The pressure when the volume is reduced to 0.42 L is (y - b) ÷ m.
What is pressure?Pressure is the force per unit area applied to a surface or object. In the physical sciences, pressure is a measure of the force exerted on a surface by a fluid, such as a gas or liquid. Pressure is the result of the weight of the fluid pushing down on a surface. In physics, pressure is often expressed as the ratio of force to area. Pressure is typically measured in units of pascals (Pa) or pounds per square inch (psi). Pressure can also be measured in atmospheres (atm), bars, or torr.
The equation for the line representing the relationship between Volume (L) and (1/pressure) is y = mx + b, where m is the slope and b is the y-intercept.
Since we know the Volume (L) is 0.42, we can use this value to solve for the pressure.
Using the equation, we can calculate the pressure by solving for x:
x = (y - b) ÷ m
Therefore, the pressure when the volume is reduced to 0.42 L is (y - b) ÷ m.
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the inner planets of the solar system are rocky whereas the outer planets contain a higher proportion of ice and gas. this differentiation occurred in the early solar system because:
The differentiation, that the inner planets of the solar system are rocky while the outer planets contain a higher proportion of ice and gas, occurred in the early solar system due to the temperature gradient in the protoplanetary disk.
This occurs because in the inner regions of the disk, temperatures were too high for volatile elements such as hydrogen and helium to condense, while in the outer regions, temperatures were low enough for these elements to condense, forming the gas and ice giants.
In addition, due to the increased gravity in the inner regions of the disk, heavier elements, such as metals and rocks, were able to accumulate more easily, leading to the formation of the terrestrial planets.
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