Galaxies

A rotation curve that refuses to fall

Beyond the edge of a galaxy's light there is nothing left to enclose, so the orbital speed should fall away as the inverse square root of radius. It does not fall at all, and the shape of that refusal says the missing mass arrives at a constant rate for as far out as anyone can measure.

Assumes Shell theorem and Harmonic law.

Every orbit in this collection so far has been drawn around a mass that was, for the purposes of the drawing, a point. A planet around the Sun, a moon around a planet, a star around the centre of a binary: in each case the whole of the mass sits inside the orbit, and the speed of anything going round it falls as the inverse square root of distance.

A galaxy is the first object here whose mass is not a number but a function of radius. And when that function is measured, by the only method that reaches far enough, it does not do what the light says it should.

The rotation curve of NGC 3198, decomposed. Circular speed against radius for a three-component model of NGC 3198: a Hernquist bulge of 1.0×10⁹ M☉, an exponential disc of 2.20×10¹⁰ M☉ with a scale length of 2.6 kpc, and a pseudo-isothermal halo whose asymptotic speed is not chosen but solved for — it is whatever brings the total to the measured 150 km/s at 30 kpc, and comes out at 171 km/s. The components add in quadrature because accelerations add. The disc alone peaks at 5.7 kpc and falls away; the total does not.
Fig. 1 The circular speed against radius for a model of NGC 3198, decomposed into the three things that might be producing it. The disc’s own contribution peaks near two and a bit scale lengths and falls away thereafter, which is what a finite, centrally concentrated mass does. The total does not fall. The halo curve is what has to be added to keep it from falling, and its asymptotic speed is not chosen here — it is solved for, as whatever brings the total to the flat speed the spectroscopy actually measures.

What the light predicts

A disc galaxy’s brightness falls off exponentially with radius. That is an observation rather than a model: Ken Freeman established it in 1970 across a large sample, and the exponential is good over several factors of e in surface brightness, with a scale length of a couple of kiloparsecs for a galaxy of this size.

The light of NGC 3198 falls off exponentially. V-band surface brightness against radius for an exponential disc of scale length 2.6 kpc and a stellar mass-to-light ratio of 1.4 in solar units. The vertical axis is magnitudes per square arcsecond and runs the astronomers' way, with brighter upward; because a magnitude is already a logarithm, an exponential disc is a straight line on it, and the slope is one scale length per 1.086 magnitudes. The conventional edge of a galaxy, the 25th magnitude isophote, falls at 12.0 kpc — and the rotation curve is still flat at 30 kpc, 2.5 times further out.
Fig. 2 The surface brightness of an exponential disc, in magnitudes per square arcsecond. Because a magnitude is already a logarithm, an exponential disc plots as a straight line, and the slope is one scale length per 1.086 magnitudes. The vertical dashed line is the twenty-fifth-magnitude isophote — the conventional edge of a galaxy, and the edge that appears in a catalogue. There is very little light beyond it, and that is the whole difficulty: the rotation curve is still perfectly flat at three times that radius.

An exponential disc has a finite total mass, and nearly all of it is inside four scale lengths. So outside four scale lengths a test particle should be orbiting what is, to a good approximation, a point — and a sphere, or a sufficiently distant flattened distribution, pulls like a point.

That gives an immediate and sharp prediction: outside the light, v=GM/rv = \sqrt{GM/r}, so the speed falls as r1/2r^{-1/2}. This is not a modelling assumption. It is the same statement as the harmonic law, which is verified to eight digits in the solar system, and which every spacecraft in this collection is navigated by.

What is measured instead

What NGC 3198's light predicts, against what it does. The observed curve of NGC 3198 against the curve its luminous mass alone would produce. Inside the disc the two nearly agree; at 30 kpc the observed speed is 2.56 times the luminous prediction, which is a factor of 6.8 in enclosed mass. The dotted curve is the pure Keplerian √(GM/r) for the 2.30×10¹⁰ M☉ of stars and gas, drawn from 10 kpc outwards where essentially all of it is enclosed — the fall every planetary system in this collection obeys, and no galaxy does.
Fig. 3 The same galaxy, with the luminous prediction drawn against the observation. Inside the disc they very nearly agree, which is important: the disagreement is not a general failure of gravitation but something that switches on where the light runs out. At thirty kiloparsecs the observed speed is more than twice the luminous prediction, which is a factor of five or six in enclosed mass.

