Interplanetary Compression Dynamics

"All the planets in our solar system would fit between Earth and the Moon." This geometric curiosity, recently popularized on CBS Survivor, is mathematically accurate but dynamically catastrophic.

The Geometric Truth

The sum of planetary diameters equals approximately 380,016 km, which indeed fits within the average Earth-Moon distance of 384,400 km. However, this "fit" requires perfect linear alignment and assumes static bodies.

The Gravitational Reality

This simulator implements the full N-body problem with 11 gravitating masses: the Sun (as central reference), eight planets, the Moon, and Pluto. The gravitational force on body $i$ is:

$$ \vec{F}_i = \sum_{j \neq i} G \frac{m_i m_j}{|\vec{r}_{ij}|^3} \vec{r}_{ij} $$

where $G = 6.674 \times 10^{-11} \text{ m}^3\text{kg}^{-1}\text{s}^{-2}$ is the gravitational constant.

Initial Condition Modes

Position Modes:

Velocity Modes:

Orbital Stability

For circular orbit velocity at radius $r$:

$$ v_{\text{circ}} = \sqrt{\frac{GM_{\odot}}{r}} $$

Interactive Controls

  1. Choose Configuration: All settings apply immediately - no apply button needed.
  2. Drag Planets (Position): In pause mode, drag planets radially to adjust orbital radius and angle.
  3. Edit Velocity: Shift-click planet to open velocity editor, adjust magnitude and direction.
  4. View Modes: Toggle between Solar System view and Earth-Moon zoom, or ride planets.
  5. Dynamic Scaling: Planets scale based on separation to maintain visibility.
  6. Start Simulation: Observe gravitational interactions in real-time.

⚙️ Control Center

1.0× Scale

📹 Camera POV

Medium
Sim Time
0.0 hr
Collisions
0
Energy Δ%
0.00
Max Accel
0
Most Perturbed Body
Lyapunov Approx
0.000
⚠️ Reality Check: Jupiter's mass alone would tidally disrupt Earth within minutes at this proximity. This is a thought experiment, not engineering advice.

Edit Velocity Vector

Direction: 0° = +X axis (right), 90° = +Z axis (up in top view)