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KOI-730 as a System of Four Planets in a Chain of Resonances Daniel Fabrycky UC Santa Cruz Matthew Holman, Joshua Carter, Jason Rowe, Darin Ragozzine,

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Presentation on theme: "KOI-730 as a System of Four Planets in a Chain of Resonances Daniel Fabrycky UC Santa Cruz Matthew Holman, Joshua Carter, Jason Rowe, Darin Ragozzine,"— Presentation transcript:

1 KOI-730 as a System of Four Planets in a Chain of Resonances Daniel Fabrycky UC Santa Cruz Matthew Holman, Joshua Carter, Jason Rowe, Darin Ragozzine, William Borucki, David Koch, and the Kepler Team

2 Planets in Resonance Resonances are common among RV-discovered gas giants (~1 period commensurability in 3 multi systems: Wright et al. 2011, a 4:2:1 chain in GJ 876: Rivera et al. 2010) Kepler has found Neptune-size pairs especially abundant near resonances (Lissauer et al. 2011) Theories suggest the Solar System giants may have started in a resonant chain (Morbidelli et al. 2007, Thommes et al. 2008)

3 KOI-730: Three Pairs of First-Order Resonances 3:4:6:8 P P/P=1.33411(8) 4:3 P/P=1.50157(5) 3:2 P/P=1.33341(3) 4:3 candidateperiod (d)R p (R E ) 730.047.38311.8 730.029.84992.1 730.0114.79032.8 730.0219.72162.4

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5 Laplace-type resonances Involves 3 planets at once Io, Europa, & Gaynmede obey λ I -3λ E +2λ G =180°

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8 TTVs??

9 Theory: Match P, T 0 coplanar mass: M p = R p 2.06 e = 0 Observed: transit times through Q8 P=7.3831 d dP/dE= -1±1 s P=9.8499 d dP/dE= 0±3 s P=19.7216 d dP/dE= -12±12 s P=14.7903 d dP/dE= 15±2 s relax

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12 Lee & Peale 02 GJ 876 b/c Disk Migration Theory Rules-of-thumb for resonance capture: Converging and slow Low eccentricity favors first-order resonances High eccentricity favors high-order resonances

13 Capture into Resonance ✓ first-order resonances ✓ Laplace-type resonances ✓ moderate eccentricities ✓ increased stability

14 A candidate system of 4 low-mass planets on compact, resonant orbits It informs migration models: limits the speed, direction, and damping properties It’s the missing link to RV exoplanet systems, the Kepler multis, and maybe even the Solar System giants KOI-730:

15 Coorbital no more KOI-730.03’s period was revised from 9.861 days to twice that: 19.722 days. This took it out of 1:1 resonance with KOI- 730.02. This was apparent even in the Q1-Q2 data and is confirmed by the data through Q8.

16 Stellar properties (determined by photometry, accounting for a blended companion, and fit to isochrones): Kp 15.3 mag


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