COSMOS CosmicVelocities
|
|
|
- Mitchell Young
- 5 years ago
- Views:
Transcription
![COSMOS CosmicVelocities Lessonplan [1]](/docs-images/80/82448558/images/1-2.jpg "Galileo Navigation Satellite; Credits:")
1 COSMOS CosmicVelocities Lessonplan [1] Galileo Navigation Satellite; Credits: ESA ( www. virtuelleschule.at/inlot Guided Research Model
2 General Informations Duration: 6 x 50 min Vocabulary: Newton slawof gravity, Cavendishconstant, centripetaland centrifugal force, gravitational field, kinetic energy, gravitational potential energy Tools and Materials: Computer, internet, paper, pencils, work sheets
3 General Informations Aims and Objectives: Students should be able to understandtheprincipleof Newton slawof gravityand apply it correctly understand the relevance of the cosmic velocities differentiatebetweencircular, elliptic, parabolicand hyperbolic paths of spacecrafts calculate the cosmic velocities from Newton s law of gravity use java applets independently and understand the physics behind it
4 EducationalPhase 1 Stimulation: 1 x 25 min presentation of selected photos of satellites short trailer about launches in Cape Canaveral discussionaboutgeostationarysatellites, GPS and GALILEO
5 EducationalPhase 2 Scientific Prediction: 1 x 25 min General discussion about the launch of the rockets which velocities are necessary to move within the gravitational field of the earth (satellites) the launch of the rockets which velocities are necessary to escape the gravitational field of the earth (spacecrafts) internet-sites which deal with cosmic velocities
6 EducationalPhase 3 Experimental Activities 1 1 x 25 min Run thejavaappletby varyingthehorizontal and vertical velocities [2] Java-Applet Newtons Berg
7 EducationalPhase 3 Experimental Activities 2 1 x 25 min Simulation of Newton s lunarcalculation : fillingin a worksheet [3] Work Sheet Der Mond als geworfener Apfel?
8 EducationalPhase 3 Experimental Activities 3 1 x 50 min Calculation of the cavendish constant from an experiment [4] Graphic from Leybold Didaktik
9 EducationalPhase 4 Abstractionof the findings 1: 1 x 50 min Calculating work needed to move within the gravitationalfieldof the earth [5] From
10 EducationalPhase 4 Hypothesis: Homogeneous field [6] From
11 EducationalPhase 4 [7] From
12 EducationalPhase 4 [8] From
13 EducationalPhase 4 Abstraction of findings 2: 1 x 50 min calculationof the1st and 2nd cosmicvelocity by using the equation above constructing conic sections using GEOGEBRA (
![EducationalPhase 4 [9] From http://leifi.physik.](/docs-images/80/82448558/images/14-4.jpg "uni-muenchen.")
14 EducationalPhase 4 [9] From
15 EducationalPhase 5 Consolidation: 1 x 50 min discussion of evolving problems calculatingtheheightand velocityof a GPS satellite internetresearch: howlongwill ittakefor voyager1 to leavethe solar system internet research: find the trajectory of the spacecraft GENESIS [10] Trajectory of spacecraft GENESIS; From Sterne und Weltraum 7/2003
16 RelatedSubject: Chemistry 2 H 2 + O 2 2 H 2 O + ENERGY Regarding spacecrafts, this chemical reaction is essential in two ways: 1) launch of spacecrafts: propulsion 2) power supplyon board: fuelcell [12] From /rocket
Alien Earths Using Conic Sections to Explore the Solar System
Alien Earths Using Conic Sections to Explore the Solar System Teachers: Amena Mitha and Andy Eschbacher Target Audience: 11 th Grade Algebra II and Physics students Project Description: The Alien Earths
Distance = Rate x Time Middle grades
Distance = Rate x Time Middle grades Lesson Summary Students practice using the equation distance = rate x time using trajectory data from the Apollo 11 lunar landing mission. Prior Knowledge & Skills
60 C From Bicycle to Space. Dionysis Konstantinou Corina Toma. Space Travel
60 C From Bicycle to Space Dionysis Konstantinou Corina Toma C Space Travel From Bicycle Length to Space of the CDay61 introduction Imagine travelling from one planet to another Why is it that we have
Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016
Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016 Why are celestial motions and forces important? They explain the world around us.
