Question

the table below shows data on the average density and composition of planets in our solar system. type example density (g/cm³) composition terrestrial earth 5.5 rock, metal jovian jupiter 1.3 gas, ice dwarf pluto 2.0 ice, rock based on the data, what trend do you notice about planetary density and composition? how does this relate to the location of planets in the solar system?

Explanation:

Step1: Analyze density values

The terrestrial planet (Earth) has a density of 5.5 g/cm³, the Jovian planet (Jupiter) has a density of 1.3 g/cm³ and the dwarf - planet (Pluto) has a density of 2.0 g/cm³. Terrestrial planets are denser, mainly composed of rock and metal. Jovian planets are less dense, composed of gas and ice. Dwarf - planets have intermediate density and are composed of ice and rock.

Step2: Relate to solar - system location

Terrestrial planets are closer to the Sun. The high temperatures near the Sun allowed only heavier elements like rock and metal to condense, forming dense planets. Jovian planets are farther from the Sun, where it is colder, allowing lighter elements like hydrogen and helium to condense, forming less - dense gas and ice planets. Dwarf - planets like Pluto are in the outer regions and have a mix of ice and rock, with an intermediate density.

Answer:

The trend in planetary density and composition is that terrestrial planets close to the Sun are dense and composed of rock and metal, Jovian planets farther out are less dense and composed of gas and ice, and dwarf - planets in the outer regions have intermediate density and are composed of ice and rock. This relates to location as the proximity to the Sun affects the types of elements that can condense to form planets, with high temperatures near the Sun favoring the formation of dense, rocky planets and lower temperatures in the outer regions allowing for the formation of less - dense gas and ice planets.