Thermal effects of circumplanetary disc formation around proto-gas giant planets

Research output: Contribution to journalArticle

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Abstract

The formation of a circumplanetary disc and accretion of angular momentum on to a protoplanetary system are investigated using three-dimensional hydrodynamical simulations. The local region around a protoplanet in a protoplanetary disc is considered with sufficient spatial resolution: the region from outside the Hill sphere to the Jovian radius is covered by the nested-grid method. To investigate the thermal effects of the circumplanetary disc, various equations of state are adopted. Large thermal energy around the protoplanet slightly changes the structure of the circumplanetary disc. Compared with a model adopting an isothermal equation of state, in a model with an adiabatic equation of state, the protoplanet's gas envelope extends farther, and a slightly thick disc appears near the protoplanet. However, different equations of state do not affect the acquisition process of angular momentum for the protoplanetary system. Thus, the specific angular momentum acquired by the system is fitted as a function only of the protoplanet's mass. A large fraction of the total angular momentum contributes to the formation of the circumplanetary disc. The disc forms only in a compact region in very close proximity to the protoplanet. Adapting the results to the Solar system, the proto-Jupiter and Saturn have compact discs in the region of r < 21r Jup(r < 0.028 rH,Jup) and r < 66rSat(r < 0.061rH,Sat), respectively, where rJup(r H,Jup) and rSat(rH,Sat) are the Jovian and Saturnian (Hill) radius, respectively. The surface density has a peak in these regions due to the balance between centrifugal force and gravity of the protoplanet. The size of these discs corresponds well to the outermost orbit of regular satellites around Jupiter and Saturn. Regular satellites may form in such compact discs around proto-gas giant planets.

Original languageEnglish
Pages (from-to)514-524
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume392
Issue number2
DOIs
Publication statusPublished - Jan 1 2009
Externally publishedYes

Fingerprint

gas giant planets
temperature effect
protoplanets
temperature effects
planet
equation of state
angular momentum
gas
Saturn
Jupiter
equations of state
Jupiter (planet)
solar system
adiabatic equations
spatial resolution
accretion
gravity
centrifugal force
radii
protoplanetary disks

All Science Journal Classification (ASJC) codes

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Thermal effects of circumplanetary disc formation around proto-gas giant planets. / Machida, Masahiro.

In: Monthly Notices of the Royal Astronomical Society, Vol. 392, No. 2, 01.01.2009, p. 514-524.

Research output: Contribution to journalArticle

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