1 Class #23 Celestial engineering Kepler’s Laws Energy, angular momentum and Eccentricity.

Slides:



Advertisements
Similar presentations
A New Look at Conic Sections
Advertisements

Review Chap. 12 Gravitation
1 Class #22 Celestial engineering Central Forces DVD The power of Equivalent 1-D problem and Pseudopotential  Kepler’s 3 rd law Orbits and Energy  The.
1 Class #24 of 30 Exam -- Tuesday Additional HW problems posted Friday (also due Tuesday). Bring Index Card #3. Office hours on Monday 3:30-6:00 Topics.
1 Class #19 of 30 Celestial engineering - II Reduced 2-body problem Kepler 1 st, 2 nd and 3 rd laws Cometary collision prediction A whiff of scattering.
Kepler. Inverse Square Force  Force can be derived from a potential.  < 0 for attractive force  Choose constant of integration so V (  ) = 0. m2m2.
Kepler’s Laws of Planetary Motion Newton’s Laws of Gravity
Conservation of Momentum
Parabolas $ $300 $300 $ $ $ $ $ $ $ $ $ $ $ $ $ $100.
NJIT Physics 320: Astronomy and Astrophysics – Lecture II Carsten Denker Physics Department Center for Solar–Terrestrial Research.
ASTR 2310: Chapter 3 Orbital Mechanics Newton's Laws of Motion & Gravitation (Derivation of Kepler's Laws)‏ Conic Sections and other details General Form.
Planets Along the Ecliptic. Retrograde Motion Retrograde Motion Explained.
Newton’s Laws of Motion and Planetary Orbits Gravity makes the solar system go round.
Sect. 13.3: Kepler’s Laws & Planetary Motion. German astronomer (1571 – 1630) Spent most of his career tediously analyzing huge amounts of observational.
Gravity & orbits. Isaac Newton ( ) developed a mathematical model of Gravity which predicted the elliptical orbits proposed by Kepler Semi-major.
Kinetics of Particles:
Special Applications: Central Force Motion
Typical interaction between the press and a scientist?!
Lecture 5: Gravity and Motion
Two-Body Systems.
Physics 201: Lecture 24, Pg 1 Chapter 13 The beautiful rings of Saturn consist of countless centimeter-sized ice crystals, all orbiting the planet under.
MA4248 Weeks 4-5. Topics Motion in a Central Force Field, Kepler’s Laws of Planetary Motion, Couloumb Scattering Mechanics developed to model the universe.
Homework 1 due Tuesday Jan 15. Celestial Mechanics Fun with Kepler and Newton Elliptical Orbits Newtonian Mechanics Kepler’s Laws Derived Virial Theorem.
Lecture 4: Gravity and Motion Describing Motion Speed (miles/hr; km/s) Velocity (speed and direction) Acceleration (change in velocity) Units: m/s 2.
Physics 430: Lecture 19 Kepler Orbits Dale E. Gary NJIT Physics Department.
Orbits Read Your Textbook: Foundations of Astronomy –Chapter 5 Homework Problems –Review Questions: 3, 4, 5, 9, 10 –Review Problems: 1, 3, 4 –Web Inquiries:
Ast 1001 lecture Sept 13 (kd). 4. How Orbits Work Astronomy 1001, Sept 2007 – Prof. K. Davidson.
ASTRONOMY 340 FALL 2007 Class #2 6 September 2007.
Planetary Orbits Planetary orbits in terms of ellipse geometry. In the figure, ε  e Compute major & minor axes (2a & 2b) as in text. Get (recall k =
50 Miscellaneous Parabolas Hyperbolas Ellipses Circles
Sect. 3.7: Kepler Problem: r -2 Force Law Inverse square law force: F(r) = -(k/r 2 ); V(r) = -(k/r) –The most important special case of Central Force.
Circles Ellipse Parabolas Hyperbolas
Circles – An Introduction SPI Graph conic sections (circles, parabolas, ellipses and hyperbolas) and understand the relationship between the.
Projectile and Satellite Motion PROJECTILE MOTION We choose to break up Projectile Motion as a combination of vertical free-fall motion and horizontal.
