Motions of the Sun Model Exploration

Similar documents
MiSP Astronomy - Seasons Worksheet #1 L2

MiSP Astronomy Seasons Worksheet #1 L1

Student Exploration: Seasons: Earth, Moon, and Sun

Practice Questions: Seasons #1

Earth Motions Packet 14

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

Astronomy 101 Lab: Seasons

1. Which continents are experiencing daytime? 2. Which continents are experiencing nighttime?

Astron 104 Laboratory #2 The Celestial Sphere

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

Computer Activity #3 SUNRISE AND SUNSET: THE SEASONS

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

Practice Questions: Seasons #2

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.

Earth Science Seasons Test Name Per Date

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

What causes the seasons? 2/11/09

4. What verb is used to describe Earth s

Page 1. Name:

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

March 21. Observer located at 42 N. Horizon

Astronomy 101: 9/18/2008

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

SC.8.E.5.9. Summer and Winter Gizmo

Earth, Sun, and Stars

Student Exploration: Seasons in 3D

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

NAME; LAB # SEASONAL PATH OF THE SUN AND LATITUDE Hemisphere Model #3 at the Arctic Circle

The Celestial Sphere. From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere.

LAB: What Events Mark the Beginning of Each Season?

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

drinking straw, protractor, string, and rock. observer on Earth. Sun across the sky on March 21 as seen by an

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.

Venus Project Book, the Galileo Project, GEAR

Seasonal Path of the Sun and Latitude

LESSON PLAN - Optimum Orientation of Solar Panels Using Soltrex Data

Oberth: Energy vs. Momentum

Exercise 7.0 THE CHANGING DIURNAL CIRCLES OF THE SUN

You have learned that Earth s 24-hour day night cycle is caused

CA1 2.11: Designing an Equatorial Sundial Activity

The Rotating Sky Student Guide

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

Chapter 4 Earth, Moon, and Sky 107

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

Seasons. What causes the seasons?

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

CHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM

ClassAction: Coordinates and Motions Module Instructor s Manual

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

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.

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

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

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

Phys Lab #1: The Sun and the Constellations

Aileen A. O Donoghue Priest Associate Professor of Physics

1. The pictures below show the Sun at midday. Write winter, spring or summer under the correct picture.

Earth rotates on a tilted axis and orbits the Sun.

Daylight Data: Days and Nights Around the World

ME 476 Solar Energy UNIT THREE SOLAR RADIATION

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

3. The diagram below shows the Moon at four positions in its orbit around Earth as viewed from above the North Pole.

ASTRONOMY Merit Badge Requirements

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

ì<(sk$m)=cdfdhh< +^-Ä-U-Ä-U

Chapter 2 Discovering the Universe for Yourself

OBSERVING PROJECT PARTNER ELECTION

The Earth Orbits the Sun Student Question Sheet (Advanced)

TILT, DAYLIGHT AND SEASONS WORKSHEET

Name: Exam 1, 9/30/05

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

Seasons and Ecliptic Simulator

The Rotating Sky Student Guide

Earth is rotating on its own axis

Calculations Equation of Time. EQUATION OF TIME = apparent solar time - mean solar time

01) The Sun s rays strike the surface of the Earth at 90 degrees at the on December 22.

Grade 6 Standard 2 Unit Test Astronomy

Discovering the Night Sky

Discovering the Night Sky

Chapter 2 Discovering the Universe for Yourself

What Patterns Can Be Observed in a Year?

What Is the Relationship Between Earth s Tilt and the Seasons?

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

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

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.

Seasons ASTR 101 2/12/2018

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

2.1 Patterns in the Night Sky

Rotation and Revolution

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

This clementine orange is an oblate spheroid. Earth is more rounded than this clementine, but it is still an oblate spheroid.

