We need to calculate the average density of the Sun using its mass and radius to determine its physical state.
Concept: Mass density
The average mass density (ρ) of a spherical object is defined as the ratio of its total mass (M) to its total volume (V). For a sphere of radius R, the volume is given by:
V=34πR3
The density is then:
ρ=VM
Given:
- Mass of the Sun (M) = 2.0×1030 kg
- Radius of the Sun (R) = 7.0×108 m
Solving:
- First, calculate the volume of the Sun:
V=34πR3=34×π×(7.0×108 m)3=34×π×3.43×1026 m3≈1.4×1027 m3
- Next, calculate the average density:
ρ=VM=1.4×1027 m32.0×1030 kg≈1.4×103 kg⋅ m−3
- Comparison with known densities:
- Density of gases (at STP) is approximately 1 kg⋅ m−3.
- Density of liquids (like water) is approximately 1000 kg⋅ m−3.
- Density of solids typically ranges from 1000 kg⋅ m−3 to 20000 kg⋅ m−3.
The calculated density of 1.4×103 kg⋅ m−3 is much higher than that of typical gases and falls within the range of densities for solids and liquids. This high density, despite the high temperature, is due to the intense gravitational attraction pulling the solar plasma toward the center.
Answer
1.4×103 kg⋅ m−3
This value lies in the range of densities of solids and liquids.