Newton's Rings

Rest a slightly curved lens on a flat sheet of glass, shine sodium light down on it, and a bull's-eye of dark and bright circles springs into view — tightly packed far out, widely spaced near the middle, and, most tellingly, dark at the very point where the two glasses touch. These are Newton's rings, and they are a ruler written in light. The thin film here is not a soap bubble or an oil slick but the sliver of trapped air between the lens and the plate, a wedge that is zero thickness at the contact point and thickens outward as t≈r2/2Rt\approx r^2/2R. Light reflected from the bottom of the lens and from the top of the plate interferes, and because the gap depends only on how far you are from the centre, the fringes of constant thickness are perfect circles. The dark centre is the detail that made this pattern historically decisive. Where the glasses touch there is no gap at all, so naively the two reflections should arrive in step and blaze bright — yet the spot is black. The resolution is a half-wave: the reflection off the plate (air into denser glass) flips the wave's sign, while the reflection off the lens (glass into rarer air) does not, so the two beams meet exactly out of phase at contact. That extra π\pi, owned here by reversibility (recalled by name from aq-optics-stokes-relations-phase-reflection), is why a plain measurement of ring radii turns into a wavelength-accurate assay of a lens's curvature — and why the same rings still certify the flatness of optical surfaces to a fraction of a wavelength today.

Key takeaways
  • Newton's rings are circular fringes of equal thickness formed by amplitude-splitting interference in the air gap between a convex lens (radius of curvature RR) and a flat plate.
  • The gap grows quadratically, t≈r2/2Rt\approx r^2/2R, so equal-thickness contours are concentric circles and ring radii scale as m\sqrt{m} — crowded outward, sparse near the centre.
  • The point of contact is dark in reflection because the plate reflection adds a half-wave (π\pi) that the lens reflection does not — the signature of the pattern.
  • Dark rings (air, near normal) sit at rm=mλRr_m=\sqrt{m\lambda R}; plotting rm2r_m^2 against order gives a straight line of slope λR\lambda R, the route to RR or λ\lambda.
  • A liquid of index nn in the gap shrinks every radius by 1/n1/\sqrt{n} — a one-line refractometer.
  • Key idea: the quadratic air gap t≈r2/2Rt\approx r^2/2R plus the half-wave flip at the plate put reflected dark rings at rm=mλRr_m=\sqrt{m\lambda R}, with a dark centre — so rm2r_m^2 is linear in ring order and reads out RR or λ\lambda.
The core insight

Between a sphere of radius RR and a flat, the trapped-gap thickness grows as t≈r2/2Rt\approx r^2/2R. A half-wave phase shift at the lower (air-to-glass) reflection makes the contact point dark, and destructive interference then places dark rings at rm=mλRr_m=\sqrt{m\lambda R} in air. Ring radii grow as m\sqrt{m}, so rm2r_m^2 is exactly linear in order — the slope is λR\lambda R, and the pattern becomes a metrology tool.

Where this lives today

Newton's rings never left the optical shop. Lay a precision test flat on a lens or mirror under monochromatic light and the equal-thickness fringes map the air gap between them: a perfectly figured surface gives clean circles, and every departure — a turned edge, a low zone, a scratch — bends a fringe by an amount that reads the height error to a small fraction of a wavelength. Counting or fringe-analysing these patterns is how flats, prisms, and lens surfaces are still certified to λ/10\lambda/10 or better, and modern phase-shifting interferometers are just this idea automated with a piezo-scanned reference and a camera. The same physics shows up as a nuisance to be engineered away. Wherever two nearly-flat surfaces are pressed together — a phone screen laminated to its glass, a photographic negative in a scanner gate, two bonded optical windows — a thin residual air gap breeds unwanted Newton's rings that mar the image. The cures are all gap control: index-matching fluids or adhesives to erase the optical path difference, deliberate anti-Newton-ring textures to break the coherence of the gap, or vacuum bonding to remove the air entirely. The dark centre that puzzled Newton is now a manufacturing spec.

