1g Constant Acceleration

The 1 g transfer model represents an idealized symmetric acceleration and deceleration profile using sustained proper acceleration. In this reference case, the vehicle accelerates for the first half of the trajectory, performs an inertial reorientation maneuver, and then decelerates along the remaining half of the transfer arc.

The calculator illustrates the relativistic relationship between ship proper time, Earth-frame elapsed time, distance, and peak velocity. As distance increases, time dilation becomes operationally significant: elapsed time aboard the vehicle diverges from the external reference frame while the vehicle remains below c.

This model is a kinematic reference only. It does not include propulsion duty-cycle limits, fuel-margin constraints, interstellar medium interaction, relativistic debris exposure, accumulated radiation dose, navigation uncertainty, gravitational perturbations, thermal-management limits, or cosmological-scale effects at extreme distances.

Distance: - ly
Travel time (ship): - y
Travel time (Earth): - y
Top speed: -
Proxima Centauri system

Proxima Centauri

Proxima Centauri is the nearest stellar target to the Solar System and the primary focus of the 1gSpace mission architecture. The star is a low-mass red dwarf gravitationally associated with the Alpha Centauri A/B binary, but it remains dynamically distinct and hosts its own compact planetary system.

The operational target is Proxima b, a terrestrial-mass planet in the system's temperate orbital region. Because the planet is expected to be tidally locked, the most relevant surface environment is the terminator region between the permanent day and night hemispheres, where thermal gradients may permit comparatively stable long-duration operations.

Mission planning treats Proxima b as an environment requiring staged verification rather than assumption-based settlement. ACEP provides the first orbital and atmospheric dataset, ISV Innes performs crew-directed survey and surface-access validation, and later logistics and transport stages proceed only after the site, hazards, and operating constraints have been characterized.

Explore Interactive 3D Model Watch 3D Model Overview

Long-Duration Settlement

The long-duration settlement phase begins only after the reconnaissance, crewed validation, and uncrewed logistics stages have reduced the major environmental and operational uncertainties associated with Proxima b surface operations.

ISV Proxima is defined as the downstream population-transfer vehicle, responsible for transporting the larger colony element and the primary habitat systems required for permanent settlement. Its role depends on prior validation by ACEP, ISV Innes, and ISV Anglada, rather than operating as an isolated first-arrival vehicle.

Eternal Sunset is the supported initial settlement node. It is planned around transported habitats, delivered infrastructure, external logistics capacity, and pre-positioned surface systems, allowing the first permanent population to stabilize operations and develop reliable local workflows.

Eternal Sunrise represents the later self-derived expansion stage. Unlike Eternal Sunset, it is not planned around additional interstellar transport or external construction support. Its development must depend on in-situ materials, local manufacturing, mature resource extraction, established work practices, population structure, technical culture, governance norms, and operational methods developed on Proxima b itself.

In program terms, the mission sequence advances from reconnaissance to validation, from validation to supported habitation, and from supported habitation to local expansion. The objective is not only arrival, but the creation of a repeatable engineering and social framework for sustained planetary operations.