Nothing in the sky is weighed in kilograms
Assumes Harmonic law and Shell theorem.
Ask how heavy the Sun is and the answer given is kilograms. Four significant figures, and the fifth is uncertain — not because the Sun is hard to observe, but because nobody can weigh anything to better than about twenty parts in a million using gravity, and the difficulty is entirely in a laboratory on Earth.
Ask instead for the Sun’s gravitational parameter, the product , and the answer is , good to something like a part in .
The same object, the same physics, six orders of magnitude of difference in how well it is known. Everything in this essay follows from noticing which of those two numbers astronomy actually uses.
What an orbit actually reports
Newton’s law contains the product of two things that never appear separately in any orbital calculation. Write the acceleration of a body at distance from a mass :
and occur together and nowhere else. No measurement of any trajectory — a moon, a planet, a spacecraft, a star in a binary — can separate them, because the equation of motion has no term in which they are apart. What an orbit determines is the product, and the product has its own name and symbol, , the standard gravitational parameter. Every gravitational quantity in astronomy is of this kind. Escape speed is . Orbital speed is . The Schwarzschild radius is . The Hill radius involves only mass ratios. In none of them can be removed from , and in none of them does anybody want to.
The system built to avoid the problem
Astronomy noticed this early and built its unit system around it.
Gauss, in 1809, defined a constant by fixing the Earth’s orbital period, the Earth’s mass and the astronomical unit, and taking in those units. The consequence was that was a defined number, 0.01720209895, rather than a measured one, and every planetary calculation could be carried out to full precision with no reference to any laboratory. Masses were quoted in solar masses. Distances were quoted in astronomical units. Times were quoted in days. In that system the gravitational constant does not appear.
The consequence is a fact worth stating plainly. The mass ratios in the solar system were known to a few parts in a thousand more than a century before anybody had a decent value of , because a ratio of masses is a ratio of two values and the divides out. Newton computed the Sun-to-Jupiter ratio in the Principia and got 1067 against a modern 1047, with no gravitational constant in existence at the time and no concept of one. The unit system was retired in stages: the astronomical unit is now a defined length, exactly 149,597,870,700 metres, fixed by the IAU in 2012 after radar and spacecraft ranging had made the old parallax-based determinations obsolete; and is now quoted as a measured quantity in SI units. But the underlying situation is unchanged. Planetary ephemerides are fitted with values as parameters, and no ephemeris in the world contains .
Why the constant is so hard
The gravitational constant has been measured for two and a quarter centuries and its uncertainty has improved by about three orders of magnitude in that time — while became exact, became exact, and the electron’s magnetic moment reached twelve significant figures. Four features of gravity explain the gap, and none of them is going away.
It cannot be shielded. Every electromagnetic measurement can be put inside a Faraday cage and its background removed. There is no gravitational cage, so the mass of the experimenter, the water table under the building and the tidal position of the Moon are all present in the signal.
It cannot be modulated. The standard defence against drift and noise is to switch the effect on and off at a known frequency and detect only that frequency. Gravity has no switch. What torsion-balance experiments do instead is move the source masses, which introduces exactly the systematic — a change of geometry — that the measurement is most sensitive to.
It is absurdly weak. The gravitational attraction between two protons is smaller than their electrostatic repulsion by about . A laboratory measurement of works with forces of order newtons in the presence of the Earth’s pull on the same apparatus, which is times larger.
And it needs a mass metrology, not just a force metrology. Every other route to a fundamental constant can be made to depend on a frequency, and frequencies are the best-measured quantities in existence. The source masses must be weighed, their density inhomogeneities characterised, and their positions known to microns. Several of the discrepant results in the figure differ in ways that have been traced to how the source masses’ density was assumed to be distributed.
The result is the state the hero figure shows: not a random scatter around a value, but a set of careful experiments with small quoted errors that disagree with each other. CODATA’s response has been to inflate the recommended uncertainty by a factor of several beyond what a weighted combination would give — an admission that at least one unidentified systematic is at large.
Cavendish did not measure G
The experiment everybody names is the one that did not do this.
Henry Cavendish’s 1798 paper is titled Experiments to Determine the Density of the Earth, and that is what it reports: 5.48 times the density of water, against a modern 5.514. The gravitational constant appears nowhere in it, for the excellent reason that it had not been invented — Newton’s law was written as a proportionality, and the symbol with a numerical value attached does not appear in the literature until Cornu and Baille in 1873.