The measured curve is flat. Not slowly declining, not falling with a shallower exponent than expected — flat, from a few kiloparsecs out to the last radius at which there is any gas left to measure, which in NGC 3198 is about thirty kiloparsecs, more than eleven disc scale lengths.

The consequence is arithmetic and it is stark. If vv is constant then

M(<r)=v2rGr,M(<r) = \frac{v^2 r}{G} \propto r,

so the enclosed mass grows linearly, without limit, for as far as the measurement reaches. That straightness is the finding. A galaxy with more mass than its light suggested would be unremarkable — stellar mass-to-light ratios are uncertain at the tens of per cent level, and there is dust, and there are faint stars. A galaxy in which the enclosed mass rises linearly through the region where the light has already stopped is a different kind of statement, because there is no amount of unaccounted-for starlight that produces it. Doubling the assumed mass-to-light ratio of the disc raises the luminous curve and leaves it just as flat-topped as before.

The observation behind the number

Everything above depends on being able to measure a rotation speed at radii where there are essentially no stars. That is possible for one reason: neutral hydrogen extends far beyond the stellar disc and it emits at twenty-one centimetres.

The line comes from a hyperfine transition — the electron’s spin flipping relative to the proton’s — with a transition probability so low that a given atom waits some ten million years for it. That would be hopeless for a laboratory and is ideal for a galaxy, because there are enough atoms that the emission is detectable, and because a line that faint is never optically thick, so what a radio telescope receives is proportional to the amount of gas rather than to the surface of a cloud.

The twenty-one centimetre profile of a whole disc, at 60°. The hydrogen line profile emitted by the whole of NGC 3198, integrated over radius and azimuth from the same rotation curve drawn elsewhere in this collection, at an inclination of 60° and with an 8 km/s thermal and turbulent spread convolved in. The two horns are not two rings of extra gas: they are where the line-of-sight velocity stops changing with azimuth, at the near and far ends of the major axis, so a wide range of azimuth piles into a narrow range of velocity. The width at twenty per cent of the peak is 259 km/s, which is 2 v sin i to within 1 km/s — and it is the whole of what a distant galaxy's spectrum gives, which is why the Tully–Fisher relation is stated in terms of it.
Fig. 4 What a distant galaxy’s hydrogen emission looks like when the whole disc is inside one beam: a double-horned profile, computed here by integrating the emission over radius and azimuth for the rotation curve above at an inclination of sixty degrees. The horns are not two rings of extra gas. They are where the line-of-sight velocity stops changing with azimuth, at the two ends of the major axis, so a wide range of azimuth piles up into a narrow range of velocity. The width between the outer edges is twice the rotation speed times the sine of the inclination.

For a galaxy that can be resolved, the observation is a velocity per position on the sky, and the rotation curve is built by fitting tilted rings — annuli each with their own inclination and position angle — to the velocity field. Two things have to be got right and neither is free. The inclination enters every velocity as sini\sin i, and it is estimated from the shape of the outer isophotes, which is why a galaxy seen nearly face-on is nearly useless for this. And the beam of a radio telescope is not a point: it averages over a region, which smooths the curve and, in the steeply rising inner part, biases it low.

The classic case is NGC 3198, whose curve van Albada and colleagues worked out in 1985 and which is still the textbook example, because the flat part extends further in units of the disc scale length than almost anywhere else. Vera Rubin and Kent Ford’s optical work through the 1970s had already found flat curves in dozens of spirals; the radio measurements extended them past the light, which is where the argument becomes unanswerable.

Two further things about that measurement deserve to be said, because they are the reason the curve can be trusted at all.

The velocity comes from a Doppler shift, and a shift measures only the component of motion along the line of sight. For a rotating disc that is exactly the useful component — the approaching side is blueshifted, the receding side redshifted — but it means the whole curve is measured in units of sini\sin i and nothing observed in one galaxy can remove that factor.

And the radius is an angle. Converting it to kiloparsecs needs a distance, so every rotation curve inherits whichever rung of the distance ladder its galaxy sits on. A distance error rescales both axes: radii move in proportion, speeds do not move at all, and so the inferred enclosed mass moves in proportion too. The shape — flat or falling — survives it untouched, which is why the argument here is made from the shape.

What a flat curve does to an orbit

A curve that is flat rather than Keplerian changes the character of the orbits inside it, and the change is worth seeing because it separates a galaxy from every other system in this collection.

