SOLAR GEOMETRY (AND SOLAR RADIATION)

Size: px
Start display at page:

Download "SOLAR GEOMETRY (AND SOLAR RADIATION)"

Transcription

1 SOLAR GEOMETRY (AND SOLAR RADIATION) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 1 Solar Radiation Components glass will reflect some incoming radiation; absorb some; and transmit some SHGF (above) is solar heat gain factor a measure of the quantity of solar energy that will pass through a sheet of single-pane clear glass at a given time of the year for a given orientation under design conditions Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 2 1

2 Solar Radiation: A Resource or a Problem? force mitigating element: building envelope resultant radiation is an environmental force; it can be an asset or a liability depending upon site/project//context/opr Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 3 Solar Context Distance Sun Earth the solar constant is a mean value of the solar radiation intensity found at the edge of the Earth s atmosphere solar constant (Btuh/sq ft) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 4 2

3 Solar Context Tilt the tilt of the Earth s axis, relative to the sun s position, accounts for the seasons (as solar angle of incidence changes) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 5 Site Context Latitude Muncie s latitude is approximately 40 deg N (a convenient latitude often used in design data tables) latitude locates a site in the north-south context, relative to the equator Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 6 3

4 Mitad del Mundo, Quito marking the equator Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 7 Site Context Longitude Muncie = apx. 85 deg W longitude locates a site in the east-west context, relative to the prime meridian (in Greenwich, England) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 8 4

5 Greenwich, England prime meridian Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 9 Solar-Site Context summer spring/fall NORTHERN HEMISPHERE winter the sun follows defined and predictable paths on a daily and annual basis Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 10 5

6 Solar Angles Altitude ALTITUDE ANGLE the angle between a horizontal ground plane and the line describing the position of the sun in the sky vault Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 11 Altitude Angle Patterns noon noon altitude angle; describes height of the sun in the sky varies with month and time of day Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 12 6

7 Altitude Angle Patterns << site latitude for any given month and time, altitude angle varies with latitude Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 13 Solar Angles Azimuth AZIMUTH ANGLE the angle between south and the position of the sun in the sky vault as projected onto the horizontal ground plane Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 14 7

8 Azimuth Angle Patterns azimuth angle varies with month and time of day; range is most extensive in summer Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 15 Solar Position Relative to Site conceptually simple, but three-dimensional Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 16 8

9 Solar Position Conventions Azimuth angle is usually measured from South in architecture but sometimes from the North in other disciplines (or in the Southern hemisphere) South is always solar South; not magnetic South or plan South see next slide Altitude angle is measured from the horizontal Times are always expressed as solar time see upcoming slide Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 17 South, Souther, Southiest Plan South is usually an arbitrary designation used for convenience Solar South is by definition the position of the sun at solar noon Solar South marks the center of symmetry of the daily solar path Solar South differs from Magnetic South (as read on a compass) by the local magnetic deviation value Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 18 9

10 Magnetic Deviation solar reference magnetic deviation compass reference magnetic deviation magnetic deviation varies with site location Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 19 Magnetic Deviation zero deviation line designing for east-central Indiana is not too deviant Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 20 10

11 Solar versus Clock Time LST CT + DST local solar time = clock time +/- equation of time value +/- (4)(local standard time meridian local longitude) +/- daylight saving time adjustment example, Muncie, June 21: latitude adjustment = (4)(75-85) = -40 minutes; DST adjustment = 60 minutes; ET adjustment = -3 minutes bottom line: solar and clock time are rarely identical, and can differ by +/- an hour; this matters when solar loads are combined with clock-based loads Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 21 Clock Time Influences equation of time US time zones (political devices) and time zone reference meridians; the sun is not influenced by politics Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 22 11

12 Sunpath Information The sun s location at any time can be accurately predicted. Such information is readily available in several formats: Graphic sunpath diagrams: Horizontal projection diagrams (including the SBSE Sun Angle Calculator) Vertical projection diagrams Sunpeg diagrams Tabular data (as in the ASHRAE Handbook) Online calculators (interactive databases) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 23 Sunpath Diagrams horizontal projection sunpath diagram l-e-s-s.co.uk/guides/physics/solargeometry.htm sun paths for selected days can be projected downward onto a horizontal plane (the plane is a surrogate for the Earth s surface) to generate a diagram Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 24 12

13 Sunpath Diagrams Pilkington Sun Angle Calculator available from SBSE via CERES sun paths for multiple latitudes are provided, with usability enhancements Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 25 Sunpath Diagrams vertical projection sunpath diagram sun paths for selected days can be plotted on a vertical surface (acting as a surrogate for the site horizon) to generate a diagram Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 26 13

