Spaceflight

An ocean found in a Doppler residual

A spacecraft flying past a moon is deflected by hundreds of metres a second, and the part of that deflection which says whether the moon has an ocean is two millimetres a second. Everything larger has to be modelled and removed first, exactly, and what is left over is an interior.

Assumes Radiometric navigation and Love numbers.

A spacecraft’s position is measured from a frequency: a signal is sent up, transponded coherently, received back, and the round-trip Doppler shift gives the line-of-sight velocity to a fraction of a millimetre per second. That precision is what makes deep-space navigation possible.

It also makes something else possible, which was not the original purpose. A spacecraft is a test particle, and a test particle’s trajectory records the field it moved through. If everything else about that trajectory can be modelled, the residual is the field — and the field, for a body nobody can enter, is the only access to the inside.

Two interiors, 2.59 mm/s apart, against a floor of 0.02. What a radio link measures when a spacecraft flies past a moon. The horizontal axis is time from closest approach in minutes and the vertical axis is the accumulated change in the line-of-sight velocity in millimetres per second, after the pull of the moon as a point mass has been fitted and removed. What is left is the part of the field that is not spherically symmetric, and the two curves are what two interiors predict for it. The upper one is a body whose tidal Love number is 0.616 — a shell floating on a global liquid layer, free to deform almost as a fluid would. The lower one is a body solid throughout, at 0.03. They differ by 2.59 millimetres per second in the accumulated deflection, against a floor of 0.02 for a coherent two-way X-band link integrated over tens of seconds: 130 standard deviations in a single pass. That ratio is the whole reason the measurement is possible, and it is worth stating what is being compared. The point-mass deflection itself is 837 metres per second — five orders of magnitude larger than the signature of interest — so the interior is not read off the Doppler curve but off the residual left after a model of everything larger has been subtracted: the moon's mass, the planet's, the spacecraft's own thrusting and outgassing, the plasma along the path, the station's motion, and relativity. Every one of those has to be right to a part in a hundred thousand before the last curve here means anything, which is why gravity science needs many passes and a global fit rather than one flyby and a subtraction. The published uncertainty on Titan's k₂ is eleven per cent rather than the fraction of a per cent this signal-to-noise would suggest, and the difference is entirely correlations with the other parameters in that fit — a reminder that a formal error on a curve is not the error on the number extracted from it. The straight-line path assumed here is exact only in the limit of a fast flyby; a slow one bends, and the bending is solved for rather than approximated.
Fig. 1 The residual two interiors predict, over one flyby, after the point mass has been fitted and removed. The upper curve is a body whose tidal Love number is 0.616 — a shell floating on a global ocean, free to deform nearly as a fluid would. The lower one is a body solid throughout. They differ by 2.6 millimetres per second in the accumulated deflection, against a floor of 0.02 for a coherent X-band link, which is a hundred and thirty standard deviations in a single pass.

A one-way Doppler measurement would require the spacecraft to carry a clock as good as the ground station’s, which no spacecraft does. So the measurement is two-way: the ground transmits a carrier locked to a hydrogen maser, the spacecraft’s transponder multiplies it by a fixed rational number and sends it straight back, and the ground compares what returns with what it sent.

The comparison is of phase rather than of frequency, accumulated over an integration time of tens of seconds. Counting cycles of an X-band carrier at eight gigahertz over sixty seconds is counting about half a trillion cycles, and a fractional error of 101310^{-13} corresponds to a line-of-sight velocity error of about three hundredths of a millimetre per second.

That is the floor, and it is set by the maser, by the troposphere’s wet delay, and by the plasma along the path. Every one of those is a term that has to be calibrated rather than assumed.

