Learning Objectives: Where do the elements come from? What can we learn from telescopes? How do heavy elements form?

Slides:



Advertisements
Similar presentations
Section 2: Nuclear Fission and Fusion
Advertisements

If you look up at the sky at night, the heavens appear to be unchanging. In 1917 Einstein wrote down the theory of General Relativity. His equations indicated.
Garfield Graphics included with kind permission from PAWS Inc. All Rights Reserved. Fusion The power source of the stars!
7: Atomic and Nuclear Physics 7.3 Nuclear reactions, fission and fusion.
14.2 Galactic Recycling Our Goals for Learning How does our galaxy recycle gas into stars? Where do stars tend to form in our galaxy?
Nuclear Physics Lesson 13
Binding Energy Binding Energy per Nucleon. Binding Energy The term binding energy is used to indicate the energy that would be required to form an atom.
Part I: Chapter 25 Radioactive decay & Half Life
Nuclear Chemistry Bravo – 15,000 kilotons. CA Standards.
A nucleus can be specified By an atomic number and a Mass number.
Where do elements come from?. Remember the Big Bang? The theory states that Universe today retains an imprint of its initial cosmic mixture of elements.
The Genesis of the Elements Saliya Ratnayaka For Chem 510 October 22,2004.
Taking the fingerprints of stars, galaxies, and interstellar gas clouds Absorption and emission from atoms, ions, and molecules.
Energy from fusion - “that” equation. The energy from stars comes from nuclear fusion in the core. Light nuclei fuse together & release energy - it takes.
Announcements Pick up graded homework (projects, tests still in progress) Turn in Homework 10 by 5:00 Vote tomorrow! Transit of Mercury (crossing in front.
Unit 2 – The Atom Nuclear Chemistry Fusion and Fission.
NUCLEAR FUSION NUCLEAR FISSION. chools/gcsebitesize/scie nce/add_aqa/atoms_rad iation/nuclearact.shtmlhttp:// chools/gcsebitesize/scie.
IB Assessment Statements, Topic 7.3  Nuclear Reactions Describe and give an example of an artificial (induced) transmutation Construct and.
 The visible light we see is only a small amount of energy coming from various objects.  By studying other forms of energy, astronomers can learn more.
Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion.
Ever ask yourself the question… How did this all begin?
Unit 2 – The Atom Nuclear Chemistry Fusion and Fission.
Nuclear Energy and Mass Defect Lesson 5. Objectives   use the law of conservation of charge and mass number to predict the particles emitted by a nucleus.
Section 1: Structure of the Sun
Atomic Structure Chapter 4
Nuclear Fusion Nuclear Fusion is a process in which two or more smaller nuclei collide and form a new, larger nucleus. In some fusion reactions, a neutron,
NUCLEAR CHEMISTRY QUIZ.
Stellar Life Stages Star Birth and Death.
The UniverseSection 1 Question of the Day: Jackie used a portable electric drill to remove screws from a broken wooden table. He noticed that the screws.
The Sun Section 1 Section 1: Structure of the Sun Preview Objectives The Sun’s Energy Nuclear Fusion Mass Changing into Energy The Sun’s Interior The Sun’s.
Topic – Physics 2a Mass defect and binding energy Prior learning Atomic structure Electrical forces Key words –Atomic nucleus,mass difference, mass of.
Chapter 29 The Sun 29.1 Structure of the Sun
THE NUCLEUS: A CHEMIST’S VIEW. Nuclear Symbols Element symbol Mass number, A (p + + n o ) Atomic number, Z (number of p + )
ELEMENTS atomic number = Z = number of protons = p mass number = number of nucleons = p + n atomic mass = experimental measurement of the mass of the.
The UniverseSection 1 Section 1: The Life and Death of Stars Preview Key Ideas Bellringer What Are Stars? Studying Stars The Life Cycle of Stars.
Section 1: Structure of the Sun
Nuclear Fusion By: Yours Truly, Christie Osadchy, and The Fool Who Ripped His Pants.
Chapter 21 Nuclear Chemistry John A. Schreifels Chemistry 212.
Energy (J) 299,792,458 m/s Mass (Kg) Speed of Light Squared.
The UniverseSection 1 Key Ideas 〉 How are stars formed? 〉 How can we learn about stars if they are so far away? 〉 What natural cycles do stars go through?
 a.I can describe the big bang theory and the evidence that supports this theory. b. I can describe the nebular theory of solar system formation and the.
Jeopardy $100 Fundamental Forces Uses for Nuclear Physics Decay Nuclear Stability Einstein’s Famous Equation $200 $300 $400 $500 $400 $300 $200 $100 $500.
ETA CARINAE – NATURE’S OWN HADRON COLLIDER We still do not know one thousandth of one percent of what nature has revealed to us. - Albert Einstein -
Nuclear Physics.
Binding energy sketch the variation of binding energy per nucleon with nucleon number. explain what is meant by nuclear fusion and nuclear fission. explain.
5.3.4 Nuclear Fission and Fusion. (a) select and use Einstein’s mass–energy equation ΔE = Δmc 2.
NUCLEAR FUSION.
Living By Chemistry SECOND EDITION
Review Videos-Radioactivity Review Videos-Strong and Weak Nuclear Forces.
Nuclear Reactions Nuclear Reactions.
Welcome– 10/17 Collect Lab Reports Big Bang Theory and Life Cycle of the Star Notes Nuclear Chemistry Notes HW: NONE!
Unit 3: Part 2 of the Atom Nuclear Chemistry I. The Nucleus (p. 701 – 704 in Class Modern Chemistry Text) I. The Nucleus (p. 701 – 704 in Class Modern.
 Explain how stars form.  Explain how stars get their energy.  Give examples of why stars change over time.  Compare the evolution of medium and high.
Click Above to Jump to Modern Atomic Theory Section
Earth in Space Benchmarks
NUCLEAR FUSION Process of combining two light nuclei to
Nuclear Energy and Mass Defect
Nuclear Reactions.
Section 2: Nuclear Fission and Fusion
Astronomy Created by Educational Technology Network
14.2 Galactic Recycling Our Goals for Learning
Chapter 13 Nuclear Chemistry.
Unit 3: Part 2 of the Atom Nuclear Chemistry
Unit 11 - Nuclear Chemistry
Nuclear Chemistry Bravo – 15,000 kilotons.
Bell Work: Radioactivity
Nuclear Chemistry Chapter 21.
Section 2: Nuclear Fission and Fusion
Presentation transcript:

