Barycenter of Solar System Earth-Moon barycenter? Moon orbits what?



Similar documents
From Aristotle to Newton

Newton s Law of Gravity

EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1

Astronomy 1140 Quiz 1 Review

Vocabulary - Understanding Revolution in. our Solar System

astronomy A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

Chapter 25.1: Models of our Solar System

circular motion & gravitation physics 111N

Newton s Law of Universal Gravitation

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES

CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS

Motions of Earth, Moon, and Sun

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015

Reasons for Seasons. Question: TRUE OR FALSE. Question: TRUE OR FALSE? What causes the seasons? What causes the seasons?

Exercise: Estimating the Mass of Jupiter Difficulty: Medium

Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?

Study Guide due Friday, 1/29

Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:

Are Those Sunspots Really on the Sun?

Newton s Laws. Newton s Imaginary Cannon. Michael Fowler Physics 142E Lec 6 Jan 22, 2009

A = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great.

The University of Texas at Austin. Gravity and Orbits

Lab Activity on the Causes of the Seasons

Gravitation and Newton s Synthesis

Coordinate Systems. Orbits and Rotation

1.1 A Modern View of the Universe" Our goals for learning: What is our place in the universe?"

CELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton

How To Understand General Relativity

Introduction to the Solar System

USING MS EXCEL FOR DATA ANALYSIS AND SIMULATION

How To Understand The Theory Of Gravity

Planetary Orbit Simulator Student Guide

Celestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun)

The Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following:

The following words and their definitions should be addressed before completion of the reading:

UNIT V. Earth and Space. Earth and the Solar System

Exercise 5.0 LUNAR MOTION, ELONGATION, AND PHASES

Space Poems For Preschool Children

Study Guide: Solar System

Astromechanics Two-Body Problem (Cont)

2. Orbits. FER-Zagreb, Satellite communication systems 2011/12

The Gravitational Field

Chapter 3 The Science of Astronomy

Lesson 26: Reflection & Mirror Diagrams

Lecture 13. Gravity in the Solar System

How did the Solar System form?

Curiosity's Fight Path to Mars. A Project for Differential Equations (Math 256)

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton

An Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science

Unit 8 Lesson 2 Gravity and the Solar System

1. Mass, Force and Gravity

Section 4: The Basics of Satellite Orbits

TIDES. 1. Tides are the regular rise and fall of sea level that occurs either once a day (every 24.8 hours) or twice a day (every 12.4 hours).

Chapter 9 Circular Motion Dynamics

Lecture L17 - Orbit Transfers and Interplanetary Trajectories

Topic 7A: Tides, Part II. Online Lecture: The Bulge Theory of Tides

Earth In Space Chapter 3

I n t e r a c t i n g G a l a x i e s - Making Ellipticals Te a c h e r N o t e s

1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram?

Earth in the Solar System

DIRECT ORBITAL DYNAMICS: USING INDEPENDENT ORBITAL TERMS TO TREAT BODIES AS ORBITING EACH OTHER DIRECTLY WHILE IN MOTION

III. Applications of Force and Motion Concepts. Concept Review. Conflicting Contentions. 1. Airplane Drop 2. Moving Ball Toss 3. Galileo s Argument

The Hidden Lives of Galaxies. Jim Lochner, USRA & NASA/GSFC

AP Environmental Science Graph Prep

Educator Guide to S LAR SYSTEM El Prado, San Diego CA (619)

Notes: Most of the material in this chapter is taken from Young and Freedman, Chap. 13.

Gravity. in the Solar System. Beyond the Book. FOCUS Book

Force on Moving Charges in a Magnetic Field

Chapter 7 Our Planetary System. Agenda. Intro Astronomy. Intro Astronomy. What does the solar system look like? A. General Basics

Class 2 Solar System Characteristics Formation Exosolar Planets

5- Minute Refresher: Daily Observable Patterns in the Sky

Version A Page The diagram shows two bowling balls, A and B, each having a mass of 7.00 kilograms, placed 2.00 meters apart.

Orbital Mechanics. Angular Momentum

Orbital Dynamics with Maple (sll --- v1.0, February 2012)

Name: Date: Period: Gravity Study Guide

Chapter 5: Circular Motion, the Planets, and Gravity

Chapter 1 Our Place in the Universe

Use the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.

Earth, Moon, and Sun Study Guide. (Test Date: )

Week 1-2: Overview of the Universe & the View from the Earth

Artificial Satellites Earth & Sky

GRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter

A.4 The Solar System Scale Model

Lab 6: Kepler's Laws. Introduction. Section 1: First Law

Freely Falling Bodies & Uniformly Accelerated Motion

Penn State University Physics 211 ORBITAL MECHANICS 1

The Sun. Solar radiation (Sun Earth-Relationships) The Sun. The Sun. Our Sun

Exploration of the Solar System

Scales of the Universe

Sun Earth Relationships

Centripetal Force. This result is independent of the size of r. A full circle has 2π rad, and 360 deg = 2π rad.

