🚀 Acceleration Conversion Calculator

Convert between m/s², g-force, ft/s², Gal (galileo), km/h·s, mph/s, mGal, in/s² and 20+ units — with kinematics, SUVAT equations, centripetal, SHM, angular, Coriolis & gravitational acceleration formulas in MathJax

20+ Units SI · CGS · Imperial · Geophysical m/s² ↔ g · ft/s² · Gal Free & Instant

🔄 Acceleration Unit Converter

1 m/s² = 0.101972 g
Formula: value × 0.101972

🌍 All Units at Once

💡 Definition: Acceleration = rate of change of velocity: \( \mathbf{a} = \dfrac{d\mathbf{v}}{dt} \) — SI unit is m/s². All units convert through m/s² as the base. Standard gravity: \( g_n = 9.80665\,\text{m/s}^2 \) (exact).

📖 How to Use This Acceleration Conversion Calculator

  1. 1
    Filter by Unit Category (Optional)

    Click SI/Metric (m/s², km/s², cm/s²), Imperial/US (ft/s², in/s², mi/s²), Geophysical (Gal, mGal, cGal), or Practical (g-force, km/h·s, mph/s) to narrow the dropdowns. "All Units" shows all 22 units together.

  2. 2
    Enter Your Acceleration Value

    Type the value into "Enter Value." Accepts any numeric input — from milligals (geophysics gravity surveys) to km/s² (rocket propulsion). Scientific notation auto-applies for extreme values.

  3. 3
    Select From and To Units

    Choose source in "From Unit" and target in "To Unit." The result and exact conversion factor appear instantly in the teal result box below.

  4. 4
    Use Quick-Convert Buttons

    Click preset buttons — m/s²↔g, m/s²↔ft/s², m/s²→Gal, km/h·s→m/s², g→ft/s² — for the most common acceleration conversions. Both dropdowns update automatically.

  5. 5
    View All Units & Copy

    "All Units at Once" shows your acceleration in every supported unit simultaneously. Click "📋 Copy Result" to copy the primary conversion for engineering reports, physics coursework, or automotive testing.

📐 Acceleration Unit Conversion Factors

UnitSymbolIn m/s²MathTypical Use
Metre/s²m/s²1 (base)\(1\,\text{m/s}^2\)SI standard, all physics
Standard gravityg / gₙ9.80665\(g_n = 9.80665\,\text{m/s}^2\)Aerospace, automotive G-loads
Foot/s²ft/s²0.3048\(0.3048\,\text{m/s}^2\)US/Imperial engineering
Inch/s²in/s²0.0254\(0.0254\,\text{m/s}^2\)Precision mechanics
km/h per secondkm/h·s0.277778\(1000/3600\,\text{m/s}^2\)Vehicle performance specs
mph per secondmph/s0.44704\(0.44704\,\text{m/s}^2\)US automotive testing
Gal (galileo)Gal0.01\(10^{-2}\,\text{m/s}^2\)Geophysics, gravimetry
MilligalmGal1×10⁻⁵\(10^{-5}\,\text{m/s}^2\)Precision gravity surveys
Kilometre/s²km/s²1,000\(10^3\,\text{m/s}^2\)Rocket propulsion
cm/s²cm/s²0.01\(10^{-2}\,\text{m/s}^2\)CGS system (= 1 Gal)

🚀 Understanding Acceleration — A Complete Physics & Engineering Guide

Acceleration is one of the three fundamental kinematic quantities — alongside position and velocity — that completely describe the motion of any object. While velocity tells you how fast something is moving and in what direction, acceleration tells you how quickly that velocity is changing. A car speeding up, a ball thrown upward and decelerating under gravity, a spacecraft firing its rockets, a seismometer detecting ground tremors, or a fighter pilot pulling out of a dive all experience acceleration — just at vastly different magnitudes and in many different unit systems.

Accurately converting between acceleration units is critical in automotive engineering (0–60 mph performance), aerospace (G-load tolerance), geophysics (gravity surveys in milligals), physics education (SUVAT kinematics), and structural engineering (earthquake response spectra). This guide covers every acceleration unit, every key formula, and practical worked examples across all these domains.

