Please turn off cell phones - thanks! panda.unm.edu/courses/sanfratello/sp09/astro101 Remember - Read syllabus and schedule (contains textbook reading.

Slides:



Advertisements
Similar presentations
Earth-Moon-Sun System
Advertisements

Chapter 17 Earth’s Cycles
Chapter 17 Earth’s Cycles
Moon Phases and eclipses.
27.3 – Sun-Earth-Moon System
Chapter 1 Charting the Heavens
Chapter 3 The Cycles of the Moon.
Celestial Sphere Stars seem to be on the inner surface of a sphere surrounding the Earth.
Motion of Earth and Moon around the Sun
Chapter 0 Charting the Heavens
Astronomy Foundations – Chapter 0
Info for the Test Bring a #2 pencil. No electronic devices: No calculators, cell phones, headphones, etc. No books, notes, etc. No hats. Grades will be.
Please turn off cell phones - thanks! panda.unm.edu/courses/sanfratello/astro101 Remember - Read syllabus and schedule (contains textbook reading assignments.
Angular Measure 90 o 20 o 360 o, or 360 degrees, in a circle. 1 o = 60' or arcminutes 1' = 60" or arcseconds 1" = 1000 mas or milli-arcseconds.
Please turn off cell phones - thanks! panda.unm.edu/courses/sanfratello/astro101 Remember - Read syllabus and schedule (contains textbook reading assignments.
Our Moon.
Question 1 Constellations appear to move across the sky at night because 1) the Earth orbits the Sun. 2) the Moon orbits the Earth. 3) stars are in constant.
The Earth-Moon-Sun System
The Night Sky. Ancient Astronomy Early astronomers paid attention to the sky and were careful to not offend the gods that rule the skies. The time it.
Moon Phases, and Eclipses
Introduction to Astronomy. What is astronomy? Astronomy is the science that studies the universe. It includes the observation and interpretation of planets,
Chapter 1: The Cycles of the Sky
© 2011 Pearson Education, Inc. Lecture Outlines Chapter 1 Astronomy Today 7th Edition Chaisson/McMillan.
© 2011 Pearson Education, Inc. Lecture Outlines Chapter 1 Astronomy Today 7th Edition Chaisson/McMillan.
Earth Science 22.2A Earth-Sun System
The Sky at Night What do we see?. The Sky at Night What do we see? The Moon Planets Perhaps a meteor shower, comet, or other rare event Stars - about.
THE MOON. REVOLUTION AND ROTATION Relative to stars, Moon moves eastward by about 13° per day. Eastward motion is faster than that of Sun; meaning Moon.
The Sun-Earth-Moon System (Chapter 3). Student Learning Objectives Associate cycles in the sky with time Describe why Earth has seasons Determine the.
Equinoxes and Solstices When the ecliptic and celestial equator intersect, day and night are each 12 hours long: the equinox. When the Sun reaches its.
The Moon’s Motions After completing this section, students will describe the types of eclipses (Standard PI – 070)
Alta High Astronomy Intro: Astronomy A stellar course to be in!
Chapter 1 Earth, Moon, and Sun Section 3 Phases, Eclipses, and Tides.
The Earth’s Moon. Motions of Earth’s Moon Revolution of the moon around Earth affects: phases of the moon, tides and eclipses Revolution of the moon around.
Ch Movements of the Moon. From earth, moon appears to orbit the earth, but from space, earth and moon orbit each other as they go around the sun.
Charting the Heavens TEKS: A.7: The student knows the role of the Moon in the Sun, Earth, and Moon system By the end of today, IWBAT… Answer the Review.
The Moon (Earth’s natural satellite) Phases, Eclipses & Tides.
CHAPTER 3 Eclipses and the Motion of the Moon CHAPTER 3 Eclipses and the Motion of the Moon.
Please turn off cell phones & laptops - thanks! panda.unm.edu/courses/sanfratello/SP09/astro101.html Remember - Read syllabus and schedule (contains links.
1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.
Chapter 0 Lecture Charting the Heavens.
Earth’s Orbit and the Seasons. Seasons on the Earth.
Astronomy 105 ä Student Information Sheet ä Class Syllabus ä Lab Syllabus ä Course Supplies ä Text ä Lab Manual ä Scantron 882-ES ä Flashlight with red.
A Quick Tour of the Universe (and this course) Part 2.
Space Study Guide Review. 1.What causes the Earth to orbit the Sun? A: The straight, forward motion of the Earth and the pull of gravity between the Sun.
Motions of the Earth Ch Rotation the turning, or spinning, of a body on its axis. Two measurements for rotation Mean solar day is the time interval.
ASTR 111 – 003 Fall 2007 Lecture 02 Sep. 10, 2007 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I: Solar System Ch1: Astronomy and.
ASTR 111 – 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy II Ch1: Astronomy and the Universe.
Universe Tenth Edition Chapter 3 Eclipses and the Motion of the Moon Roger Freedman Robert Geller William Kaufmann III.
SOLAR ECLIPSE One consequence of the Moon's orbit about the Earth is that the Moon can shadow the Sun's light as viewed from the Earth (2)
Chapter 0: Charting the Heavens. Units of Chapter 0 The “Obvious” View Earth’s Orbital Motion The Motion of the Moon The Measurement of Distance Science.
Chapter 22 Origin of Modern Astronomy Section 2 The Earth-Moon-Sun System Notes 22-2.
Discovering the Universe Eighth Edition Discovering the Universe Eighth Edition Neil F. Comins William J. Kaufmann III CHAPTER 1 Discovering the Night.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 1.
Chapter 19 Earth, Moon, and Sun. Bellwork Write about a scientific observation you made over the weekend. Don’t ask me, “What if I didn’t make one!”
22 Chapter 22 Origin of Modern Astronomy Starter 1.Compare and contrast the geocentric and heliocentric models. 2.Describe Kepler’s three laws of planetary.
Lunar Phases & Eclipses Astronomy The Moon orbits the Earth about once a “moonth” with one complete cycle of the lunar phases each month…
May 14,  How long does it take for a planet to orbit around the sun?
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 1.
Eclipses and the Motion of the Moon Chapter Three.
© 2011 Pearson Education, Inc. Chapter 1 Charting the Heavens.
CALCULATION OF ASTRONOMICAL DATA
© 2017 Pearson Education, Inc.
© 2017 Pearson Education, Inc.
Bellwork 9/17 What causes the seasons?
Astronomy-Part 10 Notes The Earth-Moon-Sun Systems
The Sun, moon, and earth as a system
Earth’s Motions Astronomy.
19.3 Phases, Eclipses, Tides Key concepts: What causes the phases of the moon? What are solar and lunar eclipses? What causes the tides? Key terms: phases,
Earth’s Motions.
Chapter 22 Section 2.
Presentation transcript:

