Day, Night & the Seasons. Lecture 2 1/15/2013

Similar documents
Day, Night & the Seasons. Lecture 2 1/21/2014

Celestial Sphere & Solar Motion Lab (Norton s Star Atlas pages 1-4)

What do you think? 2/3/09. Mastering Astronomy Assignment 2. Constellations the 88 semi-rectangular regions that make up the sky

Motions of the Earth

Time, coordinates and how the Sun and Moon move in the sky

Using Angles. Looking at the Night Sky. Rising and Setting Stars. Nightly Motion of the Stars. Nightly Motion of the Stars

Daily Motions. Daily Motions. Solar and Sidereal Days. Annual Motions of the Sun. Coordinate system on Earth. Annual Motion of the Stars.

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

How can we describe the motion of the sun in the sky? Where is the Sun at noon today? What about the path of the Sun?

Astronomy 115 Section 4 Week 2. Adam Fries SF State

Lecture 2 Motions in the Sky September 10, 2018

Astronomy 122 Section 1 TR Outline. The Earth is Rotating. Question Digital Computer Laboratory

Local Coordinates. These are centered upon you, the observer.

What causes the seasons? 2/11/09

Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION

Astronomy 101: 9/18/2008

Discovering the Night Sky

Discovering the Night Sky

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

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

A2 Principi di Astrofisica. Coordinate Celesti

Chapter 2 Discovering the Universe for Yourself

The. Astronomy is full of cycles. Like the day, the month, & the year In this section we will try to understand these cycles.

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

Chapter 2 Discovering the Universe for Yourself

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

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

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

Summary Sheet #1 for Astronomy Main Lesson

Phases of the Moon. Two perspectives: On Earth, or outside the Moon s orbit. More Phases. What if we zoom out? Phases of the Moon Demo 2/3/17

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

ASTRO Fall 2012 LAB #2: Observing the Night Sky

Day, Night, Year, and Seasons

Seasons Page 520. A. What Causes Seasons?

Daylight Data: Days and Nights Around the World

b. So at 12:00 p.m., are the shadows pointing in the direction you predicted? If they are not, you must explain this observation.

Ch. 2 Discovering the Universe for Yourself

Go to Click on the first animation: The north pole, observed from space

Physics Lab #4:! Starry Night Student Exercises I!

Observing the Universe for Yourself

Seasons. What causes the seasons?

Eclipses September 12th, 2013

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

Phys Lab #1: The Sun and the Constellations

The Earth and the Sky

The Sky Perceptions of the Sky

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

5 - Seasons. Figure 1 shows two pictures of the Sun taken six months apart with the same camera, at the same time of the day, from the same location.

6/17. Universe from Smallest to Largest:

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

Lecture #03. January 20, 2010, Wednesday

Oberth: Energy vs. Momentum

5 - Seasons. Figure 1 shows two pictures of the Sun taken six months apart with the same camera, at the same time of the day, from the same location.

LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME. a. understand the basic concepts needed for any astronomical coordinate system.

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

The following terms are some of the vocabulary that students should be familiar with in order to fully master this lesson.

Introduction To Modern Astronomy I: Solar System

The Earth, Moon, and Sky. Lecture 5 1/31/2017

REVIEW CH #0. 1) Right ascension in the sky is very similar to latitude on the Earth. 1)

Practice Exam #3. Part 1: The Circumpolar Constellations

Reading Reminders. Your Questions via JiTT2

November 20, NOTES ES Rotation, Rev, Tilt.notebook. vertically. night. night. counterclockwise. counterclockwise. East. Foucault.

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.

Academic Year Second Term. Science Revision Sheet. Grade

Practice Questions: Seasons #1

Exercise 7.0 THE CHANGING DIURNAL CIRCLES OF THE SUN

Knowing the Heavens. Goals: Constellations in the Sky

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.

Astronomy 100 Section 2 MWF Greg Hall

Knowing the Heavens. Goals: Constellations in the Sky

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

Tilted Earth Lab Why Do We Have Seasons?

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

Viewed from Earth's north pole, the rotation of Earth and its moon are counter-clockwise.!

The sky and the celestial sphere

Planet Earth. Part 2

Chapter 4 Earth, Moon, and Sky 107

(1) How does the annual average sun angle at solar noon (that is, the sun angle at noon averaged over a full year) depend on latitude?

Introduction To Astronomy Lesson 1

Reminder: Seasonal Motion

Earth-Sun Relationships. The Reasons for the Seasons

Exercise 2: The UW planetarium

Astronomical coordinate systems. ASTR320 Monday January 22, 2018

Name: Exam 1, 9/30/05

ClassAction: Coordinates and Motions Module Instructor s Manual

The Sun-Earth-Moon System

PHYS 160 Astronomy Test #1 Fall 2017 Version B

The Ecliptic on the Celestial. Sphere. The Celestial Sphere. Astronomy 210. Section 1 MWF Astronomy Building. celestial equator are not

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position.

