Gauss’s planetary equations

E29372

Gauss’s planetary equations are a set of differential equations in celestial mechanics that describe how a planet’s orbital elements change over time under the influence of perturbing forces.

AI illustration

How this image was made

AI-generated illustration of Gauss’s planetary equations

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of Gauss’s planetary equations (Gauss’s planetary equations are a set of differential equations in celestial mechanics that describe how a planet’s orbital elements change over time under the influence of perturbing forces.)

All labels observed (3)

How this entity was disambiguated

Statements (45)

Predicate Object
instanceOf mathematical formulation in celestial mechanics ⓘ
set of differential equations ⓘ
appliesTo Keplerian orbital elements ⓘ
asteroid orbits ⓘ
cometary orbits ⓘ
osculating orbital elements ⓘ
planetary orbits ⓘ
satellite orbits ⓘ
assumes perturbing forces small compared to central gravity ⓘ
two-body Keplerian reference orbit plus small perturbations ⓘ
category orbital perturbation theory ⓘ
describes time evolution of orbital elements ⓘ
variation of orbital elements under perturbations ⓘ
domain classical mechanics ⓘ
expressedIn non-singular form for non-circular, non-equatorial orbits ⓘ
field astrodynamics ⓘ
celestial mechanics ⓘ
orbital mechanics ⓘ
governs time derivative of argument of periapsis ⓘ
time derivative of eccentricity ⓘ
time derivative of inclination ⓘ
time derivative of longitude of ascending node ⓘ
time derivative of mean anomaly ⓘ
time derivative of semi-major axis ⓘ
historicalPeriod 19th century ⓘ
mathematicalForm first-order ordinary differential equations ⓘ
namedAfter Carl Friedrich Gauss ⓘ
relatedTo Lagrange’s planetary equations ⓘ
variation of parameters method ⓘ
relates perturbing accelerations to rates of change of orbital elements ⓘ
requires gravitational parameter of central body ⓘ
usedFor analytical orbit perturbation analysis ⓘ
effect of atmospheric drag on low Earth orbits ⓘ
effect of non-gravitational forces on orbits ⓘ
effect of solar radiation pressure on orbits ⓘ
effect of third-body perturbations ⓘ
long-term orbital evolution studies ⓘ
spacecraft trajectory design ⓘ
usedIn long-term stability analysis of planetary systems ⓘ
mission analysis ⓘ
orbit determination ⓘ
uses normal perturbing acceleration ⓘ
perturbing acceleration components ⓘ
radial perturbing acceleration ⓘ
transverse perturbing acceleration ⓘ

How these facts were elicited

Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Carl Friedrich Gauss → hasConceptNamedAfter → Gauss’s planetary equations ⓘ
Lagrange’s planetary equations → canBeWrittenIn → Gauss’s form of planetary equations ⓘ
linked to: Gauss’s planetary equations
Lagrange’s variation of parameters method → relatedTo → Gauss’s form of the planetary equations ⓘ
linked to: Gauss’s planetary equations