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Gorbillian Transit & Navigation Calculator

Calculate travel distances, transit times, effective velocities, and ETAs across the Sol System and the Zul'Elkoen Star Map — combining real normal-space propulsion physics with the fictional Gorbillian metric transit system.

SOL TRANSIT REFERENCE

NAVIGATION INPUT

Standard high-performance planetary and interplanetary propulsion; preferred for local operations where Gorbillian fields are unsafe or undesirable.

Gorbillian DriveThe Gorbillian Modulator engineers the local spacetime metric, reducing the effective spatial interval the vessel must traverse. It is not a warp drive and does not itself produce thrust.

Engage the Gorbillian metric field for interstellar transit.

COMPARE GORBILLIAN SETTINGS

Effective distance, transit rate, and total time for each spatial setting (VPPS 8, Fusion Propulsion).

SettingEffective DistanceEff. RateGorbillian TransitTotal Time
Normal Space18.2 AU0.015c0.0 s14 d 1 h
Mu1.2 AU12.251c12 min 21 s24 min 52 s
Thule0.2 AU83.333c1 min 49 s14 min 20 s
Ys0.0 AU7.999896e+31c0.0 s12 min 31 s

COMPARE PROPULSION SYSTEMS

Transit time for each propulsion system on the selected route (normal space only).

Conventional RocketIonFusionQuantum VacuumAntimatter0.0 s81 d 0 h162 d 0 h243 d 1 h324 d 1 h

THE PHYSICS BEHIND THE FICTION

Real equations, fictional extension

Distance, Speed and Time (real)

d = v t

Distance equals velocity multiplied by time. This is the foundation of every transit calculation here.

Acceleration and Deceleration (real)

v = a t    d = ½ a t²

A vessel accelerates at a constant rate aRate of change of velocity. Here expressed in g (1 g ≈ 9.81 m/s²). The vessel accelerates for half the journey and decelerates for the other half. for half the journey, then decelerates for the other half. If the route is long enough, it reaches its cruise velocityThe maximum practical sustained velocity of a normal-space propulsion system. The vessel cruises at this speed only if the route is long enough to reach it. and coasts; otherwise it turns around at the midpoint.

Effective Gorbillian Distance (fictional)

De = D × (1 − R)

The Gorbillian field reduces the effective spatial interval the vessel must traverse. RThe Gorbillian Modulator engineers the local spacetime metric, reducing the effective spatial interval the vessel must traverse. It is not a warp drive and does not itself produce thrust. is the spatial-reduction fraction for the selected setting (Mu, Thule, or Ys).

Gorbillian Transit Time (fictional)

tG = D(1 − R) / VVPPS

The vessel transits the reduced effective distance at its VPPSVessel Propulsive Performance Scale — here used as the vessel's transit velocity through the engineered Gorbillian pathway, as a fraction of c. VPPS velocity never exceeds c. velocity. VPPS velocity never exceeds c.

Effective Normal-Space Transit Rate (fictional)

Veffective = VVPPS / (1 − R)

This effective rateEffective Normal-Space Transit Rate — how quickly the journey is completed relative to the original physical distance. This is NOT the spacecraft's local speed through space; it can exceed c because the Gorbillian field shortens the path. describes how quickly the journey is completed relative to the original physical distance. It can exceed c because the path is shortened — the spacecraft is not locally moving through space faster than light.

Three-Dimensional Stellar Separation (real)

D = √[(X₂−X₁)² + (Y₂−Y₁)² + (Z₂−Z₁)²]

Interstellar distances use true 3D coordinates in light-yearsA unit of DISTANCE — the distance light travels in one Earth year (≈ 9.46 trillion km). Not a unit of time., not a subtraction of Sol-distances. Where coordinates are not yet established, the calculator reports the distance as unavailable rather than inventing a value.

A light-yearA unit of DISTANCE — the distance light travels in one Earth year (≈ 9.46 trillion km). Not a unit of time. is a unit of distance, not time — the distance light travels in one Earth year. An AUAstronomical Unit — the mean distance between Earth and the Sun (≈ 149.6 million km). is Earth's mean distance from the Sun. A parsecA unit of stellar distance equal to about 3.26 light-years. ≈ 3.26 light-years.

Explore the Real Science

Long before hypothetical interstellar drives, engineers learned to transform thermal energy into motion — and to navigate by the stars. Explore the real science behind the transit.

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