Stars

The interior read from a comb of frequencies

A star's surface moves by about twenty centimetres a second, in thousands of overlapping sound modes at once. Two numbers off that spectrum give a mass and a radius with almost no stellar model in the chain, and a third gives an age.

Assumes Hydrostatic equilibrium, Variable stars and Binary stars.

The account of why the biggest stars die first contains one sentence saying that two seismic observables scale as a star’s mean density and as its surface gravity, and that the pair therefore gives a mass and a radius. That sentence is a promissory note, and this is the rung that pays it.

The spectrum below is what the note is written on: not a light curve and not one oscillation, but a comb of some forty resonances of the Sun, each a standing sound wave filling the whole body of the star, all ringing at once and together moving the surface by a fraction of a metre per second.

14 radial orders of the Sun, at 135.1 μHz apart. The p-mode spectrum of the Sun — 1 solar mass in 1 solar radius — from the asymptotic relation with its second-order term, drawn as 14 radial orders of ℓ = 0, 1 and 2 under a Gaussian envelope centred on ν_max = 3,090 μHz. Two numbers are marked and they do very different work. The large separation, 135.1 μHz, is the spacing between consecutive ℓ = 0 modes and fixes the mean density. The small separation, 9.00 μHz, is 2.7 pixels on this axis — it fixes the age, and it is why the échelle diagram exists rather than being a convenience. The vertical axis is the measurement: each mode moves the surface by about 20.0 cm s⁻¹ at the peak, and brightens it by a few parts per million, which is why this was impossible before a decade-long velocity series. Each mode is one line: its true width is set by its lifetime and is far below a pixel here.
Fig. 1 Fourteen radial orders of the Sun’s p-mode spectrum, from the asymptotic relation for 1 solar mass in 1 solar radius: degrees =0\ell = 0, 1 and 2 under an envelope centred on 3,090 μHz, a period of five and a half minutes. Consecutive =0\ell = 0 modes lie 135.1 μHz apart, which fixes the mean density; the 9.00 μHz beside it is 2.7 pixels wide and fixes the age. The vertical axis is what had to be detected — about 20 cm s⁻¹ per mode.

Two numbers, and what each is a proxy for

Almost everything in the spectrum can be discarded; two summary numbers carry the argument.

The first is the large separation Δν\Delta\nu, the spacing between consecutive radial modes — 135.1 μHz for the Sun. The resonances are the frequencies that fit a whole number of half-wavelengths into a sound wave’s round trip through the star, so Δν\Delta\nu is the reciprocal of that crossing time, and a crossing time divided into a size is a mean density:

Δνρˉ    M/R3.\Delta\nu \propto \sqrt{\bar\rho} \;\propto\; \sqrt{M/R^3}.

The second is νmax\nu_{\max}, the frequency of maximum power — the centre of the envelope, 3,090 μHz, where the modes are excited hardest. The envelope tracks the atmosphere’s acoustic cutoff frequency, which for an isothermal layer is the sound speed over the pressure scale height, and that ratio is a surface gravity divided by the square root of a temperature:

νmaxgTeff    MR2Teff.\nu_{\max} \propto \frac{g}{\sqrt{T_{\rm eff}}} \;\propto\; \frac{M}{R^2 \sqrt{T_{\rm eff}}}.

One observable is a mean density and the other is a surface gravity, which is to say one is M/R3M/R^3 and the other is M/R2M/R^2 — two independent combinations of the same two unknowns.

Why the comb is nearly evenly spaced

Even spacing is not obvious. A star is a cavity of appalling complexity, its sound speed varying by two orders of magnitude between centre and photosphere, its modes carrying three quantum numbers rather than one.

What rescues the arithmetic is that at high radial order the asymptotic form of the wave equation makes frequency linear in order:

ν(n,)  =  Δν[n+2+ε+α2(nnmax)2]    (+1)D0.\nu(n,\ell) \;=\; \Delta\nu\left[\,n + \frac{\ell}{2} + \varepsilon + \frac{\alpha}{2}(n - n_{\max})^2\right] \;-\; \ell(\ell+1)\,D_0.

The bracket is the comb: nn counts radial nodes, \ell is the surface degree, ε\varepsilon a dimensionless offset near 1.45 for the Sun set by the outermost layers, α\alpha a small curvature term. Set α\alpha and D0D_0 to zero and the spectrum is exactly periodic in nn with period Δν\Delta\nu, the odd degrees falling halfway between the even.

