A100 Solar System Today’s APODAPOD  Read Chapter 1 in text – History of Astronomy  Rooftop, Kirkwood Sessions TONIGHT  1 st Homework due Friday (get.

Slides:



Advertisements
Similar presentations
Motions of the Earth and Sky
Advertisements

Fix Astronomy Chapter 2.
Prof. D.C. Richardson Sections
Warm-UP NoteBook – ORGANIZE Earth, Moon and Sun Study Guide Vocabulary
The Sun-Earth-Moon System
Earth’s Motions, Solar Radiation, and the Seasons
Unit III: The Earth in Space
The Earth’s Movement.
The Sky
Topic 4 Motions of the Earth, Moon, and Sun
Apparent/Actual Motions Summary
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon.
The night sky? With the naked eye, we can see more than 2000 stars as well as the Milky Way. Remind students that we often use the term “constellation”
A100 Solar System The Sun Today Today’s APOD Monday, Sept. 8
Chapter 8 Earth in Space. How long does it take for Earth to complete one full rotation?
Sky Motions Diurnal Motion Annual Motion.
Earth Motions and the Heavens
Aim: What are the apparent motions of the stars and planets?
Page #136 Feb. 5, 2013 Focus: Day & Night, Seasons, Rotation & Revolution Objective: explain how the movement of the Earth affect different cycles EQ:
Do Not Write What is in Yellow APPARENT MOTIONS OF THE CELESTIAL OBJECTS.
Discovering the Universe for Yourself
Constellations A constellation is a region of the sky.
Chapter 1: The Cycles of the Sky
Our goals for learning:
Constellations.
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
Chapter 2 Discovering the Universe for Yourself
The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The 88 official constellations cover the celestial sphere.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 1 If you could hover over the Earth’s north rotational pole.
Groups of dark brown streaks have been photographed by the Mars Reconnaissance Orbiter on melting pinkish sand dunes covered with light frost. Dark sand.
NATS From the Cosmos to Earth A model of the celestial sphere shows the patterns of the stars, the borders of the 88 official constellations, the.
Solar Motion. Label front flap MOTIONS OF THE EARTH -DAY & NIGHT.
Motions of the Earth Our goals for learning: What are the main motions of the Earth in space? How do we see these motions on the ground? How does it affect.
Astronomy by eye: motions in the Sky
© 2010 Pearson Education, Inc. Discovering the Universe for Yourself.
Last time: 2.1. Patterns in The Sky: Stars and constellations, TODAY: celestial coordinates 2.2 Seasons,…Precession 2.2 (cont.) The Moon and Eclipses.
Chapter 1 Predicting the Motions of the Stars, Sun, and Moon.
Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as.
© 2005 Pearson Education Inc., publishing as Addison-Wesley Chapter 2 Discovering the Universe for Yourself Mark Twain (1835 – 1910) American author, from.
Chapter 6: Earth’s Motions in Space Ms. Johnson Foundations.
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.
Mastering Astronomy.
1 Lines in the Sky In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring.
Happy Haunted Homeroom October 9, 2012 Today is Tuesday, you have academic and I.S. with your Period 2 teacher.
Seasons of the Year.
EARTH IN SPACE. A reminder about earth  The earth is almost a sphere  We locate points on the sphere with 3 coordinates – Longitude (180º W º.
Copyright © 2015, W. W. Norton & Company Prepared by Lisa M. Will, San Diego City College Lecture Slides CHAPTER 2: Patterns in the Sky—Motions of Earth.
The Daily Motion As the Earth rotates, the sky appears to us to rotate in the opposite direction. The sky appears to rotate around the N (or S) celestial.
What causes the seasons?
Sky Motions  Diurnal Motion Annual Motion. DIURNAL MOTION o Daily East / West motion of the sky Due to the Earth’s rotation (15°/hour) [360°/24 hours.
Astronomy: Apparent Motions Making sense of celestial observations.
Chapter 8: Planet Earth and Its Moon Lesson 1 How Does Earth Move?
© 2010 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself.
Chapter 4: Rising & Setting Stars © BRIEF
Astronomy vs. Astrology Astronomy: Astronomy: The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion,
Motion in the Sky. Discussion What is a year? Discussion What is a day?
Motion of the Moon. Review Question Describe the path the Sun will take across the sky on the day of the autumnal equinox as viewed from the Earth’s equator.
Before, you learned Stars seem to rise, cross the sky, and set because Earth turns The Sun is very large and far from Earth Earth orbits the Sun Now,
Astronomy Unit 1 The celestial sphere and the seasons.
Astronomy Chapter 1 Charting the Universe. Obj.#1 What is Astronomy? Astronomy is the study of the Universe The universe is the total of all space, time,
Research Experiences for Undergraduates (REU)
Chapter 2: Discovering the Universe for Yourself
SUN-EARTH-MOON SYSTEM The Sun-Earth-Moon System
University of Scouting March 24, 2012 Gary G. Smith
Celestial Motions Chapter 2.
ASTRO UNIT 1 REVIEW.
Celestial Motions Chapter 2.
Presentation transcript:

A100 Solar System Today’s APODAPOD  Read Chapter 1 in text – History of Astronomy  Rooftop, Kirkwood Sessions TONIGHT  1 st Homework due Friday (get it on Oncourse) The Sun Today Wednesday, Sept. 10 & Friday, Sept. 12

