Date: Problem Set # 1. Unit conversion is an important part of any scientific research. Please view the following link: c = (gh) α (3)
|
|
- Matthew Davidson
- 6 years ago
- Views:
Transcription
1 Problem Set # 1 Instructions: Numerical answers require units and appropriate numbers of significant digits. Remember to show your work! Review Problems: R-1. (3 points) For the function f(x) = 4x 3 6x + 2 (1) (a) Find the indefinite integral, F(x), of this function. (b) Evaluate the constant of integration if F(x = 2) = 23. (c) Check your answer by differentiating F(x) to show that df(x) dx = f(x) (2) R-2. (4 points) Unit conversion: Unit conversion is an important part of any scientific research. Please view the following link: Here, we are going to work on a simple example. Speed of tsunamis, c, depends only on the ocean depth and is given by the following formula in the high seas. c = (gh) α (3) where g is the acceleration due to gravity and h is the ocean depth at any point. EARTH Fall 2017
2 (a) Using the units (dimensions), find the exponent α. (b) Assuming that the typical ocean depth is 4000 m, calculate the typical speed of tsunami waves in m/s. (c) Calculate the tsunami speed in km/h. (d) Calculate the tsunami speed in mi/h. (e) How do these numbers compare with the speed of a jet airliner? 1. (4 points) Consider the equations for the gravitational force and the electrostatic force: F g = Gm 1m 2 F r 2 E = kq 1q 2 r 2 (a) Compare the two equations. In what ways do they differ? (b) A large ship (mass = kg) is out at sea when a small fish (mass = 2 kg) swims 1 meters below it. How much force does the fish exert on the ship? How much force does the ship exert on the fish? Should the fish be worried about getting pulled to the ship? Why or why not? 2. (5 points) To determine the size of the moon, use the fact that it appears to be the same size as a dime held 154 cm from the observer (this is called having the same angular diameters). If the moon is km away, what is the radius of the moon? How does the moon compare in volume to the earth? Figure 1: Dime and the Moon. EARTH Fall 2017
3 3. (5 points) The acceleration of gravity on the lunar surface is about 1 that on the earth s 6 surface. Given the moon s radius from problem 2, find its mass and average mean density. 4. (3 points) Your lazy roommate thinks that instead of actually working on problem 3, you can instead say that if the acceleration of gravity on the moon was 1 that on earth, its mean 6 density is 1 that of earth. Why isn t this correct? 6 5. (3 points) A model often used for the moon is that it is made of (green) cheese. Test this model by comparing its density to a block of Monterey Jack with dimensions 4 cm 6 cm 6 cm and a mass of 143 grams. 6. (4 points) Show how gravity at the Moon s surface would change if its: (a) Radius is kept constant, but density is doubled; (b) Radius is doubled, but density is kept constant. 7. (6 points) We saw in class that a body in orbit has an orbital period which depends on its distance from the center of the planet being orbited. Some satellites are put in synchronous orbit that is, with a period equal to one planetary day so that they stay above the same point on the surface as the planet rotates. For the planet Mars, how large is the radius of this orbit? How high above Mars s surface is the satellite? 8. (4 points) Moment of inertia factors I/MR 2 (and other information) for the various planets can be found on the website or on the class website by clicking on the planetary fact sheet, which is found underneath TOPIC 1: Size, Mass, & Density of the Earth. Find the values for the Sun, Venus, Mars, the moon, Earth, and Jupiter. Put these values in order from largest to smallest and explain what they tell about the density distribution (the way that the density changes from the surface to the center of an object). EARTH Fall 2017
4 9. (8 points) The formulas for calculating the mass and moment of inertia of a planet are: M = 4π a 0 ρ(r)r 2 dr I = 8 a 3 π ρ(r)r 4 dr 0 Given these formulas, show that a two-shell planet with mantle density ρ m, core density ρ c, radius a, and core radius r c, has a mass and moment of inertia: M = 4 3 π[ρ ma 3 + (ρ c ρ m )r 3 c] I = 8 15 π[ρ ma 5 + (ρ c ρ m )r 5 c] C-1. 1 (8 points) Using the results of problem 9: (a) Write a spreadsheet or program that takes as inputs a, ρ m, ρ c, and r c and computes r c /a, I, M, and I/Ma 2 (Hint: In Excel the symbol ˆ is used to raise a quantity to a power). (b) Test this by setting ρ m = ρ c. What is I/Ma 2 and why? (c) Test this by setting ρ c = 0 and r c = 0.99a. What is I/Ma 2 and why? (d) Derive a plausible two-layer model for Mercury, assuming I/Ma 2 = In addition to your answers for parts (a) to (d), please hand in a printout or screenshot of your code or excel spreadsheet. C-2. (10 points) Use the uploaded coordinates from the entire class (on the online spreadsheet) in Lab#0 and follow these steps to make a histogram of latitudes and longitudes of the measurements. Note: Watch the YouTube video at to see how you can make histograms in Excel. (a) On a new spreadsheet on your computer, copy and paste all the longitudes in a single column and all the latitudes in another one as shown in Fig Problems numbered as C-# are computer problems. EARTH Fall 2017
