Moho Depth Estimator Calculator
Estimate the depth of the Mohorovicic discontinuity using seismic refraction data. Calculate crustal thickness from P-wave arrival times, velocities.
Moho Depth Estimator Calculator
Calculator
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Formula: H = ti * Vm * Vc / (2 * sqrt(Vm^2 - Vc^2))
Worked example โ Estimated Moho Depth: ~35 km | Critical Angle: 49.95 deg
Formula
H = ti * Vm * Vc / (2 * sqrt(Vm^2 - Vc^2))
Where H is the Moho depth, ti is the time intercept (Pn arrival time minus distance/mantle velocity), Vm is the upper mantle P-wave velocity, and Vc is the average crustal P-wave velocity. This is derived from the seismic refraction time-intercept method.
Worked Examples
Example 1: Continental Crust Moho Depth
Problem:A seismic station 150 km from an earthquake records the direct Pg arrival at 24.2 s and the refracted Pn arrival at 25.8 s. Upper crust velocity is 6.2 km/s and mantle velocity is 8.1 km/s.
Solution:Time difference = 25.8 - 24.2 = 1.6 s (Pg still leads, so the profile is inside the crossover) Time intercept = tPn - (distance/Vm) = 25.8 - (150/8.1) = 25.8 - 18.52 = 7.28 s Critical angle = arcsin(6.2/8.1) = 49.95 degrees Moho depth H = ti * Vm * Vc / (2 * sqrt(Vm^2 - Vc^2)) H = ti * 8.1 * 6.2 / (2 * sqrt(65.61 - 38.44)) H = 7.28 * 50.22 / (2 * 5.214) = 7.28 * 4.817 = 35.1 km
Result:Estimated Moho Depth: ~35 km | Critical Angle: 49.95 deg
Example 2: Thin Oceanic Crust Estimation
Problem:An ocean bottom seismometer 40 km from a controlled source records Pg at 5.88 s and Pn at 6.09 s. Oceanic crust velocity is 6.8 km/s and mantle velocity is 8.0 km/s.
Solution:Time difference = 6.09 - 5.88 = 0.21 s Time intercept = 6.09 - (40/8.0) = 6.09 - 5.00 = 1.09 s Critical angle = arcsin(6.8/8.0) = 58.21 degrees Moho depth calculation uses the same refraction formula H = ti * 8.0 * 6.8 / (2 * sqrt(64 - 46.24)) H = 1.09 * 54.4 / (2 * 4.214) = 1.09 * 6.454 = 7.0 km
Result:Estimated Moho Depth: ~7 km | Critical Angle: 58.21 deg
Frequently Asked Questions
What is the Mohorovicic discontinuity and why is its depth important?
The Mohorovicic discontinuity, commonly called the Moho, is the boundary between the Earth's crust and the underlying mantle. It was discovered in 1909 by Croatian seismologist Andrija Mohorovicic when he noticed that seismic waves from earthquakes showed a sudden increase in velocity at a certain depth, indicating a change in rock composition. The Moho depth is critically important for understanding crustal structure, tectonic processes, and isostatic equilibrium. Continental Moho typically lies at 30 to 50 km depth, while oceanic Moho is much shallower at 5 to 10 km. Knowing the Moho depth helps geologists assess mineral potential and earthquake hazards.
How do seismic refraction surveys estimate Moho depth?
Seismic refraction surveys estimate Moho depth by analyzing the travel times of compressional P-waves that travel along different paths through the crust and upper mantle. Direct P-waves (Pg) travel through the crust, while refracted P-waves (Pn) travel down to the Moho, along the crust-mantle boundary at mantle velocity, and back up to the surface. At sufficient distance from the source, Pn waves arrive before Pg waves because they travel faster along the Moho despite covering a longer path. The time-intercept or crossover distance method uses these arrival time differences along with known crustal and mantle velocities to calculate the depth to the Moho boundary.
What are typical P-wave velocities in the crust and upper mantle?
P-wave velocities increase with depth and density. In sedimentary layers near the surface, velocities range from 2 to 4 km/s depending on rock type and consolidation. Upper crustal crystalline rocks typically have velocities of 5.8 to 6.4 km/s, with granite averaging around 6.0 km/s and granodiorite around 6.2 km/s. Lower crustal rocks have higher velocities of 6.5 to 7.2 km/s due to increased pressure and more mafic composition. Just below the Moho, upper mantle peridotite has velocities of 7.8 to 8.2 km/s, with 8.1 km/s being a commonly used global average for Pn velocity calculations in refraction seismology.
