Motions for systems and structures in space, described by a set denoted Avd. Theorems for local implosion; Li, dl and angular velocities

Size: px
Start display at page:

Download "Motions for systems and structures in space, described by a set denoted Avd. Theorems for local implosion; Li, dl and angular velocities"

Transcription

1 Journal of Physics and Astronomy Research Vol. 2(3), pp , September, ISSN: XXXX-XXXX JPAR Research Article Motions for systems and structures in space, described by a set denoted Avd. Theorems for local implosion; Li, dl and angular velocities Lena J-T Strömberg previously Department of Solid Mechanics, Royal Institute of Technology, KTH, Sweden lena_str@hotmail.com In order to describe general motions and matter in space, functions for angular velocity and density are assumed and denoted Avd, as an abbreviation. The framework provides a unified approach to motions at different scales. It is analysed how Avd enters and rules, in terms of results from equations, in field experiments and observations at Earth. Chaos may organize according to Avd, such that more order, Cosmos, appear in complex nonlinear dynamical systems. This reveals that Avd may be governing and that deterministic systems can be created without assuming boundaries and conditions for initial values and forces from outside. A mathematical model for the initiation of Logos (when a paper accelerates into a narrow circular orbit), was described, and denoted local implosion; Li. The theorem for dl, provides discrete solutions to a power law, and this is related to locations of satellites and moons. Key words: Angular velocity, density, Avd, Logos, Local implosion, Discrete locations, Theorems, Deterministic Chaos, Cosmos, unification of kinematics, Lena s lemma for Riemenn -function INTRODUCTION With the purpose of finding origin of motions, and a proper description without introducing pressure and forces, a small model will be proposed, and denoted Avd, as an abbreviation for angular velocity and density. This is based on functions derived for a non-circular planetary orbit, Strömberg (2014, 2015). Several applications are covered in Strömberg (2014, 2015), e.g. planetary motions, locations, distributed matter, frequencies in acoustics and occurrence of a factor 3/2, also known from Correia and Laskar (2004) as the ratio of sidereal and orbital rotation of Mercury. If assumed valid at different scales, the model is a unification of kinematics, which concerns the geometry of motion in space. Experiments with natural complex motions, not steady, monotonic and linear, but where Avd enter, will be presented and analysed. Theorems for angular velocities are proposed. To model the paper experiment, with aggregation occurring with a large, denoted as a local implosion, a differential equation is derived. Assuming an iterative solution with transients, a capture into steady states, corresponding to e.g. planetary orbits, is obtained. Within the framework, discrete and quantised solutions are obtained without assuming a differential equation. Model for the origin of motions: Avd Definition. To describe presence of Cosmos, for dynamical systems in space, a set of functions is defined. This will be known as Avd. Avd consists of the functions i) (t)= 0 exp(-2(r ecc/r 0)sin(f 0t)) where 0 is constant

2 Strömberg L 070 Figure1. Left. Front view of the paper at small oscillations. Right. After entering Li, with a rapid rotational velocity ii) (t)= 0 exp (2(r ecc/r 0)sin(f 0t)) where 0 is constant where i) is derived in Strömberg (2015), and ii) is the Ledensity introduced in Strömberg (2014), such that the continuity of mass, is fulfilled, (i.e. point wise no expansion or compaction of mass matter.) Conclusions of physics, for motions, by analysis of Avd Conjecture A-Ph (Avd to Physics) Elements/Functions in Avd may couple with motion of a material body in space Functional relations for the elements may provide information on physical laws for motion, and other properties, e.g. invariants and magnitudes, The coupling requires energy, which is supplied by initial motion of the body in space, and then another motion or process may begin The functions in Avd are derived for an orbiting planet with eccentricity. At Earth, this could be present as a tide, or a memory of a past non-circular orbit. To be applicable at a smaller scale, angular velocities are assumed to be scaled, or that an Avd is created by a motion in the system, interacting with the surroundings. Next the results from experiments for a motion will be presented and analysed. Avd appearing in a free falling paper (A5, thin) To obtain knowledge of pure motion, a field experiment of a natural composed motion not pre-arranged and as little as possible pertubated, will be analysed in terms of Avd. It can be described and ruled by an angular velocity, within short time intervals. 1.First, the paper moves with small horizontal oscillations c.f. Fig. 1 left, given by the functions 2.Then it achieves a large angular acceleration. With this it accelerates into a circular path, where the shape gets much more curved, Fig. 1 right. The space-time when curved will be known as initially, Logos, and then Local implosion, Li. After one lap, the 'internal energy', in the circular shape is released, and the paper achieves its original shape. In the flat shape it moves in a fast translation, in a different direction. (This may be related to diffusion and isotropic behaviour in space). At this state, it is also possible that it obtains degrees of freedom, d.o.f. that we cannot observe with the eye, (such that presence in other dimension), coupling with the surrounding, e.g. Newtonian gravity, and the oscillation at phase 1, or an own rotational frame created at Logos, however probably not, since only one lap. Performing the experiment, you may note that when too close, the paper approaches towards thee, (in compaction, contraction, by attraction) and then bumps outward again. Sometimes it twists, in oscillations or a twisting lap instead of a Li, and sometimes it moves in an opposite horizontal direction before the fast lap. Detailed description of Logos and Li. Before Logos, as increases, the curvature increases, and at entire revolution, it forms a small circle. This could be due to either, or all, of the following hypothesis It copies the motion at larger scale for Earth rotation An own gravitational field is created It obeys a Bernoulli s law, such that a large pressure drop balances the increased velocity, and an isotropic compressive state is prevailed. A mathematical model for the initiation of Li will be formulated Theorem Local implosion: Initiation of the phase 2, for a falling paper, can be modelled with the function in Avd, since these admits high angular acceleration. Proof. A differentiation of (i), gives the angular acceleration d /dt= f 0 0 exp(-2(recc/r0)sin(f 0t)) )(-2(recc/r0)cos(f 0t)) A linearisation for small f 0t close to f 0t = gives the differential equation d /dt= 0f 02(re/r0), which can be integrated exactly, to read = 0exp(2(re/r0) f 0t). This means that can increase rapidly, as is the case when entering Li. Another description which gives an increased is this format is obtained by assuming that r0, i.e. the radius of curvature approaches zero.

