How He Did It #1: The Big Bang and Creative Destruction

Size: px
Start display at page:

Download "How He Did It #1: The Big Bang and Creative Destruction"

Transcription

1 How He Did It #1: The Big Bang and Creative Destruction Photo: N. Smith, University of California David Siegrist, Ph.D. Wrestlers March 29, 2015 David W. Siegrist Material may not be reproduced except with proper attribution and for personal/educational but non-commercial purposes. No derivatives.

2 The Big Bang and Creative Destruction (H/t to J. Schumpeter) Usually, we expect to blow up Something, and get Nothing. Nothing but ash and trash. In the Big Bang, Nothing is said to have exploded into Something. And that Something grew exponentially and engendered life, among many other things. Materialists say that was the result of chance. However, a universe in which Nothing grows into Something is hardly the result of chance, and needs to be explained. I believe that a theistic explanation is much more realistic than chance. In a universe where everything is winding down after the Big Bang, why does complexity build up, e.g., stars, planets, life? More consistent with a Creator and a Purpose.

3 Sir Arthur Eddington on Entropy as a Central Narrative of the Universe Energy can be dissipated so that it can no longer do useful work. That dissipation is known as entropy. The law that entropy always increases holds I think the supreme position among the laws of nature. If someone points out to you that your pet theory is in disagreement with Maxwell s equations, then so much the worse for Maxwell s equations. If it is found to be contradicted by observation, well these experimentalists do bungle things sometimes. But if your theory is found to be against the 2d Law of Thermodynamics, I can give you no hope; there is nothing for it but to collapse in deepest humiliation.

4 Entropy At the beginning, the universe had high energy and order. (All the four forces were unified, for instance). Hence: Low entropy. The narrative of the universe may appear to be one of expansion and cooling, gradually running down over time and becoming more disordered. Leading to eventual heat death as energy dissipates. However, we find structure in the universe as well, some of it quite fine-grained. How can we account for that complexity? Has entropy (codified in the 2d Law of Thermodynamics) been violated?

5 Entropy Loophole Entropy can actually decrease in a local area, provided that overall entropy continues to increase in its larger environment. For instance, the earth uses radiation from the sun to do useful work. Entropy decreases where order is created, say by growing a plant. However, in the wider system, entropy is still created at a greater rate. The useful work of growing the plant is outpaced by the waste heat generated in that process. Entropy example: The drive to Pittsburgh, in which the gasoline used has an amount of stored energy, some of which provides the actual motive power to travel ( Useful work ), while the majority of the gasoline s energy is dissipated as waste heat ( Entropy ) out the tailpipe. We will discuss creating complexity and entropy further later, but first we need to cover why there is something rather than nothing.

6 There has to be Something before there can be Complex Structure As we know from E=Mc2, matter may be seen as a congealed form of energy. As the universe expanded and cooled, matter precipitated out of the primordial dense radiation. Created a particle zoo. Quarks combined to became protons and neutrons. With electrons, they become atoms. Atoms form everything that we experience as matter. Why energy should form matter is not well known. Humans can create particles in atom smashers.

7 A Funny Thing about Creating Through a Big Bang To build physical complexity, one needs basic stuff as well as energy to do the work to make that stuff more interesting. A Big Bang is a natural heat engine. A heat engine works by higher energy material passing from one area to disperse in an area of lower energy (heat). The universe is a heat engine. It has a overall heat of 2.7 degrees above absolute zero left over from the Big Bang. The sun acts as a heat engine, warming the earth and preforming useful work here. Starting through a Big Bang is conducive to the universe accumulating complexity because it builds in an energy source to do work, as well as providing a heat sink to dissipate the energy. Energy moving from the source to the sink can do useful work. WMAP image of the cosmos

8 The Large Scale Structure of the Universe Formed from the Big Bang (Largely drawn from Cosmic Evolution). Vast gas clouds spread as the universe expanded and cooled. Quarks and electrons formed Hydrogen and Helium. Inhomogeneities led to the clustering of some of these clouds. In some of these clusters, the gas infell on itself due to gravitational attraction. Large amounts of gas infalling leads to large, dense structures that have tremendous heat and pressure in the center. If heat and pressure are sufficient, these large structures start to fuse their inner Hydrogen into heavier elements. This nuclear fusion throws off a tremendous amount of energy as a star.

9 Further Creation of Large Structure Due to Physics As very large stars consume all their hydrogen, they start to fuse other lighter elements into heavier ones. When their fuel ultimately runs out, these large stars may collapse and then explode in Supernovas. These spread the heavier elements into space. Clouds of space dust may form into planets due to gravitational forces. These planets may orbit next generation stars, also due to gravity. The heavy elements enable the planets to support life, among other interesting things. Images from Wikipedia

10 More about those Particles of Matter What is all that cosmic structure made of? Recall that matter coalesced out of the primordial energy released at the Beginning of time. Matter is made up of atoms. Atoms are made of protons, neutrons, and electrons. Protons and neutrons are made of two types of Quarks. They are Bound so tightly that labs don't find single quarks.

