The formula is:
T = PV/nR,
Where:
* T is the temperature in kelvin
* P is the pressure in atmospheres
* n is the number of moles
* R is the gas constant
From PV = nRT you solve for n (moles). Thus, n = PV/RT
From PV = nRT you solve for n (moles). Thus, n = PV/RT
(Explanation) this is simply taking the ideal gas law PV=nRT, and dividing by P on both sides to isolate the V, kinda like solving an algebra problem
if you were traveling to the earths core, what would you see and what would the temperature be?
All bond will break at high temperature; in another word, bond will not form more quickly in higher temperature but instead it form at low temperature.
The formula is: T = PV/nR, Where: * T is the temperature in kelvin * P is the pressure in atmospheres * n is the number of moles * R is the gas constant
The formula is: T = PV/nR, Where: * T is the temperature in kelvin * P is the pressure in atmospheres * n is the number of moles * R is the gas constant
V=nRT/P
From PV = nRT you solve for n (moles). Thus, n = PV/RT
(Explanation) this is simply taking the ideal gas law PV=nRT, and dividing by P on both sides to isolate the V, kinda like solving an algebra problem
From PV = nRT you solve for n (moles). Thus, n = PV/RT
Make V explicit in the general for of the gas law: P.V = n.R.T then you get V = (n.R.T) / P
From PV = nRT you solve for n (moles). Thus, n = PV/RT
From PV = nRT you solve for n (moles). Thus, n = PV/RT
From PV = nRT you solve for n (moles). Thus, n = PV/RT
From PV = nRT you solve for n (moles). Thus, n = PV/RT
(Explanation) this is simply taking the ideal gas law PV=nRT, and dividing by P on both sides to isolate the V, kinda like solving an algebra problem