Distance From the Sun

Similar documents
Exploring the Poles (Without Leaving Your Classroom!)

Evaluation copy. Ground Temperature Measurements. computer OBJECTIVES MATERIALS PRE-LAB QUESTIONS

Evaluation copy. Momentum: A Crash Lesson. computer OBJECTIVES MATERIALS

PRELIMINARY ACTIVITY FOR. Seasons and Angle of Insolation

Evaluation copy. First-Class Levers. computer OBJECTIVES MATERIALS

The Magnetic Field of a Permanent Magnet. Evaluation copy

Center of Mass. Evaluation copy

Heat of Combustion: Magnesium. This equation can be obtained by combining equations (1), (2), and (3): (1) MgO(s) + 2 HCl(aq) MgCl 2 (aq) + H 2 O(l)

Evaluation copy. The Molar Mass of a Volatile Liquid. computer OBJECTIVES MATERIALS

Determining the Concentration of a Solution: Beer s Law. Evaluation copy. Figure 1

Energy of a Tossed Ball. Evaluation Copy. Motion Detector. Figure 1. volleyball, basketball, or other similar

Photosynthesis and Respiration. Evaluation copy

Chemical Equilibrium: Finding a Constant, Kc

Diffusion through Membranes. Evaluation copy. dialysis tubing, 2.5 cm 12 cm

Cart on a Ramp. Evaluation Copy. Figure 1. Vernier Dynamics Track. Motion Detector Bracket

Evaluation copy. Acids and Bases. computer OBJECTIVES MATERIALS

Rate Law Determination of the Crystal Violet Reaction. Evaluation copy

Newton s Third Law. Evaluation copy

Establishing a Table of Reduction Potentials: Micro-Voltaic Cells. Evaluation copy

Evaluation copy. Transpiration. Computer OBJECTIVES

Spring Thing: Newton s Second Law. Evaluation copy

Ashes to Ashes: Using evaporation rate to identify an unknown liquid

Acid Rain. Evaluation copy

Computer 3. Lifetime Measurement

The Decomposition of Hydrogen Peroxide. Evaluation copy

Energy Storage and Transfer: Gravitational Energy. Evaluation copy. Vernier Photogate (Extension only)

Transpiration. Evaluation copy

Measuring Momentum: Using distance moved after impact to estimate velocity

Acid-Base Titration. Evaluation copy

Weather Stations. Evaluation copy. 9. Post live weather data on the school s web site for students, faculty and community.

Seasons and Angle of Insolation

Standardizing a Solution of Sodium Hydroxide. Evaluation copy

Evaluation copy 10A. Impulse and Momentum. Experiment INTRODUCTION OBJECTIVES MATERIALS PRE-LAB QUESTIONS

What Causes the Seasons?

Spectrometer User s Guide

What Causes the Seasons?

Ocean Optics Red Tide UV-VIS Spectrometer (Order Code: SPRT-UV-VIS)

Purpose of the experiment

Graphing Motion (Part 1 Distance)

Unit: Planetary Science

Coulomb s Law Mini-Lab

Falling Objects. Experiment OBJECTIVES MATERIALS

The activities below cover LO1: Be able to apply the principles of good laboratory practice. Associated files:

DIFFUSION THROUGH MEMBRANES STANDARDS B C.4 INTRODUCTION

L ESSON P LAN:DETERMINING THE E FFECT OF D ISTANCE (PART 1) AND I NCLINATION (PART 2)

Yes, inner planets tend to be and outer planets tend to be.

Picket Fence Free Fall

Where IS North? LabQuest OBJECTIVES

Date Course Name Instructor Name Student(s) Name. Atwood s Machine

Astron 104 Laboratory #4 Orbital Motion of a Planet

APS 1030 Astronomy Lab 79 Kepler's Laws KEPLER'S LAWS

Writing Scientific Notation ACTIVITY: Finding ph Levels. How can you write a number in. scientific notation?

Physics/Science Unit P1: Universal Physics Foundation Tier Wednesday 5 June 2013 Afternoon Time: 1 hour plus your additional time allowance

Just How Big Is Our Solar System?

PH104 Lab 2 Measuring Distances Pre-Lab

6 TH GRADE ACCURATE PLANET SIZES AND DISTANCE FROM THE SUN ACTIVITY

Static and Kinetic Friction

Lesson 2 The Inner Planets

EXPLORING THE RELATIONSHIP BETWEEN LIGHT INTENSITY AND DISTANCE

What is Crater Number Density?

Learning Outcomes in Focus

How Do We Get Light from Matter: The Origin of Emission

THE CONSERVATION OF ENERGY - PENDULUM -

Putting Earth In Its Place

Falling Objects. LabQuest OBJECTIVES MATERIALS PROCEDURE

Intensity of Light and Heat. The second reason that scientists prefer the word intensity is Well, see for yourself.

ASTROMATH 101: BEGINNING MATHEMATICS IN ASTRONOMY

Experiment 14 It s Snow Big Deal

ASTRO 1050 LAB #1: Scientific Notation, Scale Models, and Calculations

READY-TO-USE LESSON PLANS. Meet the Planets

Earth Mars Oppositions and Conjunctions

Lesson 5 Why the Earth s formation gives us seasons

Chapter 4. Forces and the Laws of Motion. CH 4 Forces and the Laws of Motion.notebook. April 09, Changes in Motion. A. Force

Investigation: Transit Tracks

Student s guide CESAR Science Case The Venus transit and the Earth-Sun distance

PHYSICS LAB FREE FALL. Date: GRADE: PHYSICS DEPARTMENT JAMES MADISON UNIVERSITY

Simple Harmonic Motion

ASTRONOMY 25 SUMMER 2017 PROJECT 2: THE HEIGHT OF THE SUN

Work and Energy. This sum can be determined graphically as the area under the plot of force vs. distance. 1

VOYAGE OF DISCOVERY TEACHER PAGE

Conservation of Momentum Using PASCO TM Carts and Track to Study Collisions in One Dimension

Name Class Date. Chapter 23 Touring Our Solar System Investigation 23

Empirical Gas Laws (Parts 1 and 2) Pressure-volume and pressure-temperature relationships in gases

Transit Tracks. Activity G14. What s This Activity About? Tips and Suggestions. What Will Students Do? What Will Students Learn?

