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

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

A2 Principi di Astrofisica. Coordinate Celesti

Seasons. What causes the seasons?

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

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

Astronomy 101: 9/18/2008

Reminder: Seasonal Motion

Introduction to Astronomy

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

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

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

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

Motions of the Earth

Earth-Sun Relationships. The Reasons for the Seasons

Summary Sheet #1 for Astronomy Main Lesson

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

Topic Guide: The Celestial Sphere. GCSE (9-1) Astronomy. Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0)

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

Introduction To Modern Astronomy I: Solar System

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

Phys Lab #1: The Sun and the Constellations

Lecture 2 Motions in the Sky September 10, 2018

UNIT 3: EARTH S MOTIONS

(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?

A Warm Up Exercise. The Motion of the Sun. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise

Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION

Chapter 4 Earth, Moon, and Sky 107

Celestial Sphere Spectroscopy (Something interesting; e.g., advanced data analyses with IDL)

Astronomy 115 Section 4 Week 2. Adam Fries SF State

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

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

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

(1) Over the course of a day, the sun angle at any particular place varies. Why?

Practice Questions: Seasons #1

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

Knowing the Heavens. Goals: Constellations in the Sky

CHAPTER 2 A USER'S GUIDE TO THE SKY

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

The Earth-Moon-Sun System

Earth s Orbit. Sun Earth Relationships Ridha Hamidi, Ph.D. ESCI-61 Introduction to Photovoltaic Technology

Knowing the Heavens. Goals: Constellations in the Sky

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

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Motion of the Sun. motion relative to the horizon. rises in the east, sets in the west on a daily basis. Basis for the unit of time, the DAY

Oberth: Energy vs. Momentum

6/17. Universe from Smallest to Largest:

4 Solar System and Time

The Sky Perceptions of the Sky

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

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

C) wavelength C) eastern horizon B) the angle of insolation is high B) increases, only D) thermosphere D) receive low-angle insolation

CELESTIAL COORDINATES

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

Astr 1050 Mon. Jan. 31, 2017

Student Exploration: Seasons in 3D

C) the seasonal changes in constellations viewed in the night sky D) The duration of insolation will increase and the temperature will increase.

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

ClassAction: Coordinates and Motions Module Instructor s Manual

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.

Cartesian Coordinates Need two dimensional system 2 number lines perpendicular to each other X-axis is horizontal Y-axis is vertical Position relative

Seasons ASTR 101 2/12/2018

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

Physics 312 Introduction to Astrophysics Lecture 3

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

Astronomy 101 Exam 1 Form A

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

Aim: What causes Seasons?

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.

James T. Shipman Jerry D. Wilson Charles A. Higgins, Jr. Chapter 15 Place and Time

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

Planet Earth. Part 2

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

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

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.

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.

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

LAB: What Events Mark the Beginning of Each Season?

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

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

SUBJECT : GEOGRAPHY ROTATION AND REVOLUTION This paper consists of 5 printed pages.

Exercise 7.0 THE CHANGING DIURNAL CIRCLES OF THE SUN

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

Observing the Universe for Yourself

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

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

Aileen A. O Donoghue Priest Associate Professor of Physics

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

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

Astronomical coordinate systems. ASTR320 Monday January 22, 2018

Meridian Circle through Zenith, North Celestial Pole, Zenith Direction Straight Up from Observer. South Celestial Pole

Astronomy 291. Professor Bradley M. Peterson

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

Astronomy 100 Section 2 MWF Greg Hall

Name: Exam 1, 9/30/05

Precession and The Celestial Poles

ASTRO Fall 2012 LAB #2: Observing the Night Sky

Fundamentals of Satellite technology

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

Transcription:

Sun: rises in the east sets in the west travels on an arc across the sky 24 hours Daily Motions Solar Day = 24 hours Stars: stars travel on arcs in the sky moving from east to west. some stars rise and set others do not and are circumpolar due to Rotation of Earth 23 hour 56 min Daily Motions Sidereal Day = 23 hours 56 min Solar and Sidereal Days Why is the Solar Day longer than the Sidereal Day? Annual Motions of the Sun The altitude of the Sun changes with season It reaches a maximum on the summer solstice (June 21 in the northern hemisphere) Its minimum altitude is reached on the winter solstice (December 21 in the northern hemisphere) The sunrise and sunset points along the horizon also change with season It rises and sets due east on the equinox (Sep 21, and March 21) It rises north of east in the summer south of east in the winter Annual Motion of the Stars Coordinate system on Earth Every day a given star or constellation rises and sets 4 minutes earlier with respect to the Sun Therefore after one year it returns to the same position relative to the Sun Gainesville: 29.6510N, 82.3250W 1