Where each mode turns back: ℓ = 0 through the centre, ℓ = 300 in the outer 2 per cent. Why a set of frequencies is a depth profile and a single frequency is not. An acoustic wave travelling into a star meets a rising sound speed and is refracted back; it turns where its horizontal phase speed matches the local sound speed, which happens at c(r)/r = 2πν/√(ℓ(ℓ+1)). The horizontal axis is the angular degree on a logarithmic scale and the vertical axis is the fractional radius of that turning point, drawn at 2000, 3090, 4000 microhertz. The ordering is the content. A radial mode, ℓ = 0, has no horizontal phase speed at all and passes straight through the centre. Degrees one and two turn deep in the core. By ℓ = 300 the mode is trapped in the outer 2 per cent and knows nothing about anything below. So a frequency measured to a part in ten thousand constrains an average of the interior weighted in a way the mode itself decides, and measuring thousands of modes of different degree gives thousands of differently weighted averages — which is a solvable inverse problem, and is how the base of the convection zone was located at 0.713 of the radius rather than assumed. The sound speed here is a polytrope's rather than a tabulated solar model's, so the curve is the right shape and the wrong star in its outer tenth, where the real Sun is convective and this one is not. What the picture cannot show is the frequency dependence at fixed degree, which is weaker but not negligible: a higher-frequency mode of the same degree turns slightly deeper, and the three curves separating toward the right is that effect.
Fig. 2 Which part of the interior each frequency is a statement about. A mode of angular degree ℓ is refracted back toward the surface at the depth where its horizontal phase speed matches the local sound speed, so ℓ = 0 passes through the centre and ℓ = 300 is trapped in the outer two per cent. That is the whole reason a list of frequencies contains a profile rather than a single average: thousands of modes sample thousands of overlapping depth ranges, each with its own weighting, and recovering the sound speed from them is a linear inverse problem with an honest error bar at every radius.

The two relations invert, and that is the method

Two equations in two unknowns, both read off one spectrum, and the algebra closes. Writing every quantity as a ratio to the Sun’s,

RR=(νmax/νmax,)(T/T)1/2(Δν/Δν)2,MM=(νmax/νmax,)3(T/T)3/2(Δν/Δν)4.\frac{R}{R_\odot} = \frac{(\nu_{\max}/\nu_{\max,\odot})\,(T/T_\odot)^{1/2}}{(\Delta\nu/\Delta\nu_\odot)^{2}}, \qquad \frac{M}{M_\odot} = \frac{(\nu_{\max}/\nu_{\max,\odot})^{3}\,(T/T_\odot)^{3/2}}{(\Delta\nu/\Delta\nu_\odot)^{4}}.

A temperature is needed, and comes from the colours. Everything else on the right is a frequency. There is no evolutionary track, no opacity table, no mixing length and no distance.

The plane the two relations make, and how badly it is conditioned in mass. The large separation against the frequency of maximum power, both logarithmic, for four stars whose masses, radii and temperatures are stated and whose frequencies are computed from them — the Sun at 3,090 and 135 μHz; a subgiant at 671 and 39.0 μHz; a red-clump star at 34 and 4.06 μHz; a red giant at 4.43 and 0.862 μHz. Over the plane are lines of constant radius, at 1, 3, 10, 30 solar radii, and of constant mass, at 0.8 and 2. The two families are not at right angles and that is the finding: the constant-mass lines run at a slope of about 0.77 and the constant-radius lines at 0.5, so a factor of 2.5 in mass moves a star only 0.11 decades across the plane. Mass enters the inversion at the quarter power of the observables and radius at the first, which is why an asteroseismic radius is good to a few per cent and an asteroseismic mass to something nearer ten. Every point here was put on the plane by the relations and then read back off it: solving the two equations for mass and radius returns the stated values to 7.8e-16.
Fig. 3 The plane the two relations make, for four stars whose masses, radii and temperatures are stated and whose frequencies follow from them: the Sun at 3,090 and 135 μHz, a subgiant at 671 and 39.0, a red-clump star at 34.0 and 4.06, a red giant at 4.43 and 0.862. Constant-radius lines run at a slope of 0.5 and constant-mass lines at about 0.77, so the two families are nowhere near perpendicular — and 0.8 to 2 solar masses spans 0.11 decades, a factor of 2.5 in mass squeezed into a tenth of one. Solving the pair back returns the stated values to 8×10168\times10^{-16}.