What Cavendish did was compare two attractions. His torsion balance measured the pull of two lead spheres on two smaller ones; the Earth’s pull on the same small spheres was already known, being their weight. The ratio of the two attractions, with the geometry, gives the ratio of the Earth’s mass to the lead spheres’ — and the lead spheres could be weighed. A density came out, not a constant.
That framing is worth recovering, because it is the same trick the rest of this essay is about, run in the other direction. Cavendish did not need because he took a ratio; astronomy does not need because it takes ratios. Extracting a constant from his result is a modern back-formation, and doing it gives , which is within one per cent of the current value and better than several nineteenth-century determinations that were trying.
And it costs astronomy almost nothing
Here is the part that surprises people, and it is the reason this essay belongs in a collection about the sky rather than one about metrology.
A 22-parts-per-million uncertainty in propagates directly into the mass of every astronomical body expressed in kilograms. It propagates into essentially nothing else, because astronomy almost never expresses a mass in kilograms. Where the constant does bite is at the joins between astronomy and physics, and the list is short and specific: the number of baryons in a star, which needs a mass in kilograms and a proton mass; the mean density of the universe expressed as a critical density, where appears explicitly in ; the equation of state of a neutron star, where a laboratory nuclear physics must be matched to an astronomical mass. It also bites, quietly, wherever a stellar model is integrated: the interior equations carry explicitly, so the pressure that holds a star up and the gradient that decides whether it convects are computed with it. In each of those a 22-ppm uncertainty is negligible against everything else in the calculation — the critical density’s own uncertainty is dominated by , which is disputed at the level of eight per cent, or three and a half thousand times worse.
What was actually measured, and when the units changed
The astronomical unit is the hinge of this whole story, because for three centuries it was the one length in the solar system that had to be measured rather than computed.
Every planetary distance was known as a ratio to the Earth’s, from Kepler’s laws and timed observations, to a precision far better than the absolute scale. Fixing that scale required one absolute measurement, and successive attempts are a history of the subject: the transits of Venus of 1761, 1769, 1874 and 1882, whose timings gave the solar parallax to about a part in a thousand; the parallax of the asteroid Eros at its 1930–31 opposition, which reached about ; and then radar.
The 1961 radar echoes from Venus fixed the astronomical unit to about a part in overnight, and spacecraft tracking has since improved it to a few parts in . At that point the AU stopped being a measurement at all and became a defined conversion factor. The last absolute length in solar-system astronomy was retired by a radio pulse and a stopwatch.
The Earth’s own parameter tells the same story one step closer to home. Satellite laser ranging — bouncing pulses off retroreflectors on LAGEOS and its successors, and timing the return to a few millimetres — gives , to about two parts in . Dividing by to obtain the Earth’s mass in kilograms throws away four of those nine digits at a stroke. The Earth is the best-characterised object in the universe and its mass is the worst-known thing about it.
What the picture cannot show
The hero figure computes a difference between its two groups and the difference is not the story. It reports 9.3 standard deviations between the torsion-balance family and the rest, which is what its arithmetic gives; but the same arithmetic applied within the torsion-balance family would report an equally severe inconsistency. The disagreement does not sort by method. It sorts, as far as anybody can tell, by laboratory, and that is precisely what makes it hard to fix.
Nothing here says is variable. A constant that different experiments disagree about is not the same as a constant that changes, and the astronomical constraints on the latter are far tighter than the laboratory ones on the former: lunar laser ranging bounds below about per year, and binary-pulsar timing does comparably well. The best evidence that is constant comes from the sky; the best measurements of its value do not.
And the two headline numbers are not directly comparable. at a part in is the parameter of an ephemeris fitted to ranging data over decades, and its uncertainty is a formal one within a model containing hundreds of other parameters. It is an excellent number and it is not the same kind of object as a laboratory result with an error budget itemised line by line.
And a figure of determinations is not a figure of the truth. Every interval drawn in the hero figure is its own authors’ honest estimate of their own systematics, and the whole content of the picture is that at least one of those estimates is wrong. A plot like this can show inconsistency and can never show which point is at fault; identifying that requires somebody to repeat somebody else’s apparatus, which is expensive, unglamorous and exactly what the field has spent the last decade doing.
