Atoms The Basis of All Materials RPI - ERTH 2330 The Atom - - PowerPoint PPT Presentation

atoms
SMART_READER_LITE
LIVE PREVIEW

Atoms The Basis of All Materials RPI - ERTH 2330 The Atom - - PowerPoint PPT Presentation

Atoms The Basis of All Materials RPI - ERTH 2330 The Atom Neutron - neutral particle Proton - positively charged particle Electron - negatively charged particle E.B. Watson Our story begins with light Visible light part


slide-1
SLIDE 1

Atoms

RPI - ERTH 2330

The Basis of All Materials

slide-2
SLIDE 2
  • Neutron - neutral particle
  • Proton - positively charged particle
  • Electron - negatively charged particle

E.B. Watson

The Atom

slide-3
SLIDE 3

Visible light – part of the EM spectrum Longer v = f, and v = 299,792,458 m / s (~3 E 8) in a vacuum is length of a cycle in m, f is Hz (cycles per second) Higher f Our story begins with light…

slide-4
SLIDE 4

FREQUENCY (f) number of cycles per unit time [units = Hertz (Hz)] 1 Hz = 1 cycle/s T = 1/f; f = 1/T; T f = 1 Wave Terms

slide-5
SLIDE 5

Dispersion

High f – more “bending” in prism Refraction – producing constituent wavelengths

slide-6
SLIDE 6

Refraction

Waves are bent as the move through materials with different wave propagating properties

E.B. Watson

slide-7
SLIDE 7

The spectrum of the hydrogen atom

E.B. Watson

slide-8
SLIDE 8

Violet 1 7.3E14 Hz Violet 2 6.9E14 Hz Green 6.2E14 Hz Red 4.6E14 Hz What are the wavelengths (v=c)? = v / f

slide-9
SLIDE 9

Photo-Electric Effect

Incident light causes movement of charge. Electrons move from the surface of the negatively-charged metal plate The intensity of the light determines how many electrons are produced, but not their kinetic

  • energy. Wavelength changes kinetic energy
slide-10
SLIDE 10

Small packets, or quanta, possessing specific amounts of energy. An incident photon is either totally absorbed by "target" matter or not absorbed at all* The energy of the photons in a monochromatic beam of light

E = h f

h is (Planck’s constant 6.626 E -34 Js) *Quantization of photons is like counting children - you can’t have a partial child PHOTONS

slide-11
SLIDE 11

Ephoton = EH - EL = h f

Energy transitions in Hydrogen

slide-12
SLIDE 12

Line n Violet 6 Violet 5 Blue-green 4 Red 3

Balmer relationships

Any hot gas at low pressure will produce a line spectrum, although the spectra of other gases are more complex than that of hydrogen. Hydrogen spectra

slide-13
SLIDE 13

Bohr model - a "solar-system" model. assumptions:

  • an electron is in specific "allowed" orbits
  • the allowed orbits are described by

m v r = n h / 2

Angular momentum Planck’s const.

F = m v2 / r and F = k q1 q2 / r2

Bohr saw this as charged particles on circular path set the forces equal

slide-14
SLIDE 14

Bohr specific radii for electrons j k l

E.B. Watson

slide-15
SLIDE 15

It requires energy to remove electrons Energy increases with orbital distance. Lowest energy configuration – ground state Quantum number Energy level at quantum number Energy level at ground state

slide-16
SLIDE 16

You can use this to determine changes in the amount of energy Describes the change in energy of an electron moved from 1st orbital (the ground state in H) to the n orbital

slide-17
SLIDE 17

E.B. Watson

slide-18
SLIDE 18

Electrons are attracted to the protons in the nucleus. Great, how big is the nucleus?

E.B. Watson

slide-19
SLIDE 19

E.B. Watson E.B. Watson

slide-20
SLIDE 20

Elements differ from one another by the number

  • f protons they contain (Z)

Hydrogen (H) – 1 proton Helium (He) – 2 protons Sodium (Na) – 11 protons Francium (Fr) – 87 protons A neutral atom will have as many electrons as protons. Many atoms for each element will have the same number of neutrons as protons Elements of the same Z that differ in the number

  • f neutrons are isotopes.
slide-21
SLIDE 21

Atoms Electron Neutrons Proton Mass 9.109 E -31 kg 1.673 E -27 kg 1.673 E -27 kg Charge (-1) 1.602 E -19 coul. (0) None (+1) 1.602 E -19 coul. Z = number of protons N = number of neutrons A = atomic mass number (N + Z) Element = unique Z Isotope = unique Z, different N What happens to A? 14C

slide-22
SLIDE 22

Isotope Same Z, different N Carbon (C ) Z = 6 Carbon-12

12C

6 protons, 6 neutrons 98.89% Carbon-13

13C

6 protons, 7 neutrons 1.11% Carbon-14

14C

6 protons, 8 neutrons trace Atomic mass units (u) Every isotope is scaled to 12C (12.000 u)

slide-23
SLIDE 23

The total mass (“atomic weight”) of any element is the sum of the weighted mass of its isotopes. For example, Oxygen has three isotopes mass (rel 12C) Abundance

16O

15.99491 99.759%

17O

16.99914 0.037%

18O

17.00016 0.204% (15.994191 x 0.99759) + (16.99914 x 0.00037) + (17.00016 x 0.00204) = 15.9994 u

slide-24
SLIDE 24
  • The interactions of electromagnetic radiation and

electrons reveal the energy structure of the atoms

  • The interaction of charged nuclei reveal the size of

atomic nuclei

  • The number of protons(+) determines the element’s

identity

  • It also determines the number of electrons (-)
  • The number of electrons controls the behavior of the

atom

  • The number of neutrons may vary - isotopes
  • Atomic mass is normalized to 12C
  • Atomic mass for an element is a function of isotope

abundance and mass.