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Atom
Fundamental unit of matter in chemistry.
Subatomic Particles
Particles making up an atom: protons, neutrons, electrons.
Neutron
Neutral particle in an atom's nucleus.
Electron
Negatively charged particle surrounding the nucleus.
Atomic Number (Z)
Number of protons in an atom's nucleus.
Mass Number (A)
Total number of protons and neutrons in nucleus.
Charge of Proton
Fundamental unit of charge: +1 e (1.6 × 10^-19 C).
Charge of Electron
Equal in magnitude to proton, but negative: -1 e.
Bohr Model
Early model of atom, electrons in fixed orbits.
Quantum Mechanical Model
Modern model, electrons in probabilistic orbitals.
Valence Electrons
Electrons in outermost shell, important for bonding.
Hydrogen Isotopes
Protium, deuterium, and tritium are hydrogen isotopes.
Electrostatic Force
Attraction between oppositely charged particles.
Gravitational Force
Weak attraction based on mass of particles.
Quarks
Fundamental particles making up protons and neutrons.
Leptons
Elementary particles, includes electrons.
Gluons
Particles that mediate strong force between quarks.
Nucleus
Central part of an atom containing protons and neutrons.
Electrons
Negatively charged subatomic particles in orbitals.
Cation
Positively charged atom due to electron loss.
Anion
Negatively charged atom due to electron gain.
Atomic Mass Unit (amu)
Unit defined as 1/12 the mass of carbon-12. and Unit for measuring mass of atomic particles.
Proton
Positively charged subatomic particle in the nucleus.
Neutron
Neutral subatomic particle in the nucleus.
Electron Mass
Approximately 1/1836 of a proton's mass.
Binding Energy
Energy required to hold protons and neutrons together.
Reactivity
Tendency of an atom to engage in chemical reactions.
Electrostatic Pull
Attractive force between charged particles.
Atomic Weight
Weighted average mass of an element's isotopes.
Electrons in Neutral Atom
Equal to the number of protons.
Atomic Mass Calculation
Mass number approximates atomic mass in amu.
Isotopes
Atoms of the same element with different neutrons.
Protium
Hydrogen isotope with one proton, atomic mass 1 amu.
Deuterium
Hydrogen isotope with one proton, one neutron, 2 amu.
Tritium
Hydrogen isotope with one proton, two neutrons, 3 amu.
Half-Life
Time for half of a radioactive sample to decay.
Stability
Longer half-lives indicate greater isotope stability.
Avogadro's Number
6.02 × 10²³, number of particles in a mole.
Mole
Quantity equal to Avogadro's number of entities.
Atomic Mass
Mass of an average atom in atomic mass units.
Planck's Constant
6.626 x 10⁻³⁴ J•s, relates energy and frequency.
Quantum Theory
Energy emitted in discrete packets called quanta.
Centripetal Force
Force keeping electron in circular orbit around nucleus.
Energy Transition
Energy change when an electron jumps energy levels.
Photon Wavelength
Distance between successive peaks of emitted light.
Energy of a Photon
Energy calculated from its wavelength.
Chemical Properties
Similar characteristics exhibited by isotopes due to identical protons.
Angular Momentum
Defined as L = mvr, quantized in Bohr's model.
Kinetic Energy
Calculated as K = ½ mv² for moving objects.
Bohr's Model
Describes electron orbits with quantized energy levels.
Principal Quantum Number (n)
Positive integer indicating electron energy levels.
Rydberg Unit of Energy (Ry)
Value equal to 2.18 × 10⁻¹⁸ J.
Speed of Light (c)
Constant value of 3 x 10⁸ m/s.
Energy Equation 1
E = -Ry/n², relates energy to quantum number.
Ground State
Lowest energy state of an atom, stable configuration.
Quantized Energy
Energy changes occur in discrete amounts.
Negative Energy Values
Indicates attractive force between electron and nucleus.
Discreteness of Energy Levels
Energy levels are not continuous, but quantized.
Electron Orbit
Defined pathway around the nucleus in Bohr's model.
Attractive Force
Force between electron and proton, represented negatively.
Energy Increase
Electron energy becomes less negative as n increases.
Quantization Concept
Similar to discrete steps on a staircase.
Equation for Angular Momentum
L = nh, where n is a quantum number.
Temperature Effect
Atoms exist in ground state unless heated or irradiated.
Force Representation
Negative sign indicates attraction in energy equations.
Conceptual Understanding
Focus on ratios and relationships for problem-solving.
Energy Transfer
Movement of energy between electron orbits.
Electron Jump
Transition of electron to higher energy orbit.
Ground State
Lowest energy state of an atom (n=1).
Excited State
State when electrons occupy higher energy levels.
Atomic Emission Spectrum
Light emitted when electrons return to ground state.
Photon Emission
Release of energy as photons during transitions.
Speed of Light (c)
Velocity of light in vacuum, 3.00 × 10⁸ m/s.
Wavelength (λ)
Distance between successive peaks of a wave.
Quantized Energy Levels
Discrete energy states electrons can occupy.
Line Spectrum
Spectrum showing distinct lines for specific transitions.
Fluorescence
Emission of light from excited electrons returning to ground state.
Emission Spectrum
Spectrum of light emitted by excited atoms.
Energy Equation 2
E = hf; relates energy to frequency.
Frequency Equation
c = fλ; relates speed of light to frequency and wavelength.
Atomic Fingerprint
Unique emission spectrum identifying elements.
Hydrogen Emission Spectrum
Simplest emission spectrum, used for analysis.
Energy Transition
Movement between quantized energy levels.
Subshell
Energy level within an atom's electron configuration.
Electromagnetic Energy
Energy carried by photons in electromagnetic waves.
Excitation Sources
Heat or energy forms causing electron transitions.
Discrete Energy Amounts
Specific energy values emitted during transitions.
Lyman series
Hydrogen emission lines from n≥2 to n=1.
Balmer series
Hydrogen emission lines from n≥3 to n=2.
Paschen series
Hydrogen emission lines from n≥4 to n=3.
Energy transitions
Changes between quantum energy levels in atoms.
Photon wavelength
Distance between successive peaks of light waves.
Energy and wavelength relationship
Energy is inversely proportional to wavelength.
Planck's quantum theory
Energy quantization based on photon emission.
Bohr's model
Atomic structure model describing electron orbits.
Atomic absorption spectrum
Unique wavelengths absorbed by an element's electrons.
Atomic emission spectrum
Unique wavelengths emitted by an element's electrons.
Energy absorption
Electrons gain energy to move to higher levels.
Energy emission
Electrons lose energy moving to lower levels.
Conservation of energy
Energy remains constant in transitions between levels.