3 J. Phys. Astron. Res. 071 Algebra and Functions on Avd I. Non-dimensional format II. Logarithmic ln of the non-dimensional format, gives a harmonic III. Power expressions. Solutions to nonlinear differential equations, and may be the source of forced vibrations. Result for Earth equator power law Relations for power expressions, in the format p = C q will be known as power laws. With the conditions at Earth, it will be shown that a power law is valid for discrete times, or if a spatial description with t=, discrete angles,. The relation 2 = G4 /3(1) Is derived from balance of centripetal acceleration and Newtonian law of gravity, and rules both discrete masses (i.e. satellites), and arbitrary mass elements parts of Earth equator considered as a continuum. The result is experimentally valid without introducing the force, by measurement of density and angular velocity. Theorem for discrete (quantised) locations, dl. Theorem dl. With and from Avd, (1) implies discrete solutions for the locations. Proof. Identification of the time dependent parts in (1). The results provide a link between a continuum description, and the motions of discrete masses e.g. moons around a planet. If (1) was assumed for Gas Giants at formation, the number of satellites may be compared with the close moons for Jupiter (8), and moons of Saturnus (24). With angular velocity, the angles may be expressed with discrete times. Assuming extension in radial direction provides the orbits and quantisation. To summarize, this will be denoted the Lena-theorem for dl. Lena-theorem for Updated angular velocities, Uav. As an opposite of fast acceleration derived above, we shall consider an iterative format, which stabilize w into a constant proportional to. In conjunction with original format, will also be calculated from previous values, updated with transients. The ratio, will depend on the parameters in the functions of Avd, and the Riemann sum for the Riemann -function. Preliminaries. Consider a subdivision of the logarithmic format ln( ), into ln( n+1 ), where n= n-1exp(- 1/g(n) 2 ), n are integers or rationals and g(n) is a function of n. Theorem Uav: Assume from Avd, the harmonic for ln ( n+1 )=-2(r ecc/r 0)sin(f 0t). The iterative format n = n- 1exp (-1/n 2 ), where n are e.g. integers 1,2,3, or half integers 3/2, 5/2, 7/2,gives a stable constant solution, such that n = n-1, for large n. The exact value (for half integers)is given by n = 0 exp(-2(r ecc/r 0)sin(f 0t)- (2)), where is the Riemann -function for half integers. Lena s Lemma: relates to the complex Riemann - function (z)=(1 exp(-zln(2)) -1 ( (z)+1), where z = a+ib and (z)= (1/n z ) Proof of Lemma: Evaluation and identification of terms in the sum. Proof. Insertion and evaluation of ln of products into sums of ln, and identification with the Riemann sum. Remarks.With n being half integers, values more close to the ratios for gas giants and the planets are obtained, also for smaller eccentricities. With the complex Riemann z-function, a harmonic oscillation is obtained, depending on a dimensionless parameter b, and with almost constant frequency for small b. Such couplings may have been used in earlier calculations and when formulating inventing the Riemann hypothesis. Cosmos Subsequently also the word figure will be used for the coupling, to manifest that it is something visible which embodies in a structure. ConjectureA- (Avd-to-cosmos) Functions of Avd may appear in other dynamical systems, e.g. as Cosmos i) to create order when chaos ii) to minimize d.o.f. iii) to obtain a constant energy, or a steady motion Such cosmos can be included equations and modelling, as 2 nd and higher order effects, or as an additional overall principle or constraint. Examples. Two clocks at the same wall achieve a synchronised period. Women living together can achieve the same evaluation-period, however this could be more related to the orientation to the heart as a vertical dumb bell, and the tide.

4 Strömberg L 072 Figure 2. The motion of the (metallic) flakes is partly rotational, and downward direction due to gravity from outside, is not so noticeable. Additional examples of systems in such motions Avd figures in dynamical systems, e.g. a free falling paper. Other examples may be Motions of flakes, in a liquid bulb chamber. When turned upside down, the downward motion due to gravity, is accomplished with (visually almost dominated by) much rotation. When bulb is subjected to motion back and forth around the vertical axis, very much rotation is transferred to the flakes, such that they rotate rapidly, in small arcs, c.f. Figure 2. Smoke rings in a gravity field, rising since lighter than air, and form a spiral, consistent with Avd. A whirlwind, created over hot sea. Logos occurs in flows on curved surfaces, e.g. the eye globe. More detailed and extensive models of fluid structure interaction with whirls are treated in e.g. Walther and Koumoutsakos (2001) and van Rees et al. (2013). CONCLUSION In order to describe general motions and matter in space, two functions from Strömberg, 2014, 2015), called Avd were introduced. These were compared with field experiments for multi-d.o.f. motions, and composed systems. It was discussed how these may enter and rule and whether this can be a valid model for many systems in complex interaction with the surrounding. If so, chaos may organize according to Avd, and nonlinear deterministic systems can be described without an a priori assumption of forces and pressure through boundary conditions. Since applicable at different scales, Avd provides a unification, not of forces, but of kinematics. The same path, but more slow is found for a falling leaf or feather sailing in the air, e.g. in the film Forrest Gump. A mathematical model for Logos, when the paper starts accelerates into a narrow circular orbit, denoted Local implosion, Li, was described. This is characterized by a large curvature of the paper. If the kinetic energy is bounded, then the velocity is also bounded, such that a large angular velocity multiplied with a small radius of the orbit, is limited and may be initialized with a finite kinetic energy from previous motion. The word Logos is from Aristotle (4 th century BC). For shape memory alloys Auricchio et al (2008), hard inclusions of martensite are modelled, with small spheres that may unwarp during steady state loading. In this context, it can be mentioned that in classical construction steel, the martensite gives a harder but more brittle behavior. In some applications ductile steels may be preferred, since they can withstand small cracks, and other loads e.g. weld residuals and environment. A theorem for dl, provided discrete solutions to a power law, and this was related to locations of satellites and moons. From an iterative format, stable constant values of angular velocities were obtained from a summary of rationals, derived from results for Riemann -function.