OBSERVING PROJECT PARTNER ELECTION

PH104 Lab 1 Light and Matter Pre-lab

FreeFall Student Activity Guide

Large and small planets

Developed and Published by. AIMS Education Foundation

Define umbra and penumbra. Then label the umbra and the penumbra on the diagram below. Umbra: Penumbra: Light source

NAME: PERIOD: DATE: LAB PARTNERS: LAB #39 ECCENTRICITY OF PLANETARY ORBITS

Patterns in the Solar System (Chapter 18)

Chemistry with Mr. Faucher. Acid-Base Titration

Evaporation and Intermolecular Attractions

Conservation of Energy

Obtain an optical "bench" setup (there should be three sliding mounts on the calibrated horizontal bar. The setup is shown in the diagram below.

Observing Sessions and Lab Activity Reports

LAB MECH8.COMP From Physics with Computers, Vernier Software & Technology, 2003.

Lesson 1 The Structure of the Solar System

LABORATORY INVESTIGATION

Transcription:

Distance From the Sun Computer 32 Have you ever thought about what it would be like if you were on another planet looking back at the sun? In this activity, you will use the Light Probe to get an idea of how much light the planets would receive. OBJECTIVES In this activity, you will Make a simulation of the planets of our solar system to scale. Measure the amount of light from a light source at different distances. Draw conclusions about conditions on other planets. MATERIALS computer with Logger Lite software installed Go! Link interface TI Light Probe meter stick table or floor lamp with 60 watt bulb tape and marking pen PROCEDURE Part I Marking the Distances of the Planets 1. Make sure the Light Probe is connected to the Go! Link and that the Go! Link is connected to the computer. 2. Start Logger Lite on your computer. 3. Open the file for this activity by doing the following: a. Click the Open button,. b. Open the file called Elementary Science. c. Open the file called 32 Distance from Sun. Evaluation copy Elementary Science with Vernier 32-1

Computer 32 4. Now you will use the meter stick and tape to make a scale model that shows the relative distances of the planets from the sun by following the steps below: a. Put 0 cm end of the meter stick at the light. b. Measure 10 cm from the light and mark the place with a piece of tape labeled Mercury. In this model, 25 cm is one Astronomical Unit, or AU. One AU is the distance from the Sun to the Earth. All of the other planet distances are compared to this distance between Earth and the Sun. c. Measure 20 cm from the light. Mark this place with a piece of tape labeled Venus. d. Continue marking the distances from the sun to the planets, using the Table of Distances, below. Table of Distances Planet Distance in meters Distance in AU Mercury 10 cm 0.4 AU Venus 18 cm 0.7 AU Earth 25 cm 1 AU Mars 38 cm 1.5 AU Jupiter 125 cm 5 AU Part II How Much Light Would Each Planet Get From the Sun? Key Question How does the light level change when you get farther away from the sun? Prediction Click on the Prediction button,, and draw how you think the light level will change as you increase the distance between the Light Probe and the light bulb. 5. Turn the lamp on, and then darken the room as much as possible. 6. Collect data by following the steps below: a. Decide who will hold the Light Probe and who will enter the data into the computer. b. Click to begin data collection. c. Put the probe at the position where Mercury is located in the model so the probe is pointing towards the lamp. 32-2 Elementary Science with Vernier

Distance From the Sun d. Look at the live meter on the computer screen, showing what light level is reaching the probe. Move the tip around a bit to get the highest reading you can. Careful: Make sure you are still pointing towards the lamp! e. Click to save this data point. f. In the box that appears on the screen, enter in the value for the planet location in AU based on the table above (for Mercury this value is 0.4) and then click. 7. Repeat Step 6 for each of the planets in the model. 8. When you have collected all your data, click to end data collection. 9. Write your observations on the Observations Sheet below. Observations Sheet Write observations about how the light level changes as you move away from the sun. Elementary Science with Vernier 32-3

Computer 32 ANALYZE YOUR DATA 1. Use the data from your graph to describe the light levels of the first five planets. 2. Write about two ways that we on Earth depend on the sun. 3. Imagine you have traveled to one of the outermost planets. Write a sentence that describes what the sunlight on the planet might be like and how the sun would look from that planet. 4. Imagine that we are going to try to begin a colony on another planet. Using what you know about how we on Earth depend on the Sun, and your data from this activity, describe what you would need to make the colony a place where humans could survive. Good job!! 32-4 Elementary Science with Vernier

Vernier Lab Safety Instructions Disclaimer THIS IS AN EVALUATION COPY OF THE VERNIER STUDENT LAB. This copy does not include: Safety information Essential instructor background information Directions for preparing solutions Important tips for successfully doing these labs The complete Elementary Science with Vernier lab manual includes 43 labs and essential teacher information. The full lab book is available for purchase at: http://www.vernier.com/cmat/ewv.html Vernier Software & Technology 13979 S.W. Millikan Way Beaverton, OR 97005-2886 Toll Free (888) 837-6437 (503) 277-2299 FAX (503) 277-2440 info@vernier.com www.vernier.com