Lagrange point
Lagrange points are stable positions near large bodies in orbit. When two large bodies are in orbit around each other, there are places that a third body can occupy. Lagrange points are found in the orbits of Earth and the Sun, or the Moon and the Earth.[1] The most well-known natural occupants of Lagrange points are Trojan asteroids.
The points are five places where a small object (such as a man-made satellite) can orbit. At those points, the gravitational forces of the two large bodies and forces due to motion all balance up. So, at those places, a small object keeps more or less in a stable position. Dust clouds, asteroids, and man-made satellites are found in those points.
This effect is named after the mathematician Joseph-Louis Lagrange, who wrote a paper on this in 1772 (long before we put satellites into orbit).
The five places are called L1, L2, L3, L4 and L5. The first three (L1, L2, L3) are called metastable because if a satellite gets a bit out of place, it will fall away from that point, and not come back without using fuel. L4 and L5 are considered stable - if a satellite gets a bit out of place, it will be pulled back into place by the gravity and centripetal forces, and oscillate around the Lagrange point. This can result in very wide swings around L4 and L5, sometimes called by such names as "tadpole" and "horseshoe" orbits.
NASA has inserted satellites into two Lagrange points of the Sun-Earth system. The L1 point (between the Earth and the sun) is used for satellites in a halo orbit to watch the sun, looking for solar flares. The L2 point (beyond the Earth) is used for space telescopes such as the James Webb Space Telescope launched on 25 December 2021. It is a million miles (about 1.5 million kilometers) from Earth.[2]
Because L4 and L5 are stable, they have attracted dust clouds. The Earth-Sun system has attracted a few asteroids and the bigger planets have more and larger ones. These asteroids are called Trojan asteroids.[3]
Lagrange Point Media
Lagrange points in the Sun–Earth system (not to scale). This view is from the north, so that Earth's orbit is counterclockwise.
Gravitational accelerations at Template:L4
Lagrangian points equipotential
Net radial acceleration of a point orbiting along the Earth–Moon line
STL 3D model of the Roche potential of two orbiting bodies, rendered half as a surface and half as a mesh
Sun–planet Lagrange points to scale (Click for clearer points.)
The satellite ACE in an orbit around Sun–Earth Template:L1
References
- ↑ "Lagrange points". NASA. Retrieved 14 May 2013.
- ↑ "James Webb Space Telescope". NASA. Retrieved 14 May 2013.
- ↑ "Earth's Trojan asteroid". NASA. Archived from the original on 24 May 2013. Retrieved 14 May 2013.