Lab Module 1: The Observing Project
|
|
- Juniper Gilbert
- 7 years ago
- Views:
Transcription
1 Lab Module 1 The Observing Project The Location and Time of Sunset OR Fremont Peak Observatory (Worth 15 points) Due Date: The last lab class before finals I. The Location and Time of Sunset Background Science depends on observations particularly careful, well-documented observations. This exercise requires that you make a series of observations and collect them systematically in a notebook that will be handed in at the end of the semester. Equipment Camera; notebook; pencil; compass (recommended) Objectives You will track the seasonal changes in the time and location of the sun over the course of the semester by observing sunset (or sunrise) at least once every other week for at least eight consecutive weeks (a total of 4 observations) and photographing your observations. Background At this very moment, you might be nice and relaxed, sitting in a comfortable chair, reading this lab manual. You are probably completely unaware that you are literally hurtling through space as you read this sentence. With every beat of your heart, you are propelled more than 10 miles through our Solar System, more than100 miles through our galaxy! Indeed, the Earth is not a stationary point in the Universe. Its motion results in changes in the observed night sky changes that have been noticed by humans for eons. City lights and prime-time TV have eliminated our intimacy with the night sky, especially since the average person no longer relies on this intimacy for survival. We will try to recover some of this knowledge now by systematically observing the Sun. The orbital motion of the Earth about the Sun results in some obvious changes in the night sky. For instance, you can see the constellation of Orion, the hunter, in the January 1
2 night sky while Sagittarius makes its debut in July when the Earth is on the other side of the Sun. There are, however, some less obvious changes that occur due to the tilt of the Earth s rotational axis relative to the plane traced out by its orbit about the Sun. This little accident of nature results in the seasons experienced (and enjoyed!) north and south of the equator. More specifically, the tilt causes the Sun to rise and set at different locations and times depending on the time of year and your location (latitude) on the Earth. The purpose of this lab is to get you to observe this phenomenon yourself. You are the scientist. The question you will investigate is: where and when does the Sun set (or rise) each day (week)? As a precaution, you should not look directly at the Sun (even through a camera lens) before it sets as it could cause severe eye damage! Choose and describe your location: Choose some observing location with a reasonably unobstructed view of the western horizon (or eastern if you prefer to observe sunrise). The view of the horizon should have at least one reference landmark. The reference landmark that you choose will help you to determine the direction of motion of the Sun and how far it moves every day. Examples of landmarks include a tree, building, telephone pole, edge of a cliff. Sketch the location on your paper. Describe in detail the exact location from which you made your sketch and indicate on your picture which landmark you chose as the reference. It is important that every time you make an observation of the rising or setting Sun, you will need to return to this exact location and look towards the same direction, so be very specific in your description. Determine time of sunset: Before each observation you need to find out the time of sunset (or sunrise) by going to the internet site: Enter the date, the city, and state of your observing location. Do NOT photograph the sunset (or sunrise) at the same time every week as the sunset time will change! Record date and time of sunset from the website: Important: include whether the time is Pacific Standard Time or Pacific Daylight Time. 2
3 Measure and record the angular distance of the sunset from the reference landmark: Use the reference landmark on the horizon to determine the Sun s location. Use your fist and thumb to determine approximately how many degrees horizontally in the sky it is away from the reference landmark (that is measure it s angular distance from the landmark). One fist represents about ten degrees in the sky and 1 thumb represents about 2 degrees in the sky. Record the value of the angular distance in degrees. Take a picture of the Sun when it is starting to touch the horizon: Once every other week, return to your observing location and watch the sunset (or sunrise). For each observation, you should make sure to allow yourself plenty of time to get to the observing location before sunset. Ideally you should get there approximately 20 minutes before sunset. You should take a picture of the Sun when it is low in the horizon, before it actually sets. As a precaution, you should not look directly, or through the camera at the Sun before it sets as it could cause severe eye damage! Continue to make Sun observations at least once every two weeks (doesn t have to be the same day) throughout the semester. Obtain at least 4 cloud free observations during a minimum of 8 weeks of observations. IT IS IMPORTANT TO KEEP THE CAMERA ON THE SAME ZOOM EVERY TIME YOU PHOTOGRAPH IT! Determine and label the direction of North and South: Remember that the Sun sets in the West and West is always left of North. Turn so that the Sun is directly to the left of you. Then the direction you are facing is North