GRADE 8: Earth and space 1. UNIT 8E.1 8 hours. The Solar System. Resources. About this unit. Previous learning. Expectations
GRADE 8: Earth and space 1 The Solar System UNIT 8E.1 8 hours About this unit This is the only unit on Earth and Space in Grade 8. This unit builds on work done in Grade 6 and leads into work on the wider
Status of the Gravitational Redshift Test with Eccentric Galileo Satellites
Status of the Gravitational Redshift Test with Eccentric Galileo Satellites J. Ventura-Traveset, R. Prieto-Cerdeira, D. Blonski ICG 11, Sochi, 7 November 2016 Contents 1. Galileo satellites 5 & 6 Status
spacecraft mass = kg xenon ions speed = m s 1 Fig. 2.1 Calculate the mass of one xenon ion. molar mass of xenon = 0.
1 (a) A solar-powered ion propulsion engine creates and accelerates xenon ions. The ions are ejected at a constant rate from the rear of a spacecraft, as shown in Fig. 2.1. The ions have a fixed mean speed
Chapter 6 Gravitation and Newton s Synthesis
Chapter 6 Gravitation and Newton s Synthesis If the force of gravity is being exerted on objects on Earth, what is the origin of that force? Newton s realization was that the force must come from the Earth.
Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.
Chapter 12 Gravity Units of Chapter 12 Newton s Law of Universal Gravitation Gravitational Attraction of Spherical Bodies Kepler s Laws of Orbital Motion Gravitational Potential Energy Energy Conservation
Lecture D30 - Orbit Transfers
J. Peraire 16.07 Dynamics Fall 004 Version 1.1 Lecture D30 - Orbit Transfers In this lecture, we will consider how to transfer from one orbit, or trajectory, to another. One of the assumptions that we
L eaving Earth and arriving at another planet or asteroid requires
Designing Interplanetary Transfers L eaving Earth and arriving at another planet or asteroid requires a spacecraft to implement a sequence of manoeuvres. These include changes of velocity needed to escape
TOPIC 2.1: EXPLORATION OF SPACE
TOPIC 2.1: EXPLORATION OF SPACE S4P-2-1 S4P-2-2 S4P-2-3 S4P-2-4 S4P-2-5 Identify and analyze issues pertaining to space exploration. Examples: scale of the universe, technological advancement, promotion
VISUAL PHYSICS ONLINE
VISUAL PHYSICS ONLINE EXCEL SIMULATION MOTION OF SATELLITES DOWNLOAD the MS EXCEL program PA50satellite.xlsx and view the worksheet Display as shown in the figure below. One of the most important questions
Part 4: Exploration 1
Part 4: Exploration 1 Reaction Engine An engine, such as a jet or rocket engine, that ejects gas at high velocity and develops its thrust from the resulting reaction This movement follows Newton s Third
Conceptual Physical Science 6 th Edition
1 2 1 Conceptual Physical Science 6 th Edition Chapter 4: GRAVITY, PROJECTILES, AND SATELLITES Sections 4.1, 4.5-4.9 only 3 2017 Pearson Education, Inc. This lecture will help you understand: The Universal
9.2 Worksheet #3 - Circular and Satellite Motion
9.2 Worksheet #3 - Circular and Satellite Motion 1. A car just becomes airborne as it comes off the crest of a bridge that has circular cross section of radius 78.0 m. What is the speed of the car? 2.
The 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
Newton s Laws and the Nature of Matter
Newton s Laws and the Nature of Matter The Nature of Matter Democritus (c. 470-380 BCE) posited that matter was composed of atoms Atoms: particles that can not be further subdivided 4 kinds of atoms: earth,
II. Universal Gravitation - Newton 4th Law
Periodic Motion I. Circular Motion - kinematics & centripetal acceleration - dynamics & centripetal force - centrifugal force II. Universal Gravitation - Newton s 4 th Law - force fields & orbits III.
General Physics I. Lecture 7: The Law of Gravity. Prof. WAN, Xin 万歆.