14 Sunpath Diagrams sunpeg diagram primarily used to properly orient a scale model to the sun (real or simulated); the shadow cast by the peg (gnomon) shows date and time Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 27 Tabular Solar Position Data Mechanical and Electrical Equipment for Buildings (10 th ed) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 28 14

15 Online Solar Position Data susdesign.com/sunangle/ Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 29 Why Architects Should Understand Solar Geometry abcnews.go.com/ Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 30 15

SOLAR GEOMETRY (AND RADIATION)

SOLAR GEOMETRY (AND RADIATION) SOLAR GEOMETRY (AND RADIATION) Ball State Architecture ENVIRONMENTAL SYSTEMS 1 Grondzik 1 Solar Radiation Components glass will reflect some incoming radiation; absorb some; and transmit some SHGF (above)

More information

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

Earth s Orbit. Sun Earth Relationships Ridha Hamidi, Ph.D. ESCI-61 Introduction to Photovoltaic Technology 1 ESCI-61 Introduction to Photovoltaic Technology Sun Earth Relationships Ridha Hamidi, Ph.D. Spring (sun aims directly at equator) Winter (northern hemisphere 23.5 tilts away from sun) 2 Solar radiation

More information

Chapter Seven. Solar Energy

Chapter Seven. Solar Energy Chapter Seven Solar Energy Why Studying Solar energy To know the heat gain or heat loss in a building In making energy studies In the design of solar passive homes. Thermal Radiation Solar spectrum is

More information

ME 476 Solar Energy UNIT THREE SOLAR RADIATION

ME 476 Solar Energy UNIT THREE SOLAR RADIATION ME 476 Solar Energy UNIT THREE SOLAR RADIATION Unit Outline 2 What is the sun? Radiation from the sun Factors affecting solar radiation Atmospheric effects Solar radiation intensity Air mass Seasonal variations

More information

announcements 5/1/08 L10 Analysis and Design Tools 5/1/08 Analysis and Design Tools

announcements 5/1/08 L10 Analysis and Design Tools 5/1/08 Analysis and Design Tools Analysis and Design Tools ARCH 331/431 Spring 2008 Lecture 10 announcements 5/1/08 Information Meeting: INDIA program winter 2009 Friday May 2, 12:30, Gould 208P Assignment 4: Shading Model Studies Available

More information

Lecture #03. January 20, 2010, Wednesday

Lecture #03. January 20, 2010, Wednesday Lecture #03 January 20, 2010, Wednesday Causes of Earth s Seasons Earth-Sun geometry Day length Solar angle (beam spread) Atmospheric beam depletion Shape and Size of the Earth North Pole E Geoid: not

More information

Chapter 1 Solar Radiation

Chapter 1 Solar Radiation Chapter 1 Solar Radiation THE SUN The sun is a sphere of intensely hot gaseous matter with a diameter of 1.39 10 9 m It is, on the average, 1.5 10 11 m away from the earth. The sun rotates on its axis

More information

EE Properties of Sunlight. Y. Baghzouz Professor of Electrical Engineering

EE Properties of Sunlight. Y. Baghzouz Professor of Electrical Engineering EE 495-695 2.2 Properties of Sunlight Y. Baghzouz Professor of Electrical Engineering Azimuth angle The azimuth angle is the compass direction from which the sunlight is coming. At the equinoxes, the sun

More information

Gnomon (a thin, round stick at least a foot long and capable of being put into the ground or stood up vertically)

Gnomon (a thin, round stick at least a foot long and capable of being put into the ground or stood up vertically) Name: Partner(s): Lab #3 Celestial Navigation Due 7/2 Objectives In this lab you will take measurements of the sun s motion around noon and the north star s position in the sky. You will use this data

More information

Astronomy 101: 9/18/2008

Astronomy 101: 9/18/2008 Astronomy 101: 9/18/2008 Announcements Pick up a golf ball at the front of the class or get one from Alex; you will need it for an in-class activity today. You will also need the question sheet from Alex.