and the opposite direction is South. If you are observing the sunrise, remember that the sun rises in the East and East is always right of North. In this case, turn so that the Sun is directly to the right of you. Then the direction you are facing is North and the opposite direction is South. Label North and South on your photos. If it is cloudy that week, do your observations the following week. You should attempt to get at least 4 good (cloud free) observations of the sunset over a minimum of 8 weeks. Once your observations are all complete, paste or tape your photographs neatly onto a sheet of paper. You can also print them out if they are digital photos. You may either put them all on one piece of paper if they can fit or choose to put each photo on its own sheet. Above each observation label the date, sunset time, and the angular distance of the Sun. Label North and South on each photograph. 3
4 Interpreting Your Results At the end of the semester, summarize your findings regarding sunset (sunrise) on a page in your observing notebook. As you describe your findings, answer the following questions: 1) How many TOTAL degrees did the position of sunset (sunrise) move between your first and eighth week of observation. Was the position of sunset moving northwards or southwards during the 8 weeks of observations? 2) How did the time of sunset change over the course of the semester (i.e. was it setting earlier or later)? How many total hours or minutes did it change from the first observation to the eighth week? To do this correctly, you must consider whether or not your time measurements were in STANDARD or DAYLIGHT time and subtract or add an hour to compensate for the time change if there was a time change during your observations. 3) What do you think is causing the changes in sunset location and time? 4) During the next six months after your last observation, how will the time of the sunset or sunrise change? Will the location of sunset or sunrise move northwards or southwards? 1
5 II. Fremont Peak Observatory Field Trip (Worth 15 points alone or 10 points additional extra credit if the Sunset Project is turned) Equipment Flashlight with red cellophane; notebook; pencil Objectives You will obtain the opportunity to visit Fremont Peak Observatory and view astronomical objects through telescopes. Important Note: If you are in the lecture class, you will automatically receive credit for one of the observing projects if you choose to go on this field trip. To ensure proper credit, make sure you indicate on the cover page of your write up that you would like credit for this in the lecture also. Introduction Fremont Peak Observatory is located in the beautiful Fremont Peak State Park in San Juan Bautista. It is about a 1 hour drive from Salinas. The road up the mountain is very windy and at times steep. Be very careful when driving at night. The date of the field trip will be announced several weeks ahead of time in class. The entire observing experience should last until about 10:00pm. Dress warmly and bring a flashlight that is covered with red cellophane. You can also bring your planisphere with you. Once you arrive at the observatory, please be courteous. The staff at Fremont Peak Observatory are providing us with a service by allowing us to access their observatory; please respect them and the facilities. You can find out all the information (including directions) on their website: Or you can call them: (831) Bring $6.00 in correct change for the parking fee. 2
6 Part I: Telescope Observations 1. Once you arrive at the observatory, there should be several telescopes set to view different objects in the sky. Sketch at least three objects. Take some time to look through the telescope. Do not move the telescope! Try to capture the image in your mind. Don t sketch the object as you are observing it through the telescope. Draw the object afterwards in order to let others have a chance to observe the object. 2. Make sure that your drawing is to scale with the eyepiece. 3. Write a sentence describing what the object looked like. 4. Also fill in all the required information. If you don t know the information, ask the people who are operating the telescope. Part II: Instructor s Signature This is very important. In order for you to obtain credit for this assignment, you must ask your instructor or Fremont Peak volunteer to sign your observations sheet and make sure they record the date. Part III: Journal Entry 1. Your journal entry should be at least 400 words typed. 2. Describe your thoughts from the time you drove up the mountain until you came back down. 2. Describe the objects you saw. Which one fascinated you the most and why? 3. What was the weather like? 4. Did you do anything else besides look through the telescope? 5. What did you think about the entire experience? Note: By choosing to go to Fremont Peak Observatory, you assume all liabilities. 3
7 Instructor s or Volunteer s Signature and Date: Object 1: Object Name: Date/Time : Telescope Diameter: Draw what you see through the telescope above. Describe in words what you see here: Extra Credit: Focal Length Objective: Eyepiece: Magnification=Fobj/Feye: Object 2: Object Name: Date/Time : Telescope Diameter: Draw what you see through the telescope above. Describe in words what you see here: Extra Credit: Focal Length Objective: Eyepiece: Magnification=Fobj/Feye: 4