Fall equinox means 12 hours of sunlight for everyone, everywhere

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

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

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

Indoor Lab #2: The Starry Sky

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

EARTH S REVOLUTION -and- EARTH S ROTATION

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

Geography Class 6 Chapters 3 and

Transcription:

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 you will see. Now I will point out some parts of this page you can manipulate. You can change the orientation of Earth here. If you click and hold your curse button, you can turn the Earth and position it so that your view is straight on rather than angled. You can change the date or time of day here You can change the latitude of the stick figure on Earth here (typing in the number or dragging the bar) Here is where you can find out the solar elevation angle (the altitude) and the azimuth, as the sun moves across the sky. There s some other number here as well, but those two will be the ones you will be recording Here is where you start and stop time in the animation. The sun will appear to rise and set continuously in this animation.

3. Let s start exploring by reorienting the Earth to a different view. Using your mouse, click and drag the Earth so that south is towards the top of your screen and the horizon is parallel to the top of your screen. This is what you should see when you are finished. 4. Now unclick the boxes on the bottom right of your screen that say show the Sun s declination circle and show the underside of the celestial sphere. a. This is what you should see now 5. change the Latitude to 39.1 N (which is the latitude of Cincinnati, Ohio) 6. Now change the date to June 15 th 7. Change the time of day to 6:00 am. From this point on, you will be answering questions about certain things you will observe. You may need to back up and try again, or manipulate your model to find the answer. This means feel free to play around with the numbers and tools on your screen to find the answers. Good Luck!

Motions of the Sun Exploration 1. A.) In the model, is the sun currently in the Cincinnati Sky at 6 am? B.) What evidence from the page did you sue to answer that question? 2. At what two times is the sun at an altitude of 0? (you can spin the hands of the clock or type in a time to figure this out- BTW, you can also grab the Sin in the model and move it along its path) and 3. Using your times above in question 2, calculate how much daylight we will have during June 15 th. Write that answer in the blank below. 4. Now you are going to record sunrise and sunset times for one year in Cincinnati in the table below. Use the sunrise/sunset chart you are given to find the information you need. Do this step first, then calculate the hours of daylight for each date (elapsed time). January 15 th Date Sunrise Time Sunset Time Hours of Daylight (Elapsed Time) February 15 th March 15 th April 15 th May 15 th June 15 th July 15 th August 15 th September 15 th October 15 th November 15 th December 15th

5. A.) Look at your chart in number 4, what do you notice about hours of daylight in winter months versus summer months? B.) What do you notice about sunrise and sunset times in winter months versus summer months? 6. Now using the Motions of the Sun Simulator go back to January 15 th and find the Sun s highest altitude for the day. Record that information in the chart below. Repeat for the other dates. Date January 15 th February 15 th March 15 th April 15 th May 15 th June 15 th July 15 th August 15 th September 15 th October 15 th November 15 th December 15 th Highest Altitude (Zenith) Average High Temperature 40 degrees Fahrenheit 45 degrees Fahrenheit 55 degrees Fahrenheit 66 degrees Fahrenheit 75 degrees Fahrenheit 83 degrees Fahrenheit 87 degrees Fahrenheit 86 degrees Fahrenheit 79 degrees Fahrenheit 68 degrees Fahrenheit 56 degrees Fahrenheit 43 degrees Fahrenheit

7. A.) What do you notice about the highest altitude of the Sun in winter months versus summer months? B.) What relationship do you notice between the average high temperature and the highest solar elevation (zenith)? 8. Now using the Motion of the Sun Simulator, let s explore how the sun moves across the sky differently at different latitudes. a. Change the latitude of the stick figure to 0. Change the time of day to 6:00 am. Change the date to June 15 th. As you can see, the sun is just rising for this person on the equator. b. Start the animation by clicking on the start animation button. c. Watch the sun move across the sky for several days. Watch how the shadow of the stick figure changes throughout the day. d. What do you notice about the altitude of the sun? How does that affect the stick figure s shadow midday? What is the path of the Sun? Horizontally or vertically? e. Change the latitude of the stick figure to 90 N. Change the time of day to 6:00 am. Change the date to June 15 th. As you can see, it s currently daytime at the North Pole. f. Start the animation by clicking on the start animation button. g. Watch the sun move across the sky for several days. Watch how the shadow of the stick figure changes throughout the day. h. What do you notice about the altitude of the Sun? How is the path of the sun different at the North Pole different from at the Equator? What about the stick figure s shadow?