An eight-hour pass, and a 351 m s⁻¹ sinusoid that is the whole of the angle. Above: the range rate a two-way Doppler measurement returns over one pass from Goldstone, for a spacecraft receding at 14.6 km s⁻¹. Nothing here is an angle. The measurement is the fractional shift of a carrier the spacecraft coherently turned around and sent back, and its interpretation is that the distance is changing at some rate. Below: the same data with the spacecraft's own smooth signature removed. What is left is a sinusoid of exactly one cycle per day — the station's own motion, carried east at 379 metres a second by the rotation of the Earth, projected onto the line of sight. Its amplitude is that speed times cos δ and returns a declination of 22.0°; its zero crossing is the moment the spacecraft passed the meridian and returns the right ascension. The Earth's rotation is the interferometer. With Doppler good to 0.05 mm s⁻¹ at a 60-second cadence, 480 samples fit that amplitude to 0.003 mm s⁻¹ and the declination to 23 nanoradians — which is 4.7 milliarcseconds, from an instrument with no image plane and no angular resolution of any kind. What the picture cannot show is the part that makes this hard in practice: the spacecraft's own signature is not a straight line but a trajectory with unmodelled accelerations in it, and separating a slow non-gravitational force from a slow drift in the angles is the whole art of the fit.
Fig. 2 What a pass looks like before anything is removed. The dominant signature is a sinusoid of hundreds of metres per second amplitude at one cycle per day — the station’s own motion as the Earth turns — and the spacecraft’s trajectory is a slow drift underneath it. Every quantity of interest is a small residual after the diurnal term, the Earth’s orbital motion, the spacecraft’s own thrusting and the media delays have all been subtracted, and each of those subtractions is a model with parameters of its own.

There is a second observable in the same signal that is worth distinguishing, because the two are often lumped together as “tracking”. Ranging measures the round-trip time of a modulation imposed on the carrier, and gives a distance to a metre or two. Doppler measures the rate of change of that distance and gives a velocity to hundredths of a millimetre per second. For a gravity measurement the second is far more useful, because what a field does to a trajectory is an acceleration, and integrating an acceleration once gives a velocity while integrating it twice gives a position that has drifted away from any initial condition.

So gravity science is done in the velocity domain. The observable is a curve of line-of-sight velocity against time through the encounter, and the interior appears as a particular shape in it.

Why the tidal part is the variable part

A moon’s gravity field, measured on a flyby, is dominated by its mass. Fitting that leaves a residual containing the quadrupole — the departure from sphericity — and a moon’s quadrupole has two parts.

One is static: the permanent bulge produced by its rotation and by the average tide from its primary. That part is indistinguishable from any other contribution to J2J_2, and it says very little about the interior on its own, because a rigid body and a fluid one can have the same permanent figure if the fluid one froze in an earlier shape.

The other part varies. A moon on an eccentric orbit experiences a tide whose strength changes through the orbit, and a deformable body responds by changing shape — so its quadrupole oscillates at the orbital period, with an amplitude proportional to the tidal Love number. To first order in the eccentricity the variable part is 3e3e times the static one, which for Titan’s e=0.0288e = 0.0288 is about nine per cent.

That is the signal. It is small, and it is the only part of the field that separates a body that deforms from one that does not.

The consequence for mission design is stark: a single flyby cannot do it. What is needed is several flybys at different points of the moon’s orbit, so that the varying part can be seen to vary, and the static part solved for simultaneously. Titan’s Love number came from six such encounters spread over years. It is worth attaching the numbers to that hierarchy, because the ratios are what make the measurement difficult rather than the absolute values. For a thousand-kilometre flyby of Titan the point-mass deflection is around eight hundred metres per second. The static quadrupole contributes something like a metre per second. The variable tidal part is a few millimetres per second. Each step down is a factor of a thousand, and each one has to be modelled to better than a part in a thousand before the next is visible.

That is the shape of every measurement in this essay and it is the reason gravity science is a matter of fitting rather than of reading. Nothing is measured directly; everything is a parameter in a joint solution, and the interior is whatever is left when the rest of the universe has been accounted for.

What has to be removed first

The chain from a frequency to a Love number passes through a great many models, and it is worth listing them because the final error bar is dominated by them rather than by the noise.

The station. Its position in a terrestrial reference frame, the Earth’s orientation including polar motion and the length-of-day variation, and solid-Earth and ocean tides at the station.

The media. The troposphere’s dry and wet delays, calibrated with water-vapour radiometers; the ionosphere’s dispersion, removed by observing at two frequencies; and the solar plasma along the path, which is the worst of the three near solar conjunction and is the reason gravity-science passes are scheduled away from it.

The planetary ephemeris. The positions of the Sun, the target planet and the moon, each of which has its own uncertainty.

Relativity. The Shapiro delay, the gravitational frequency shift, and the aberration of the light path — all of which are larger than the signal.

The spacecraft itself. Solar radiation pressure, thermal re-radiation from the spacecraft’s own surfaces, anisotropic emission from its radioisotope generators, and any propulsive event including attitude-control thruster firings. This is usually the limiting term, and it is why gravity-science passes are flown with the reaction wheels doing the pointing.