8 Object 3: Object Name: Date/Time : Telescope Diameter: Draw what you see through the telescope above. Describe in words what you see here: Extra Credit: Focal Length Objective: Eyepiece: Magnification=Fobj/Feye: Object 4: Object Name: Date/Time : Telescope Diameter : Draw what you see through the telescope above. Describe in words what you see here: Extra Credit: Focal Length Objective: Eyepiece: Magnification=Fobj/Feye: 5
FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES
FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF FIRST GRADE UNIVERSE WEEK 1. PRE: Describing the Universe. LAB: Comparing and contrasting bodies that reflect light. POST: Exploring
More informationLab Activity on the Causes of the Seasons
Lab Activity on the Causes of the Seasons 2002 Ann Bykerk-Kauffman, Dept. of Geological and Environmental Sciences, California State University, Chico * Objectives When you have completed this lab you
More informationFinding Stars and Constellations Earth & Sky
Finding Stars and Constellations Earth & Sky Name: Introduction If you carefully watched the night sky over a period of time, you would notice that it s not always the same. There are certain changes that
More informationINDEPENDENT PROJECT: The Spring Night Sky
INDEPENDENT PROJECT: The Spring Night Sky Your Name: What is the difference between observing and looking? As John Rummel said to the Madison Astronomical Society, January 11, 2002: Looking implies a passive
More informationUse WITH Investigation 4, Part 2, Step 2
INVESTIGATION 4 : The Sundial Project Use WITH Investigation 4, Part 2, Step 2 EALR 4: Earth and Space Science Big Idea: Earth in Space (ES1) Projects: Tether Ball Pole Sundial Globe and a Light Indoors
More informationINDEPENDENT PROJECT: The Spring Night Sky
INDEPENDENT PROJECT: The Spring Night Sky Your Name: What is the difference between observing and looking? As John Rummel said to the Madison Astronomical Society, January 11, 2002: Looking implies a passive
More informationPhases of the Moon. Preliminaries:
Phases of the Moon Sometimes when we look at the Moon in the sky we see a small crescent. At other times it appears as a full circle. Sometimes it appears in the daylight against a bright blue background.
More informationCELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS
INTRODUCTION CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS This is a scientific presentation to provide you with knowledge you can use to understand the sky above in relation to the earth. Before
More informationShadows, Angles, and the Seasons
Shadows, Angles, and the Seasons If it's cold in winter, why is Earth closer to the Sun? This activity shows the relationship between Earth-Sun positions and the seasons. From The WSU Fairmount Center
More informationEDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1
Instructor: L. M. Khandro EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 1. An arc second is a measure of a. time interval between oscillations of a standard clock b. time
More informationWhich month has larger and smaller day time?
ACTIVITY-1 Which month has larger and smaller day time? Problem: Which month has larger and smaller day time? Aim: Finding out which month has larger and smaller duration of day in the Year 2006. Format
More informationActivity 10 - Universal Time
Activity 10 - Universal Time Teacher s Guide Scientists use the Universal Time reference to talk about data that is taken around the globe. Universal Time is the time kept in the time zone centered on
More informationExercise: Estimating the Mass of Jupiter Difficulty: Medium
Exercise: Estimating the Mass of Jupiter Difficulty: Medium OBJECTIVE The July / August observing notes for 010 state that Jupiter rises at dusk. The great planet is now starting its grand showing for
More informationCelestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun)
Lecture 3: Motions of the and Moon ecliptic (path of ) ecliptic (path of ) The 23.5 degree tilt of Earth s spin axis relative to its orbital axis around the causes the seasons Celestial Sphere Celestial
More informationLesson 1: Phases of the Moon
Lesson 1: Phases of the Moon The moon takes 29.5 days to revolve around the earth. During this time, the moon you see in the sky appears to change shape. These apparent changes, which are called phases,
More informationSolar Matters II Teacher Page
Solar Matters II Teacher Page Sun Misconceptions Student Objective understands why some common phrases about the Sun are incorrect can describe how the Earth s rotation affects how we perceive the Sun
More informationChanges in Our Sky Grade Two
Ohio Standards Connection: Earth and Space Sciences Benchmark A Observe constant and changing patterns of objects in the day and night sky. Indicator 2 Observe and describe how the sun, moon and stars
More information5- Minute Refresher: Daily Observable Patterns in the Sky
5- Minute Refresher: Daily Observable Patterns in the Sky Key Ideas Daily Observable Patterns in the Sky include the occurrence of day and night, the appearance of the moon, the location of shadows and
More informationActivities: The Moon is lit and unlit too
Activities: The Moon is lit and unlit too Key objectives: This activity aims to help student to: Identify the different phases of the Moon Know that the Moon does not produce its own light, but reflects
More informationScience Benchmark: 06 : 01 Standard 01: THE MYSTICAL MOON axis of rotation,
Science Benchmark: 06 : 01 The appearance of the lighted portion of the moon changes in a predictable cycle as a result of the relative positions of Earth, the moon, and the sun. Standard 01: Students
More informationThe following questions refer to Chapter 19, (PAGES 259 278 IN YOUR MANUAL, 7 th ed.)
GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Locating the Planets (Chapter 19) and the Moon and Sun (Chapter 21) For this assignment you will require: a calculator, colored pencils, a metric
More informationBasic Coordinates & Seasons Student Guide
Name: Basic Coordinates & Seasons Student Guide There are three main sections to this module: terrestrial coordinates, celestial equatorial coordinates, and understanding how the ecliptic is related to
More informationObserving the Constellations of the Zodiac
Observing the Constellations of the Zodiac Activity UCIObs 3 Grade Level: 8 12 Source: Copyright (2009) by Tammy Smecker Hane. Contact tsmecker@uci.edu with any questions. Standards:This activity addresses
More informationAST 114 Spring 2016 Introduction to the Night Sky INTRODUCTION TO THE NIGHT SKY
NAME: INTRODUCTION TO THE NIGHT SKY What will you learn in this Lab? This lab will introduce you to the layout of the night sky: constellations and stars, their names and the patterns they make, and the
More informationCalculating Astronomical Unit from Venus Transit
Calculating Astronomical Unit from Venus Transit A) Background 1) Parallaxes of the Sun (the horizontal parallaxes) By definition the parallaxes of the Sun is the angle β shown below: By trigonometry,
More informationMeasuring Your Latitude from the Angle of the Sun at Noon
Measuring Your Latitude from the Angle of the Sun at Noon Background: You can measure your latitude in earth's northern hemisphere by finding out the altitude of the celestial equator from the southern
More informationNewton s Law of Gravity
Gravitational Potential Energy On Earth, depends on: object s mass (m) strength of gravity (g) distance object could potentially fall Gravitational Potential Energy In space, an object or gas cloud has
More informationDouglas Adams The Hitchhikers Guide to the Galaxy
There is a theory which states that if ever anybody discovers exactly what the Universe is for and why it is here, it will instantly disappear and be replaced by something even more bizarre and inexplicable.
More informationExploring the Phases of the Moon
Exploring the Phases of the Moon Activity UCIObs 5 Grade Level: 3 5 Source: Copyright (2009) by Tammy Smecker-Hane. Contact tsmecker@uci.edu with questions. Standards: This activity addresses these California
More informationExam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti
Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking
More informationCoordinate Systems. Orbits and Rotation
Coordinate Systems Orbits and Rotation Earth orbit. The earth s orbit around the sun is nearly circular but not quite. It s actually an ellipse whose average distance from the sun is one AU (150 million
More informationCELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault
CELESTIAL MOTIONS Stars appear to move counterclockwise on the surface of a huge sphere the Starry Vault, in their daily motions about Earth Polaris remains stationary. In Charlottesville we see Polaris
More informationRising and Setting of the Moon
Rising and Setting of the Moon Activity UCIObs 6 Grade Level: 3 5 Source: Copyright (2009) by Tammy Smecker-Hane. Contact tsmecker@uci.edu with questions. Standards: This activity addresses these California
More informationThe ecliptic - Earth s orbital plane
The ecliptic - Earth s orbital plane The line of nodes descending node The Moon s orbital plane Moon s orbit inclination 5.45º ascending node celestial declination Zero longitude in the ecliptic The orbit
More informationEarth, Sun and Moon is a set of interactives designed to support the teaching of the QCA primary science scheme of work 5e - 'Earth, Sun and Moon'.
