titan atmosphere and evolution chris mckay nasa ames chris.mckay@nasa

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Titan atmosphere and evolution Chris McKay NASA Ames [email protected] With Kevin Zanhle Jeff Moore, Brian Toon, Feng Tian

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Titan atmosphere and evolution Chris McKay NASA Ames [email protected]. With Kevin Zanhle Jeff Moore, Brian Toon, Feng Tian. Talking points. Titan’s current thermal and chemical structure is adequately understood. The central problem in extrapolating this over time is CH 4 . - PowerPoint PPT Presentation

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Page 1: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Titan atmosphere and evolution

Chris McKay NASA Ames

[email protected]

With Kevin Zanhle Jeff Moore, Brian Toon, Feng Tian

Page 2: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Talking points

• Titan’s current thermal and chemical structure is adequately understood.

• The central problem in extrapolating this over time is CH4.

• There is good evidence for ~10x CH4.

• Two scenarios- continuously wet Titan- recently wet Titan

• Both have significant issues.

Page 3: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Organic haze

N2-N2, CH4-N2, CH4-CH4, H2-N2 collision induced opacity

Anti-greenhouse

Greenhouse

Page 4: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

The Greenhouse Effect on Titan is due to N2 and CH4

From McKay et al. Science 1991

Page 5: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

The Antigreenhouse Effect due to Haze

From McKay et al. Science 1991

Page 6: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa
Page 7: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa
Page 8: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Net global averaged solar flux normalized to total incident solar flux. DSIR results compared to model of McKay et al. 1989. Figure from Tomasko et al (2007).

Page 9: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Energy balance in Titan’s atmosphere Chemistry

3.8 W m-2

From McKay et al. Science 1991

C6H6N

C6H6

N2-N2, N2-CH4, CH4-CH4 C2H6

Cold trap limits CH4

~1%

H2

~1010 cm-2s-1

~108 years

CH4

T(z)

Page 10: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Methane on Titan today

RH CH4 0.43 (Nieman et al. 2005)

Atmosphere 400 gm-C/cm2 (Lorenz et al. 2008)

Lakes 20 – 200 gm-C/cm2

Dunes 200 – 640 gm-C/cm2

Page 11: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Fluvial activity at the Equator

Large lakes at the Equator in the past

Storms require high RH at the equator.

Flooding the equator to form seas implies ~ 10x atmospheric CH4.

Page 12: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

N2 Clouds

Titan’s surface temperature over time with lakes

With N2 condensation (preliminary, but no obvious way to deep freeze)

Page 13: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

CH4 limiting flux (the loss rate of H2) is reduced in the past but only ~4x.

Page 14: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Continuously Wet Titan• Outgassing of 40x atmospheric CH4 (and 40Ar)

provides enough CH4 to last to the present time.

• Photochemistry produces 39x C2H6 and 1x dune material.

• Dunes are visible.

• C2H6 peculates into the surface.

• CH4 photochemical lifetime implies we are coincidentally close to the end of CH4. Waiting for cryovolcanios or at the end of the wet era.

• Not clear how to hide the C2H6 (> 200 m is hidden, with or without CH4).

Page 15: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

1 Gyr ago10x current CH4

Today1.2x atmospheric CH4

100 Myr No CH4

Recently wet Titan: an initial cold inventory, no cryovolcanism, recent atmosphere & past rain,

Page 16: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

Recently Wet Titan• Titan spends most of its history in a Triton-like state. • Runaway greenhouse nx108 Gyr ago with production

of nx atmospheric CH4 (and 40Ar) provides enough CH4 to last to the present time. Minimum n ~ 5 , implies wet age is > 5x108 years

• Photochemistry produces C2H6 and tholin, C2H6 converts to dunes. Dunes have nx C.

• No hidden C2H6

• CH4 photochemical lifetime implies we are coincidentally close to the end of CH4.

• Not clear how to keep a Triton-like state cold enough to shut off CH4 photolysis.

• Not clear how C2H6 converts to dune material.

Page 17: Titan atmosphere and evolution Chris McKay  NASA Ames chris.mckay@nasa

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