Source files: 1 | Classes: 1 | Methods: 1 | Enums: 0

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GTOS.Astronomy.Core

AstronomyCoreAtomics

static class

Source: AstronomyCoreAtomics.cs

Constants and Fields

ASTRONOMICAL_UNIT_m

const double

BOLTZMANN_CONSTANT_J_per_K

const double

CalculationFailure

const double

GRAVITATIONAL_CONSTANT_m3_per_kg_s2

const double

HUBBLE_CONSTANT_km_per_s_per_Mpc

const double

LIGHT_YEAR_m

const double

PARSEC_m

const double

SOLAR_LUMINOSITY_W

const double

SOLAR_MASS_kg

const double

SOLAR_RADIUS_m

const double

SPEED_OF_LIGHT_m_per_s

const double

STEFAN_BOLTZMANN_CONSTANT

const double

Methods

CalculateSemiMajorAxis

double CalculateSemiMajorAxis ( double orbital_period_s, double central_body_mass_kg )

Calculate semi-major axis from orbital period (Kepler's 3rd law)
a³ = (GMT²) / (4π²)

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Generated from GTOS Savants source -- 2026-03-22