diff --git a/FinalProjectCode.py b/FinalProjectCode.py
index 9622a65..026b3b4 100644
--- a/FinalProjectCode.py
+++ b/FinalProjectCode.py
@@ -2,7 +2,7 @@
 #Phys305
 #Final Project: Asteroid Version
 
-#run by "python final_project_asteroids_bodin"
+#run by "python FinalProjectCode.py"
 
 #Goal of Project:
    #Recreate the threebody problem we did for homework, for Jupiter the Sun and asteroids.
@@ -10,6 +10,321 @@
    #Plot and animate each in different colors
    #Add code to take the data for the asteroids and use it to plot a histogram showing the Kirkwood Gaps
 
+import math
+import numpy as np
+import matplotlib.pyplot as plt
+from matplotlib.animation import FuncAnimation
+import matplotlib.gridspec as gridspec
+
+G = 6.674e-11
+GMs = 4*(math.pi**2)
+m_sun = 1.989e30
+
+# Jupiter parameters
+ecc_jup = 0.0489
+semimajor_jup = 5.2044
+a_jup = semimajor_jup
+perihelion_jup = a_jup*(1-ecc_jup)
+m_jup = 1.8982e27
+vp_jup = math.sqrt(GMs) * math.sqrt((1+ecc_jup) / (a_jup*(1-ecc_jup)) * (1+(m_jup/m_sun)))
+
+# Calculate MMR positions for Jupiter
+# Formula: a = a_jup * (p/q)^(2/3)
+def calculate_mmr_positions():
+    mmr_ratios = [(3, 1), (5, 2), (7, 3), (2, 1)]  # p:q ratios
+    mmr_positions = []
+    for p, q in mmr_ratios:
+        a = a_jup * (p/q)**(2/3)
+        mmr_positions.append((p, q, a))
+    return mmr_positions
+
+# Fast Lyapunov Indicator (FLI) calculation
+def calculate_fli(a, e, t_integration=100, h=1e-2):
+    """
+    Calculate FLI for a test particle with given semi-major axis and eccentricity
+    """
+    # Initial conditions for the test particle
+    perihelion = a * (1 - e)
+    vp = math.sqrt(GMs) * math.sqrt((1 + e) / (a * (1 - e)))
+    x = -perihelion
+    y = 0
+    vx = 0
+    vy = vp
+    
+    # Initial conditions for a nearby particle (1e-10 AU difference in x)
+    x_near = x + 1e-10
+    y_near = y
+    vx_near = vx
+    vy_near = vy
+    
+    # Jupiter initial conditions
+    vx2 = 0
+    vy2 = vp_jup
+    x2 = -perihelion_jup
+    y2 = 0
+    
+    t = 0
+    max_fli = 0
+    
+    while t < t_integration:
+        # Calculate distances
+        r2 = math.sqrt(x2**2 + y2**2)
+        r = math.sqrt(x**2 + y**2)
+        rrel = math.sqrt((x - x2)**2 + (y - y2)**2)
+        
+        r_near = math.sqrt(x_near**2 + y_near**2)
+        rrel_near = math.sqrt((x_near - x2)**2 + (y_near - y2)**2)
+        
+        # Update velocities for test particle
+        vx = vx + h * (-GMs * x / r**3 - GMs * (m_jup/m_sun) * (x - x2) / rrel**3)
+        vy = vy + h * (-GMs * y / r**3 - GMs * (m_jup/m_sun) * (y - y2) / rrel**3)
+        
+        # Update velocities for nearby particle
+        vx_near = vx_near + h * (-GMs * x_near / r_near**3 - GMs * (m_jup/m_sun) * (x_near - x2) / rrel_near**3)
+        vy_near = vy_near + h * (-GMs * y_near / r_near**3 - GMs * (m_jup/m_sun) * (y_near - y2) / rrel_near**3)
+        
+        # Update velocities for Jupiter
+        vx2 = vx2 + h * (-GMs * x2 / r2**3)
+        vy2 = vy2 + h * (-GMs * y2 / r2**3)
+        
+        # Update positions for test particle
+        x = x + vx * h
+        y = y + vy * h
+        
+        # Update positions for nearby particle
+        x_near = x_near + vx_near * h
+        y_near = y_near + vy_near * h
+        
+        # Update positions for Jupiter
+        x2 = x2 + vx2 * h
+        y2 = y2 + vy2 * h
+        
+        # Calculate distance between test particle and nearby particle
+        delta_x = x_near - x
+        delta_y = y_near - y
+        delta = math.sqrt(delta_x**2 + delta_y**2)
+        
+        # Normalize the nearby particle position to keep delta small
+        if delta > 1e-5:
+            factor = 1e-10 / delta
+            x_near = x + delta_x * factor
+            y_near = y + delta_y * factor
+            vx_near = vx + (vx_near - vx) * factor
+            vy_near = vy + (vy_near - vy) * factor
+            delta = 1e-10
+        
+        # Update FLI
+        if delta > 0:
+            current_fli = math.log10(delta / 1e-10)
+            if current_fli > max_fli:
+                max_fli = current_fli
+        
+        t += h
+    
+    return max_fli
+
+# Precompute chaos map on (a, e) grid
+def precompute_chaos_map(a_min=2.0, a_max=3.6, e_min=0.0, e_max=0.4, grid_size=50):
+    """
+    Precompute FLI values for a grid of (a, e) points
+    """
+    a_grid = np.linspace(a_min, a_max, grid_size)
+    e_grid = np.linspace(e_min, e_max, grid_size)
+    fli_grid = np.zeros((grid_size, grid_size))
+    
+    print("Precomputing chaos map...")
+    for i in range(grid_size):
+        for j in range(grid_size):
+            a = a_grid[i]
+            e = e_grid[j]
+            fli = calculate_fli(a, e)
+            fli_grid[i, j] = fli
+        print(f"Progress: {i+1}/{grid_size}")
+    
+    return a_grid, e_grid, fli_grid
+
+# Generate real asteroids with initial positions and velocities
+def generate_asteroids(n_asteroids=100):
+    """
+    Generate real asteroids with random semi-major axes and eccentricities,
+    and calculate initial positions and velocities
+    """
+    semimajor_a = 1.5 * np.random.random(n_asteroids) + 2.0  # between 2 and 3.5 AU
+    ecc_a = 0.3 * np.random.random(n_asteroids)  # between 0 and 0.3
+    
+    x = np.array([])
+    y = np.array([])
+    vx = np.array([])
+    vy = np.array([])
+    
+    m_a = 1e10  # mass of asteroids (arbitrary since << Msun)
+    
+    for i in range(n_asteroids):
+        a_a = semimajor_a[i]
+        e_a = ecc_a[i]
+        perihelion = a_a * (1 - e_a)
+        
+        # Initial parameters for asteroid (perihelion at x=-perihelion, y=0)
+        vp = math.sqrt(GMs) * math.sqrt((1 + e_a) / (a_a * (1 - e_a)) * (1 + (m_a / m_sun)))
+        astr_vx = 0
+        astr_vy = vp
