Acceleration Converter

Acceleration — From Zero to Light Speed

Master acceleration units across automotive, aviation, space, and physics. From g-forces to planetary gravities, convert with confidence and understand what the numbers mean.

Why Pilots Black Out at 9g: Understanding the Forces That Move Us
This converter handles 40+ acceleration units from standard gravity (1g = 9.80665 m/s² exactly) to automotive performance (0-60 mph times), aviation g-forces (fighter jets pull 9g), geophysics precision (microgal for oil prospecting), and extreme physics (LHC protons at 190 million g). Acceleration measures how fast velocity changes—speeding up, slowing down, or changing direction. The key insight: F = ma means doubling force or halving mass doubles acceleration. G-forces are dimensionless ratios to Earth's gravity—at 5g sustained, your blood struggles to reach your brain and vision tunnels. Remember: free fall isn't zero acceleration (it's 1g downward), you just feel weightless because net g-force is zero!

Foundations of Acceleration

Acceleration
Rate of velocity change over time. SI unit: meter per second squared (m/s²). Formula: a = Δv/Δt

Newton's Second Law

F = ma connects force, mass, and acceleration. Double the force, double the acceleration. Halve the mass, double the acceleration.

  • 1 N = 1 kg·m/s²
  • More force → more acceleration
  • Less mass → more acceleration
  • Vector quantity: has direction

Velocity vs Acceleration

Velocity is speed with direction. Acceleration is how fast velocity changes — speeding up, slowing down, or changing direction.

  • Positive: speeding up
  • Negative: slowing down (deceleration)
  • Turning car: accelerating (direction changes)
  • Constant speed ≠ zero acceleration if turning

G-Force Explained

G-force measures acceleration as multiples of Earth's gravity. 1g = 9.81 m/s². Fighter pilots feel 9g, astronauts 3-4g at launch.

  • 1g = standing on Earth
  • 0g = free fall / orbit
  • Negative g = upward acceleration (blood to head)
  • Sustained 5g+ requires training
Quick Takeaways
  • 1g = 9.80665 m/s² (standard gravity - exact)
  • Acceleration is change in velocity over time (Δv/Δt)
  • Direction matters: turning at constant speed = acceleration
  • G-forces are dimensionless multiples of standard gravity

Unit Systems Explained

SI/Metric & CGS

International standard using m/s² as base with decimal scaling. CGS system uses Gal for geophysics.

  • m/s² — SI base unit, universal
  • km/h/s — automotive (0-100 km/h times)
  • Gal (cm/s²) — geophysics, earthquakes
  • milligal — gravity prospecting, tidal effects

Imperial/US System

US customary units still used in American automotive and aviation alongside metric standards.

  • ft/s² — engineering standard
  • mph/s — drag racing, car specs
  • in/s² — small-scale acceleration
  • mi/h² — rarely used (highway studies)

Gravitational Units

Aviation, aerospace, and medical contexts express acceleration as g-multiples for intuitive understanding of human tolerance.

  • g-force — dimensionless ratio to Earth gravity
  • Standard gravity — 9.80665 m/s² (exact)
  • Milligravity — microgravity research
  • Planetary g — Mars 0.38g, Jupiter 2.53g

The Physics of Acceleration

Kinematics Equations

Core equations relate acceleration, velocity, distance, and time under constant acceleration.

v = v₀ + at | s = v₀t + ½at² | v² = v₀² + 2as
  • v₀ = initial velocity
  • v = final velocity
  • a = acceleration
  • t = time
  • s = distance

Centripetal Acceleration

Objects moving in circles accelerate toward center even at constant speed. Formula: a = v²/r

  • Earth orbit: ~0.006 m/s² toward Sun
  • Car turning: lateral g-force felt
  • Roller coaster loop: up to 6g
  • Satellites: constant centripetal acceleration

Relativistic Effects

Near light speed, acceleration becomes complex. Particle accelerators achieve 10²⁰ g instantaneously at collision.

