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Escape Velocity

ESCAPE VELOCITY

*Use scientific notation for mass (e.g. 1.9e27 for Jupiter)
BREAKOUT SPEED
11186.0

METERS PER SECOND (M/S)


Mach: 32.8
Gravity: 1.00 G
TRAJECTORY TYPE:

Terrestrial Planet Escape

Vector Ve

The Great Departure. Escape velocity is the point where Momentum Overcomes Mass. It’s the speed required to turn a planet into a distant memory.

  • πŸ”“ No Orbit: You aren't looping; you are leaving.
  • βš–οΈ Mass Independent: A marble and a Starship need the same speed.
  • 🌠 Hyperbolic: Your path becomes a "V" shape rather than a circle.
πŸš€
GRAVITY BREAKOUT
11.2 km/s
PATH: βœ… HYPERBOLIC EXIT
ESCAPE-SYNC ACTIVE βœ…

Vector Mass

The Source Code. Central Mass is the Weight of Authority. Every orbital maneuver you perform is a direct negotiation with the kilograms packed into the center of the planet.

  • πŸ’Ž Density: How tightly M is packed changes the "Surface Gravity."
  • πŸ”„ Influence: M dictates the shape of every possible orbit.
  • πŸ—οΈ Static: Unlike your fuel, the Central Mass never changes.
πŸͺ
GRAVITY SOURCE (M)
5.97 x 10²⁴ kg
BODY: βœ… EARTH (TERRA)
MASS-SYNC ACTIVE βœ…

Radius (r)

The Distance Matrix. Radius is the Leash of Gravity. It determines how much energy you need to maintain your position in the vacuum.

  • πŸ“ Core-Focus: Always measured from the center of mass.
  • πŸ“‰ Fall-off: Higher r = Lower G-load = Slower orbital speed.
  • πŸ›°οΈ Altitude: Only a fraction of the total radial distance.
πŸŒ‘
RADIAL COORDINATE (r)
6,771 km
ALTITUDE: 400 KM
RADIAL-SYNC ACTIVE βœ…

Limit: ve

The Zero-Point. Minimum escape velocity is the Kinetic Key. It’s the exact moment your momentum outweighs the planet's structural pull.

  • πŸ”“ Parabolic: Your path becomes an open curve.
  • 🏁 Finality: No more fuel is needed to keep going.
  • πŸ“‰ Radial: The further you start, the lower the cost.
πŸš€
VELOCITY THRESHOLD
11,186 m/s
ESCAPE: βœ… SUCCESSFUL
BREAKOUT-SYNC ACTIVE βœ