Celestial Sphere You can imagine that the stars and sun are attached to the surface of a great sphere The earth appears to be at the center of the sphere The sphere rotates from east to west on an axis that points to the north celestial pole To explain the daily motions of the sky you can imagine the sphere rotating once in 23 hours 56 minutes Parts of the Celestial Sphere Celestial pole - extends from the rotation axis of the earth all stars appear to rotate about this point some stars are circumpolar some stars rise & set Celestial equator - extends from the earth s equator Your latitude on earth determines the angle at which stars will rise & set with respect to your local horizon Where are we? The position of a celestial pole near the horizon, tells us we must be near the Equator. Also consider the angles the star trails make with the horizon: 90 degrees. Question You are kidnapped, drugged and placed in a dark room for an indefinite period of time! You escape and find a radio to call for help but you don t know where you are! Luckily, it s a clear night. You watch the stars for while and you see the stars rising at a 20 degree angle with respect to your horizon. What can you tell your rescuers about your location? 2

Annual Motion of Sun The sun moves along a repeatable path on the celestial sphere throughout the year. This path is called the ECLIPTIC Sun moves east ward relative to stars on celestial sphere It moves 360 degrees in a year about 1 degree per day The constellations through which we see the sun move are the constellations of the ZODIAC This apparent motion is due to the Earth orbiting the Sun Annual Motions of the Stars The constellations that are visible on a given night are those opposite from the Sun on the celestial sphere Thus you see different stars at different times of the year as the Sun moves along the ecliptic relative to the stars The apparent motion is due to the Earth orbiting the Sun Annual Motions of the Stars Coordinate system on Earth Gainesville: 29.6510N, 82.3250W Coordinate Systems Altitude : angular distance above horizon Azimuth : angular distance measured along horizon to location of object By convention azimuth is measured from the north going eastward Advantages Disadvantages Equatorial Coordinate System Declination the angular distance of a star along a circle north or south of celestial equator (degrees:arcmin:arcsec) Right Ascension the angular distance of a object measured eastward from the vernal equinox along the celestial equator (H:M:S) 3

Seasons With the annual motion of the Earth around the Sun, we notice a cyclic pattern in the weather, known as the seasons. Observations: Seasons are reversed in the Northern and Southern Hemispheres For example, you re at the beach at Cape Cod in July, they re skiing in New Zealand! The region near the equator is hottest; poles are the coldest The Sun s position in the sky changes Reasons for the Seasons? What causes this pattern? Two Possible Models: Distance of the Earth from the Sun? Tilt of the Earth s axis with respect to the Earth s orbital plane (ecliptic) Reason for Seasons: Distance? Predictions: Relation between Earth-Sun distance and season for example, the Earth should be closest to the Sun in summer Same season every where on Earth since the Earth is tiny compared to the Earth- Sun distance Reason for Seasons: Distance? Observations: Reason for Seasons: Distance? Predictions don t match Observations: Seasons are reversed in the Northern and Southern Hemispheres For example, you re at the beach at Cape Cod in July, they re skiing in New Zealand! The Earth is closest to the Sun during northern winter Reason for the Seasons: Tilt? The Earth s axis of rotation is tilted by 23.5 degrees with respect to the ecliptic pole As the Earth moves around the Sun, the Earth s north pole points to a fixed position in space 4

Reason for the Seasons: Tilt? Predictions: Summer occurs in hemisphere pointed toward the Sun Winter occurs in the hemisphere pointed away from the Sun Therefore: Seasons are reversed in northern and southern hemisphere Reason for the Seasons: Tilt It s warmer in the summer and colder in the winter for two reasons: the Sun is higher in the sky in the summer the days are longer the Sun reaches it s highest point in the sky on the summer solstice (June 21 in northern hemisphere) Reason for the Seasons: Tilt The angle at which the Sun s rays strike the surface of the Earth is closer to a right angle (90 degrees) in the summer Therefore the Earth s surface intercepts more rays of Sunlight and hence more energy This is the main reason that it is warmer in the summer Reason for the Seasons Demonstration Reason for the Seasons: Tilt Predictions match observations: The northern hemisphere and southern hemisphere seasons are reversed The region near the equator is hottest; poles are coldest Question When is the hottest time of year in Quito Ecuador? If the Earth s rotation axis was perpendicular to it s orbital plane (ecliptic), what would you expect the seasons to be like? If the Earth s rotation axis was parallel to it s orbital plane (ecliptic), what daily and annual effects would this have? 5

Temperature in Ecuador Gainesville: 29.6510N, 82.3250W What is special about the Tropics (i.e. between +23.5degrees and -23.5 degrees latitude)? Assignment Reference Reading Astronomy & Astrophysics by Zelik and Gregory - chapter 1, chapter 3, chapter 4-1 & 4-2 The Physical Universe, An Introduction to Astronomy by Shu 6