The exponents in that inversion are the least glamorous and most consequential fact. A fractional error in Δν\Delta\nu arrives doubled in the radius and quadrupled in the mass; an error in νmax\nu_{\max} arrives at the first power in the radius and the third in the mass. The same spectrum therefore yields a radius good to a few per cent and a mass good to nearer ten, and no improvement in the frequencies changes the ratio between those two figures.

The fold that turns a spacing into a fact

A spacing quoted off a spectrum invites the objection that it was fitted. The answer is a change of coordinates, not a better fit.

Cut the frequency axis into strips of width Δν\Delta\nu and stack them. If the guessed spacing is right, every radial order lands at the same horizontal position and the comb collapses into vertical ridges, one per degree; if it is wrong, each successive order is displaced a little further and the ridges lean. The lean shows up long before the error would be noticeable in the unfolded spectrum, which is what makes Δν\Delta\nu a property of the data.

The same comb folded at 135.1 μHz — three ridges and their curvature. Frequency against frequency modulo Δν, for 14 radial orders of the Sun. Folding at 135.1 μHz stacks the orders into three near-vertical ridges, one for each degree, and that is what makes Δν a fact about the data rather than a fitted parameter: get it wrong and the ridges lean. What is left over is the curvature — the ℓ = 0 ridge wanders 6.7 per cent of Δν across the drawn range, which is the departure from the asymptotic relation and the part of the spectrum that knows about the star's outer layers. The small separation is here too and here it is visible: 9.00 μHz between the ℓ = 0 and ℓ = 2 ridges, 39 pixels on this axis against 39 — the same quantity that is three pixels wide in the unfolded spectrum. A constant offset of 27 μHz has been subtracted before folding so that no ridge wraps round the edge.
Fig. 4 The same fourteen orders folded at 135.1 μHz — frequency against frequency modulo Δν\Delta\nu, with 27 μHz subtracted first so no ridge wraps round the edge. Three near-vertical ridges appear, one per degree, and their verticality is the test: a wrong folding period tips them. What is left over is curvature — the =0\ell = 0 ridge wanders by 6.7 per cent of Δν\Delta\nu, which is the part of the spectrum that knows about the outermost layers. The 9.00 μHz that was 2.7 pixels wide unfolded is 39 pixels here.

Nine microhertz, and an age

The last term in the asymptotic relation, (+1)D0-\ell(\ell+1)D_0, separates degrees of the same parity. Its observable is the small separation δν02\delta\nu_{02}, the gap between an =0\ell = 0 mode and the =2\ell = 2 mode that would otherwise sit on it: 9.00 μHz for the Sun, 6.7 per cent of Δν\Delta\nu and three parts in a thousand of νmax\nu_{\max}.

That gap dates the star, because D0D_0 is an integral of the gradient of the sound speed, weighted towards the deep interior. Quadrupole modes penetrate slightly less far than radial ones, so their difference is sensitive to a small central region and almost nothing else — and that is the region whose composition is changing, as hydrogen gives way to helium and the sound-speed gradient steepens. Nine microhertz is a measurement of how much hydrogen is left.

Plotting δν02\delta\nu_{02} against Δν\Delta\nu therefore gives a diagram whose model grid is a grid of masses and ages, and among main-sequence stars of similar Δν\Delta\nu the small separation falls as the star ages. The ages come out good to 10 or 20 per cent for a solar-type star — remarkable for a single field star with no cluster around it and no turn-off to read.

One honesty is owed. The ratio δν02/Δν\delta\nu_{02}/\Delta\nu rises from 0.067 for the Sun to 0.125 for the red giant below, opposite to the trend just described — but Δν\Delta\nu has itself fallen by two orders of magnitude between those stars, and a fraction of a collapsing denominator is not a clock. The diagnostic is the pair, not the quotient.

What is actually measured: twenty centimetres a second

Every frequency above rests on an amplitude that is absurdly small. A solar radial mode moves the photosphere at about 20 cm s⁻¹ — a Doppler shift of seven parts in ten thousand million — and in brightness it is a few parts per million. Nothing about the Sun is faint, so the difficulty is not photons: the signal sits four or five orders of magnitude below the star’s own variability, and a single measurement of it is meaningless.

