PPT-Chapter 6: The Structure of Matter
Author : stefany-barnette | Published Date : 2018-11-06
Section 2 Ionic and Covalent Bonding Objectives Why do atoms form bonds How do ionic bonds form What do atoms joined by covalent bonds share What gives metals their
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Chapter 6: The Structure of Matter: Transcript
Section 2 Ionic and Covalent Bonding Objectives Why do atoms form bonds How do ionic bonds form What do atoms joined by covalent bonds share What gives metals their distinctive properties. Not in compact objects (brown dwarfs, etc.). Baryons should also contribute to . nucleosynthesis. But we got it to work out assuming it’s . not. baryons. Most likely: it will be some sort of undiscovered particle: . Chapter 2 Goals. Make a Title Page for Chapter 2.. Write the Chapter Goals on the Title Page. What are characteristic properties of matter and how are they used to identify matter?. What is the underlying structure of matter, and how do the properties we observe relate to this underlying structure?. Extragalactic Distance Scale. Cepheids. M. V. =-3.35logΠ-2.13+2.13(B-V) . Π. =period (days). Novae M. V. (max)=-9.96-2.31log(. Δm. /day). first 2 . mags. Planetary Nebulae Luminosity Function M. Lisa Randall. Harvard University. @. lirarandall. . What do we know about dark matter?. It has gravitational interactions—of matter!. Gravitational . lensing. Rotation curves in galaxies. Detailed measurements of energy abundances—total and normal matter. Pre-SUSY Summer School. Melbourne, June 29-July 1, 2016 . An . Introduction. to. Particle. Dark . Matter. Santa Cruz Institute for Particle Physics. University of California, Santa Cruz. Thank you. 13. On your list of 16 factors for . Freakonomics, . label each factor with one of the following symbols:. AB. – does this factor deal with a kid’s . ability. OPP. – does this factor deal with a kid’s . Peter Jacobs. Lawrence Berkeley National Laboratory. Lecture 2. Initial conditions: . partonic. structure and global observables . 6/20/11. 1. Hot Matter at RHIC and LHC - Lecture 2. Recap from yesterday:. 4.1 Early Theories of . Matter (& Early Chemistry – Alchemy and Related). 4.2 Subatomic Particles & Nuclear Atom. 4.2.5 Ultimate Structure of Matter – The Standard Model (Not in Book). Section 4.1 Early Ideas About Matter. 1.)I will define homogeneous mixtures , heterogeneous mixtures, physical changes, and chemical changes.. 2.)I will identify homogeneous mixtures, heterogeneous mixtures, physical changes, and chemical changes.. UEQ: How does the structure of matter influence its physical and chemical behavior?. LEQ: How is matter classified?. Bell Work 09/19/2012. Write question and answer.. Can you chemically break down an atom? Why or why not? . 2-1 Energy . 2-2 Temperature . 2-3 Matter . 2-4 Elements and Compounds . 2-5 Mixtures . 2-1 Energy. Name 3 basic forms of nrg. State the law of conservation of nrg. Need for nrg. Heat water for cooking, bathing, etc.. Matter describes anything that has . mass. and . volume. Can matter be invisible? . YES. Ex. . Air. Matter and Atoms. History of atoms. Democritus. Was a . Greek. philosopher in . 400 BC. Thought the universe was made of . The INITIAL patterns of evolution L eonid E. Grinin Laboratory for monitoring of socio-political destabilization risks, HSE THE ORIGINS OF THE WORLD’S FUNDUMENTALS AND THE BASIC SIMILARITIES OF THE MATTER Review. Pollution & Recycling. Projects?. Next Physical Science Class. Jan. 8. th. Finals Class Jan. 15. th. 4 pm. .5 for passing the Final. All Power Points will be on line on my web site. You will be given back your notes, you can use the .
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