General Physics I Lecture 7: The Law of Gravity Prof. WAN, Xin 万歆 xinwan@zju.edu.cn http://zimp.zju.edu.cn/~xinwan/ Outline Newton's law of universal gravitation Motion of the planets; Kepler's laws Measuring
Chapter 13: universal gravitation
Chapter 13: universal gravitation Newton s Law of Gravitation Weight Gravitational Potential Energy The Motion of Satellites Kepler s Laws and the Motion of Planets Spherical Mass Distributions Apparent
Lord Strathcona Elementary School, Vancouver School District. Ingrid Sulston (scientist); Reid McInnes and Phyllis Daly (teachers)
Science Unit: Lesson 10: Space Rockets: Exploring the Solar System Summary: In part one of this two-part lesson, students make and launch Alka-seltzer rockets and learn about the chemical reaction causing
Newton s Second Law: Force, Velocity and Acceleration
Newton s Second Law: Force, Velocity and Acceleration Duration: - class periods About this Poster Essential Question: What are the relationships between force, mass, and? Objectives: Students will see
Design of Orbits and Spacecraft Systems Engineering. Scott Schoneman 13 November 03
Design of Orbits and Spacecraft Systems Engineering Scott Schoneman 13 November 03 Introduction Why did satellites or spacecraft in the space run in this orbit, not in that orbit? How do we design the
ESA s Juice: Mission Summary and Fact Sheet
ESA s Juice: Mission Summary and Fact Sheet JUICE - JUpiter ICy moons Explorer - is the first large-class mission in ESA's Cosmic Vision 2015-2025 programme. Planned for launch in 2022 and arrival at Jupiter
Deep Space Communication*
Deep Space Communication* Farzin Manshadi JPL Spectrum Manager September 20-21, 2012 * Based on Material provided by Dr. Les Deutsch Introduction ITU defines deep space as the volume of Space at distances
Gravity and Orbits. Objectives. Clarify a number of basic concepts. Gravity
Gravity and Orbits Objectives Clarify a number of basic concepts Speed vs. velocity Acceleration, and its relation to force Momentum and angular momentum Gravity Understand its basic workings Understand
Beyond the Book. Beyond the Book. FOCUS Book
FOCUS Book Scientists and engineers use models to plan investigations and to describe results. Create a scale model that represents part or all of Voyager 1 or Voyager 2 s journey so far. Your model can
5.12 The Aerodynamic Assist Trajectories of Vehicles Propelled by Solar Radiation Pressure References...
1 The Two-Body Problem... 1 1.1 Position of the Problem... 1 1.2 The Conic Sections and Their Geometrical Properties... 12 1.3 The Elliptic Orbits... 20 1.4 The Hyperbolic and Parabolic Trajectories...
Saint Lucie County Science Scope and Sequence
Course: Honors Physics 1 Course Code: 2003390 UNIT 4 TOPIC of STUDY: Newton s Laws of Motion and the Law of Gravity STANDARDS: 10: Energy, 12: Motion ~Net force produces motion ~There are four fundamental
Astrodynamics (AERO0024)
Astrodynamics (AERO0024) 10. Interplanetary Trajectories Gaëtan Kerschen Space Structures & Systems Lab (S3L) Motivation 2 6. Interplanetary Trajectories 6.1 Patched conic method 6.2 Lambert s problem
PHYSICS 12 NAME: Gravitation
NAME: Gravitation 1. The gravitational force of attraction between the Sun and an asteroid travelling in an orbit of radius 4.14x10 11 m is 4.62 x 10 17 N. What is the mass of the asteroid? 2. A certain
ASEN 5050 SPACEFLIGHT DYNAMICS Interplanetary
ASEN 5050 SPACEFLIGHT DYNAMICS Interplanetary Prof. Jeffrey S. Parker University of Colorado Boulder Lecture 29: Interplanetary 1 HW 8 is out Due Wednesday, Nov 12. J2 effect Using VOPs Announcements Reading:
Physics I. Unit 1 Methods in Science (Systems of Units) Competencies (Do) Students should be able to demonstrate scientific methods.
Physics I Unit 1 Methods in Science (Systems of Units) Estimated Time Frame Big Ideas for Units 10 Days Tools are needed for the study of Physics, such as measurement, conversions, significant figures,
GRADE 6: Physical processes 3. UNIT 6P.3 6 hours. The effects of forces. Resources. About this unit. Previous learning.