Learning Objectives: Where do the elements come from? What can we learn from telescopes? How do heavy elements form?

The equation below shows a typical fusion reaction that occurs in stars. It is interesting to note that the overall mass of the reactants is bigger than the overall mass of the products. Drag the labels in the correct place. Where do the elements come from? Helium IonPositronHydrogen Ion What happens to the missing mass? Why do you think two anti-electrons are released? Is this equation balanced? In what sense is/isn’t it? What happens to the reactants in this process?

ALT + Click to edit this text, or delete and use INK for PowerPoint (the interactive pen in the bottom left corner) to write your conclusions! ALT + Click to edit this text, or delete and use INK for PowerPoint (the interactive pen in the bottom left corner) to write your conclusions! Einstein discovered that: Where do the elements come from? Reactants mass = 6.69x kg Do you think this energy is large or small? Why? How many reactions like this one do you think occur in a star every second? Use the information below and the above equation to work out the energy released by the fusion reaction Products mass = 6.64x kg What do E, m and c mean? What other reactions could occur in a star? Would they produce more or less energy?

The binding energy per nucleon is a measurement of the energy that holds each particle (nucleon) in the nucleus of an atom. Average Binding Energy per Nucleon (1.66 x J) What can you notice about the Binding Energy per Nucleon in different elements? Compare the B.E. Per Nucleon of He and H. What can you notice? Could you use this graph to predict the energy released by nuclear reactions? Explain your answer Which is the most stable element? Why did you choose that one? Where do the elements come from?

Drag the labels in the correct place on the graph. Average Binding Energy per Nucleon (1.66 x J) In this region nuclear fusion happens In this region nuclei are very stable In this region nuclear fission happens

What can we learn from telescopes? The next three images show the same region of rapid star formation in the Orion Nebula and the wavelengths emitted by the cosmic gas surrounding these newly born stars. Use the information in these images to discuss the possible consequences of the presence of these molecules in such regions.

What types of molecules are these? What elements can you spot in this emission spectrum? What would your Biology teacher associate these molecules with? What can we learn from telescopes? Orion Nebula (Herschel Space Observatory) What would you Chemistry teacher associate these molecules with?

Do you think Scientists expected to find these molecules in young star forming regions? Explain your answer. Were you expecting to find these molecules in young star forming regions? What other elements are formed in a young star? Would you expect to find heavier elements like Iron in this region? Why? What can we learn from telescopes?

What do the sharp peaks in the spectral graph mean? Which molecule is most abundant in this star forming region? Why are these molecules important? Why are Scientists interested in them? What can we learn from telescopes? Orion Nebula (Herschel Space Observatory) Do you think Scientists are looking at a particular part of the EM Spectrum here? Why?

What is this type of star called? In what stage of its life is this star? What will happen to this star eventually according to the theory of evolution of stars? What can we learn from telescopes? VY Canis Majoris (Herschel) What elements would you expect this star to produce when it comes to the end of its life?

Why is this called Tycho’s Supernova? What elements can you spot in this emission spectrum? Compare the elements from this supernova with the elements surrounding young stars. What can you notice? How do heavy elements form? Tycho's Supernova Would we be able to see these Supernova remnants, if we used the same instruments Thyco used? Why?

Complete the postcard below to tell Tycho Brahe how much we have discovered about “his” Supernova and other stars with modern telescopes Tycho Brahe Benátky nad Jizerou Czech Republic 11 th November 1572 Front of Postcard Back of Postcard How do heavy elements form?

Where do the elements come from? A variety of elements are found in regions surrounding relatively young stars What can we learn from telescopes? Modern telescopes (especially space telescopes) allow us to observe all the EM waves emitted by stars, not just visible light How do heavy elements form? Heavy elements like Iron are found in remnants of dead stars (Supernovae) and this suggests that such elements form in the last stages of the life of a star Learning outcomes