How does crustal thickness vary across different tectonic settings?
Crustal thickness varies dramatically depending on the tectonic environment. Oceanic crust is relatively thin and uniform at 5 to 10 km, created at mid-ocean ridges through basaltic volcanism. Normal continental crust averages 30 to 40 km in thickness. Mountain belts formed by continental collision have thickened crust reaching 50 to 70 km, with the Himalayan-Tibetan plateau having the thickest crust on Earth at up to 80 km. Rift zones and extensionally thinned regions may have crustal thicknesses of only 20 to 25 km. Volcanic arcs above subduction zones typically have crust 25 to 45 km thick, while continental margins transition from thick continental to thin oceanic crust.
What other methods besides seismic refraction can estimate Moho depth?
Several geophysical methods complement seismic refraction for Moho depth estimation. Receiver function analysis uses teleseismic earthquakes recorded at broadband stations to detect the P-to-S wave conversion at the Moho, providing depth estimates beneath individual stations. Deep seismic reflection profiling uses controlled sources and multichannel recording to image the Moho as a reflective boundary. Gravity surveys exploit the density contrast between crust and mantle to model crustal thickness variations over large areas. Surface wave tomography analyzes seismic wave dispersion to map crustal thickness across continents. Each method has advantages and limitations regarding resolution, coverage, and cost.
What is the time intercept and how does it relate to the crossover distance?
The time intercept is where the straight Pn travel-time line, extrapolated back to zero source-receiver offset, meets the time axis. It equals twice the Moho depth times the square root of the difference of the squared velocities, divided by the product of the velocities, which is what Moho Depth Estimator Calculator inverts for depth. The crossover distance is the offset at which Pn first arrives ahead of Pg, and the two are linked: crossover equals twice the depth times the square root of the sum of the velocities divided by their difference. For a 35 kilometre Moho with 6.2 and 8.1 kilometres per second, that ratio is about 2.74, so crossover falls near 190 kilometres.
Why does the head wave only exist beyond the critical angle?
Snell's law fixes the refraction angle at the crust-mantle boundary. As the incidence angle increases, the refracted ray bends further from the vertical, and at the critical angle, the arcsine of the crustal velocity divided by the mantle velocity, the refracted ray travels horizontally along the interface. With 6.2 and 8.1 kilometres per second that angle is about 50 degrees. Only at or beyond it does the wave propagate along the Moho at mantle velocity while continuously leaking energy back into the crust as the Pn head wave. At smaller angles the energy transmits into the mantle and never returns, which is why refraction surveys need long offsets.
Why must a refraction profile be shot in both directions when the Moho dips?
The single-shot geometry assumed here treats the crust-mantle boundary as horizontal. If the Moho dips, the apparent Pn velocity measured shooting downdip is lower than the true mantle velocity and the updip apparent velocity is higher, so a one-way profile returns a biased depth and a mantle velocity that is not real. Reversed shooting, recording the same line from both ends, separates the two effects: for small dips the true velocity is close to the harmonic mean of the two apparent velocities, and the dip angle follows from their difference. Unreversed profiles across a tilted Moho can be wrong by several kilometres.
How is average crustal density inferred from the crustal P-wave velocity?
Moho Depth Estimator Calculator applies a linear velocity-density relation of the Birch type, adding 0.32 times the crustal velocity in kilometres per second to a constant of 0.77 to give density in grams per cubic centimetre. At 6.2 kilometres per second that returns about 2.75, consistent with granodioritic upper crust. Such relations hold reasonably well for crystalline silicate rocks of similar mean atomic weight, and the Nafe-Drake curve covers the strongly non-linear low-velocity sediments where they fail. The density estimate matters because it converts Moho depth into the pressure at the crust-mantle boundary and lets refraction results be compared against gravity models.
How much does an error in picking the Pn arrival shift the estimated depth?
Depth scales linearly with the time intercept, and for crustal and mantle velocities of 6.2 and 8.1 kilometres per second the multiplier is about 4.8 kilometres per second of intercept. A tenth of a second of picking error therefore moves the Moho by roughly half a kilometre. Because the intercept is the Pn arrival minus distance over mantle velocity, the same sensitivity applies to any error in the assumed mantle velocity or in the source origin time, which for earthquake sources is itself an inversion result. Emergent Pn onsets in noisy records are the usual practical limit on precision.
References
Background & Theory
History
Reviewed for accuracy by Daniel Agrici, Founder & Lead Developer ยท Editorial policy
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