The physical picture

Think of the air gap as a very shallow wedge, flat at the middle and opening up as you move outward. A ray coming down is split into two: a little reflects off the curved underside of the lens, and the rest crosses the gap and reflects off the flat plate below. The second beam travels an extra round trip 2t2t through the gap before rejoining the first, and wherever that extra path — with the reflection phase folded in — lands the two beams out of step, you see a dark ring. Because tt is fixed by radius alone, "out of step" happens on circles, and the eye reads off a set of concentric rings centred on the contact point.

Figure
Cross-section: a convex lens on a flat plate traps an air wedge t(r) ≈ r²/2R; the lens reflection carries no phase flip, the plate reflection adds +π
A sphere of radius R resting on a flat: the trapped air gap thickens as t(r) ≈ r²/2R lens (glass) plate (glass) air gap contact, t = 0 incident glass→air: no flip air→glass: +π t(r) r The two reflected beams differ by 2t plus a half-wave; equal-thickness contours are circles ⟹ concentric rings.

The half-wave shift is the crux of the whole pattern, and it is worth being precise about. At the contact point the geometric gap is exactly zero, so the two reflected beams travel identical distances. If reflection were phase-neutral they would arrive perfectly in step and the centre would be bright. Instead, the beam bouncing off the plate is reflecting from air into denser glass — an external reflection that flips its sign by π\pi — while the beam bouncing off the lens reflects from glass into rarer air and keeps its sign. The net half-wave difference survives all the way to t=0t=0, so the centre is dark. This asymmetry between the two reflections is exactly the content of the Stokes reversibility relations; here we simply use its verdict. The other fingerprint is the spacing. Because the gap is quadratic in radius, equal steps in optical path do not correspond to equal steps in radius: the rings are widely spaced near the centre and crowd together as you go out, with radii climbing as m\sqrt{m}. Squaring undoes the crowding — rm2r_m^2 marches up in equal steps of λR\lambda R — and that clean linearity is what makes the pattern a measuring instrument rather than a curiosity.

Figure
Punchline: dark-ring radius rises as √m along a line of slope √(λR); marked points r₁ = 2.43 mm, r₅ = 5.43 mm, r₁₀ = 7.68 mm for Na light (589.3 nm), R = 10 m
The measuring line: dark-ring radius vs √m is straight, slope √(λR) = 2.43 mm 0 2 4 6 8 ring radius r (mm) √m (square root of dark-ring order) 0 1 2 3 m=1: 2.43 mm m=5: 5.43 mm m=10: 7.68 mm m=0: dark centre r = √(λR)·√m

The core equations

Everything starts with the shape of the gap. A sphere of radius RR dropped onto a plane makes a gap whose depth is the sagitta of the arc: exact geometry gives a square-root, but for the shallow gaps of a large-RR lens (millimetre radii, metre-scale RR) it collapses to a parabola. This one approximation is why the rings scale as m\sqrt{m}.

t(r)=R−R2−r2  ≈  r22R(r≪R)(1)t(r) = R-\sqrt{R^2-r^2} \;\approx\; \frac{r^2}{2R} \qquad (r \ll R) \qquad (1)

where: tt — local gap thickness; RR — radius of curvature of the lens surface; rr — radial distance from contact. The approximation drops a term of order r4/R3r^4/R^3, utterly negligible when r/R∼10−4r/R \sim 10^{-4}. The two reflected beams differ by the round trip 2t2t across the gap, plus one crucial half-wave. Of the two reflections only the lower one — air into the denser plate — is external and flips the phase by π\pi; the upper one, glass into rarer air, does not. Near normal incidence cos⁡θt→1\cos\theta_t\to1 and the geometric term is simply 2nt2nt.

Δ=2ntcos⁡θt+λ2  ≈  2nt+λ2(2)\Delta = 2nt\cos\theta_t + \frac{\lambda}{2} \;\approx\; 2nt + \frac{\lambda}{2} \qquad (2)

where: Δ\Delta — optical path difference of the two reflected beams; nn — index of the medium in the gap (n=1n=1 for air); θt\theta_t — refraction angle in the gap (near normal here); λ\lambda — vacuum wavelength; the λ/2\lambda/2 is the half-wave stamped on by the plate reflection (owned by aq-optics-stokes-relations-phase-reflection, recalled here). Because Δ=λ/2\Delta=\lambda/2 already at t=0t=0, the centre is dark. Setting Δ\Delta to a destructive half-integer of λ\lambda cancels the λ/2\lambda/2 on both sides and leaves an integer condition on the geometric path, which the sagitta turns into ring radii. Dark rings are the natural thing to count in reflection because the strong, high-contrast fringes are the dark ones bracketing bright annuli.