is a set of interactives designed to support the teaching of the QCA primary science scheme of work 5e - ''. Learning Connections Primary Science Interactives are teaching tools which have been created
More informationThe Reasons for the Seasons
The Reasons for the Seasons (The Active Learning Approach) Materials: 4 Globes, One light on stand with soft white bulb, 4 flashlights, Four sets of "Seasons" Cards, Four laminated black cards with 1 inch
More informationAstronomy Merit Badge Workbook
Merit Badge Workbook This workbook can help you but you still need to read the merit badge pamphlet. The work space provided for each requirement should be used by the Scout to make notes for discussing
More informationASTR 1030 Astronomy Lab 65 Celestial Motions CELESTIAL MOTIONS
ASTR 1030 Astronomy Lab 65 Celestial Motions CELESTIAL MOTIONS SYNOPSIS: The objective of this lab is to become familiar with the apparent motions of the Sun, Moon, and stars in the Boulder sky. EQUIPMENT:
More informationLunar Phase Simulator Student Guide
Name: Lunar Phase Simulator Student Guide Part I: Background Material Answer the following questions after reviewing the background pages for the simulator. Page 1 Introduction to Moon Phases Is there
More informationDETERMINING SOLAR ALTITUDE USING THE GNOMON. How does the altitude change during the day or from day to day?
Name Partner(s) Section Date DETERMINING SOLAR ALTITUDE USING THE GNOMON Does the Sun ever occur directly overhead in Maryland? If it does, how would you determine or know it was directly overhead? How
More informationIn this project, you will be observing at least three objects with a telescope or binoculars, and drawing what you see.
Telescopic Observations Materials: Paper, pencil, camera, Telescope or Binoculars In this project, you will be observing at least three objects with a telescope or binoculars, and drawing what you see.
More informationPTYS/ASTR 206 Section 2 Spring 2007 Homework #2 (Page 1/5) NAME: KEY
PTYS/ASTR 206 Section 2 Spring 2007 Homework #2 (Page 1/5) NAME: KEY Due Date: start of class 2/6/2007 5 pts extra credit if turned in before 9:00AM (early!) (To get the extra credit, the assignment must
More informationExploring Solar Energy Variations on Earth: Changes in the Length of Day and Solar Insolation Through the Year
Exploring Solar Energy Variations on Earth: Changes in the Length of Day and Solar Insolation Through the Year Purpose To help students understand how solar radiation varies (duration and intensity) during
More informationastronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.
1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were increased,
More informationPROFESSIONAL REFRACTOR MODEL 78-0040 25
30 0 30 60 90 1 2 3 4 PROFESSIONAL REFRACTOR MODEL 78-0040 25 24 22 21 20 19 5 9060 18 6 7 17 16 15 8 14 13 9 11 12 10 Figure 1 1. Objective Lens 2. Mounting Screws (2) 3. Declination Axis 4. Equatorial
More informationFull credit for this chapter to Prof. Leonard Bachman of the University of Houston
Chapter 6: SOLAR GEOMETRY Full credit for this chapter to Prof. Leonard Bachman of the University of Houston SOLAR GEOMETRY AS A DETERMINING FACTOR OF HEAT GAIN, SHADING AND THE POTENTIAL OF DAYLIGHT PENETRATION...
More informationMaybe you know about the Energy House.