5 Figure 2: Copy and paste the values for longitude and latitude into a spreadsheet. (b) In a third column, list the bins between in longitude and between in latitude. (c) Use Excel s Data Analysis tool under the Data tab to make a histogram. Note: If the Data Analysis tool is not available on your computer, you can enable it at Tools>Excel Add-ins>Analysis ToolPak. (d) Turn in a printout of your histogram attached to this handout. C-3. (5 points) Use Google Earth to plot the measurements on a map: (a) Save the only two columns in the spreadsheet you made in C-2 in the CSV (comma sparated) format which is going to be a text file. (b) Open Google Earth, and click on File>Import; from the dialog box that opens, select your CSV file. EARTH Fall 2017
6 (c) In the new dialog box, make sure the Comma option is checked and also the Field Type is set to Delimited. Click Next. (d) In the drop-down menue, set the Latitude Field to the the one that begins with and the Longitude Field to the one that begins with Click Next. (e) Make sure the field types are set to floating point. Click Finish. (f) You are asked if you want to apply a template to the features you ingested. Choose Yes. (g) Check Create new template. Click OK. (h) You can edit the appearance of your points on the map by setting the attributes (colors & icon) here. When your are done, click OK. save your template if you want. (i) On the left side pane, double click on your file name, and make sure to check the boxes next to your points to make them appear on the map. (j) Zoom into the map until you get a close view of the points, and then save the view as an image. (k) Attach the image to this handout before you turn it in. C-4. (5 points) Usually, geospatial measurements are considered to be accurate(=exact) in geodesy. For istance if you double click/tap on a fixed point (say the corner of the planter which you measured in Lab#0) in Goole Earth or Google Map, you get coordinates that are fixed. But the values you got for your location s coordinates (the blue dot in Google Map) vary every time you make a measurement. Try to quantify how the set of measurements by the entire class compares to the reference value, i.e W, N. How accurate/precise are the measurements? (Hint: think in terms of resolution) EARTH Fall 2017
You Might Also Like. I look forward helping you focus your instruction while saving tons of time. Kesler Science Station Lab Activities 40%+ Savings!
Thanks Connect Thank you for downloading my product. I truly appreciate your support and look forward to hearing your feedback. You can connect with me and find many free activities and strategies over
More information= v = 2πr. = mv2 r. = v2 r. F g. a c. F c. Text: Chapter 12 Chapter 13. Chapter 13. Think and Explain: Think and Solve:
NAME: Chapters 12, 13 & 14: Universal Gravitation Text: Chapter 12 Chapter 13 Think and Explain: Think and Explain: Think and Solve: Think and Solve: Chapter 13 Think and Explain: Think and Solve: Vocabulary:
More informationPhysics E-1ax, Fall 2014 Experiment 3. Experiment 3: Force. 2. Find your center of mass by balancing yourself on two force plates.
Learning Goals Experiment 3: Force After you finish this lab, you will be able to: 1. Use Logger Pro to analyze video and calculate position, velocity, and acceleration. 2. Find your center of mass by
More informationAdding point data. Account not required
Adding point data Find patterns in mountains of data You begin to get a strong sense of what maps can do from this lesson. The image shows a total of 58,000 airline routes on one map. The Web Mercator
More informationRemember that C is a constant and ë and n are variables. This equation now fits the template of a straight line:
CONVERTING NON-LINEAR GRAPHS INTO LINEAR GRAPHS Linear graphs have several important attributes. First, it is easy to recognize a graph that is linear. It is much more difficult to identify if a curved
More informationPatterns in the Solar System (Chapter 18)
GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Patterns in the Solar System (Chapter 18) For this assignment you will require: a calculator, colored pencils, a metric ruler, and meter stick.