  • LHC protons: 190 million g
  • Time dilation affects perceived acceleration
  • Mass increases with velocity
  • Light speed: unreachable limit

Gravity Across the Solar System

Surface gravity varies dramatically across celestial bodies. Here's how Earth's 1g compares to other worlds:

Celestial BodySurface GravityFacts
Sun274 m/s² (28g)Would crush any spacecraft
Jupiter24.79 m/s² (2.53g)Largest planet, no solid surface
Neptune11.15 m/s² (1.14g)Ice giant, similar to Earth
Saturn10.44 m/s² (1.06g)Low density despite size
Earth9.81 m/s² (1g)Our reference standard
Venus8.87 m/s² (0.90g)Near-twin to Earth
Uranus8.87 m/s² (0.90g)Same as Venus
Mars3.71 m/s² (0.38g)Easier to launch from
Mercury3.7 m/s² (0.38g)Slightly less than Mars
Moon1.62 m/s² (0.17g)Apollo astronaut jumps
Pluto0.62 m/s² (0.06g)Dwarf planet, very low

G-Force Effects on Humans

Understanding what different g-forces feel like and their physiological effects:

ScenarioG-ForceHuman Effect
Standing still1gNormal Earth gravity
Elevator start/stop1.2gBarely noticeable
Car braking hard1.5gPushed against seatbelt
Roller coaster3-6gHeavy pressure, thrilling
Fighter jet turn9gVision tunneling, possible blackout
F1 car braking5-6gHelmet feels 30kg heavier
Rocket launch3-4gChest compression, hard to breathe
Parachute opening3-5gBrief jolt
Crash test20-60gSerious injury threshold
Ejection seat12-14gSpinal compression risk

Real-World Applications

Automotive Performance

Acceleration defines car performance. 0-60 mph time translates directly to average acceleration.

  • Sports car: 0-60 in 3s = 8.9 m/s² ≈ 0.91g
  • Economy car: 0-60 in 10s = 2.7 m/s²
  • Tesla Plaid: 1.99s = 13.4 m/s² ≈ 1.37g
  • Braking: -1.2g max (street), -6g (F1)

Aviation & Aerospace

Aircraft design limits based on g-tolerance. Pilots train for high-g maneuvers.

  • Commercial jet: ±2.5g limit
  • Fighter jet: +9g / -3g capability
  • Space Shuttle: 3g launch, 1.7g re-entry
  • Eject at 14g (pilot survival limit)

Geophysics & Medical

Tiny acceleration changes reveal underground structures. Centrifuges separate substances using extreme acceleration.

  • Gravity survey: ±50 microgal precision
  • Earthquake: 0.1-1g typical, 2g+ extreme
  • Blood centrifuge: 1,000-5,000g
  • Ultracentrifuge: up to 1,000,000g

Acceleration Benchmarks

ContextAccelerationNotes
Snail0.00001 m/s²Extremely slow
Human walking start0.5 m/s²Gentle acceleration
City bus1.5 m/s²Comfortable transport
Standard gravity (1g)9.81 m/s²Earth surface
Sports car 0-60mph10 m/s²1g acceleration
Drag racing launch40 m/s²4g wheelie territory
F-35 catapult launch50 m/s²5g in 2 seconds
Artillery shell100,000 m/s²10,000g
Bullet in barrel500,000 m/s²50,000g
Electron in CRT10¹⁵ m/s²Relativistic

Quick Conversion Math

g to m/s²

Multiply g-value by 10 for quick estimate (exact: 9.81)

  • 3g ≈ 30 m/s² (exact: 29.43)
  • 0.5g ≈ 5 m/s²
  • Fighter at 9g = 88 m/s²

0-60 mph to m/s²

Divide 26.8 by seconds to 60mph

  • 3 seconds → 26.8/3 = 8.9 m/s²
  • 5 seconds → 5.4 m/s²
  • 10 seconds → 2.7 m/s²

mph/s ↔ m/s²

Divide by 2.237 to convert mph/s to m/s²

  • 1 mph/s = 0.447 m/s²
  • 10 mph/s = 4.47 m/s²
  • 20 mph/s = 8.94 m/s² ≈ 0.91g

km/h/s to m/s²

Divide by 3.6 (same as speed conversion)

  • 36 km/h/s = 10 m/s²
  • 100 km/h/s = 27.8 m/s²
  • Quick: divide by ~4

Gal ↔ m/s²

1 Gal = 0.01 m/s² (centimeters to meters)

  • 100 Gal = 1 m/s²
  • 1000 Gal ≈ 1g
  • 1 milligal = 0.00001 m/s²

Planetary Quick Refs

Mars ≈ 0.4g, Moon ≈ 0.17g, Jupiter ≈ 2.5g

  • Mars: 3.7 m/s²
  • Moon: 1.6 m/s²
  • Jupiter: 25 m/s²
  • Venus ≈ Earth ≈ 0.9g

