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SCIENCE · INVESTIGATE AND EXPLAIN

Identify a pattern with multiple lines

Retain one-feature ambiguity and test a single-species hypothesis using additional distinct transitions.

Learning outcome: Calculate residuals and use multiple features without inventing certainty or treating unreported lines as nondetections.

Starting recap

Compatibility requires each revealed feature to match a distinct selected transition of one listed species within ±0.10 nm.

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Try

A’s first feature matches H I and He I; its second feature at 486.13 nm leaves selected H I compatibility.

Open the experiment

Predict

Does the closest of two passing reference wavelengths justify a unique identification from one feature?

Experiment

Capture A and B with the first feature only, calculate their candidate residuals, then reveal all recorded features and compare the changes.

Compare spectral features and independent calibration

Fictional spectrum records · selected atomic reference comparisons · Seven fictional supplied records compared with eight selected NIST air-wavelength values for neutral H, He and Na. Inclusive +/-0.10 nm is a teaching compatibility tolerance, not a source uncertainty or line width. Every revealed feature must map to a distinct selected transition of one species. Unreported lines never imply absence. Before calibration, zero offset is provisional. No measured stellar spectrum, abundance analysis, temperature inference, Doppler fitting or complete catalogue is supplied.

Reset keeps your prediction, captures and practice history.

A: emission pattern: emission. These are fictional supplied feature positions. Reference markers are selected neutral-atom transitions, not a complete list of lines. Roman numeral I means neutral.

Provisional comparison: calibration not yet supplied. Applied subtraction: 0.00 nm. Raw observations stay unchanged as evidence is revealed.

Air wavelength (nm) · feature positions, not intensity380400450500550600650690Raw recordCorrected recordH I referencesHe I referencesNa I referencesTinted record spans: coverage. Outside each span: unavailable, not zero light.
Detail: 388.4–389.4 nm · same fixed scale for every caseCorrected featuresH I referenceHe I reference388.4388.6388.8389.0389.2389.4Features outside this window are not moved into the inset.

The ±0.10 nm matching tolerance is stipulated for this exercise. It is not a confidence interval, NIST uncertainty, line width or instrument resolution. No line strengths are measured here.

Supplied features and independent correction (nm in air)
FeatureRaw centerCorrected centerAvailability
1388.90000388.90000Supplied
2Not yet revealedNot yet revealedRecorded, unrevealed

1 revealed feature(s). Raw coverage: 380.00–680.00 nm. Corrected coverage: 380.00–680.00 nm. An unreported reference line is not negative evidence, even inside the covered interval. A narrow record cannot supply a second feature merely because a later evidence stage is selected.

Can ONE listed species explain every revealed feature using distinct selected transitions?
SpeciesResultFirst compatible assignment: feature → reference; signed residual
H ICompatible within this library

1 → h-388 (388.90490 nm); -0.00490 nm

He ICompatible within this library

1 → he-388 (388.86489 nm); 0.03511 nm

Na INo complete assignmentNo assignment claimed.

Several listed patterns remain compatible. More discriminating observed features are needed.

A match is conditional support within this selected-line, single-species comparison. It does not establish abundance, stellar temperature or complete composition. Failure may reflect a mixture, omitted transitions, motion or calibration; it does not prove an element absent.

Inspect the independent calibration record

Not yet supplied. Select the calibration evidence stage. Zero subtraction at earlier stages is provisional, not evidence of a calibrated instrument.

Compare schematic spectrum types

These drawings show patterns, not measured heights or a model of a stellar atmosphere. All three use the same schematic horizontal wavelength direction.

Schematic only · wavelength increases to the rightContinuousEmissionAbsorption

A hot dense source can supply a continuum; excited low-density gas can supply emission lines; cooler gas along the view of a continuum source can produce absorption features. The corresponding transition positions may coincide while strengths depend on physical conditions. A dark line is reduced light at selected wavelengths, not no light everywhere.

Inspect selected reference wavelengths and sources
Selected NIST air wavelengths; source angstroms divided by ten
ID / speciesSource Ånm in airSource row
h-388 / H I3889.049388.90490RCWM80
h-434 / H I4340.462434.04620MK00a
h-486 / H I4861.2786486.12786MK00a
he-388 / He I3888.6489388.86489M02
he-447 / He I4471.479447.14790M60a
he-587 / He I5875.6148587.56148M02
na-588 / Na I5889.950588.99500R56
na-589 / Na I5895.924589.59240R56

Selected factual values from J. E. Sansonetti and W. C. Martin, NIST Handbook of Basic Atomic Spectroscopic Data, SRD 108, accessed 26 October 2026. These are selected multiplet components, not intensity-weighted centroids. Source intensities and database tables are not reproduced. NIST distinguishes Standard Reference Data licensing from ordinary federal works; no public-domain or CC license is asserted for the compilation. NIST accuracy disclaimer. Synthetic records and diagrams are authored teaching material.