More informationComputer simulation of radioactive decay
Computer simulation of radioactive decay y now you should have worked your way through the introduction to Maple, as well as the introduction to data analysis using Excel Now we will explore radioactive
More informationUSING THE EXCEL CHART WIZARD TO CREATE CURVE FITS (DATA ANALYSIS).
USING THE EXCEL CHART WIZARD TO CREATE CURVE FITS (DATA ANALYSIS). Note to physics students: Even if this tutorial is not given as an assignment, you are responsible for knowing the material contained
More informationPatterns in the Solar System (Chapter 18)
GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Patterns in the Solar System (Chapter 18) For this assignment you will require: a calculator, colored pencils, a metric ruler, and meter stick.
More informationDISCRETE RANDOM VARIABLES EXCEL LAB #3
DISCRETE RANDOM VARIABLES EXCEL LAB #3 ECON/BUSN 180: Quantitative Methods for Economics and Business Department of Economics and Business Lake Forest College Lake Forest, IL 60045 Copyright, 2011 Overview
More informationStudent Exploration: Uniform Circular Motion
Name: Date: Student Exploration: Uniform Circular Motion Vocabulary: acceleration, centripetal acceleration, centripetal force, Newton s first law, Newton s second law, uniform circular motion, vector,
More informationIllustrate It! You will need to set out colored pencil and markers at this station.
Kesler Science Station Lab Comets, Meteors, and Asteroids Teacher Directions Explore It! I will spend much of my time at this station making sure that the students are doing the orbits correctly. I have
More informationGravity and the Laws of Motion
Gravity and the Laws of Motion Mass Mass is the amount of stuff (matter) in an object. Measured in grams (kg, mg, cg, etc.) Mass will not change unless matter is added or taken away. Weight Weight is the
More informationLab 11 Simple Harmonic Motion A study of the kind of motion that results from the force applied to an object by a spring
Lab 11 Simple Harmonic Motion A study of the kind of motion that results from the force applied to an object by a spring Print Your Name Print Your Partners' Names Instructions April 20, 2016 Before lab,
More informationUnit: Planetary Science
Orbital Motion Kepler s Laws GETTING AN ACCOUNT: 1) go to www.explorelearning.com 2) click on Enroll in a class (top right hand area of screen). 3) Where it says Enter class Code enter the number: MLTWD2YAZH
More informationI. Introduction. II. An Introduction to Starry Night NAME: ORBITAL MOTION
NAME: ORBITAL MOTION What will you learn in this Lab? You will be using some special software to simulate the motion of planets in our Solar System and across the night sky. You will be asked to try and
More informationGravity Investigation
Gravity Investigation Name: Learning Target #14: I am able to use evidence to support the claim that gravitational interactions are attractive and depend on the masses of objects. From acorns to apples,
More information2. What is the force weight of a 45 kg desk? 3. Give a scenario example for each of Newton s Laws.
Catalyst 1.What is the unit for force? Newton (N) 2. What is the force weight of a 45 kg desk? 3. Give a scenario example for each of Newton s Laws. HANDS UP!! 441 N 4. What is net force? Give an example.
More informationDid the Samoa Tsunami Affect the Movement of a Drifter in Monterey Bay? name
Did the Samoa Tsunami Affect the Movement of a Drifter in Monterey Bay? name In this lab we will gain experience manipulating the drifter data in Google Earth. During the September 2009 deployment of the
More informationGPS Worldwide Laboratory: a community of knowledge-seekers spanning the globe
Laboratory B: (predicting and verifying satellite visibility) Lab Date: 1 November 2014 1 day depending on your time zone). YOU MUST DO THIS PARTICULAR LAB ON THE SPECIFIED DAY. Lab Goals: Predict when
More information1. Double-click the ArcMap icon on your computer s desktop. 2. When the ArcMap start-up dialog box appears, click An existing map and click OK.
