First MIDTERM Exam: This Thursday, Sep. 9, covering chapters 1 2. Short review later today

Similar documents
Observing the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.

First MIDTERM Exam: Mon, Sep. 22, covering chapters tutorials (review later today).

Appearance of the Sky Orientation Motion of sky Seasons Precession (?)

Before you Sit. Please Pick-up: Blue Information Sheet for Evening Observing. 1 Red and 1 Blue ticket for Observing/ Planetarium

Welcome back. Scale. Week 2 Updates. PHYS 1302 Astronomy of the Solar System

Appearance of the Sky Orientation Motion of sky Seasons Precession (?)

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself

Astronomy 291. Professor Bradley M. Peterson

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.

Brock University. Test 1, October 2017 Number of pages: 9 Course: ASTR 1P01, Section 1 Number of Students: 470 Date of Examination: October 3, 2017

It s Full of Stars! Outline. A Sky Full of Stars. Astronomy 210. lights), about how many stars can we see with

At Home Phases Demo. Astronomy 210. Section 1 MWF Astronomy Building. Geocentric vs. Heliocentric system. The Motion of the Planets

Introduction To Modern Astronomy I: Solar System

Homework 1 (from text) Latest Deep Impact Results: 2. Discovering the Universe for Yourself.

Dive into Saturn.

Lecture 2: Motions of the Earth and Moon. Astronomy 111 Wednesday August 30, 2017

Today in Space News: Earth s oldest rock found on the Moon.

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Science : Introduction to Astronomy. Lecture 2 : Visual Astronomy -- Stars and Planets. Robert Fisher

3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.

1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.

The Sky Perceptions of the Sky

Knowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations

Astr 1050 Mon. Jan. 31, 2017

Brock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014

Exam 1 is Feb. 1 (next Tuesday) This will cover everything we have done so far Earth motions The celestial sphere and observations from Earth Seasons

Reading Reminders. Your Questions via JiTT2

HISTORY OF ASTRONOMY, PART 1. How our understanding of the Universe has changed

Today. Tropics & Arctics Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME

Chapter 1 Image Slides. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Discovering the Night Sky

Discovering the Night Sky

PHYSICS 107. Lecture 4 Ancient Astronomy

1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.) Ecliptic

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.

Astronomy 101: 9/18/2008

Astronomy 103: First Exam

Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION

Brock University. Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016

Introduction to Astronomy

Astronomy is the oldest science! Eclipses. In ancient times the sky was not well understood! Bad Omens? Comets

The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses. Chapters 2 and S1

Today. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME

Summary Sheet #1 for Astronomy Main Lesson

CHAPTER 2 A USER'S GUIDE TO THE SKY

Knowing the Heavens. Goals: Constellations in the Sky

lightyears observable universe astronomical unit po- laris perihelion Milky Way

Knowing the Heavens. Goals: Constellations in the Sky

2. Knowing the Heavens

6/17. Universe from Smallest to Largest:

2.1 Patterns in the Night Sky

Newton s Universal Law of Gravitation and planetary orbits. Gravity (cont.) / Night Sky / Seasons 1/23/07

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified

Dr. Tariq Al-Abdullah

2. Modern: A constellation is a region in the sky. Every object in the sky, whether we can see it or not, is part of a constellation.

1. The Moon appears larger when it rises than when it is high in the sky because

Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon

Seasons. What causes the seasons?

AST 2010 Descriptive Astronomy Study Guide Exam I

ASTR 1P01 Test 1, September 2018 Page 1 BROCK UNIVERSITY

Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods?

AST 1002 Section 1 (Dobrosavljevic) PLANETS, STARS, GALAXIES

Remember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st

chapter 10 questions_pictures removed.notebook September 28, 2017 Chapter 10 What We Know About the Universe Has Taken Us Thousands of Years to Learn

Discovering the Universe for Yourself

Name and Student ID Section Day/Time:

Name: Exam 1, 9/30/05

Today FIRST HOMEWORK DUE NEXT TIME. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy

Question 1. What motion is responsible for the apparent motion of the constellations (east to west) across the sky?

