Andrew Prentice Explained

Andrew Prentice is an Australian mathematician. He is known for developing an alternative model of planetary formation. In contrast to the conventional model where planetary accretion occurs within a continuous disk, according to Prentice's "Modern Laplacian Theory" each planet accretes within a discrete circumsolar gas ring.[1] Prentice's nested gas rings arise due to the effect of 'supersonic turbulent convection' in slowing the infall of interstellar dust and gas. Instead of collapsing directly to form a flat continuous disk, due to 'turbulent stress' the gas temporarily remains puffed up in a vast rotating spheroidal atmosphere around the protosolar core. This atmosphere spins faster as it slowly contracts. It rids itself of excess angular momentum by sequentially shedding gas rings from its equator. The same process repeats itself on a much smaller scale for each of the giant planets to produce their regular satellite systems. Prentice has used his unorthodox model to make a range of surprisingly accurate predictions about the Solar System. He is currently Emeritus Professor in the School of Mathematical Sciences at Monash University.[2]

Lecturing style

Andrew Prentice was a member of the lecturing staff at Monash University, Clayton; he received a Vice-Chancellor's Award for Teaching Excellence in 2011.[3]

Predictions

In 2014 the ALMA radio telescope started observing the inner regions around young stars,[4] such as HL Tauri and AS 209,where planets were thought to be forming. To the surprise of the astronomical community ALMA found that most of these stars are encircled by sets of concentric rings, similar to those described by Prentice in 1978,[5] rather than continuous disks.

Prentice has made a long list of controversial predictions about the nature of our Solar System in an attempt to demonstrate the validity of his Modern Laplacian Theory. Critics have dismissed the theory pointing out that the convectively driven 'supersonic turbulence' proposed by Prentice is theoretically impossible and that his gas rings would be dynamically unstable, but to the surprise of many of his colleagues, NASA missions have confirmed that many of his deductions from the theory were remarkably accurate. Some of his best known predictions are:[6]

Selected works

External links

Notes and References

  1. Prentice, A.J.R.. 1978. Origin of the solar system – I: Gravitational contraction of the turbulent protosun and the shedding of a concentric system of gaseous laplacian rings. The Moon and the Planets. 19. 3. 341–398. 10.1007/bf00898829. 1978M&P....19..341P . 123376299.
  2. Web site: CSPA Staff: Andrew Prentice . 20 November 2013 . https://web.archive.org/web/20140319070049/http://mdsadmin-new.monash.edu.au/cgi-bin/staffsearch/staffsearch?name=Andrew%20Prentice . 19 March 2014 . dead .
  3. Web site: Outstanding Staff Honoured. 26 October 2011. Monash University.
  4. Web site: ALMA Campaign Provides Unprecedented Views of the Birth of Planets | ALMA .
  5. Prentice, A.J.R.. 1978. Origin of the solar system – I: Gravitational contraction of the turbulent protosun and the shedding of a concentric system of gaseous laplacian rings. The Moon and the Planets. 19. 3. 341–398. 10.1007/bf00898829. 1978M&P....19..341P . 123376299.
  6. http://www.monash.edu.au/pubs/monmag/issue13-2004/research/stars.html Journey to the origin of the Solar System (Monash Magazine article)