This guide explains why gps would fail without einstein in plain language, with the exact figures and how to work them out yourself.
- Today
- Saturday, 31 October 2026 · ISO week 44 · day 304 of the year
Computed on every visit from the time-zone database and standard astronomical formulas, so these never go stale. The article below is unchanged.
How Satellite Navigation Depends on Nanosecond Timing
Every GPS position fix is secretly a time measurement. Satellites orbiting approximately 20,200 kilometres overhead broadcast their precise spatial coordinates and the timestamp of transmission from onboard atomic clocks. Your smartphone receives these signals, measures the precise time delay between transmission and arrival, and multiplies that delay by the speed of light—which covers roughly 30 centimetres per nanosecond (0.29979 metres per nanosecond)—to determine its distance from each satellite.
Because a receiver in a phone does not contain its own atomic clock, it cannot know the exact instant a signal arrived relative to satellite time using a single satellite feed. To solve for four unknown variables—latitude ($x$), longitude ($y$), altitude ($z$), and receiver clock bias ($t$)—the phone must intersect distance measurements from at least four distinct satellites simultaneously. Positioning accuracy down to a few metres therefore demands timing accuracy down to a few nanoseconds. If satellite clocks drift by even a microsecond, the resulting distance error stretches to 300 metres.
The Relativistic Conflict: Speed vs. Gravity
At nanosecond precision, Albert Einstein’s theories of relativity are not abstract theoretical concepts; they are daily engineering specifications. Two distinct relativistic effects act on GPS satellite clocks at the same time, pulling their rates in opposite directions:

- Special Relativity (Velocity Effect): Einstein’s 1905 Special Theory of Relativity dictates that a clock moving relative to a stationary observer runs slower than a clock at rest. GPS satellites orbit the Earth at approximately 14,000 kilometres per hour (3.87 kilometres per second). Relative to a receiver on the stationary ground, this orbital velocity causes satellite atomic clocks to lose approximately 7 microseconds per day.
- General Relativity (Gravitational Effect): Einstein’s 1915 General Theory of Relativity shows that gravity warps time: clocks deeper within a gravitational well tick slower than clocks situated higher up where gravity is weaker. Because GPS satellites orbit at an altitude of 20,200 km (giving an orbital radius of roughly 26,600 km from Earth’s center, compared to Earth’s surface radius of ~6,378 km), they experience significantly weaker gravitational pull than ground stations. This reduced gravity causes the satellite clocks to run faster by approximately 45 microseconds per day.
Because these two relativistic phenomena operate simultaneously, their net effect is cumulative. Subtracting the 7 microseconds lost to orbital velocity from the 45 microseconds gained due to higher gravitational potential leaves a net gain: satellite clocks run approximately 38 microseconds per day fast relative to clocks on Earth’s surface.
Worked Calculation: The Daily Drift Rate
To understand how rapidly an uncorrected system degrades, consider the direct multiplication of time error by the velocity of light ($c = 299,792,458 text{ m/s}$):
$$text{Distance Error} = text{Time Offset} times text{Speed of Light}$$
$$text{Distance Error} = 38 times 10^{-6} text{ seconds} times 299,792,458 text{ metres/second} approx 11,392 text{ metres}$$
Without compensation, satellite clocks gain roughly 38 microseconds every 24 hours, accumulating more than 11.3 kilometres (7 miles) of positioning error per day. Within just one hour of operation, the positioning drift exceeds 470 metres—rendering car navigation, aviation guidance, and maritime routing completely useless before lunch.
| Relativistic Effect | Physical Cause | Underlying Physics | Clock Impact (μs/day) | Position Impact if Uncorrected |
|---|---|---|---|---|
| Time Dilation | Orbital speed (~14,000 km/h) | Special Relativity | -7.2 μs / day | Lags ~2.16 km / day |
| Gravitational Redshift | Weak gravity at 20,200 km | General Relativity | +45.8 μs / day | Advances ~13.73 km / day |
| Net Combined Effect | Combined orbit dynamics | General + Special Relativity | +38.6 μs / day | Drifts ~11.5 km / day |
How Engineers Solved Relativity in System Design
To keep satellite navigation synchronized across Earth, system architects employ a two-part correction strategy combining hardware factory tuning with real-time algorithmic adjustments.

