ISS feels 0 g but pulls 0.9 g
The International Space Station circles Earth at 7.66 km/s with a radius of ~6,780 km, so it’s constantly accelerating inward at 8.7 m/s² (0.89 g)—astronauts feel weightless because they’re in steady free fall.
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When an object moves along a circular path, its direction changes constantly—even if its speed stays the same. That continuous change of direction requires an inward (radial) acceleration called centripetal acceleration. For uniform circular motion (constant speed), the magnitude is a = v² / r, where v is the speed and r is the path radius. To produce that acceleration, some agent must supply a centripetal force toward the center: Fc = m v² / r. Dividing a by standard gravity g₀ = 9.80665 m/s² converts acceleration into g-forces—a familiar way to compare ride intensity to everyday weight on Earth.
Two quick, equivalent viewpoints help build intuition. (1) As speed increases, the path tries to “straighten out,” so you need more inward pull to bend it—hence the v² factor. (2) As radius grows, the curve becomes gentler; less inward pull is needed, so the same speed feels milder on a big turn than on a tight corner. Designers of rollercoasters and racetracks exploit this trade-off constantly.
It is also useful to connect linear and angular quantities. The angular speed is ω = v / r (radians per second), the period for one full revolution is T = 2π / ω = 2πr / v, and revolutions per minute follow as rpm = 60 / T. These let you translate a measured lap time or spin rate into forces and g-levels quickly.
Consider a 75 kg rider taking a 15 m radius turn at 20 m/s. The inward acceleration is a = 20² / 15 = 26.67 m/s², which is about 2.72 g. The required inward force is Fc = m a = 75 × 26.67 ≈ 2.0 × 10³ N. The angular speed is ω = v/r = 1.333 rad/s, so the period is T = 2π/ω ≈ 4.71 s and the spin rate is about 12.7 rpm.
The calculator reports the required inward force; in practice this may be supplied by friction (tires on road), track normal force (coasters), string tension (whirling a mass), or gravity itself in orbital motion. In all cases, the numbers let you reason about design limits, comfort, and safety with clear, testable physics.
The International Space Station circles Earth at 7.66 km/s with a radius of ~6,780 km, so it’s constantly accelerating inward at 8.7 m/s² (0.89 g)—astronauts feel weightless because they’re in steady free fall.
A jet pulling 9 g at 250 m/s needs a turn radius of just 710 m. A 75 kg pilot effectively “weighs” 675 kg, so their seat must push with about 6.6 kN.
Take a 20 m radius loop at 20 m/s: the bottom loads riders with 3.0 g while the top eases to 1.0 g. Tweaking radius or speed keeps restraints comfortable yet exciting.
A rotating habitat with a 100 m radius only needs 3 RPM to mimic 1 g. Double the radius to 200 m and you can drop to 2.1 RPM—slow enough to keep most people comfortable.
A 0.25 m drum spinning at 1,200 RPM sees 3,950 m/s² of inward pull (~403 g). No wonder rinse water gets ripped out so fast.