Standards Alignment
NGSS Alignment
Atomency was built from the ground up around the Next Generation Science Standards. Every feature maps to specific high school performance expectations, disciplinary core ideas, and science and engineering practices.
NGSS performance expectations are three-dimensional — they integrate Disciplinary Core Ideas (DCI), Science and Engineering Practices (SEP), and Crosscutting Concepts (CCC). Atomency is designed to support all three dimensions, not just content delivery.
Performance Expectations Covered
HS-PS1-1
Periodic table as a model — electron configurations, periodic trends
HS-PS1-2
Explaining chemical reactions from electron states and bonding patterns
HS-PS1-6
Equilibrium, Le Chatelier's Principle, shifting conditions
HS-PS1-7
Conservation of mass — balanced chemical equations
HS-PS1-8
Nuclear decay, fission, fusion — changes in the nucleus
HS-PS2-6
Molecular-level structure and its role in material properties
HS-PS3-4
Gas laws — energy, pressure, temperature, volume relationships
HS-ESS1-1
Nuclear processes in stars — fusion, energy release, element formation
HS-PS1-1
Periodic Table as a Model
Students use the periodic table to predict bonding behavior and electron configuration. The molecular builder visualizes how group and period position determines valence, bond count, and resulting geometry — directly operationalizing the periodic table as a predictive model.
HS-PS1-2
Constructing Explanations for Chemical Reactions
By placing atoms and observing bond formation in real time, students develop and revise explanations for why certain elements bond the way they do based on electron states, electronegativity differences, and bond polarity.
HS-PS2-6
Molecular Structure and Material Properties
The molecular property panel surfaces boiling point, polarity, bond type, and formal charges for every structure. Students directly observe how molecular-level geometry drives macroscopic properties.
HS-PS1-2
Explaining Reaction Outcomes
The simulator derives reaction type and products from element properties — no lookup table. Students see how electron configuration and electronegativity drive reaction classification, building the mechanistic reasoning NGSS requires.
HS-PS1-7
Conservation of Mass in Chemical Reactions
Every reaction produced by the simulator is fully balanced using Gaussian elimination. Atom counts on both sides are equal and displayed — giving students a direct mathematical representation of conservation of mass.
HS-PS1-7
Mathematical Representations of Atom Conservation
Directly supports the core mathematical practice of this standard — using stoichiometric coefficients to demonstrate that atoms are conserved. Works for any reaction across all 118 elements with no hardcoded cases.
HS-PS1-8
Nuclear Composition Changes and Energy Release
Students develop and interact with dynamic models of radioactive decay — observing changes in proton and neutron count, decay mode selection, half-life behavior, and the visual nuclear equation for every step in a decay chain. The simulator is the core model this standard asks students to develop.
HS-ESS1-1
Nuclear Processes in Stars
Fusion modeling and heavy element decay chains connect to stellar nucleosynthesis. The nuclear equation display makes visible how element transmutation occurs — grounding the ESS1 concept in a manipulable physical model.
HS-PS1-6
Chemical Equilibrium and Le Chatelier's Principle
Students directly manipulate concentration, temperature, and pressure conditions to observe equilibrium shifts. The ICE table and equilibrium constant calculations are shown step by step, fulfilling the mathematical and modeling expectations of this standard.
HS-PS3-4
Energy, Temperature, and Thermal Systems
The kinetic molecular theory simulation makes visible the relationship between temperature, particle speed, and pressure — grounding the macroscopic gas laws in particle-level behavior. Students can plan and observe how changing one variable redistributes energy across a system.
Disciplinary Core Idea Coverage
PS1.A
Structure and Properties of Matter
Periodic table, molecular builder, VSEPR, property panels
PS1.B
Chemical Reactions
Reaction simulator, equation balancer, kinetics
PS1.C
Nuclear Processes
Nuclear decay simulator, decay chains, fusion modeling
PS2.B
Types of Interactions
Bond type classification, ionic vs. covalent, electronegativity
PS3.B
Conservation of Energy
Gas laws, KMT, enthalpy estimation in reaction simulator
ESS1.A
The Universe and Its Stars
Nuclear fusion modeling, heavy element decay chains
Science & Engineering Practices Supported
SEP 2
Developing and using models — molecular builder, nuclear decay, gas laws
SEP 5
Using mathematics — equation balancer, ICE tables, gas law calculations
SEP 6
Constructing explanations — reaction simulator, bonding analysis
SEP 8
Obtaining, evaluating, and communicating information — PubChem integration, export