11 Matter is Also Not all that Solid In an atom, the nucleus is to the electron cloud as a fly is to a stadium. What we experience as solid is mostly extremely thinly filled space. (The space is filled by the electron wave). The solidity illusion is created by electromagnetic charge s repulsion of like charges, among other factors. How the indeterminate quantum world turns into our classical macro view of physics, with touchable objects that we can experience and make sense of, needs to be explained by naturalists since its not needed physically. Copenhagen Interpretation of Quantum Mechanics that QM world should not be thought of with classical physics concepts. Not: Is it Really a wave or a particle? 1. Macroscopic level - Matter 2. Molecular level. 3. Atomic level. 4. Subatomic level - Electron 5. Subatomic level - Quarks 6. String level

12 Quarks Bond into Stable Structure Due to a Mysterious Charge There are two main kinds of quarks. They bind together due to color charge. The color charge binds quarks so tightly (through the exchange of gluons ) that single quarks are never found by themselves. Quarks make up protons and neutrons. Protons are one of the few stable particles. They don t decay. Neutrons decay if they are outside the nucleus. Protons and neutrons stay together in atoms due to this strong force. (1 of only 4 forces that we know of). Protons and nuclei are a critical part of structure of the universe. Naturalists need to account for the strong force and color charge, inter alia, just happening. A proton, composed of two up quarks and one down quark.

13 At a Basic Level, Matter Itself Isn t all that Straightforward Subatomic particles have a property known as spin. (This isn t actually spin as we know it, but a special intrinsic property that can be up or down ). 1/2 spin particles rotate 720 degrees back to original. Spin can be measured by scientists in magnetic fields. Matter (Fermions) have fractional spin, e.g., 1/2, 3/2. Energy carriers (Bosons) have integer spin, e.g., 1, 2. (Matter particles can t be in the same quantum state. Bosons like photons can actually prefer to share the same space/state with each other, such as with lasers.) Besides spin, matter and energy carriers are very similar. Something we should remember if we ask how God, who transcends time and space, can create material things. After a 360 degree rotation, the spiral flips between clockwise and counterclockwise orientations. It returns to its original configuration after spinning a full 720 degrees. "Spin One- Half (Slow)" by Jason Hise, Wikimedia.

14 Matter is Made of Atoms There are about 100 kinds of atoms. Each atom has a different number of protons in its nucleus. (Elements with more protons than 92 are unstable). Each atom has an equal number of protons (positive) and electrons (negative charge). Atoms are electrically neutral. Atoms have a tiny but dense, positive nucleus and a cloud of negative electrons (e - ). Atoms can be categorized into groups that share similar chemical properties (as in the Periodic Table).

15 Outer Electron Shells Obey the Duet, Octet, and 18 Rules 18 The bonding in carbon dioxide (CO2): all atoms are surrounded by 8 electrons. Atoms are a bit like the letters in the alphabet from which words (recognizable materials) are made. Atoms bind with each other based on the number of electrons in their outer shell. Atoms bind together in molecules. (Millions of different kinds). Molecular properties are different from those of the constituent atoms. Atoms want to have a completed outer ring. (Energy advantage- PW Atkins). A basic source of structure in the world. Everything around us. Electrons don t collapse in on the nucleus, despite its opposite electrical charge, due to the Pauli Exclusion Principle and Quantum Mechanics.

16 Atoms have Different Properties Depending on the Number of Electrons in their Outer Shell

17 Kind of like Atoms want to plug in to other appropriate atoms to fill both their outer electron rings. Bosons bond the fermions/matter together. The atom lego bricks combine to build molecular structures of great diversity, complexity and richness. The stuff and forces of the universe seem to lend themselves to achieving variety and complexity. Very conducive to a central narrative of building up complexity with the aid of an energy source. It could have been different. (But we wouldn t be here).

18 The Way Atoms Bind Together in Molecules Drives Their Structure (from PW Atkins, What is Chemistry?) Ionic Bonding: If atoms borrow or lend an electron, the atoms (now ions) become electromagnetically attracted to each other They cling together and form solids. Covalent bonds share electrons between the atoms. The molecules can be independent and form gases. Metallic bonds. Metal atoms share their excess electrons, making the metals malleable, strong, and good conductors of electricity.

19 Something about Carbon Carbon absorbs energy from the sun extremely well and resonate. Carbon forms rings that are stable when they resonate. Carbon rings tend to pi stack in offset layers due to electric charge. The pattern is found in DNA.

20 Carbon Is a Key to Chemistry Carbon can bind to itself & form chains. These backbones can be soluble. Great examples: Petroleum, plastics, DNA, proteins... In living things, simple monomers are linked to form larger polymers, made up of repetitive sequences of monomer sub-units. Amino acids are linked to form proteins. Simple carbohydrates polymerize to form complex sugars and starches. Fatty acids make up lipids, and Nucleotides link to form nucleic acids such as RNA and DNA. (Taggart, UM)

21 Atoms are Just a Small Part of the Stuff of the Universe Dark energy and matter aren't well understood. Dark matter has a gravitational affect on the rotation of galaxies. Dark energy pervades space, and has an anti-gravitational impact. All the matter that we know is basically a small contamination of the mass-energy that makes up the universe. All that other mass-energy does not support the construction of complexity as we know it. Dark particles interact weakly, and so are hardly suitable for building complexity. A further cosmic process was needed to create regular matter in this universe that we could comprehend/be part of. That further suggests to me the unlikelihood that the universe we know happened just by chance, because it would have been simpler to have a less complicated universe.

22 Conclusion A central tendency in the universe is to build up complexity locally whole dissipating energy globally. Creating the universe through a Big Bang supplies a continuing energy source that sometimes builds complexity. The world manifests itself in a way that is not just natural, but has many aspects that require further explanation. E.g., mass equates to energy; ill-understood spin makes something matter instead of energy; the classical structure we see is very different from the quantum underpinnings (e.g., wavicles instead of particles, etc.); and is based on things that are smaller and more ephemeral than they appear; etc. Occam s Razor would suggest that the universe, already so mightily improbable, would not be more complicated than it needs to be. To me, these unusual characteristics would be supportive of a purpose to the universe. That is, to create that structure intentionally, presumably for the enjoyment of the Creator, rather than through random chance. In coming weeks, I plan to show how this central tendency to build complexity is further borne out in the world. Having a Creator is very compatible with science s discoveries. Coincidence is not.

