Showing 12 results
Rutherford Gold Foil Scattering
Fire a continuous stream of alpha particles at a dense lattice of Gold nuclei (Au-79). Watch how the inverse-square Coulomb law dictates violent scattering trajectories, proving that atoms are mostly empty space harboring microscopic dense positive cores.
VSEPR Molecular Geometry
Explore 3D molecular geometries for common electron-domain configurations. Rotate and inspect tetrahedral, trigonal planar, linear, octahedral, and bent structures. Understand how lone pairs distort ideal bond angles.
Titration Curve Simulator
Simulate acid-base titrations and analyze pH curves for strong-strong, weak-strong, and polyprotic titrations. Visualize how pH changes as titrant is added, identify equivalence points, buffer regions, and half-equivalence points where pH = pKa. Understand the Henderson-Hasselbalch equation, calculate buffer capacity, and select appropriate indicators based on their pKa values and the pH at equivalence.
Atomic Orbital Shapes
Visualize the three-dimensional shapes of atomic orbitals (s, p, d, and f) that describe the probability distribution of electrons around the nucleus. Explore how quantum numbers (n, l, mₗ, mₛ) define orbital characteristics including energy level, shape, orientation, and electron spin. Understand the relationship between orbital shapes and chemical bonding, electron configuration, and the periodic table structure.
Galvanic (Voltaic) Cell
Explore galvanic (voltaic) cells that convert chemical energy into electrical energy through spontaneous redox reactions. Visualize electron flow from anode (oxidation) to cathode (reduction), ion movement through the salt bridge, and calculate cell potential using E°cell = E°cathode - E°anode. Understand the Nernst equation, concentration effects on voltage, and applications in batteries and fuel cells.
Electron Configuration
Build electron configurations for atoms and ions using the Aufbau principle, Hund's rule, and the Pauli exclusion principle. Visualize how electrons fill orbitals in order of increasing energy (1s, 2s, 2p, 3s, 3p, 4s, 3d...), understand noble gas notation shortcuts, and identify valence electrons. Explore exceptions like chromium and copper, and connect electron configuration to periodic trends and chemical reactivity.
Enthalpy vs Entropy (ΔG)
Explore the relationship between enthalpy (ΔH), entropy (ΔS), and Gibbs free energy (ΔG) using the equation ΔG = ΔH - TΔS. Understand how temperature affects spontaneity: exothermic reactions with increasing entropy are always spontaneous, while endothermic reactions with decreasing entropy are never spontaneous. Visualize how ΔG < 0 indicates spontaneous processes, ΔG = 0 represents equilibrium, and ΔG > 0 means non-spontaneous reactions.
First-Order Kinetics Decay
Analyze first-order reactions where the rate depends linearly on one reactant concentration: rate = k[A]. Visualize exponential decay using the integrated rate law ln[A]t = ln[A]₀ - kt, and understand that first-order reactions have constant half-life t₁/₂ = 0.693/k independent of initial concentration. Explore applications in radioactive decay, drug metabolism, and chemical decomposition reactions.
Galvanic vs Electrolytic Cells
Compare galvanic cells (spontaneous, ΔG < 0, generate electricity) with electrolytic cells (non-spontaneous, ΔG > 0, require external voltage). Visualize how galvanic cells convert chemical energy to electrical energy in batteries, while electrolytic cells use electrical energy to drive non-spontaneous reactions in electroplating, electrolysis, and metal purification. Understand electrode polarity differences and the role of external power sources.
Gas Laws
Explore the fundamental gas laws that describe relationships between pressure, volume, temperature, and amount of gas. Visualize Boyle's Law (P₁V₁ = P₂V₂), Charles's Law (V₁/T₁ = V₂/T₂), Gay-Lussac's Law (P₁/T₁ = P₂/T₂), Avogadro's Law (V₁/n₁ = V₂/n₂), and the Combined Gas Law. Understand how these individual laws combine to form the Ideal Gas Law PV = nRT.
Ideal Gas Law Simulator
Simulate the Ideal Gas Law PV = nRT to explore how pressure, volume, temperature, and moles of gas are related. Manipulate variables to see real-time effects on gas behavior, calculate unknown quantities using R = 0.0821 L·atm/(mol·K), and understand the assumptions of ideal gas behavior. Explore deviations from ideality at high pressure and low temperature where real gases exhibit intermolecular forces and molecular volume.
Intermolecular Forces
Explore the attractive forces between molecules that determine physical properties like boiling point, melting point, and solubility. Compare London dispersion forces (weakest, present in all molecules), dipole-dipole interactions (polar molecules), and hydrogen bonding (strongest IMF, requires H bonded to N, O, or F). Understand how molecular structure, polarity, and molecular weight affect IMF strength and predict relative boiling points.