Module 2, Lesson 1 The earth moves In this activity, you will observe worldwide patterns of seismic activity (earthquakes) and volcanic activity (volcanoes). You will analyze the relationships of those
More information6 TH GRADE ACCURATE PLANET SIZES AND DISTANCE FROM THE SUN ACTIVITY
6 TH GRADE ACCURATE PLANET SIZES AND DISTANCE FROM THE SUN ACTIVITY Summary: Accurate planet size and distance from the Sun is studied in this lesson. Each student constructs a correctly scaled diagram
More informationLab 4: Gauss Gun Conservation of Energy
Lab 4: Gauss Gun Conservation of Energy Before coming to Lab Read the lab handout Complete the pre-lab assignment and hand in at the beginning of your lab section. The pre-lab is written into this weeks
More informationNewton's 2 nd Law. . Your end results should only be interms of m
Newton's nd Law Introduction: In today's lab you will demonstrate the validity of Newton's Laws in predicting the motion of a simple mechanical system. The system that you will investigate consists of
More informationNewton s Law of Universal Gravitation
Newton s Law of Universal Gravitation 2009 by Goodman & Zavorotniy www.njctl.org 1 Newton's Law of Universal Gravitation Gravitational Force Click on the topic to go to that section Gravitational Field
More informationLAB 10: GRAVITY ANOMALIES AND CORRECTIONS
NAME: LAB TIME: LAB 10: GRAVITY ANOMALIES AND CORRECTIONS The following lab will introduce you to the basic concepts of gravitational forces, accelerations, and using variations in gravity to understand
More informationGravity Teacher s Guide
Gravity Teacher s Guide 1.0 Summary Gravity is the 9 th and final Dynamica activity to be done before the Post-Test. This activity has not undergone many changes from the last school year. It should take
More informationExam 1: Physics 2113 Spring :00 PM, Monday, February 3, Abdelwahab Abdelwahab Lee Zuniga Tzanov Zuniga Sec 1 Sec 2 Sec 3 Sec 4 Sec 5 Sec 6
Exam 1: Physics 2113 Spring 2016 6:00 PM, Monday, February 3, 2016 Last Name First Name Clearly circle your section: MON/WEDS/FRI SECTIONS TUES/THURS SECTIONS Abdelwahab Abdelwahab Lee Zuniga Tzanov Zuniga
More informationMoment of Inertia: Rotational Energy
Lab Section (circle): Day: Monday Tuesday Time: 8:00 9:30 1:10 2:40 Moment of Inertia: Rotational Energy Name Partners Pre-Lab You are required to finish this section before coming to the lab; it will
More informationThank you for your purchase!
TM Thank you for your purchase! Please be sure to save a copy of this document to your local computer. This activity is copyrighted by the AIMS Education Foundation. All rights reserved. No part of this
More informationLecture 23: Jupiter. Solar System. Jupiter s Orbit. The semi-major axis of Jupiter s orbit is a = 5.2 AU
Lecture 23: Jupiter Solar System Jupiter s Orbit The semi-major axis of Jupiter s orbit is a = 5.2 AU Jupiter Sun a Kepler s third law relates the semi-major axis to the orbital period 1 Jupiter s Orbit
More informationDownloading GPS Waypoints
Downloading Data with DNR- GPS & Importing to ArcMap and Google Earth Written by Patrick Florance & Carolyn Talmadge, updated on 4/10/17 DOWNLOADING GPS WAYPOINTS... 1 VIEWING YOUR POINTS IN GOOGLE EARTH...
More informationAP Physics 1 Summer Assignment Packet
AP Physics 1 Summer Assignment Packet 2017-18 Welcome to AP Physics 1 at David Posnack Jewish Day School. The concepts of physics are the most fundamental found in the sciences. By the end of the year,
More informationName. Satellite Motion Lab
Name Satellite Motion Lab Purpose To experiment with satellite motion using an interactive simulation in order to gain an understanding of Kepler s Laws of Planetary Motion and Newton s Law of Universal
More informationTEACHER Worksheet: Phases of the Moon and Tides
TEACHER Worksheet: Phases of the Moon and Tides Subject: Physics & Astronomy Grades levels: 6-8 Description: Data pattern recognition exercise where students compare the two daily datasets (for one month)
More information(THIS IS AN OPTIONAL BUT WORTHWHILE EXERCISE)
PART 2: Analysis in ArcGIS (THIS IS AN OPTIONAL BUT WORTHWHILE EXERCISE) Step 1: Start ArcCatalog and open a geodatabase If you have a shortcut icon for ArcCatalog on your desktop, double-click it to start
More informationAssignment 1. Due Feb. 11, 2019
Assignment 1 Due Feb. 11, 2019 Show all work and turn in answers on separate pages, not on these pages. Circle your final answers for clarity. Be sure to show/explain all of your reasoning and that your
More informationThe Cosmic Perspective Seventh Edition. Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Chapter 4 Lecture
Chapter 4 Lecture The Cosmic Perspective Seventh Edition Making Sense of the Universe: Understanding Motion, Energy, and Gravity 2014 Pearson Education, Inc. Making Sense of the Universe: Understanding
More informationGEOL212 Due 9/24/18 Homework 4
GEOL212 Due 9/24/18 Homework 4 General instructions: Although you are allowed to discuss homework questions with your classmates, your work must be uniquely your own. Thus, please answer all questions
More informationA = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great Pearson Education, Inc.