Acceleration — Kinematic Definition
\[ \mathbf{a} = \frac{d\mathbf{v}}{dt} = \frac{d^2\mathbf{x}}{dt^2} \qquad a_{\text{avg}} = \frac{\Delta v}{\Delta t} = \frac{v_f - v_i}{t_f - t_i} \]
\(\mathbf{a}\) = acceleration vector (m/s²)  ·  \(\mathbf{v}\) = velocity vector (m/s)  ·  \(\mathbf{x}\) = position vector (m)  ·  \(t\) = time (s)  ·  SI unit: metre per second squared (m/s²)  ·  Acceleration is a vector — it has magnitude and direction

🌍 Standard Gravity & G-Force — The Most Important Acceleration Reference

Standard gravity (\(g_n\)) is the defined acceleration due to gravity at Earth's surface, adopted by the CGPM (General Conference on Weights and Measures) as the exact value \(9.80665\,\text{m/s}^2\). This is used as the reference point for g-force — the ratio of an acceleration to standard gravity — and is the foundation of force unit conversions between SI (N) and gravitational (kgf, lbf) systems.

In engineering and physiology, g-force (G) is far more intuitive than m/s² for expressing human experience. "You feel 3 G" is immediately meaningful; "you experience 29.4 m/s²" is not. G-force is standard in aerospace, automotive crash testing, roller coaster design, military aviation, and sports medicine.

G-Force — Definition & Conversion

\( g_n = 9.80665\,\text{m/s}^2 \quad \text{(exact, defined by CGPM 1901)} \)

\( G = \frac{a}{g_n} \qquad a\,[\text{m/s}^2] = G \times 9.80665 \)

\( g_n = 9.80665\,\text{m/s}^2 = 32.17405\,\text{ft/s}^2 = 980.665\,\text{Gal} = 980665\,\text{mGal} \)

\( 1\,G \approx 0\text{–}1G: \text{normal human activity} \quad 3\text{–}9G: \text{fighter pilot manoeuvres} \quad {>}16G: \text{usually fatal} \)

Actual gravity varies: \(g = 9.7639\,\text{m/s}^2\) (equator, 4,000 m) to \(g = 9.8337\,\text{m/s}^2\) (poles, sea level). Standard gravity \(g_n\) is a fixed defined constant used for unit conversion — not a measurement of actual local gravity.
📌 Worked Example — Fighter Pilot G-Load Conversion

Problem: An F-16 pilot pulling a hard turn experiences 7.5 G. Express this in m/s², ft/s², and km/h·s.

m/s²: \( 7.5 \times 9.80665 = \mathbf{73.55\,\text{m/s}^2} \)

ft/s²: \( 73.55 \div 0.3048 = \mathbf{241.3\,\text{ft/s}^2} \)

km/h·s: \( 73.55 \div 0.27778 = \mathbf{264.8\,\text{km/h·s}} \) (velocity increases by 264.8 km/h every second)

Context: Human G-force tolerance: ~1 G sustained comfortable, ~4–6 G with anti-G suit sustainable, ~9 G brief maximum with training. At 7.5 G without protective equipment, blood pools in the legs, causing unconsciousness (G-LOC) within 3–5 seconds.

📐 SUVAT Equations — Kinematics of Constant Acceleration

When acceleration is constant (uniform), five kinematic quantities are linked by the SUVAT equations: displacement (s), initial velocity (u), final velocity (v), acceleration (a), and time (t). These equations are the backbone of classical mechanics — used in everything from projectile calculations to vehicle braking distance to orbital mechanics.

SUVAT Equations — Constant Acceleration

\( v = u + at \qquad \text{(velocity after time } t) \)

\( s = ut + \tfrac{1}{2}at^2 \qquad \text{(displacement in time } t) \)

\( v^2 = u^2 + 2as \qquad \text{(velocity at displacement } s) \)

\( s = \tfrac{1}{2}(u + v)t \qquad \text{(displacement from average velocity)} \)

\( s = vt - \tfrac{1}{2}at^2 \qquad \text{(displacement using final velocity)} \)

\(s\) = displacement (m)  ·  \(u\) = initial velocity (m/s)  ·  \(v\) = final velocity (m/s)  ·  \(a\) = acceleration (m/s²)  ·  \(t\) = time (s)  ·  Valid for constant acceleration only  ·  Free fall: \(u = 0\), \(a = g_n = 9.80665\,\text{m/s}^2\)
📌 Worked Example — Car 0 to 100 km/h Acceleration

Problem: A Tesla Model S accelerates from 0 to 100 km/h (27.78 m/s) in 2.1 seconds. Find the average acceleration in m/s², g-force, ft/s², and mph/s.