More information

Module 2: Mapping Topic 2 Content: Determining Latitude and Longitude Notes

Module 2: Mapping Topic 2 Content: Determining Latitude and Longitude Notes Introduction In order to more easily locate points on a globe or map, cartographers designed a system of imaginary vertical lines (also called parallels) and horizontal lines (also called meridians) that

More information

Sunlight and its Properties Part I. EE 446/646 Y. Baghzouz

Sunlight and its Properties Part I. EE 446/646 Y. Baghzouz Sunlight and its Properties Part I EE 446/646 Y. Baghzouz The Sun a Thermonuclear Furnace The sun is a hot sphere of gas whose internal temperatures reach over 20 million deg. K. Nuclear fusion reaction

More information

Sunlight and its Properties II. EE 446/646 Y. Baghzouz

Sunlight and its Properties II. EE 446/646 Y. Baghzouz Sunlight and its Properties II EE 446/646 Y. Baghzouz Solar Time (ST) and Civil (clock) Time (CT) There are two adjustments that need to be made in order to convert ST to CT: The first is the Longitude

More information

Which Earth latitude receives the greatest intensity of insolation when Earth is at the position shown in the diagram? A) 0 B) 23 N C) 55 N D) 90 N

Which Earth latitude receives the greatest intensity of insolation when Earth is at the position shown in the diagram? A) 0 B) 23 N C) 55 N D) 90 N 1. In which list are the forms of electromagnetic energy arranged in order from longest to shortest wavelengths? A) gamma rays, x-rays, ultraviolet rays, visible light B) radio waves, infrared rays, visible

More information

Earth & Space Science, Interpreting Data DURATION Preparation: 5 minutes Activity: 40 minutes (total over one day)

Earth & Space Science, Interpreting Data DURATION Preparation: 5 minutes Activity: 40 minutes (total over one day) Objectives In this activity students will: 1. Observe how the position of the sun in the sky changes during the course of the day 2. Discover the cardinal directions by tracking the motion of the sun Materials

More information

Page 1. Name:

Page 1. Name: Name: 1) What is the primary reason New York State is warmer in July than in February? A) The altitude of the noon Sun is greater in February. B) The insolation in New York is greater in July. C) The Earth

More information

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

C) wavelength C) eastern horizon B) the angle of insolation is high B) increases, only D) thermosphere D) receive low-angle insolation 1. What is the basic difference between ultraviolet, visible, and infrared radiation? A) half-life B) temperature C) wavelength D) wave velocity 2. In New York State, the risk of sunburn is greatest between

More information

Practice Questions: Seasons #1

Practice Questions: Seasons #1 1. Seasonal changes on Earth are primarily caused by the A) parallelism of the Sun's axis as the Sun revolves around Earth B) changes in distance between Earth and the Sun C) elliptical shape of Earth's

More information

L.O: THE ANGLE OF INSOLATION ANGLE INSOLATION: THE ANGLE SUNLIGHT HITS THE EARTH

L.O: THE ANGLE OF INSOLATION ANGLE INSOLATION: THE ANGLE SUNLIGHT HITS THE EARTH L.O: THE ANGLE OF INSOLATION ANGLE INSOLATION: THE ANGLE SUNLIGHT HITS THE EARTH 1. The graph below shows air temperatures on a clear summer day from 7 a.m. to 12 noon at two locations, one in Florida

More information

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

Cartesian Coordinates Need two dimensional system 2 number lines perpendicular to each other X-axis is horizontal Y-axis is vertical Position relative General Physical Science Chapter 15 Place and Time Space and Time Einstein Space and time related Single entity Time is the 4 th dimension! Cartesian Coordinates Need some system to tell us where something

More information

The Earth is a Rotating Sphere

The Earth is a Rotating Sphere The Earth is a Rotating Sphere The Shape of the Earth Earth s Rotation ( and relative movement of the Sun and Moon) The Geographic Grid Map Projections Global Time The Earth s Revolution around the Sun

More information

LONGITUDE AND LATITUDE. Semi great circles joining the true or geographic poles of the earth (true meridians).

LONGITUDE AND LATITUDE. Semi great circles joining the true or geographic poles of the earth (true meridians). MERIDIANS OF LONGITUDE LONGITUDE AND LATITUDE Semi great circles joining the true or geographic poles of the earth (true meridians). They are measured from 0 to 180 degrees East and West of the PRIME MERIDIAN,

More information

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D)

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D) 1. The hottest climates on Earth are located near the Equator because this region A) is usually closest to the Sun B) reflects the greatest amount of insolation C) receives the most hours of daylight D)

More information

ME 430 Fundamentals of Solar Energy Conversion for heating and Cooling Applications