How Conversions Work

Base-unit method
Convert any unit to m/s² first, then from m/s² to target. Quick checks: 1g ≈ 10 m/s²; mph/s ÷ 2.237 → m/s²; Gal × 0.01 → m/s².
  • Step 1: Convert source → m/s² using toBase factor
  • Step 2: Convert m/s² → target using target's toBase factor
  • Alternative: Use direct factor if available (g → ft/s²: multiply by 32.17)
  • Sanity check: 1g ≈ 10 m/s², fighter jet 9g ≈ 88 m/s²
  • For automotive: 0-60 mph in 3s ≈ 8.9 m/s² ≈ 0.91g

Common Conversion Reference

FromToMultiply ByExample
gm/s²9.806653g × 9.81 = 29.4 m/s²
m/s²g0.1019720 m/s² × 0.102 = 2.04g
m/s²ft/s²3.2808410 m/s² × 3.28 = 32.8 ft/s²
ft/s²m/s²0.304832.2 ft/s² × 0.305 = 9.81 m/s²
mph/sm/s²0.4470410 mph/s × 0.447 = 4.47 m/s²
km/h/sm/s²0.27778100 km/h/s × 0.278 = 27.8 m/s²
Galm/s²0.01500 Gal × 0.01 = 5 m/s²
milligalm/s²0.000011000 mGal × 0.00001 = 0.01 m/s²

Quick Examples

3g → m/s²≈ 29.4 m/s²
10 mph/s → m/s²≈ 4.47 m/s²
100 km/h/s → m/s²≈ 27.8 m/s²
500 Gal → m/s²= 5 m/s²
9.81 m/s² → g= 1g
32.2 ft/s² → g≈ 1g

Worked Problems

Sports Car 0-60

Tesla Plaid: 0-60 mph in 1.99s. What's the acceleration?

60 mph = 26.82 m/s. a = Δv/Δt = 26.82/1.99 = 13.5 m/s² = 1.37g

Fighter Jet & Seismology

F-16 pulling 9g in ft/s²? Earthquake at 250 Gal in m/s²?

Jet: 9 × 9.81 = 88.3 m/s² = 290 ft/s². Earthquake: 250 × 0.01 = 2.5 m/s²

Moon Jump Height

Jump with 3 m/s velocity on Moon (1.62 m/s²). How high?

v² = v₀² - 2as → 0 = 9 - 2(1.62)h → h = 9/3.24 = 2.78m (~9 ft)

Common Mistakes to Avoid

  • **Gal vs g confusion**: 1 Gal = 0.01 m/s², but 1g = 9.81 m/s² (nearly 1000× difference)
  • **Deceleration sign**: Slowing down is negative acceleration, not a different quantity
  • **g-force vs gravity**: G-force is acceleration ratio; planetary gravity is actual acceleration
  • **Velocity ≠ acceleration**: High speed doesn't mean high acceleration (cruise missile: fast, low a)
  • **Direction matters**: Turning at constant speed = acceleration (centripetal)
  • **Time units**: mph/s vs mph/h² (3600× different!)
  • **Peak vs sustained**: Peak 9g for 1s ≠ sustained 9g (latter causes blackout)
  • **Free fall isn't zero acceleration**: Free fall = 9.81 m/s² acceleration, zero g-force felt

Fascinating Acceleration Facts

Flea Power

A flea accelerates at 100g when jumping — faster than a space shuttle launch. Their legs act like springs, releasing energy in milliseconds.

Mantis Shrimp Punch

Accelerates its club at 10,000g, creating cavitation bubbles that collapse with light and heat. Aquarium glass doesn't stand a chance.

Head Impact Tolerance

Human brain can survive 100g for 10ms, but only 50g for 50ms. American football hits: 60-100g regularly. Helmets spread impact time.

Electron Acceleration

Large Hadron Collider accelerates protons to 99.9999991% light speed. They experience 190 million g, circling the 27km ring 11,000 times per second.

Gravity Anomalies

Earth's gravity varies by ±0.5% due to altitude, latitude, and underground density. Hudson Bay has 0.005% less gravity due to ice age rebound.

Rocket Sled Record

US Air Force sled hit 1,017g deceleration in 0.65s using water brakes. Test dummy survived (barely). Human limit: ~45g with proper restraints.

Space Jump

Felix Baumgartner's 2012 jump from 39km hit 1.25 Mach in free fall. Acceleration peaked at 3.6g, deceleration at parachute opening: 8g.

