Origins Lecture 9; April

Similar documents
HNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian

Comets and Kuiper Belt Objects 4/24/07

Physics 133: Extragalactic Astronomy ad Cosmology

When you have completed this workbook, you should know and understand the following:

Foundations of Astrophysics

The Universe in my pocket. The Solar System. Gloria Delgado Inglada. 4 No. 4. Instituto de Astronomía, UNAM, Mexico

Why is this important to scientists, and why is it important to you as a teacher or parent of a child who wants to know how many planets there are?

Dwarf Planets. Defining Dwarf Planets

Matt A. Wood, Professor Dept. of Physics & Space Sciences Florida Institute of Technology

28-Aug-17. A Tour of Our Solar System and Beyond. The Sun

1/13/16. Solar System Formation

outline 1. in the beginning. The Big Bang 2. galaxies -- different types 3. stars -- life cycle 4. the solar system -- sun and planets

Introduction to the Universe. What makes up the Universe?

Phys 214. Planets and Life

Lecture Outlines. Chapter 6. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

Does it matter what you call an object? Does the public care so much? Were scientists made fun of, but not HP Computer Company?

Young Solar-like Systems

Our Solar System and Its Place in the Universe

LESSON topic: formation of the solar system Solar system formation Star formation Models of the solar system Planets in our solar system

Across the Universe. By Gabrielle Sierra

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am

The Solar System. Name Test Date Hour

The Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour

Search for Extra-Terrestrial Intelligence

Habitability Outside the Solar System. A discussion of Bennett & Shostak Chapter 11 HNRS 228 Dr. H. Geller

Lecture 12: Extrasolar planets. Astronomy 111 Monday October 9, 2017

Introduction to the Universe

TABLE OF CONTENTS. click one to go to that page, or just go on. What is the Solar System? Neptune (Pluto) The Sun. Asteroids. Mercury.

Astro-2: History of the Universe

Astronomy 330 HW 2. Outline. Presentations. ! Alex Bara

Solar System Test Review

You are here! The Solar System! Jo-Anne Brown

Unit 12 Lesson 1 What Objects Are Part of the Solar System?

Occam s Razor: William of Occam, 1340(!)

Extrasolar Planets. Today. Dwarf Planets. Extrasolar Planets. Next week. Review Tuesday. Exam Thursday. also, Homework 6 Due

Extrasolar planets. Lecture 23, 4/22/14

Astronomy 330 HW 2. Outline. Presentations. ! Kira Bonk ascension.html

Our Solar System. Lesson 5. Distances Between the Sun and the Planets

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC

Sol o ar a r S yste t m e F o F r o m r at a i t on o The Ne N b e u b l u a a Hypothesis

Planets Beyond our Solar System: The New Astronomical Revolution

What is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1

Chapter 15: The Origin of the Solar System

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

Space Test Review. Unit Test on Thursday April 17

Searching for Other Worlds

The Observer November 2006 (#6)

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999

What s in Our Solar System?

known since prehistoric times almost 10 times larger than Jupiter

The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller.

Charles Keeton. Principles of Astrophysics. Using Gravity and Stellar Physics. to Explore the Cosmos. ^ Springer

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

1. Galaxy (a) the length of a planet s day. 2. Rotational Period (b) dust and gases floating in space

Lecture Outlines. Chapter 15. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

Planets in other Star Systems

Astronomy 1140 Quiz 4 Review

The Trouble with 'Planets'

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

Earth in the Universe Unit Notes

Honors 228 Astrobiology w/ Dr. H. Geller Meeting #2 - Physical Origins. Presented 21 January 2010

Plan. Questions? Syllabus; administrative details. Some Definitions. An Idea of Scale

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

Chapter 06 Let s Make a Solar System

II Planet Finding.

Astronomy: Exploring the Universe

Announce/Remind. Reading: Section 6.1, 6.2 for today. Adjusted Exam 1 Grades + buy-back results on course Grades tab. 569 points bought back!

Beyond the Book. FOCUS Book

9.2 - Our Solar System

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

Lecture 3: Chapter 1- Charting the Heavens. Assignment: Read Chapter 1 of Astronomy Today

The formation & evolution of solar systems

Astronomy: Exploring the Universe

Cosmology Vocabulary

Astronomy 210 Midterm #2

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company

Lecture Outlines. Chapter 15. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

AST 248. Is Pluto a Planet?