If vv is constant, the orbital period at radius rr is 2πr/v2\pi r/v, so it grows linearly with radius rather than as r3/2r^{3/2}. At the Sun’s distance from the Galactic centre that period is about 230 million years; at twice the distance it is 460 million rather than the 650 million a Keplerian galaxy would give. The Sun has gone round some twenty times since it formed, and a star at 30 kiloparsecs perhaps six.

More consequentially, the orbits do not close. In a Keplerian potential the radial oscillation frequency and the angular frequency are equal — which is exactly why an orbit is a closed ellipse and why the whole of celestial mechanics has such a convenient starting point. In a flat-rotation-curve potential the radial frequency is 2\sqrt{2} times the angular one, so a star that is displaced from a circular orbit traces a rosette that never repeats. Every galactic orbit is precessing, all the time, and the amount of the precession is fixed by the shape of the curve.

Why the inner part agrees, and why that matters

It would be easy to read the discrepancy as a failure of the theory of gravitation at large distances, and that reading has been seriously pursued. But note what the figures show inside a few kiloparsecs: the luminous prediction and the observation agree there, and they agree without any adjustment.

That is a strong constraint on any explanation. Whatever produces the outer speeds contributes almost nothing at the centre, so it cannot be a modification that scales with distance in a simple way and it cannot be extra mass concentrated where the stars are. It has to be a component that is diffuse, extended, and — in the inner regions — subdominant. The Milky Way shows the same shape, measured by an entirely different route, and its curve is worth drawing because the numbers are the ones a reader is most likely to have heard.

The rotation curve of the Milky Way, decomposed. Circular speed against radius for a three-component model of the Milky Way: a Hernquist bulge of 15.0×10⁹ M☉, an exponential disc of 5.00×10¹⁰ M☉ with a scale length of 3 kpc, and a pseudo-isothermal halo whose asymptotic speed is not chosen but solved for — it is whatever brings the total to the measured 220 km/s at 30 kpc, and comes out at 225 km/s. The components add in quadrature because accelerations add. The disc alone peaks at 6.6 kpc and falls away; the total does not.
Fig. 5 The Milky Way’s rotation curve, decomposed in the same way. The Sun sits at 8.2 kiloparsecs, where the circular speed is about 230 km/s — a number known to a few per cent from the proper motion of the radio source at the Galactic centre, which is one of the most direct measurements in the subject. The disc’s contribution peaks inside the Sun’s orbit and is already falling there; the halo’s is still rising.

The coincidence in the middle of the figure

There is a feature of the decomposition that ought to be more remarkable than it usually seems, and it has a name.

The disc’s contribution rises, peaks at about two and a quarter scale lengths, and falls. The halo’s rises monotonically. For the total to be flat, the halo’s rise has to compensate the disc’s fall — not roughly, but closely enough that no bump or dip appears in the observed curve at the crossover, and the observed curves are smooth to a few per cent.

That is a coincidence, because the two components have nothing to do with one another. The disc’s scale length is set by how the baryons cooled and settled; the halo’s core radius and asymptotic speed are set by how the dark matter collapsed. There is no reason for the second to know about the first, and yet the sum has no feature where they exchange dominance.

The problem has been called the disc–halo conspiracy since the 1980s, and it is the strongest argument against reading the decomposition too literally. Three responses are on offer and none is decisive.

The first is that the conspiracy is manufactured by the fitting. If the disc’s mass-to-light ratio is a free parameter chosen to make the total smooth, then smoothness is an output of the procedure rather than a property of the galaxy — which is precisely the disc–halo degeneracy stated as a criticism.

The second is that it is physical: the baryons settling into the disc pull the halo inwards, so the halo’s inner profile is shaped by the disc that formed inside it and the two are not independent after all. That is adiabatic contraction, it is calculable, and it produces some of the required correlation.

The third is that it is not a coincidence but a clue — that the acceleration scale at which the discrepancy appears is a constant across galaxies, which is the empirical claim underlying modified dynamics.

It is worth noticing that the three responses are not mutually exclusive and that the first one is testable on its own. If the smoothness were manufactured by the fit, then galaxies whose disc mass-to-light ratio is constrained independently — by stellar population modelling, or by the vertical velocity dispersion of the disc’s own stars — should show a residual bump at the crossover where the free fit produces none. Such measurements exist for a handful of nearby galaxies, and they do not show a bump, which weakens the first explanation without settling between the other two.

A feature that requires an explanation in one framework and is definitional in another is the sharpest kind of evidence available, and this one has not yet been made to decide between them.