A metre along the line of sight and 4 kilometres across it. Above: the round-trip light time of a ranging signal, against distance. It is a straight line of slope one, which is the point — the delay is the distance, with no model and no calibration between them, and a code correlated to a few nanoseconds gives the radial coordinate of a spacecraft at Mars to about 1 metre. Below: what the same tracking session gives across the line of sight. The angle is good to 50 nanoradians — the Doppler noise alone would give 12, and the difference is the troposphere, the station coordinates and the solar plasma, none of which average down — and an angle times a distance is a length that grows: at Mars's 0.52 au it is 4 kilometres, 3890 times the radial error. The error region of an interplanetary spacecraft is therefore not a sphere but a pancake, thin along the line of sight and enormously wide across it, and every operational consequence follows from that shape: a Mars arrival is aimed at a corridor in the plane of the sky rather than at a distance, the last approach manoeuvres are almost entirely lateral, and the observation that improves the fit most is never another day of Doppler but a single differenced measurement against a quasar. The cheapest observable measures the coordinate that matters least.
Fig. 3 The geometry that makes some directions easy and others hard. A Doppler measurement gives the line-of-sight component of velocity to a fraction of a millimetre per second and constrains the two transverse components hardly at all — the error region is a pancake, thin along the line of sight and thousands of times wider across it. A flyby’s geometry decides how much of the deflection falls into the well-measured direction, and it is designed for that.

Why the published error is not the noise

The figure at the top of this essay says a hundred and thirty sigma. The published uncertainty on Titan’s Love number is eleven per cent, which is nine sigma.

The difference is entirely correlations. In a real analysis the Love number is one parameter among dozens solved for simultaneously: the mass, the static J2J_2 and C22C_{22}, the moon’s ephemeris, the spacecraft’s state at each encounter, the non-gravitational accelerations. Several of those produce signatures in the Doppler residual that resemble the tidal one, and the fit cannot fully separate them.

The formal error on a parameter in a joint fit is the square root of the corresponding diagonal element of the inverse of the normal matrix, and when parameters are correlated that is much larger than the error the parameter would have alone. Quoting the single-parameter precision would be reporting the wrong number by an order of magnitude.

This is a general feature of the technique and not a criticism of it. It is also the reason that adding a flyby helps far more than adding integration time to an existing one: a new encounter at a different orbital phase breaks a correlation, and lowering the noise on an existing one does not.

A nanosecond across the Earth is 35.69 nanoradians on the sky. The angular accuracy of a differenced-delay measurement against the length of the baseline it is measured on, both axes logarithmic, for three levels of delay precision. The relation is σ_θ = cσ_τ/B and nothing else, so every curve is a straight line of slope −1.00: the only two ways to measure an angle better are a better clock or a wider Earth, and only one of those is available. The three marked baselines are the ones that exist — the deep-space complexes in California, Spain and Australia, 8,400, 10,600, 11,700 kilometres apart. On the longest of them a delay good to 0.05 nanoseconds is 1.28 nanoradians, which at 0.52 astronomical units is 100 metres across the line of sight; a more typical 0.15-nanosecond measurement on the shortest baseline is 5.35 nanoradians. What makes any of this survivable is that the same pair of antennas observes a quasar a few degrees away immediately afterwards. The quasar is at infinity, its position is known better than the measurement, and subtracting its delay from the spacecraft's removes the clock offsets, the water vapour over each dish and the station coordinates in one step — so the number that comes out is not a delay at all but an angular separation from a fixed point in the sky.
Fig. 4 The complementary observable, which measures the direction the Doppler cannot. Observing the spacecraft and a quasar alternately with two widely separated antennas gives the angle between them to nanoradians, in the plane of the sky. Combining an angular measurement with a line-of-sight one turns the pancake into something closer to a sphere, and for gravity science it constrains the flyby geometry that the field is being solved against.

There is a useful diagnostic that follows from all this and that a reader can apply to any published gravity result. Ask how many independent encounters went into it, and at what spread of orbital phase. A field determined from one flyby has its parameters completely entangled; three encounters at similar phases add little; six spread through an orbit are what separate a static quadrupole from a tidal one. The number of flybys is a better guide to the reliability of a result than the number of significant figures.