Extrasolar Planets. Materials Light source to mimic star Ball to mimic planet Light meter Interface

Our Solar System. Dr. G. M. Ballabh THE SOLAR FAMILY. Many many satellites of the planets. Many Comets and asteroids

The Solar System - I. Alexei Gilchrist. [The Story of the Solar System]

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..

The Universe and Galaxies

Universe Celestial Object Galaxy Solar System

5. How did Copernicus s model solve the problem of some planets moving backwards?

AST 105. Overview of the Solar System

1. Cosmology is the study of. a. The sun is the center of the Universe. b. The Earth is the center of the Universe

Final Exam. Sample Questions. Final Exam. Which of the following statement is true? THE FINAL IS DECEMBER 15 th : 7-10pm!

PTYS/ASTR 206 Section 2 Spring 2007 Homework #6 (Page 1/4) NAME: KEY

PLANETARY SYSTEM: FROM GALILEO TO EXOPLANETS

What is the Solar System?

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Astronomy Today. Eighth edition. Eric Chaisson Steve McMillan

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects.

The Moon s relationship with Earth The formation of the Moon The surface of the Moon Phases of the Moon Travelling to the Moon

Which of the following correctly describes the meaning of albedo?

Where in the Solar System Are Smaller Objects Found?

Our Planetary System. Chapter 7

Cosmology Overview (so far): Cosmology Overview (so far): The Age of the Universe. The Big Bang. The Age of the Universe

Transcription:

Origins Lecture 9; April 29 2014

Previously on Origins Demarcation: what is science? Falsification: how do you test scientific theories?

Today on Origins Repeatibility: science and the supernatural Corroboration: what is a good scientific theory Is Earth a special/unique place?

Physical cosmology Experiments and Observations force us to modify/change our view of the Universe. Examples: Galileo s observations of Sun spots proved that the heavens are not time-invariant Hubble s measurement of galaxy redshifts showed that the Universe is not static High speed motions of stars in galaxies show that either we do not understand gravity or there is a large amount of dark matter, i.e. different stuff that the ones that makes you and me (and Earth)

Tools of the trade: Telescopes as time machines

Physical cosmology: a fundamental dilemma Experiments and observations can only be from one point in space and time: Earth now. Yet we would like to construct a scientific theory that describes the universe everywhere and at all times.

and its solution Hypothesis: our local sample of the universe is no different from more remote and inaccessible places This assumption is deeply rooted in two fundamental principles of physics: The laws of physics (whatever they are!) do not depend on space and time. Popper calls it the principle of the uniformity of nature Physical explanations of natural phenomena should be as simple as possible (Ockham s razor)

A testable working solution We can measure whether we are in anyway in a special place in the Universe. We will discuss this at length in this class We can test the laws of physics through observations. Examples: Spectroscopy of distant stars and galaxies to probe atomic physics. Do we see the same transitions? Constants of nature (such as the electron charge). Where they different a few billion years ago?

There are plenty of phenomena we do not understand. Example: How does your cell-phone work? However, they are measurable phenomena with repeatable experiments Technology may appear magic or myth but it IS FUNDAMENTALLY NOT Unexplained

vs magic/miracles Magic and miracles imply a behavior that differs than expected - i.e. NON REPEATABLE If miracles were proven to exist, this would falsify one of the fundamental hypothesis of science, that is that the laws of nature do not bend to people s or (deity s) will. SCIENTIFIC EVIDENCE OF MAGIC/MIRACLE WOULD BE MOST REVOLUTIONARY AND TRANSFORMATIVE

A good scientific theory What constitutes a good scientific theory? If a theory can never be proven right, how is one theory better than another? Note the use of the derogatory expression just a theory by creationists According to Popper: The better theory is the one that passes more stringent tests, both in number and in quality The better theory is the more falsifiable one, if it doesn t fail Old theories often become limiting cases of new theories (e.g. Newton vs Einstein)

How about validating the method? What constitutes a good method? Is the scientific method good? Does the question even make sense? My view is that a method is good as long as it allows you to achieve what you want. What do you want? The scientific method answers some questions/obtain some results. What are they? If we need to answer other questions we need different tools.