What rescues it is that the signal is coherent and the noise is not. A mode’s power piles up in one bin of a Fourier transform while the noise spreads across all of them, so the noise per frequency bin falls as the square root of the number of measurements. The arithmetic runs on stated inputs: 30 parts per million per half-hour cadence, some 70,000 cadences in four uninterrupted years, a per-bin noise near a tenth of a part per million — against a mode amplitude of a few. The detection is bought with time.

On the Sun the record is full-disc velocity, from ground networks since the 1970s and from space since 1996; those series fix the solar reference values these figures use. On other stars it is photometry: Kepler stared at one field for four years and produced usable combs for some hundreds of solar-type dwarfs and of order sixteen thousand red giants — two orders of magnitude more stars than the whole catalogue whose masses are measured any other way.

The dates explain the delay. Leighton, Noyes and Simon reported a patchy five-minute velocity oscillation of the solar surface in 1962 without knowing what it was; it was proposed as trapped standing waves around 1970, Deubner resolved the predicted ridges in 1975, and the evenly spaced peaks came out of full-disc velocity work at the end of that decade. Reaching a second star took twenty years more: the first convincing solar-type comb elsewhere came from a few nights on α Centauri A in 2001.

seven radial orders of a red giant, at 0.8623 μHz apart. The p-mode spectrum of a red giant — 1.1 solar masses in 30 solar radii — from the asymptotic relation with its second-order term, drawn as seven radial orders of ℓ = 0, 1 and 2 under a Gaussian envelope centred on ν_max = 4.43 μHz. Two numbers are marked and they do very different work. The large separation, 0.8623 μHz, is the spacing between consecutive ℓ = 0 modes and fixes the mean density. The small separation, 0.108 μHz, is 9.9 pixels on this axis — it fixes the age, and it is why the échelle diagram exists rather than being a convenience. The vertical axis is the measurement: each mode moves the surface by about 45.9 m s⁻¹ at the peak, which is why this was impossible before a decade-long velocity series. Each mode is one line: its true width is set by its lifetime and is far below a pixel here.
Fig. 5 The same construction for a red giant of 1.1 solar masses and 30 solar radii: seven radial orders under an envelope centred near 4 μHz, a period of two and a half days rather than five and a half minutes. The large separation has collapsed to 0.8623 μHz because the mean density has, and the amplitude has gone the other way — 45.9 m s⁻¹ per mode, two hundred times the Sun’s. Giants are easy in amplitude and hard in resolution: splitting the 0.108 μHz small separation takes months of baseline.
The same comb folded at 0.8623 μHz — three ridges and their curvature. Frequency against frequency modulo Δν, for seven radial orders of a red giant. Folding at 0.8623 μHz stacks the orders into three near-vertical ridges, one for each degree, and that is what makes Δν a fact about the data rather than a fitted parameter: get it wrong and the ridges lean. What is left over is the curvature — the ℓ = 0 ridge wanders 7.7 per cent of Δν across the drawn range, which is the departure from the asymptotic relation and the part of the spectrum that knows about the star's outer layers. The small separation is here too and here it is visible: 0.108 μHz between the ℓ = 0 and ℓ = 2 ridges, 70 pixels on this axis against 70 — the same quantity that is three pixels wide in the unfolded spectrum. A constant offset of 1 μHz has been subtracted before folding so that no ridge wraps round the edge.
Fig. 6 The giant folded, at 0.8623 μHz. Three ridges again, one per degree — and the small separation that is three pixels wide in the spectrum above is 70 pixels here, because the fold stacks seven orders on one another instead of asking a single pair of peaks to be resolved. That is what the change of coordinates buys on a star where resolution is the binding constraint. The ridges bend by 7.7 per cent of Δν\Delta\nu across the range against 6.7 for the Sun, and what the drawing does not show is the forest of mixed modes a real giant’s =1\ell = 1 ridge breaks into.

The only other place this works

A mass and a radius in physical units, with no stellar model in the chain, is not something astronomy hands out. Double-lined eclipsing binaries are the one other source of it, and the comparison is worth making term by term.