GRADE 6: Physical processes 3 The effects of forces UNIT 6P.3 6 hours About this unit This unit is the third of three units on physical processes for Grade 3 and the second of two on forces. It builds
Circular Motion PreTest
Circular Motion PreTest Date: 06/03/2008 Version #: 0 Name: 1. In a series of test runs, a car travels around the same circular track at different velocities. Which graph best shows the relationship between
AP Physics Multiple Choice Practice Gravitation
AP Physics Multiple Choice Practice Gravitation 1. Each of five satellites makes a circular orbit about an object that is much more massive than any of the satellites. The mass and orbital radius of each
LAUNCHES AND LAUNCH VEHICLES. Dr. Marwah Ahmed
LAUNCHES AND LAUNCH VEHICLES Dr. Marwah Ahmed Outlines 2 Video (5:06 min) : https://youtu.be/8t2eyedy7p4 Introduction Expendable Launch Vehicles (ELVs) Placing Satellite into GEO Orbit Introduction 3 Introduction
Physics Mechanics. Lecture 29 Gravitation
1 Physics 170 - Mechanics Lecture 29 Gravitation Newton, following an idea suggested by Robert Hooke, hypothesized that the force of gravity acting on the planets is inversely proportional to their distances
Why Don t We See Stars in the Daytime?
Why Don t We See Stars in the Daytime? Photo Credit: ESA Hubble NASA At night, we see many stars in the sky. Those stars are made of burning gases. They are hot, and they shine. But stars are in the sky
Dynamics and Space O O O O O O O O O O O O O O O O O O O O O. Evaluation of Progress VECTORS, SCALARS AND DISPLACEMENT
Dynamics and Space VECTORS, SCALARS AND DISPLACEMENT http://www.bbc.co.uk/education/guides/zvt4jxs/revision/1 I can describe a scalar quantity as a quantity that requires magnitude only. I can give examples
End-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.
HW Chapter 5 Q 7,8,18,21 P 4,6,8. Chapter 5. The Law of Universal Gravitation Gravity
HW Chapter 5 Q 7,8,18,21 P 4,6,8 Chapter 5 The Law of Universal Gravitation Gravity Newton s Law of Universal Gravitation Every particle in the Universe attracts every other particle with a force that
/////// ///////////// Module ONE /////////////// ///////// Space
// // / / / / //// / ////// / /// / / // ///// ////// ////// Module ONE Space 1 Gravity Knowledge and understanding When you have finished this chapter, you should be able to: define weight as the force
South Slave Divisional Education Council. Physics 20. Curriculum Package February 2012
South Slave Divisional Education Council Physics 20 Curriculum Package February 2012 2012 Unit A: Kinematics Focusing Questions: How do changes in position, velocity and acceleration allow us to predict
AP PHYSICS C SYLLABUS. Paul A. Tipler and Gene P. Mosca. Physics for Scientists and Engineers, 6 th. Course Description
AP PHYSICS C SYLLABUS. Text Paul A. Tipler and Gene P. Mosca. Physics for Scientists and Engineers, 6 th edition Extended Veraion Course Description AP Physics C is equivalent to a first year college physics
Chapter Review USING KEY TERMS UNDERSTANDING KEY IDEAS. Skills Worksheet. Multiple Choice
Skills Worksheet Chapter Review USING KEY TERMS Complete each of the following sentences by choosing the correct term from the word bank. mass gravity friction weight speed velocity net force newton 1.
MAE 180A: Spacecraft Guidance I, Summer 2009 Homework 4 Due Thursday, July 30.
MAE 180A: Spacecraft Guidance I, Summer 2009 Homework 4 Due Thursday, July 30. Guidelines: Please turn in a neat and clean homework that gives all the formulae that you have used as well as details that
Year 12 Physics. 9.2 Space
Year 12 Physics 9.2 Space Contextual Outline Scientists have drawn on advances in areas such as aeronautics, material science, robotics, electronics, medicine and energy production to develop viable spacecraft.
A study of trajectories to the Neptune system using gravity assists
Advances in Space Research 40 (2007) 125 133 www.elsevier.com/locate/asr A study of trajectories to the Neptune system using gravity assists C.R.H. Solórzano a, A.A. Sukhanov b, A.F.B.A. Prado a, * a National
Name. 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
Chapter 6 More complicated orbits and spacecraft trajectories
There s three major functions under navigation Trajectory design, which is designing the trajectory that ll get you to your destination, or meet those science requirements. For Juno, we needed to get to
A mass is suspended by a string from a fixed point. The mass moves with constant speed along a circular path in a [1 mark] horizontal plane.
![A mass is suspended by a string from a fixed point. The mass moves with constant speed along a circular path in a [1 mark] horizontal plane.](/thumbs/78/77486004.jpg "A mass is suspended by a string from a fixed point. The mass moves with constant speed along a circular path in a [1 mark] horizontal plane.")