Outline: Is Earth a special/unique place? Extrasolar planets Techniques State of the art Limitations Habitable Planets Selection effects Extraterrestrial life Drake s Equation

A physicist s answer We phrase the question in statistical terms: How frequent are planets like the Earth? In other words, is Earth unique? Let s take a look! Let s measure!

But before looking at exoplanets The question can be rephrased in statistical terms: How frequent are planets like the Earth? Let s take a look! Let s measure! How many planets does our solar system have? What is a planet?

2006 IAU RESOLUTION B5: Definition of a Planet in the Solar System Contemporary observations are changing our understanding of planetary systems, and it is important that our nomenclature for objects reflect our current understanding. This applies, in particular, to the designation "planets". The word "planet" originally described "wanderers" that were known only as moving lights in the sky. Recent discoveries lead us to create a new definition, which we can make using currently available scientific information.

2006 IAU RESOLUTION B5: Definition of a Planet in the Solar System The IAU therefore resolves that planets and other bodies, except satellites, in our Solar System be defined into three distinct categories in the following way: (1) A planet is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighborhood around its orbit. (2) A "dwarf planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape2, (c) has not cleared the neighborhood around its orbit, and (d) is not a satellite.

2006 IAU RESOLUTION B5: Definition of a Planet in the Solar System The IAU therefore resolves that planets and other bodies, except satellites, in our Solar System be defined into three distinct categories in the following way: (3) All other objects,except satellites, orbiting the Sun shall be referred to collectively as "Small Solar System Bodies". Notes: The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. An IAU process will be established to assign borderline objects to the dwarf planet or to another category. Class 3 currently includes most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs),comets, and other small bodies.

2006 IAU RESOLUTION B6: Pluto The IAU further resolves: Pluto is a "dwarf planet" by the above definition and is recognized as the prototype of a new category of Trans- Neptunian Objects. An IAU process will be established to select a name for this category.

Extrasolar planets A minimalist definition. Celestial body that is: Gravitationally bound to a star No nuclear fusion How do we find them? As of today Radial velocities: 507 Transit: 302 Microlensing: 18 Direct Imaging: 30 Timing: 16 (not discussed here) http://exoplanet.eu/

Radial Velocities Very difficult measurement! Speed <m/s. Orbital inclination

Mercury s 2006 transit as imaged by NASA satellite Soho Planet Transit

Extrasolar Planets Transit

Planet Transit: Kepler Launched 3/6/9; first light 4/8/9; expect ~50 Earths

Kepler s new planets

The amazing system Kepler 11

The amazing system Kepler 11

The amazing system Kepler 11

Microlensing

Direct Imaging

Summary of findings 5-10% of stars surveyed show planets. Fraction increases with abundance of heavy elements Check out http://exoplanet.eu

Planet Hunting in Santa Barbara

Limitations. Selection effects Most methods depend on ratio of properties of star and planet. Small planets are hard to find! Mass ratio (wobble) Luminosity ratio (direct detection) Radius ratio (transit) And on orbital properties. Small orbits are easier to find. We have only surveyed for 10 years, it s hard to find long periods

Future prospects

When is a planet habitable? For humans: Liquid Water? (distance from star) Gravity? (mass range) Atmosphere? Rocky? (mass range) Shielded by meteors? Stable orbit? For other forms of life? Very difficult to say Habitable planets

A habitable planet? Mass similar to Earth Liquid water on the surface movie

Extraterrestrial life: how many? Check out: http://www.pbs.org/lifebeyondearth/listening/drake.html

Crude estimates R*~1/yr (large stars are too fast ; small stars are too cold ) fp~1 (most sun-like stars probably have planets) Ne? 1 like our own? fl~1? Life arose very fast on Earth fi? 1 fc? 1 L? >100yr =>N=10? More in section If you are interested, read article by Bounama et al. posted on the web site describing more sophisticated models. According to their model, complex life is common enough that there is a chance to detect life in the atmosphere of a planet within the next decades!

Summary: Is Earth a special/unique place? What does the question mean? How do we find planets? What are habitable planets? Selection effects Is there extraterrestrial life? Drake s Equation

The End See you on Thursday!