SOLAR SYSTEM

Detailed explanation-1: -Emergence of planets. Two processes are important in planet formation. Condensation is the production of solid dust grains as gases in the molecular cloud cool, and accretion is the collision of the dust grains to form clumps and progressively larger bodies, some of which grow into planets (Fig.

Detailed explanation-2: -Accretion is the process in which material from the outer plate and trench (during the periods of discontinuous subduction) is removed and added to the outer continental margin or by other mechanisms such as imbricate thrusting or a combination of folding and thrusting (Karig, 1974; Karig and Sherman, 1975).

Detailed explanation-3: -This process is called accretion. The objects formed by accretion are called planetesimals (small planets): they act as seeds for planet formation.

Detailed explanation-4: -Within the solar nebula, scientists believe that dust and ice particles embedded in the gas moved, occasionally colliding and clumping together. Through this process, called “accretion, ‘’ these microscopic particles formed larger bodies that eventually became planetesimals with sizes up to a few kilometers across.

Detailed explanation-5: -In this context, accretion refers to the process of cooled, solidified grains of dust and ice orbiting the protostar in the protoplanetary disk, colliding and sticking together and gradually growing, up to and including the high-energy collisions between sizable planetesimals.