# ARCHITECTURE AND DYNAMICS OF KEPLER'S CANDIDATE MULTIPLE TRANSITING PLANET SYSTEMS

@article{Lissauer2011ARCHITECTUREAD, title={ARCHITECTURE AND DYNAMICS OF KEPLER'S CANDIDATE MULTIPLE TRANSITING PLANET SYSTEMS}, author={Jack J. Lissauer and Darin Ragozzine and Daniel C. Fabrycky and Jason H. Steffen and Eric B. Ford and Jon M. Jenkins and Avi Shporer and Matthew J. Holman and Jason F. Rowe and Elisa V. Quintana and Natalie M. Batalha and William J. Borucki and Stephen T. Bryson and Douglas A. Caldwell and Joshua A. Carter and David R. Ciardi and Edward Wood Dunham and Jonathan J. Fortney and Thomas Gautier and Steve B. Howell and David G. Koch and David W. Latham and Geoffrey W. Marcy and Robert C. Morehead and Dimitar D. Sasselov}, journal={The Astrophysical Journal Supplement Series}, year={2011}, volume={197} }

About one-third of the ∼1200 transiting planet candidates detected in the first four months of Kepler data are members of multiple candidate systems. There are 115 target stars with two candidate transiting planets, 45 with three, 8 with four, and 1 each with five and six. We characterize the dynamical properties of these candidate multi-planet systems. The distribution of observed period ratios shows that the vast majority of candidate pairs are neither in nor near low-order mean-motion…

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## References

SHOWING 1-10 OF 69 REFERENCES

### A FIRST COMPARISON OF KEPLER PLANET CANDIDATES IN SINGLE AND MULTIPLE SYSTEMS

- Physics, Geology
- 2011

In this Letter, we present an overview of the rich population of systems with multiple candidate transiting planets found in the first four months of Kepler data. The census of multiples includes 115…

### TRANSIT TIMING OBSERVATIONS FROM KEPLER. I. STATISTICAL ANALYSIS OF THE FIRST FOUR MONTHS

- Geology, Physics
- 2011

The architectures of multiple planet systems can provide valuable constraints on models of planet formation, including orbital migration, and excitation of orbital eccentricities and inclinations.…

### FIVE KEPLER TARGET STARS THAT SHOW MULTIPLE TRANSITING EXOPLANET CANDIDATES

- Physics, Geology
- 2010

We present and discuss five candidate exoplanetary systems identified with the Kepler spacecraft. These five systems show transits from multiple exoplanet candidates. Should these objects prove to be…

### A closely packed system of low-mass, low-density planets transiting Kepler-11

- Physics, GeologyNature
- 2011

Kepler spacecraft observations of a single Sun-like star are reported that reveal six transiting planets, five with orbital periods between 10 and 47 days and a sixth planet with a longer period, among the smallest for which mass and size have both been measured.

### SECULAR ORBITAL DYNAMICS OF HIERARCHICAL TWO-PLANET SYSTEMS

- Physics, Geology
- 2010

The discovery of multi-planet extrasolar systems has kindled interest in using their orbital evolution as a probe of planet formation. Accurate descriptions of planetary orbits identify systems that…

### Dynamical Models of the Resonant Pair of Planets Orbiting the Star GJ 876

- Physics, Geology
- 2001

We present two planet fits to the radial velocity measurements of the M dwarf star GJ 876 that account for the mutual perturbations between the planets, as well as their interactions with the star.…

### CHARACTERISTICS OF KEPLER PLANETARY CANDIDATES BASED ON THE FIRST DATA SET

- Physics, Geology
- 2010

In the spring of 2009, the Kepler Mission commenced high-precision photometry on nearly 156,000 stars to determine the frequency and characteristics of small exoplanets, conduct a guest observer…

### PLANET–PLANET SCATTERING IN PLANETESIMAL DISKS

- Physics, Geology
- 2009

We study the final architecture of planetary systems that evolve under the combined effects of planet–planet and planetesimal scattering. Using N-body simulations we investigate the dynamics of…

### TEN NEW AND UPDATED MULTIPLANET SYSTEMS AND A SURVEY OF EXOPLANETARY SYSTEMS

- Geology, Physics
- 2009

We present the latest velocities for ten multiplanet systems, including a re-analysis of archival Keck and Lick data, resulting in improved velocities that supersede our previously published…

### A Pair of Resonant Planets Orbiting GJ 876

- Physics, Geology
- 2001

Precise Doppler measurements during 6 yr from the Lick and Keck observatories reveal two planets orbiting GJ 876 (M4V). The orbital fit yields companion masses of M sin i = 0.56 and 1.89 MJ, orbital…