initial data: n 2 and ch 4 densities near the surface
DESCRIPTION
Titan’s Photochemical Model: Oxygen Species and Comparison with Triton and Pluto Vladimir Krasnopolsky. Initial data: N 2 and CH 4 densities near the surface Products: vertical profiles of 83 neutral species and 33 ions from 0 to 1600 km. Main Features. - PowerPoint PPT PresentationTRANSCRIPT
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Titan’s Photochemical Model: Oxygen Species and Comparison with
Triton and Pluto
Vladimir Krasnopolsky
• Initial data: N2 and CH4 densities near the surface• Products: vertical profiles of 83 neutral
species and 33 ions from 0 to 1600 km
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Main Features• The only after-Cassini model of coupled neutral and ion
chemistry• Hydrocarbon chemistry is extended to C12H10 • Radiative transfer using the Huygens data and a code for
the aggregate particles• Ion chemistry is extended to C10H11
+ • Ambipolar diffusion and escape of ions• Involves effects of magnetospheric electrons, protons,
and cosmic rays• The number of reactions is reduced to 415 with column
rates for each reaction
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Calculated extinction by haze using the Huygens data, refractive indices from Khare84, and a
code for aggregate particles
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Ionization by solar EUV, magnetospheric electrons, protons, and cosmic rays
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Calculated absorption of solar EUV and UV on Titan (λ in nm)
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Oxygen species formed by meteorite H2O and magnetospheric O+
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Production of haze (100 m/Byr total)
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Calculated and observed ionospheric profiles
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Three bodies with N2-CH4 atmospheres: Titan, Triton, and Pluto
• Titan 1.5 bar, Triton 40 μbar, Pluto 15 μbar. Why are they so different?
• Titan at 10 AU, Triton at 30 AU, Pluto at 30-50 AU• Titan T = 94 K, Triton T = 40 K, Pluto T = 38 -29 K• Titan N2 is completely in the atmosphere, and N2
is in surface ice on Triton and Pluto
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Triton: mostly atomic composition (Krasnopolsky and Cruikshank 1995)
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Pluto: molecular composition. [N]Triton/[N]Pluto ≈ 104 (Krasnopolsky and Cruikshank 1999)
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Triton’s ionosphere: atomic ions, emax = 3x104 cm-3 (Krasnopolsky and Cruikshank 1995)
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Pluto’s ionosphere: molecular ions, emax = 800 cm-3 (Krasnopolsky and Cruikshank 1999)
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Why are Triton and Pluto so different?Conclusion: Triton still keeps
Voyager-type chemistry