  We have carried out an extensive study of the possibility of the detection of
Earth-mass and super-Earth Trojan planets using transit timing variation method
with the Kepler space telescope. We have considered a system consisting of a
transiting Jovian-type planet in a short period orbit, and determined the
induced variations in its transit timing due to an Earth-mass/super-Earth
Trojan planet. We mapped a large section of the phase space around the 1:1
mean-motion resonance and identified regions corresponding to several other
mean-motion resonances where the orbit of the planet would be stable. We
calculated TTVs for different values of the mass and orbital elements of the
transiting and perturbing bodies as well as the mass of central star, and
identified orbital configurations of these objects (ranges of their orbital
elements and masses) for which the resulted TTVs would be within the range of
the variations of the transit timing of Kepler's planetary candidates. Results
of our study indicate that in general, the amplitudes of the TTVs fall within
the detectable range of timing precision obtained from the Kepler's
long-cadence data, and depending on the parameters of the system, their
magnitudes may become as large as a few hours. The probability of detection is
higher for super-Earth Trojans with slightly eccentric orbits around
short-period Jovian-type planets with masses slightly smaller than Jupiter. We
present the details of our study and discuss the implications of its results.
