Predictions for a planet just inside Fomalhaut's eccentric ring
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...Resonance overlap studies have shown how a planet can sculpt the inner edge of a disk (e.g., Quillen 2006, Mustill & Wyatt 2012)....
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24 citations
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Cites background from "Predictions for a planet just insid..."
...Some authors have assumed that planetesimals in a debris disk have had their free eccentricities completely damped by collisions (Quillen 2006; Chiang et al. 2009) resulting in a ring of planetesimals on orbits with eccentricity equal to the forced eccentricity from the planet....
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...…of a planet on an eccentric orbit interacting with a debris disk have assumed either no particular collisional evolution of the planetesimal orbits (Wyatt 1999; Wilner et al. 2002; Quillen & Thorndike 2002; Moran et al. 2004), or complete collisional damping (Quillen 2006; Chiang et al. 2009)....
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...Then — in stark contrast to Wyatt (1999), which did not incorporate collisions — collisions break up the spiral before it can wrap once more around the star, leaving an apsealigned ring shown in the lower right, as described by Quillen (2006)....
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...Many authors have analyzed resolved images of debris disks to predict the presence of exoplanets and constrain their locations, orbits, and physical properties (e.g. Wyatt et al. 1999; Greaves et al. 2005; Quillen 2006; Stark & Kuchner 2008)....
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References
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"Predictions for a planet just insid..." refers background in this paper
...2 T H E P E R I C E N T R E G L OW M O D E L A N D A N E C C E N T R I C E D G E I N F O M A L H AU T ’ S D I S C We follow the theory for secular perturbations induced by a planet (e.g. Murray & Dermott 1999; Wyatt et al. 1999)....
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...Secular perturbations in the plane can be described in terms of the complex eccentricity variable, z = e exp(i ), where e is the object’s eccentricity and is its longitude of periastron (e.g. Murray & Dermott 1999; Wyatt et al. 1999)....
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...The functions, b js (α), are Laplace coefficients (see Murray & Dermott 1999 for definitions and numerical expressions)....
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...The time variation of z is ż = zforced + zproper(t) (1) where zforced = b23/2(α) b13/2(α) ep exp(i p) (2) (Murray & Dermott 1999; Wyatt et al. 1999)....
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1,601 citations
"Predictions for a planet just insid..." refers background or methods in this paper
...(4) We have recovered the scaling with planet mass predicted by previous works (Goldreich & Tremaine 1980; Franklin et al. 1980; Lissauer & Espresate 1998) but have also included a dependence on distance from the planet....
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...Franklin et al. (1980), Goldreich & Tremaine (1980) and Lissauer & Espresate (1998) showed that spiral density waves were efficiently driven at a Lindblad resonance by a satellite when the collision time-scale was above a critical one, t crit, where t crit ∝ μ−2/3, and μ ≡ m p/M ∗ is the ratio of…...
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488 citations
"Predictions for a planet just insid..." refers background in this paper
...The width of this zone has been measured numerically and predicted theoretically for a planet in a circular orbit by predicting the semi-major axis at which the first-order mean motion resonances overlap (Wisdom 1980; Duncan, Quinn & Tremaine 1989; Murray & Holman 1997; Mudryk & Wu 2006)....
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459 citations
"Predictions for a planet just insid..." refers background in this paper
...1 I N T RO D U C T I O N The nearby star Fomalhaut hosts a ring of circumstellar material (Aumann 1985; Gillett 1985) residing between 120 and 160 au from the star (Holland et al. 1998; Dent et al. 2000; Holland et al. 2003)....
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