Gyroscope and Its Applications
In February 1953 a transport aircraft took off from Bedford, Massachusetts and flew to Los Angeles with no radio fixes, no celestial sightings, and no view of the ground it needed. A one-ton instrument in its belly — gyroscopes and accelerometers, integrating Newton's laws in real time — knew where the aircraft was the entire way. The error after twelve hours of flight was about ten miles. Every airliner, submarine, and spacecraft since has carried a descendant of that box, and the physics inside it is the physics of this article: a symmetric top spun so fast that its angular momentum becomes a reference direction more trustworthy than the horizon. A gyroscope is mechanically nothing more than that top — a rotor with spinning about its symmetry axis. What turns it into an instrument is a regime and a choice. The regime: spin angular momentum so large that disturbing torques can barely move it, . The choice: either isolate the rotor in gimbals and read orientation off its space-fixed axis, or constrain it and measure the reaction torque it exerts when the vehicle turns. Rigidity or reaction — every gyroscopic device in history is one of the two. This article is the applications payoff of the whole rigid-body chapter. The precession law, the Euler-angle kinematics, and the heavy-top machinery are assembled here into the gyrocompass that finds true north from Earth's own spin, the MEMS chip in your phone that senses rotation with a vibrating speck of silicon, the fiber-optic loop that detects rotation with nothing moving at all, and the four quartz spheres that measured the curvature of spacetime.
- A gyroscope is a fast-spinning rigid rotor whose large spin angular momentum makes its orientation resist applied torques: drift rate .
- Every application exploits one of two principles: rigidity in space (a torque-isolated rotor holds an inertial direction — attitude reference, INS) or reaction torque from forced precession (rate gyros, CMGs, stabilizers).
- A free gyro holds an inertial direction, not an Earth-fixed one — to an earthbound observer it drifts at up to ; making it useful means either compensating that rate or exploiting it.
- The gyrocompass exploits it: a pendulous rotor constrained near the horizon oscillates about true north with — settling period ≈ 84 min by deliberate Schuler tuning.
- MEMS gyros replace the rotor with a vibrating proof mass read out through the Coriolis acceleration ; optical gyros use the Sagnac phase with no moving parts.
- Grade is set by drift: consumer MEMS wander by degrees per hour, navigation-grade instruments by thousandths, and Gravity Probe B's gyros by less than a milliarcsecond per year.
- Key idea: angular momentum, not the spin axis itself, is what responds to torque: forces to chase the torque, so a perpendicular torque rotates a large spin angular momentum sideways (precession) instead of tipping it over.
Where this lives today
Your phone carries three MEMS gyroscopes that cost about a dollar and drift like drunkards — tens of degrees per hour of bias instability — yet fused with accelerometers, magnetometer, and GPS they stabilize your camera, orient your maps, and let a drone hover in gusting wind with control loops running on equation (12) a thousand times per second. One grade up, tactical FOGs and ring-laser gyros guide airliners between GPS fixes; the hemispherical resonator gyro — a vibrating quartz wineglass exploiting the same Coriolis physics as MEMS, but in a millimetre-perfect resonator — now flies on spacecraft with drift measured in ten-thousandths of a degree per hour and no wear-out mechanism, having replaced spinning rotors almost everywhere. The deep-physics end of the family is the quietest. Gravity Probe B's four gyroscopes — niobium-coated fused-quartz spheres round to forty atoms, electrostatically levitated and spun in vacuum, read out by SQUID magnetometers — orbited Earth from 2004 to 2005 to test whether spacetime itself precesses a gyroscope. General relativity predicted a geodetic drift of 6606 milliarcseconds per year from the curvature of space around Earth and a frame-dragging drift of 39 mas/yr from Earth's rotation dragging spacetime around with it. The mission measured both: and mas/yr. The humble demand behind those error bars — a stray-torque drift below degrees per hour, thirteen orders of magnitude quieter than your phone — is still equation (2), , pushed to its physical limit. Meanwhile large ring-laser gyros anchored in bedrock (the 4-metre ring at Wettzell) now track fluctuations in Earth's own rotation rate at the part-per-billion level — the gyroscope, invented to show the planet turns, has become the instrument that watches it stumble.
