materials-chemistry
States of matter, phase transitions, kinetic molecular theory, atmospheric chemistry, green chemistry, and sustainable synthesis. Covers solid/liquid/gas/plasma properties, phase diagrams, vapor pressure, gas laws, ozone chemistry, greenhouse effect, the 12 principles of green chemistry, atom economy, solvent selection, and catalysis for sustainability. Use when reasoning about material properties, environmental chemistry, or designing greener chemical processes.
git clone --depth 1 https://github.com/Tibsfox/gsd-skill-creator /tmp/materials-chemistry && cp -r /tmp/materials-chemistry/examples/skills/chemistry/materials-chemistry ~/.claude/skills/materials-chemistrySKILL.md
# Materials Chemistry How matter behaves — its phase, its response to temperature and pressure, its interactions with the atmosphere, and whether its production harms or heals the environment — is the domain of materials chemistry. This skill connects the microscopic world of molecules and intermolecular forces to the macroscopic behavior of substances, the chemistry of Earth's atmosphere, and the design of sustainable chemical processes. **Agent affinity:** franklin (materials/applied chemistry, primary) **Concept IDs:** chem-states-of-matter, chem-atmospheric-chemistry, chem-green-chemistry ## States of Matter ### The Four States | State | Particle arrangement | Particle motion | Shape | Volume | Compressibility | |---|---|---|---|---|---| | Solid | Fixed, ordered lattice | Vibration only | Fixed | Fixed | Nearly zero | | Liquid | Close but disordered | Slide past each other | Container shape | Fixed | Very low | | Gas | Far apart, random | Rapid, random | Container shape | Container volume | High | | Plasma | Ionized gas | Extremely rapid | Container shape | Container volume | High | **Kinetic molecular theory (KMT) for gases:** 1. Gas particles are in constant, random motion. 2. The volume of individual particles is negligible relative to the container. 3. No attractive or repulsive forces between particles. 4. Collisions are perfectly elastic (kinetic energy is conserved). 5. Average kinetic energy is proportional to absolute temperature: KE_avg = (3/2)kT. Assumptions 2 and 3 define an ideal gas. Real gases deviate at high pressure (particle volume matters) and low temperature (intermolecular forces matter). ## Gas Laws | Law | Equation | Constant conditions | Relationship | |---|---|---|---| | Boyle's | P1V1 = P2V2 | T, n | Inverse (P and V) | | Charles's | V1/T1 = V2/T2 | P, n | Direct (V and T) | | Avogadro's | V1/n1 = V2/n2 | T, P | Direct (V and n) | | Combined | P1V1/T1 = P2V2/T2 | n | All three above | | Ideal gas | PV = nRT | None fixed | R = 0.08206 L-atm/mol-K | | Dalton's | P_total = P1 + P2 + ... | — | Partial pressures add | ### Worked Example: Ideal Gas Law **Problem.** What volume does 2.50 mol of N2 occupy at 25.0 C and 1.25 atm? V = nRT / P = (2.50)(0.08206)(298.15) / 1.25 = 49.0 L. ### Worked Example: Dalton's Law **Problem.** A gas mixture contains 0.40 atm N2, 0.20 atm O2, and 0.10 atm CO2. What is the total pressure and the mole fraction of N2? P_total = 0.40 + 0.20 + 0.10 = 0.70 atm. Mole fraction of N2: X_N2 = P_N2 / P_total = 0.40 / 0.70 = 0.571. ### Real Gases: Van der Waals Equation (P + a(n/V)^2)(V - nb) = nRT The a-term corrects for intermolecular attractions. The b-term corrects for particle volume. Gases with strong IMFs (H2O, NH3) have large a values. Gases with large molecules have large b values. ## Phase Transitions | Transition | Direction | Energy change | Name | |---|---|---|---| | Solid to liquid | Melting | Endothermic | Fusion | | Liquid to gas | Boiling/evaporation | Endothermic | Vaporization | | Solid to gas | — | Endothermic | Sublimation | | Gas to liquid | — | Exothermic | Condensation | | Liquid to solid | Freezing | Exothermic | Solidification | | Gas to solid | — | Exothermic | Deposition | **Heating curve.** When heating a substance at constant pressure: temperature rises through the solid phase, plateaus at the melting point (energy goes to breaking lattice, not raising T), rises through the liquid phase, plateaus at the boiling point (energy goes to overcoming IMFs), then rises through the gas phase. **Worked example.** *How much energy is needed to convert 36.0 g of ice at -10.0 C to steam at 110.0 C?* **Step 1.** Heat ice from -10 to 0 C: q1 = m x c_ice x delta-T = 36.0 x 2.09 x 10.0 = 752 J. **Step 2.** Melt ice at 0 C: q2 = m x delta-H_fus = 36.0 x 334 = 12,024 J. **Step 3.** Heat water from 0 to 100 C: q3 = 36.0 x 4.184 x 100 = 15,062 J. **Step 4.** Boil water at 100 C: q4 = 36.0 x 2260 = 81,360 J. **Step 5.** Heat steam from 100 to 110 C: q5 = 36.0 x 2.01 x 10.0 = 724 J. **Total:** 752 + 12,024 + 15,062 + 81,360 + 724 = 109,922 J = 110 kJ. Note: the vaporization step dominates (74% of total energy). This is why steam burns are far more severe than hot water burns — the condensation of steam releases enormous energy. ## Phase Diagrams A phase diagram maps the stable phase as a function of temperature and pressure. **Key features:** - **Triple point:** The unique temperature and pressure where solid, liquid, and gas coexist in equilibrium. For water: 0.01 C, 0.006 atm. - **Critical point:** Above this temperature and pressure, the liquid-gas boundary disappears — the substance becomes a supercritical fluid. For water: 374 C, 218 atm. For CO2: 31 C, 73 atm. - **Normal boiling point:** Temperature where liquid-gas curve crosses 1 atm. - **Normal melting point:** Temperature where solid-liquid curve crosses 1 atm. **Water's anomaly.