T6 [200 marks] 1. A mass is suspended by a string from a fixed point. The mass moves with constant speed along a circular path in a horizontal plane. The resultant force acting on the mass is A. zero.
Newton s Legacy. 1- accelerate to break free of Earth. Rocket Science: How to send a spacecraft to Mars
Reading: today: web-based reading on satellite orbits; Chap. 3 Sec. 5 Chap. 7, Sect. 1, 2 (for next week) Exam 1: Tuesday, September 26, 6:45-8:00. Room assignments on course website ESSAY QUESTION Homework
arxiv: v1 [gr-qc] 7 Oct 2009
![arxiv: v1 [gr-qc] 7 Oct 2009](/thumbs/81/83216793.jpg "arxiv: v1 [gr-qc] 7 Oct 2009")
Earth Flyby Anomalies Michael Martin Nieto 1 and John D. Anderson 2 Michael Martin Nieto is a fellow at Los Alamos National Laboratory and John D. Anderson is a senior research scientist emeritus at the
LOTNAV. A Low-Thrust Interplanetary Navigation Tool: The Trajectory Reconstruction Module
LOTNAV A Low-Thrust Interplanetary Navigation Tool: The Trajectory Reconstruction Module Juan Luis Cano González Mission Analysis Division Deimos Space S.L. -1- The LOTNAV Tool The Low-Thrust Interplanetary
Applied Mathematics B Study Guide
Science, Engineering and Technology Portfolio School of Life and Physical Sciences Foundation Studies (Applied Science/Engineering) Applied Mathematics B Study Guide Topics Kinematics Dynamics Work, Energy
LEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona
LEARNING ABOUT THE OUTER PLANETS Can see basic features through Earth-based telescopes. Hubble Space Telescope especially useful because of sharp imaging. Distances from Kepler s 3 rd law, diameters from
Understanding Motion, Energy & Gravity
Speed, Velocity & Acceleration Understanding Motion, Energy & Gravity Chapter 4 speed: distance traveled per unit time (e.g., m/s, mph, km/ hr) velocity: speed & direction acceleration: change in velocity
PSI AP Physics C Universal Gravity Multiple Choice Questions
PSI AP Physics C Universal Gravity Multiple Choice Questions 1. Who determined the value of the gravitational constant (G)? (A) Newton (B) Galileo (C) Einstein (D) Schrödinger (E) Cavendish 2. Who came
Delta RV Physical Science Revised Integrated Skills. Skill/Concept
Delta RV Physical Science Revised-2009 Content Standard: Properties and Principles of Matter and Energy GLE: Changes in properties and states of matter provide evidence of the atomic theory of matter A
The Pioneer Anomaly: Effect, New Data and New Investigation
The Pioneer Anomaly: Effect, New Data and New Investigation Slava G. Turyshev Jet Propulsion Laboratory, California Institute of Technology Seminar at the Sternberg Astronomical Institute Moscow State
Understanding Motion, Energy & Gravity
Speed, Velocity & Acceleration Understanding Motion, Energy & Gravity Chapter 4 speed: distance traveled per unit time (e.g., m/s, mph, km/ hr) velocity: speed & direction acceleration: change in velocity
Sunlight in the Night
Sunlight in the Night Photo Credit: Yarl You cannot see the sun in the nighttime. But did you know that you can see the sun s light at night? Here s how it works. When it is dark, you see the moon shining
Introduction to Astronomy
Introduction to Astronomy AST0111-3 (Astronomía) Semester 2014B Prof. Thomas H. Puzia Newton s Laws Big Ball Fail Universal Law of Gravitation Every mass attracts every other mass through a force called
Chapter 10. Projectile and Satellite Motion
Chapter 10 Projectile and Satellite Motion Which of these expresses a vector quantity? a. 10 kg b. 10 kg to the north c. 10 m/s d. 10 m/s to the north Which of these expresses a vector quantity? a. 10
7 Study Guide. Gravitation Vocabulary Review
Date Period Name CHAPTER 7 Study Guide Gravitation Vocabulary Review Write the term that correctly completes the statement. Use each term once. Kepler s second law Newton s law of universal gravitation
A SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE
DOING PHYSICS WITH MATLAB A SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE Download Directory: Matlab mscripts mec_satellite_gui.m The [2D] motion of a satellite around the Earth is computed from