Do you think the Sun s Path will be different in the South Pole at this time of the year? Let s see! i. Change the latitude of the stick figure to 90 S. change the time of day to 6:00 am. Change the date to June 15 th. As you can see, it s currently night time at the South Pole. j. Start the animation by clicking on the start animation button. k. Watch the sun move across the sky for several days. Watch how the shadow of the stick figure changes throughout the day. l. What do you notice about the altitude of the Sun? How is the path of the Sun different at the North Pole than the South Pole in June? Why do you think this is? Is it dark or light outside and for how long? Now let s explore what each of these paths look like in January. Do you think they will be the same or different? 9. What will the Sun s path at the equator will be like in January? a. Change the latitude of the stick figure to 0. Change the time of day to 6:00 am. Change the date to January 15 th. Next set it to June 15 th. 6:00 am. b. Start the animation by clicking on the start animation button. Watch the sun move across the sky for several days. Watch how the shadow of the stick figure changes throughout the day. c. Compare the path of the Sun in January at the equator to the path in June. How are these paths similar or different? How are the shadows? Is it dark or light outside? What are the sun s altitudes in January and June? What do you think the Sun s path at the North Pole will be like at this time of year? Let s see! d. Change the Latitude of the stick figure to 90 N. Change the time of day to 6:00 am. Change the date to January 15 th. e. Start the animation by clicking on the start animation button. Watch the sun move across the sky for several days. Watch how the shadow of the stick figure changes throughout the day. f. Compare the path of the Sun in January at the North Pole to the path in June. How are these paths similar or different? How are the shadows? Is it dark or light outside? What are the sun s altitudes in January and June?

What do you think the Sun s path at the South Pole will be like at this time of year? Let s see! g. Change the latitude of the stick figure to 90 S. Change the time of day to 6:00 am. Change the date to January 15 th. h. Start the animation by clicking on the start animation button. i. Watch the sun move across the sky for several days. Watch how the shadow of the stick figure changes throughout the day. j. Compare the path of the sun in January at the South Pole to the path in June. How are these paths similar or different? How are the shadows? Is it dark or light outside? What are the sun s altitudes in January and June? k. What did you notice about the path of the Sun at the North and South Poles during different times of year? Why do you think they are polar opposites (excuse the puns)? l. Have you ever heard the expression land of the midnight sun? What do you think that is a reference to? Change the latitude of the stick figure to 90 N, Change the time of day to 00:00 am (midnight), Change the date to June 15th, to find out the answer.

Number of Hours of Daylight Now answer the following questions. Circle the correct answer. 10. When does the South Pole have a greater number of hours of daylight than anywhere else on earth? a. When the South Pole is angled away from the Sun b. When the South Pole is angled towards the Sun c. When the South Pole is not angled at all towards or away from the Sun d. Never 11. For two locations in the Northern Hemisphere during the Northern hemisphere s summer, when will Location A have a longer day than Location B a. If location A is on a higher line of latitude than location B b. If location A is closer to the equator than location B c. One location will never have a longer day than the other because they are both in the same hemisphere d. If location A is closer to the prime meridian than location B Amount of daylight 18 16 14 12 10 8 6 4 2 0 15-Jan Months 15-Jul Place 1 Place 2 12. A student who lives at place 1 measured the number of hours of sunlight on a day in January and on a day in July. Another student, who lives at Place 2 made the same measurement on the same two days. Both places are in the northern hemisphere. Based on their measurements, as shown in the graph above, what must be TRUE about place two? A. Place 2 is closer to the Equator than Place 1 B. Place 2 is farther from the Equator than Place 1 C. Place 2 is father to the east than Place 1 D. Place 2 could be north, south, or east of place 1, because the number of hours of sunlight cannot be used to compare the location of one place to another.