5 J. Phys. Astron. Res. 073 ACKNOWLEDGEMENTS To Tech Power Oslo, Stiftelsen Jernkontoret and Dr Rebbah. The author acknowledged the contributions of Prof. Marcos Voelzke, Željko Prebeg, Dr. Cyd Ropp and J. Ponce de Leon for donating their time, critical evaluation, constructive comments, and invaluable assistance toward the improvement of this very manuscript. REFERENCES Aristotle 4th century B. Rhetoric, Greek treatise on the art of persuasion. Auricchio F, Mielke A, and Stefanelli U (2008).A rateindependent model for the isothermal quasi-static evolution of shape-memory materials, Math. Models Methods Appl. Sci. 18, 125. Correia A, Laskar J (2004).Mercury's capture into the 3/2 spin-orbit resonance as a result of its chaotic dynamics. Nature 429, Strömberg L (2014). A model for non-circular orbits derived from a two-step linearisation of the Kepler laws. Journal of Physics and Astronomy Research 1(2): Strömberg L (2015). Models for locations in the solar system. Journal of Physics and Astronomy Research 1(2): Strömberg L (2014).Generalized potentials describing orbits in the solar system. Derivation of a close force acting on the inner moon Phobos. Journal of Aerospace Science and Technology 1: van Rees W.M., Gazzola M., Koumoutsakos P (2013).Optimal shapes for anguilliform swimmers at intermediate Reynolds numbers. Journal of Fluid Mechanics, 722. Walther J.H., Koumoutsakos P (2001).Three-dimensional vortex methods for particle-laden flows with two-way coupling, J. Comput. Physics 167: Accepted 15 August, 2015 Citation: Strömberg L (2015). Motions for systems and structures in space, described by a set denoted Avd.Theorems for local implosion; Li, dl and angular velocities. Journal of Physics and Astronomy Research, 2(3): Copyright: 2015 Strömberg L. This is an open-access article distributed under the terms of the creative commons attribution license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are cited.

previously Department of Solid Mechanics, Royal Institute of Technology, KTH, Sweden

previously Department of Solid Mechanics, Royal Institute of Technology, KTH, Sweden Hypergravity derived from the Le-density and applied to a model for explosion. Analysis of universal constants of gravity and light in conjunction with the J-space. Lena J-T Strömberg previously Department

More information

previously Department of Solid Mechanics, Royal Institute of Technology, KTH, Sweden

previously Department of Solid Mechanics, Royal Institute of Technology, KTH, Sweden Observations for lateral light at a hole adjacent to lines of different colours. Comparison with the eye in terms of iris and blue make up. Analysis of monochromatic light. Lena J-T Strömberg previously

More information

Models for locations and motions in the solar system

Models for locations and motions in the solar system Journal of Physics and Astronomy Research Vol. 2(1), pp. 054-058, March, 2015. www.premierpublishers.org, ISSN: 2123-503x JPAR Review Models for locations and motions in the solar system Lena Strömberg

More information

D DAVID PUBLISHING. Generalised Potentials describing orbits in the Solar System. Derivation of a Close-force acting on the inner moon Phobos.

D DAVID PUBLISHING. Generalised Potentials describing orbits in the Solar System. Derivation of a Close-force acting on the inner moon Phobos. Journal of Aerospace Science and Technology 1 (2014) 11-20 Generalised Potentials describing orbits in the Solar System. Derivation of a Close-force acting on the inner moon Phobos. Lena Strömberg Previously

More information

Chapter 13: universal gravitation

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

More information

Circular Motion and Gravity Lecture 5

Circular Motion and Gravity Lecture 5 Circular Motion and Gravity Lecture 5 ˆ Today we talk about circular motion. There are two reasons to do this... ˆ Last week we talked about Newton s laws in problems dealing with straight-line motion.

More information

2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity

2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion: Examples from Daily Life Some of the topics we will explore: How do we describe motion? (Speed,

More information

4.3 Conservation Laws in Astronomy

4.3 Conservation Laws in Astronomy 4.3 Conservation Laws in Astronomy Our goals for learning: Why do objects move at constant velocity if no force acts on them? What keeps a planet rotating and orbiting the Sun? Where do objects get their

More information

Physics for Scientists and Engineers 4th Edition, 2017

Physics for Scientists and Engineers 4th Edition, 2017 A Correlation of Physics for Scientists and Engineers 4th Edition, 2017 To the AP Physics C: Mechanics Course Descriptions AP is a trademark registered and/or owned by the College Board, which was not

More information

Physics. Chapter 9 Gravity

Physics. Chapter 9 Gravity Physics Chapter 9 Gravity The Newtonian Synthesis Gravity is a Universal Force The Newtonian Synthesis According to legend, Newton discovered gravity while sitting under an apple tree. The Falling Moon