Physics Lab #2: Learning Starry Night, Part 1

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

Your web browser (Safari 7) is out of date. For more security, comfort and the best experience on this site: Update your browser Ignore

Astronomy. The Seasons

Name EMS Study Guide. Two important objects that travel around our star are: Planets are not - they don t give off light like stars do

Astronomy 11. No, this course isn t all about Star Wars

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

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

AST 2010 Descriptive Astronomy Study Guide Exam I

Chapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc.

Admin. 8/29/17. If you re at North Pole, you ll NEVER see stars that are below your horizon. Key Concepts: Lecture 4

Transcription:

Day, Night & the Seasons Lecture 2 1/15/2013

Logistics The following students see me after class: Dahms, Doyle, Kavalle, Jennings, Melton, Polsky, Soriano, Augustinovich, Briggs Anyone who was not here on first day see me after class Pin Numbers - if you have not set one up, see me after class MUST bring Lecture Tutorials for Introductory Astronomy to every lecture Any problems with website? 2

Why is Science important? One of the most beautiful things about science is that it equips you to think for yourself Adrian Gaylord The video Why Science mentions several reasons why science is important, which resonated with you best and why?

Motion of Earth Earth rotates, orbits and is tilted This motion/orientation of the Earth accounts for: Rising and Setting of the Sun Visible stars/constellations Seasons 4

Rotation: Earth Rotates

Orbit: The Earth orbits the Sun The ecliptic is the path of the Sun along the celestial sphere (apparent path of Sun in sky) (a little relativity) it is also the path of the Earth in its orbit around the Sun

Orientation The Earth has an obliquity Obliquity is the tilt of planets rotation axis with respect to the ecliptic The Earth s rotation axis is tilted 23.5 o from perpendicular to the ecliptic plane

Earth s Rotation causes night and day The Earth rotates on its axis once a day This rotation causes the appearance that the Sun rises in the East and sets in the West Night time is when our position on Earth rotates out of the light. We can see Earth s rotation in stellar motion

At night we see Stars 9

The Constellations When we look at the night sky we see patterns, which we call constellations. Many famous constellations such as Orion, Gemini, Virgo

The Celestial Sphere To locate stars in the night sky astronomers created a sky map, called the Celestial Sphere A sphere centered on Earth: Equator is extension of Earth s equator Longitude - Right Ascension measured from vernal equinox Latitude - Declination

What do you think? Do the stars stay in the same position in the sky all day/night long? Do we see the same stars all year round every night?

What do you think? What causes the stars to move? Do the stars actually move in the way they appear from Earth?

Class Demo Lets set up: What is at the center of the Solar System? The Earth the Sun? The stars and constellations are closer/farther from Earth than the Sun? The constellations/stars are the same/different distance from the Sun?

Orbit: The Earth orbits the Sun The ecliptic is the path of the Sun along the celestial sphere (apparent path of Sun in sky) (a little relativity) it is also the path of the Earth in its orbit around the Sun

The Seasons http://www.youtube.com/watch?v=_xln5-1qgrm 16

Which of these are true and which are false and what evidence is there to support your answer? Earth is closer to the Sun in summer than it is in the winter. When it is summer, the Sun is giving off more energy and when it is winter the Sun is giving off less energy. When it is summer, more sunlight reaches Earth than it does during the winter.

The Seasons The Earth has an obliquity Obliquity is the tilt of planets rotation axis with respect to its orbit around the Sun The Earth s rotation axis is tilted 23.5 o from perpendicular to the ecliptic plane

The Seasons Vernal Equinox Northern Hemisphere Winter Solstice Northern Hemisphere Summer Solstice Northern Hemisphere Autumnal Equinox Northern Hemisphere Seasons are caused by the tilt of the Earth s rotation axis In (our) Summer, Northern Hemisphere is tilted toward Sun. In Winter Northern Hemisphere is tilted away from the Sun.

The Seasons

Where would the Sun be on your birthday?

Seasons In summer months Sun is higher in the sky, more hours of sunlight, more heat Sun is more intense, more heat

Position of Sun in Sky also depends on latitude Equator 20 o 50 o 70 o 23

When the Sun is high in the sky during the day, the number of daylight hours is greater and the amount of direct sunlight received is greater. This results in Summer.

When the Sun is low in the sky during the day, the number of daylight hours is less and the amount of direct sunlight received is less. This results in Winter.

Lecture Tutorial (p.93): Seasons Work with a partner! Read the instructions and questions carefully. Discuss the concepts and your answers with one another. Come to a consensus answer you both agree on. If you get stuck or are not sure of your answer, ask another group. If you get really stuck or don t understand what the Lecture Tutorial is asking, ask one of us for help.

The Reason for Seasons The obliquity (tilt) of the Earth causes two effects that lead to seasons 1. Longer/Shorter daylight hours 2. More/Less intense sunlight Seasons are not caused by Earth being closer/further from the Sun Seasons are not caused by the tilt allowing certain latitudes to be closer/further from the Sun Seasons are not a distance effect 27