Chapter 32 Lecture Notes

Chapter 32 Lecture Notes Chapter 32 Lecture Notes Physics 2424 - Strauss Formulas: mc 2 hc/2πd 1. INTRODUCTION What are the most fundamental particles and what are the most fundamental forces that make up the universe? For a brick

More information

The Big Bang Theory, General Timeline. The Planck Era. (Big Bang To 10^-35 Seconds) Inflationary Model Added. (10^-35 to 10^-33 Of A Second)

The Big Bang Theory, General Timeline. The Planck Era. (Big Bang To 10^-35 Seconds) Inflationary Model Added. (10^-35 to 10^-33 Of A Second) The Big Bang Theory, General Timeline The Planck Era. (Big Bang To 10^-35 Seconds) The time from the exact moment of the Big Bang until 10^-35 of a second later is referred to as the Planck Era. While

More information

Chapter 22: Cosmology - Back to the Beginning of Time

Chapter 22: Cosmology - Back to the Beginning of Time Chapter 22: Cosmology - Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Future of universe depends on the total amount of dark and normal matter Amount of matter

More information

Chapter 5 Newton s Universe

Chapter 5 Newton s Universe Chapter 5 Newton s Universe Lecture notes about gravitation Dr. Armen Kocharian Units of Chapter 5 The Idea of Gravity: The Apple and the Moon The Law of Gravity: Moving the Farthest Star Gravitational

More information

Announcement. Station #2 Stars. The Laws of Physics for Elementary Particles. Lecture 9 Basic Physics

Announcement. Station #2 Stars. The Laws of Physics for Elementary Particles. Lecture 9 Basic Physics Announcement Pick up your quiz after this lecture as you leave the lecture hall. Homework#2 due on Thursday No hand-written homework! Please staple them! Put it in the box before the lecture begins! Station

More information

Particles and Forces

Particles and Forces Particles and Forces Particles Spin Before I get into the different types of particle there's a bit more back story you need. All particles can spin, like the earth on its axis, however it would be possible

More information

Introduction to Cosmology Big Bang-Big Crunch-Dark Matter-Dark Energy The Story of Our Universe. Dr. Ugur GUVEN Aerospace Engineer / Space Scientist

Introduction to Cosmology Big Bang-Big Crunch-Dark Matter-Dark Energy The Story of Our Universe. Dr. Ugur GUVEN Aerospace Engineer / Space Scientist Introduction to Cosmology Big Bang-Big Crunch-Dark Matter-Dark Energy The Story of Our Universe Dr. Ugur GUVEN Aerospace Engineer / Space Scientist The Age of the Universe Through various measurements

More information

The Contents of the Universe (or/ what do we mean by dark matter and dark energy?)

The Contents of the Universe (or/ what do we mean by dark matter and dark energy?) The Contents of the Universe (or/ what do we mean by dark matter and dark energy?) Unseen Influences Dark Matter: An undetected form of mass that emits little or no light but whose existence we infer from

More information

PHL424: 4 fundamental forces in nature

PHL424: 4 fundamental forces in nature PHL424: 4 fundamental forces in nature The familiar force of gravity pulls you down into your seat, toward the Earth's center. You feel it as your weight. Why don't you fall through your seat? Well, another

More information

Particles in the Early Universe

Particles in the Early Universe Particles in the Early Universe David Morrissey Saturday Morning Physics, October 16, 2010 Using Little Stuff to Explain Big Stuff David Morrissey Saturday Morning Physics, October 16, 2010 Can we explain

More information

FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! QUARKS! FERMIONS! Gauge Bosons! Fermions! Strange and Charm! Top and Bottom! Up and Down!

FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! QUARKS! FERMIONS! Gauge Bosons! Fermions! Strange and Charm! Top and Bottom! Up and Down! FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! --Bosons are generally associated with radiation and are sometimes! characterized as force carrier particles.! Quarks! Fermions! Leptons! (protons, neutrons)!

More information

Stellar Evolution: Outline

Stellar Evolution: Outline Stellar Evolution: Outline Interstellar Medium (dust) Hydrogen and Helium Small amounts of Carbon Dioxide (makes it easier to detect) Massive amounts of material between 100,000 and 10,000,000 solar masses

More information

Chapter 22 Back to the Beginning of Time

Chapter 22 Back to the Beginning of Time Chapter 22 Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Back to the Big Bang The early Universe was both dense and hot. Equivalent mass density of radiation (E=mc

More information

Forces and Nuclear Processes

Forces and Nuclear Processes Forces and Nuclear Processes To understand how stars generate the enormous amounts of light they produce will require us to delve into a wee bit of physics. First we will examine the forces that act at

More information

Chapter 33 The History of a Star. Introduction. Radio telescopes allow us to look into the center of the galaxy. The milky way

Chapter 33 The History of a Star. Introduction. Radio telescopes allow us to look into the center of the galaxy. The milky way Chapter 33 The History of a Star Introduction Did you read chapter 33 before coming to class? A. Yes B. No You can see about 10,000 stars with the naked eye. The milky way Radio telescopes allow us to

More information

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES Q1. The figure below shows what scientists over 1000 years ago thought the solar system was like. Give one way that the historical model of the solar

More information

1. Four different processes are described in List A. The names of these processes are given in List B.

1. Four different processes are described in List A. The names of these processes are given in List B. Nuclear fission and nuclear fusion 1. Four different processes are described in List A. The names of these processes are given in List B. Draw a line to link each description in List A to its correct name

More information

LIVING IN THE ENVIRONMENT 17 TH

LIVING IN THE ENVIRONMENT 17 TH MILLER/SPOOLMAN LIVING IN THE ENVIRONMENT 17 TH CHAPTER 2 Science, Matter, Energy, and Systems Core Case Study: A Story About a Forest Hubbard Brook Experimental Forest in New Hampshire Compared the loss

More information

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass.

