The Great Escape
Heating Hydrogen to the Limit
Imagine a tiny hydrogen molecule resting on the surface of the Earth. It's jiggling around, possessing a certain amount of kinetic energy due to its temperature. Now, what if we wanted to heat this molecule up so much that its random thermal motion becomes violent enough to break free from Earth's gravitational pull entirely?
This is a classic intersection of Thermodynamics and Gravitation. We are looking for the exact temperature T where the root mean square (RMS) velocity of the gas molecule, vrms, perfectly matches the escape velocity of the Earth, ve.
The Master Equations
From gravitation, we know that the escape velocity from the surface of a planet is given by:
where g is the acceleration due to gravity and Re is the radius of the Earth.
On the other hand, the kinetic theory of gases tells us that the RMS velocity of a gas molecule at an absolute temperature T is:
where kB is the Boltzmann constant and m is the mass of a single molecule.
The Setup and The Trap
Our condition is simple: vrms=ve.
Equating the two expressions and squaring both sides to eliminate the square roots, we get:
Rearranging this to solve for our target variable, the temperature T:
Now, here is where the examiners set a brilliant trap. We need the mass of a single hydrogen molecule, m. Usually, we find this by dividing the molar mass by Avogadro's number (NA=6.02×1023 mol−1).
However, look closely at the units provided in the question: NA=6.02×1026 kg−1. This is not the standard Avogadro's number per mole; it is the number of molecules in a kilomole!
Since the molar mass of H2 is 2 kg/kmol, the mass of a single molecule is simply:
The Final Calculation
Substituting this expression for m back into our temperature equation:
Now, we carefully plug in the given numerical values:
T=3×(1.38×10−23)×(6.02×1026)2×10×(6.4×106)×2
This value is closest to 104 K.
At this blistering temperature, the average hydrogen molecule is zipping around fast enough to escape Earth's gravity forever. This is precisely why our atmosphere retains heavier gases like nitrogen and oxygen, but lighter gases like hydrogen have long since boiled away into space!