More information

Basic Physics. Isaac Newton ( ) Topics. Newton s Laws of Motion (2) Newton s Laws of Motion (1) PHYS 1411 Introduction to Astronomy

Basic Physics. Isaac Newton ( ) Topics. Newton s Laws of Motion (2) Newton s Laws of Motion (1) PHYS 1411 Introduction to Astronomy PHYS 1411 Introduction to Astronomy Basic Physics Chapter 5 Topics Newton s Laws Mass and Weight Work, Energy and Conservation of Energy Rotation, Angular velocity and acceleration Centripetal Force Angular

More information

Lecture 13. Gravity in the Solar System

Lecture 13. Gravity in the Solar System Lecture 13 Gravity in the Solar System Guiding Questions 1. How was the heliocentric model established? What are monumental steps in the history of the heliocentric model? 2. How do Kepler s three laws

More information

Chapter 5 Review : Circular Motion; Gravitation

Chapter 5 Review : Circular Motion; Gravitation Chapter 5 Review : Circular Motion; Gravitation Conceptual Questions 1) Is it possible for an object moving with a constant speed to accelerate? Explain. A) No, if the speed is constant then the acceleration

More information

Quantitative Skills in AP Physics 1

Quantitative Skills in AP Physics 1 This chapter focuses on some of the quantitative skills that are important in your AP Physics 1 course. These are not all of the skills that you will learn, practice, and apply during the year, but these

More information

Chapter 5 Circular Motion; Gravitation

Chapter 5 Circular Motion; Gravitation Chapter 5 Circular Motion; Gravitation Units of Chapter 5 Kinematics of Uniform Circular Motion Dynamics of Uniform Circular Motion Highway Curves, Banked and Unbanked Newton s Law of Universal Gravitation

More information

1. Solar System Overview

1. Solar System Overview Astronomy 241: Foundations of Astrophysics I 1. Solar System Overview 0. Units and Precision 1. Constituents of the Solar System 2. Motions: Rotation and Revolution 3. Formation Scenario Units Text uses

More information

Dynamical properties of the Solar System. Second Kepler s Law. Dynamics of planetary orbits. ν: true anomaly

Dynamical properties of the Solar System. Second Kepler s Law. Dynamics of planetary orbits. ν: true anomaly First Kepler s Law The secondary body moves in an elliptical orbit, with the primary body at the focus Valid for bound orbits with E < 0 The conservation of the total energy E yields a constant semi-major

More information

Newton s Laws and the Nature of Matter

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,

More information

Physics Test 7: Circular Motion page 1

Physics Test 7: Circular Motion page 1 Name Physics Test 7: Circular Motion page 1 hmultiple Choice Read each question and choose the best answer by putting the corresponding letter in the blank to the left. 1. The SI unit of angular speed

More information

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields Gravity Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields Simulation Synchronous Rotation https://www.youtube.com/watch?v=ozib_l eg75q Sun-Earth-Moon System https://vimeo.com/16015937

More information

B.Sc. (Semester - 5) Subject: Physics Course: US05CPHY01 Classical Mechanics

B.Sc. (Semester - 5) Subject: Physics Course: US05CPHY01 Classical Mechanics 1 B.Sc. (Semester - 5) Subject: Physics Course: US05CPHY01 Classical Mechanics Question Bank UNIT: I Multiple choice questions: (1) The gravitational force between two masses is (a) Repulsive (b) Attractive

More information

2007 Problem Topic Comment 1 Kinematics Position-time equation Kinematics 7 2 Kinematics Velocity-time graph Dynamics 6 3 Kinematics Average velocity

2007 Problem Topic Comment 1 Kinematics Position-time equation Kinematics 7 2 Kinematics Velocity-time graph Dynamics 6 3 Kinematics Average velocity 2007 Problem Topic Comment 1 Kinematics Position-time equation Kinematics 7 2 Kinematics Velocity-time graph Dynamics 6 3 Kinematics Average velocity Energy 7 4 Kinematics Free fall Collisions 3 5 Dynamics

More information

How do we describe motion?

How do we describe motion? Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion: Examples from Everyday Life Our goals for learning: How do we describe motion? How is mass different

More information

Circular Motion Test Review

Circular Motion Test Review Circular Motion Test Review Name: Date: 1) Is it possible for an object moving with a constant speed to accelerate? Explain. A) No, if the speed is constant then the acceleration is equal to zero. B) No,

More information

DIVIDED SYLLABUS ( ) - CLASS XI PHYSICS (CODE 042) COURSE STRUCTURE APRIL

DIVIDED SYLLABUS ( ) - CLASS XI PHYSICS (CODE 042) COURSE STRUCTURE APRIL DIVIDED SYLLABUS (2015-16 ) - CLASS XI PHYSICS (CODE 042) COURSE STRUCTURE APRIL Unit I: Physical World and Measurement Physics Need for measurement: Units of measurement; systems of units; SI units, fundamental

More information

Chapter 5 Centripetal Force and Gravity. Copyright 2010 Pearson Education, Inc.

Chapter 5 Centripetal Force and Gravity. Copyright 2010 Pearson Education, Inc. Chapter 5 Centripetal Force and Gravity v Centripetal Acceleration v Velocity is a Vector v It has Magnitude and Direction v If either changes, the velocity vector changes. Tumble Buggy Demo v Centripetal

More information

Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Copyright 2012 Pearson Education, Inc.

Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Copyright 2012 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 1 4.1 Describing Motion: Examples from Everyday Life Our goals for learning: How do we describe motion? How is mass different

More information

12/1/2014. Chapter 5 Circular Motion; Gravitation. Contents of Chapter 5. Contents of Chapter Kinematics of Uniform Circular Motion

12/1/2014. Chapter 5 Circular Motion; Gravitation. Contents of Chapter 5. Contents of Chapter Kinematics of Uniform Circular Motion Lecture PowerPoints Chapter 5 Physics: Principles with Applications, 7 th edition Giancoli Chapter 5 Circular Motion; Gravitation This work is protected by United States copyright laws and is provided

More information

1 The displacement, s in metres, of an object after a time, t in seconds, is given by s = 90t 4 t 2

1 The displacement, s in metres, of an object after a time, t in seconds, is given by s = 90t 4 t 2 CFE Advanced Higher Physics Unit 1 Rotational Motion and Astrophysics Kinematic relationships 1 The displacement, s in metres, of an object after a time, t in seconds, is given by s = 90t 4 t 2 a) Find

More information

Chapter 13. Gravitation

Chapter 13. Gravitation Chapter 13 Gravitation e = c/a A note about eccentricity For a circle c = 0 à e = 0 a Orbit Examples Mercury has the highest eccentricity of any planet (a) e Mercury = 0.21 Halley s comet has an orbit

More information

9/13/ Describing Motion: Examples from Everyday Life. Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity

9/13/ Describing Motion: Examples from Everyday Life. Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity 9/13/17 Lecture Outline 4.1 Describing Motion: Examples from Everyday Life Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity Our goals for learning: How do we describe motion?

More information

Newton s Gravitational Law

Newton 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 information

Class XI Physics Syllabus One Paper Three Hours Max Marks: 70

Class XI Physics Syllabus One Paper Three Hours Max Marks: 70 Class XI Physics Syllabus 2013 One Paper Three Hours Max Marks: 70 Class XI Weightage Unit I Physical World & Measurement 03 Unit II Kinematics 10 Unit III Laws of Motion 10 Unit IV Work, Energy & Power

More information

Epicycles the short form.

Epicycles the short form. Homework Set 3 Due Sept 9 CO 4.15 just part (a). (see CO pg. 908) CO 4.1 CO 4.36 (a),(b) CO 5.14 (assume that Sun currently has its max. u velocity.) CO 5.16 (Keplerian orbit = orbit around a point mass)

More information

Regular Physics Semester 1

Regular Physics Semester 1 Regular Physics Semester 1 1.1.Can define major components of the scientific method 1.2.Can accurately carry out conversions using dimensional analysis 1.3.Can utilize and convert metric prefixes 1.4.Can

More information

Lecture Fall 2005 Astronomy 110 1

Lecture Fall 2005 Astronomy 110 1 Lecture 9 + 10 Fall 2005 Astronomy 110 1 Isaac Newton and the birth of Physics If I have seen farther than others, it is because I have stood on the shoulders of giants. Sir Isaac Newton (1642 1727) Nature

More information

Natural Questions. About 2000 years ago Greek scientists were confused about motion. and developed a theory of motion

Natural Questions. About 2000 years ago Greek scientists were confused about motion. and developed a theory of motion Natural Questions First natural question: Next question: What these things made of? Why and how things move? About 2000 years ago Greek scientists were confused about motion. Aristotle --- First to study

More information

SPRING GROVE AREA SCHOOL DISTRICT. Course Description. Instructional Strategies, Learning Practices, Activities, and Experiences.

SPRING GROVE AREA SCHOOL DISTRICT. Course Description. Instructional Strategies, Learning Practices, Activities, and Experiences. SPRING GROVE AREA SCHOOL DISTRICT PLANNED COURSE OVERVIEW Course Title: Advanced Placement Physics 1 Grade Level(s): 10-12 Units of Credit: 1.5 credits Classification: Elective Length of Course: 30 cycles

More information

2. For a S.H.O. determine, (a) the total energy (E), the kinetic and potential energies. of half amplitude:

2. For a S.H.O. determine, (a) the total energy (E), the kinetic and potential energies. of half amplitude: The amplitude of vibration and hence, the energy transferred into the vibrating system is found to depend on the difference between f and, its maximum when the frequency of the external force is equal

More information

9.3 Worked Examples Circular Motion

9.3 Worked Examples Circular Motion 9.3 Worked Examples Circular Motion Example 9.1 Geosynchronous Orbit A geostationary satellite goes around the earth once every 3 hours 56 minutes and 4 seconds, (a sidereal day, shorter than the noon-to-noon

More information

EART162: PLANETARY INTERIORS

EART162: PLANETARY INTERIORS EART162: PLANETARY INTERIORS Francis Nimmo Last Week Applications of fluid dynamics to geophysical problems Navier-Stokes equation describes fluid flow: Convection requires solving the coupled equations

More information

Chapter 9 Uniform Circular Motion

Chapter 9 Uniform Circular Motion 9.1 Introduction Chapter 9 Uniform Circular Motion Special cases often dominate our study of physics, and circular motion is certainly no exception. We see circular motion in many instances in the world;

More information

Astronomy 111 Review Problems Solutions

Astronomy 111 Review Problems Solutions Astronomy 111 Review Problems Solutions Problem 1: Venus has an equatorial radius of 6052 km. Its semi-major axis is 0.72 AU. The Sun has a radius of cm. a) During a Venus transit (such as occurred June

More information

Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.

