Rayleigh limit
Two equally bright point sources become hard to distinguish when their angular separation falls below this diffraction-limited scale.
Concept module
Image two nearby point sources through one finite aperture and see why diffraction, wavelength, and aperture diameter limit how sharply an optical system can separate them.
The simulation shows two distant point sources on the left, one finite lens aperture in the middle, and one detector strip on the right. Each source sends light through the same aperture, and the detector strip brightens according to the combined diffraction-limited image profile. Optional overlays show the aperture diameter on the lens, the current point-spread centers on the detector, and the Rayleigh blur scale around those centers. A movable detector sample marks one position on the strip and reports the current normalized exposure there. With wavelength 550 nm and aperture 2.4 mm, the Rayleigh limit is about 0.28 mrad. The current point separation is 0.32 mrad, which is 1.14 times that limit. The pair is near the Rayleigh threshold.
Interactive lab
Keep the stage, graph, and immediate control feedback in one working view.
Optical Resolution / Imaging Limits
A finite aperture turns each point into a diffraction blur. Aperture, wavelength, and source separation all stay tied to the same detector profile.
Resolution state
Graphs
Switch graph views without breaking the live stage and time link.
Image-plane profile
Shows the combined detector profile and the two individual point-spread contributions for the current aperture-limited image.
Controls
Adjust the physical parameters and watch the motion respond.
Longer wavelength broadens each point-spread blur.
A larger clear aperture improves resolving power by shrinking the diffraction pattern.
Sets how far apart the two object points are in angle.
Moves the live sample point along the detector profile.
More tools
Secondary controls, alternate presets, and less-used toggles stay nearby without crowding the main bench.
More presets
Presets
Predict -> manipulate -> observe
Keep the active prompt next to the controls so each change has an immediate visible consequence.
Try this
Equation map
Select a symbol to highlight the matching control and the graph or overlay it most directly changes.
Longer wavelengths broaden the diffraction blur, so nearby points become harder to distinguish.
Equations in play
Choose an equation to sync the active symbol, control highlight, and related graph mapping.
More tools
Detailed noticing prompts, guided overlays, and challenge tasks stay available without taking over the main bench.
What to notice
Use one prompt at a time so the aperture, the detector strip, and the graph stay tied to the same live resolution story.
Try this
Why it matters
Guided overlays
Focus one overlay at a time to see what it represents and what to notice in the live motion.
Overlay focus
Marks the clear aperture diameter directly on the lens.
What to notice
Why it matters
It keeps resolving power attached to the aperture geometry instead of treating blur as a mysterious screen effect.
Challenge mode
Use the real aperture-limited detector profile to hit resolution targets instead of switching to a detached puzzle model.
2 of 4 checks
Suggested start
The checklist updates from the live simulation state, active graph, overlays, inspect time, and compare setup.
Rayleigh limit
Two equally bright point sources become hard to distinguish when their angular separation falls below this diffraction-limited scale.
Image-plane spacing
At fixed focal length, angular separation maps to detector spacing.
Image-plane blur radius
The same diffraction limit can be read as the characteristic size of one point-spread core on the detector.
Progress
Not startedMastery: NewLocal-firstStart exploring and Open Model Lab will keep this concept's progress on this browser first. Challenge mode has 2 compact tasks ready. No finished quick test, solved challenge, or completion mark is saved yet.
Try this setup
Copy the live bench state and reopen this concept with the same controls, graph, overlays, and compare context.
Stable links
Starter track
Step 5 of 50 / 5 completeEarlier steps still set up Optical Resolution / Imaging Limits.
Previous step: Dispersion / Refractive Index and Color.
Short explanation
An imaging system does not send each object point to a mathematically perfect point on the detector. A finite aperture diffracts the light, so each point becomes a blur pattern with a finite width.
This page keeps that story bounded on purpose: two equal point sources, one finite lens aperture, and one detector strip. The same wavelength, aperture diameter, point separation, and detector sample drive the stage, the profile graph, the overlays, the worked examples, the prediction prompts, the challenge checks, and the quick test so imaging limits stay tied to one honest diffraction-limited picture instead of a giant Fourier-optics platform.
Key ideas
Live worked example
550 nm nm
2.4 mm mm
0.28 mrad mrad
1. Start from the Rayleigh estimate
2. Substitute the live wavelength and aperture
3. Map that blur scale onto the detector
Current Rayleigh limit
Common misconception
If the lens is focused correctly, two nearby points should always stay perfectly separate.
Correct focus removes defocus blur, but it does not remove diffraction from a finite aperture.
That is why nearby points can still merge when the aperture is small or the wavelength is long, even in an otherwise ideal imaging setup.
Mini challenge
Prediction prompt
Check your reasoning
Quick test
Variable effect
Question 1 of 4
Choose one answer to reveal feedback, then test the idea in the live system if a guided example is available.
Accessible description
The simulation shows two distant point sources on the left, one finite lens aperture in the middle, and one detector strip on the right. Each source sends light through the same aperture, and the detector strip brightens according to the combined diffraction-limited image profile.
Optional overlays show the aperture diameter on the lens, the current point-spread centers on the detector, and the Rayleigh blur scale around those centers. A movable detector sample marks one position on the strip and reports the current normalized exposure there.
Graph summary
The graph shows normalized exposure against detector height, with one combined profile and two dashed component profiles for the individual point-spread contributions.
Hovering the graph previews the matching detector position on the stage, so the spatial profile stays linked to the same image plane rather than turning into a detached time plot.
Read next
These suggestions come from the concept registry, so the reason label reflects either curated guidance or the fallback progression logic.
Use two coherent slits and one screen to connect path difference, phase difference, and fringe spacing to wavelength, slit separation, and screen distance on one compact optics bench.
Trace principal rays through converging and diverging lenses, connect the signed thin-lens equation to the diagram, and watch image distance and magnification respond to the same object setup.
Watch a wave spread after one narrow opening, see why diffraction grows when wavelength competes with slit width, and build the wave-optics bridge toward double-slit interference.