Science Olympiad Dynamic Planet 2025 – 400 Free Practice Questions to Pass the Exam

Rodinia's formation is primarily attributed to the accretion and collision of landmasses. During the Proterozoic Eon, the landmasses on Earth were not as stable or fixed as they are today. Rather, they were dynamic and experienced significant geological processes. The process of accretion involves smaller landmasses merging together, forming larger continental structures due to tectonic forces.

Additionally, during the time of Rodinia's formation, the tectonic plates were more actively converging, leading to major collisions of continental blocks. These collisions caused the landmasses to crumple and fold, creating the vast, interconnected expanse of land that we recognize as a supercontinent. This process resulted in significant geological features, such as mountain ranges, which are indicative of the intense tectonic activity during that era.

While other processes listed in the choices, such as volcanic activity, seafloor spreading, and glacial shifts, certainly played important roles in Earth's geology over different periods, they do not directly explain the primary mechanism behind the formation of Rodinia. Volcanic activity might contribute to landmass development but does not account for the large-scale assembly that characterizes supercontinent formation. Seafloor spreading primarily relates to the