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass. The Four Fundamental Forces What are the four fundamental forces? The Four Fundamental Forces What are the four fundamental forces? Weaker Stronger Gravitational, Electromagnetic, Strong and Weak Nuclear

More information

1. What does this poster contain?

1. What does this poster contain? This poster presents the elementary constituents of matter (the particles) and their interactions, the latter having other particles as intermediaries. These elementary particles are point-like and have

More information

ORIGIN OF THE ELEMENETS

ORIGIN OF THE ELEMENETS VISUAL PHYSICS ONLINE ORIGIN OF THE ELEMENETS Watch Video: The Origin of the Elements The ordinary matter in our universe (known as baryonic matter) is made up of 94 naturally occurring elements. It is

More information

32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES

32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32.1 Biological Effects of Ionizing Radiation γ-rays (high-energy photons) can penetrate almost anything, but do comparatively little damage.

More information

THE STANDARD MODEL OF MATTER

THE STANDARD MODEL OF MATTER VISUAL PHYSICS ONLINE THE STANDARD MODEL OF MATTER The "Standard Model" of subatomic and sub nuclear physics is an intricate, complex and often subtle thing and a complete study of it is beyond the scope

More information

Gravity simplest. fusion

Gravity simplest. fusion Gravity simplest fusion The life of a star has a complex relationship with gravity: 1. Gravity is what brings the original dust together to make a star 2. Gravity wants to crush the star Gravity pulls

More information

Outline - March 18, H-R Diagram Review. Protostar to Main Sequence Star. Midterm Exam #2 Tuesday, March 23

Outline - March 18, H-R Diagram Review. Protostar to Main Sequence Star. Midterm Exam #2 Tuesday, March 23 Midterm Exam #2 Tuesday, March 23 Outline - March 18, 2010 Closed book Will cover Lecture 8 (Special Relativity) through Lecture 14 (Star Formation) only If a topic is in the book, but was not covered

More information

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars Classifying Stars In the early 1900s, Ejnar Hertzsprung and Henry Russell made some important observations. They noticed that, in general, stars with higher temperatures also have brighter absolute magnitudes.

More information

Relative Sizes of Stars. Today Exam#3 Review. Hertzsprung-Russell Diagram. Blackbody Radiation

Relative Sizes of Stars. Today Exam#3 Review. Hertzsprung-Russell Diagram. Blackbody Radiation Today Exam#3 Review Exam #3 is Thursday April 4th in this room, BPS 40; Extra credit is due 8:00 am Tuesday April 9 Final Exam is 3:00pm Monday April 8 in BPS 40 The exam is 40 multiple choice questions.

More information

Directed Reading A. Section: The Life Cycle of Stars TYPES OF STARS THE LIFE CYCLE OF SUNLIKE STARS A TOOL FOR STUDYING STARS.

Directed Reading A. Section: The Life Cycle of Stars TYPES OF STARS THE LIFE CYCLE OF SUNLIKE STARS A TOOL FOR STUDYING STARS. Skills Worksheet Directed Reading A Section: The Life Cycle of Stars TYPES OF STARS (pp. 444 449) 1. Besides by mass, size, brightness, color, temperature, and composition, how are stars classified? a.

More information

The Formation of the Solar System

The Formation of the Solar System Earth and the Solar System The Formation of the Solar System Write a number beside each picture to rank each from the oldest (1) to the youngest (4). The universe includes everything that exists: all matter,

More information

Introduction to the Standard Model of elementary particle physics

Introduction to the Standard Model of elementary particle physics Introduction to the Standard Model of elementary particle physics Anders Ryd (Anders.Ryd@cornell.edu) May 31, 2011 Abstract This short compendium will try to explain our current understanding of the microscopic

More information

Homework 6 Name: Due Date: June 9, 2008

Homework 6 Name: Due Date: June 9, 2008 Homework 6 Name: Due Date: June 9, 2008 1. Where in the universe does the general expansion occur? A) everywhere in the universe, including our local space upon Earth, the solar system, our galaxy and

More information

2 Energy from the Nucleus

2 Energy from the Nucleus CHAPTER 4 2 Energy from the Nucleus SECTION Atomic Energy BEFORE YOU READ After you read this section, you should be able to answer these questions: What is nuclear fission? What is nuclear fusion? What

More information

Stellar processes, nucleosynthesis OUTLINE

Stellar processes, nucleosynthesis OUTLINE Stellar processes, nucleosynthesis OUTLINE Reading this week: White 313-326 and 421-464 Today 1. Stellar processes 2. Nucleosynthesis Powerpoint credit: Using significant parts of a WHOI ppt 1 Question