Plans and experiments for the Energy House can be found at Design Coalition s website at www.designcoalition.org Maybe you know about the Energy House. Here are some more ideas for leaning about the sun
More informationGETTING STARTED IN STAR GAZING. The fact you are here in this introductory session says you have an interest in the hobby of
GETTING STARTED IN STAR GAZING by Nelson Tilden Sun City Oro Valley Astronomy Club The fact you are here in this introductory session says you have an interest in the hobby of astronomy, but please note
More informationMotions of the Earth. Stuff everyone should know
Motions of the Earth Stuff everyone should know Earth Motions E W N W Noon E Why is there day and night? OR Why do the Sun and stars appear to move through the sky? Because the Earth rotates around its
More informationNote S1: Eclipses & Predictions
The Moon's Orbit The first part of this note gives reference information and definitions about eclipses [14], much of which would have been familiar to ancient Greek astronomers, though not necessarily
More informationExploration of the Solar System
Exploration of the Solar System I. Phases of the Moon all about perspective. In this section you will use WWT to explore how the moon appears to change phases from our vantage point on Earth over the course
More informationCOASTLINING THE ZODIAC
COASTLINING THE ZODIAC Astronomy books and skywatching guides offer a wide variety of charts for naked-eye observation of the skies. What works best for each person will depend on various factors such
More informationThe Lunar Phase Wheel
The Lunar Phase Wheel A lunar phase wheel is a simple device to help you to visualize the positions of the Earth, Moon, and Sun at various times of the day or month, and then predict the phases and the
More information1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram?
1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram? 5. During how many days of a calendar year is the Sun directly overhead
More informationLenses and Telescopes
A. Using single lenses to form images Lenses and Telescopes The simplest variety of telescope uses a single lens. The image is formed at the focus of the telescope, which is simply the focal plane of the
More informationCycles in the Sky. Teacher Guide: Cycles in the Sky Page 1 of 8 2008 Discovery Communications, LLC
Cycles in the Sky What is a Fun damental? Each Fun damental is designed to introduce your younger students to some of the basic ideas about one particular area of science. The activities in the Fun damental
More informationThe Size & Shape of the Galaxy
name The Size & Shape of the Galaxy The whole lab consists of plotting two graphs. What s the catch? Aha visualizing and understanding what you have plotted of course! Form the Earth Science Picture of
More informationSeasons on Earth LESSON
LESSON 4 Seasons on Earth On Earth, orange and red autumn leaves stand out against the blue sky. NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION (NOAA) PHOTO LIBRARY/NOAA CENTRAL LIBRARY INTRODUCTION Nearly
More informationWhere on Earth are the daily solar altitudes higher and lower than Endicott?
Where on Earth are the daily solar altitudes higher and lower than Endicott? In your notebooks, write RELATIONSHIPS between variables we tested CAUSE FIRST EFFECT SECOND EVIDENCE As you increase the time
More informationHeat Transfer. Energy from the Sun. Introduction
Introduction The sun rises in the east and sets in the west, but its exact path changes over the course of the year, which causes the seasons. In order to use the sun s energy in a building, we need to
More informationWhat Causes Climate? Use Target Reading Skills
Climate and Climate Change Name Date Class Climate and Climate Change Guided Reading and Study What Causes Climate? This section describes factors that determine climate, or the average weather conditions
More informationExercise 5.0 LUNAR MOTION, ELONGATION, AND PHASES
Exercise 5.0 LUNAR MOTION, ELONGATION, AND PHASES I. Introduction The Moon's revolution in orbit around the center of gravity (barycenter) of the Earth- Moon System results in an apparent motion of the
More informationView Through a Telescope Classroom Activity
View Through a Telescope Classroom Activity The Classroom Activity introduces students to the context of a performance task, so they are not disadvantaged in demonstrating the skills the task intends to
More informationFry Phrases Set 1. TeacherHelpForParents.com help for all areas of your child s education
Set 1 The people Write it down By the water Who will make it? You and I What will they do? He called me. We had their dog. What did they say? When would you go? No way A number of people One or two How
More informationMaking a reflector telescope
Making a reflector telescope telescope built by Sir Isaac Newton Replica of the first reflector Nowadays, professional astronomers use another type of telescope that is different to the first telescope