Two angles from one sinusoid, and each of them fails where the other is best. What a pass of 8 hours of 0.05 mm s⁻¹ Doppler from Goldstone is worth as an angle, against the declination of the spacecraft. The diurnal signature carries both angles and carries them differently. Its amplitude is the station's east velocity times cos δ, so inverting it for the declination divides by sin δ and the error runs away at the celestial equator: at 2° it is 244 nanoradians, thirty times worse than at 45°. Its phase is the right ascension directly, and recovering a phase from a sinusoid of amplitude proportional to cos δ divides by that cosine, so the right ascension is the one that fails near the pole. The two curves cross at exactly 45° because 1/sin and 1/cos do. Neither failure is a defect of the instrument, and neither can be reduced by tracking longer: at zero declination the station's motion is entirely along the line of sight all day, so no amount of it contains any information about how far north the spacecraft is. The geometry is degenerate rather than noisy. That is the whole reason a deep-space network also observes quasars: a differenced one-way range against a source of known position measures the plane-of-sky angle directly and does not care about the declination at all — and every Mars mission needs it, because a transfer to Mars spends most of its cruise within ten degrees of the equator.
Fig. 5 What a pass constrains and what it does not. The information a tracking arc carries about each parameter depends on the geometry, and the parameters an encounter is insensitive to are not improved by observing it longer. That is the reason a gravity campaign is designed as a set of encounters at chosen phases rather than as an integration time, and it is the practical form of the correlation problem this essay is about.

The signal the whole result rests on scales with two things a mission designer chooses, and both are worth reading at values a real trajectory might have taken.

Two interiors, 4.98 mm/s apart, against a floor of 0.02. What a radio link measures when a spacecraft flies past a moon. The horizontal axis is time from closest approach in minutes and the vertical axis is the accumulated change in the line-of-sight velocity in millimetres per second, after the pull of the moon as a point mass has been fitted and removed. What is left is the part of the field that is not spherically symmetric, and the two curves are what two interiors predict for it. The upper one is a body whose tidal Love number is 0.616 — a shell floating on a global liquid layer, free to deform almost as a fluid would. The lower one is a body solid throughout, at 0.03. They differ by 4.98 millimetres per second in the accumulated deflection, against a floor of 0.02 for a coherent two-way X-band link integrated over tens of seconds: 249 standard deviations in a single pass. That ratio is the whole reason the measurement is possible, and it is worth stating what is being compared. The point-mass deflection itself is 1041 metres per second — five orders of magnitude larger than the signature of interest — so the interior is not read off the Doppler curve but off the residual left after a model of everything larger has been subtracted: the moon's mass, the planet's, the spacecraft's own thrusting and outgassing, the plasma along the path, the station's motion, and relativity. Every one of those has to be right to a part in a hundred thousand before the last curve here means anything, which is why gravity science needs many passes and a global fit rather than one flyby and a subtraction. The published uncertainty on Titan's k₂ is eleven per cent rather than the fraction of a per cent this signal-to-noise would suggest, and the difference is entirely correlations with the other parameters in that fit — a reminder that a formal error on a curve is not the error on the number extracted from it. The straight-line path assumed here is exact only in the limit of a fast flyby; a slow one bends, and the bending is solved for rather than approximated.
Fig. 6 The same two interior models at a flyby altitude of three hundred kilometres rather than a thousand. The difference between them grows to nearly five millimetres a second, because the tidal signal falls off steeply with altitude — which is why the decisive passes are the lowest ones and why they are also the most dangerous.
Two interiors, 1.30 mm/s apart, against a floor of 0.02. What a radio link measures when a spacecraft flies past a moon. The horizontal axis is time from closest approach in minutes and the vertical axis is the accumulated change in the line-of-sight velocity in millimetres per second, after the pull of the moon as a point mass has been fitted and removed. What is left is the part of the field that is not spherically symmetric, and the two curves are what two interiors predict for it. The upper one is a body whose tidal Love number is 0.616 — a shell floating on a global liquid layer, free to deform almost as a fluid would. The lower one is a body solid throughout, at 0.03. They differ by 1.30 millimetres per second in the accumulated deflection, against a floor of 0.02 for a coherent two-way X-band link integrated over tens of seconds: 65 standard deviations in a single pass. That ratio is the whole reason the measurement is possible, and it is worth stating what is being compared. The point-mass deflection itself is 419 metres per second — five orders of magnitude larger than the signature of interest — so the interior is not read off the Doppler curve but off the residual left after a model of everything larger has been subtracted: the moon's mass, the planet's, the spacecraft's own thrusting and outgassing, the plasma along the path, the station's motion, and relativity. Every one of those has to be right to a part in a hundred thousand before the last curve here means anything, which is why gravity science needs many passes and a global fit rather than one flyby and a subtraction. The published uncertainty on Titan's k₂ is eleven per cent rather than the fraction of a per cent this signal-to-noise would suggest, and the difference is entirely correlations with the other parameters in that fit — a reminder that a formal error on a curve is not the error on the number extracted from it. The straight-line path assumed here is exact only in the limit of a fast flyby; a slow one bends, and the bending is solved for rather than approximated.
Fig. 7 And at twice the flyby speed. The spacecraft spends half as long inside the region where the signal is large, and the accumulated velocity difference falls in proportion — so a slow encounter is worth as much as a low one, and a mission gets to choose between them only through its arrival geometry.