More information

THE NUCLEUS: A CHEMIST S VIEW Chapter 20

THE NUCLEUS: A CHEMIST S VIEW Chapter 20 THE NUCLEUS: A CHEMIST S VIEW Chapter 20 "For a long time I have considered even the craziest ideas about [the] atom[ic] nucleus... and suddenly discovered the truth." [shell model of the nucleus]. Maria

More information

Preview. Subatomic Physics Section 1. Section 1 The Nucleus. Section 2 Nuclear Decay. Section 3 Nuclear Reactions. Section 4 Particle Physics

Preview. Subatomic Physics Section 1. Section 1 The Nucleus. Section 2 Nuclear Decay. Section 3 Nuclear Reactions. Section 4 Particle Physics Subatomic Physics Section 1 Preview Section 1 The Nucleus Section 2 Nuclear Decay Section 3 Nuclear Reactions Section 4 Particle Physics Subatomic Physics Section 1 TEKS The student is expected to: 5A

More information

Review: HR Diagram. Label A, B, C respectively

Review: HR Diagram. Label A, B, C respectively Stellar Evolution Review: HR Diagram Label A, B, C respectively A C B a) A: White dwarfs, B: Giants, C: Main sequence b) A: Main sequence, B: Giants, C: White dwarfs c) A: Main sequence, B: White Dwarfs,

More information

Outline: Cosmological Origins. The true basics of life The age of Earth and the Universe The origin of the heavy elements Molecules in space

Outline: Cosmological Origins. The true basics of life The age of Earth and the Universe The origin of the heavy elements Molecules in space Outline: Cosmological Origins The true basics of life The age of Earth and the Universe The origin of the heavy elements Molecules in space Reminder: HW #1 due in one week Homework is on class webpage

More information

Life and Death of a Star. Chapters 20 and 21

Life and Death of a Star. Chapters 20 and 21 Life and Death of a Star Chapters 20 and 21 90 % of a stars life Most stars spend most of their lives on the main sequence. A star like the Sun, for example, after spending a few tens of millions of years

More information

Learning Outcomes 2. Key Concepts 2. Misconceptions and Teaching Challenges 3. Vocabulary 4. Lesson and Content Overview 5

Learning Outcomes 2. Key Concepts 2. Misconceptions and Teaching Challenges 3. Vocabulary 4. Lesson and Content Overview 5 UNIT 3 GUIDE Table of Contents Learning Outcomes 2 Key Concepts 2 Misconceptions and Teaching Challenges 3 Vocabulary 4 Lesson and Content Overview 5 BIG HISTORY PROJECT / UNIT 3 GUIDE 1 Unit 3 Stars and

More information

What is the solar system?

What is the solar system? Notes Astronomy What is the solar system? 11.1 Structure of the Solar System Our solar system includes planets and dwarf planets, their moons, a star called the Sun, asteroids and comets. Planets, dwarf

More information

PHYSICS 107. Lecture 27 What s Next?

PHYSICS 107. Lecture 27 What s Next? PHYSICS 107 Lecture 27 What s Next? The origin of the elements Apart from the expansion of the universe and the cosmic microwave background radiation, the Big Bang theory makes another important set of

More information

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe The Big Bang Theory The Big Bang Theory The Big Bang Theory is the most widely accepted scientific explanation

More information

The expansion of the Universe, and the big bang

The expansion of the Universe, and the big bang The expansion of the Universe, and the big bang Q: What is Hubble s law? A. The larger the galaxy, the faster it is moving way from us. B. The farther away the galaxy, the faster it is moving away from

More information

21/11/ /11/2017 Space Physics AQA Physics topic 8

21/11/ /11/2017 Space Physics AQA Physics topic 8 Space Physics AQA Physics topic 8 8.1 Solar System, Orbits and Satellites The eight planets of our Solar System Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune As well as the eight planets, the

More information

Daily Science 03/30/2017

Daily Science 03/30/2017 Daily Science 03/30/2017 The atmospheres of different planets contain different gases. Which planet is most likely Earth? a. planet 1 b. planet 2 c. planet 3 d. planet 4 KeslerScience.com Can you name

More information

The heavens declare the glory of God; and the firmament sheweth his handiwork. Psalm 19:1

The heavens declare the glory of God; and the firmament sheweth his handiwork. Psalm 19:1 The heavens declare the glory of God; and the firmament sheweth his handiwork. Psalm 19:1 If you look up at the sky at night, the heavens appear to be unchanging. In 1917 Einstein wrote down the theory

More information

and two neutrons. It is so improbable that four protons all happen to hit at once and two convert that this never happens. Instead, there is a

and two neutrons. It is so improbable that four protons all happen to hit at once and two convert that this never happens. Instead, there is a Last time we left off at hydrogen and helium, because that s all that formed for the first hundred million years of the universe except for dribbly little bits of lithium and beryllium. As this isn t enough

More information

UNIT 1: BIOCHEMISTRY

UNIT 1: BIOCHEMISTRY UNIT 1: BIOCHEMISTRY UNIT 1: Biochemistry Chapter 6.1: Chemistry of Life I. Atoms, Ions, and Molecules A. Living things consist of atoms of different elements 1. An atom is the smallest basic unit of matter

More information

ET: Astronomy 230 Section 1 MWF Astronomy Building. Outline. The Early Universe? HW1 due today!