Q13.1 The mass of the Moon is 1/81 of the mass of the Earth. Compared to the gravitational force that the Earth exerts on the Moon, the gravitational force that the Moon exerts on the Earth is A. 81 2
More informationThe force of gravity holds us on Earth and helps objects in space stay
96 R E A D I N G The force of gravity holds us on Earth and helps objects in space stay in orbit. The planets in the Solar System could not continue to orbit the Sun without the force of gravity. Astronauts
More informationUnit 5 Gravitation. Newton s Law of Universal Gravitation Kepler s Laws of Planetary Motion
Unit 5 Gravitation Newton s Law of Universal Gravitation Kepler s Laws of Planetary Motion Into to Gravity Phet Simulation Today: Make sure to collect all data. Finished lab due tomorrow!! Universal Law
More informationLinear Motion with Constant Acceleration
Linear Motion 1 Linear Motion with Constant Acceleration Overview: First you will attempt to walk backward with a constant acceleration, monitoring your motion with the ultrasonic motion detector. Then
More informationDisplaying Latitude & Longitude Data (XY Data) in ArcGIS
Displaying Latitude & Longitude Data (XY Data) in ArcGIS Created by Barbara Parmenter and updated on 2/15/2018 If you have a table of data that has longitude and latitude, or XY coordinates, you can view
More informationThe Circular Motion Lab
Name Date Class Answer questions in complete sentences The Circular Motion Lab Introduction We have discussed motion in straight lines and parabolic arcs. But many things move in circles or near circles,
More informationMIS 0855 Data Science (Section 005) Fall 2016 In-Class Exercise (Week 4) Visualizing with Maps
MIS 0855 Data Science (Section 005) Fall 2016 In-Class Exercise (Week 4) Visualizing with Maps Objective: Learn how to use Tableau s powerful mapping tools Learning Outcomes: Learn at what levels (e.g.
More informationChapter 5 Lecture Notes
Formulas: a C = v 2 /r a = a C + a T F = Gm 1 m 2 /r 2 Chapter 5 Lecture Notes Physics 2414 - Strauss Constants: G = 6.67 10-11 N-m 2 /kg 2. Main Ideas: 1. Uniform circular motion 2. Nonuniform circular
More informationPrelab 4: Revolution of the Moons of Jupiter
Name: Section: Date: Prelab 4: Revolution of the Moons of Jupiter Many of the parameters astronomers study cannot be directly measured; rather, they are inferred from properties or other observations of
More informationInvestigating the Solar System
Investigating the Solar System This Workbook belongs to: Our Local Star: The Sun Location in The Solar System Interesting Facts 1. 2. 3. 4. Name of Star: THE SUN 5. Draw and Color your own Sun in the blank
More informationFIFTH MIDTERM -- REVIEW PROBLEMS
Physics 2210 Fall 2005 Paolo Gondolor FIFTH MIDTERM -- REVIEW PROBLEMS A solution set is available on the course web page in pdf format (no solutions for 27-29). 7 1. Assume that the planet Uranus has
More informationPHYSICS 221 Fall 2016 EXAM 2: November 02, :15pm 10:15pm. Name (printed): Recitation Instructor: Section #:
PHYSICS 221 Fall 2016 EXAM 2: November 02, 2016 8:15pm 10:15pm Name (printed): Recitation Instructor: Section #: INSTRUCTIONS: This exam contains 25 multiple-choice questions, plus 2 extra-credit questions,
More informationWork and Energy. computer masses (200 g and 500 g) If the force is constant and parallel to the object s path, work can be calculated using
Work and Energy OBJECTIVES Use a Motion Detector and a Force Sensor to measure the position and force on a hanging mass, a spring, and a dynamics cart. Determine the work done on an object using a force
More informationAssignment #0 Using Stellarium
Name: Class: Date: Assignment #0 Using Stellarium The purpose of this exercise is to familiarize yourself with the Stellarium program and its many capabilities and features. Stellarium is a visually beautiful
More information5.24 Page 1. Universal gravitational constant. acceleration of apple. kgs
5.24 Page 1 5.24 F N Force of gravity G 6.673 10 11 m 3 m 1 0.20 kg Mass of apple m earth 5.98 10 24 kg Mass of the earth r earth 6.38 10 6 m Radius of the earth a m s 2 acceleration of apple F = G m 1
More information1. Write the symbolic representation and one possible unit for angular velocity, angular acceleration, torque and rotational inertia.