Guiding Questions. Discovering the Night Sky. iclicker Qustion

Test 1 Review Chapter 1 Our place in the universe

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe

Chapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0

A2 Principi di Astrofisica. Coordinate Celesti

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

SAMPLE First Midterm Exam

Name: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter.

[04] Seasons, Phases, and Eclipses (9/7/17)

2 OBSERVING THE SKY: THE BIRTH OF ASTRONOMY

a. 0.1 AU b. 10 AU c light years d light years

Astronomy I Exam I Sample Name: Read each question carefully, and choose the best answer.

Chapter 3: Ancient Astronomy

The Celestial Sphere. Chapter 1. Constellations. Models and Science. Constellations. Diurnal vs. Annular Motion 9/16/2010

Planetary Motion from an Earthly Perspective

Astronomy 101 Exam 1 Form A

BROCK UNIVERSITY. Test 1: October 2014 Number of pages: 9 Course: ASTR 1P01, Section 2 Number of students: 950

CHAPTER 2 A USER'S GUIDE TO THE SKY

PHYS 160 Astronomy Test #1 Name Answer Key Test Version A

10/17/2012. Observing the Sky. Lecture 8. Chapter 2 Opener

Astronomy Club of Asheville March 2018 Sky Events

Astronomy 102: Stars and Galaxies Examination 1 February 3, 2003

Guidepost. Chapter 2 A User s Guide to the Sky. Constellations Constellations (2) 8/27/2015. Outline. Outline (continued)

Transcription:

Announcements First MIDTERM Exam: This Thursday, Sep. 9, covering chapters 1 2. Short review later today Homework #1: Due last Fri. 10% penalty/day remains in effect; if you haven t finished, still worth it Essay questions: your grade will likely increase after we have graded your written answers.

Universe=Time Machine Light is fastest in the universe: (~200,000 miles per second!), but the universe is big! The amount of time it takes light to reach us: Moon: 1 second Sun: 8 minutes Sirius: 8 years Andromeda Galaxy: 2.5 million years

We can see the earliest stars and galaxies in the universe when they were born!

Last Time Earth s axis precesses slowly like a top. Polaris won t always be the north star! Phases of the moon: not due to shadow of earth on moon, but geometry of earth-moonsun (remember the styrofoam ball!). Half the moon is always illuminated (except during lunar eclipses). Moon slips on the celestial sphere, like the sun, but much faster, moving 1/2 per hour! Rises ~52min earlier each day.

Last Time Eclipses occur when moon falls in earth s shadow (lunar) or earth falls in moon s shadow (solar). Eclipses are rare because the moon s orbit around the earth is tipped 5 relative to the earth s orbit around the sun. Both occur at the same frequency, but lunar seen by half the earth, solar only a small region on the earth s surface.

Upcoming Eclipses Aug 21, 2017 (time is UT = EST + 5hrs = EDT + 4hrs)

Upcoming Eclipses April 8, 2024

Why is a Lunar eclipse visible over a larger area of the earth than a solar eclipse? A) During eclipse, the moon is further from the sun than the earth. B) The shadow of the earth at the moon is larger than the shadow of the moon at the earth. C) Roughly Half the earth is facing the moon during lunar eclipse. A C B D

Why is a Lunar eclipse visible over a larger area of the earth than a solar eclipse? A C B D A) During eclipse, the moon is further from the sun than the earth. B) The shadow of the earth at the moon is larger than the shadow of the moon at the earth. C) Roughly Half the earth is facing the moon during lunar eclipse.

An Eclipse of the sun from somewhere else (the Stereo B spacecraft). APOD/2007-03-03

An Eclipse of the sun from somewhere else (the Stereo B spacecraft). APOD/2007-03-03

The Science of Astronomy Astronomy has at its roots the observation of patterns in the night sky: motion of the sun and moon phases of the moon eclipses motion of the planets

Motions of the Planets Planet = Greek for wanderer 5 visible planets (others too faint): Mercury, Venus, Mars, Jupiter, Saturn Total of 7 wandering objects (including Sun and Moon).

