Determination of the size, mass, and density of "exomoons" from photometric transit timing variations
A. Simon, K. Szatmary, G.M. Szabo

TL;DR
This paper introduces a method using photometric transit timing variations ($TTV_p$) to estimate the size, mass, and density of exomoons from transit data, validated through simulations of the Earth-Moon system.
Contribution
It presents a novel $TTV_p$ analysis technique that predicts exomoon size and mass more accurately than previous methods, including approximations for unknown density ratios.
Findings
Estimated Moon size within 20% of real value using real density ratio.
Predicted Moon mass within a factor of 2 assuming equal densities.
Method improves exomoon parameter estimation from transit data.
Abstract
Precise photometric measurements of the upcoming space missions allow the size, mass, and density of satellites of exoplanets to be determined. Here we present such an analysis using the photometric transit timing variation (). We examined the light curve effects of both the transiting planet and its satellite. We define the photometric central time of the transit that is equivalent to the transit of a fixed photocenter. This point orbits the barycenter, and leads to the photometric transit timing variations. The exact value of depends on the ratio of the density, the mass, and the size of the satellite and the planet. Since two of those parameters are independent, a reliable estimation of the density ratio leads to an estimation of the size and the mass of the exomoon. Upper estimations of the parameters are possible in the case when an upper limit of is known.…
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