ROTATIONAL DYNAMICS Pre-Lab Questions Page Name: Class: Roster Number: Instructor: 1. Write the symbolic representation and one possible unit for angular velocity, angular acceleration, torque and rotational
More informationData Structures & Database Queries in GIS
Data Structures & Database Queries in GIS Objective In this lab we will show you how to use ArcGIS for analysis of digital elevation models (DEM s), in relationship to Rocky Mountain bighorn sheep (Ovis
More informationPhysics 2211 M Quiz #2 Solutions Summer 2017
Physics 2211 M Quiz #2 Solutions Summer 2017 I. (16 points) A block with mass m = 10.0 kg is on a plane inclined θ = 30.0 to the horizontal, as shown. A balloon is attached to the block to exert a constant
More informationNewton's Law of Universal Gravitation
Section 2.17: Newton's Law of Universal Gravitation Gravity is an attractive force that exists between all objects that have mass. It is the force that keeps us stuck to the earth and the moon orbiting
More informationMathematica Project 3
Mathematica Project 3 Name: Section: Date: On your class s Sakai site, your instructor has placed 5 Mathematica notebooks. Please use the following table to determine which file you should select based
More informationExploring Graphs of Polynomial Functions
Name Period Exploring Graphs of Polynomial Functions Instructions: You will be responsible for completing this packet by the end of the period. You will have to read instructions for this activity. Please
More informationGravity and Coulomb s Law
AP PHYSICS 1 Gravity and Coulomb s Law 016 EDITION Click on the following link or scan the QR code to complete the evaluation for the Study Session https://www.surveymonkey.com/r/s_sss Copyright 016 National
More informationNewton s Gravitational Law
1 Newton s Gravitational Law Gravity exists because bodies have masses. Newton s Gravitational Law states that the force of attraction between two point masses is directly proportional to the product of
More informationGravity. James H Dann, Ph.D. Say Thanks to the Authors Click (No sign in required)
Gravity James H Dann, Ph.D. Say Thanks to the Authors Click http://www.ck12.org/saythanks (No sign in required) To access a customizable version of this book, as well as other interactive content, visit
More informationMath Lab 10: Differential Equations and Direction Fields Complete before class Wed. Feb. 28; Due noon Thu. Mar. 1 in class
Matter & Motion Winter 2017 18 Name: Math Lab 10: Differential Equations and Direction Fields Complete before class Wed. Feb. 28; Due noon Thu. Mar. 1 in class Goals: 1. Gain exposure to terminology and
More informationHooke s Law. Equipment. Introduction and Theory
Hooke s Law Objective to test Hooke s Law by measuring the spring constants of different springs and spring systems to test whether all elastic objects obey Hooke s Law Equipment two nearly identical springs,
More informationChapter 4 Thrills and Chills +Math +Depth Acceleration of the Moon +Concepts The Moon is 60 times further away from the center of Earth than objects on the surface of Earth, and moves about Earth in an
More informationInvestigating Factors that Influence Climate
Investigating Factors that Influence Climate Description In this lesson* students investigate the climate of a particular latitude and longitude in North America by collecting real data from My NASA Data
More informationEnd-of-Chapter Exercises
End-of-Chapter Exercises Exercises 1 12 are primarily conceptual questions that are designed to see if you have understood the main concepts of the chapter. Treat all balls with mass as point masses. 1.