Smallest Measurable

Atomic gravimeters detect 10⁻¹⁰ m/s² (0.01 microgal). Can measure height changes of 1cm or underground caves from surface.

The Evolution of Acceleration Science

From Galileo's ramps to particle colliders approaching light speed, our understanding of acceleration evolved from philosophical debate to precise measurement across 84 orders of magnitude. The quest to measure 'how fast things speed up' drove automotive engineering, aviation safety, space exploration, and fundamental physics.

1590 - 1687

Galileo & Newton: Founding Principles

Aristotle claimed heavier objects fall faster. Galileo proved him wrong by rolling bronze balls down inclined planes (1590s). By diluting gravity's effect, Galileo could time acceleration with water clocks, discovering that all objects accelerate equally regardless of mass.

Newton's Principia (1687) unified the concept: F = ma. Force causes acceleration inversely proportional to mass. This single equation explained falling apples, orbiting moons, and cannon trajectories. Acceleration became the link between force and motion.

  • 1590: Galileo's inclined plane experiments measure constant acceleration
  • 1638: Galileo publishes Two New Sciences, formalizing kinematics
  • 1687: Newton's F = ma connects force, mass, and acceleration
  • Established g ≈ 9.8 m/s² through pendulum experiments

1800s - 1954

Precision Gravity: From Pendulums to Standard g

19th-century scientists used reversible pendulums to measure local gravity to 0.01% precision, revealing Earth's shape and density variations. The Gal unit (1 cm/s², named for Galileo) was formalized in 1901 for geophysical surveys.

In 1954, the international community adopted 9.80665 m/s² as standard gravity (1g)—chosen as sea level at 45° latitude. This value became the reference for aviation limits, g-force calculations, and engineering standards worldwide.

  • 1817: Kater's reversible pendulum achieves ±0.01% gravity precision
  • 1901: Gal unit (cm/s²) standardized for geophysics
  • 1940s: LaCoste gravimeter enables 0.01 milligal field surveys
  • 1954: ISO adopts 9.80665 m/s² as standard gravity (1g)

1940s - 1960s

Human G-Force Limits: Aviation & Space Age

WWII fighter pilots experienced blackouts during tight turns—blood pooled away from the brain under sustained 5-7g. Post-war, Col. John Stapp rode rocket sleds to test human tolerance, surviving 46.2g in 1954 (deceleration from 632 mph to zero in 1.4 seconds).

The Space Race (1960s) required understanding sustained high-g. Yuri Gagarin (1961) endured 8g launch and 10g re-entry. Apollo astronauts faced 4g. These experiments established: humans tolerate 5g indefinitely, 9g briefly (with g-suits), but 15g+ risks injury.

  • 1946-1958: John Stapp rocket sled tests (46.2g survival)
  • 1954: Ejection seat standards set at 12-14g for 0.1 seconds
  • 1961: Gagarin's flight proves human space travel viable (8-10g)
  • 1960s: Anti-g suits developed allowing 9g fighter maneuvers

1980s - Present

Extreme Acceleration: Particles & Precision

The Large Hadron Collider (2009) accelerates protons to 99.9999991% light speed, achieving 1.9×10²⁰ m/s² (190 million g) in circular acceleration. At these speeds, relativistic effects dominate—mass increases, time dilates, and acceleration becomes asymptotic.

Meanwhile, atomic interferometer gravimeters (2000s+) detect 10 nanogal (10⁻¹¹ m/s²)—so sensitive they measure 1cm height changes or underground water flow. Applications range from oil prospecting to earthquake prediction and volcano monitoring.

  • 2000s: Atomic gravimeters achieve 10 nanogal sensitivity
  • 2009: LHC begins operation (protons at 190 million g)
  • 2012: Gravity mapping satellites measure Earth's field to microgal precision
  • 2020s: Quantum sensors detect gravitational waves via tiny accelerations
  • **Round 9.81 to 10** for mental math — close enough for estimates, 2% error
  • **0-60 time to g**: Divide 27 by seconds (3s = 9 m/s² ≈ 0.9g, 6s = 4.5 m/s²)
  • **Check direction**: Acceleration vector shows which way change happens, not motion direction
  • **Compare to 1g**: Always relate to Earth gravity for intuition (2g = twice your weight)
  • **Use consistent time units**: Don't mix seconds and hours in same calculation
  • **Geophysics uses milligal**: Oil prospecting needs ±10 mgal precision, water table ±50 mgal
  • **Peak vs average**: 0-60 time gives average; peak acceleration much higher at launch
  • **G-suits help**: Pilots withstand 9g with suits; 5g unassisted causes vision issues
  • **Free fall = 1g down**: Skydivers accelerate at 1g but feel weightless (net zero g-force)
  • **Jerk matters too**: Rate of acceleration change (m/s³) affects comfort more than peak g
  • **Scientific notation auto**: Values < 1 µm/s² display as 1.0×10⁻⁶ m/s² for readability

