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CED objectives

Emission and Absorption Spectra

▶︎  Watch it animatedinteractive step-through · ~3 min · optional ⚙︎  Open the appletLevel Ladder · choose where the atom starts and finishes, and let the subtraction decide whether a photon comes out or goes in

Bound-state energies are negative because zero is defined at the ionized state, so $-13.6$ eV is hydrogen's lowest level and the levels stack upward toward zero. A transition emits or absorbs a photon whose energy is the difference between two levels, so hydrogen falling from $n = 3$ to $n = 2$ emits $1.89$ eV at $656$ nm. Absorption takes energy in and moves the atom up a level while emission gives it out and drops the atom down, which is why an element shows the same wavelengths as bright lines or as dark gaps. Ionization is the jump to $E = 0$, costing $13.6$ eV from hydrogen's ground state, and any surplus becomes kinetic energy of the freed electron.

Four errors dominate. Ranking levels by the size of the number, so $-13.6$ eV reads as the highest level and every arrow on the diagram reverses. Setting a photon's energy equal to a single level rather than to the difference between two. Having the atom emit to climb and absorb to drop, or reading the dark lines in a stellar spectrum as light the gas produced. And treating ionization as a transition to the highest level drawn rather than to zero binding energy.

put the values on a number line and every arrow follows 0 eV: ionized, electron free n = 4, −0.85 n = 3, −1.51 n = 2, −3.40 n = 1, −13.6: LOWEST EMISSION, down: 1.89 eV out ABSORPTION, up: 1.89 eV in IONIZATION: to 0, costs 13.6 eV ranking by magnitude puts the ground state at the top and reverses every arrow here
The same 1.89 eV labels both the up arrow and the down arrow. Which direction it goes is what absorption and emission name.
one element, one set of wavelengths, two ways of seeing it EMISSION: bright lines on a dark field a hot gas dropping down between levels ABSORPTION: dark gaps cut from a continuum a cooler gas climbing up, removing those wavelengths on the way to the detector
The four positions are identical in both strips, because the same level differences produce them. Only the direction of the transition differs.

The work

3 ways in · any order
Lesson
Emission and Absorption Spectra

Puts the negative level energies on a number line, takes each photon's energy from a difference between two levels, points absorption up and emission down, and locates ionization at zero binding energy.

Skill check · 10 scenarios
Diagnostic
10-item topic check

Ten items spanning the failure modes of this topic: ranking levels by magnitude, taking a photon's energy from one level, reversing emission and absorption, and treating ionization as a jump to the highest level drawn. Take it cold to find which one is yours, or after the lesson to confirm it is not.

Not started · 10 items · ~15 min
Targeted Practice
Drill a single misconception

Pick one of the failure modes you missed and drill it on its own. The round is adaptive: two correct in a row clears it for now and moves you to the next. Two in a row is a checkpoint, not proof: if the error resurfaces later, the misconception comes back.

Take the diagnostic to identify your misconceptions