More informationAfter you read this section, you should be able to answer these questions:
CHAPTER 3 1 SECTION Properties of Matter What Is Matter? 8.8.b California Science Standards BEFORE YOU READ After you read this section, you should be able to answer these questions: What are the properties
More informationLearning Goals The particle model for a complex object: use the center of mass! located at the center of mass
PS 12A Lab 3: Forces Names: Learning Goals After you finish this lab, you will be able to: 1. Use Logger Pro to analyze video and calculate position, velocity, and acceleration. 2. Measure the normal force
More informationQuestions Chapter 13 Gravitation
Questions Chapter 13 Gravitation 13-1 Newton's Law of Gravitation 13-2 Gravitation and Principle of Superposition 13-3 Gravitation Near Earth's Surface 13-4 Gravitation Inside Earth 13-5 Gravitational
More informationPHYSICS 221 SPRING EXAM 2: March 30, 2017; 8:15pm 10:15pm
PHYSICS 221 SPRING 2017 EXAM 2: March 30, 2017; 8:15pm 10:15pm Name (printed): Recitation Instructor: Section # Student ID# INSTRUCTIONS: This exam contains 25 multiple-choice questions plus 2 extra credit
More informationHow many states. Record high temperature
Record high temperature How many states Class Midpoint Label 94.5 99.5 94.5-99.5 0 97 99.5 104.5 99.5-104.5 2 102 102 104.5 109.5 104.5-109.5 8 107 107 109.5 114.5 109.5-114.5 18 112 112 114.5 119.5 114.5-119.5
More informationMEASUREMENT OF THE CHARGE TO MASS RATIO (e/m e ) OF AN ELECTRON
MEASUREMENT OF THE CHARGE TO MASS RATIO (e/m e ) OF AN ELECTRON Object This experiment will allow you to observe and understand the motion of a charged particle in a magnetic field and to measure the ratio
More informationUsing Microsoft Excel
Using Microsoft Excel Objective: Students will gain familiarity with using Excel to record data, display data properly, use built-in formulae to do calculations, and plot and fit data with linear functions.
More informationInquiry 6.1 Gravity s effect on objects in motion
Inquiry 6.1 Gravity s effect on objects in motion Directions: Follow the procedures below. Write down the purpose, background information and answer any of the questions on your paper. Remember to include
More informationAn area chart emphasizes the trend of each value over time. An area chart also shows the relationship of parts to a whole.
Excel 2003 Creating a Chart Introduction Page 1 By the end of this lesson, learners should be able to: Identify the parts of a chart Identify different types of charts Create an Embedded Chart Create a
More informationBoyle s Law and Charles Law Activity
Boyle s Law and Charles Law Activity Introduction: This simulation helps you to help you fully understand 2 Gas Laws: Boyle s Law and Charles Law. These laws are very simple to understand, but are also
More informationPHYSICS 211 LAB #8: Periodic Motion
PHYSICS 211 LAB #8: Periodic Motion A Lab Consisting of 6 Activities Name: Section: TA: Date: Lab Partners: Circle the name of the person to whose report your group printouts will be attached. Individual
More informationCH 8. Universal Gravitation Planetary and Satellite Motion
CH 8 Universal Gravitation Planetary and Satellite Motion Sir Isaac Newton UNIVERSAL GRAVITATION Newton: Universal Gravitation Newton concluded that earthly objects and heavenly objects obey the same physical
More information1 What Is Matter? Math Focus
CHAPTER 1 1 What Is Matter? SECTION The Properties of Matter BEFORE YOU READ After you read this section, you should be able to answer these questions: What is matter? What is volume and mass? What are
More informationFigure 2.1 The Inclined Plane
PHYS-101 LAB-02 One and Two Dimensional Motion 1. Objectives The objectives of this experiment are: to measure the acceleration due to gravity using one-dimensional motion, i.e. the motion of an object
More informationLarge and small planets
Large and small planets Journey through the Solar System C 41 time 50 minutes. Preparation For the activity Planets show the planets under each other on the board, as shown in the table. learning outcomes
More informationLab #10 Atomic Radius Rubric o Missing 1 out of 4 o Missing 2 out of 4 o Missing 3 out of 4
Name: Date: Chemistry ~ Ms. Hart Class: Anions or Cations 4.7 Relationships Among Elements Lab #10 Background Information The periodic table is a wonderful source of information about all of the elements
More informationAST101: Our Corner of the Universe Lab 5: Solar System Models
