Planetary migration is a theoretical process that proposes that planets can change or migrate from their original orbits over time due to various gravitational interactions and forces acting upon them. This concept has been proposed as a potential explanation for the surprising orbits observed in many extrasolar planets (planets outside our solar system) discovered by astronomers.
The process of planetary migration can occur in different ways:

1. Type I migration: This applies to low-mass planets, such as Earth-like or super-Earth planets, embedded in a protoplanetary disk (the rotating disk of gas and dust surrounding a young star). These planets can exchange angular momentum with the disk material, causing them to spiral inward or outward from their initial orbits.
2. Type II migration: This process involves more massive planets, like Jupiter or Saturn, which open a gap or cavity in the protoplanetary disk. The gravitational interactions between the planet and the disk material can cause the planet to migrate inward or outward, depending on the disk’s properties and the planet’s mass.
3. Planet-planet scattering: In this scenario, gravitational interactions between multiple planets in a system can lead to close encounters or collisions, causing one or more planets to be scattered onto highly eccentric (elongated) or inclined orbits.

Planetary migration may account for the surprising orbits of many extrasolar planets in the following ways:

1. Hot Jupiters: These are gas giant planets that orbit extremely close to their parent stars, much closer than the orbit of Mercury in our solar system. Planetary migration can explain how these massive planets ended up in such tight orbits after initially forming much farther out.
2. Eccentric and inclined orbits: Many extrasolar planets have been found with highly eccentric or inclined orbits, which are difficult to explain by the traditional models of planet formation. Planet-planet scattering and migration can produce such orbits.
3. Retrograde orbits: Some extrasolar planets have been discovered orbiting in the opposite direction to the rotation of their host stars, known as retrograde orbits. Planetary migration and scattering events can potentially produce these unusual orbits.

While planetary migration is a theoretical concept, it has gained acceptance as a plausible explanation for the observed diversity of exoplanetary systems, which often differ significantly from the architecture of our own solar system. However, further research and observations are still needed to fully understand the processes and mechanisms involved in planetary migration.