Where else the same measurement has been made

Enceladus. Three close flybys measured a gravity field whose J2J_2 and C22C_{22} ratio departs from the hydrostatic value in a way consistent with a regional or global sea. The gravity result on its own was ambiguous; combined with the libration amplitude it is not.

Europa. Galileo’s flybys gave J2J_2 and C22C_{22} and hence a moment of inertia of 0.346 — a differentiated body with a metallic core — but not a Love number, because the flybys were too few and not spread in orbital phase. Europa’s tidal response is the primary objective of two missions now on their way.

Jupiter. A close polar orbit measured the zonal harmonics to degree ten and beyond, and read a dilute core out of them. The same instrument and the same technique, applied to a body that is all interior — and the odd harmonics, which a symmetric body cannot have, gave the depth of the winds.

The Moon. Two spacecraft flying in formation measured their separation to microns with a link between them, which is a far more sensitive geometry than a link to the Earth, and produced a lunar gravity field to degree 900.

Two frequencies, and why one is not enough

The link described above was treated as a single carrier, and a gravity-science spacecraft carries two. The reason is the one term in the error budget that cannot be modelled and can be cancelled.

The solar plasma along the signal path is a dispersive medium: it delays a signal by an amount proportional to the square of the wavelength. Everything else in the chain — the geometry, the troposphere’s wet delay, the spacecraft’s own motion — is non-dispersive and affects both frequencies identically.

So observing at two well-separated frequencies and differencing gives the plasma term directly, and removing it leaves the part that is about the trajectory. That is the same differencing logic that removes the clock offset from an interferometric delay, applied to a different contaminant.

The choice of frequencies follows from the same scaling. A carrier at 32 gigahertz suffers about a fourteenth of the phase noise from plasma that one at 8.4 gigahertz does, so the higher band is where the measurement is made and the lower one is there partly to calibrate it and partly because it is what the rest of the spacecraft’s communications use.

The cost is that a higher frequency needs a tighter beam and therefore better pointing, and it is more strongly attenuated by rain at the ground station. Those are the reasons the higher band was not adopted for everything, and they are why a gravity campaign is scheduled against weather at the receiving complex in a way ordinary tracking is not.

The measurement’s precision is therefore a property of the sky between two points as much as of the equipment at either end, and the term that dominates it varies over the solar cycle.

There is a result from exactly this apparatus that has nothing to do with any moon, and it is worth recording because it shows what a well-characterised link is worth once it exists.

When a spacecraft passes behind the Sun as seen from the Earth, the radio signal travels through the Sun’s gravitational field, and general relativity says the round-trip time is lengthened by an amount depending on how close the path passes to the Sun. The effect is a delay of about a fifth of a millisecond at grazing incidence, and it is proportional to a parameter that measures how much space-time curvature a unit mass produces — exactly one in general relativity, and adjustable in the alternatives.

Measuring it requires the same things a gravity flyby requires: a coherent two-way link, a model of everything else affecting the path, and a way to remove the plasma. The last of those is the hard part, because the signal is passing through the corona, which is where the plasma is thickest and most variable — so the experiment is done at the one geometry where the dominant error term is at its worst.

The dual-frequency link is what makes it possible, and the result is a confirmation of the prediction to about two parts in a hundred thousand, which stood for two decades as the tightest test of its kind.

That is a measurement of the theory of gravitation, made with equipment built to find out where a spacecraft was, using a calibration developed to weigh a moon. The instrument was a radio link and everything else about it was a choice of what to point it through, which is the most economical description of this whole technique.

