Titans Methane Weather Thank you. We started the week hearing about - - PowerPoint PPT Presentation

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Titans Methane Weather Thank you. We started the week hearing about - - PowerPoint PPT Presentation

Mar 20, 2023 282 likes •665 views

Titans Methane Weather Thank you. We started the week hearing about cosmology, large scale structure, & galaxy formation. Today we zoomed in to extrasolar planets. So, lets zoom in from thinking about planets around other stars to

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Titan’s Methane Weather

Henry Roe (Lowell Observatory) Emily Schaller (IfA, University of Hawaii) Michael Brown (Caltech) Chadwick Trujillo (Gemini Observatory)

20 May 2009 - Joint Subaru/Gemini Science Meeting Thank you. We started the week hearing about cosmology, large scale structure, & galaxy formation. Today we zoomed in to extrasolar planets. So, let’s zoom in from thinking about planet’s around other stars to an object in our own solar system Today I would like to talk about a project we have been working on using Gemini and other telescopes to study weather and climate on Saturn’s largest moon Titan. Acknowledge collaborators. I would like to spend the first few minutes giving a brief introduction to Titan.

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Titan’s Methane Weather

Henry Roe (Lowell Observatory) Emily Schaller (IfA, University of Hawaii) Michael Brown (Caltech) Chadwick Trujillo (Gemini Observatory)

20 May 2009 - Joint Subaru/Gemini Science Meeting Thank you. We started the week hearing about cosmology, large scale structure, & galaxy formation. Today we zoomed in to extrasolar planets. So, let’s zoom in from thinking about planet’s around other stars to an object in our own solar system Today I would like to talk about a project we have been working on using Gemini and other telescopes to study weather and climate on Saturn’s largest moon Titan. Acknowledge collaborators. I would like to spend the first few minutes giving a brief introduction to Titan.

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When we look at the surfaces of Titan & Earth we see some remarkable similarities. If you had never seen any of these images before, you would probably have a hard time identifying which were from Titan and which were from Earth. The materials are very different on Titan (water ice instead of rock, liquid methane instead of water, etc, but the processes on the surface and in the atmosphere are familiar.

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Titan Earth

When we look at the surfaces of Titan & Earth we see some remarkable similarities. If you had never seen any of these images before, you would probably have a hard time identifying which were from Titan and which were from Earth. The materials are very different on Titan (water ice instead of rock, liquid methane instead of water, etc, but the processes on the surface and in the atmosphere are familiar.

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30-year Seasonal Cycle

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Mean daily insolation on Titan

30-year Seasonal Cycle

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~80% N2 ~90% N2

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~80% N2 ~90% N2

Thick vs. thin Trace species: Oxygen (we all like) Water - condensible, triple point, phase transitions On Titan - water = rock, but near triple point of methane and few percent methane

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Methane Water

~80% N2 ~90% N2

Thick vs. thin Trace species: Oxygen (we all like) Water - condensible, triple point, phase transitions On Titan - water = rock, but near triple point of methane and few percent methane

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Thin shell even though surface area much less: Titan/Earth atmos mass = 2x Titan: 4m/10cm Earth: 1

  • 10cm/1

m With that much condensible in the atmosphere, where’s liquid on surface? How to look for it?

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Titan’s Surface Mapped by Cassini

Cassini map of Titan’s surface. No liquids at low latitudes, but evidence of fluid flow

  • everywhere. Lots of lakes in North, a few in south.
  • pportunity to discuss, temporal coverage of Cassini
  • vs. ground-based

90°N 0° 90°S

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Titan

Methane in atmosphere Irreversible loss of methane at top of atmosphere All methane gone in 10myr

Methane

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Titan

Methane in atmosphere Irreversible loss of methane at top of atmosphere All methane gone in 10myr

Methane

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Titan

Methane in atmosphere Irreversible loss of methane at top of atmosphere All methane gone in 10myr

Methane

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Some Questions

  • Methane weather? Where? When? How?
  • Source of methane?
  • Hydrology/Meteorology: Where? When? How?
  • Seasonal climate change; Massive monsoon?
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Methane transmission

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Methane transmission

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Methane transmission

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Small angular size As Joe Jensen discussed on Monday: Flexibility of Gemini Operations are key Importance of Queue! Snapshot needs only 15- 20 minutes Maximize efficient use of Gemini with small telescopes to trigger ToO’s and fill-in temporal record.

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Small angular size As Joe Jensen discussed on Monday: Flexibility of Gemini Operations are key Importance of Queue! Snapshot needs only 15- 20 minutes Maximize efficient use of Gemini with small telescopes to trigger ToO’s and fill-in temporal record.

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Small angular size As Joe Jensen discussed on Monday: Flexibility of Gemini Operations are key Importance of Queue! Snapshot needs only 15- 20 minutes Maximize efficient use of Gemini with small telescopes to trigger ToO’s and fill-in temporal record.

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Results

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South polar clouds

Typical south polar clouds of early-to-mid southern summer. Can see more data on our poster at this meeting.

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Dissipation of south polar clouds

Schaller et al. 2006b Icarus

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Titan

North Pole South Pole

Southern Summer

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Titan

North Pole South Pole

Southern Summer Southern Fall

North Pole South Pole

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Roe et al. 2005 ApJL

Discovery of mid-latitude clouds at 40°S

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Geographic Control of mid-Latitude Clouds

Roe et al. 2005 Science

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Lake-effect clouds in the north polar region

lines of latitude are 5deg ISS in green, VIMS in red, gemini in blue

  • M. Brown et al. 2009 GRL
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Tropical storms & atmospheric waves Schaller et al. 2009 in press

accepted to Nature Event last spring Proves the value of our multi- telescope approach Wave activity GCM’s predict no/few clouds equatorially ever, AND no southern clouds in current season. This shows how Titan’s atmosphere can generate clouds & precip at time/places that ‘ should’ be dry

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3-color image constructed from K’, H210, & Brgamma amazing amount of color variation in the rings amazing amount of detail in dynamics of saturn atmosphere

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Mimas

Mimas is “ death-star moon” because of a large crater and its appearance 400 km across

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F-ring & Pandora Janus

Janus is <200 km across F-ring discovered in 1979 by the Pioneer 11 imaging team. Constrained by 2 shepard moons (Pandora & Prometheus) Pandora <100km across

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F-ring & Pandora

Janus is <200 km across F-ring discovered in 1979 by the Pioneer 11 imaging team. Constrained by 2 shepard moons (Pandora & Prometheus) Pandora <100km across

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Thank you to all the Gemini staff who have helped with these observations!

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Summary

  • Titan has active methane meteorology
  • Ground-based observing required to provide necessary

temporal coverage

  • Gemini is key to ground-based observing
  • Discoveries in past 5 years include:
  • South polar cloud field in late southern spring
  • Seasonal shutdown of south polar cloud field

(monsoonal shift of winds)

  • Mid-southern latitude clouds that are geographically

controlled likely indicate region of geologic activity and methane resupply

  • Northern lake-effect clouds
  • Wave-activity can communicate globally and generate

clouds at latitudes/seasons not predicted by global circulation models

  • Have only observed a fraction of Titan’s 30-year seasonal

cycle Need to continue observing!