ET: Astronomy 230 Section 1 MWF Astronomy Building. Outline. The Early Universe? HW1 due today! This Class (Lecture 5): From Atoms to Molecules to Clouds Next Class: Star Formation ET: Astronomy 230 Section 1 MWF 1400-1450 134 Astronomy Building HW1 due today! Outline What is life made of? We are

More information

Lecture 19: Building Atoms and Molecules

Lecture 19: Building Atoms and Molecules Lecture 19: Building Atoms and Molecules +e r n = 3 n = 2 n = 1 +e +e r y even Lecture 19, p 1 Today Nuclear Magnetic Resonance Using RF photons to drive transitions between nuclear spin orientations in

More information

Reading and Announcements. Read Chapter 14.1, 14.2 Homework #6 due Tuesday, March 26 Exam #2, Thursday, March 28

Reading and Announcements. Read Chapter 14.1, 14.2 Homework #6 due Tuesday, March 26 Exam #2, Thursday, March 28 Reading and Announcements Read Chapter 14.1, 14.2 Homework #6 due Tuesday, March 26 Exam #2, Thursday, March 28 The life of the Sun The Sun started as a cloud of gas. Gravity caused the cloud to collapse.

More information

Possible Extra Credit Option

Possible Extra Credit Option Possible Extra Credit Option Attend an advanced seminar on Astrophysics or Astronomy held by the Physics and Astronomy department. There are seminars held every 2:00 pm, Thursday, Room 190, Physics & Astronomy

More information

Life Cycle of a Star Worksheet

Life Cycle of a Star Worksheet Life Cycle of a Star Worksheet A STAR IS BORN STAGES COMMON TO ALL STARS All stars start as a nebula. A nebula is a large cloud of gas and dust. Gravity can pull some of the gas and dust in a nebula together.

More information

Name: Space Questions. Class: Date: Time: Marks: Comment s:

Name: Space Questions. Class: Date: Time: Marks: Comment s: Space 2 33 Questions Name: Class: Date: Time: Marks: Comment s: Q. Read the passage. In the SolarSystem, the inner planets, such as the Earth, contain elements which are eavierthan the elements hydrogen

More information

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following:

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following: Unit 3 The Universe Chapter 4 ~ The Formation of the Universe o Section 1 ~ The Scale of the Universe o Section 2 ~ The Formation of the Universe o Section 3 ~ The Future of the Universe Chapter 5 ~ Galaxies

More information

1 A Solar System Is Born

1 A Solar System Is Born CHAPTER 16 1 A Solar System Is Born SECTION Our Solar System California Science Standards 8.2.g, 8.4.b, 8.4.c, 8.4.d BEFORE YOU READ After you read this section, you should be able to answer these questions:

More information

GraspIT Questions AQA GCSE Physics Space physics

GraspIT Questions AQA GCSE Physics Space physics A. Solar system: stability of orbital motions; satellites (physics only) 1. Put these astronomical objects in order of size from largest to smallest. (3) Fill in the boxes in the correct order. the Moon

More information

LESSON 1. Solar System

LESSON 1. Solar System Astronomy Notes LESSON 1 Solar System 11.1 Structure of the Solar System axis of rotation period of rotation period of revolution ellipse astronomical unit What is the solar system? 11.1 Structure of the

More information

Before proceeding to Chapter 20 More on Cluster H-R diagrams: The key to the chronology of our Galaxy Below are two important HR diagrams:

Before proceeding to Chapter 20 More on Cluster H-R diagrams: The key to the chronology of our Galaxy Below are two important HR diagrams: Before proceeding to Chapter 20 More on Cluster H-R diagrams: The key to the chronology of our Galaxy Below are two important HR diagrams: 1. The evolution of a number of stars all formed at the same time

More information

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013 Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013 1 Matter Particles Quarks: Leptons: Anti-matter Particles Anti-quarks: Anti-leptons: Hadrons Stable bound states of quarks Baryons:

More information

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE Cosmology Cosmology is the study of the universe; its nature, origin and evolution. General Relativity is the mathematical basis of cosmology from which

More information

Earlier in time, all the matter must have been squeezed more tightly together and a lot hotter AT R=0 have the Big Bang

Earlier in time, all the matter must have been squeezed more tightly together and a lot hotter AT R=0 have the Big Bang Re-cap from last lecture Discovery of the CMB- logic From Hubble s observations, we know the Universe is expanding This can be understood theoretically in terms of solutions of GR equations Earlier in

More information

1. Star: A object made of gas found in outer space that radiates.

1. Star: A object made of gas found in outer space that radiates. 1. Star: A object made of gas found in outer space that radiates. 2. Stars produce extremely great quantities of energy through the process of. The chemical formula for nuclear fusion looks like this:

More information

Exam #3. Final Exam. Exam 3 review. How do we measure properties of a star? A detailed outline of study topics is here:

Exam #3. Final Exam. Exam 3 review. How do we measure properties of a star? A detailed outline of study topics is here: Exam #3 Exam #3 is Thursday 4/9 in this room You can bring page of notes (front and back) Bring your calculator and a # pencil Exam 3 covers material from 4/1 onward (only 8 lectures) Consequently, no

More information

Mr. Carpenter s Biology Biochemistry. Name Pd

Mr. Carpenter s Biology Biochemistry. Name Pd Mr. Carpenter s Biology Biochemistry Name Pd Chapter 2 Vocabulary Atom Element Compound Molecule Ion Cohesion Adhesion Solution Acid Base Carbohydrate Monosaccharide Lipid Protein Amino acid Nucleic acid

More information

Low mass stars. Sequence Star Giant. Red. Planetary Nebula. White Dwarf. Interstellar Cloud. White Dwarf. Interstellar Cloud. Planetary Nebula.