ME 430 Fundamentals of Solar Energy Conversion for heating and Cooling Applications ME 430 Fundamentals of Solar Energy Conversion for heating and Cooling Applications Lecture (1 of 2) Solar Energy Resource and Availability C. Cruickshank and S. Harrison 2008 The Solar Constant 1 Variation

More information

Motion of the Sun. View Comments

Motion of the Sun. View Comments Login 2017 Survey to Improve Photovoltaic Education Christiana Honsberg and Stuart Bowden View Comments Instructions 1. Introduction 2. Properties of Sunlight 2.1. Basics of Light Properties of Light Energy

More information

The Sun. Fabio Peron Università IUAV - Venezia. Earth-Sun relationships. The Sun. Photosphere (Emits much of the solar radiant power)

The Sun. Fabio Peron Università IUAV - Venezia. Earth-Sun relationships. The Sun. Photosphere (Emits much of the solar radiant power) Università IUAV Venezia Corso di Fisica Tecnica Ambientale Laboratorio Integrato Innovazione-Sostenibilità Sun and solar radiation Fabio Peron Università IUAV - Venezia The Sun The Sun Earth-Sun relationships

More information

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

The Celestial Sphere. Chapter 1. Constellations. Models and Science. Constellations. Diurnal vs. Annular Motion 9/16/2010 The Celestial Sphere Chapter 1 Cycles of the Sky Vast distances to stars prevent us from sensing their true 3-D arrangement Naked eye observations treat all stars at the same distance, on a giant celestial

More information

1.4j interpret simple shadow stick data to determine local noon and observer s longitude

1.4j interpret simple shadow stick data to determine local noon and observer s longitude 1.4j interpret simple shadow stick data to determine local noon and observer s longitude There are many opportunities for making observations of shadows cast with a vertical stick and the Sun. Observations

More information

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

Appearance of the Sky Orientation Motion of sky Seasons Precession (?) Today Appearance of the Sky Orientation Motion of sky Seasons Precession (?) The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The ecliptic is the Sun s apparent

More information

For most observers on Earth, the sun rises in the eastern

For most observers on Earth, the sun rises in the eastern 632 CHAPTER 25: EARTH, SUN, AND SEASONS WHAT IS THE SUN S APPARENT PATH ACROSS THE SKY? For most observers on Earth, the sun rises in the eastern part of the sky. The sun reaches its greatest angular altitude

More information

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

Appearance of the Sky Orientation Motion of sky Seasons Precession (?) Today Appearance of the Sky Orientation Motion of sky Seasons Precession (?) The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The ecliptic is the Sun s apparent

More information

APPENDIX F ACTIVITY #1 - CALCULATION OF THE TILT OF THE EARTH S AXIS AND THE OBSERVER S LATITUDE

APPENDIX F ACTIVITY #1 - CALCULATION OF THE TILT OF THE EARTH S AXIS AND THE OBSERVER S LATITUDE APPENDIX F ACTIVITY #1 - CALCULATION OF THE TILT OF THE EARTH S AXIS AND THE OBSERVER S LATITUDE The calculation of the Tilt of the Earth s Axis and the Observer s Latitude is essentially a reversal of

More information

Latitude and Longitude. North. Latitude. South

Latitude and Longitude. North. Latitude. South Latitude and Longitude North Latitude Longitude South 54 North America 55 Longitude Latitude United States 56 Latitude New York 72w 44n 42n 57 Site Location The site location is specified by a latitude

More information

3. The Sun s Position

3. The Sun s Position 3. The Sun s Position In order to understand how to collect energy from the sun, one must first be able to predict the location of the sun relative to the collection device. In this chapter we develop

More information

ILLUSTRATING SHADOWS TABLE OF CONTENTS

ILLUSTRATING SHADOWS TABLE OF CONTENTS ILLUSTRATING SHADOWS TABLE OF CONTENTS 316 pages Introduction Chapter Page Introduction and "A Quick Hands On Project" Part One 1 10 The approximate evolution of the dial 2 13 How the earth does its thing

More information

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

Chapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc. Chapter S1 Lecture The Cosmic Perspective Seventh Edition Celestial Timekeeping and Navigation 2014 Pearson Education, Inc. Celestial Timekeeping and Navigation 2014 Pearson Education, Inc. S1.1 Astronomical

More information

Principles of Energy Conversion Part 11A. Solar Energy Insolation

Principles of Energy Conversion Part 11A. Solar Energy Insolation Principles of Energy Conversion Part 11A. Solar Energy Insolation April 19, 2018 19 Solar Radiation 3 19.1 Overview and Background.............................. 3 19.2 Solar Energy......................................

