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.
Foundations of Acceleration
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
- 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.
- 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 Body | Surface Gravity | Facts |
|---|---|---|
| Sun | 274 m/s² (28g) | Would crush any spacecraft |
| Jupiter | 24.79 m/s² (2.53g) | Largest planet, no solid surface |
| Neptune | 11.15 m/s² (1.14g) | Ice giant, similar to Earth |
| Saturn | 10.44 m/s² (1.06g) | Low density despite size |
| Earth | 9.81 m/s² (1g) | Our reference standard |
| Venus | 8.87 m/s² (0.90g) | Near-twin to Earth |
| Uranus | 8.87 m/s² (0.90g) | Same as Venus |
| Mars | 3.71 m/s² (0.38g) | Easier to launch from |
| Mercury | 3.7 m/s² (0.38g) | Slightly less than Mars |
| Moon | 1.62 m/s² (0.17g) | Apollo astronaut jumps |
| Pluto | 0.62 m/s² (0.06g) | Dwarf planet, very low |
G-Force Effects on Humans
Understanding what different g-forces feel like and their physiological effects:
| Scenario | G-Force | Human Effect |
|---|---|---|
| Standing still | 1g | Normal Earth gravity |
| Elevator start/stop | 1.2g | Barely noticeable |
| Car braking hard | 1.5g | Pushed against seatbelt |
| Roller coaster | 3-6g | Heavy pressure, thrilling |
| Fighter jet turn | 9g | Vision tunneling, possible blackout |
| F1 car braking | 5-6g | Helmet feels 30kg heavier |
| Rocket launch | 3-4g | Chest compression, hard to breathe |
| Parachute opening | 3-5g | Brief jolt |
| Crash test | 20-60g | Serious injury threshold |
| Ejection seat | 12-14g | Spinal 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
| Context | Acceleration | Notes |
|---|---|---|
| Snail | 0.00001 m/s² | Extremely slow |
| Human walking start | 0.5 m/s² | Gentle acceleration |
| City bus | 1.5 m/s² | Comfortable transport |
| Standard gravity (1g) | 9.81 m/s² | Earth surface |
| Sports car 0-60mph | 10 m/s² | 1g acceleration |
| Drag racing launch | 40 m/s² | 4g wheelie territory |
| F-35 catapult launch | 50 m/s² | 5g in 2 seconds |
| Artillery shell | 100,000 m/s² | 10,000g |
| Bullet in barrel | 500,000 m/s² | 50,000g |
| Electron in CRT | 10¹⁵ m/s² | Relativistic |
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
- 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
| From | To | Multiply By | Example |
|---|---|---|---|
| g | m/s² | 9.80665 | 3g × 9.81 = 29.4 m/s² |
| m/s² | g | 0.10197 | 20 m/s² × 0.102 = 2.04g |
| m/s² | ft/s² | 3.28084 | 10 m/s² × 3.28 = 32.8 ft/s² |
| ft/s² | m/s² | 0.3048 | 32.2 ft/s² × 0.305 = 9.81 m/s² |
| mph/s | m/s² | 0.44704 | 10 mph/s × 0.447 = 4.47 m/s² |
| km/h/s | m/s² | 0.27778 | 100 km/h/s × 0.278 = 27.8 m/s² |
| Gal | m/s² | 0.01 | 500 Gal × 0.01 = 5 m/s² |
| milligal | m/s² | 0.00001 | 1000 mGal × 0.00001 = 0.01 m/s² |
Quick Examples
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
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
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
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
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 Name | Symbol | m/s² Equivalent | Usage Notes |
|---|---|---|---|
| centimeter per second squared | cm/s² | 0.01 | Lab settings; same as Gal in geophysics. |
| kilometer per hour per second | km/(h⋅s) | 0.277778 | Automotive specs; 0-100 km/h times. |
| kilometer per hour squared | km/h² | 0.0000771605 | Rarely used; academic contexts only. |
| kilometer per second squared | km/s² | 1,000 | Astronomy and orbital mechanics; planetary accelerations. |