Angular Velocity vs. Linear Velocity

Explain the Big Bang Theory and give two pieces of evidence which support it.

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)

Orbital Mechanics and Space Geometry

SOLVING EQUATIONS WITH RADICALS AND EXPONENTS 9.5. section ( )( ). The Odd-Root Property

The Celestial Sphere. Questions for Today. The Celestial Sphere 1/18/10

x x y y Then, my slope is =. Notice, if we use the slope formula, we ll get the same thing: m =

Transcription:

Barycenter of Solar System Earth-Moon barycenter? Moon orbits what? Dr. Scott Schneider Friday Feb 24 th, 2006 Sponsored by the Society of Physics Students (SPS) Webpage : http://qbx6.ltu.edu/s_schneider/astro/astroweek_2006.shtml

Brought to you by The Letter Q (as in Quisp) The number 3.1415 Code Red! Diet Coke (after the sugar shakes set in). Britney Spears?

Who orbits what? Planets in the solar system orbit the Sun? Actually they orbit the center of mass Called the barycenter of the solar system Barycenter has smooth path through galaxy (but Sun/planets wiggle ) Earth/Moon system also has a barycenter

How do you calculate the barycenter? Start with how to you find the positions of the planets Fancy dancy powerful computers can calculate the positions based on Newton s law of Gravity (and Einstein (JPL) Those time series (way too large to be emailed ) can be analyzed (VSOP theory) Fourier series approximation (based on time) Now you just need to know the coefficients Can then reconstruct the position information

To find the planet locations Pick a planet.. (poor Pluto too tough, but too far away) Pick a date Pick a coordinate system Heliocentric = measured from the Sun (center) Earth-Sun plane point of Aries (Earth-Sun: Spring) Geocentric = measured from Earth (center) Get back either X, Y, Z Measured in Astronomical Units (AU) (Earth-Sun distance) or l (longitude), b (latitude), r (radial distance)

Just some sums (many!) For each of the coordinates (x, y, z or l, b, r) have up to 5 coefficients for a time polynomial Coefficients generated from long cosine series Some series have over 2000 terms for one coefficent for one variable!

First you get the planets, then you get the power If you have all the locations of the planets Let s use x, y, z for the planets Can now find the center of mass of the system weighted average of the planets + Sun Measured from the center of the Sun Since planet distances measured from Sun, we find barycenter from center of sun Can watch barycenter move around disk of the Sun Remember, actually sun (and planets) orbit barycenter!

Equations for Barycenter What are the subscripts 1 through 8?? Once we have X, Y, Z for barycenter can calculate the net distance from the Sun center Denote this distance as G units of Sun radius

How to plot the barycenter info? Can plot distance G against time Watch for highs and lows When is it near Sun center far from Sun center? Can plot barycenter on xy graph of Sun s disk Watch path of barycenter Remember really Sun moving around barycenter Get too dizzy to try to have Sun wiggle around barycenter! Since we know the planet locations can also plot them on a solar system xy plane Might be interesting to see where the planets are when the Sun is near or far from the barycenter! Computer Program Demo!

Results from the Barycenter demo The barycenter not confined to the Sun s interior! From 1940-2060 G = outside Sun 62 % of the time Can also spend more than 10 years inside Jupiter is the big dog planet! When G is near zero often have Jupiter on one side other planets on the other side G can be more than 2 solar radii This usually means all the planets are on the same side of the Sun G = 1 passing through radius of sun Watch how the shift in the planets is related to this! How would we use this info about a solar system barycenter? A star would wiggle to an outside observer based on the planets

Earth/Moon barycenter Earth mass much larger than Moon Keeps the barycenter inside the Earth Distance from Earth center is 70-80% Earth radius Why does the distance vary? Boring to plot that (basically a circle) No cool looping in and out of the radius.. Where does the Earth-Moon line stick out? Can calculate location of moon Similar to the planets a series calculation Then plot it on the surface of the Earth longitude/latitude Seems easy how could anyone make a mistake? Computer Program Demo!

Rookie Mistakes! and results Forgot to take into account Earth axis tilt doh! Forgot to take into account rotation of Earth! Short time (1 year) paths of moon shift a little Why is there any shift at all in a year? Longer time (10 years) starts to fill in band Why does it fill in? What factors? What else does that band represent? What if there was an observer along one of those tracks?

Moon orbits the Earth, right? Seems like an obvious question? This was at least one thing the ancients got right! We have full moons and new moons! Moon must get between us and the Sun! What does the orbit look like in space Jump in a rocket and rise above the Earth-Sun plane Look down on the Moon orbit as the Earth-Moon system goes around the Sun My prediction is that there are NO loop-de-loops! Skygazer Demo 1!

Um uh. er Ok, I really thought there wasn t supposed to be any outward motion of the moon Wait.. What was that line about x400 scale? Could the scaling of the moon orbit create that motion (the motion that offends me!)? Let s try scaling down the moon-orbit? Skygazer Demo 2!