More information

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

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations. Chapter 1: Discovering the Night Sky Constellations: Recognizable patterns of the brighter stars that have been derived from ancient legends. Different cultures have associated the patterns with their

More information

Penn State Project CANDLE

Penn State Project CANDLE Teachers: This lesson is dedicated to providing a foundational knowledge of the earth s geometrical relation to the sun and how to predict the suns position in the sky given a time, date, and position

More information

Oberth: Energy vs. Momentum

Oberth: Energy vs. Momentum 1 2 The Oberth Effect 3 Oberth: Energy vs. Momentum 4 The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2-dimensional surface the Celestial Sphere. 5 The Celestial

More information

Time Zones. Doug Fischer Geog 106 LRS

Time Zones. Doug Fischer Geog 106 LRS Time Zones Doug Fischer Geog 106 LRS Learning goals Students should be able to Explain time zones as a function of longitude Calculate time differences between different locations Demonstrate corrections

More information

Photovoltaic Systems Solar Radiation

Photovoltaic Systems Solar Radiation PowerPoint Presentation Photovoltaic Systems Solar Radiation The Sun Solar Radiation Sun- Earth Relationships Array Orientation Solar Radiation Data Sets Estimating Array Performance Arizona Solar Power

More information

Why does Earth rotate and what s the evidence? (besides watching it from space ships or satellites) Week 18 January 5, 2015

Why does Earth rotate and what s the evidence? (besides watching it from space ships or satellites) Week 18 January 5, 2015 Why does Earth rotate and what s the evidence? (besides watching it from space ships or satellites) Week 18 January 5, 2015 The sun determines our solar time everywhere on earth as Earth rotates. Can you

More information

Latitude and Longitude

Latitude and Longitude Latitude and Longitude Finding Your Location on a Sphere Coordinate Systems n When you are locating a point on a flat surface you can use Cartesian coordinates of x and y. n The point 2, 3 is plotted on

More information

CA1 2.11: Designing an Equatorial Sundial Activity

CA1 2.11: Designing an Equatorial Sundial Activity Purpose: To design an equatorial sundial and learn about motions of the sun and earth that have a bearing on its design. Materials: poster board, length of stiff wire or dowel rod, tape, protractor, ruler,

More information

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

LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME. a. understand the basic concepts needed for any astronomical coordinate system. UNIT 2 UNIT 2 LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME Goals After mastery of this unit, you should: a. understand the basic concepts needed for any astronomical coordinate system. b. understand

More information

Exercise 6. Solar Panel Orientation EXERCISE OBJECTIVE DISCUSSION OUTLINE. Introduction to the importance of solar panel orientation DISCUSSION

Exercise 6. Solar Panel Orientation EXERCISE OBJECTIVE DISCUSSION OUTLINE. Introduction to the importance of solar panel orientation DISCUSSION Exercise 6 Solar Panel Orientation EXERCISE OBJECTIVE When you have completed this exercise, you will understand how the solar illumination at any location on Earth varies over the course of a year. You

More information

Polar Sundial. Cut carefully on this line. Cut on this line.

Polar Sundial. Cut carefully on this line. Cut on this line. 1 The Sundial Primer - "Dialling Guides" The purpose of the "Dialling Guides" is to provide an easy method for laying out the hour lines for a number of polar sundials located at any latitude in either

More information

Complete the following: a. Lines of latitude are parallel to the equator. Name:

Complete the following: a. Lines of latitude are parallel to the equator. Name: Name: Date: Social Studies Introduction: Basic Geography Period: Latitude Latitude is defined as a measurement of distance in degrees north and south of the equator. The word latitude is derived from the

More information

Earth-Sun Relationships. The Reasons for the Seasons

Earth-Sun Relationships. The Reasons for the Seasons Earth-Sun Relationships The Reasons for the Seasons Solar Radiation The earth intercepts less than one two-billionth of the energy given off by the sun. However, the radiation is sufficient to provide

More information

Earth Science Seasons Test Name Per Date

Earth Science Seasons Test Name Per Date Name Per Date Page 1 1. The diagram below represents four positions of the Earth as it revolves around the Sun. 5. Base your answer to the following question on the diagram below, which shows the apparent