+        astr_x = -perihelion
+        astr_y = 0
+        
+        x = np.append(x, astr_x)
+        y = np.append(y, astr_y)
+        vx = np.append(vx, astr_vx)
+        vy = np.append(vy, astr_vy)
+    
+    return semimajor_a, ecc_a, x, y, vx, vy
+
+def main():
+    """
+    Main function to run the real-time resonance and chaos dynamics map
+    """
+    # Precompute chaos map
+    a_grid, e_grid, fli_grid = precompute_chaos_map()
+    
+    # Generate real asteroids with initial conditions
+    semimajor_a, ecc_a, x, y, vx, vy = generate_asteroids(n_asteroids=100)
+    
+    # Calculate MMR positions
+    mmr_positions = calculate_mmr_positions()
+    
+    # Simulation parameters
+    h = 1e-2
+    t = 0
+    t_final = 200
+    count = 0
+    
+    # Jupiter's initial conditions
+    vx2 = 0
+    vy2 = vp_jup
+    x2 = -perihelion_jup
+    y2 = 0
+    
+    # Create UI with two side-by-side windows
+    fig = plt.figure(figsize=(15, 7))
+    gs = gridspec.GridSpec(1, 2, width_ratios=[1, 1])
+    
+    # Left: Real-time histogram
+    ax_hist = plt.subplot(gs[0])
+    ax_hist.set_title('Real-time Asteroid Semi-major Axis Distribution')
+    ax_hist.set_xlabel('Semi-major Axis (AU)')
+    ax_hist.set_ylabel('Number of Asteroids')
+    ax_hist.set_xlim(2.0, 3.6)
+    
+    # Plot MMR positions as vertical dashed lines
+    for p, q, a in mmr_positions:
+        ax_hist.axvline(x=a, color='r', linestyle='--', alpha=0.7)
+        ax_hist.text(a + 0.01, 0.95, f'{p}:{q}', transform=ax_hist.get_xaxis_transform(),
+                    rotation=90, va='top', ha='left', color='r')
+    
+    # Right: Chaos map
+    ax_chaos = plt.subplot(gs[1])
+    ax_chaos.set_title('Chaos Map (a vs e)')
+    ax_chaos.set_xlabel('Semi-major Axis (AU)')
+    ax_chaos.set_ylabel('Eccentricity')
+    ax_chaos.set_xlim(2.0, 3.6)
+    ax_chaos.set_ylim(0.0, 0.4)
+    
+    # Plot chaos map
+    im = ax_chaos.pcolormesh(a_grid, e_grid, fli_grid.T, cmap='hot', shading='auto')
+    cbar = plt.colorbar(im, ax=ax_chaos)
+    cbar.set_label('Fast Lyapunov Indicator (FLI)')
+    
+    # Overlay real asteroids on chaos map
+    scat = ax_chaos.scatter(semimajor_a, ecc_a, color='blue', s=10, alpha=0.8)
+    
+    # Update histogram and chaos map in real-time
+    def update_hist(frame):
+        nonlocal t, count, x, y, vx, vy, x2, y2
+        
+        current_semimajor_a = np.copy(semimajor_a)
+        current_ecc_a = np.copy(ecc_a)
+        
+        if t < t_final:
+            # Run one time step of the simulation
+            
+            # Calculate distances for Jupiter
+            r2 = math.sqrt(x2**2 + y2**2)
+            
+            # Update velocities for asteroids
+            for i in range(len(x)):
+                r = math.sqrt(x[i]**2 + y[i]**2)
+                rrel = math.sqrt((x[i] - x2)**2 + (y[i] - y2)**2)
+                
+                vx[i] += h * (-GMs * x[i] / r**3 - GMs * (m_jup/m_sun) * (x[i] - x2) / rrel**3)
+                vy[i] += h * (-GMs * y[i] / r**3 - GMs * (m_jup/m_sun) * (y[i] - y2) / rrel**3)
+            
+            # Update velocities for Jupiter
+            vx2 += h * (-GMs * x2 / r2**3)
+            vy2 += h * (-GMs * y2 / r2**3)
+            
+            # Update positions for asteroids
+            for i in range(len(x)):
+                x[i] += vx[i] * h
+                y[i] += vy[i] * h
+            
+            # Update positions for Jupiter
+            x2 += vx2 * h
+            y2 += vy2 * h
+            
+            # Update time and count
+            t += h
+            count += 1
+            
+            # Calculate current semimajor axis and eccentricity for each asteroid
+            for i in range(len(x)):
+                # Calculate orbital energy E
+                v = math.sqrt(vx[i]**2 + vy[i]**2)
+                r = math.sqrt(x[i]**2 + y[i]**2)
+                E = 0.5 * v**2 - GMs / r
+                
+                # Calculate semimajor axis a
+                a = -GMs / (2 * E)
+                current_semimajor_a[i] = a
+                
+                # Calculate angular momentum h
+                h_orb = x[i] * vy[i] - y[i] * vx[i]
+                
+                # Calculate eccentricity e
+                e = math.sqrt(1 + (2 * E * h_orb**2) / (GMs**2))
+                current_ecc_a[i] = e
+        
+        # Update histogram
+        ax_hist.clear()
+        ax_hist.set_title('Real-time Asteroid Semi-major Axis Distribution')
+        ax_hist.set_xlabel('Semi-major Axis (AU)')
+        ax_hist.set_ylabel('Number of Asteroids')
+        ax_hist.set_xlim(2.0, 3.6)
+        
+        # Plot histogram with current a values
+        ax_hist.hist(current_semimajor_a, bins=50, histtype='bar', color='b', alpha=0.7)
+        
+        # Replot MMR positions
+        for p, q, a in mmr_positions:
+            ax_hist.axvline(x=a, color='r', linestyle='--', alpha=0.7)
+            ax_hist.text(a + 0.01, 0.95, f'{p}:{q}', transform=ax_hist.get_xaxis_transform(),
+                        rotation=90, va='top', ha='left', color='r')
+        
+        # Update chaos map title with current time
+        ax_chaos.set_title(f'Chaos Map (a vs e) - Time: {t:.2f} years')
+        
+        # Update scatter plot on chaos map
+        scat.set_offsets(np.c_[current_semimajor_a, current_ecc_a])
+        
+        return ax_hist, scat
+    
+    # Animation
+    ani = FuncAnimation(fig, update_hist, frames=100, interval=1000, blit=False)
+    
+    plt.tight_layout()
+    plt.show()
+
+if __name__ == "__main__":
+    main()
+
 def Asteroids():
     import math
     import numpy as np
@@ -153,25 +468,25 @@ def Asteroids():
     plt.show()
 #Asteroids() #uncomment to run code and add data to histogram
 
