# Transits of Inclined Exomoons - Hide and Seek and an Application to   Kepler-1625

**Authors:** David V. Martin, Daniel C. Fabrycky, Benjamin T. Montet

arXiv: 1901.06366 · 2019-04-24

## TL;DR

This paper analyzes the transit probabilities of inclined exomoons, demonstrating that many may frequently avoid transit, which impacts detection strategies and the interpretation of non-transit observations, especially in systems like Kepler-1625.

## Contribution

It provides an analytic equation for exomoon transit probability and explores how orbital inclination and misalignment affect transit detection likelihood.

## Key findings

- Exomoons can often avoid transiting if their orbits are large and misaligned.
- Approximately 40% transit probability for the Kepler-1625 exomoon candidate.
- Multiple non-transits are needed to confidently rule out the exomoon.

## Abstract

A Neptune-sized exomoon candidate was recently announced by Teachey & Kipping, orbiting a 287 day gas giant in the Kepler-1625 system. However, the system is poorly characterized and needs more observations to be confirmed, with the next potential transit in 2019 May. In this Letter, we aid observational follow up by analyzing the transit signature of exomoons. We derive a simple analytic equation for the transit probability and use it to demonstrate how exomoons may frequently avoid transit if their orbit is larger than the stellar radius and sufficiently misaligned. The nominal orbit for the moon in Kepler-1625 has both of these characteristics, and we calculate that it may only transit roughly 40% of the time. This means that approximately six non-transits would be required to rule out the moon's existence at 95% confidence. When an exomoon's impact parameter is displaced off the star, the planet's impact parameter is displaced the other way, so larger planet transit durations are typically positively correlated with missed exomoon transits. On the other hand, strong correlations do not exist between missed exomoon transits and transit timing variations of the planet. We also show that nodal precession does not change an exomoon's transit probability and that it can break a prograde-retrograde degeneracy.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1901.06366/full.md

## References

39 references — full list in the complete paper: https://tomesphere.com/paper/1901.06366/full.md

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Source: https://tomesphere.com/paper/1901.06366