Scientific context: NASA introduction to spectra and NASA on stellar composition and temperature. This comparison is not a stellar-atmosphere simulation.

2 compatible listed patterns: H I, He I.

Calibration is not yet revealed; this is a provisional zero-offset comparison. Several listed patterns remain compatible. More discriminating observed features are needed.

Captures preserve the supplied spectrum record and evidence stage. Replaying compares fictional feature positions with selected reference transitions; it is not a new measurement, complete stellar classification or abundance analysis.

Understand

Preserve the ambiguity before adding evidence

Select record A with only its first feature revealed. The supplied center is 388.90 nm. It is close to both a selected hydrogen reference at 388.9049 nm and a helium reference at 388.86489 nm. Before revealing another feature, write both candidates in your notebook.

Compute signed residuals as supplied center minus reference. For hydrogen the residual is −0.00490 nm; for helium it is +0.03511 nm. Both absolute differences are smaller than the stipulated 0.10 nm tolerance. The closer numerical match does not automatically become a unique identification: the model retains every compatible candidate instead of inventing a probability ranking.

The selected source wavelengths are from the air sections of the NIST hydrogen and helium tables. They identify specific listed transitions rather than calculated centroids of neighboring components. The exercise does not model resolved multiplet shapes.

Use a second feature to test the hypothesis

Reveal all recorded features in A. The second center is 486.13 nm, close to the selected H I reference 486.12786 nm. Its residual is +0.00214 nm. The selected helium references cannot explain this second feature, so hydrogen remains the compatible single-species candidate under the stated comparison.

Now inspect B. Its first feature, 388.88 nm, is also compatible with both nearby references. Its second feature is 447.15 nm, matching the He I reference 447.1479 nm with residual +0.00210 nm. The added evidence selects a different compatible single-species hypothesis.

Make a two-row paper ledger for each case. Include raw center, candidate reference, signed residual and pass/fail against the tolerance. Capture the ambiguous state before the additional feature. Otherwise, a final candidate list can hide the reasoning that made the second observation useful.

Define exactly what compatibility means

The question is whether every revealed feature can be associated with a distinct selected transition of one listed neutral species. A feature cannot borrow one transition twice to explain two separate observed features. This one-to-one assignment requirement prevents duplicate use of the same reference from creating false multi-line support.

The candidate universe is small: H I, He I and Na I, with only eight selected reference wavelengths altogether. Compatibility is not a proof that the source contains only that element. Failure means the particular selected-line single-species hypothesis does not explain every revealed feature, not that the species is absent from the source.

There is also no requirement that every reference transition appear in the supplied record. The listed features are selected reports, not a complete detection inventory. An unreported line must not be treated as a verified nondetection, even when its wavelength lies within the covered interval.

Check another pattern and the units

Record C supplies 589.00 and 589.59 nm. Compare these with selected Na I references 588.9950 and 589.5924 nm. The residuals are +0.00500 and −0.00240 nm, so two distinct selected sodium transitions explain the pair within tolerance. NIST sodium references.

The tolerance is an authored rule for simplified records. It is neither a confidence interval nor the precision of the reference source. Perform comparisons using the full listed values rather than rounding everything to one decimal place first. Rounding near a tolerance boundary can change a decision.

At stages before calibration is revealed, these comparisons assume zero offset provisionally. A pattern that becomes incompatible after adding evidence cannot regain compatibility simply by ignoring the inconvenient line. A separately supported calibration correction is a different operation, explored next.

Transfer to a new supplied pair

A paper record has independently confirmed zero offset and centers 434.05 and 486.12 nm. Compare them with the selected hydrogen references 434.0462 and 486.12786 nm. Do both pass, and what claim remains too strong?

Check the spectrum-patterns transfer

The residuals are +0.0038 and −0.00786 nm, both within ±0.10 nm and associated with distinct H I transitions. The pair is compatible with the selected single-species hydrogen hypothesis. It does not establish that the source contains only hydrogen or determine its abundance.

Apply

A first feature within tolerance of both H I and He I supports:

Public practice checks a specific claim. It does not establish independent mastery.

Explain the value of a second feature, the one-to-one matching rule and the limits of the eight-line reference subset.

Continue

Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.

Skipping retains experiments and awards no mastery.

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