This is the code I have. I would need:
This is the content of the python file:
import numpy as np
# Constants for each planet (some values will be hypothetical or approximate)
planetary_data = {
'Mercury': {
'mass': 3.30e23, # kg
'radius': 2.4397e6, # m
'theta': 0.03, # degrees
'rotation_period': 58.6667 * 24 * 3600, # seconds
'rp': 4.6e10, # m
'eccentricity': 0.2056
},
'Venus': {
'mass': 4.87e24,
'radius': 6.0518e6,
'theta': 177.4,
'rotation_period': 243 * 24 * 3600,
'rp': 1.07577e11,
'eccentricity': 0.0067
},
'Earth': {
'mass': 5.97e24,
'radius': 6.371e6,
'theta': 23.4,
'rotation_period': 23.933 * 3600,
'rp': 1.471e11,
'eccentricity': 0.0167
},
'Mars': {
'mass': 6.42e23,
'radius': 3.3895e6,
'theta': 25.2,
'rotation_period': 24.6 * 3600,
'rp': 2.066e11,
'eccentricity': 0.0934
},
'Jupiter': {
'mass': 1.90e27,
'radius': 6.9911e7,
'theta': 3.1,
'rotation_period': 9.9167 * 3600,
'rp': 7.4052e11,
'eccentricity': 0.0489
},
'Saturn': {
'mass': 5.68e26,
'radius': 5.8232e7,
'theta': 26.7,
'rotation_period': 10.55 * 3600,
'rp': 1.35255e12,
'eccentricity': 0.0565
}
}
# Calculate the spin angular momentum vector
def calculate_spin_angular_momentum(mass, radius, rotation_period, theta):
I = (2/5) * mass * radius**2 # Moment of inertia for a sphere
omega = 2 * np.pi / rotation_period # Angular velocity
L = I * omega # Magnitude of angular momentum
theta_rad = np.radians(theta)
S = L * np.array([np.sin(theta_rad), 0, np.cos(theta_rad)])
return S
# Example calculation
for planet, data in planetary_data.items():
S = calculate_spin_angular_momentum(
data['mass'], data['radius'], data['rotation_period'], data['theta']
)
print(f"Spin angular momentum vector for {planet}: {S}")
- Badges
- Science method
- Similar topics
- Methodology
- Crystallography
- X-ray Diffraction