The physical picture
Spin a rotor up to speed and mount it in two nested gimbals, so that the frame can turn any way it likes without exerting torque on the rotor axis. Now rotate the frame. The rotor does not care. Its angular momentum is a vector fixed in inertial space, and with no torque path to it, — the axis keeps pointing at the same distant star while the vehicle around it pitches, rolls, and yaws. Read the gimbal angles and you have the vehicle's orientation, mechanically, with no external reference. This is gyroscopic rigidity, and it is nothing but angular momentum conservation dressed up as an instrument.
The complementary principle appears when the rotor is not free. Clamp one gimbal so the vehicle's turn is transmitted to the rotor as a forced precession , and the rotor answers with the reaction torque derived in the Gyroscopic Precession article. Measure that torque (or the spring deflection it causes) and you have a rate gyro — an instrument that outputs how fast the vehicle is turning. Amplify instead of measure and you have a control-moment gyro that steers a spacecraft. Rigidity gives you orientation; reaction gives you rotation rate and torque authority. Everything that follows — gyrocompass, MEMS chip, laser ring — is one of these two ideas wearing different hardware. One subtlety upgrades the whole subject from demo to instrument: a free gyro holds an inertial direction, and we do not live in an inertial frame. Point a perfect gyro at the horizon and walk away: to you it will appear to tilt and drift at up to Earth's rotation rate, , because the ground under it is turning. An "apparent drift" of fifteen degrees per hour is catastrophic for a compass and useless for navigation — until you realize the drift is Earth's rotation, at which point you can compensate it (directional gyro), integrate it away (INS), or harness it to find north (gyrocompass).
The dynamics an instrument builder needs
The master law and its instrument-grade consequences come first. About the rotor's support point,
where: — net external torque; — total angular momentum, dominated for a fast rotor by the spin term . Engineers call the angular momentum capacity; it is the currency in which all gyroscopic performance is priced. A stray torque — bearing friction, mass unbalance, gimbal flexure — does not tip the axis; it precesses it at
where: — the slow wander of the reference axis, the drift rate that defines an instrument's grade. Equation (2) is the fast-top precession law of the Gyroscopic Precession article read as an error budget: to build a better gyro, raise or starve the torque. A consumer MEMS part drifts by tens of degrees per hour; a marine gyrocompass by hundredths; Gravity Probe B, with electrostatically levitated quartz spheres in vacuum, reached below degrees per hour — the same formula spanning thirteen orders of magnitude. Forcing the axis to turn at costs whoever does the forcing a torque, and the rotor pushes back:
where: the reaction is perpendicular to both the turn and the spin — derived and dissected in the Gyroscopic Precession article. Linear in with the enormous gain , equation (3) is why a modest gimbal motor tilting a 100-kg rotor can slew the entire ISS, and why a rate gyro's tiny spring deflection reads vehicle turn rate directly. For anything quantitative about orientation you need the kinematics: the rotor axis direction is tracked by the Euler angles , with the angular velocity decomposing as
where: — the line of nodes; the full construction, body-frame components and all, lives in the Angular Velocity in Terms of Euler Angles article. Feeding (4) into the symmetric-top Lagrangian yields two conserved momenta and the effective potential — the machinery derived in the Heavy Symmetric Top article. Two of its results matter constantly in gyro engineering. First, steady precession under a constant torque exists at two rates,
where: the slow branch in the fast-spin limit is the operating point of every precession-based instrument. Second, any disturbance superposes nutation — a nodding of the axis at frequency and amplitude
where: the scalings say that spinning faster makes the wobble both faster and smaller — for instrument rotors at tens of thousands of rpm, nutation is a kilohertz shiver of microradian size, handled by damping and otherwise ignored (the Nutation article does the full analysis). And with no torque at all, the axis of a slightly-misaligned rotor traces the free precession cones of the Free Symmetric Top article at
where: — the coning rate seen in the rotor frame. In an instrument this free coning is a defect (it smears the reference axis), which is why precision rotors are spun about their axis of maximum moment of inertia and fitted with nutation dampers.
