3.4 The Jeans mass for fragmentation
The typical mass of a planet formed through fragmentation can be estimated starting from the definition of its Jeans mass. The Jeans criterion states that a gas cloud will collapse if the cloud’s kinetic energy is less than the magnitude of its gravitational energy; the minimum mass of a gas cloud for which the Jeans criterion is met is known as the Jeans mass. For the geometry of a protoplanetary disc, the Jeans mass in terms of the surface density is

where T and
are the temperature and mean molecular mass of the gas. Noting that the sound speed is given by
(Equation 3), so the Jeans mass may be written as

Using Q = 1 to express the surface density Σ for a disc that is just becoming unstable (Equation 22) this becomes:

Then, recognising that
(Equation 6) and
(Equation 2), we have


Therefore, this gives the final result:

-
Estimate the Jeans mass for a typical disc with H/r = 0.05, centred on a Sun-like star.
-
Inserting values into Equation 25:


(This is about 1.6 Jupiter masses.)
OpenLearn - The formation of exoplanets
Except for third party materials and otherwise, this content is made available under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 Licence, full copyright detail can be found in the acknowledgements section. Please see full copyright statement for details.