1:1
1:3
3:1
1:9
9:1
Two isolated charged spheres with radii R and 3R are connected by a conducting wire.
When connected, the potentials equalize: \[ V_A = V_B \] \[ \frac{kQ_A}{R} = \frac{kQ_B}{3R} \]
Charge Ratio is \[ \frac{Q_A}{Q_B} = \frac{R}{3R} = \frac{1}{3} \]
Alternatively, since capacitance C ∝ radius: \[ \frac{C_A}{C_B} = \frac{R}{3R} = \frac{1}{3} \] And Q = CV, so when V equalizes: \[ \frac{Q_A}{Q_B} = \frac{C_A}{C_B} = \frac{1}{3} \]
1. Understand the concept of charge distribution:
When two charged conductors are connected by a conducting wire, charge flows between them until they reach the same potential.
2. Recall the formula for the potential of a sphere:
The electric potential (V) of a conducting sphere with charge Q and radius R is given by:
\[V = \frac{kQ}{R}\]
where k is Coulomb's constant.
3. Set the final potentials equal:
Let \(Q_A\) and \(Q_B\) be the initial charges on spheres A and B, and \(Q_A'\) and \(Q_B'\) be their final charges after they are connected. Since the spheres reach the same potential after connection:
\[V_A' = V_B'\]
\[\frac{kQ_A'}{R} = \frac{kQ_B'}{3R}\]
4. Solve for the charge ratio:
Simplify the equation:
\[Q_A' = \frac{Q_B'}{3}\]
\[\frac{Q_A'}{Q_B'} = \frac{1}{3}\]
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Electric Field is the electric force experienced by a unit charge.
The electric force is calculated using the coulomb's law, whose formula is:
\(F=k\dfrac{|q_{1}q_{2}|}{r^{2}}\)
While substituting q2 as 1, electric field becomes:
\(E=k\dfrac{|q_{1}|}{r^{2}}\)
SI unit of Electric Field is V/m (Volt per meter).