rm dark=mλRn,rm bright=(m−12)λRn(3)r_m^{\,\text{dark}} = \sqrt{\frac{m\lambda R}{n}}, \qquad r_m^{\,\text{bright}} = \sqrt{\frac{\left(m-\tfrac12\right)\lambda R}{n}} \qquad (3)

where: mm — ring order; dark m=0,1,2,…m=0,1,2,\dots (with m=0m=0 the central dark spot), bright m=1,2,3,…m=1,2,3,\dots. In air (n=1n=1) this is rm=mλRr_m=\sqrt{m\lambda R}; the 1/n1/\sqrt{n} is the refractometry lever. Absolute ring orders are hard to pin down — the innermost rings are smeared by imperfect contact and dust — so the workhorse relation for measurement differences two rings, cancelling any constant offset and the unknown zero order entirely.

rm+p2−rm2=p λRn(4)r_{m+p}^2 - r_m^2 = \frac{p\,\lambda R}{n} \qquad (4)

where: pp — number of orders between the two measured rings. The slope of rm2r_m^2 versus order is λR/n\lambda R/n, from which RR (known λ\lambda) or λ\lambda (known RR) drops out with no need to know mm absolutely.

Derivation ARing radii from the air gap and the half-wave reflection

The goal is to turn the geometry of a sphere on a plane into the ring-radius law and, along the way, to prove the one counter-intuitive fact — that the point of contact is dark, not bright. We take near-normal monochromatic light on a plano-convex lens (curved side down) resting on a flat plate, with a medium of index nn filling the gap, and follow the two reflected beams from the sagitta through the destructive-interference condition.

Step 1. Read the gap depth off the circle: the right triangle from the sphere's centre gives R2=r2+(R−t)2R^2=r^2+(R-t)^2, so t=R−R2−r2t=R-\sqrt{R^2-r^2}, and dropping t2t^2 against 2Rt2Rt leaves t≈r2/2Rt\approx r^2/2R. Why: for a large-RR lens the gap is a shallow parabola, which is exactly what makes ring radii grow as m\sqrt{m} rather than linearly.

Step 2. Write the path difference of the two reflected beams as Δ=2nt+λ/2\Delta=2nt+\lambda/2. The round trip across the gap contributes 2nt2nt; the extra λ/2\lambda/2 is the half-wave flip on the external reflection at the plate (air into denser glass), which the internal reflection at the lens does not share. Why: only the sign-flipping reflection adds a half-wave, and that asymmetry — the Stokes result — is the entire reason the centre behaves oddly.

Step 3. Impose destructive interference for dark rings, Δ=(m+12)λ\Delta=(m+\tfrac12)\lambda. The λ/2\lambda/2 appears on both sides and cancels, leaving the clean integer condition 2nt=mλ2nt=m\lambda. Why: the reflection phase does not disappear — it silently renumbers the fringes, which is why counting from the wrong reference biases RR.

Step 4. Substitute the sagitta, 2n (rm2/2R)=mλ2n\,(r_m^2/2R)=m\lambda, i.e. nrm2/R=mλn r_m^2/R=m\lambda, and solve: rm=mλR/nr_m=\sqrt{m\lambda R/n}, which is mλR\sqrt{m\lambda R} in air. Why: this is the owned result — a direct, measurable link from a ring radius to λ\lambda, RR, and the gap medium.