Planet Location Planets always found in Zodiac 18º wide belt centered on ecliptic Mercury and Venus always close to sun Mars, Jupiter, Saturn seen everywhere (in Zodiac) Sometimes near sun (conjunction) Sometimes opposite to sun (opposition)

What is Science scientia: knowledge. Not all knowledge comes from science.

Science is a Human endeavor Perceptions: sight, touch, etc. The sky looks blue. Curiosity: A question regarding your perception. Why is the sky blue? Imagination: come up with a possible explanation (hypothesis). The sky reflects the blue oceans Skepticism: Test the hypothesis playing devils advocate Wrong. No oceans in Arizona

Science is a Human endeavor Perceptions: sight, touch, etc. The sky looks blue. Curiosity: A question regarding your perception. Why is the sky blue? Imagination: come up with a possible explanation (hypothesis). The sky reflects the blue oceans Skepticism: Test the hypothesis playing devils advocate Wrong. No oceans in Arizona

What is science? There is something fascinating about science. One gets such wholesale returns of conjecture out of such a trifling investment of fact. Mark Twain Not a perfect enterprise.

Hallmarks of Science Natural Causes: Scientific models invoke only natural causes. Occam s razor: Simplest possible model is (usually) the best. Verifiability: Others must be able to verify findings. Falsifiability: Scientific models or theories must make predictions. If they don t agree, the model will be abandoned.

That s just like your theory, dude. A scientific theory is different from a hypothesis. It must: 1. Explain a wide variety of observations with a few simple principles, AND 2. be supported by a large, compelling body of evidence, AND 3. not have failed any crucial tests of validity.

Can Theories be wrong? Yes! (remember falsifiability?) newton s law of gravity stood for 200 years. Einstein showed that newton s law only works in certain situations (like those we encounter on earth).

Examples of non-science UFO s: no one can verify an individual UFO account. astrology (which is not astronomy): predictions no better than random chance. Plenty of useful fields of knowledge are non-scientific it s not an insult. Example: Learning to sing.

Planets Known in Ancient Times Mercury: difficult to see, always close to the Sun Venus: bright, morning or evening star Mars: Red Jupiter: very bright Saturn: moderately bright

Venus, Mercury, Mars from Perth, Australia APOD/2008 09 12

The Planet s Motion Planets wander on the celestial sphere, slipping day by day, just like the sun and the moon, but less uniform in motion. Diurnal motion like fixed stars Rise in east Transit high/low in south (from the Northern hemisphere) Set in west Usually slipping from W to E, but varying in speed and brightness.

How did the Greeks explain planetary motion? The underpinnings of the Greek geocentric model were laid by Aristotle: The Earth is at the center of the Universe Heavens are perfect : objects move on perfect circles or spheres.

But how do you explain this? Mars (and to lesser extent, Jupiter and Saturn) seems to stop, turn around!, and then continue across the sky throughout the year. Time-lapse photograph of Mars as it moves through the sky over many weeks

A B Where Would You Look To See A Planet Rise When It Is In Retrograde Motion? A) Near The Eastern Horizon B) Near The Western Horizon C) It never rises C D

A B Where Would You Look To See A Planet Rise When It Is In Retrograde Motion? C D A) Near The Eastern Horizon B) Near The Western Horizon C) It never rises

Retrograde Motion? Naturally explained by the earth catching up to and lapping the other planet in their mutual orbits around the sun. Interactive Fig. 2.27.

You observe Mars and find that it is undergoing retrograde motion. What time does it transit? A) About 6am B) Noon C) About 6pm D) Midnight A C B D

Being lapped At opposition! You observe Mars and find that it is undergoing retrograde motion. What time A C B D does it transit? A) About 6am B) Noon C) About 6pm D) Midnight Where is the sun?

Being lapped At opposition! You observe Mars and find that it is undergoing retrograde motion. What time A C B D does it transit? A) About 6am B) Noon C) About 6pm D) Midnight Where is the sun?