The moment the technique became a science instrument

It is worth recording that gravity science was not designed. Deep-space tracking exists to navigate, and the accuracy it achieves was driven by the need to hit an aim point at a planet after a cruise of years.

The first interior results were by-products. Ranging and Doppler data collected for navigation were reprocessed afterwards, and the masses of the outer planets and their major satellites — quantities that had been known to a per cent from centuries of astrometry — improved by three or four orders of magnitude within a decade of the first flybys. The moment-of-inertia factors that populate the comparison of solar-system interiors mostly came out of that reprocessing.

What changed later was that missions began to be flown for the measurement: trajectories chosen for their gravity yield rather than for their imaging opportunities, encounters scheduled at particular orbital phases, and passes flown with the spacecraft’s own accelerations minimised. The Titan Love number is a result of that second era, and it could not have been extracted from data taken for any other purpose. Both of those results share a property worth naming: the quantity that limited them was the same one, and it was neither the clock nor the antenna. It was the plasma between here and there, which is why the two frequencies are the instrument as much as the dish is.

What the residual cannot say

It does not see the ocean. What is measured is a deformation larger than a solid can produce. Everything after that — that the deformation is due to a decoupling shell, that the decoupling layer is liquid, that the liquid is water — is inference, of the kind a Love number always requires, resting on the composition being what a body of that density and formation location should be made of.

It does not give a depth. A Love number is one integral of the interior; it constrains a combination of the shell’s thickness, the ocean’s depth and the underlying rigidity, and inverting for any one requires assuming the others. Titan’s ocean depth is quoted with a range of hundreds of kilometres.

It is a snapshot. The measurement is of a response at one frequency, the orbital one. A body whose rheology is frequency-dependent — which is every real body — responds differently at other periods, and nothing in a flyby campaign measures that. The ambiguity between a stiff interior and a soft one is not resolved by a static Love number either. And the tracking geometry itself at a high declination, since what a single pass can separate depends on how much of the sky the antenna sweeps through during it.

An eight-hour pass, and a 189 m s⁻¹ sinusoid that is the whole of the angle. Above: the range rate a two-way Doppler measurement returns over one pass from Goldstone, for a spacecraft receding at 14.6 km s⁻¹. Nothing here is an angle. The measurement is the fractional shift of a carrier the spacecraft coherently turned around and sent back, and its interpretation is that the distance is changing at some rate. Below: the same data with the spacecraft's own smooth signature removed. What is left is a sinusoid of exactly one cycle per day — the station's own motion, carried east at 379 metres a second by the rotation of the Earth, projected onto the line of sight. Its amplitude is that speed times cos δ and returns a declination of 60.0°; its zero crossing is the moment the spacecraft passed the meridian and returns the right ascension. The Earth's rotation is the interferometer. With Doppler good to 0.05 mm s⁻¹ at a 60-second cadence, 480 samples fit that amplitude to 0.003 mm s⁻¹ and the declination to 10 nanoradians — which is 2.0 milliarcseconds, from an instrument with no image plane and no angular resolution of any kind. What the picture cannot show is the part that makes this hard in practice: the spacecraft's own signature is not a straight line but a trajectory with unmodelled accelerations in it, and separating a slow non-gravitational force from a slow drift in the angles is the whole art of the fit.
Fig. 8 An eight-hour pass on a target sixty degrees north. The antenna’s own motion carried by the Earth’s rotation is a smaller fraction of the line-of-sight direction, so the geometric signature that separates a position error from a velocity error is weaker — and a target near the pole is one whose position is hardest to fix from Doppler alone.

Where the ladder goes

The earlier rungs of this anchor were about navigation: a position from a frequency and an angle from a quasar. Both are about knowing where a spacecraft is. This one is about what the spacecraft is for.

The natural next steps are the ones the missions now in flight will supply. A spacecraft in orbit around an icy moon rather than flying past it can measure the time-variable field over many cycles, separating the tidal response from everything static, and can reach the higher harmonics that say how the shell’s thickness varies. And a link between two spacecraft — the geometry that mapped the Moon — measures a gradient rather than a velocity, which is a far stronger constraint on a small body’s field than anything achievable from the Earth.

About the same objects

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

What links here

Essays that link to this one from their own argument.

The objects this essay names

Each one links to every other essay that touches it.

CovarianceDeep-space networkDoppler trackingFlybyGravity scienceLove numberOrbit determinationSolar plasmaSystematic errorTwo-way coherentZonal harmonic