Step 1: \( a = \frac{v - u}{t} = \frac{27.78 - 0}{2.1} = \mathbf{13.23\,\text{m/s}^2} \)

G-force: \( G = 13.23 / 9.80665 = \mathbf{1.35\,G} \)

ft/s²: \( 13.23 / 0.3048 = \mathbf{43.4\,\text{ft/s}^2} \)

mph/s: \( 13.23 / 0.44704 = \mathbf{29.6\,\text{mph/s}} \)

Distance travelled: \( s = \frac{1}{2} \times 13.23 \times 2.1^2 = \mathbf{29.2\,\text{m}} \) — less than 30 metres to reach 100 km/h.

⭕ Centripetal Acceleration — Circular Motion

Any object moving in a circle at constant speed is continuously accelerating — not because its speed changes, but because its direction changes continuously. This is centripetal acceleration, always directed toward the centre of the circular path. It is why a car turning a corner needs grip from the road (the centripetal force), and why satellites in orbit are in continuous free-fall toward Earth.

Centripetal Acceleration

\( a_c = \frac{v^2}{r} = \omega^2 r = \frac{4\pi^2 r}{T^2} \)

\( F_c = m a_c = \frac{mv^2}{r} \qquad \text{(centripetal force, always inward)} \)

\( v = \omega r \qquad \omega = \frac{2\pi}{T} = 2\pi f \)

\(a_c\) = centripetal acceleration (m/s²)  ·  \(v\) = tangential speed (m/s)  ·  \(r\) = radius (m)  ·  \(\omega\) = angular velocity (rad/s)  ·  \(T\) = period (s)  ·  \(f\) = frequency (Hz)  ·  Centripetal acceleration points toward centre — centrifugal acceleration is equal in magnitude but outward (non-inertial frame only)
📌 Worked Example — Car Cornering Acceleration

Problem: A car rounds a motorway on-ramp at 60 km/h (16.67 m/s) with radius 50 m. Find centripetal acceleration in m/s² and G.

\[ a_c = \frac{v^2}{r} = \frac{16.67^2}{50} = \frac{277.9}{50} = \mathbf{5.56\,\text{m/s}^2} \]

G-force: \( 5.56 / 9.80665 = \mathbf{0.567\,G} \)

Context: A typical road tyre can sustain ~0.85 G lateral. At 0.567 G the car is within limits. If the driver increases speed to 80 km/h on the same corner: \(a_c = 22.22^2/50 = 9.88\,\text{m/s}^2 = 1.01\,G\) — beyond typical tyre limits, leading to a slide.

🌊 Acceleration in Simple Harmonic Motion (SHM)

Simple Harmonic Motion — Acceleration

\( a = -\omega^2 x \qquad \text{(SHM restoring acceleration)} \)

\( |a_{\max}| = \omega^2 A \qquad \text{(maximum at extreme displacement, } x = \pm A) \)

\( x(t) = A\cos(\omega t + \phi) \qquad v(t) = -A\omega\sin(\omega t + \phi) \qquad a(t) = -A\omega^2\cos(\omega t + \phi) \)

\( \omega = 2\pi f = \frac{2\pi}{T} \qquad T_{\text{pendulum}} = 2\pi\sqrt{\frac{L}{g}} \qquad T_{\text{spring}} = 2\pi\sqrt{\frac{m}{k}} \)

\(a\) = instantaneous acceleration (m/s²)  ·  \(x\) = displacement from equilibrium (m)  ·  \(A\) = amplitude (m)  ·  \(\omega\) = angular frequency (rad/s)  ·  \(T\) = period (s)  ·  Acceleration is max at endpoints (zero velocity) and zero at equilibrium (max velocity)

🌐 The Gal (Galileo) — Geophysics & Gravity Surveys

The gal (symbol Gal, also called the galileo in honour of Galileo Galilei) is a CGS unit of acceleration equal to exactly 1 cm/s² = 0.01 m/s². It was adopted by geophysicists and geodesists specifically because Earth's gravitational field varies by only a few parts per million from place to place — values that are cumbersome to express in m/s² or g-units. The gal, and especially the milligal (mGal = 0.001 Gal = 10⁻⁵ m/s²), are the operational units of modern gravimetry.