Complete Units Reference

SI / Metric Units

Unit NameSymbolm/s² EquivalentUsage Notes
centimeter per second squaredcm/s²0.01Lab settings; same as Gal in geophysics.
kilometer per hour per secondkm/(h⋅s)0.277778Automotive specs; 0-100 km/h times.
kilometer per hour squaredkm/h²0.0000771605Rarely used; academic contexts only.
kilometer per second squaredkm/s²1,000Astronomy and orbital mechanics; planetary accelerations.
meter per second squaredm/s²1SI base for acceleration; universal scientific standard.
millimeter per second squaredmm/s²0.001Precision instrumentation.
decimeter per second squareddm/s²0.1Small-scale acceleration measurements.
dekameter per second squareddam/s²10Rarely used; intermediate scale.
hectometer per second squaredhm/s²100Rarely used; intermediate scale.
meter per minute squaredm/min²0.000277778Slow acceleration over minutes.
micrometer per second squaredµm/s²0.000001Microscale acceleration (µm/s²).
nanometer per second squarednm/s²1.000e-9Nanoscale motion studies.

Gravitational Units

Unit NameSymbolm/s² EquivalentUsage Notes
Earth gravity (average)g9.80665Same as standard gravity; legacy naming.
milligravitymg0.00980665Microgravity research; 1 mg = 0.00981 m/s².
standard gravityg₀9.80665Standard gravity; 1g = 9.80665 m/s² (exact).
Jupiter gravityg♃24.79Jupiter: 2.53g; would crush humans.
Mars gravityg♂3.71Mars: 0.38g; colonization reference.
Mercury gravityg☿3.7Mercury surface: 0.38g; easier to escape than Earth.
microgravityµg0.00000980665Ultra-low gravity environments.
Moon gravityg☾1.62Moon: 0.17g; Apollo mission reference.
Neptune gravityg♆11.15Neptune: 1.14g; slightly higher than Earth.
Pluto gravityg♇0.62Pluto: 0.06g; very low gravity.
Saturn gravityg♄10.44Saturn: 1.06g; low for its size.
Sun gravity (surface)g☉274Sun surface: 28g; theoretical only.
Uranus gravityg♅8.87Uranus: 0.90g; ice giant.
Venus gravityg♀8.87Venus: 0.90g; similar to Earth.

Imperial / US Units

Unit NameSymbolm/s² EquivalentUsage Notes
foot per second squaredft/s²0.3048US engineering standard; ballistics and aerospace.
inch per second squaredin/s²0.0254Small-scale mechanisms and precision work.
mile per hour per secondmph/s0.44704Drag racing and automotive performance (mph/s).
foot per hour squaredft/h²0.0000235185Academic/theoretical; rarely practical.
foot per minute squaredft/min²0.0000846667Very slow acceleration contexts.
mile per hour squaredmph²0.124178Rarely used; academic only.
mile per second squaredmi/s²1,609.34Rarely used; astronomical scales.
yard per second squaredyd/s²0.9144Rarely used; historical contexts.

CGS System

Unit NameSymbolm/s² EquivalentUsage Notes
gal (galileo)Gal0.011 Gal = 1 cm/s²; geophysics standard.
milligalmGal0.00001Gravity surveys; oil/mineral prospecting.
kilogalkGal10High-acceleration contexts; 1 kGal = 10 m/s².
microgalµGal1.000e-8Tidal effects; subsurface detection.

Specialized Units

Unit NameSymbolm/s² EquivalentUsage Notes
g-force (fighter jet tolerance)G9.80665G-force felt; dimensionless ratio to Earth gravity.
knot per hourkn/h0.000142901Very slow acceleration; tide flows.
knot per minutekn/min0.00857407Gradual speed changes at sea.
knot per secondkn/s0.514444Maritime/aviation; knot per second.
leo (g/10)leo0.9806651 leo = g/10 = 0.981 m/s²; obscure unit.

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