What the picture cannot show

A rotation curve is a statement about mass inside a radius, and nothing else. It cannot distinguish a spherical halo from a thick, flattened one, because the enclosed mass is what enters and the shape is not. Flattening is constrained by other things — the vertical structure of the disc, the shapes of tidal streams — but not by the curve.

It says nothing about what the mass is. Every figure here is consistent with a halo of faint stars, of cold gas, of compact objects, or of a particle that has never been detected. The exclusion of the ordinary possibilities came later and from elsewhere: counts of faint stars, the absence of enough microlensing events towards the Magellanic Clouds, and the amount of ordinary matter allowed by the light-element abundances.

The straight line in the enclosed-mass figure has a beginning and an end. It is drawn where there is gas to measure. Inside a kiloparsec the beam of a radio telescope averages over the steep rise and the curve there is not measured so much as reconstructed; outside the last measured point, the curve is not known to be flat, it is simply not known.

And the decomposition is not unique. The three components in the first figure add in quadrature to the total, and a heavier disc with a lighter halo fits nearly as well as a lighter disc with a heavier one — the disc–halo degeneracy, which is the standing frustration of the subject. What the data fix tightly is the total; how it is divided depends on a mass-to-light ratio for the stars that has to come from stellar population models rather than from the curve.

How long it took to be believed

The history is instructive because the evidence arrived a long time before the conclusion did.

Jan Oort noticed in 1932 that the vertical motions of stars near the Sun implied more mass in the local disc than the counted stars supplied. Fritz Zwicky applied the virial theorem to the Coma cluster in 1933 and found a mass some two orders of magnitude above the light. Neither result changed anybody’s mind, and the reasons are ordinary: both were single measurements of hard quantities, both had error bars that a determined sceptic could widen, and neither had a shape to it — each was one number, larger than another number.

The rotation curves were different in kind. By the mid-1970s Vera Rubin and Kent Ford had optical curves for dozens of spirals, each one flat, each measured the same way, and each flat over a range of radius. Then the radio measurements pushed past the light and kept being flat. What made the case was not any single galaxy but the repetition of a shape across a population, which is the form of evidence this subject deals in more often than it deals in single crucial measurements — as the census of exoplanets also found.

It is worth being honest that the shape was not universally read as mass. Modified dynamics was proposed in 1983 precisely because a flat curve is what a modified force law would also produce, and it fits individual galaxy curves impressively well. What it does not do as easily is the cluster and the cosmological evidence, which is why the mass reading is the mainstream one — but the rotation curve alone does not settle it, and an essay that claimed otherwise would be overstating a genuinely good figure.

The same three readings for a second galaxy and a different viewing geometry are what turn one flat curve into a statement about galaxies.

The rotation curve of NGC 3198, decomposed. Circular speed against radius for a three-component model of NGC 3198: a Hernquist bulge of 1.0×10⁹ M☉, an exponential disc of 2.20×10¹⁰ M☉ with a scale length of 2.6 kpc, and a pseudo-isothermal halo whose asymptotic speed is not chosen but solved for — it is whatever brings the total to the measured 150 km/s at 30 kpc, and comes out at 171 km/s. The components add in quadrature because accelerations add. The disc alone peaks at 5.7 kpc and falls away; the total does not.
Fig. 6 The decomposition for a second spiral. The disc and bulge components fall as the light does, the observed curve does not, and the halo required to make up the difference has the same shape and a different amplitude — which is the pattern, not the exception.
What the Milky Way's light predicts, against what it does. The observed curve of the Milky Way against the curve its luminous mass alone would produce. Inside the disc the two nearly agree; at 30 kpc the observed speed is 2.24 times the luminous prediction, which is a factor of 5.2 in enclosed mass. The dotted curve is the pure Keplerian √(GM/r) for the 6.50×10¹⁰ M☉ of stars and gas, drawn from 12 kpc outwards where essentially all of it is enclosed — the fall every planetary system in this collection obeys, and no galaxy does.
Fig. 7 And the Keplerian prediction for the Milky Way. From inside the Galaxy the measurement is much harder and the conclusion is the same: the curve does not fall past the visible edge of the disc, and the discrepancy grows with radius rather than sitting at any particular place.

The generalisation

The pattern here recurs whenever a dynamical measurement is compared against a photometric one, and it is worth stating in its general form: a speed measures a mass, a brightness measures a luminosity, and the ratio of the two is a hypothesis.