More informationMoon Phases and Tides in the Planning the D-Day Invasion Part I: The Phases of the Moon
The Science and Technology of WWII Moon Phases and Tides in the Planning the D-Day Invasion Part I: The Phases of the Moon Objectives: 1. Students will determine what causes the moon to go through a cycle
More informationGeneral Astronomy Phys1810 Fall 2015. Observing Exercises
Observing Exercises You will complete 3 of the following exercises: Exercise 1: Sketching the North Circumpolar Cap (mandatory) Exercise 2: Seasonal Constellations Exercise 3: Telescope Observations Exercise
More informationAstronomy 1140 Quiz 1 Review
Astronomy 1140 Quiz 1 Review Prof. Pradhan September 15, 2015 What is Science? 1. Explain the difference between astronomy and astrology. (a) Astrology: nonscience using zodiac sign to predict the future/personality
More informationCelestial Observations
Celestial Observations Earth experiences two basic motions: Rotation West-to-East spinning of Earth on its axis (v rot = 1770 km/hr) (v rot Revolution orbit of Earth around the Sun (v orb = 108,000 km/hr)
More informationStellar, solar, and lunar demonstrators
Stellar, solar, and lunar demonstrators Rosa M. Ros, Francis Berthomieu International Astronomical Union, Technical University of Catalonia (Barcelona, España), CLEA (Nice, France) Summary This worksheet
More informationAn Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science
An Introduction to Astronomy and Cosmology 1) Astronomy - an Observational Science Why study Astronomy 1 A fascinating subject in its own right. The origin and Evolution of the universe The Big Bang formation
More informationUnderstanding Depth Of Field, Aperture, and Shutter Speed Supplement to Mastering the Nikon D7000
Understanding Depth Of Field, Aperture, and Shutter Speed Supplement to Mastering the Nikon D7000 This supplemental information is intended for readers of Mastering the Nikon 7000 only. Please do not distribute
More informationGOODNIGHT, MOON (AND STARS)
2 WEEK GOODNIGHT, MOON (AND STARS) EXPERIMENT: STARLIGHT FLASHLIGHT AND MOON JOURNAL Do you ever notice how the night sky changes above you? The moon s shape changes throughout the month, and the constellations
More informationKINDERGARTEN PHYSICS
KINDERGARTEN PHYSICS 3 WEEKS LESSON PLANS AND ACTIVITIES APPLIED SCIENCE OVERVIEW OF KINDERGARTEN SCIENCE AND MATH WEEK 1. PRE: Describing and comparing nests, birds, and eggs. LAB: Describing different
More informationLines of Latitude and Longitude
ED 5661 Mathematics & Navigation Teacher Institute Keith Johnson Lesson Plan Lines of Latitude and Longitude Lesson Overview: This lesson plan will introduce students to latitude and longitude along with
More information1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.
Chapter 1 1-1. How long does it take the Earth to orbit the Sun? a.) one sidereal day b.) one month c.) one year X d.) one hour 1-2. What is the name given to the path of the Sun as seen from Earth? a.)
More informationThe Observed Calendar of the Second Temple Dates For 2014
www.120jubilees.com The Observed Calendar of the Second Temple Dates For 2014 The Observed Calendar of the Second Temple Era was used by the official priests of the Second Temple from at least 520 BC to
More informationAstronomy Club of Asheville October 2015 Sky Events
October 2015 Sky Events The Planets this Month - page 2 Planet Highlights - page 10 Moon Phases - page 13 Orionid Meteor Shower Peaks Oct. 22 nd - page 14 Observe the Zodiacal Light - page 15 2 Bright
More informationSolar energy and the Earth s seasons
Solar energy and the Earth s seasons Name: Tilt of the Earth s axis and the seasons We now understand that the tilt of Earth s axis makes it possible for different parts of the Earth to experience different
More informationAstrock, t he A stronomical Clock
Astrock, t he A stronomical Clock The astronomical clock is unlike any other clock. At first glance you ll find it has similar functions of a standard clock, however the astronomical clock can offer much
More informationOA3-10 Patterns in Addition Tables
OA3-10 Patterns in Addition Tables Pages 60 63 Standards: 3.OA.D.9 Goals: Students will identify and describe various patterns in addition tables. Prior Knowledge Required: Can add two numbers within 20
More informationRenewable Energy. Solar Power. Courseware Sample 86352-F0
Renewable Energy Solar Power Courseware Sample 86352-F0 A RENEWABLE ENERGY SOLAR POWER Courseware Sample by the staff of Lab-Volt Ltd. Copyright 2009 Lab-Volt Ltd. All rights reserved. No part of this
More informationEarth, Moon, and Sun Study Guide. (Test Date: )
Earth, Moon, and Sun Study Guide Name: (Test Date: ) Essential Question #1: How are the Earth, Moon, and Sun alike and how are they different? 1. List the Earth, Moon, and Sun, in order from LARGEST to
More informationSolar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?