Both rungs share a question this essay has dodged. If a mass ratio is what astronomy measures, and the solar mass is the unit, then what is being asserted when a galaxy is said to weigh solar masses? The answer is that a ratio has been taken between two gravitational parameters twelve orders of magnitude apart, measured by entirely different means, and that the chain connecting them is as long as any distance ladder — which is a different essay and a longer one.
Weighing an ice sheet
There is a class of measurement in which a mass in kilograms is genuinely what is wanted, and it is worth describing because it shows that even there the constant mostly cancels.
A pair of satellites in the same orbit, separated by a couple of hundred kilometres and ranging to each other by microwave link, measure the distance between themselves to a fraction of a micron. As they pass over a region of excess mass, the leading satellite is accelerated first and the separation changes; a hundred kilometres later the trailing one catches the same pull and it changes back.
Integrating those changes over the whole orbit, month after month, maps the Earth’s gravity field and — more usefully — how it changes. The changes are seasonal and secular: groundwater moving, ice sheets shrinking, the crust rebounding from the last glaciation.
The results are quoted in gigatonnes per year, which is a mass rate in kilograms, and the numbers are the primary measurement of how fast the Greenland and Antarctic ice sheets are losing mass.
Now notice what the constant does there. What is measured is a change in the gravitational parameter of a region — a change in , not in — so converting it to a mass requires dividing by , and a 22-parts-per-million error in is a 22-parts-per-million error in the ice loss. The published uncertainties on those rates are several per cent, dominated by how the signal is separated from the crust’s rebound. The constant contributes a term a thousand times smaller than the smallest thing anyone argues about.
Even the one measurement whose answer must be in kilograms is unaffected, because a mass difference inherits the same fractional error as a mass and the fractional error is negligible against everything else.
The redefinition that left it out
In 2019 the SI base units were redefined so that a set of constants take exact values: the speed of light, the Planck constant, the elementary charge, the Boltzmann constant and the Avogadro constant. The kilogram in particular stopped being a lump of metal in a vault and became a quantity derived from the Planck constant, realised by an instrument that balances a mechanical force against an electromagnetic one.
The gravitational constant was not in the list, and it could not have been.
The redefinition works by tying each unit to a phenomenon whose measurement reduces to a frequency, because frequencies can be measured to eighteen digits against an atomic clock. The kilogram’s realisation is a comparison between mechanical and electrical power, both of which reduce to voltages and velocities that are ultimately frequencies.
There is no frequency in gravity. Every route to requires measuring a force, or a displacement, or a period of a torsion oscillator whose restoring constant must itself be calibrated — and none of them reduces to a frequency comparison against a clock. So cannot be fixed by definition without making some other quantity worse, and it remains one of the few constants in the tables that is measured rather than assigned.
The situation has a curious consequence for the mass of the Sun. Now that the kilogram is defined through the Planck constant, expressing a solar mass in kilograms means connecting an astronomical measurement to a quantum-mechanical definition through a constant known to twenty-two parts in a million — and the chain from a planet’s orbit to a photon’s energy passes through the least reliable link in the whole system of units.
The constant that governs the largest structures in the universe is the one the metrologists could not include, and the reason is that gravity does not oscillate at a frequency anybody can count.
One more dataset puts the same disagreement beside a constant everybody agrees is measured well.
Where the ladder goes next
The obvious rung is the one where the ratio trick runs out: extragalactic astronomy, where masses are quoted in solar masses because there is no alternative, and the solar mass itself has become a unit rather than a measurement. The rung beside it is the geodetic one — the Earth’s own , known to two parts in from satellite laser ranging, against the Earth’s mass, known to 22 parts in , which is the same disparity as the Sun’s and considerably easier to check.
What this makes readable
Essays that name this one as a prerequisite.
- The field a satellite is allowed to feel gravitation
What links here
The 8 of 16 essays linking to this one that name the most of the same objects.
- The third law is wrong by the mass of the planet orbits
- The region a planet may keep a moon in gravitation
- The stage that has to be thrown away spaceflight
- A birth rate measured from light nothing young emitted galaxies
- A clock that runs down and says what it is stars
- A comet that arrives a day early orbits
- A floor under the centre that assumes nothing stars
- A particle count taken from a dwarf galaxy cosmology
The objects this essay names
Each one links to every other essay that touches it.
Astronomical unit (AU)Dimensional analysisGravitational constantKepler's third lawMass ratioRadar rangingSolar massStandard gravitational parameterSystematic errorTorsion-balance