Wednesday, August 14, 2019
Development of the Atomic Model Essay
460 ââ¬â 370? BC ââ¬â Democritus ââ¬â first theory of atom ââ¬â All matter is composed of particles called atoms which canââ¬â¢t be subdivided ââ¬â different materials had different properties because their atoms were different ââ¬â atoms have different sizes, regular shape, are in constant motion, and have empty space 450 BC ââ¬â Empedocles ââ¬â matter is composed of four elements ââ¬â earth, air, fire, water 384 ââ¬â 322 Aristotle ââ¬â no voids! Opposed Democritusââ¬â¢ theory ââ¬â 4 elements earth, fire, air water with dry, hot, moist and cold 500 ââ¬â 1600 A.D. ââ¬â age of alchemy Late 1700ââ¬â¢s ââ¬â law of conservation of mass ââ¬â mass doesnââ¬â¢t change during a chemical reaction 1799 ââ¬â Proust ââ¬â law of constant composition ââ¬â compounds always have same proportion by mass of their elements 1766-1844 John Dalton (English) postulates atoms as a billiard ball model ââ¬â all matter is made of particles called atoms ââ¬â all atoms of an element are identical ââ¬â atoms of different elements have different properties ââ¬â atoms combine to form compounds ââ¬â atoms are neither created nor destroyed during a chemical reaction Late 1800ââ¬â¢s ââ¬â Sir William Crookes and others ââ¬â used sealed glass tubes to generate a glow ââ¬â Cathode rays were attracted to positive plates ââ¬â therefore negatively charged ââ¬â Rays could be blocked ââ¬â therefore a particle ââ¬â Negatively charged particles were called electrons 1897 JJ Thomson ââ¬â used cathode ray tube and developed raisin bun model ââ¬â Electrons randomly distributed through positive mass ââ¬â told not to touch ââ¬â broke everything but could see what was wrong with equipment 1904 Hantaro Nagaoka ââ¬â developed Saturn model 1911 Earnest Rutherford ââ¬â Thomsonââ¬â¢s research assistant ââ¬â testing Thomsonââ¬â¢s theory ââ¬â gold foil experiment ââ¬â surprised ââ¬â like shooting a cannon ball at a piece of tissue paper and having the cannon ball bounce back at you! ââ¬â Most of atom is empty space, positively charged nucleus ââ¬â Electrons in a cloud around the nucleus ââ¬â had hands of gold and knew how to use them to get answers ââ¬â didnââ¬â¢t mention electrons because he didnââ¬â¢t know what they did ââ¬â he did know they werenââ¬â¢t in orbits because the energy degenerates and in the atom, it doesnââ¬â¢t 1886 ââ¬â Goldstein ââ¬â discovery of the proton (shown to be a fundamental particle 20 years later) ââ¬â 1837 times heavier than an electron 1932 James Chadwick ââ¬â discovered neutrons by bombarding Be with alpha particles ââ¬â Gave off rays which werenââ¬â¢t deflected by outside fields ââ¬â Neutron had mass approximately equal to a proton 1900 Max Planck ââ¬â energy is absorbed and released in chunks called quantum (compare playing a piano vs a violin) Einstein ââ¬â radiant energy ââ¬â energy packets called photons ; described photoelectric effect from observing that radiant energy on metal releases electrons 1913 Niels Bohr (worked first with JJ Thomson then with Rutherford) developed model for hydrogen where the electron orbits the nucleus. ââ¬â He explained the H emission spectra and the explanation was the foundation for n, the principle quantum number ââ¬â the concept of energy levels ââ¬â Mathematical predictions of lines only worked for hydrogen ââ¬â won a Nobel prize for looking at the solar system and comparing it to the atom 1924 Louis de Broglie showed that if radiant energy could act like a stream of particles, then matter could act like a wave ââ¬â the wave property of electrons 1927 Werner Heisenberg ââ¬â developed uncertainty principle ââ¬â impossible to know both exact momentum and location of an electron due to dual nature of matter 1926 Erwin Schodinger ââ¬â Schodingerââ¬â¢s wave equation ââ¬â quantum mechanics (advanced calculus needed) takes into account the wave and particle nature of electrons. ââ¬â equation (2 gives info on location of electron in terms of probability density ââ¬â wave functions are called orbitals ââ¬â [pic], where E is energy, e2 is electric potential, r is orbital radius and h is Planckââ¬â¢s constant 1925 Wolfgang Pauli ââ¬â each orbital has only 2 electrons is now explained due to direction of spin of electrons. Spinning electrons create magnetic field. Only 2 electrons of opposite spin in an orbital referred to as Pauli exclusion principle Hundââ¬â¢s rule ââ¬â half fill each orbital before adding second electron Aufbau principle ââ¬â energy sublevel must be filled before moving onto next higher sublevel Principle Quantum Number, n ââ¬â integer that Bohr used to label the orbits and energy levels ââ¬â a main shell of electrons ââ¬â seen in low resolution spectra ââ¬â still used today although we now use orbitals instead of orbits Secondary Quantum Number, l ââ¬â Arnold Sommerfeld (1915) extended Bohrââ¬â¢s theory. ââ¬â H has 3 elliptical orbitals for n = 2 ââ¬â Explained the observed line splitting seen for H in high resolution line spectra ââ¬â Introduced l to describe sublevels ââ¬â l has values 0 to n-1 ââ¬â relates energy levels to shape of electron orbital and explains regions of the periodic table ââ¬â l=0, s orbital ââ¬â sharp ââ¬â l=1, p orbital ââ¬â principle ââ¬â l=2, d orbital ââ¬â diffuse ââ¬â l=3, f orbital ââ¬â fundamental Magnetic Quantum Number, ml ââ¬â from experimentation with emission line spectra ââ¬â place a gas discharge tube near a strong external magnet, and some single lines split into new lines not initially seen ââ¬â done by Pieter Zeeman in 1897 ââ¬â called normal Zeeman Effect ââ¬â Zeeman Effect explained by Sommerfeld and Peter Debye (1916) ââ¬â They proposed that the orbits could exist at various angles ââ¬â If orbits in space are in different planes, the energies of the orbits are different when the atom is near a strong magnet ââ¬â For each value of l, ml can vary from ââ¬âl to +l ââ¬â If l = 1, ml can be -1, 0, 1 suggesting 3 orbits with the same energy and shape but with a different orientation in space (degenerate orbitals) Spin Quantum Number, ms ââ¬â to explain more and new evidence, ie the additional line splitting seen in a magnetic field ââ¬â student of Bohr and Sommerfeld ââ¬â Pauli ââ¬â suggested each electron spins on its axis and is like a tiny magnet. ââ¬â Could only have one of two spins equal in magnitude, opposite in direction (vector) ââ¬â Values + à ½ or ââ¬â à ½ ââ¬â Opposite pair is a stable arrangement like bar magnets stored in pairs arranged opposite to each other (produce no magnetism) ââ¬â If single unpaired electrons present, magnetism is present and atom is affected by magnetic fields Overall ââ¬â each electron in an atom is described by a set of 4 quantum numbers ââ¬â fits perfectly arrangement of electrons and the structure of the periodic table
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