Solar System 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? A) Earth B) Sun C) Moon D) Polaris 2. Which object orbits Earth in both the Earth-centered
More informationASTR 100 Introduction to Astronomy Syllabus for Fall 2015
Instructor Information Name Office Email Office Hours Course Information ASTR 100 Introduction to Astronomy Syllabus for Fall 2015 Prof. Emily Hardegree-Ullman 125 Astronomy emilyehu@illinois.edu Tuesdays
More informationChapter 6 Telescopes: Portals of Discovery. How does your eye form an image? Refraction. Example: Refraction at Sunset.
Chapter 6 Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning:! How does your eye form an image?! How do we record images? How does your eye form an image?
More informationOrientation to the Sky: Apparent Motions
Chapter 2 Orientation to the Sky: Apparent Motions 2.1 Purpose The main goal of this lab is for you to gain an understanding of how the sky changes during the night and over the course of a year. We will
More informationEarth, Moon, and Sun Inquiry Template Eclipses
One Stop Shop For Educators The following instructional plan is part of a GaDOE collection of Unit Frameworks, Performance Tasks, examples of Student Work, and Teacher Commentary. Many more GaDOE approved
More informationBuilding Models to Scale
Day Laboratory - 1 Building Models to Scale Introduction Can you picture the dimensions of the solar system? Probably not. The sizes and distances involved are so great that the mind tends to give up,
More informationUnit One Organizer: The Stars and Our Solar System (Approximate Time: 7 Weeks)
The following instructional plan is part of a GaDOE collection of Unit Frameworks, Performance Tasks, examples of Student Work, and Teacher Commentary. Many more GaDOE approved instructional plans are
More informationEquations, Lenses and Fractions
46 Equations, Lenses and Fractions The study of lenses offers a good real world example of a relation with fractions we just can t avoid! Different uses of a simple lens that you may be familiar with are
More informationThe Analemma for Latitudinally-Challenged People
The Analemma for Latitudinally-Challenged People Teo Shin Yeow An academic exercise presented in partial fulfillment for the degree of Bachelor of Science with Honours in Mathematics Supervisor : Associate
More informationMapping the Magnetic Field
I Mapping the Magnetic Field Mapping the Magnetic Field Vector Fields The electric field, E, and the magnetic field, B, are two examples of what are termed vector fields, quantities which have both magnitude
More informationReasons for Seasons. Question: TRUE OR FALSE. Question: TRUE OR FALSE? What causes the seasons? What causes the seasons?
Reasons for Seasons Question: TRUE OR FALSE? Earth is closer to the Sun in summer and farther from the Sun in winter. Question: TRUE OR FALSE? Earth is closer to the Sun in summer and farther from the
More informationExplain the Big Bang Theory and give two pieces of evidence which support it.
Name: Key OBJECTIVES Correctly define: asteroid, celestial object, comet, constellation, Doppler effect, eccentricity, eclipse, ellipse, focus, Foucault Pendulum, galaxy, geocentric model, heliocentric
More informationEARTH'S MOTIONS. 2. The Coriolis effect is a result of Earth's A tilted axis B orbital shape C revolution D rotation
EARTH'S MOTIONS 1. Which hot spot location on Earth's surface usually receives the greatest intensity of insolation on June 21? A Iceland B Hawaii C Easter Island D Yellowstone 2. The Coriolis effect is
More informationThis booklet is for candidates who are applying for entry level jobs with New York State and with local governments in the state.
New York State Department of Civil Service Publication Civil Service Examinations How To Take A Written Test This booklet is for candidates who are applying for entry level jobs with New York State and
More informationSECOND GRADE 1 WEEK LESSON PLANS AND ACTIVITIES
SECOND GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF SECOND GRADE UNIVERSE WEEK 1. PRE: Discovering stars. LAB: Analyzing the geometric pattern of constellations. POST: Exploring
More informationScience Standard 4 Earth in Space Grade Level Expectations
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
More informationMotion & The Global Positioning System (GPS)
Grade Level: K - 8 Subject: Motion Prep Time: < 10 minutes Duration: 30 minutes Objective: To learn how to analyze GPS data in order to track an object and derive its velocity from positions and times.
More information