More information

Designing with the Pilkington Sun Angle Calculator

Designing with the Pilkington Sun Angle Calculator Designing with the Pilkington Sun Angle Calculator In 1951, Libbey-Owens-Ford introduced the first Sun Angle Calculator, to provide a relatively simple method of determining solar geometry variables for

More information

Lecture 4: August 30, 2010

Lecture 4: August 30, 2010 Lecture 4: August 30, 2010 How many hospitals are there in the USA? Announcements: First homework has been posted Due Friday (10 th ) First Observatory Opportunity Thursday Night September 2, 8:30pm Will

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

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

The Earth, Moon, and Sky. Lecture 5 1/31/2017 The Earth, Moon, and Sky Lecture 5 1/31/2017 From Last Time: Stable Orbits The type of orbit depends on the initial speed of the object Stable orbits are either circular or elliptical. Too slow and gravity

More information

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

Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods? Chapter S1 Celestial Timekeeping and Navigation S1.1 Astronomical Time Periods Our goals for learning:! How do we define the day, month, year, and planetary time periods?! How do we tell the time of day?!

More information

COMPUTER PROGRAM FOR THE ANGLES DESCRIBING THE SUN S APPARENT MOVEMENT IN THE SKY

COMPUTER PROGRAM FOR THE ANGLES DESCRIBING THE SUN S APPARENT MOVEMENT IN THE SKY COMPUTER PROGRAM FOR THE ANGLES DESCRIBING THE SUN S APPARENT MOVEMENT IN THE SKY B. BUTUC 1 Gh. MOLDOVEAN 1 Abstract: The paper presents software developed for the determination of the Sun-Earth geometry.

More information

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red Name: Topic 6 Test 1. Which process is responsible for the greatest loss of energy from Earth's surface into space on a clear night? A) condensation B) conduction C) radiation D) convection 2. Base your

More information

Section 2. Locating Astronomical Objects in the Night Sky What Do You See? What Do You See? Think About It. Investigate.

Section 2. Locating Astronomical Objects in the Night Sky What Do You See? What Do You See? Think About It. Investigate. Section 2 Locating Astronomical Objects in the Night Sky Section 2 Locating Astronomical Objects in the Night Sky What Do You See? What Do You See? Learning Outcomes In this section, you will Construct

More information

ZW2000 and Your Vertical Sundial Carl Sabanski

ZW2000 and Your Vertical Sundial Carl Sabanski 1 The Sundial Primer created by At this point I assume that you have downloaded and set up ZW2000 on your computer and have also read the overview document. If not please read Getting Started with ZW2000

More information

What are Latitude and Longitude?

What are Latitude and Longitude? What are Latitude and Longitude? By Encyclopaedia Britannica, adapted by Newsela staff on 08.29.17 Word Count 959 Level 950L A few miles from Quito, Ecuador's capital, is the equator line. It is located

More information

Geography Class 6 Chapters 3 and

Geography Class 6 Chapters 3 and CHAPTER 3 MOTIONS OF THE EARTH The Earth is always travelling in Space. That makes each person on Earth, a Space Traveller. No one feels the movement of the Earth because humans are too tiny when compared

More information

Chapter 6. Solar Geometry. Contents

Chapter 6. Solar Geometry. Contents Chapter 6. Solar Geometry Contents 6.1 Introduction 6.2 The Sun 6.3 Elliptical Orbit 6.4 Tilt of the Earth s Axis 6.5 Consequences of the Altitude Angle 6.6 Winter 6.7 The Sun Revolves Around the Earth!

More information

Motions of the Sun Model Exploration

Motions of the Sun Model Exploration Name Date Bell Motions of the Sun Model Exploration 1. Go to the University of Nebraska-Lincoln Motions of the Sun Simulator: http://astro.unl.edu/naap/motion3/animations/sunmotions.swf 2. This is what

More information

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

More information

Laboratory Exercise #7 - Introduction to Atmospheric Science: The Seasons

Laboratory Exercise #7 - Introduction to Atmospheric Science: The Seasons Laboratory Exercise #7 - Introduction to Atmospheric Science: The Seasons page - 1 Section A - Introduction: This lab consists of both computer-based and noncomputer-based questions dealing with atmospheric

More information

PHYSICAL GEOGRAPHY. By Brett Lucas

PHYSICAL GEOGRAPHY. By Brett Lucas PHYSICAL GEOGRAPHY By Brett Lucas INTRODUCTION Introduction to Earth Geography as a Field of Learning Geography is from two Greek words, Geo Earth, and Graphien to write. Elements/Branches of Geography

