A student is creating a model to compare and contrast different objects in the Solar System in the model most of which objects in the Solar System will be found in a belt between Mars and Jupiter.
In the model, the student can include the following objects that are commonly found in the asteroid belt between Mars and Jupiter:
1. Asteroids: These are rocky and metallic remnants from the early formation of the Solar System. They vary in size and composition, ranging from small rocks to dwarf planets like Ceres.
2. Ceres: As the largest object in the asteroid belt, Ceres is considered a dwarf planet. It is composed of a rocky core covered by an icy mantle and may have subsurface liquid water.
3. Vesta: It is the second-largest object in the asteroid belt and is known for its large impact crater, Rheasilvia. Vesta is rocky and consists of a differentiated interior with a metallic core.
4. Pallas, Hygiea, and other large asteroids: These are some of the larger asteroids located in the belt. They have distinct shapes and compositions, with Pallas being the third-largest asteroid in the belt.
5. Other smaller asteroids: The asteroid belt contains numerous smaller asteroids that vary in size and composition. Some may have irregular shapes, while others can be more spherical in nature.
By including these objects in the model, the student can visually compare and contrast their sizes, appearances, and compositions. Additionally, they can highlight the unique characteristics of each object and discuss their significance in the Solar System's evolution.