Algebra Conic Section Review. Review Conic Section 1. Why is this section called conic section? 2. Review equation of each conic section A summary of.
Section 9.1 Quadratic Functions and Their Graphs.
Jeopardy CirclesParabolasEllipsesHyperbolas Mixed Conics Q $100 Q $200 Q $300 Q $400 Q $500 Q $100 Q $200 Q $300 Q $400 Q $500 Final Jeopardy.
Chapter 8: Test Your Proficiency 8-2 Parabolas 8-3 Circles 8-4 Ellipses 8-5 Hyperbolas 8-6 Identifying Conic Sections Directions: Select a section to work.
Conic Sections.
Circles Ellipse Parabolas Hyperbolas
Conics Conics Review. Graph It! Write the Equation?
1 Presented at Central University of Finance and Economics 中央财经大学 Beijing by 卜若柏 Robert Blohm Chinese Economics and Management Academy 中国经济与管理研究院
Spring 2002 Lecture #21 Dr. Jaehoon Yu 1.Kepler’s Laws 2.The Law of Gravity & The Motion of Planets 3.The Gravitational Field 4.Gravitational.
T. K. Ng, HKUST Lecture III: (1)Reference frame problem: Coriolis force (2)Circular motion and angular momentum (3)Planetary motion (Kepler ’ s Laws)
Q12.1 The mass of the Moon is 1/81 of the mass of the Earth.
Kepler’s Laws & Planetary Motion
Find the distance between (-4, 2) and (6, -3). Find the midpoint of the segment connecting (3, -2) and (4, 5).
Unit 5: Conics Feb. 3, What is Conics? This is the short term for conic sections. -Conic Sections include circles, parabolas, ellipses, and hyperbolas.
Kepler’s Law Eric Angat teacher. Orbit Eccentricity The eccentricity of an ellipse can be defined.
Section Orbital Motion of Satellites and Kepler’s Laws
Polar Equations of Conics. Directrix is perpendicular to the polar axis at a distance p units to the left of the pole Directrix is perpendicular to the.
WRITING EQUATIONS OF CONICS IN VERTEX FORM MM3G2.
Celestial Mechanics I Introduction Kepler’s Laws.
The Motion of Planets Kepler’s laws Johannes Kepler.
Equation of a Parabola. Do Now  What is the distance formula?  How do you measure the distance from a point to a line?
PHYS 2006 Tim Freegarde Classical Mechanics. 2 Newton’s law of Universal Gravitation Exact analogy of Coulomb electrostatic interaction gravitational.
Chapter 10 – Conic Sections 1) Circles 2) Parabolas 3) Ellipses 4) Hyperbolas.
Day 4 Orbits and Gravity OpenStax Astronomy Ch. 3
Classical Mechanics PHYS 2006 Tim Freegarde.
Classical Mechanics PHYS 2006 Tim Freegarde.
Sect. 6-5: Kepler’s Laws & Newton’s Synthesis
Kepler’s Laws of Planetary Motion Newton’s Laws of Gravity
Eccentricity Notes.
Aim: How do we compute Eccentricity?
Algebra 2: Conic Sections
Chapter 2 - Part 1 The two body problem
Chapter 10 Algebra II Review JEOPARDY Jeopardy Review.
Gravitational Fields, Circular Orbits and Kepler’s Laws
Presentation transcript:

1 Class #23 Celestial engineering Kepler’s Laws Energy, angular momentum and Eccentricity

2 Kepler’s 1 st, 2 nd and 3 rd laws (1610) 1 st Law – Planets move in ellipses with sun at one focus 2 nd law is direct consequence of momentum conservation “Equal areas are swept out in equal times” True for ALL central forces Third law demonstrated previously relates period to semi-minor radius

3 Kepler’s 3 rd law

4

5 Converting I

6 Converting II

7 Converting III

8 Properties of ellipses :30

9 E, L and Eccentricity The physics is in E and L. Epsilon is purely a geometrical factor. Epsilon equation applies to ALL conic sections (hyperbolae, ellipses, parabolas).

10 Energy and Eccentricity EccentricityEnergyOrbit E<0 Circle E<0 Ellipse E=0 Parabola E>0 hyperbola

11 E, L and Eccentricity The physics is in E and L, and it transfers to quantum mechanics.