Ok, well, that s better Scaling the system by 400x gave loops Note: MANY books show the orbit like that! Bringing the scale down to 100x got rid of the loops But, there is still the curving outward part? Let s try scaling down the moon-orbit again? Skygazer Demo 3!

Almost there. Scaling by 20 gives us a hint that maybe the moon path doesn t curve outward Run Demo 4 1 to 1 scale Note: we can remove Earth orbit just in case Now it looks like the orbit is only curving inward never bends outward Can we prove that with data? Skygazer Demo 4!

Calculate Moon AND Earth! Find the distance of the Earth to the Sun Find the distance from Moon to Earth Add them together find the Moon-Sun distance! Should be able to show that it doesn t curve outward! So.. On to the results!

Umm uhh errr Distance from Moon to Sun (zoomed) 1.025 1.02 1.015 Distance in AU 1.01 1.005 1 0.995 0.99 0.985 0.98 0.975 0 500 1000 1500 2000 2500 3000 3500 4000 Tenth of a Day Wait maybe if I just change the vertical scale?

Umm uhh errr part 2 Distance from Moon to Sun (no zoom) 1.2 1 Distance in AU 0.8 0.6 0.4 0.2 0 0 500 1000 1500 2000 2500 3000 3500 4000 Tenth of a Day Any ideas? (Not Brad!)

Can t plot on XY axes! The curving outward is a polar plot idea Clearly the Moon has to occasionally come closer to the Sun than the Earth, and go farther out If curving inward meant getting closer to the Sun all the time it would crash! Then what does it mean to be always curving inward? Here is an example an ellipse! Clearly the object in elliptical orbit comes closer and farther But, the orbit path never curves outward! Very clever but the Moon orbit isn t exactly elliptical

How can we show the curvature? Dr. Scott puzzled and puzzed, until his puzzler was sore! Note: Dr. Scott never reuses jokes just ask any of the students that have him for more than one term!

Calculus to the rescue!! A day spent not thinking about vectors is a day wasted! We can use vectors to verify the only curving inward nature And vectors very happily don t worry about limitations like XY plots to try to illustrate curvature! And, since we have already calculated the XY positions, we can easily calculate vectors and use certain properties of vectors (mysterious!)

What vectors are needed? If we connect the moon s position on one date, to the position on the next date we have a vector! And if we join the second position to a third another vector Those two vectors will have a relative angle between them Can create a cross product of the vectors If the two vectors are only the XY plane, the cross product will be in the Z direction only!! And, +z or z direction determined by curvature!

Simple ellipse with vectors and cross If vectors turn inward then cross product points out of the page/board (+z direction = +k)

Inward curve gives negative value! If vectors turn outward then cross product points INTO of the page/board (-z direction = -k)!! We now have a method to prove the curving inward Moon orbit!

Drum roll Cross Product of Moon Vectors Z component (positive is good!) 0.000000009 0.000000008 0.000000007 0.000000006 0.000000005 0.000000004 0.000000003 0.000000002 0.000000001 0 0 500 1000 1500 2000 2500 3000 3500 Time And, he sticks the landing! Yup, Olympics were on TV when I was doing this Also note only the X and Y values contribute to the Z component of the cross (so only using X and Y is not a problem!)

What further tests? More resolution - try 30 days (that would be enough for moon to go out then in full orbit of Earth) Using about 4000 points 10x resolution! Still good!! Cross Product of Moon Vectors - 30 days Z component (positive is good!) 0.00018 0.000175 0.00017 0.000165 0.00016 0.000155 0.00015 0.000145 0.00014 0 500 1000 1500 2000 2500 3000 3500 Time

So what affects orbit curvature? Our Moon is essentially unique in the solar system Most other moons have the loop-de-loop type behavior Some just curve outward some loop some do both! Curve-outward orbits related to mass ratios of Sun and planet compared to the distance ratio of Moon to planet We can create a simulation system with fake orbits The principles would still apply Can adjust radii and orbit periods watch cross product!

Fake moon orbits sun model Have circular orbit for planet around sun Have circular orbit of moon around planet Adjust the ratio of planet orbit period to moon orbit period Adjust the distance of moon-to-planet vs planet-to-sun Watch the cross product to see if it goes negative (loops or curves outward)! Excel Demo!

Bonus: Planets lining up in space? Planets can t line up in a straight line (from the Sun) Orbits are tilted nodes don t line up periods don t line up Didn t you see the talk last Tuesday? They can line up in some other line in space We ll consider three planets middle occults outside ones One planet crosses in front of another occultation Does each outside planet see the same event? Depends on how far away they are from each other Marvin the Martian and Earth and Venus yes Non-reciprocal Occultation of Jupiter Venus Mars (1930) -No Skygazer Demos!

References Jean Meeus is an Astronomer from Belgium does some absolutely amazing astronomical calculations. Has many excellent books : Astronomical Algorithms Astronomy Morsels More Astronomy Morsels Astronomy Morsels III please.. MORE!!

This talk, and other exciting things can be found http://qbx6.ltu.edu/s_schneider/astro/index.shtml Thank you, Good Night, Drive Safely!