Gal — Geophysics Unit

\( 1\,\text{Gal} = 1\,\text{cm/s}^2 = 0.01\,\text{m/s}^2 = 10^{-2}\,\text{m/s}^2 \)

\( 1\,\text{mGal} = 10^{-3}\,\text{Gal} = 10^{-5}\,\text{m/s}^2 \)

\( g_n = 9.80665\,\text{m/s}^2 = 980.665\,\text{Gal} = 980{,}665\,\text{mGal} \)

\( \Delta g_{\text{typical variation}} \approx 100\text{–}500\,\text{mGal} \quad \text{(equator to pole)} \)

Modern superconducting gravimeters resolve sub-microgal (µGal = 10⁻⁸ m/s²) changes — used to detect groundwater, oil reservoirs, magma movements, and post-glacial rebound. Earthquake seismology uses cm/s² (Gal) in peak ground acceleration (PGA) safety ratings for structures.
🌍 Seismic engineering: Building codes specify earthquake resistance by peak ground acceleration (PGA) in units of g-force or Gal (cm/s²). Japan's seismic intensity scale uses Gal; the Modified Mercalli scale correlates qualitatively with G-force. A PGA of 980 Gal = 1 g = 9.80665 m/s² represents maximum expected ground acceleration in the most severe earthquakes (Richter 8+). Most modern building codes design for 0.1–0.4 g in seismic zones.

🔄 Angular Acceleration — Rotational Kinematics

Angular Acceleration & Conversion to Linear

\( \alpha = \frac{d\omega}{dt} \qquad \text{(angular acceleration, rad/s}^2\text{)} \)

\( a_{\text{tangential}} = \alpha \times r \qquad \text{(linear acceleration at radius } r) \)

\( a_{\text{total}} = \sqrt{a_t^2 + a_c^2} = \sqrt{(\alpha r)^2 + (\omega^2 r)^2} = r\sqrt{\alpha^2 + \omega^4} \)

\( \omega = \omega_0 + \alpha t \qquad \theta = \omega_0 t + \tfrac{1}{2}\alpha t^2 \qquad \omega^2 = \omega_0^2 + 2\alpha\theta \)

\(\alpha\) = angular acceleration (rad/s²)  ·  \(\omega\) = angular velocity (rad/s)  ·  \(\theta\) = angular displacement (rad)  ·  \(r\) = radius (m)  ·  Rotational SUVAT equations mirror linear SUVAT: replace \(s\to\theta\), \(u\to\omega_0\), \(v\to\omega\), \(a\to\alpha\)

🏎️ Vehicle Acceleration — km/h·s, mph/s & Real-World Performance

In automotive engineering and consumer performance reporting, acceleration is expressed in two practical units that relate directly to how drivers experience it:

  • km/h per second (km/h·s): How many km/h of speed the vehicle gains each second. 1 km/h·s = 1000/3600 m/s² = 0.27778 m/s².
  • miles per hour per second (mph/s): The US equivalent. 1 mph/s = 0.44704 m/s². A 0–60 mph car test covering 60 mph / time_in_seconds gives the average acceleration in mph/s.
Practical Vehicle Acceleration Conversions

\( 1\,\text{km/h·s} = \frac{1000}{3600}\,\text{m/s}^2 = 0.27\overline{7}\,\text{m/s}^2 \)

\( 1\,\text{mph/s} = 0.44704\,\text{m/s}^2 \quad \text{(exact: 1609.344 m/mile ÷ 3600)} \)

\( a_{\text{avg}} = \frac{\Delta v}{t} \qquad \text{0–100 km/h in 4 s:} \quad a = \frac{100\,\text{km/h·s}}{4} = 25\,\text{km/h·s} = 6.944\,\text{m/s}^2 = 0.708\,G \)

\( s_{0-60} = \frac{v^2}{2a} = \frac{(26.82)^2}{2 \times 4.47} = \frac{719.3}{8.94} = 80.5\,\text{m} \quad \text{(0–60 mph in 6 s)} \)

Standard gravity \(g_n = 9.80665\,\text{m/s}^2 = 35.30\,\text{km/h·s} = 21.936\,\text{mph/s}\) — a car accelerating at 1 G gains 35.3 km/h each second.