Which formula answers which question
| you want | use | notes |
|---|---|---|
| how good is my gyro | , eq. (2) | grade = drift; raise , starve |
| torque from a forced turn | , eq. (3) | rate gyros, CMGs, stabilizers |
| gyrocompass settling | , eq. (8) | period ; fails at the poles |
| gyrocompass latitude error | , eq. (9) | small tilt equilibrium offset |
| optical rotation sensing | , eq. (11) | area × turns is the gain |
| MEMS rotation sensing | , , eq. (12) | Coriolis readout of a vibrating mass |
| exact top dynamics | eqs. (5)–(7) | derived in the Heavy Symmetric Top and Free Symmetric Top articles |
The gyrocompass — north from the planet's own spin
A free gyro drifts relative to the ground; the gyrocompass turns that bug into its sensing principle. Mount the rotor so its axis stays near the horizontal plane, and make it pendulous — hang a small mass below the rotor case, so that any tilt of the axis above the horizon produces a gravity torque about the horizontal. Now the feedback loop closes by itself. If the spin axis points east of true north by azimuth , Earth's rotation tilts the local horizon under it, so the axis — inertially fixed — appears to rise at a rate proportional to . The rising tilt engages the pendulous torque, and by equation (3) that torque precesses the axis in azimuth, back toward the meridian. Point west of north and the loop runs in reverse. True north is the only azimuth where nothing happens: the axis oscillates about the meridian and, with damping, settles on it.
We derive the equation of motion for the azimuth error of a pendulous gyrocompass and obtain equation (8): simple harmonic oscillation about true north with , plus the latitude-error tilt (9). The model: a rotor of angular momentum capacity , axis constrained near the horizontal plane at latitude , with pendulosity (restoring torque coefficient for tilt). Two small angles track the axis: azimuth east of the meridian and elevation above the horizon. The strategy is to write how Earth's rotation changes apparently, and how the pendulous torque changes by precession, then combine the two first-order equations into one oscillator. Watch the roles: Earth's rotation is the sensor (it converts azimuth error into tilt), the pendulous mass is the actuator (it converts tilt into corrective precession) — neither alone finds north.
Step 1. Earth-rotation kinematics. At latitude the Earth's angular velocity has a horizontal (north) component and a vertical component . An axis held at small azimuth east of north is nearly perpendicular to neither; relative to the local horizon, its far end appears to rise at
Why: the horizon plane continuously rotates about the north-south horizontal axis at ; an axis lying along that rotation axis () is unaffected, while a misaligned axis picks up apparent tilt in proportion to its misalignment — this is how the compass senses without any external reference.
Step 2. Pendulous response. A tilt hangs the pendulous mass off-vertical, producing a torque about the horizontal axis perpendicular to the rotor axis. By the precession law (1) this torque swings the rotor axis in azimuth at
Why the sign: the torque direction is such that an axis tilted up (east of north) precesses westward, back toward the meridian — trace it with and the right-hand rule. The term is the vertical Earth rate, which uniformly rotates all horizontal directions and will only shift the equilibrium.
Step 3. Combine. Differentiate the equation and substitute Step 1:
giving simple harmonic motion of the azimuth about true north,
where: — the north-seeking oscillation frequency; period . Why real compasses settle rather than oscillate forever: a deliberate damping torque (typically by restricting the pendulous fluid or offsetting the damping weight) is added, decaying the oscillation onto the meridian in a couple of periods.
Step 4. Equilibrium tilt. Setting in Step 2 shows the settled axis is not exactly horizontal but carries a constant tilt
where: — the small "latitude error" tilt whose pendulous torque precesses the axis just fast enough to track the meridian as Earth turns; it grows toward the poles and must be corrected in the readout. Verified: dimensions of (8) are ; the loop fails at the poles where () — gyrocompasses are unusable in polar latitudes, as ship navigators know. Numbers in Worked example 2: , at give min and . The 84-minute value is the deliberate Schuler tuning used at design latitude.
The choice of an 84-minute period is not an accident of my example numbers — it is the Schuler period, , the period of a pendulum as long as Earth's radius. An instrument tuned to it has a magic immunity: when the ship accelerates, the apparent gravity tilts, but a Schuler-tuned loop responds by tracking the accelerating vehicle's actual local vertical rather than being fooled — accelerations do not excite a north error. Every inertial navigation system carries the same 84-minute oscillation in its error dynamics for the same reason.