A binary needs two stars, two visible spectra and an orbit within a degree or two of edge-on; it delivers masses and radii to 0.2 per cent from Kepler’s third law and geometry. A comb needs one star and a long time series, and delivers a radius to a few per cent and a mass to nearer ten. So the binary is far the more precise, on a few hundred systems selected by a severe geometric accident; the comb is the cruder, on tens of thousands selected by nothing but brightness.

AI Phoenicis, drawn to scale. The two orbits about the common centre of mass, seen at the system's inclination of 88.5° — so nearly edge on that the ellipses are almost lines. Radii, separation and the size ratio are all to scale: the separation is 47.9 solar radii and the stars are 1.805 and 2.9303. Eclipses happen at all because the orbit is seen this close to edge on, and that single fact is what converts a spectroscopic orbit into two radii.
Fig. 7 The other method’s requirement, drawn to scale: two orbits about a common centre of mass at 88.5°, so nearly edge-on that the ellipses are almost lines. The separation is 47.9 solar radii, the stars are 1.805 and 2.9303, and the ratio of the orbits is the inverse ratio of the masses. None of this geometry is optional — the eclipse fixes the inclination, and the inclination turns a spectroscopic mass sum into two masses. A comb needs none of it.

The two methods meet on the few red giants that happen to sit in eclipsing binaries, and that meeting is the only external check the scaling relations have. It was not reassuring at first: the earliest such comparisons found seismic masses larger than the dynamical ones by of order fifteen per cent, which sent the Δν\Delta\nu relation back for a correction rather than the binaries. That is the right direction of deference, and it exists only because two methods answer one question.

One mode instead of thousands

A classical Cepheid is the same physics with the mode count set to one: its period is the crossing time itself, while the Sun’s crossing time appears only in a spacing. A Cepheid pulsates because a helium ionisation layer acts as a valve and pumps one mode to enormous amplitude, making the star a self-excited oscillator on a limit cycle. The Sun has no such valve: its modes are driven by the turbulence of its own convection zone, a broadband source, so every mode the cavity supports is excited a little and none is excited much. Huge amplitude in one mode buys a period anyone can measure and nothing else; tiny amplitude in a thousand modes buys the interior.

The structure reaches beyond stars: the microwave background’s acoustic peaks are a standing sound wave in a different cavity, and their spacing is likewise a size divided by a sound speed. A comb is what a bounded medium makes, and a spacing read off one is a crossing time.

Where the model stops, unevenly

The claim above was almost no stellar model, and the qualification has three parts.

The Δν\Delta\nu relation has a physical derivation behind it, but its constant is set at the Sun; the νmax\nu_{\max} relation is weaker still, resting on a proportionality to the acoustic cutoff which has no complete theory and is calibrated on one star. So the Sun is inside the chain — a far shorter chain than an evolutionary track, and not nothing.

The near-surface layers are the second part. One-dimensional convection gets the outermost few hundred kilometres wrong, and the resulting offset — the surface term — reaches several microhertz at the solar νmax\nu_{\max}. It biases Δν\Delta\nu at the per cent level, and a per cent in Δν\Delta\nu is four per cent in the mass.

Inside a star that is holding itself up (polytrope n = 1.5). Temperature, density and pressure through a star, as fractions of their central values, against fractional radius. All three come from one numerical integration of the Lane–Emden equation at index 1.5, which is the hydrostatic balance written for a gas whose pressure is a power of its density. The inner half of the radius holds 46% of the mass, and the outer half is nearly weightless — which is why the load, and so the temperature, is concentrated where the burning is.
Fig. 8 The interior the scaling relations do not look at. The same Lane–Emden integration at index 1.5 — the polytrope of a fully convective star, drawn here in its own right rather than as the dashed comparison it was above — gives a mass distribution of a quite different shape: the inner half of the radius holds 46 per cent of the mass here against 90 per cent at index 3, and the dimensionless surface sits at ξ1=3.652\xi_1 = 3.652 rather than 6.896. Two such stars can be given the same mean density, and Δν\Delta\nu is a function of nothing but the mean density, so everything separating these two cavities is precisely what a summary number discards — and what ε\varepsilon, the curvature term and the surface offset are left to carry.