🌍 Real-World Acceleration Reference Table

Object / Eventm/s²G-ForceNotes
🐌 Slow elevator start0.5–10.05–0.10 GBarely perceptible
🚗 Average car braking4–80.4–0.8 GFriction-limited by tyre
⬇️ Earth free fall (sea level)9.806651.000 GStandard gravity —exact definition
🚗 Tesla Model 3 0–100 km/h~9.5~0.97 G3.1 s (Performance variant)
✈️ Commercial airline takeoff2–40.2–0.4 GPassenger-comfort limited
🏎️ Formula 1 braking40–604–6 GCarbon-ceramic brakes + downforce
🎢 Roller coaster peak29–593–6 GBrief, 0.3–1 s
✈️ F-16 hard turn~73~7.5 GAnti-G suit required
🚀 Space Shuttle launch~29~3 GMax at main engine cutoff
💥 Car crash airbag trigger200–100020–100 G~1 ms duration
🔫 Bullet in gun barrel~500,000~50,000 GVery brief; ~1 ms

📦 Acceleration Unit System Guide

📐

m/s² — SI Standard

The SI unit. 1 m/s² = the acceleration that changes velocity by 1 m/s each second. Universal in physics, engineering, and all scientific computing. \(g_n = 9.80665\,\text{m/s}^2\) sets the scale for G-loads.

g-force (G) — Aerospace & Human Tolerance

\(1\,G = g_n = 9.80665\,\text{m/s}^2\). The intuitive unit for human experience and aerospace. Sustained: 0–1 G normal, 4–6 G trained pilots, 9+ G extreme brief. Converts: G × 9.80665 = m/s².

🌍

Gal & mGal — Geophysics

\(1\,\text{Gal} = 0.01\,\text{m/s}^2\). \(1\,\text{mGal} = 10^{-5}\,\text{m/s}^2\). Geophysics, gravimetry, seismology. Earth's gravity range: 978–983 Gal. Gravity surveys detect oil/water at µGal precision.

🏎️

km/h·s & mph/s — Automotive

\(1\,\text{km/h·s} = 0.2778\,\text{m/s}^2\). \(1\,\text{mph/s} = 0.4470\,\text{m/s}^2\). Used in vehicle performance specs — 0 to 100 km/h, 0 to 60 mph tests. Directly links time and velocity gain.

N
Written & Reviewed by Num8ers Editorial Team — Classical Mechanics, Aerospace Engineering, Geophysics & Automotive Performance Specialists Last updated: April 2026 · Conversion factors verified against NIST SP 811 (2008), BIPM SI Brochure 9th edition (2019), CGPM Resolution 3 (1901) for standard gravity, and ISO 80000-3 (2019) for kinematic quantities.

