ग्रह प्राणी,

planetesimals's Usage Examples:

streaming instability is a hypothetical mechanism for the formation of planetesimals in which the drag felt by solid particles orbiting in a gas disk leads.

Alternatively, the planetesimals in this system may have unusual physical properties.

also be produced and maintained as the remnants of collisions between planetesimals, otherwise known as asteroids and comets.

disk phase and the inclusion of gravitational interactions between planetesimals in the outer disk into the model.

Jan Oort, is a theoretical concept of a cloud of predominantly icy planetesimals proposed to surround the Sun at distances ranging from 2,000 to 200.

Protoplanets are thought to form out of kilometer-sized planetesimals that gravitationally perturb each other"s orbits and collide, gradually.

The more massive planetesimals accrete some smaller ones, while others shatter in collisions.

This process continues until the planetesimals interact.

Millions of asteroids exist: many are shattered remnants of planetesimals.

natural satellites, meteoroids, comets, planetesimals and circumstellar disks.

temperatures around 190 K and which likely represent small dust grains of sublimating ice from icy planetesimals.

Iron meteorites originate from cores of planetesimals.

During the formation of the Solar System, there were probably many more (planetesimals), but they have all merged with or been destroyed by the four remaining.

Synonyms:

celestial body, heavenly body,

Antonyms:

artifact,