More information

MiSP Astronomy Seasons Worksheet #1 L1

MiSP Astronomy Seasons Worksheet #1 L1 MiSP Astronomy Seasons Worksheet #1 L1 Name Date CHANGING HOURS OF DAYLIGHT ON LONG ISLAND Introduction You sometimes hear people say, Days are longer in the summer and shorter in the winter. That is a

More information

Phys Lab #1: The Sun and the Constellations

Phys Lab #1: The Sun and the Constellations Phys 10293 Lab #1: The Sun and the Constellations Introduction Astronomers use a coordinate system that is fixed to Earth s latitude and longitude. This way, the coordinates of a star or planet are the

More information

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

Chapter 1 Image Slides. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 1 Image Slides Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. CH. 1: CYCLES OF THE SKY CO a 1.1 The Celestial Sphere CO b The nearest star to us is about

More information

Earth is tilted (oblique) on its Axis!

Earth is tilted (oblique) on its Axis! MONDAY AM Radiation, Atmospheric Greenhouse Effect Earth's orbit around the Sun is slightly elliptical (not circular) Seasons & Days Why do we have seasons? Why aren't seasonal temperatures highest at

More information

MiSP Astronomy - Seasons Worksheet #1 L2

MiSP Astronomy - Seasons Worksheet #1 L2 MiSP Astronomy - Seasons Worksheet #1 L2 Name Date Changing Hours of Daylight on Long Island (L 1, 2, 3) Introduction You sometimes hear people say, Days are longer in the summer and shorter in the winter.

More information

Aileen A. O Donoghue Priest Associate Professor of Physics

Aileen A. O Donoghue Priest Associate Professor of Physics SOAR: The Sky in Motion Life on the Tilted Teacup Ride Celestial Coordinates and the Day Aileen A. O Donoghue Priest Associate Professor of Physics Reference Points Poles Equator Prime Meridian Greenwich,

More information

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

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 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 noon: highest point of Sun in sky relative to the horizon 1 altitude:

More information

b. Assuming that the sundial is set up correctly, explain this observation.

b. Assuming that the sundial is set up correctly, explain this observation. Astronomy 100 Name(s): Exercise 3: Seasons in the sun The following exercise illustrates some basic ideas about time, and how our position in the solar system uniquely configures the measurement of time.

More information

Solar Time, Angles, and Irradiance Calculator: User Manual

Solar Time, Angles, and Irradiance Calculator: User Manual Solar Time, Angles, and Irradiance Calculator: User Manual Circular 674 Thomas Jenkins and Gabriel Bolivar-Mendoza 1 Cooperative Extension Service Engineering New Mexico Resource Network College of Agricultural,

More information

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

Time, coordinates and how the Sun and Moon move in the sky Time, coordinates and how the Sun and Moon move in the sky Using the colors and magnitudes of quasars drawn from the SDSS Catalog Archive Server to distinguish quasars from stars using the light they emit

More information

3. This room is located in a building in New York State. On which side of the building is the window located? (1) north (3) east (2) south (4) west

3. This room is located in a building in New York State. On which side of the building is the window located? (1) north (3) east (2) south (4) west 1. The planetary winds in Earth s Northern Hemisphere generally curve to the right due to Earth s (1) orbit around the Sun (2) spin on its axis (3) magnetic field (4) force of gravity Base your answers

More information

Period 14 Activity Sheet: Energy in Nature

Period 14 Activity Sheet: Energy in Nature Period 14 Activity Sheet: Energy in Nature 14.1 The Earth-Sun System 1) Energy from the sun Observe the models of the Earth, Moon, and Sun in the room. a) Imagine that the distance between the Earth and

More information

Discovering the Night Sky

Discovering the Night Sky Discovering the Night Sky Guiding Questions 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same stars

More information

Discovering the Night Sky

Discovering the Night Sky Guiding Questions Discovering the Night Sky 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same stars

More information

6/17. Universe from Smallest to Largest:

6/17. Universe from Smallest to Largest: 6/17 Universe from Smallest to Largest: 1. Quarks and Leptons fundamental building blocks of the universe size about 0 (?) importance: quarks combine together to form neutrons and protons. One of the leptons

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

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. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

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

Knowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations Knowing the Heavens Chapter Two Guiding Questions 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same

More information

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

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc. Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the

More information

CHAPTER 2 Strand 1: Structure and Motion within the Solar System

CHAPTER 2 Strand 1: Structure and Motion within the Solar System CHAPTER 2 Strand 1: Structure and Motion within the Solar System Chapter Outline 2.1 EARTH, MOON, AND SUN SYSTEM (6.1.1) 2.2 GRAVITY AND INERTIA (6.1.2) 2.3 SCALE OF SOLAR SYSTEM (6.1.3) 2.4 REFERENCES

More information

Astro 101 Lab #2. Start up the Stellarium program. If you do not remember how to use the user interface, please refer to Lab#1 or the user s guide.