The same reasoning weighs a binary star, where it is uncontroversial because both members are visible. It weighs a cluster of galaxies, where Fritz Zwicky applied it in 1933 and got an answer four hundred times the visible mass — four decades before the rotation curves, and largely ignored. It weighs a planetary system from a star’s reflex motion, and there the unseen component is a planet and nobody finds it surprising.

What makes the galactic case different is not the method but the shape of the answer. An unseen companion, an unseen planet, an underestimated stellar mass — all of those are corrections. A component whose enclosed mass rises linearly through and beyond the visible object is not a correction to the visible object; it is a larger object that the visible one is sitting inside.

And the twenty-one-centimetre profile at a steeper inclination, since the inclination is the one geometric quantity the whole measurement is divided by.

The twenty-one centimetre profile of a whole disc, at 80°. The hydrogen line profile emitted by the whole of NGC 3198, integrated over radius and azimuth from the same rotation curve drawn elsewhere in this collection, at an inclination of 80° and with an 8 km/s thermal and turbulent spread convolved in. The two horns are not two rings of extra gas: they are where the line-of-sight velocity stops changing with azimuth, at the near and far ends of the major axis, so a wide range of azimuth piles into a narrow range of velocity. The width at twenty per cent of the peak is 293 km/s, which is 2 v sin i to within 3 km/s — and it is the whole of what a distant galaxy's spectrum gives, which is why the Tully–Fisher relation is stated in terms of it.
Fig. 8 The line profile for a galaxy seen at eighty degrees rather than sixty. The horns move further apart in exact proportion to the sine of the inclination, so a rotation speed inferred from a profile is only as good as the inclination — and for a galaxy seen nearly face-on the correction is a division by a small number.

One more reading shows how much of the decomposition is actually determined by the curve.

Three mass models, 3.0× apart in the disc, agreeing to 3.6 km/s everywhere. NGC 3198's rotation curve, decomposed three ways. The stellar disc has been scaled by 0.1, 0.5, 0.9 times its photometric mass, and for each scaling the halo's asymptotic speed and core radius have been fitted — not chosen — to reproduce the same total. The heavy curve and the marked points are that total: the three models agree with it to 3.63 km/s at every radius, well inside a measurement error of 4.5. The light curves below are the disc's own contribution, and at 17 kpc they differ by a factor of 3.0 — from 26 to 77 km/s — with the halo taking up exactly the slack, 128 down to 104. The curve is one function and the decomposition asks for two. The free parameter is the mass-to-light ratio of the stars, which the kinematics never measures, and it is why a "maximum disc" fit and a halo-dominated fit are both published for the same galaxy. The degeneracy does have one hard edge: scaling the disc to 1.35 times its photometric mass cannot be fitted by any halo in the family — the best leaves 5.6 km/s rms — because past the maximum-disc solution the stars alone already overshoot the curve and a halo cannot have negative mass. That is the one thing a rotation curve says about M/L on its own, and it is an upper limit. What separates the rest has to come from somewhere else: the vertical velocity dispersion of the disc, which weighs the stars alone; gas-rich dwarfs where there is scarcely a disc to argue about; or the baryonic Tully–Fisher relation, which ties the halo's speed to the baryons and would be a coincidence if the two were independent.
Fig. 9 Three mass models spanning nearly the whole allowed range of disc mass-to-light ratio. All three fit the observed curve within its errors and they differ by a factor of nine in the stellar mass of the inner galaxy — the flatness is certain and the decomposition is not.

The flatness is a measurement and the decomposition is a model, and the two are routinely quoted with the same confidence. Only the first of them is what the observations actually establish.

Where the ladder goes next

The immediate question is what the ratio of the two curves looks like as a function of radius, and what it implies about how the mass is distributed rather than merely how much of it there is. The next essay takes that up.

Later rungs on this anchor: the disc–halo degeneracy and the maximum-disc hypothesis; the universal shapes fitted to halo profiles and the argument about whether their centres are cusped or cored; the baryonic Tully–Fisher relation and what it says about the coupling between the two components; the rotation curves of dwarf galaxies, where the halo dominates everywhere and the measurement is hardest; the outer curves traced by satellite galaxies and streams rather than by gas; the vertical structure of the disc as a second, independent dynamical constraint; and what modified dynamics gets right, which is more than its critics usually allow and less than a full account requires.

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 29 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.

Circular velocityDark haloDark matterEnclosed massExponential discFreeman's lawKeplerian declineMass-to-light ratioRotation curveThe 21-centimetre line