** Water's solid-liquid line slopes to the left (negative slope), meaning increasing pressure on ice at certain temperatures causes melting. This is because ice is less dense than liquid water — pressure favors the denser phase. Most substances have a positive-sloping solid-liquid line. ### Worked Example: Reading a Phase Diagram **Problem.** CO2 at 1 atm and -78.5 C is a solid (dry ice). What happens when you warm it at 1 atm? At 1 atm, CO2's triple point is at 5.1 atm — well above 1 atm. Therefore, the 1 atm line passes only through solid and gas regions. CO2 sublimes directly from solid to gas at -78.5 C without ever becoming liquid. This is why dry ice "smokes" but never forms a puddle. **To get liquid CO2:** you must exceed 5.1 atm. CO2 fire extinguishers operate at about 60 atm, where CO2 exists as a liquid. ## Vapor Pressure and Clausius-Clapeyron **Vapor pressure** is the pressure exerted by a substance's vapor in equilibrium with its liquid. It increases with temperature (more molecules have enough energy to escape the liquid). **Clausius-Clapeyron eq
Major art movements and their historical context for art education. Covers 12 movements from the Renaissance to contemporary art, their defining characteristics, key artists, signature works, and the intellectual/social forces that produced them. Use when analyzing artworks in historical context, understanding stylistic lineages, identifying influences across periods, or connecting studio practice to art-historical precedent.
Color theory principles for art education. Covers the three color properties (hue, saturation, value), color mixing systems (subtractive and additive), color relationships (complementary, analogous, triadic, split-complementary), color temperature, simultaneous contrast and the relativity of color perception, and practical palette construction. Use when analyzing color in artworks, planning color schemes, understanding optical phenomena in painting, or investigating Albers's Interaction of Color experiments.
The creative process in art from idea to exhibition. Covers five phases of creative work (inspiration, incubation, exploration, execution, reflection), sketchbook practice, artist statements, critique methodology (formal and conceptual), portfolio development, and the studio as a working environment. Use when guiding students through project development, facilitating critique sessions, developing artist statements, curating portfolios, or understanding how professional artists structure their creative practice.
Digital art tools, techniques, and workflows for art education. Covers raster and vector workflows, digital painting, photo manipulation, generative and procedural art, 3D modeling and rendering, pixel art, the relationship between traditional skills and digital execution, and ethical considerations of AI-generated imagery. Use when working with digital tools, evaluating digital art, or bridging traditional art concepts into digital practice.
Observational drawing and visual perception techniques for art education. Covers contour drawing, gesture drawing, negative space, proportion and measurement, value mapping, spatial depth cues, and the cognitive shift from symbolic to perceptual seeing. Use when teaching drawing fundamentals, analyzing observational accuracy, or developing visual literacy in any medium.
Three-dimensional art and sculptural thinking for art education. Covers additive and subtractive sculptural processes, armature construction, modeling in clay, carving principles, casting and moldmaking, assemblage and found-object sculpture, installation art as expanded sculpture, and the conceptual transition from pictorial to spatial thinking. Use when working with three-dimensional media, analyzing sculptural form, understanding spatial composition, or investigating the relationship between sculpture and site.
Celestial coordinate systems and sky positioning. Covers horizon (altitude-azimuth), equatorial (right ascension-declination), ecliptic, and galactic systems; epoch and precession; coordinate transformations; planisphere use; and practical sky-locating from any latitude and date. Use when locating objects, planning observations, converting catalog coordinates, or teaching the geometry of the sky.
Observational cosmology from Hubble's law to the CMB. Covers redshift, Hubble expansion, the cosmological parameters, the cosmic microwave background, large-scale structure, galaxy rotation curves and dark matter, Type Ia SNe and dark energy, and the current state of Lambda-CDM. Use when reasoning about the large-scale universe, interpreting cosmological surveys, or teaching the Big Bang evidence chain.