SETI public: On the migration-induced resonances in a system of two planets with masses in th

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Paper: astro-ph/0507611
Date: Tue, 26 Jul 2005 16:34:07 GMT (2167kb)

Title: On the migration-induced resonances in a system of two planets with
masses in the Earth mass range

Authors: J. C. B. Papaloizou (QMUL, London and DAMPT, Cambridge) and E.
Szuszkiewicz (Institute of Physics and CASA*, University of Szczecin)
Comments: 26 pages with 19 low resolution Postscript figures, abstract
abridged, accepted for publication in MNRAS
\\
We investigate orbital resonances expected to arise when a system of two
planets, with masses in the range 1-4 Earth masses, undergoes convergent
migration while embedded in a section of gaseous disc where the flow is
laminar. We consider surface densities corresponding to 0.5-4 times that
expected for a minimum mass solar nebula at 5.2 AU. Using hydrodynamic
simulations we find that when the configuration is such that convergent
migration occurs the planets can become locked in a first order
commensurability for which the period ratio is (p+1)/p with p being an
integer
and migrate together maintaining it for many orbits. Relatively rapid
convergent migration as tends to occur for disparate masses, results in
commensurabilities with p larger than 2. However, in these cases the
dynamics
is found to have a stochastic character. When the convergent migration is
slower, such as occurs in the equal mass case, lower p commensurabilities
such
as 3:2 are attained which show much greater stability. In one already known
example of a system with nearly equal masses in the several Earth mass range
(planets around pulsar PSR B1257+12) the two largest planets are
intriguingly
close to a 3:2 commensurability. A very similar behaviour is obtained when
the
systems are modeled using an N body code with simple prescriptions for the
disc
planet interaction. Using that, we found that an 8:7 resonance established
in a
hydrodynamic simulation run for 10-100 thousand orbits could be maintained
for
more than million orbits. Resonant capture leads to a rise in eccentricities
that can be predicted using a simple analytic model constructed in this
paper.
We find that the system with the 8:7 commensurability is fully consistent
with
this prediction.

\\ ( http://arXiv.org/abs/astro-ph/0507611 , 2167kb)

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