The third is the conditioning visible in the scaling plane, and it is a limit rather than an error bar. Mass moves a star across that plane by the quarter power of the observables while radius moves it by the first, so the mass is squeezed into a tenth of a decade where the radius has three. No amount of extra signal fixes a geometry that unfavourable; what fixes it is a second kind of observation, which is what the binaries supply.

What the picture cannot show

Mode widths, and heights that are draws rather than values. Every mode here is one line of zero width. A real solar mode is about 1 μHz wide, because it is damped and lives a few days, and a real peak is a Lorentzian whose centroid must be fitted. On the drawn axis 1 μHz is a third of a pixel — which is why the drawing can get away with lines and why an analysis cannot. And convective driving is random, so the envelope is smooth only in expectation.

Rotation. Every mode with >0\ell > 0 is split into 2+12\ell+1 components by rotation, and the drawing gives each degree one line. Those splittings are the only measurement of a star’s internal rotation there is, so the figure drops the subject’s most spectacular result to keep the comb legible.

Mixed modes, which is the giant panel’s real deficiency. In an evolved star the =1\ell = 1 modes couple to gravity modes trapped in the dense core, and what should be one ridge becomes a forest. Those modes are how a red giant is told apart from a red-clump star of identical Δν\Delta\nu, and the drawing shows a clean ridge where the real spectrum shows the interesting mess.

And the granulation background. Convection produces a rising continuum at low frequency which, in a giant, sits directly beneath the envelope. These drawings have no noise floor; in practice the floor is the star.

The splitting that measures a rotation nobody can see

The drawings give each degree one line, and a real spectrum gives each degree several. The reason is rotation, and what it delivers is the one quantity in stellar physics that has no other route to it at all.

A mode with >0\ell > 0 is degenerate in a spherical star: the 2+12\ell+1 orientations of its angular pattern have identical frequencies. Rotation breaks the symmetry, because a wave travelling with the rotation and one travelling against it complete their circuits at different rates, so the degenerate multiplet splits into components separated by roughly the rotation frequency.

That is straightforward. What makes it a measurement of the interior is that different modes sample different depths. A mode’s splitting is an average of the rotation rate along its own cavity, weighted by where it spends its time — so a set of modes with different penetration depths gives a set of differently weighted averages, and inverting them returns a profile.

For the Sun the answer is the one described elsewhere in this collection: a differentially rotating convection zone above a radiative interior that turns as a solid body, with a thin shear layer between.

For a red giant the answer is more startling and is the field’s most consequential result. The mixed modes of an evolved star penetrate to the core, so their splittings measure the core’s rotation directly — and the core turns about ten times faster than the envelope.

Ten sounds like a lot and it is far too little. A star’s core contracts enormously between the main sequence and the giant branch while its envelope expands, and if each conserved its own angular momentum the core would end up spinning hundreds or thousands of times faster than the surface. What is observed is ten.

So angular momentum is being transported outward from the core, efficiently, by something. The candidates are internal gravity waves, magnetic fields threading the interior, and instabilities driven by the shear itself, and none of them at its computed strength produces the observed coupling. Every standard stellar-evolution code underestimates the transport by one to two orders of magnitude.

A frequency splitting of a few hundred nanohertz, measured on stars too distant to resolve, has falsified the angular-momentum transport in every model of stellar interiors, and the replacement has not been found.

Where the ladder goes next

Later rungs on this anchor: ε\varepsilon as a diagnostic of the surface layers; mixed modes and the period spacing of the core gravity modes, which separate hydrogen-shell from helium-core burning at identical Δν\Delta\nu; rotational splitting, and the finding that giant cores turn far more slowly than angular momentum conservation alone permits; and the inversions that recover a whole sound-speed profile rather than two summary numbers.

And a rung facing outward: every transiting planet’s radius is a ratio multiplied by a stellar radius, and for the best-characterised systems that stellar radius comes from a comb — which makes a planet’s size a consequence of counting sound waves in the star it crosses.

What this makes readable

Essays that name this one as a prerequisite.

About the same objects

Not linked from either essay — found by the objects both name.

What links here

The 8 of 17 essays linking to this one that name the most of the same objects.

The objects this essay names

Each one links to every other essay that touches it.

AsteroseismologyConvectionEclipsing binaryGranulationHelioseismologyHydrostatic equilibriumMain sequence lifetimePower spectrumStellar densityStellar evolutionStellar radiusSurface gravity