AST0: Our Corner of the Universe Lab 5: Solar System Models Name: Partners: NetID: Lab section number: Introduction Objectives The Solar System Models Lab introduces the universe as envisioned by early
More informationElectric Fields and Equipotentials
OBJECTIVE Electric Fields and Equipotentials To study and describe the two-dimensional electric field. To map the location of the equipotential surfaces around charged electrodes. To study the relationship
More information-ASTR 204 Application of Astroimaging Techniques
Lab 5 - JPL Ephemeris, Binary Maker 3 In Lab 5 we ll look at another ephemeris generating tool; Horizons Web-Interface from JPL, and Binary Maker 3 program for generating radial velocity curves and 3-D
More informationDeveloping a Scientific Theory
Name Date Developing a Scientific Theory Equipment Needed Qty Equipment Needed Qty Photogate/Pulley System (ME-6838) 1 String (SE-8050) 1 Mass and Hanger Set (ME-8967) 1 Universal Table Clamp (ME-9376B)
More informationGravity. Earth and Space. Gravity. Background
Background Gravity All of the celestial bodies in the solar system move in predictable patterns known as orbits, and this motion is controlled by gravity. Gravity is a force of attraction between two or
More informationPhysics Lab #6:! Mercury!
Physics 10293 Lab #6: Mercury Introduction Today we will explore the motions in the sky of the innermost planet in our solar system: Mercury. Both Mercury and Venus were easily visible to the naked eye
More information1. What does the catapult exert on or apply to the plane?
Unit 1: Forces and Motion Lesson 2.b Newton s Second Law of Motion Newton s laws predict the motion of most objects. As a basis for understanding this concept: Students know how to apply the law F = ma
More informationLesson Overview Activity video available at edu.zspace.com. Objectives
Gravitational Force Evidence Lesson Overview Activity video available at edu.zspace.com Students will plan and build a structure in Newton's Park to demonstrate the concept of gravity pulling objects "down."
More informationGravity and Orbits. 1. Choose the picture you think shows the gravity forces on the Earth and the Sun.
Name: Grade: Gravity and Orbits Pre-lab 1. Choose the picture you think shows the gravity forces on the Earth and the Sun. (a longer arrow to represents a big force, and a shorter arrow represent a smaller
More informationName: Pd Parent Signature of completion:
Chap 18: Draw or Download a picture showing the order of the planets Section 1: The Nine Planets (452-462) Read Measuring Interplanetary Distances and look at figure 2 on pg 45 What is an astronomical
More informationYes, inner planets tend to be and outer planets tend to be.
1. Planet Density Make some general comments about inner and outer planets density Inner Planets Density Outer Planets Density Is there a pattern or a trend in planet density? Yes, inner planets tend to
More informationGravity Modelling Forward Modelling Of Synthetic Data
Gravity Modelling Forward Modelling Of Synthetic Data After completing this practical you should be able to: The aim of this practical is to become familiar with the concept of forward modelling as a tool
More informationOverview Objectives Materials Background Activity Procedure
Overview In this activity, students will explore how to determine how to assemble information about plant distributions, and relate those distributional to the environment by assembling information on
More informationAPS 1030 Astronomy Lab 79 Kepler's Laws KEPLER'S LAWS
APS 1030 Astronomy Lab 79 Kepler's Laws KEPLER'S LAWS SYNOPSIS: Johannes Kepler formulated three laws that described how the planets orbit around the Sun. His work paved the way for Isaac Newton, who derived
More informationData Visualization with GIS, Dr. Chris Badurek Visualization and Computing Teacher s Workshop. Part 1: Getting Started with Tectonic Hot Spot Mapping
Data Visualization with GIS, Dr. Chris Badurek Visualization and Computing Teacher s Workshop Part 1: Getting Started with Tectonic Hot Spot Mapping Lesson Overview This lesson is designed to help students
More informationmodule, with the exception that the vials are larger and you only use one initial population size.
Population Dynamics and Space Availability (http://web.as.uky.edu/biology/faculty/cooper/population%20dynamics%20examples%2 0with%20fruit%20flies/TheAmericanBiologyTeacher- PopulationDynamicsWebpage.html
More information