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— CH. 1 · INTRODUCTION —

Invariable plane

~3 min read · Ch. 1 of 5
5 sections
  • The invariable plane is a hidden reference frame at the heart of our Solar System. It passes through the barycenter, the true center of mass, perpendicular to the system's total angular momentum vector. French astronomer Pierre-Simon Laplace identified this concept, and it bears his name in two related but distinct forms that are easy to confuse. The first question worth sitting with is this: in a system as chaotic as orbiting planets, how can anything be truly "invariable"? The answer turns out to depend almost entirely on four giant worlds, and on what we choose to ignore.

  • Pierre-Simon Laplace gave his name to two related but distinct astronomical concepts, and mixing them up is a genuine pitfall. The invariable plane, sometimes called the "Laplacian plane" or the "plane of maximum areas," is fixed for the entire planetary system. It derives from the sum of all angular momenta across every body in the system. The Laplace plane is different. It refers to the plane around which an individual satellite's orbital plane precesses. The two planes are equivalent only in the special case where all perturbers and orbital resonances are far from the precessing body. Laplace's own name for the invariable plane was the "plane of maximum areas," where "area" meant the product of a body's radius, its radial velocity, and its mass. That framing captures something geometrically intuitive: the plane that maximizes the spread of orbital sweeping across all bodies at once.

  • Jupiter contributes 60.3% of the Solar System's total angular momentum, more than all other bodies combined. Saturn follows at 24.5%, Neptune at 7.9%, and Uranus at 5.3%. Together the four giant planets account for about 98% of the system's angular momentum. The invariable plane sits within 0.5 degrees of Jupiter's own orbital plane, calculated precisely at 0.3219 degrees. The Sun itself forms a counterbalance to the planets. When Jupiter sits on one side and the other three giant planets are diametrically opposite, the Sun sits near the barycenter. But when all four giant planets align on the same side, the Sun shifts as far as 2.17 solar radii away from the barycenter. The Sun, all non-giant planets, moons, small bodies, and the axial rotations of every object including the Sun itself add up to only about 2% of the total.

  • A perfectly invariable plane would require every body to be a point mass or a perfectly spherical rigid body, and the Milky Way's gravity would need to be perfectly uniform. None of those conditions hold exactly. Real bodies are non-spherical, and tidal friction allows a small transfer of angular momentum from axial rotation into orbital revolution. This shifts both the magnitude and the direction of orbital angular momentum through precession, because rotational axes are not parallel to orbital axes. The data show how this plays out across time. In the year 2009, Jupiter sat 0.32 degrees from the invariable plane; by the year 168000, its inclination will be 0.23 degrees. Saturn moves from 0.93 degrees in 2009 to 1.01 degrees at year 168000. Uranus shifts from 1.02 degrees to 1.12 degrees. These deviations are exceedingly small relative to the system's total momentum. External torques from passing stars and Milky Way galactic tides exist but are tinier still.

  • For most practical work in Newtonian dynamics, the invariable plane can be treated as a genuine inertial frame of reference. The total angular momentum of the Solar System is very nearly conserved despite tidal friction, ejected material, gravitational waves leaving the system, and gravitational nudges from neighboring stars. The plane defined by the giant planets' orbits alone is stable enough for almost all purposes. This near-invariability makes the plane a useful anchor for long-term orbital simulations, where researchers need a fixed reference that does not drift with the choice of any single planet's orbit. The inclination data measured at year 142400 show Neptune at 0.55 degrees from the plane, a value that matches the year 168000 projection as well, suggesting the outer planets settle into relatively stable oscillations around this shared reference.

Common questions

What is the invariable plane of the Solar System?

The invariable plane is the plane passing through the Solar System's barycenter, perpendicular to its total angular momentum vector. It represents the weighted average of all planetary orbital and rotational planes and is also called Laplace's invariable plane.

Who is the invariable plane named after?

The invariable plane is named after the French astronomer Pierre-Simon Laplace, who called it the "plane of maximum areas." Laplace defined the "area" as the product of a body's orbital radius, its radial velocity, and its mass.

What is the difference between the invariable plane and the Laplace plane?

The invariable plane is fixed for the entire planetary system and is derived from the sum of all angular momenta across every body. The Laplace plane is specific to individual satellites and describes the plane around which a satellite's orbital plane precesses. The two are equivalent only when all perturbers and resonances are far from the precessing body.

How close is the invariable plane to Jupiter's orbital plane?

The invariable plane lies within 0.5 degrees of Jupiter's orbital plane, calculated at precisely 0.3219 degrees. Jupiter contributes 60.3% of the Solar System's total angular momentum, making it the dominant influence on the plane's orientation.

Which planets contribute most to the Solar System's angular momentum?

The four giant planets contribute about 98% of the Solar System's angular momentum. Jupiter leads at 60.3%, followed by Saturn at 24.5%, Neptune at 7.9%, and Uranus at 5.3%.

Why is the invariable plane not perfectly invariable?

Real bodies are non-spherical, and tidal friction allows a small transfer of angular momentum from axial rotation into orbital revolution. External influences such as Milky Way galactic tides and passing stars also exert tiny torques. These effects cause small changes in both the magnitude and direction of angular momentum, though the changes are exceedingly small relative to the system's total momentum.

All sources

5 references cited across the entry

  1. 1journalSatellite dynamics on the Laplace surfaceTremaine, S. et al. — 2009
  2. 2bookCelestial MechanicsP.-S., Marquis de La Place — 1829
  3. 3journalThe solar system's invariable planeD. Souami et al. — 2012