Step 5. Evaluate at the centre, m=0m=0: then r0=0r_0=0 and Δ=λ/2\Delta=\lambda/2, a purely destructive half-wave. The contact point is dark in reflected light. Why: with zero geometric path the reflection phase is all that is left, and it is exactly antiphase — the black spot that defeated a purely geometric reading of the pattern. *Verified symbolically (t=R−R2−r2→r2/2Rt=R-\sqrt{R^2-r^2}\to r^2/2R; Δ=(m+12)λ⇒2nt=mλ\Delta=(m+\tfrac12)\lambda\Rightarrow 2nt=m\lambda) and numerically (r1,5,10r_{1,5,10} for Na light, dark centre) in verify_aq-optics-newtons-rings.py.*

Go deeper · Derivation B · 1 minReading R or λ off the rings, offset and all
Derivation BReading R or λ off the rings, offset and all

Real Newton's-ring data never come with a trustworthy absolute order: the glasses never touch perfectly, so a small residual gap and dust shift the innermost fringes and hide the true m=0m=0. The goal here is to show that this ignorance costs nothing — a straight-line fit of squared radii, or better a difference of two rings, returns RR (or λ\lambda) cleanly, independent of the unknown offset.

Step 1. Allow an imperfect contact as a constant extra gap t0t_0, so the effective thickness is t=r2/2R+t0t=r^2/2R+t_0 and the dark condition 2nt=m′λ2nt=m'\lambda becomes nr2/R+2nt0=m′λn r^2/R + 2n t_0 = m'\lambda with m′m' an unknown integer relabelling. Why: modelling the defect as a constant offset captures exactly what a bad contact does — it shifts orders without changing the ring spacing.

Step 2. Rearrange to r2=(λR/n) m′−2Rt0r^2=(\lambda R/n)\,m' - 2R t_0: the squared radius is linear in the labelled order, with slope λR/n\lambda R/n and an intercept that swallows the offset. Why: the physics of interest lives entirely in the slope, so the nuisance parameter is quarantined in the intercept.

Step 3. Fit rm2=(λR/n) m+Cr_m^2=(\lambda R/n)\,m + C to the measured rings with any consistent integer labelling; the slope yields R=n⋅slope/λR=n\cdot\text{slope}/\lambda (or λ\lambda if RR is known), untouched by CC. Why: least-squares on a line is robust and self-averaging, which is why this is the standard undergraduate determination of a lens radius.

Step 4. Better still, difference two rings: rm+p2−rm2=pλR/nr_{m+p}^2-r_m^2=p\lambda R/n, so R=n(rm+p2−rm2)/(pλ)R=n(r_{m+p}^2-r_m^2)/(p\lambda) with CC gone entirely. For r5=5.43r_5=5.43 mm and r10=7.68r_{10}=7.68 mm in air at 589.3589.3 nm, this returns R=10.0R=10.0 m. Why: differencing eliminates the offset exactly rather than merely fitting around it — the cleanest single-number extraction. *Verified: the offset cancellation and R=(r102−r52)/(5λ)=10.0R=(r_{10}^2-r_5^2)/(5\lambda)=10.0 m in verify_aq-optics-newtons-rings.py.*

Go deeper · Derivation C · 1 minFilling the gap: refractometry and the complementary transmitted pattern
Derivation CFilling the gap: refractometry and the complementary transmitted pattern

Two further facts make the rings more than a curvature gauge: a liquid in the gap shrinks them in a way that measures the liquid's index, and the pattern seen in transmission is the photographic negative of the one in reflection, with a bright centre. The goal is to derive both from the same optical path difference, changing only the medium and the reflections counted.

Step 1. Replace air by a medium of index nn: the geometric round trip is unchanged but the optical path becomes 2nt2nt, so the dark condition 2nt=mλ2nt=m\lambda gives rm=mλR/nr_m=\sqrt{m\lambda R/n} — every radius multiplied by 1/n1/\sqrt n. Why: interference tracks optical, not geometric, path, so a denser gap packs the same number of wavelengths into a smaller radius.

Step 2. Turn it into a measurement: comparing a dry and a wet ring of the same order gives n=(rmair/rmliq)2n=(r_m^{\text{air}}/r_m^{\text{liq}})^2, an absolute index from pure geometry. For water, 1/1.33=0.8671/\sqrt{1.33}=0.867, so the rings shrink by about 13%13\%. Why: the ratio cancels mm, λ\lambda, and RR, leaving the index alone — a refractometer with no calibration standard.

Step 3. Now count reflections for the transmitted beams. The directly transmitted beam suffers no reflection; the twice-reflected beam that also emerges below suffers two internal reflections, whose phase contributions are equal and cancel — so between the two transmitted beams there is no net half-wave. Why: the π\pi asymmetry that darkened the reflected centre simply is not present in transmission.

