Class 8- Exospheres II

Reading:

  1. Atmospheres - Goody & Walker - pp 135-139.
  2. New Solar System - p94.
  3. HW3 answers.

What is an Exosphere?

Definition: The exosphere of an atmosphere is where the mean free path for collisions is MORE than a scaleheight.

Mean Free Path

Click on these notes to see larger versions.

 

 

Sources Processes

Diffusion - out of the regolith - important for light and inert gases - H, He, Ar (primordial? from time of formation?)

Photo-Sputtering, Adsorption and/or Thermal Evaporation

Photons hit the surface and excite atoms, "shaking" them off the surface - or heating them up

Meteoritic Bombardment -> Impact Vaporization

Micro-meteoritic flux at Earth is 120 tons / day! That's 40 +-20 million kg / year.

Ion Sputtering - Ion Implantation

Solar wind (H+, He2+, O6+, Fe8+, C4+...) impact Mercury and the Moon at 300 km/s. Ions are implanted into the surface layers - and then are sputtered off again or evaporated. Sputtering is just what it sounds like - energetic ions bombard the surface and knock off a spray of atoms at lower energies.

 

Loss Processes

Photo-Ionization

e.g. Na + photon -> Na+ + e- which, being charged, are swept away in the solar wind.

Charge Exchange

e.g. solar wind H+ + Na -> Na+ + H* the Na+ is swept away, the H* is an energetic neutral hydrogen atom, it keeps its original 300 km/s

Radiation Pressure

e.g. photon hits Na atom and bounces off - delivering momentum. Na atom moves away from the Sun.

Jeans (Thermal) Escape

When a gas atom has more speed than the escape speed, it escapes. In any distribution of atoms or molecules in a gas, there will be a fraction that is greater than the escape speed of the Moon, Mercury - or whatever object.

Thermal Speed

In a gas that is in thermal equilibrium (lots of collisions to distribute the energy) they have a Maxwell-Boltzmann distribution of energies - and speeds.

 

There is a most probable speed - sometimes called thermal speed - which is

Vo = (2kT/m)1/2

where m = molecular mass = <A> mp (<A> = molecular mass in a.m.u., mp = mass of proton)

The fraction with speeds greater than V is....

Fig 6-3

So, an atom or molecule is more likely to escape - V > Vescape - if

 

Special Case of the Galilean Satellites

The Galilean satellites are embedded in the magnetosphere of Jupiter

The atmospheres of Callisto, Ganymede and Europa come from the bombardment of their icy surfaces by energetic particles. Ion implantation, ion sputtering, ionization, charge-exchange - the works!

 

... which leads us to Io next week. And Pluto and Triton.