1. Pre-Launch Frequency Tuning (Hardware Offset)
Rather than adjusting clock output continuously in orbit, satellite atomic clocks (rubidium and cesium standards) are intentionally calibrated before launch to run slow on Earth. The standard fundamental reference frequency for GPS ground operations is 10.23 MHz. Before being placed atop a rocket, satellite clock synthesizers are set to tick at 10.22999999543 MHz.
Once the satellite reaches its target orbit at 20,200 km, gravitational frequency shifting speeds the clock back up by exact theoretical proportions, bringing its output in orbit into synchronization with ground-based 10.23 MHz clocks.
2. Orbital Eccentricity and Sagnac Corrections (Software Adjustments)
No orbit is perfectly circular. Because GPS orbits are slightly elliptical (eccentricity $e neq 0$), satellite altitude and velocity fluctuate continuously throughout each 12-hour orbit. When a satellite comes closer to Earth at perigee, it speeds up (increasing Special Relativistic slowing) and enters stronger gravity (reducing General Relativistic speeding). At apogee, the reverse occurs.
Ground control stations constantly track these elliptical orbital shifts and transmit update parameters in the navigation message. Your phone’s receiver uses an explicit mathematical formula to compute a dynamic relativistic correction factor for every signal frame it processes:
$$Delta t_r = F cdot e cdot sqrt{a} cdot sin(E)$$
where $F$ is a physical constant, $e$ is orbital eccentricity, $a$ is the semi-major axis, and $E$ is eccentric anomaly. In addition, receivers compensate for the Sagnac Effect—the rotational movement of the observer on Earth’s surface during the signal’s transit time from orbit.
Beyond Navigation: GPS as Global Timekeeping Infrastructure
The satellites carry these hardware and algorithmic corrections so reliably that GPS has evolved into global critical infrastructure for time distribution as much as positioning. Because atomic clocks in space broadcast synchronized time signals around the clock, industries across the world rely on GPS for precise microsecond and nanosecond timing:
- Electrical Power Grids: Synchrophasors across transmission lines monitor high-voltage phase angles using GPS timestamps precise to within 1 microsecond, preventing cascading blackout failures across continental networks.
- Financial Exchanges: Institutional trading networks enforce microsecond-level order matching mandated by financial regulations (such as MiFID II in Europe and CAT rules in the US), anchoring every transaction log to traceable satellite timing feeds.
- Cellular Networks: 5G telecommunication base stations use GPS time signals to coordinate frame handoffs and time-division duplexing (TDD) protocols, maintaining channel spacing without interference.
The synchronized result—atomic time, relativity included—is what ultimately feeds the live clocks at itsdately.com.
Comparing Relativistic Parameters Across Satellite Constellations
GPS is no longer the sole constellation in medium Earth orbit. Modern receivers concurrently process signals from Europe’s Galileo, Russia’s GLONASS, and China’s BeiDou constellations. Because each system operates at distinct orbital altitudes and inclinations, their clocks experience slightly different relativistic offsets.

| Constellation | Country/Region | Orbital Altitude | Orbital Velocity | Net Relativistic Clock Offset |
|---|---|---|---|---|
| GPS | United States | 20,200 km | ~3.87 km/s | +38.6 μs / day |
| Galileo | European Union | 23,222 km | ~3.67 km/s | +40.8 μs / day |
| GLONASS | Russia | 19,100 km | ~3.95 km/s | +37.2 μs / day |
| BeiDou (MEO) | China | 21,528 km | ~3.78 km/s | +39.8 μs / day |
Where Standard GPS Relativity Models Do Not Apply
Understanding relativistic time shifts requires evaluating the specific environment of the vehicle or receiver. The +38.6 microsecond/day figure applies specifically to Medium Earth Orbit (MEO) navigation constellations. In other operational contexts, the balance of relativity shifts significantly:
1. Low Earth Orbit (LEO) Satellites
Satellites orbiting in Low Earth Orbit—such as the International Space Station (~400 km altitude) or broadband constellations like Starlink (~550 km altitude)—travel at much higher velocities (~7.7 km/s) while sitting much deeper in Earth’s gravitational well. For LEO spacecraft, Special Relativity’s kinetic slowing effect dominates over General Relativity’s gravitational speeding effect. As a result, clocks on LEO spacecraft run slower than terrestrial clocks (losing roughly 25 microseconds per day on the ISS), the exact opposite of GPS satellites.
2. GPS-Denied and Indoor Environments
In locations where satellite signals cannot penetrate—such as subterranean tunnels, deep underwater mines, or heavily jammed electronic warfare zones—satellite-based timing fails entirely. To maintain synchronization without satellite connectivity, defense systems and critical data centers employ local Chip-Scale Atomic Clocks (CSAC). These micro-atomic clocks draw under 125 milliwatts of power while maintaining sub-microsecond time integrity across days without space assistance.
Frequently asked questions
Why don’t phone receivers need internal atomic clocks?
Phone receivers avoid the need for heavy, expensive atomic clocks by solving for time mathematically. By taking distance measurements from four satellites instead of three, the receiver treats its internal clock error as a fourth unknown variable alongside latitude, longitude, and altitude, recalculating local clock offset on every fix.
What happens to relativistic effects for satellites in Low Earth Orbit (LEO)?
In Low Earth Orbit (such as the ISS at ~400 km), satellites travel much faster (~7.7 km/s) and sit closer to Earth’s mass. For LEO orbits, velocity time dilation dominates over gravitational redshift, causing onboard clocks to run slower than ground clocks by roughly 25 microseconds per day.
How does orbital eccentricity alter relativistic calculations?
GPS orbits are slightly elliptical rather than perfectly circular. As a satellite moves closer to Earth (perigee) and further away (apogee), its speed and gravitational potential continuously fluctuate. Satellite navigation messages broadcast Keplerian correction parameters that allow smartphone receivers to compute real-time microsecond adjustments for these elliptical variations.
Where do these relativistic calculation formulas come from?
The time dilation figures are computed directly from Einstein’s field equations and Lorentz transformations using published astronomical values: Earth’s gravitational constant ($GM = 3.986 times 10^{14} text{ m}^3/text{s}^2$), mean Earth radius ($6,378 text{ km}$), speed of light ($299,792,458 text{ m/s}$), and semi-major orbital axis values ($26,560 text{ km}$).
Related on itsdately: How Atomic Clocks Work: The Machines That Define the Second · NTP: How Your Phone Knows the Exact Time · What Is a Leap Second — and Why It’s Being Retired
Further reading: GPS.gov — official U.S. GPS information.