Low mass stars. Sequence Star Giant. Red. Planetary Nebula. White Dwarf. Interstellar Cloud. White Dwarf. Interstellar Cloud. Planetary Nebula. Low mass stars Interstellar Cloud Main Sequence Star Red Giant Planetary Nebula White Dwarf Interstellar Cloud Main Sequence Star Red Giant Planetary Nebula White Dwarf Low mass stars Interstellar Cloud

More information

Biology Chapter 2 The Chemistry of Life Mr. Hines

Biology Chapter 2 The Chemistry of Life Mr. Hines Biology Chapter 2 The Chemistry of Life Mr. Hines Chapter 2.1 The nature of Matter Learning Target 1 List and describe the four things in the universe and their relationship 2 Explain what matter is. 3

More information

Big Bang, Black Holes, No Math

Big Bang, Black Holes, No Math ASTR/PHYS 109 Dr. David Toback Lecture 33 1 Was due Today L33 Reading: (Unit 5) Pre-Lecture Reading Questions (PLRQ) Unit 5 Revision (if desired): Was due today before class End-of-Chapter Quizzes: Chapter

More information

Beyond the Solar System 2006 Oct 17 Page 1 of 5

Beyond the Solar System 2006 Oct 17 Page 1 of 5 I. Stars have color, brightness, mass, temperature and size. II. Distances to stars are measured using stellar parallax a. The further away, the less offset b. Parallax angles are extremely small c. Measured

More information

Universe Celestial Object Galaxy Solar System

Universe Celestial Object Galaxy Solar System ASTRONOMY Universe- Includes all known matter (everything). Celestial Object Any object outside or above Earth s atmosphere. Galaxy- A large group (billions) of stars (held together by gravity). Our galaxy

More information

Cosmology. What is Cosmology?

Cosmology. What is Cosmology? Cosmology What is Cosmology? The study of the structure and evolution of the entire universe The idea is to form picture of the entire Universe: origin, size, and future We will make assumptions that what

More information

Big Bang Theory How the Universe was Formed

Big Bang Theory How the Universe was Formed Big Bang Theory How the Universe was Formed Objectives Explain the Big Bang Theory. Give evidence to support the Big Bang Theory. Dispel misconceptions about the Big Bang Theory. Explain problems with

More information

ASTR 101 General Astronomy: Stars & Galaxies

ASTR 101 General Astronomy: Stars & Galaxies ASTR 101 General Astronomy: Stars & Galaxies ANNOUNCEMENTS MIDTERM III: Tuesday, Nov 24 th Midterm alternate day: Fri, Nov 20th, 11am, ESS 450 At LAST: In the very Beginning BIG BANG: beginning of Time

More information

1 The Life Cycle of a Star

1 The Life Cycle of a Star CHAPTER 1 The Life Cycle of a Star Describe the life cycle of various size stars. Rings of glowing gas encircling Supernova 1987A, about 179,000 light-years away in the Large Magellanic Cloud, one of the

More information

How to Build a Habitable Planet Summary. Chapter 1 The Setting

How to Build a Habitable Planet Summary. Chapter 1 The Setting How to Build a Habitable Planet Summary Chapter 1 The Setting The universe as we know it began about 15 billion years ago with an explosion that is called the big bang. There is no record of any prior

More information

Chapter 17 Cosmology

Chapter 17 Cosmology Chapter 17 Cosmology Over one thousand galaxies visible The Universe on the Largest Scales No evidence of structure on a scale larger than 200 Mpc On very large scales, the universe appears to be: Homogenous

More information

Elements and Isotopes

Elements and Isotopes Section 2-1 Notes Atoms Life depends on chemistry. The basic unit of matter is the atom. Atoms are incredibly small The subatomic particles that make up atoms are protons, neutrons, and electrons. Parts

More information

NSCI 314 LIFE IN THE COSMOS

NSCI 314 LIFE IN THE COSMOS NSCI 314 LIFE IN THE COSMOS 2 BASIC ASTRONOMY, AND STARS AND THEIR EVOLUTION Dr. Karen Kolehmainen Department of Physics CSUSB COURSE WEBPAGE: http://physics.csusb.edu/~karen MOTIONS IN THE SOLAR SYSTEM

More information

Nucleus Hydrogen nucleus. hydrogen. helium

Nucleus Hydrogen nucleus. hydrogen. helium 1. (a) Once formed, a star can have a stable life for billions of years. Describe the two main forces at work in the star during this period of stability. 1.... 2.... What happens to a star once this stable

More information

High Mass Stars. Dr Ken Rice. Discovering Astronomy G

High Mass Stars. Dr Ken Rice. Discovering Astronomy G High Mass Stars Dr Ken Rice High mass star formation High mass star formation is controversial! May form in the same way as low-mass stars Gravitational collapse in molecular clouds. May form via competitive

More information

Biology Unit 4. Chemistry of Life

Biology Unit 4. Chemistry of Life Biology Unit 4 Chemistry of Life Elements Everything in our universe that has a mass and a volume is made of matter. Matter in its purest form is an element. There are 118 elements on the periodic table,

More information

Astronomy Ch. 21 Stellar Explosions. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Astronomy Ch. 21 Stellar Explosions. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch. 21 Stellar Explosions MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) A surface explosion on a white dwarf, caused

More information

2. The evolution and structure of the universe is governed by General Relativity (GR).

2. The evolution and structure of the universe is governed by General Relativity (GR). 7/11 Chapter 12 Cosmology Cosmology is the study of the origin, evolution, and structure of the universe. We start with two assumptions: 1. Cosmological Principle: On a large enough scale (large compared

More information

Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere.

Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere. Chapter 29 and 30 Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere. Explain how sunspots are related to powerful magnetic fields on the sun.

More information

1. What is the primary difference between the evolution of a low-mass star and that of a high-mass star?

1. What is the primary difference between the evolution of a low-mass star and that of a high-mass star? FYI: The Lives of Stars E3:R6b 1. Read FYI: The Lives of Stars As you read use the spaces below to write down any information you find especially interesting. Also define the bold terms used in the text.

More information

the nature of the universe, galaxies, and stars can be determined by observations over time by using telescopes

the nature of the universe, galaxies, and stars can be determined by observations over time by using telescopes the nature of the universe, galaxies, and stars can be determined by observations over time by using telescopes The spectral lines of stars tell us their approximate composition Remember last year in Physics?

More information

Today. life the university & everything. Reminders: Review Wed & Fri Eyes to the web Final Exam Tues May 3 Check in on accomodations

Today. life the university & everything. Reminders: Review Wed & Fri Eyes to the web Final Exam Tues May 3 Check in on accomodations life the university & everything Phys 2130 Day 41: Questions? The Universe Reminders: Review Wed & Fri Eyes to the web Final Exam Tues May 3 Check in on accomodations Today Today: - how big is the universe?

More information

Biology Chapter 2: The Chemistry of Life. title 4 pictures, with color (black and white don t count!)

Biology Chapter 2: The Chemistry of Life. title 4 pictures, with color (black and white don t count!) 33 Biology Chapter 2: The Chemistry of Life title 4 pictures, with color (black and white don t count!) 34 Chapter 2: The Chemistry of Life Goals Highlight all unknown words 35-36 Chapter 2: The Chemistry

More information

Q1. Describe, in as much detail as you can, the life history of a star like our Sun

Q1. Describe, in as much detail as you can, the life history of a star like our Sun Q1. Describe, in as much detail as you can, the life history of a star like our Sun..................................... (Total 6 marks) Q2. The energy radiated by a main sequence star like the Sun is

More information

Matter vs. Antimatter in the Big Bang. E = mc 2

Matter vs. Antimatter in the Big Bang. E = mc 2 Matter vs. Antimatter in the Big Bang Threshold temperatures If a particle encounters its corresponding antiparticle, the two will annihilate: particle + antiparticle ---> radiation * Correspondingly,

More information

Lecture 19: Building Atoms and Molecules

Lecture 19: Building Atoms and Molecules Lecture 19: Building Atoms and Molecules +e r n = 3 n = 2 n = 1 +e +e r ψ even Lecture 19, p 1 Today Nuclear Magnetic Resonance Using RF photons to drive transitions between nuclear spin orientations in

More information

LIFE CYCLE OF A STAR

LIFE CYCLE OF A STAR LIFE CYCLE OF A STAR First stage = Protostar PROTOSTAR Cloud of gas and dust many light-years across Gravity tries to pull the materials together Eventually, at the center of the ball of dust and gas,

More information

13.1 Fundamental Particles and Forces

13.1 Fundamental Particles and Forces 13.1 Fundamental Particles and Forces Scientists once believed atoms were the smallest particles of matter. With the advancement of technology, it became clear that atoms themselves are made of simpler

More information

How Do Stars Appear from Earth?

How Do Stars Appear from Earth? How Do Stars Appear from Earth? Magnitude: the brightness a star appears to have from Earth Apparent Magnitude depends on 2 things: (actual intrinsic brightness) The color of a star is related to its temperature:

More information

Particle physics: what is the world made of?

Particle physics: what is the world made of? Particle physics: what is the world made of? From our experience from chemistry has told us about: Name Mass (kg) Mass (atomic mass units) Decreasing mass Neutron Proton Electron Previous lecture on stellar

More information

Untitled 1/21/18, 11:31 AM Physics: What We Do and Don t Know Steven Weinberg NOVEMBER 7, 2013 ISSUE Speculations of this sort ran into an obvious dif

Untitled 1/21/18, 11:31 AM Physics: What We Do and Don t Know Steven Weinberg NOVEMBER 7, 2013 ISSUE Speculations of this sort ran into an obvious dif Untitled 1/21/18, 11:31 AM Physics: What We Do and Don t Know Steven Weinberg NOVEMBER 7, 2013 ISSUE Speculations of this sort ran into an obvious difficulty: photons have no mass, while any new particles

More information

LIFE CYCLE OF A STAR

LIFE CYCLE OF A STAR LIFE CYCLE OF A STAR First stage = Protostar PROTOSTAR Cloud of gas and dust many light-years across Gravity tries to pull the materials together Eventually, at the center of the ball of dust and gas,

More information

Big Bang Planck Era. This theory: cosmological model of the universe that is best supported by several aspects of scientific evidence and observation

Big Bang Planck Era. This theory: cosmological model of the universe that is best supported by several aspects of scientific evidence and observation Big Bang Planck Era Source: http://www.crystalinks.com/bigbang.html Source: http://www.odec.ca/index.htm This theory: cosmological model of the universe that is best supported by several aspects of scientific

More information

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON FACULTY OF SCIENCE High Energy Physics WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON AIM: To explore nature on the smallest length scales we can achieve Current status (10-20 m)

More information

Stars and Galaxies. Evolution of Stars

Stars and Galaxies. Evolution of Stars Stars and Galaxies Evolution of Stars What do you think? Read the two statements below and decide whether you agree or disagree with them. Place an A in the Before column if you agree with the statement

More information