Step 4. With no extra λ/2\lambda/2, the transmitted condition for brightness is 2nt=mλ2nt=m\lambda, satisfied at t=0t=0: the transmitted centre is bright, and the whole transmitted pattern is the complement of the reflected one (lower contrast, since the twice-reflected beam is weak). Why: energy conservation demands the reflected and transmitted patterns be complementary, and the reflection bookkeeping delivers exactly that. *Verified: index scaling r→r/nr\to r/\sqrt n (water r10=6.66r_{10}=6.66 mm) and the complementary bright transmitted centre in verify_aq-optics-newtons-rings.py.*

Limiting cases

CaseResultMeaning
Paraxial gap (r≪Rr\ll R)t≈r2/2Rt\approx r^2/2Rthe exact chord t=R−R2−r2t=R-\sqrt{R^2-r^2} becomes a parabola — the basis of every ring formula
Air gap, reflectedrm=mλRr_m=\sqrt{m\lambda R}, centre darkdark rings m=0,1,2,…m=0,1,2,\dots; bright at (m−12)λR\sqrt{(m-\tfrac12)\lambda R}
Liquid of index nnrm=mλR/nr_m=\sqrt{m\lambda R/n}radii shrink by 1/n1/\sqrt n — a refractometer
Transmitted lightcentre brightno net half-wave between the transmitted beams; complementary, low contrast
Large order mmΔr∝1/m\Delta r\propto 1/\sqrt mrings crowd together outward — the m\sqrt m signature of a quadratic gap
White lightfew coloured ringsrm∝λr_m\propto\sqrt\lambda spreads the colours; high orders wash out past the coherence length

Worked examples

1 · Sodium rings on a metre-scale lens (confidence builder)

A plano-convex lens of radius of curvature R=10.00R=10.00 m rests on an optical flat, illuminated from above with sodium light, λ=589.3\lambda=589.3 nm. Find the radius of the 10th dark ring, and show how measuring the 5th and 10th rings alone returns RR.

Step 1. Apply the air-gap dark-ring law rm=mλRr_m=\sqrt{m\lambda R}. For m=10m=10: r10=10×589.3×10−9×10.00=5.893×10−5 m=7.68 mmr_{10}=\sqrt{10\times589.3\times10^{-9}\times10.00}=\sqrt{5.893\times10^{-5}}\ \text{m}=\mathbf{7.68\ mm}. For m=5m=5, r5=2.9465×10−5=5.43r_5=\sqrt{2.9465\times10^{-5}}=5.43 mm, and m=1m=1 gives 2.432.43 mm.

Step 2. Confirm the m\sqrt m crowding: from m=1m=1 to m=5m=5 the radius grows 2.43→5.432.43\to5.43 mm (a jump of 3.003.00 mm), but from m=5m=5 to m=10m=10 only 5.43→7.685.43\to7.68 mm (a jump of 2.252.25 mm) — the same five orders, a smaller step, because Δr∝1/m\Delta r\propto1/\sqrt m.

Step 3. Now invert without knowing the absolute order: R=(r102−r52)/[(10−5)λ]R=(r_{10}^2-r_5^2)/[(10-5)\lambda]. Numerator =(7.677×10−3)2−(5.428×10−3)2=5.893×10−5−2.9465×10−5=2.9465×10−5 m2=(7.677\times10^{-3})^2-(5.428\times10^{-3})^2=5.893\times10^{-5}-2.9465\times10^{-5}=2.9465\times10^{-5}\ \text{m}^2; denominator =5×589.3×10−9=2.9465×10−6 m=5\times589.3\times10^{-9}=2.9465\times10^{-6}\ \text{m}.

Step 4. Divide: R=2.9465×10−5/2.9465×10−6=10.0 mR=2.9465\times10^{-5}/2.9465\times10^{-6}=\mathbf{10.0\ m}, recovering the lens exactly and needing only two ring radii and the wavelength. r₁₀ = 7.68 mm; R = 10.0 m from the 5th and 10th rings.