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

More information

Introduction to CLASSICAL MECHANICS

Introduction to CLASSICAL MECHANICS Introduction to CLASSICAL MECHANICS Introduction to CLASSICAL MECHANICS A.P. FRENCH Massachusetts Institute oj Technology M.G. EBISON The Institute oj Physics, London KLUWER ACADEMIC PUBLISHERS DORDRECHT

More information

VISUAL PHYSICS ONLINE

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

More information

Chapter 7. Preview. Objectives Tangential Speed Centripetal Acceleration Centripetal Force Describing a Rotating System. Section 1 Circular Motion

Chapter 7. Preview. Objectives Tangential Speed Centripetal Acceleration Centripetal Force Describing a Rotating System. Section 1 Circular Motion Section 1 Circular Motion Preview Objectives Tangential Speed Centripetal Acceleration Centripetal Force Describing a Rotating System Section 1 Circular Motion Objectives Solve problems involving centripetal

More information

Visualization of Traveling Vortices in the Boundary Layer on a Rotating Disk under Orbital Motion

Visualization of Traveling Vortices in the Boundary Layer on a Rotating Disk under Orbital Motion Open Journal of Fluid Dynamics, 2015, 5, 17-25 Published Online March 2015 in SciRes. http://www.scirp.org/journal/ojfd http://dx.doi.org/10.4236/ojfd.2015.51003 Visualization of Traveling Vortices in

More information

November 16, Henok Tadesse, Electrical Engineer, B.Sc. Ethiopia. or

November 16, Henok Tadesse, Electrical Engineer, B.Sc. Ethiopia.   or The outward acceleration of galaxies may be a result of a non uniform and non linear distribution of matter in the universe Non local gravity directed upwards due to higher density outwards! Non elliptical

More information

PHYSICS. Chapter 13 Lecture FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E RANDALL D. KNIGHT Pearson Education, Inc.

PHYSICS. Chapter 13 Lecture FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E RANDALL D. KNIGHT Pearson Education, Inc. PHYSICS FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E Chapter 13 Lecture RANDALL D. KNIGHT Chapter 13 Newton s Theory of Gravity IN THIS CHAPTER, you will learn to understand the motion of satellites

More information

Chapter 9 Circular Motion Dynamics

Chapter 9 Circular Motion Dynamics Chapter 9 Circular Motion Dynamics Chapter 9 Circular Motion Dynamics... 9. Introduction Newton s Second Law and Circular Motion... 9. Universal Law of Gravitation and the Circular Orbit of the Moon...

More information

Gravity. 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   (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 information

4.1 Describing Motion. How do we describe motion? Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity

4.1 Describing Motion. How do we describe motion? Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion Our goals for learning: How do we describe motion? How is mass different from weight? How do we describe

More information

(b) The period T and the angular frequency ω of uniform rotation are related to the cyclic frequency f as. , ω = 2πf =

(b) The period T and the angular frequency ω of uniform rotation are related to the cyclic frequency f as. , ω = 2πf = PHY 302 K. Solutions for problem set #9. Non-textbook problem #1: (a) Rotation frequency of 1 Hz means one revolution per second, or 60 revolutions per minute (RPM). The pre-lp vinyl disks rotated at 78

More information

Basic Physics. What We Covered Last Class. Remaining Topics. Center of Gravity and Mass. Sun Earth System. PHYS 1411 Introduction to Astronomy

Basic Physics. What We Covered Last Class. Remaining Topics. Center of Gravity and Mass. Sun Earth System. PHYS 1411 Introduction to Astronomy PHYS 1411 Introduction to Astronomy Basic Physics Chapter 5 What We Covered Last Class Recap of Newton s Laws Mass and Weight Work, Energy and Conservation of Energy Rotation, Angular velocity and acceleration

More information

Contents. I Introduction 1. Preface. xiii

Contents. I Introduction 1. Preface. xiii Contents Preface xiii I Introduction 1 1 Continuous matter 3 1.1 Molecules................................ 4 1.2 The continuum approximation.................... 6 1.3 Newtonian mechanics.........................

More information

Astronomy 241: Foundations of Astrophysics I. The Solar System

Astronomy 241: Foundations of Astrophysics I. The Solar System Astronomy 241: Foundations of Astrophysics I. The Solar System Astronomy 241 is the first part of a year-long introduction to astrophysics. It uses basic classical mechanics and thermodynamics to analyze

More information

Johannes Kepler ( ) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it!

Johannes Kepler ( ) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it! Johannes Kepler (1571-1630) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it! Kepler s Life Work Kepler sought a unifying principle

More information

Part I Multiple Choice (4 points. ea.)

Part I Multiple Choice (4 points. ea.) ach xam usually consists of 10 ultiple choice questions which are conceptual in nature. They are often based upon the assigned thought questions from the homework. There are also 4 problems in each exam,

More information

Radial Acceleration. recall, the direction of the instantaneous velocity vector is tangential to the trajectory

Radial Acceleration. recall, the direction of the instantaneous velocity vector is tangential to the trajectory Radial Acceleration recall, the direction of the instantaneous velocity vector is tangential to the trajectory 1 Radial Acceleration recall, the direction of the instantaneous velocity vector is tangential

More information

Name Period Date Earth and Space Science. Solar System Review

Name Period Date Earth and Space Science. Solar System Review Name Period Date Earth and Space Science Solar System Review 1. is the spinning a planetary object on its axis. 2. is the backward motion of planets. 3. The is a unit less number between 0 and 1 that describes

More information

SHAPE OF ORBITAL PATH

SHAPE OF ORBITAL PATH SHAPE OF ORBITAL PATH According to MATTER (Re-examined) Nainan K. Varghese, matterdoc@gmail.com http://www.matterdoc.info Abstract: In any system of macro bodies, relative considerations can provide only

More information

The maximum kinetic energy is directly proportional to the frequency. The time for one oscillation is directly proportional to the frequency.

The maximum kinetic energy is directly proportional to the frequency. The time for one oscillation is directly proportional to the frequency. Q1.For a body performing simple harmonic motion, which one of the following statements is correct? The maximum kinetic energy is directly proportional to the frequency. The time for one oscillation is

More information

Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Copyright 2009 Pearson Education, Inc.

Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Copyright 2009 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity How do we describe motion? Precise definitions to describe motion: Speed: Rate at which object moves speed = distance time

More information

Ay 1 Lecture 2. Starting the Exploration

Ay 1 Lecture 2. Starting the Exploration Ay 1 Lecture 2 Starting the Exploration 2.1 Distances and Scales Some Commonly Used Units Distance: Astronomical unit: the distance from the Earth to the Sun, 1 au = 1.496 10 13 cm ~ 1.5 10 13 cm Light

More information

Northwestern CT Community College Course Syllabus. Course Title: CALCULUS-BASED PHYSICS I with Lab Course #: PHY 221

Northwestern CT Community College Course Syllabus. Course Title: CALCULUS-BASED PHYSICS I with Lab Course #: PHY 221 Northwestern CT Community College Course Syllabus Course Title: CALCULUS-BASED PHYSICS I with Lab Course #: PHY 221 Course Description: 4 credits (3 class hours and 3 laboratory hours per week) Physics

More information

2.5.1 Static tides Tidal dissipation Dynamical tides Bibliographical notes Exercises 118

2.5.1 Static tides Tidal dissipation Dynamical tides Bibliographical notes Exercises 118 ii Contents Preface xiii 1 Foundations of Newtonian gravity 1 1.1 Newtonian gravity 2 1.2 Equations of Newtonian gravity 3 1.3 Newtonian field equation 7 1.4 Equations of hydrodynamics 9 1.4.1 Motion of

More information

Computational Modeling of Volcanism on Earth-like

Computational Modeling of Volcanism on Earth-like PHYSICS Computational Modeling of Volcanism on Earth-like Planets EDWARD KIM MATTHEW J.S. BEACH ETHAN BUCHMAN ABSTRACT The aim of this paper is to model the level of volcanic activity on Earth-like planets

More information

Conceptual Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson II September 5, 2017

Conceptual Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson II September 5, 2017 Conceptual Physics Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson II September 5, 2017 https://arxiv.org/abs/1711.07445 L. A. Anchordoqui (CUNY)

More information

Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the

Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the Geocentric-Heliocentric debate (Brahe s data and Kepler s analysis)

More information

Copyright 2009, August E. Evrard.

Copyright 2009, August E. Evrard. Unless otherwise noted, the content of this course material is licensed under a Creative Commons BY 3.0 License. http://creativecommons.org/licenses/by/3.0/ Copyright 2009, August E. Evrard. You assume

More information

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion Today Planetary Motion Tycho Brahe s Observations Kepler s Laws Laws of Motion Laws of Motion In 1633 the Catholic Church ordered Galileo to recant his claim that Earth orbits the Sun. His book on the

More information

Uniform Circular Motion

Uniform Circular Motion Circular Motion Uniform Circular Motion Uniform Circular Motion Traveling with a constant speed in a circular path Even though the speed is constant, the acceleration is non-zero The acceleration responsible

More information

Special Relativity: The laws of physics must be the same in all inertial reference frames.

Special Relativity: The laws of physics must be the same in all inertial reference frames. Special Relativity: The laws of physics must be the same in all inertial reference frames. Inertial Reference Frame: One in which an object is observed to have zero acceleration when no forces act on it

More information

Chapter 7: Circular Motion

Chapter 7: Circular Motion Chapter 7: Circular Motion Spin about an axis located within the body Example: Spin about an axis located outside the body. Example: Example: Explain why it feels like you are pulled to the right side

More information

AP PHYSICS 1 Content Outline arranged TOPICALLY

AP PHYSICS 1 Content Outline arranged TOPICALLY AP PHYSICS 1 Content Outline arranged TOPICALLY with o Big Ideas o Enduring Understandings o Essential Knowledges o Learning Objectives o Science Practices o Correlation to Common Textbook Chapters Much

More information

The Cosmic Perspective Seventh Edition. Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Chapter 4 Lecture

The 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 information

4.1 Describing Motion

4.1 Describing Motion Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion Our goals for learning: How do we describe motion? How is mass different from weight? How do we describe

More information

UNITS AND MEASUREMENTS

UNITS AND MEASUREMENTS Chapter Two UNITS AND MEASUREMENTS MCQ I 2.1 The number of significant figures in 0.06900 is (a) 5 (b) 4 (c) 2 (d) 3 2.2 The sum of the numbers 436.32, 227.2 and 0.301 in appropriate significant figures

More information

Gravitation. Objectives. The apple and the Moon. Equations 6/2/14. Describe the historical development of the concepts of gravitational force.

Gravitation. Objectives. The apple and the Moon. Equations 6/2/14. Describe the historical development of the concepts of gravitational force. Gravitation Objectives Describe the historical development of the concepts of gravitational force. Describe and calculate how the magnitude of the gravitational force between two objects depends on their

More information

Newton's Laws. Before Isaac Newton

Newton's Laws. Before Isaac Newton Newton's Laws Before Isaac Newton Newton's Laws There were facts and laws about the way the physical world worked, but no explanations After Newton There was a unified system that explained those facts

More information

Northwestern Connecticut Community College Course Syllabus

Northwestern Connecticut Community College Course Syllabus Northwestern Connecticut Community College Course Syllabus Course Title: Introductory Physics Course #: PHY 110 Course Description: 4 credits (3 class hours and 3 laboratory hours per week) Physics 110

More information

AP Physics C Mechanics Objectives

AP Physics C Mechanics Objectives AP Physics C Mechanics Objectives I. KINEMATICS A. Motion in One Dimension 1. The relationships among position, velocity and acceleration a. Given a graph of position vs. time, identify or sketch a graph

More information

This leads to or ( )( ). 8. B LED s are Light Emitting Diodes 9. D The expression for the period of a simple pendulum at small angles is.