| meter per second squared | m/s² | 1 | SI base for acceleration; universal scientific standard. |
| millimeter per second squared | mm/s² | 0.001 | Precision instrumentation. |
| decimeter per second squared | dm/s² | 0.1 | Small-scale acceleration measurements. |
| dekameter per second squared | dam/s² | 10 | Rarely used; intermediate scale. |
| hectometer per second squared | hm/s² | 100 | Rarely used; intermediate scale. |
| meter per minute squared | m/min² | 0.000277778 | Slow acceleration over minutes. |
| micrometer per second squared | µm/s² | 0.000001 | Microscale acceleration (µm/s²). |
| nanometer per second squared | nm/s² | 1.000e-9 | Nanoscale motion studies. |
Gravitational Units
| Unit Name | Symbol | m/s² Equivalent | Usage Notes |
|---|---|---|---|
| Earth gravity (average) | g | 9.80665 | Same as standard gravity; legacy naming. |
| milligravity | mg | 0.00980665 | Microgravity research; 1 mg = 0.00981 m/s². |
| standard gravity | g₀ | 9.80665 | Standard gravity; 1g = 9.80665 m/s² (exact). |
| Jupiter gravity | g♃ | 24.79 | Jupiter: 2.53g; would crush humans. |
| Mars gravity | g♂ | 3.71 | Mars: 0.38g; colonization reference. |
| Mercury gravity | g☿ | 3.7 | Mercury surface: 0.38g; easier to escape than Earth. |
| microgravity | µg | 0.00000980665 | Ultra-low gravity environments. |
| Moon gravity | g☾ | 1.62 | Moon: 0.17g; Apollo mission reference. |
| Neptune gravity | g♆ | 11.15 | Neptune: 1.14g; slightly higher than Earth. |
| Pluto gravity | g♇ | 0.62 | Pluto: 0.06g; very low gravity. |
| Saturn gravity | g♄ | 10.44 | Saturn: 1.06g; low for its size. |
| Sun gravity (surface) | g☉ | 274 | Sun surface: 28g; theoretical only. |
| Uranus gravity | g♅ | 8.87 | Uranus: 0.90g; ice giant. |
| Venus gravity | g♀ | 8.87 | Venus: 0.90g; similar to Earth. |
Imperial / US Units
| Unit Name | Symbol | m/s² Equivalent | Usage Notes |
|---|---|---|---|
| foot per second squared | ft/s² | 0.3048 | US engineering standard; ballistics and aerospace. |
| inch per second squared | in/s² | 0.0254 | Small-scale mechanisms and precision work. |
| mile per hour per second | mph/s | 0.44704 | Drag racing and automotive performance (mph/s). |
| foot per hour squared | ft/h² | 0.0000235185 | Academic/theoretical; rarely practical. |
| foot per minute squared | ft/min² | 0.0000846667 | Very slow acceleration contexts. |
| mile per hour squared | mph² | 0.124178 | Rarely used; academic only. |
| mile per second squared | mi/s² | 1,609.34 | Rarely used; astronomical scales. |
| yard per second squared | yd/s² | 0.9144 | Rarely used; historical contexts. |
CGS System
| Unit Name | Symbol | m/s² Equivalent | Usage Notes |
|---|---|---|---|
| gal (galileo) | Gal | 0.01 | 1 Gal = 1 cm/s²; geophysics standard. |
| milligal | mGal | 0.00001 | Gravity surveys; oil/mineral prospecting. |
| kilogal | kGal | 10 | High-acceleration contexts; 1 kGal = 10 m/s². |
| microgal | µGal | 1.000e-8 | Tidal effects; subsurface detection. |
Specialized Units
| Unit Name | Symbol | m/s² Equivalent | Usage Notes |
|---|---|---|---|
| g-force (fighter jet tolerance) | G | 9.80665 | G-force felt; dimensionless ratio to Earth gravity. |
| knot per hour | kn/h | 0.000142901 | Very slow acceleration; tide flows. |
| knot per minute | kn/min | 0.00857407 | Gradual speed changes at sea. |
| knot per second | kn/s | 0.514444 | Maritime/aviation; knot per second. |
| leo (g/10) | leo | 0.980665 | 1 leo = g/10 = 0.981 m/s²; obscure unit. |
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