A planet is moving in retrograde motion. Over the course of several nights, how will the planet appear to move relative to the background stars? A) east to west B) west to east C) It will not move at all, as planets do not move with the stars. D) It will move randomly, as planets move differently than the stars.

A planet is moving in retrograde motion. Over the course of several nights, how will the planet appear to move relative to the background stars? A) east to west B) west to east C) It will not move at all, as planets do not move with the stars. D) It will move randomly, as planets move differently than the stars.

Ancient Astronomy Earliest recorded astronomy: Babylonian/Egyptian. Chinese. Mayan. Early religion and astronomy: Association of objects in the sky with gods. Planets=lesser gods.

Planets and Gods of Mythology Planet Babylonian Greek Roman German/Norse Sun Shamash Helios Sôl Moon Sin Selenê Luna Mercury Nabû Hermes Mercurius Wotan/Odin Venus Ishtar Aphroditê Venus Fria/Freda/Frigg Mars Nergal Ares Mars Tiw Jupiter Marduk Zeus Iuppiter Thor Saturn Ninurta Kronos Saturnus

Features of Ancient Astronomy Time of day/time of year/seasons. Other calendars: e.g. the Lunar calendar (as opposed to our solar calendars), still in use in the Muslim religion. Some (e.g. jewish calendar) synchronized lunar and solar.

An Egyptian obelisk was used to tell time

Stonehenge (completed around 1550 B.C.)

Chaco Canyon, NM Winter Solstice Summer Solstice

Yucatan, Mexico: Mayan Observatory

Mid-Term Exam #1 Review Chapters 1 2 Class Exercises/Concept Questions. General Physical concepts stressed. Applied understanding of motions of earth/ moon/sun/stars/planets

Suggestions Review Big Picture, Key Concepts and Review Questions & Problems at end of each chapter. Even Better way: use the Study Area on MasteringAstronomy (nothing here is graded!). Some questions taken directly from Reading Quiz/Concept Quiz. Know how to apply concepts.

Concepts Covered Relative Size scales of the Universe. Finite speed of light: Further an object, the further back in time we see it. Things in the universe: planet, moons, comet, asteroid, star, solar system, Nebulae, galaxy, clusters. Age of the universe, and its relation to age of earth, life on earth, humankind, etc.

Concepts Covered Constellations The celestial sphere, meridian, zenith. Diurnal motions of the stars (rise/set/transit). What stars we see based on our latitude on earth. Where an object is on the celestial sphere to rise Due East, or to transit overhead (at the zenith ) Circumpolar stars. Our system of Time, based on the sun s position!

Concepts Covered Sidereal vs. solar day (Turning a little bit further ) Star rise times day by day Angular Sizes: sun, moon, angles vs. distance. Motions on the celestial sphere (why?). Sun s motion on the celestial sphere (as a consequence of earth s orbit around the sun). Ecliptic: circular path of sun through celestial sphere.

Sun/Ecliptic/Tilt Special locations on the ecliptic = special times of year: solstices, equinox. Tilt of the earth s axis compared to plane of its orbit the reason for seasons. Precession of the earth s axis. movement of the sun from S to N and back again through the year. How high does the sun go?

At some point during the summer in Toledo, the Sun passes directly overhead (at the zenith point). A) True B) False A C B D

At some point during the summer in Toledo, the Sun passes directly overhead (at the zenith point). A C B D A) True B) False

The Moon Motion of the moon on the sky. Orbit of the moon around earth. Phases of the moon (and when you see them!).

Eclipses Lunar vs. solar eclipses. Different types of eclipses. Why aren t eclipses more common? Why is one type more commonly seen than the other? Near coincidence of moon s and sun s angular sizes

Planetary motion Where planets are found on the sky ( the zodiac ). The 7 wandering objects on the sky. Retrograde motion: what causes it? Normal slippage motion of planets on the celestial sphere.

Reminders Exam on Thursday Closed Book/Notes Study on M.A./Concept quizzes, go over homework, etc. Bring a sharp #2 pencil