Joseph Hull, Instructor
Division of Science and Mathematics,
SCCC
copyright Joseph Hull
Chemistry 1: Atoms and Elements
Week
3: elements, atomic models, periodic
table, isotopes
Elements: fundamental
building block of all kinds of matter (solids, liquids, gases)
examples: oxygen, silicon, carbon, hydrogen, uranium, lead, sodium (about 100+ altogether)
individual atoms “seen” (imaged) only recently, presence/existence was inferred for many years
Atomic Model: elements often pictured as spheres but more like angry bees buzzing around hive
hive = nucleus, contains 2 particles, represent almost all the mass of an atom, usually 50:50 ratio
neutron: massive particle in nucleus, has no electrical charge (neutral)
proton: massive
particle in nucleus, has a positive
(+ve) electrical charge
usually a neutron for every
proton in the nucleus (but exceptions, see below)
nucleus
has an overall positive charge. nucleus
is very small compared to whole atom.
particles in nucleus bound together with incredibly strong force, when you rupture nucleus = BANG
angry bees = electrons, tiny particle, + massless, has a negative (-ve) electrical charge
electrons swarm/orbit around nucleus
forming electron cloud. 99.9% of atom =
empty space
electrons not tightly bound to atom, can be added or subtracted without too much effort
Problem: moving charged particles produces electromagnetic waves (= radiation)
example: hook wire to battery, electrons move through wire, EM field/waves produced
radiation produced means radiation/Energy lost, electrons should lose energy and stop…..
Bohr: at certain special distances out from the nucleus, electrons can orbit without losing energy
cannot circle/orbit nucleus at any old distance, must be at special distances from nucleus
special distances called orbitals or electron shells or energy levels
Why/how possible? take chemistry and physics to learn about quantum mechanics
lowest energy level closest to
nucleus, highest energy levels farther away
when electron drops from high E shell to lower E shell, radiation emitted (called photon)
examples: glow in the dark materials, fires, etc. all emitting photons
to push electron from low E shell to high E shell, must add/absorb photon/radiation
Periodic Table: one way of arranging the different elements.
A) either 1 or 2 letter abbreviation for each element, first letter capitalized
ex: H = hydrogen, He = helium, S = sulfur, Si = Silicon, Fe = iron, K = potassium, etc.
B) arranged by atomic number above element. atomic number = # of protons in nucleus
example: silicon (Si) has 14 protons in its nucleus (that’s how silicon is defined)
H = hydrogen = 1 = lightest element, 103 = Lr = Lawrencium = heaviest element
C) average atomic mass given below the element: average number of protons and neutrons
should be twice the atomic number (for every proton in atomic number, should be neutron).
examples: silicon, 2 x 14 = 28, actually 28.1. oxygen, 2 x 8 = 16, actually 15.99
these examples tell you that elements can have extra or missing neutrons = different flavors
different flavors of elements called isotopes. some isotopes stable, others unstable
ex: Carbon 14 (6 protons and 8 neutrons) is unstable = radioactive, will break down
Carbon 14 breaks down/decays into Carbon 12 (6 and 6) which is stable.
radioactive decay: change from unstable to stable isotope, releases radiation and particles
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