2 · A drop of water in the gap (refractometry)

The same lens and light, but now a film of water (n=1.33n=1.33) fills the gap. What happens to the rings, and how would you read the water's index from them?

Step 1. The optical path in the gap becomes 2nt2nt, so rm=mλR/nr_m=\sqrt{m\lambda R/n}: every radius is multiplied by 1/1.33=0.8671/\sqrt{1.33}=0.867. The 10th dark ring moves in from 7.687.68 mm to r10=7.68×0.867=6.66 mmr_{10}=7.68\times0.867=\mathbf{6.66\ mm}, a 13%13\% contraction.

Step 2. Read the index straight from the shrinkage. Measuring the same order dry and wet, n=(rmair/rmliq)2=(7.68/6.66)2=1.33n=(r_m^{\text{air}}/r_m^{\text{liq}})^2=(7.68/6.66)^2=1.33 — the wavelength, order, and radius all cancel, so no external standard is needed.

Step 3. Sanity-check the direction: a denser medium packs more wavelengths into the same gap, so a given order is reached at a smaller radius and the rings pull inward. A gas (n→1n\to1) would leave them essentially unchanged; a high-index oil (n=1.5n=1.5) would shrink them by 0.8160.816.

Step 4. Note the centre stays dark: the half-wave at the plate is unaffected by what fills the gap (still air-to-glass in sign), so only the spacing, not the contrast pattern, responds to nn. Water shrinks r₁₀ to 6.66 mm; n = (r_air/r_water)² = 1.33.

Physics of the portrait

The pattern carries Newton's name, yet it is a small monument to how physics actually advances: the man who measured it best drew the wrong lesson, and the wave theory he distrusted read it correctly.

Origins · 1 minNewton's Rings and how this was discovered
NR
Newton's Rings
first recorded 1665, quantified 1704 · wave optics and interferometric metrology

Newton's rings are a phenomenon before they are a person's legacy. Robert Hooke described the coloured circles between pressed glass plates in his Micrographia of 1665, but it was Isaac Newton who, in the Opticks of 1704, measured them with care — tabulating ring diameters, noting the dark centre, and establishing the quantitative m\sqrt m spacing that still bears his name. The irony is deep: Newton explained the rings with his corpuscular "fits of easy reflection and transmission," an ingenious but ultimately wrong account that avoided admitting light was a wave. The correct reading had to wait for Thomas Young, who in the first years of the nineteenth century saw the rings as interference, and for George Gabriel Stokes, who in 1849 pinned the dark central spot on the half-wave phase change at reflection. So the eponymous pattern is at once Newton's most careful optical measurement and the standing evidence against his own theory of light. Today the same rings, produced by a test flat on a polished surface, are a daily tool of the optical shop — a reminder that a good measurement outlives the theory its author attached to it.

History
1665
— Robert Hooke reports coloured rings between pressed glass plates in Micrographia
1675
— Newton presents detailed ring measurements to the Royal Society (later expanded in Opticks)
1704
— Newton publishes his quantitative study of the rings in Opticks, Book II
1717
— the second edition of Opticks adds Queries proposing aether vibrations as the cause of Newton's "fits of easy reflection and transmission"
1801
— Thomas Young interprets the rings as interference of light
1849
— George Gabriel Stokes explains the dark central spot by the half-wave reflection phase

Going further

Texts. Hecht, Optics, 5th ed., §9.4 (fringes of equal thickness; Newton's rings) · Born & Wolf, Principles of Optics, 7th ed., §7.5 · Saleh & Teich, Fundamentals of Photonics, 3rd ed., Ch. 2 (interference) · Möller, Optics (interferometric surface testing).

Provenance. The gap relation t≈r2/2Rt\approx r^2/2R follows from R2=r2+(R−t)2R^2=r^2+(R-t)^2; the dark-ring law rm=mλRr_m=\sqrt{m\lambda R} from 2t=mλ2t=m\lambda after the reflection λ/2\lambda/2 cancels (Hecht §9.4, Born & Wolf §7.5); the index scaling rm=mλR/nr_m=\sqrt{m\lambda R/n} and the offset-free difference rm+p2−rm2=pλRr_{m+p}^2-r_m^2=p\lambda R are standard laboratory results, all reproduced in verify_aq-optics-newtons-rings.py. The half-wave phase change is owned by aq-optics-stokes-relations-phase-reflection and recalled here by name. Refractive index of water (1.331.33) is the only physical constant cited, a standard tabulated value.

