Update README.md

README.md

@@ -18,11 +18,13 @@ The simulator consists of several key components:
 
 The simulator uses Newton's law of universal gravitation to calculate the forces between celestial bodies. The gravitational force between two bodies is given by:
 
-$$ F = G \frac{m_1 m_2}{r^2} $$
+$$ 
+F = G \frac{m_1 m_2}{r^2} 
+$$
 
 Where:
 - $F$ is the gravitational force between the two bodies
-- $G$ is the gravitational constant ($$6.67430 \times 10^{-11} \, \text{N} \cdot \text{m}^2 / \text{kg}^2$$)
+- $G$ is the gravitational constant ($6.67430 \times 10^{-11} \, \text{N} \cdot \text{m}^2 / \text{kg}^2$)
 - $m_1$ and $m_2$ are the masses of the two bodies
 - $r$ is the distance between the centers of the two bodies
 
@@ -31,9 +33,18 @@ Where:
 The motion of each celestial body is updated using numerical integration. We use a simple Euler method for updating positions and velocities:
 
 1. Calculate the net force on each body
-2. Calculate acceleration: $$ \vec{a} = \frac{\vec{F}}{m} $$
-3. Update velocity: $$ \vec{v}_{new} = \vec{v}_{old} + \vec{a} \Delta t $$
-4. Update position: $$ \vec{x}_{new} = \vec{x}_{old} + \vec{v}_{new} \Delta t $$
+2. Calculate acceleration:
+```math
+$$ \vec{a} = \frac{\vec{F}}{m} $$
+```
+3. Update velocity:
+```math
+$$ \vec{v}_{new} = \vec{v}_{old} + \vec{a} \Delta t $$
+```
+4. Update position:
+```math
+$$ \vec{x}_{new} = \vec{x}_{old} + \vec{v}_{new} \Delta t $$
+```
 
 Where $\Delta t$ is the time step of the simulation.