KOI-730 as a System of Four Planets in a Chain of Resonances Daniel Fabrycky UC Santa Cruz Matthew...
-
date post
21-Dec-2015 -
Category
Documents
-
view
216 -
download
0
Transcript of KOI-730 as a System of Four Planets in a Chain of Resonances Daniel Fabrycky UC Santa Cruz Matthew...
![Page 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/1.jpg)
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
![Page 2: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/2.jpg)
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)
![Page 3: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/3.jpg)
KOI-730: Three Pairs of First-Order Resonances
3:4:6:8
P/PP=1.33411(8) 4:3
P/P=1.50157(5) 3:2
P/P=1.33341(3) 4:3
candidate period (d) Rp (RE)
730.04 7.3831 1.8
730.02 9.8499 2.1
730.01 14.7903 2.8
730.02 19.7216 2.4
![Page 4: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/4.jpg)
![Page 5: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/5.jpg)
Laplace-type resonances
• Involves 3 planets at once• Io, Europa, & Gaynmede obey λI-3λE+2λG=180°
![Page 6: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/6.jpg)
![Page 7: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/7.jpg)
![Page 8: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/8.jpg)
TTVs??
![Page 9: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/9.jpg)
Theory:• Match P, T0
• coplanar• mass: Mp = Rp
2.06
• e = 0
Observed:transit timesthrough Q8
P=7.3831 ddP/dE= -1±1 s
P=9.8499 ddP/dE= 0±3 s
P=19.7216 ddP/dE= -12±12 s
P=14.7903 ddP/dE= 15±2 s relax
![Page 10: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/10.jpg)
![Page 11: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/11.jpg)
![Page 12: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/12.jpg)
Lee & Peale 02GJ 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
![Page 13: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/13.jpg)
Capture into Resonance
first-order resonances Laplace-type resonances moderate eccentricities increased stability
![Page 14: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/14.jpg)
• 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:
![Page 15: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/15.jpg)
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.
![Page 16: 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,](https://reader030.fdocuments.in/reader030/viewer/2022032521/56649d575503460f94a35757/html5/thumbnails/16.jpg)
• Stellar properties (determined by photometry, accounting for a blended companion, and fit to isochrones):
Kp15.3 mag