A Very Brief History of Statics and Dynamics
UNIVERSAL GRAVITION A Very Brief History of Statics and Dynamics The idea that a force causes motion goes back to the 4 th century B.C., when the Greeks were developing ideas about science. Aristotle (384-33
Learning Lab Seeing the World through Satellites Eyes
Learning Lab Seeing the World through Satellites Eyes ESSENTIAL QUESTION What is a satellite? Lesson Overview: Engage students will share their prior knowledge about satellites and explore what satellites
By Positively Autism. Science-Themed Reading Comprehension Passage and Activities For Students with Autism
Science-Themed Reading Comprehension Passage and Activities For Students with Autism By Positively Autism Making Learning Fun and Meaningful for Children with Autism This sample is part of a larger set
CHAPTER 7 GRAVITATION
Physics Approximate Timeline Students are expected to keep up with class work when absent. CHAPTER 7 GRAVITATION Day Plans for the day Assignments for the day 1 7.1 Planetary Motion & Gravitation Assignment
Web sites and Worksheets
Introduction Web sites and Worksheets Sandra Woodward Oakhill College Castle Hill (swoodward@oakhill.nsw.edu.au) Astronomy is a practical subject by nature. Unfortunately for teachers, many of the practical
Chapter 14 Satellite Motion
1 Academic Physics Mechanics Chapter 14 Satellite Motion The Mechanical Universe Kepler's Three Laws (Episode 21) The Kepler Problem (Episode 22) Energy and Eccentricity (Episode 23) Navigating in Space
1. Which of the following correctly lists our cosmic address from small to large?
1. Which of the following correctly lists our cosmic address from small to large? (a) Earth, solar system, Milky Way Galaxy, Local Group, Local Super Cluster, universe (b) Earth, solar system, Milky Way
This module is designed to help you explore how projectiles and space affect your life each day.
Shoot! This module is designed to help you explore how projectiles and space affect your life each day. 1. Choose A or B or C and complete ALL the requirements. A. Watch about three hours total of science-related
Earth, Earth s Moon, Mars Balloons Grades: Middle School Grade Prep Time: ~10 Minutes Lesson Time: 60 Mins
Earth, Earth s Moon, Mars Balloons Grades: Middle School Grade Prep Time: ~10 Minutes Lesson Time: 60 Mins WHAT STUDENTS DO: Construct a Planetary Model Curiosity about our place in space and whether we
Launch! This module is designed to help you explore how science affects your life each day.
Launch! This module is designed to help you explore how science affects your life each day. 1. Choose A or B or C and complete ALL the requirements. A. Watch about three hours total of science-related
Gravitation. Makes the World Go Round
Gravitation Makes the World Go Round Gravitational Force The Force of gravity is an attractive force felt between all objects that have mass. G=6.67x10-11 N m 2 /kg 2 Example 1: What is the Force of Gravity
Modeling the Orbits of the Outer Planets
Name Modeling the Orbits of the Outer Planets (a NASA New Horizons activity) Materials Paper clip Scissors Glue Pencil and crayons or markers Planet sheets Safety Concerns: Scissors. Discuss safe and proper
The escape speed for an object leaving the surface of any celestial body of mass M and radius d is
8-3 Escape Speed Vocabulary Escape Speed: The minimum speed an object must possess in order to escape from the gravitational pull of a body. In Chapter 6, you worked with gravitational potential energy
Preface. 2 Cable space accelerator 39
Contents Abstract Preface xiii xv 1 Space elevator, transport system for space elevator, 1 and tether system 1.1 Brief history 1 1.2 Short description 2 1.3 Transport system for the space elevator 5 1.4
BravoSat: Optimizing the Delta-V Capability of a CubeSat Mission. with Novel Plasma Propulsion Technology ISSC 2013
BravoSat: Optimizing the Delta-V Capability of a CubeSat Mission with Novel Plasma Propulsion Technology Sara Spangelo, NASA JPL, Caltech Benjamin Longmier, University of Michigan Interplanetary Small
Copyright 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.