Please turn off cell phones - thanks! panda.unm.edu/courses/sanfratello/sp09/astro101 Remember - Read syllabus and schedule (contains textbook reading assignments and suggested problems from the text.)‏

Astronomy Picture of the Day

Powers of Ten Video

What properties of physical objects would you expect to be important in Astronomy? Mass Size Distance from Earth Temperature Speed and Velocity Brightness (Luminosity)‏ Age Chemical composition

Question Which is longer a Solar Day or a Sidreal Day? Why? A. Solar, Earth both rotates on it's axis and orbits the sun B. Sidreal,Earth both rotates on it's axis and orbits the sun C. Solar, the Earth slows down as it rotates D. Sidreal, the Earth speeds up as it rotates

One solar day later, the Earth has rotated slightly more than 360 o. A solar day is longer than a sidereal day by 3.9 minutes (24 hours vs. 23 hours 56 minutes seconds). Difference due to rotation and revolution of Earth!

Question The “wobble” of the Earth on its axis is called _______. It is caused by _______. A. precession, the Earths rotation on it's axis B. rotation, conservation of angular momentum C. precession, the gravitational pull of the moon D. Earth's orbit around the sun, the seasons

Precession What causes precession? How long does one cycle take?

Precession The Earth has a bulge. The Moon "pulls down" on the side of the bulge closest to it, causing the Earth to wobble on its axis. Earth Moon Spin axis * * Vega Polaris Precession Period 26,000 years!

Question Why is looking out into space like looking back in time? A. ancient civilizations named the constellations B. the speed of light is infinite C. the speed of light is finite

How are the Earth, Moon, Sun, and stars laid out in space? What lies at the “center”? Motion(s) of the Earth? Motion(s) of the Moon? What about the stars?

The Motion of the Moon The Moon has a cycle of "phases", which lasts about 29 days. Which way is the Sun here? Moon moves in synchronous motion – it rotates on its axis in exactly the same amount of time it takes to orbit earth. Reflected Light

(DEMO)‏

Why doesn't the earth prevent the sunlight from reaching the moon during its “Full phase”?

Moon's orbit tilted compared to Earth-Sun orbital plane: Sun Earth Moon Side view 5.2 o

Eclipses What sort of alignment of the Earth, Moon, and Sun is required for a lunar eclipse? How about for a solar eclipse?

Eclipses Lunar Eclipse (around 100 minutes)‏ When the Earth passes directly between the Sun and the Moon. Sun Earth Moon Solar Eclipse (no more than about 8 minutes)‏ When the Moon passes directly between the Sun and the Earth. Sun Earth Moon

Lunar Eclipse

Total Solar Eclipse

Varieties of Solar Eclipses

During which phase(s) can a lunar eclipse occur? What about a solar eclipse? Why don't eclipses occur every month?

Regions of Earth that saw or will see total (red) or annular (blue) solar eclipses between the years 2000 and Each track represents the path of the Moon’s umbra across Earth’s surface during an eclipse. High-latitude tracks are broader because sunlight strikes Earth’s surface at an oblique angle near the poles and because of the projection of the map.

Triangulation - Using Geometry to Measure Distances Measure:  Angle at A  Angle at B  Length of Baseline Calculate:  Distance to object distance =baseline*tan(B)‏ (SOH CAH TOA )‏

Parallax Triangulation - Measure angles at points A and B Parallax - Know Baseline. Measure third angle in triangle made by A, B, and object in space  Baseline problem The apparent displacement (shift) of a foreground object relative to the background as the observer’s location changes is known as parallax.parallax

Parallax Geometry Parallax angle is inversely proportional to distance of object Close object causes large parallax Distant object causes small parallax The closer an object is to the observer, the larger the parallax.