Atomic Structure & Theory

For a first approximation, an atom is similar to a solar system--dense nucleus in the middle, electrons spinning around it. Theories that account for atomic structure are quantum physics and Einstein's mass-energy conversion. The nucleus is built of protons and neutrons (nucleons). Mass-energy conversion shows up when nucleons lose a tiny bit of mass when bound together. Electron clouds sculpted into orbitals (see second illustration) give atoms their observed structure.
  1. Quantum Physics

    • Prior to observation in the box, the cat is, quantum-ly speaking, dead AND alive. The image is a reference to how the idea was first presented: the cat in the box is at risk of dying if observed.

      Quantum physics properties, such as energy-position uncertainty, are unfamiliar to our experience. Strange as it may be, quantum physics accounts for observed atomic structure and behavior.

    Protons and Neutrons

    • Nucleons (protons and neutrons) make up the core of the atom. In the solar-system model, the nucleus is the "sun."

    Mass-Energy Conversion

    • Mass-energy conversion is relevant within the nucleus. Proton and neutron masses are slightly smaller when bound in a nucleus then when floating by themselves. As atoms form, the mass-converted-to-energy process is what keeps stars (and H-bombs) shining.

    Electron Cloud

    • Imagine electrons as hazy "probability clouds" of various shapes. Finding an electron some distance from the nucleus is never a certainty in the way that finding a rock some distance from a slingshot is---the "cloud" title derives from this.

    Orbital Shape

    • Atomic orbital illustrations. An electron is likely to be found in brighter regions and almost certainly never observed in dark regions.

      The "probability clouds" (orbitals) aren't scattered haphazardly around the nucleus. Orbital shapes depend on electron number and light absorption by the atom. Outermost orbitals form the (likewise hazy) boundary of an atom.

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