey of Astronomy Chapter 1