Chapter 13. Newton s Theory of Gravity The beautiful rings of Saturn consist of countless centimeter-sized ice crystals, all orbiting the planet under the influence of gravity. Chapter Goal: To use Newton
Celestial Mechanics Lecture 10
Celestial Mechanics Lecture 10 ˆ This is the first of two topics which I have added to the curriculum for this term. ˆ We have a surprizing amount of firepower at our disposal to analyze some basic problems
PROBLEM SCORE Problem 1 (30 Pts) Problem 2 (30 Pts) Choose Problem #2 or #3! Problem 4 (40 Pts) TOTAL (100 Pts)
AAE 439 Exam #1 October 20, 2008 4:30 pm 6:00 pm ARMS B71 or ARMS 1109 NAME: SOLUTIONS Read all problems carefully before attempting to solve them. Your work must be legible, and the organization must
CIRCULAR MOTION AND UNIVERSAL GRAVITATION
CIRCULAR MOTION AND UNIVERSAL GRAVITATION Uniform Circular Motion What holds an object in a circular path? A force. String Friction Gravity What happens when the force is diminished? Object flies off in
Gat ew ay T o S pace AS EN / AS TR Class # 19. Colorado S pace Grant Consortium
Gat ew ay T o S pace AS EN / AS TR 2500 Class # 19 Colorado S pace Grant Consortium Announcements: - Launch Readiness Review Cards - 11 days to launch Announcements: - Launch Readiness Review Cards - 11
FORCE. The 4 Fundamental Forces of Nature
FORCE - Force a push or pull. Results only from interaction with another object. Without interaction, forces cannot be present. - Measured in Newtons (N) 1 Newton is the amount of force required to give
Lab #8 NEUTRAL ATMOSPHERE AND SATELLITE DRAG LAB
Lab #8 NEUTRAL ATMOSPHERE AND SATELLITE DRAG LAB Introduction Goals: In this lab we explore effects of atmospheric drag on motion of satellites that are in low enough orbits to be affected by the Earth
Outline for Today: Newton s Law of Universal Gravitation The Gravitational Field Orbital Motion Gravitational Potential Energy. Hello!
PHY131H1F - Class 13 Outline for Today: Newton s Law of Universal Gravitation The Gravitational Field Orbital Motion Gravitational Potential Energy Under the Flower of Kent apple tree in the Woolsthorpe
Physics 12. Unit 5 Circular Motion and Gravitation Part 2
Physics 12 Unit 5 Circular Motion and Gravitation Part 2 1. Newton s law of gravitation We have seen in Physics 11 that the force acting on an object due to gravity is given by a well known formula: F
4.8 Space Research and Exploration. Getting Into Space
4.8 Space Research and Exploration Getting Into Space Astronauts are pioneers venturing into uncharted territory. The vehicles used to get them into space are complex and use powerful rockets. Space vehicles
Traveling Into Space. Use Target Reading Skills. How Do Rockets Work? Building Vocabulary
Traveling Into Space This section explains how rockets work. It also describes the history of space exploration and explains how space shuttles, space stations, and space probes are used in exploring space
Gravitational Fields
Gravitational Fields Examples 00 Currently, the space probe, Cassini, is between Jupiter and Saturn. Cassini s mission is to deliver a probe to one of Saturn s moons, Titan, and then orbit Saturn collecting
THE MECHANICAL UNIVERSE
THE MECHANICAL UNIVERSE MECHANICS AND HEAT, ADVANCED EDITION STEVEN С FRAUTSCHI PROFESSOR OF THEORETICAL PHYSICS CALIFORNIA INSTITUTE OF TECHNOLOGY RICHARD P. OLENICK ASSISTANT PROFESSOR OF PHYSICS, UNIVERSITY
Directed Reading B. Section: The Outer Planets
Skills Worksheet Directed Reading B Section: The Outer Planets 1. What is one way that gas giants differ from the terrestrial planets? a. They are much smaller. b. They are rocky and icy. c. They are made
AP Physics C: Mechanics: Syllabus 2
AP Physics C: Mechanics: Syllabus 2 Scoring Components SC1 The course covers instruction in kinematics. 3 SC2 The course covers instruction in Newton s laws of 4 motion. SC3 The course covers instruction
Chapter 13 Gravity Pearson Education, Inc. Slide 13-1
Chapter 13 Gravity Slide 13-1 The plan Lab this week: there will be time for exam problems Final exam: sections posted today; some left out Final format: all multiple choice, almost all short problems,
Interstellar Exploration Through Repeated External Acceleration
Interstellar Exploration Through Repeated External Acceleration Andrew Bingham NIAC Student Fellows Prize Department of Mechanical and Aeronautical Engineering, Clarkson University NIAC Fellows Meeting,