Calculating KE of Ideal Gases: Understanding its Independence from Molecule Mass

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Discussion Overview

The discussion revolves around the kinetic energy (KE) of ideal gases and its independence from the mass of the molecules. Participants explore the implications of the ideal gas law, the relationship between temperature and kinetic energy, and the behavior of gas molecules of varying masses.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant notes that the formula for kinetic energy of ideal gases suggests it is independent of molecular mass, prompting questions about the implications of this independence.
  • Another participant illustrates that in a mixed system of balls with different masses, each ball will have the same average kinetic energy, regardless of mass differences.
  • A participant proposes that while the kinetic energy calculated by the formula remains constant, heavier molecules must have lower velocities to maintain the same energy, suggesting a nuanced understanding of the relationship between mass and energy.
  • One participant explains that gas properties are defined by pressure and temperature, with temperature representing mean energy per unit quantum, and discusses how heavier molecules move slower to maintain equivalent energy levels as lighter ones.
  • Another participant introduces the concept of non-ideal gases, mentioning that energy can be tied up in rotational modes, affecting specific heat ratios.
  • A later reply references the equipartition theorem, explaining how energy is distributed among degrees of freedom in thermal equilibrium, which further complicates the understanding of kinetic energy in different types of molecules.

Areas of Agreement / Disagreement

Participants express varying interpretations of the relationship between kinetic energy, mass, and temperature, with some agreeing on the independence of kinetic energy from mass while others explore the implications of this relationship. The discussion remains unresolved with multiple competing views present.

Contextual Notes

Participants mention concepts such as equipartition of energy and the behavior of non-ideal gases, which introduce additional complexity to the discussion. The implications of molecular mass on kinetic energy and velocity are not fully resolved, indicating a need for further exploration.

apache
when you equate the two formulas for ideal gases, one is evetually left with a formula to calculate the ke. of the ideal gas (3/2kt i think) how come the ke is independent of the mass of the molecule ?
 
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If you mix many balls with different mass in a box and shake the box, each ball will have the same average kinetic energy regardless difference in their mass.
 
wait... i got an idea, does the formula mean that although the ke. will be what the formula spits out, the velocities for heavier moleules (lets say of another ideal gas) would be lower, and thus the formula would be indepndent of mass.. ?
 
Yes.
 
A simple way to see it.

The gas properties are defined by the pressure and temperature. The temperature is basically the mean energy per unit quantum, in this case atoms or molecules are the "quanta" involved, (this isn't the standard definition of quantum) and the pressure is the mean energy per unit volume. The heavier molecules move slower to have the same energy as the lighter ones.

In non-ideal gasses some of the energy is tied up in rotational modes, which is why they have differing ratios of specific heat.
 
thanks guys,
i think i finally got it !
 
Mobility of elastic gases

Originally posted by apache
thanks guys,
i think i finally got it !

Hi apache,
I am attaching the table referred to below with the hope that the narrow field of this posting causes scrambling.

VERTICAL MOBILITIES of ATMOSPHERIC GASES

The Mobilities according to Graham’s law are listed in the table above as referenced to the mobility of N2, the major molecular constituent of the atmosphere. Positive factors indicate propensities of given gases to rise while negative factors indicate falling tendencies. Those labeled “gas” are usually Brownian gases in that their boiling points are above ambient atmospheric temperatures. For example when solid Iodine sublimes, a maroon cloud hovers nearby until dispersed and/or condensed. It should be remembered that volatility is a function of boiling point temperature as contrasted with mobility, which is the inverse square root of the molecular mass.
 

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Last edited:


Originally posted by Tyger
The temperature is basically the mean energy per unit quantum, in this case atoms or molecules are the "quanta" involved, (this isn't the standard definition of quantum) and the pressure is the mean energy per unit volume...

In non-ideal gasses some of the energy is tied up in rotational modes, which is why they have differing ratios of specific heat.

Standard postulate here is "In thermal equilibrium energy is equally distributed among all available degrees of freedom (equipartition)", so temperature T is defined in such way that each degree has in the average kT/2 amount of energy. If a molecule is monoatomic, it has 3 degrees only(x,y,z), thus <E>=3kT/2, if diatomic then it has two more (rotational) degrees, thus <E>=5kT/2, and so on.
 

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