Prerequisites. Thin-Film Interference · Optical Path Difference and Phase Retardation · Two-Wave Interference and the Interference Term · Fringes of Equal Inclination and Equal Thickness. Leads to. Wavefront-Splitting and Amplitude-Splitting Interferometers · Fringe Visibility and Contrast · Conditions for Observable Interference.

Why does the gap thickness go as r²/2R and not linearly with r?

Because the lower surface is a sphere, not a wedge. The right triangle from the sphere's centre gives R2=r2+(R−t)2R^2=r^2+(R-t)^2; solving for the small root and dropping the negligible t2t^2 term leaves t≈r2/2Rt\approx r^2/2R. This is the sagitta of a shallow arc — quadratic in radius. A linear gap (a true wedge of two flats at an angle) instead gives straight, equally spaced fringes; the quadratic gap is exactly what turns them into circles with m\sqrt m spacing. The distinction matters: if you saw evenly spaced rings you would suspect a conical, not spherical, surface.

If I press the lens harder onto the plate, do the rings change?

Yes, subtly. Pressing flattens the effective contact and can introduce a small constant gap offset t0t_0 (or, with real elasticity, a slightly deformed contact), which shifts the apparent order of every ring. That is precisely why measurements use the difference rm+p2−rm2=pλRr_{m+p}^2-r_m^2=p\lambda R: it cancels any constant t0t_0 and the unknown zero order, so your extracted RR is immune to how hard you press. What you must avoid is dust or a scratch at the centre, which corrupts the innermost rings — measure the cleaner outer rings and difference them.

Newton's rings and thin-film colours look related — are they the same physics?

They are the same mechanism — amplitude-splitting interference in a thin film — differing only in the film's shape and the light. A soap bubble or oil slick is a film of slowly varying thickness lit by white light, so you see fringes of equal thickness in colour. Newton's rings are the controlled version: a precisely spherical air film lit by monochromatic light, so the equal-thickness contours are clean circles and the spacing obeys rm=mλRr_m=\sqrt{m\lambda R}. In Hecht's taxonomy both are Fizeau fringes of equal thickness; Newton's rings are simply the case engineered for measurement.

Why do I see only a few coloured rings in white light but many in a laser or sodium lamp?

Ring radius scales as λ\sqrt\lambda, so each colour makes its own set of rings, slightly offset. Near the centre the low orders of all colours nearly coincide and stay visible as tinted rings, but as the order climbs the different colours' rings drift apart and overlap into washed-out white. A monochromatic source has a single λ\lambda and a long coherence length, so high-order rings stay sharp and dozens are visible — which is why quantitative work uses a sodium lamp or laser, not daylight.

Does the pattern depend on the light hitting exactly straight down?

Only weakly, and in a known way. The exact path difference is 2ntcos⁡θt2nt\cos\theta_t, so tilting the illumination by an angle multiplies the geometric term by cos⁡θt\cos\theta_t, slightly enlarging the rings. For the near-normal viewing used in practice cos⁡θt≈1\cos\theta_t\approx1 and the correction is second order in the angle — a fraction of a percent for a few degrees. Large obliquity does shift the rings measurably and blurs them if the source is extended, which is why the standard arrangement uses near-normal incidence and views the fringes localised in the film.

Can Newton's rings measure the wavelength of light instead of the lens radius?

Yes — the two roles are interchangeable in rm+p2−rm2=pλRr_{m+p}^2-r_m^2=p\lambda R. If you know RR (from a separate spherometer or catalogue value), measuring ring radii gives λ=(rm+p2−rm2)/(pR)\lambda=(r_{m+p}^2-r_m^2)/(pR). Historically this was a route to wavelength before diffraction gratings dominated; today it more often runs the other way, using a known laser wavelength to certify a lens's radius of curvature. Either way the measurement is self-contained: a travelling microscope, monochromatic light, and the linearity of rm2r_m^2 in order.

Before this

Where this leads