Solid state — sensing rotation with nothing but vibration and light
The spinning rotor has two solid-state successors, and both descend from equations you already own. The MEMS vibrating-structure gyroscope is a Coriolis machine. A silicon proof mass is driven to oscillate along with amplitude at frequency , giving velocity amplitude . Rotate the chip about at , and in the chip's rotating frame the mass feels the Coriolis acceleration studied in the Coriolis Force article:
where: — peak Coriolis acceleration along the perpendicular sense axis ; — the resulting sense-mode amplitude when the sense resonance is matched to the drive and amplified by its quality factor ; capacitive fingers convert to a signal proportional to . The numbers are humbling: for at , ; a rotation of gives and a bare (unamplified) sense deflection of picometres — smaller than an atom. Only resonant gain ( brings it to nanometres) and femtofarad capacitance readout make the phone-scale gyro possible. Two masses driven in antiphase and read differentially cancel linear vibration — the tuning-fork architecture:
The optical gyroscope removes even the vibration. Send two light beams around the same closed loop in opposite directions and rotate the loop at : the co-rotating beam chases a receding beamsplitter while the counter-rotating beam meets an advancing one, so they complete the circuit in different times.
Go deeper · Derivation B · 2 minThe Sagnac effect — rotation sensed by counter-propagating light
We derive the Sagnac time difference , equation (10), and convert it to the interferometer phase (11) that fiber-optic and ring-laser gyros read out. The setting: a circular loop of radius rotating at about its axis, with light injected in both directions at a beamsplitter fixed to the loop. The strategy is direct special-relativity-flavored kinematics in the lab frame — compute each beam's transit time to the moving beamsplitter and subtract; the loop's area emerges naturally, and the result in fact holds for a loop of any shape. Watch the orders: we keep terms to first order in , which is enormous compared to any measurable rotation and makes the linearization exact for practical purposes.
Step 1. Transit times to a moving finish line. In the lab frame the beamsplitter rides the rim at speed . The co-rotating beam must cover the circumference plus the arc the splitter advances; the counter-rotating beam covers the circumference minus it:
Why the denominators: in the lab frame both beams travel at (light does not inherit the loop's speed); only the finish line moves, lengthening one race and shortening the other.
Step 2. Subtract and expand to first order in :
where: — the loop's enclosed area. Why area is the right variable: repeating the computation for an arbitrary planar loop replaces by the enclosed area exactly; the Sagnac effect couples to the flux of through the circuit, a geometric statement that survives in general relativity.
Step 3. Convert to optical phase. A time offset between two beams of wavelength (frequency ) is a phase ; winding the fiber into turns multiplies the enclosed area:
where: — number of fiber turns; — vacuum wavelength. Why fiber changed the game: is free gain — a kilometre of fiber on a palm-sized spool encloses twenty square metres of effective area with no moving parts, no bearings, and hence no drift at all. *Verified: dimensions check ( is dimensionless); the ring-laser variant converts into a beat frequency with the perimeter. Worked example 1 evaluates (11) for Earth's rotation: for a 1-km, 8-cm coil — matches the standard FOG scale factor per deg/h.*
Limiting cases
| Case | Result | Meaning |
|---|---|---|
| fast-rotor limit disturbance impulses | drift tiny | gyroscopic rigidity; the axis is a usable inertial reference |
| torque-free (perfectly gimballed) | const; axis fixed in inertial space | ideal attitude gyro; residual coning per eq. (7) if spin and axis misalign |
| gyrocompass at the equator | : maximal | strongest north-seeking; shortest settling |
| gyrocompass at the poles | : | no horizontal Earth-rate to sense — gyrocompasses fail in polar seas |
| slow rotor | large nutation, two branches merge | instrument regime lost; see the Heavy Symmetric Top article |
| zero rotation, MEMS/optical | , | both outputs null honestly — no spin-down error, but bias stability sets the floor |
Worked examples
1 · A fiber-optic gyro reads the planet (confidence builder)
A fiber-optic gyroscope uses of fiber wound on a coil of diameter , operating at . Its axis is aligned with Earth's rotation axis. What Sagnac phase does Earth's rotation produce, and what is the scale factor in phase per degree-per-hour?
Step 1. Coil geometry: area per turn ; number of turns .
Step 2. Earth's rate: ().
Step 3. Sagnac phase from equation (11): .
Step 4. Scale factor: dividing by gives . Navigation-grade FOGs resolve phases of nanoradians, so Earth's rotation is a large signal for them — a stationary FOG gyrocompasses by measuring the direction-dependence of exactly this phase, something no consumer MEMS part can dream of.
