20101130 charm aharonson
TRANSCRIPT
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Oded Aharonson (Caltech)Alex Hayes, Jonathan Lunine,Ralph Lorenz, Michael Allison,
Charles Elachi, Cassini RadarScience Team
Unveiling Titan:A World Strange and Familiar
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HST, Wide Field Camera 2
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Voyager 1 1980A Hazy world. Hemispheric Asymmetry,
Polar Collar/Hood
UV radiation and coronadischarge of N2/CH4mixtures
End product - tholin(from Greek muddy, viaCarl Sagan)
Image Credit: NASA/JPL/Caltech
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Titan: A New World
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Photo by K. Sturgill, Marion, Virginia
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The Magnificent Seven:
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Cassini VIMS: Titans spectral diversity
Based on Barnes et al., 2007
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Titans Dune1-2 km spacing
150 m characteristic heights
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Shuttle handheld digital cameraSTS107
Linear Dunes in the Namib Desert
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Titans Hydrologic Cycle
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Elivagar FluminaBraided, sinuous channels
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Analog Site - near Parker AZ(identified from airplane window, TUS-LAX circa 730am )
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Titans Odds @ Caltech
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The View from Huygens
Credit: ESA, NASA, Descent Imager/Spectral Radiometer Team (LPL)
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Image Credit: NASA/JPL
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2010
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200210
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0 350
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0 375 750 1,125 1,500187.5km
n
Hayes et al. , 2008
m
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Courtesy NASA/JPL-Caltech
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Image Credit: NASA / JPL / University of Arizona / DLR
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Brown et al., Nature, 2008
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Current Radar Mapping
Aharonson et al. , 2009
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Polewards of 55, now >50%coverage in both hemispheres
North South
Filled 10%
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Zebker et al. , Science, 2009
Global Shape
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Mitchell et al. , 2008
GCM
2D GCM predicts:
Eevap. ~ 2 W/m2
i.e. 0.3 m/yr
Numerical Predictions
0 375 750 1 125 1 500187 5
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2010
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170 180 190
200210
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0 375 750 1,125 1,500187.5km
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Hayes et al. , 2008
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R. Lorenz (Pers. Comm.)
l l
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t=0,Ls,p=277.7, e=0.054
Solar Insolation
Peak South Polar Insolation:7.48 W/m2
Peak North Polar Insolation:6.04 W/m2haronson et al. , 2009
400
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-100 -80 -60 -40 -20 00
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Time Since Present (kyr)
Ls
ofPerihelion
-100 -80 -60 -40 -20 026
26.5
27
27.5
28
28.5
Time Since Present (kyr)
Saturn'sObliq
uity()
-100 -80 -60 -40 -20 00
1
2
3
4
5
Time Since Present (kyr)
Saturn'sEccentricity()(%)
l l
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t=0,Ls,p=277.7, e=0.054 t=-31.5 kyr, Ls,p= 97.7, e=0.046
Solar Insolation
Aharonson et al. , 2009
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22-25
-0.7-0.04
0-6%
440-570 W/m2
O18
http://www.globalwarmingart.com/wiki/File:Milankovitch_Variations_png
Tit s Mil k it h P i ds
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~270 kyr ~45 kyr
Titans Milankovitch Periods
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MilutinMilankovi(1879 1958)
Ice Ages
JamesCroll
(1821-1890)
http://earth.rice.edu/mtpe/cryo/cryosphere/topics/ice_age.html
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11-20 km Putative Craters Sinlap, 80 km
Crater retention age:200 Myr (Wood et al., 2009) up to
1 Gyr crater retention age
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Putative Crater Distribution
Wood et al., 2009
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GCM Results
Graves, Schneider, et al.
Some Numbers
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Hypothesis consistent with
Hemispheric asymmetry in lakes Ontario Lake Ethane detection by VIMS
Insolation function energetics
Crater distribution latitudinal gradients
Some Numbers The differential heat flux can evaporate:
F~ 1.5 W/m2
L = 510 kJ/kg = 422 kg/m3
Ethane is significantly (x10,000) less volatile so is likelyto remain, and can retain residual methane in solution
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Schaller et al., 2009
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Hayes et al. , 201 0a in press)
A M d lD
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Hayes et al. , 201 0a in press)
A ModelData
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Hayes et al. , 201 0b in press)
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Hayes et al. , 201 0b in press)
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Hayes et al. , 201 0b in press)
Ontario Reduction
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Ontario Reduction
Flux: 1.00.2 m/yrHayes et al. , 201 0b, in press)
Summary
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tan =(9.1+2.5)10-4
Possible to obtain firstextra-terrestrialbathymetry of near-shore
lake regions, correlate withgeology
Seasonal methane loss rate
from southern lakes Ontario: 1.00.2 m/yr
Smaller lakes: 1.070.23,1.100.23, 1.030.25,
1.090.34 m/yr
-2.0
Summary
Summary
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So far, no demonstrable lake
height changes have beenidentified in the North(Although several putative changes areseen, in part may be due to incidenceangle variations)
Climate models vary in theirpredictions, e.g. Newman etal., Graves et al., predict
peak summer evaporation,Tokano et al. predict peak inthe winter
Summary
Summary
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Summary Cassini revealed a statistically
significant asymmetry in lakedistribution
If the asymmetry is notinherent to the crust, we
propose it is due to anasymmetry in Titans seasonsforced by the orbit
The orbital parameters varywith 10s kyr periods,suggesting a dynamichydrologic methane cycle
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Thanks