This leads to or ( )( ). 8. B LED s are Light Emitting Diodes 9. D The expression for the period of a simple pendulum at small angles is. 2013 PhysicsBowl Solutions # Ans # Ans # Ans # Ans # Ans 1 C 11 E 21 E 31 D 41 A 2 B 12 C 22 B 32 E 42 C 3 D 13 E 23 D 33 A 43 A 4 E 14 B 24 B 34 A 44 E 5 A 15 D 25 A 35 C 45 C 6 C 16 D 26 B 36 C 46 E

More information

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton. Name: Date: 1. The word planet is derived from a Greek term meaning A) bright nighttime object. B) astrological sign. C) wanderer. D) nontwinkling star. 2. The planets that were known before the telescope

More information

ASTRONOMY LECTURE NOTES MIDTERM REVIEW. ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens

ASTRONOMY LECTURE NOTES MIDTERM REVIEW. ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens ASTRONOMY LECTURE NOTES MIDTERM REVIEW ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens How Do We Locate Objects in the Sky? Local-Sky Coordinates versus Celestial-Sphere Coordinates When the sky

More information

12-Feb-18. Newton's Laws. Newton's Laws. Prelude to Newton's Laws

12-Feb-18. Newton's Laws. Newton's Laws. Prelude to Newton's Laws Newton's Laws Newton's Laws Before Isaac Newton There were facts and laws about the way the physical world worked, but no explanations After Newton There was a unified system that explained those facts

More information

13-Feb-19. Newton's Laws. Newton's Laws. Prelude to Newton's Laws

13-Feb-19. Newton's Laws. Newton's Laws. Prelude to Newton's Laws Newton's Laws 1 Newton's Laws Before Isaac Newton There were facts and laws about the way the physical world worked, but no explanations After Newton There was a unified system that explained those facts

More information

Lecture 13 REVIEW. Physics 106 Spring What should we know? What should we know? Newton s Laws

Lecture 13 REVIEW. Physics 106 Spring What should we know? What should we know? Newton s Laws Lecture 13 REVIEW Physics 106 Spring 2006 http://web.njit.edu/~sirenko/ What should we know? Vectors addition, subtraction, scalar and vector multiplication Trigonometric functions sinθ, cos θ, tan θ,

More information

Chapter 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 information

University Physics 226N/231N Old Dominion University. More Circular Motion, then Newton s Laws

University Physics 226N/231N Old Dominion University. More Circular Motion, then Newton s Laws University Physics 226N/231N Old Dominion University More Circular Motion, then Newton s Laws Dr. Todd Satogata (ODU/Jefferson Lab) satogata@jlab.org http://www.toddsatogata.net/2016-odu Wednesday, September

More information

Downloaded from

Downloaded from Chapter 8 (Gravitation) Multiple Choice Questions Single Correct Answer Type Q1. The earth is an approximate sphere. If the interior contained matter which is not of the same density everywhere, then on

More information

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws of Planetary Motion. Laws of Motion. in physics

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws of Planetary Motion. Laws of Motion. in physics Planetary Motion Today Tycho Brahe s Observations Kepler s Laws of Planetary Motion Laws of Motion in physics Page from 1640 text in the KSL rare book collection That the Earth may be a Planet the seeming

More information

Chapter 8 - Gravity Tuesday, March 24 th

Chapter 8 - Gravity Tuesday, March 24 th Chapter 8 - Gravity Tuesday, March 24 th Newton s law of gravitation Gravitational potential energy Escape velocity Kepler s laws Demonstration, iclicker and example problems We are jumping backwards to

More information

g = Gm / r 2 The Big Idea

g = Gm / r 2 The Big Idea The Big Idea Over 2500 years ago Aristotle proposed two laws of physics governing motion. One for Earthly bodies (objects on Earth) that states objects naturally go in straight lines and one for Heavenly

More information

Fineman Honors Physics Final Study Guide

Fineman Honors Physics Final Study Guide All Science Tests are on Wednesday, June 17 th. Students who take more than one Science class will take their second science final on Thursday, June 18 from 8:00-10:00 AM in the Library. The Honors Physics

More information

7. The gyroscope. 7.1 Introduction. 7.2 Theory. a) The gyroscope

7. The gyroscope. 7.1 Introduction. 7.2 Theory. a) The gyroscope K 7. The gyroscope 7.1 Introduction This experiment concerns a special type of motion of a gyroscope, called precession. From the angular frequency of the precession, the moment of inertia of the spinning

More information

Topic 6 The Killers LEARNING OBJECTIVES. Topic 6. Circular Motion and Gravitation

Topic 6 The Killers LEARNING OBJECTIVES. Topic 6. Circular Motion and Gravitation Topic 6 Circular Motion and Gravitation LEARNING OBJECTIVES Topic 6 The Killers 1. Centripetal Force 2. Newton s Law of Gravitation 3. Gravitational Field Strength ROOKIE MISTAKE! Always remember. the

More information

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Celestial motions The stars: Uniform daily motion about the celestial poles (rising and setting). The Sun: Daily motion around the celestial

More information

1 2 Models, Theories, and Laws 1.5 Distinguish between models, theories, and laws 2.1 State the origin of significant figures in measurement

1 2 Models, Theories, and Laws 1.5 Distinguish between models, theories, and laws 2.1 State the origin of significant figures in measurement Textbook Correlation Textbook Correlation Physics 1115/2015 Chapter 1 Introduction, Measurement, Estimating 1.1 Describe thoughts of Aristotle vs. Galileo in describing motion 1 1 Nature of Science 1.2

More information