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Tales from the outer solar system (8) (IT SHOULDN’T) Mike Brown Caltech Tales from the outer solar system (8) (IT SHOULDN’T) Mike Brown Caltech

Meg Schwamb Wes Fraser Darin Ragozzine Alex Lockwood Konstantin Batygin Emily Schaller Michele Bannister Meg Schwamb Wes Fraser Darin Ragozzine Alex Lockwood Konstantin Batygin Emily Schaller Michele Bannister David Rabinowitz Chad Trujillo

U Plutinos 3: 2 2: 1 ssing cro tune Nep scattered KBOs classical KBOs U Plutinos 3: 2 2: 1 ssing cro tune Nep scattered KBOs classical KBOs N

Picture of oschin, with radio link with Chad Trujillo & David Rabinowitz Picture of oschin, with radio link with Chad Trujillo & David Rabinowitz

Brown, Trujillo, Rabinowitz Brown, Trujillo, Rabinowitz

Haumea Snow White Haumea Snow White

S J U N P S J U N P

Where did it come from? -in situ formation -scattered by modest-sized planet @ ~70 Where did it come from? -in situ formation -scattered by modest-sized planet @ ~70 AU -close stellar encounter

Where did it come from? -in situ -scattered by modest-sized planet @ ~70 AU Where did it come from? -in situ -scattered by modest-sized planet @ ~70 AU -close stellar encounter

Where did it come from? -in situ -scattered by modest-sized planet @ ~70 AU Where did it come from? -in situ -scattered by modest-sized planet @ ~70 AU -close stellar encounter -dense stellar birth environment

Schwamb, Brown, Rabinowitz 2009 Schwamb, Brown, Rabinowitz 2009

241. 02 Snow white Sedna Schwamb, Brown, Rabinowitz 2009 241. 02 Snow white Sedna Schwamb, Brown, Rabinowitz 2009

Schwamb, Brown, Rabinowitz 2009 Schwamb, Brown, Rabinowitz 2009

Haumea Snow White Haumea Snow White

25% 2 hours Rabinowitz et al. 2005 25% 2 hours Rabinowitz et al. 2005

ρ = 2. 6 g/cm 3 Weidenshilling 1983 ρ = 2. 6 g/cm 3 Weidenshilling 1983

Trujillo et al. 2006 Trujillo et al. 2006

V=17. 5 FWHM=0. 063 Strehl=0. 18 V=17. 5 FWHM=0. 063 Strehl=0. 18

Haumea Hi’iaka Haumea Hi’iaka

Canup 2005 Canup 2005

Brown et al. 2007 Brown et al. 2007

EL 61 Haumea (12: 7) Isotropic v = 150 m/s Ragozzine Sw. RI Colloquium EL 61 Haumea (12: 7) Isotropic v = 150 m/s Ragozzine Sw. RI Colloquium 1999 OY 3 (7: 4) Resonance Diffusion

1999 OY 3 (7: 4) EL 61 Haumea (12: 7) Resonance Diffusion 2003 UZ 1999 OY 3 (7: 4) EL 61 Haumea (12: 7) Resonance Diffusion 2003 UZ 117 Isotropic v = 150 m/s 2005 CB 79 Ragozzine Sw. RI Colloquium Schaller and Brown 2008

V=17. 5 FWHM=0. 063 Strehl=0. 18 V=17. 5 FWHM=0. 063 Strehl=0. 18

UNSTABLE 49 -day period e = 0. 05 Mp ≈ 1/3 Pluto UNSTABLE 49 -day period e = 0. 05 Mp ≈ 1/3 Pluto

Results Masses: 0. 5% and 0. 05% Ecc: 0. 05 and 0. 23 Mutual Results Masses: 0. 5% and 0. 05% Ecc: 0. 05 and 0. 23 Mutual inc: 13 degrees Mean-motion ratio: near 8: 3 Ragozzine J 2+spin pole Colloquium Sw. RI

Model Dependent Satellite Masses, Albedos, Densities Model Dependent Satellite Masses, Albedos, Densities

Brown, Trujillo, Rabinowitz Brown, Trujillo, Rabinowitz

And they all lived happily at least for a few Gyr. The End And they all lived happily at least for a few Gyr. The End