Answer:
1. Both Pluto and Eris are SMALLER than any of the terrestrial planets.
2. Both Pluto and Eris travel in MORE ELLIPTICAL orbits than any of the terrestrial or Jovian planets.
3. Both Pluto and Eris are LESS MASSIVE than any of the terrestrial or jovian planets.
Explanation:
All the above-mentioned options are the differences between Pluto, Eris and other terrestrial and Jovian planets in our solar system.
Some characteristics of Pluto include:
- It has a mass of
- It has a diameter of 2,370 km (1,473 miles)
- It has five (5) moons (Charon, Nix, Hydra, Kerberous, and Styx)
Some characteristics of Eris include the following:
- It has one moon (Dysomia)
- It has a radius of 1,163 km (722 miles)
- It takes 557 earth years to make one trip around the sun.
Answer:
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Answer:Resources such as rocks, soil, water, and air, nonliving things that help to meet our needs. This lesson focuses on students learning about Earth's Resources. They learn that water and air are renewable resources that can be replaced quickly. They learn that soil and rocks are non-renewable and they cannot be replaced quickly.
Explanation:
Answer:
Divergent boundaries such as the mid-oceanic ridge system.
Explanation:
Divergent boundaries occur when plate boundaries pull away from each other. Molten rock or magma rise from the gap between the two plates, rising up to the sea floor where it cools down to form new crust. It is the mid-ocean ridges where you see the most magma produced and there has not been any other tectonic event or area that could match its procution since the Precambrian period.