2 · Designing a marine gyrocompass (exam level)
A marine gyrocompass rotor has spinning at rpm, and pendulosity giving a restoring torque coefficient per radian of tilt. At latitude : (a) find the north-seeking period; (b) the settled latitude-error tilt; (c) the drift rate a stray bearing torque of would cause if the same rotor were used as a free directional gyro.
Step 1. Angular momentum capacity: , so .
Step 2. North-seeking frequency from equation (8): .
Step 3. Period: — the Schuler period, by design: the pendulosity was chosen so that ship accelerations cannot masquerade as north error. With damping, the compass settles on the meridian in two to three of these periods, which is why a ship's gyrocompass is started hours before departure.
Step 4. Latitude-error tilt from equation (9): — a small, latitude-dependent tilt the readout must subtract.
Step 5. Free-gyro drift from equation (2): . A micronewton-metre of bearing friction — a fingerprint's worth — already costs of heading per day. This single number explains a century of air bearings, magnetic suspensions, and finally the flight from mechanical rotors to optical loops with no bearings at all.
Origins · 1 minArnold Sommerfeld and how this was discovered
Sommerfeld is remembered as the great teacher of quantum theory — mentor to Heisenberg, Pauli, Debye, and Bethe, nominated for the Nobel Prize a record 84 times without winning — but his first monument was mechanical. With Felix Klein he wrote the four-volume Über die Theorie des Kreisels (1897–1910), the most complete treatise on spinning bodies ever produced. What sets it apart is the fourth volume: after three volumes of rigorous top theory, Klein and Sommerfeld turned to the technical applications — the gyrocompass then being patented by Anschütz-Kaempfe, ship stabilizers, the gyroscopic effects on rifled shells and bicycle wheels — treating engineering hardware with the same mathematical seriousness as celestial mechanics. Sommerfeld consulted directly on Anschütz's gyrocompass development in Kiel; the settling-dynamics analysis in this article descends from that work. His career embodies this chapter's arc: the same serving toys, navies, and — through his students — the spinning electron itself.
Going further
References. Morin, Introduction to Classical Mechanics, ch. 9 (Angular Momentum, Part II) · Goldstein, Poole & Safko, Classical Mechanics, 3rd ed., ch. 5 · Landau & Lifshitz, Mechanics, 3rd ed., §35–37 · Taylor, Classical Mechanics, ch. 10
Provenance. Equations and limits follow Goldstein (Classical Mechanics, ch. 5), Landau–Lifshitz (Mechanics §35–37), Morin (ch. 9), and Taylor (ch. 10). Verifier should confirm: the steady-precession quadratic and its two roots; the fast-top limit; the effective-potential reduction with conserved ; the sleeping-top stability threshold ; and the torque-free precession rates. No empirical constants are quoted beyond standard . Additional results on this page: the gyrocompass dynamics and latitude error (Wrigley/Anschütz standard theory; cf. Klein–Sommerfeld vol. IV); the Sagnac results , ; MEMS Coriolis readout . Worked numbers recomputed from these formulas: FOG 1 km/8 cm/1550 nm → at Earth rate ( per deg/h); gyrocompass , , → min, ; free-gyro drift ; Earth rate ; GP-B values 6606/39 mas/yr predicted, / measured (Everitt et al. 2011).
Builds on: Angular Momentum of a Rigid Body · Principal Axes and Principal Moments of Inertia · Euler Angles · Euler's Equations of Motion · Classification of Rigid Bodies: Spherical, Symmetric, and Asymmetric Tops. Leads to: Angular Velocity in Terms of Euler Angles · Rotational Kinetic Energy · Inertia Ellipsoid.
Is there actually a tiny spinning wheel inside my phone?
No — nothing in a phone gyro spins. The MEMS chip contains micrometre-scale silicon proof masses driven to vibrate at tens of kilohertz. When the phone rotates at , each moving mass feels the Coriolis acceleration perpendicular to its velocity, deflecting it by picometres; matched resonance and capacitive combs read that deflection out as a rate signal. It is the same Coriolis force that steers hurricanes, exploited at the micron scale. The spinning-rotor gyros survive where performance or robustness demands them — but even there the trend is to vibrating structures (quartz hemispheres) and to light (fiber loops), neither of which stores any angular momentum at all.
If my phone has a gyroscope, why can't it find true north like a ship's gyrocompass?