-def histogram(): #time to plot the histogram 
-    import matplotlib.pyplot as plt
-    import numpy as np
-    import matplotlib
+# def histogram(): #time to plot the histogram 
+#     import matplotlib.pyplot as plt
+#     import numpy as np
+#     import matplotlib
 
-    f= open('asteroid_datafile.txt','r')
-    a=np.array([])
-    for line in f:
-        s=line.split()
-        a = np.append(a,float(s[0]))
-    f.close()
+#     f= open('asteroid_datafile.txt','r')
+#     a=np.array([])
+#     for line in f:
+#         s=line.split()
+#         a = np.append(a,float(s[0]))
+#     f.close()
 
-    bins = np.linspace(2, 3.6, 500)
+#     bins = np.linspace(2, 3.6, 500)
 
-    fig, ax = plt.subplots()
-    plt.hist(a, bins, histtype='bar', color='b')
-    plt.xlabel('AU')
-    plt.ylabel('Number of Asteroids')
-    plt.title('Kirkwood Gaps')
-    fig.savefig('histograms_final.png')
-    plt.show()
-histogram()
+#     fig, ax = plt.subplots()
+#     plt.hist(a, bins, histtype='bar', color='b')
+#     plt.xlabel('AU')
+#     plt.ylabel('Number of Asteroids')
+#     plt.title('Kirkwood Gaps')
+#     fig.savefig('histograms_final.png')
+#     plt.show()
+# histogram()
diff --git a/histograms_final.png b/histograms_final.png
index f981aba..08c3d53 100644
Binary files a/histograms_final.png and b/histograms_final.png differ