pat Flashcards
Circular Motion - Position
s = rθ
Circular Motion - Angular Frequency
d(θ) / dt
Circular Motion - Velocity
By combining the position and angular frequency formulas,
v = rω
Circular Motion - Centripetal Acceleration
By approximating dv between varying velocities (same magnitude) using an arc,
a = v² / r
Circular Motion - Centripetal Force
F = m (v² / r)
Circular Motion - Period
The time taken for one revolution to occur is given by,
2π / ω
Coulomb’s Law
F = kₑ(Q₁Q₂ / r²)
kₑ
kₑ = 8.99x10⁹ Nm² C⁻² OR
kₑ = 1 / 4πε₀ where ε₀ = 8.85x10⁻¹² Nm⁻¹
Results of coulomb’s law
-F => Attraction
+F => Repulsion
Moon
Astronomical body that orbits a planet. Natural satellite.
Asteroid
Rocky, metallic or icy body with no atmosphere.
Comet
Icy body that releases gases near the sun, producing an atmosphere and a gas tail.
Planet
Spheroid body that orbits a star.
Star
Spheroid, luminous body of plasma that emits radiation via fusion.
Lunar phases
New, first quarter, full, last quarter