❓ Frequently Asked Questions — Acceleration Conversion

How do I convert m/s² to g-force (G)?
Divide by 9.80665. \(G = a / g_n = a / 9.80665\). Example: 19.613 m/s² ÷ 9.80665 = 2.000 G. Reverse (G to m/s²): multiply by 9.80665. Example: 3.5 G × 9.80665 = 34.32 m/s². Standard gravity is \(g_n = 9.80665\,\text{m/s}^2\) exactly — a defined constant, not a measurement.
How do I convert m/s² to ft/s²?
Multiply by 3.28084 (= 1/0.3048). \(1\,\text{m/s}^2 = 3.28084\,\text{ft/s}^2\). Example: 9.80665 m/s² × 3.28084 = 32.174 ft/s² (standard gravity in ft/s²). Reverse (ft/s² to m/s²): multiply by 0.3048. The conversion factor is exact: 1 ft = 0.3048 m, so 1 ft/s² = 0.3048 m/s².
What is standard gravity (gₙ) and why is it defined?
\(g_n = 9.80665\,\text{m/s}^2\) exactly — a defined constant. Adopted by the CGPM in 1901. Actual gravity varies from 9.764 m/s² (at the equator at high altitude) to 9.834 m/s² (at the poles at sea level) due to Earth's rotation and shape. Standard gravity is a fixed reference for unit conversion (kgf = kg × 9.80665), not a measurement of local gravity. For precise geophysical work, local gravity is measured by gravimeters.
How do I convert km/h·s to m/s²?
Multiply by 0.27778 (= 1/3.6). \(1\,\text{km/h·s} = 1000/3600\,\text{m/s}^2 = 0.27\overline{7}\,\text{m/s}^2\). Example: A car accelerating at 25 km/h·s (gains 25 km/h per second) = 25 × 0.27778 = 6.944 m/s² = 0.708 G. Reverse (m/s² to km/h·s): multiply by 3.6.
What is a Gal (galileo) and when is it used?
1 Gal = 1 cm/s² = 0.01 m/s². Named for Galileo Galilei. Used in geophysics and gravimetry because Earth's gravity varies by only ~0.5% across the surface — variations measured in milligals (mGal = 10⁻⁵ m/s²). Standard gravity = 980.665 Gal. Modern superconducting gravimeters resolve microgal (µGal = 10⁻⁸ m/s²) changes for detecting oil reservoirs, groundwater, and tectonic movements.
What is centripetal acceleration and how is it calculated?
\(a_c = v^2/r = \omega^2 r\). Centripetal acceleration is the acceleration of an object in circular motion, always directed toward the centre. Even at constant speed, circular motion involves acceleration because direction changes continuously. Example: car at 60 km/h (16.67 m/s) on 50 m radius corner: \(a_c = 16.67^2/50 = 5.56\,\text{m/s}^2 = 0.567\,G\). Centrifugal acceleration (outward) only exists in non-inertial (rotating) reference frames.
What are the SUVAT equations and when do they apply?
SUVAT equations apply only to constant (uniform) acceleration. The five variables: s (displacement), u (initial velocity), v (final velocity), a (acceleration), t (time). Five equations connect any three: \(v = u + at\), \(s = ut + \frac{1}{2}at^2\), \(v^2 = u^2 + 2as\), \(s = \frac{1}{2}(u+v)t\), \(s = vt - \frac{1}{2}at^2\). Free fall, uniform braking, and horizontal projectile components all qualify.
What is angular acceleration and how does it convert to linear?
Angular acceleration: \(\alpha = d\omega/dt\), unit = rad/s². Linear (tangential) acceleration: \(a_t = \alpha \times r\) where r is the radius. Rotational SUVAT equations mirror linear: replace displacement with angle, linear velocity with angular velocity, linear acceleration with angular acceleration. A motor spinning up from 0 to 100 rad/s in 2s has \(\alpha = 50\,\text{rad/s}^2\); a point at 0.1 m radius has \(a_t = 50 \times 0.1 = 5\,\text{m/s}^2\).
What is acceleration in simple harmonic motion (SHM)?
\(a = -\omega^2 x\) — always proportional to displacement, opposite in direction. Maximum at extreme positions (\(|a_{max}| = \omega^2 A\)), zero at equilibrium. A pendulum of length 1 m has \(\omega = \sqrt{g/L} = \sqrt{9.807/1} = 3.13\,\text{rad/s}\), period T = 2.007 s. At amplitude 0.1 m: \(|a_{max}| = 3.13^2 \times 0.1 = 0.979\,\text{m/s}^2 = 0.100\,G\).
What is Coriolis acceleration and why does it matter?
\(\mathbf{a}_{Cor} = 2\boldsymbol{\omega} \times \mathbf{v}\) — a fictitious acceleration in rotating reference frames (like Earth). Magnitude = \(2\omega v \sin\lambda\) where λ is latitude. On Earth (\(\omega = 7.27 \times 10^{-5}\,\text{rad/s}\)), a 100 m/s aeroplane at mid-latitude experiences ~0.01 m/s² Coriolis acceleration — deflects right in the northern hemisphere, left in the southern. Drives hurricane rotation, ocean gyres, and affects long-range ballistic trajectories.
What is peak ground acceleration (PGA) in earthquake engineering?
PGA is the maximum ground acceleration during an earthquake, expressed in g-force or Gal (cm/s²). Building codes specify seismic design by PGA zone — e.g., 0.1 g (low seismicity), 0.3 g (moderate), 0.6–1.0 g (high). Japan measures seismic intensity in cm/s² (Gal). A PGA of 980 Gal = 1 g represents the most severe recorded ground motions (e.g., 2011 Tōhoku earthquake measured ~2,700 Gal = 2.76 g in some locations).
How accurate is the Num8ers Acceleration Conversion Calculator?
Uses exact or high-precision factors per NIST SP 811 and ISO 80000-3: standard gravity \(g_n = 9.80665\,\text{m/s}^2\) (exact, CGPM 1901); 1 ft = 0.3048 m (exact, 1959 agreement); 1 Gal = 0.01 m/s² (exact CGS); 1 km/h·s = 1000/3600 m/s² (exact). JavaScript double precision provides ~15 significant digits. Results are mathematically exact within floating-point arithmetic.

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