Because gyrocompassing means detecting Earth's rotation, , and a consumer MEMS gyro's bias instability — the slow wander of its zero point — is typically tens of degrees per hour. The signal is buried an order of magnitude or more below the sensor's own lies, and no averaging fixes a bias that drifts. That is why phones fall back on the magnetometer (magnetic north, with all its declination and interference problems). Navigation-grade FOGs and HRGs, with bias stability near , gyrocompass routinely: hold the instrument still, measure the rate vector, and its horizontal component points at true north. The dividing line between "toy" and "navigator" is exactly whether Earth's rotation is visible above the noise.
Why does a gyrocompass stop working near the poles?
The north-seeking torque loop runs on the horizontal component of Earth's rotation, — that is what converts an azimuth error into a growing tilt (Step 1 of the derivation). Approaching the poles, : the settling frequency collapses, the period stretches toward infinity, and the latitude-error tilt stays bounded, so it is the vanishing restoring torque — not a diverging tilt — that ends the compass at the pole. At the pole itself every horizontal direction is "south," and the instrument has nothing to seek. Polar navigation historically switched to directional gyros steered by grid headings and star fixes; today it means inertial systems and GPS, both indifferent to latitude.
What is special about the 84-minute period that keeps appearing?
It is the Schuler period, minutes — the period of a pendulum whose length is Earth's radius, equivalently of a satellite orbiting at zero altitude. Its magic: a platform or feedback loop tuned to this period tracks the local vertical exactly even when the vehicle accelerates, because the loop's response to acceleration reproduces precisely the rotation of the true vertical as the vehicle moves over the curved Earth. An accelerating ship cannot fool a Schuler-tuned gyrocompass into mistaking acceleration for tilt, and every inertial navigation system's errors oscillate at the Schuler period rather than growing secularly from velocity errors. It is the deepest of the navigation coincidences — set by the planet, not the hardware.
What actually happened with gimbal lock on Apollo?
Apollo's inertial platform hung its gyro-stabilized stable member in three nested gimbals. When two gimbal axes align — which happens at a specific vehicle attitude — the assembly loses a degree of freedom: no combination of gimbal rates can accommodate rotation about the missing axis, and the platform gets dragged, corrupting the reference alignment. A fourth gimbal removes the singularity, but at real cost in mass, complexity, and readout accuracy; NASA chose three and accepted a forbidden attitude cone, with the DSKY flashing a warning as the spacecraft approached it. Mike Collins joked about wanting a fourth gimbal for Christmas. Modern systems dodge the issue entirely: strapdown INS bolts the sensors to the vehicle and maintains orientation as a quaternion in software — quaternions, unlike Euler-angle gimbals, have no singular configuration, as the Euler Angles article explains.
When would you choose a ring-laser or fiber-optic gyro over MEMS, or vice versa?
By the drift budget and the environment. MEMS wins on cost, size, and power (dollars, millimetres, milliwatts) wherever degrees-per-hour bias is tolerable and something else — GPS, cameras, magnetometers — periodically corrects the accumulated error: phones, drones, car stability control. Optical gyros win where the sensor must be trusted unaided for hours: RLGs and FOGs have no proof mass and no bearings, so they are immune to acceleration-induced bias and to wear, deliver down to , and dominate airliners, submarines, and launch vehicles. The hemispherical resonator gyro sits in between mechanically but at the top in longevity — a vibrating quartz shell with nothing to wear out, which is why deep-space missions carry it. All three obey the same logic: eliminate the torque path of equation (2), whether by having no rotor (optical) or no contact (HRG in vacuum).
What did Gravity Probe B actually measure, and why did it need gyroscopes specifically?
General relativity predicts that a gyroscope orbiting a massive rotating body precesses even with zero mechanical torque — spacetime itself is curved (geodetic effect) and dragged around by the body's rotation (frame dragging). A gyroscope is the only instrument that can feel this: its spin axis is a pure direction-memory, so any drift not accounted for by mechanical torque is a message about the geometry it moves through. GP-B flew four fused-quartz spheres — round to about 40 atomic layers — electrostatically suspended, spun to 4000 rpm, and tracked by SQUIDs against a guide star. Prediction: 6606 mas/yr geodetic, 39 mas/yr frame dragging. Result: and . To make relativity readable, every classical drift term in had to be crushed below degrees per hour — the most perfect gyroscopes ever constructed, doing the oldest job in this chapter: pointing.