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Warm Saturns: Rings Around Exoplanets that Reside Inside the Ice Line. Hilke E. Schlichting (UCLA) Hubble Postdoctoral Fellow. Extreme Solar Systems II September. 14 th 2011 Schlichting & Chang (2011), ApJ 734, 117. Obvious Obstacles:. Poynting-Robertson drag timescale. - PowerPoint PPT Presentation
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Warm Saturns: Rings Around Exoplanets that Reside
Inside the Ice Line
Extreme Solar Systems IISeptember. 14th 2011
Schlichting & Chang (2011), ApJ 734, 117
Hilke E. Schlichting (UCLA)Hubble Postdoctoral Fellow
Obvious Obstacles:
• Best ring candidates have a > 0.1 AU• Ring lifetimes due to Poynting-Robertson drag 106-109 years
Rings must be rocky!Poynting-Robertson drag timescale
Roche Radius
For Saturn:RRoche/RP~2.2
(ice:1g/cm3)RRoche/RP~1.5
(rock:3g/cm3)
(Schlichting & Chang, 2011)
ρ =3g/cm3
ρ =5g/cm3
Warped Rings
(Schlichting & Chang, 2011)
For Reference:
J2 of Uranus & Neptune ~ 0.003
J2 of Jupiter & Saturn ~ 0.01
Ring Light Curves
Quadratic Limb Darkening as in Mandel & Agol (2001), for Ring light curves see also Barnes & Fortney (2004)
RP=1 RJ
RR1=2.0 RP
RP2=2.5 RP
RP=1 RJ
RR1=1.5 RP
RP2=2.5 RP
RP=1 RJ
RR1=2.0 RP
RP2=2.5 RP
RP=1.8 RJ
Transit duration ~ 6 hours
Time in ingress/egress ~ 2
hours
Ring Properties &Possibility for Detection
• Rings may be common• Rings must consist of rocky
material• Some Rings maybe warped
J2
• Best candidates for ring detection have a > 0.1 AU
• Obliquity damping, temperature, ideally want short cadence