Kirkwood and Rooftop Sessions Kirkwood Observatory –Open 9:30-11:30 PM (about 30 minutes) –West end of Dunn’s Woods, near 4 th & Indiana Rooftop – Swain West –9 PM –Elevator to 3 rd floor, follow signs to roof –Rain date Sept. 11 PRINT WORKSHEETS FROM ONCOURSE (SYLLABUS TOOL) BEFORE YOU COMEONCOURSE

SPECIAL Opportunities! SCOPEOUT in Cincinnati: Sept. 13 – –Phil Plaitt (Bad Astronomy) Astronomy Day – Stonebelt Stargazers – Sept. 13 –Wal-Mart in Bedford, 4-8 PM

Jupiter & the Moon in Sagittarius Sept 9Sept 8 Just look south… Jupiter is the brightest object in the southern sky

Finding Polaris Find the Big Dipper in the northwestern sky Sky chart for 9 PM TONIGHT Find an open area away from nearby lights where you have a good view of the sky North South Big Dipper’s on its side in the northwestern sky

Finding Polaris To find Polaris: find the Big Dipper follow to Polaris the Big Dipper is ALWAYS up in Indiana!

The Celestial Sphere The stars all appear to lie on a large sphere surrounding the Earth (the celestial sphere) Really, the stars are all at different distances

The Local Sky An object’s altitude (above horizon) and direction (along horizon) gives its location in your local sky

Our view from Earth: Stars near the north celestial pole are circumpolar and never set. All other stars (and Sun, Moon, planets) rise in east and set in west. Celestial equator A circumpolar star never sets This star never rises in Indiana

Altitude of the celestial pole = your latitude

Why do the constellations we see depend on latitude and time of year?  They depend on latitude because your position on Earth determines which constellations remain below the horizon.  They depend on time of year because Earth’s orbit changes the apparent location of the Sun among the stars.

The sky changes as Earth orbits the Sun  As the Earth orbits the Sun, different constellations are visible at night  At midnight, the stars on our meridian are opposite the Sun in the sky

Vocabulary Review oConstellation oEcliptic oEquator oCelestial sphere oLatitude oLongitude o Meridian o Zenith o Horizon o Altitude o North and south celestial poles

Visualizing Space

Expert Methods for Visualization  Draw diagrams  Use 3d models  Use visualization software If you have a chance, visit a planetarium…

Visualize the Earth from Space Pretend you are Superman! What do you see? –Earth –Moon –Sun –Stars Copyright 1980 by DC Comics Inc.

Welcome to Outer Space!

Which of the following four diagrams most accurately depicts the Earth's orbit around the Sun?

The Solar System from Overhead space.jpl.nasa.gov

The Solar System from “Overhead” Earth’s Orbit –91,369,000 miles on Jan 4 (minimum) –94,776,000 miles on July 4 (maximum) –average distance is 92,918,000 miles –Varies +/- about 2% from a perfect circle

Basic Ideas The Earth orbits the Sun in one year (revolves) The Earth spins around once each day (rotates) The Moon orbits the Earth about once a month (revolves)

The Earth and Moon from Mars Where are Mars, Earth the Moon and the Sun?

Visualizing the Earth in Space: What causes the Seasons…?

The Earth has seasons because…? The Earth moves closer to or farther from the Sun - it’s closer in the summer and farther in the winter. True or False?

December Weather Bondi Beach - Sydney, Australia IU’s Rose Well House

When is the Earth closest to the Sun? A. Winter B. Spring C. Summer D. Fall

Visualizing Seasons – What really happens? Textbook applet: cause_of_seasons.htm

Which of the following best explains why it is hotter in Indiana in June than it is in December? A The Sun gives off more heat energy in June. D Earth is closer to the Sun in June. B The Northern Hemisphere is closer to the Sun in June. C The Sun is higher in the sky and and provides more hours of daylight in June.

With thanks to Bill Watterson, 1990

Visualizing the Moon

Galileo Galilei's "The Phases of the Moon" Image courtesy of Biblioteca Nazionale Florence, Italy How can we understand the phases of the Moon as it circles around the Earth?

What causes the Moon to change its appearance in this way? A.As the Moon orbits Earth, Earth's shadow covers the Moon. B.Clouds block part of the Moon from our view so it is full sometimes and covered other times. C.As the Moon orbits Earth, the part of the Moon facing Earth is facing away from the Sun. Sometimes the Moon looks like this And sometimes the Moon looks like this

The Earth and Moon from Space

Thinking about the Moon How much of the Moon receives sunlight at a given time? Always half the Moon? Sometimes more or less than half? Why? During new moon (when the moon appears dark) is sunlight falling anywhere on the Moon's surface? If not, why not? If so, why don't we see it? Is the Earth or the Moon closer to the Sun at new moon? Which is closer to the Sun at full moon?

The Moon moves in its orbit about 12 degrees per day It rises about an hour later each night. Why?

Bring the perspective back to Earth Ansel Adams; copyright © 2000 George Eastman House, Rochester, NY

Understanding the Moon in the Sky I’m really way off to the right

Now I’m right here!

Moon and Venus before Dawn Where are the Earth, Moon and Sun in 3-dimensional space? Where is Venus?

The Libration of the Moon

One question I’ve always had about astronomy is…

ASSIGNMENTS this week  Read Chapter 1, History of…  Kirkwood Obs. TONIGHT  Rooftop Sky Viewing TONIGHT  1 st HW due Friday Dates to Remember