Astro 101 Lab #2. Start up the Stellarium program. If you do not remember how to use the user interface, please refer to Lab#1 or the user s guide. Name: Astro 101 Lab #2 Lab objectives 1) Learn about how the Sun s path, through the sky, changes with the changing seasons. 2) Learn about how the Sun s path changes while viewing it at different locations

More information

Observer-Sun Angles. ), Solar altitude angle (α s. ) and solar azimuth angle (γ s )). θ z. = 90 o α s

Observer-Sun Angles. ), Solar altitude angle (α s. ) and solar azimuth angle (γ s )). θ z. = 90 o α s Observer-Sun Angles Direction of Beam Radiation: The geometric relationships between a plane of any particular orientation relative to the earth at any time and the incoming beam solar radiation can be

More information

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

Meridian Circle through Zenith, North Celestial Pole, Zenith Direction Straight Up from Observer. South Celestial Pole Chapter 3 How Earth and Sky Work- Effects of Latitude In chapters 3 and 4we will learn why our view of the heavens depends on our position on the Earth, the time of day, and the day of the year. We will

More information

C) D) 2. The diagram below shows a large pendulum in motion over an 8-hour period.

C) D) 2. The diagram below shows a large pendulum in motion over an 8-hour period. 1. An observer on Earth measured the apparent diameter of the Sun over a period of 2 years. Which graph best represents the Sun's apparent diameter during the 2 years? A) B) C) D) 2. The diagram below

More information

Practice Questions: Seasons #2

Practice Questions: Seasons #2 1. How many degrees does the Sun appear to move across the sky in four hours? A) 60 B) 45 C) 15 D) 4 Practice Questions: Seasons #2 2. Base your answer to the following question on the diagram below, which

More information

Geometry of Earth Sun System

Geometry of Earth Sun System 12S56 Geometry of Earth Sun System Figure below shows the basic geometry Northern Hemisphere Winter ω equator Earth s Orbit Ecliptic ω ω SUN equator Northern Hemisphere Spring Northern Hemisphere Fall

More information

Celestial Sphere. Altitude [of a celestial object] Zenith. Meridian. Celestial Equator

Celestial Sphere. Altitude [of a celestial object] Zenith. Meridian. Celestial Equator Earth Science Regents Interactive Path of the Sun University of Nebraska Resources Copyright 2011 by Z. Miller Name Period COMPANION WEBSITES: http://www.analemma.com/ http://www.stellarium.org/ INTRODUCTION:

More information

The Earth-Moon-Sun System

The Earth-Moon-Sun System chapter 7 The Earth-Moon-Sun System section 2 Time and Seasons What You ll Learn how to calculate time and date in different time zones how to distinguish rotation and revolution what causes seasons Before

More information

Observing the Universe for Yourself

Observing the Universe for Yourself Observing the Universe for Yourself Figure 6-20 Solar-System Formation What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as well as the Milky Way. A constellation

More information

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

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself 1 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations

More information

Lesson Overview. Climate. Lesson Overview. 4.1 Climate

Lesson Overview. Climate. Lesson Overview. 4.1 Climate Lesson Overview 4.1 THINK ABOUT IT When you think about climate, you might think of dramatic headlines: Hurricane Katrina floods New Orleans! or Drought parches the Southeast! But big storms and seasonal

More information

Time Series Model of Photovoltaic Generation for Distribution Planning Analysis. Jorge Valenzuela

Time Series Model of Photovoltaic Generation for Distribution Planning Analysis. Jorge Valenzuela Time Series Model of Photovoltaic Generation for Distribution Planning Analysis Jorge Valenzuela Overview Introduction: The solar problem and our limitations Modeling What information do we have? Solar

More information

UNIT 1: THE PLANET EARTH

UNIT 1: THE PLANET EARTH UNIT 1: THE PLANET EARTH How many planets are there in our Solar System? What is the Equator? Why does life exist in our planet? Does The Earth move? What is a map? 1. Planet Earth TOPICS 2. Movements

More information