Volcanism on Io II Eruption Plumes on Io Ionian Plumes: SO2 Source

Volcanism on Io II Eruption Plumes on Io Ionian Plumes: SO2 Source

Volcanism on Io II GLY 424/524 April 22, 2002 Eruption Plumes on Io Ionian Plumes: SO2 Source • Low gravity, atmospheric pressure • Liquid SO2 “pockets” beneath the surface • Plumes on Io ~60 - 450 km – Superheated upon contact with magma – Old Faithful would be 35 km tall on Io – Boil, erupt • Powered by SO and SO2 • Vertical crustal recycling of SO2 “snow” – Tvashtar plume detected August 2001 and “frost” deposits – 500 km tall • Most plumes from lava flow front rather – Particles determined to be SO2 “snowflakes” than vent – Interaction of hot lava with old SO2 “snow” Sulfur gas (S2 or SO2) lands on the cold surface. Atoms rearrange into (S3, S4), which give the surface a red color. Eventually, S8 forms ordinary pale yellow sulfur. 1 Io Volcanic Styles Io Volcanic Styles Continued • Promethean • Pillanian – Prometheus = type locale – Pillan = type locale • Also Amirani • Also Tvashtar • Zamama • I-31A hot-spot • Culann – Short-lived, high-effusion-rate eruptions – Long-lived, steady eruptions • Large pyroclastic deposits • Produces compound flow field • Open-channel or open-sheet flows • Takes years to decades • Associated with “wandering” plumes • Lava lakes – Extensive plume deposits – Loki = type locale – Extensive, rapidly emplace flows • Also Emakong, Pele, Tupan – High temperatures Prometheus Prometheus Prometheus Prometheus • Io’s “Old Faithful” – Active since 1979 – Observed by Voyager 1 • Eruption Plume – 80 km tall – Plume source migrated 85 km to the west since 1979 • Lava flow – ~100 km long – Apparently originates in caldera 2 Prometheus Caldera & flow-front plume Prometheus Pillan Pele & Pillan April, 1997 September, 1997 July, 1999 12 km/px 5 km/px 12 km/px Pillan ~400 km diameter Pillan eruption • http://www.digitalradiance.com/sng/Io_volc ano.htm 3 Pillan Lava flows High-res images near Pillan Patera 7.2 km long ~9 m/pixel Pillan lava flows; 19 m/px Tvashtar Bright regions are saturated pixels, indicating HOT fire- fountaining on Io Temps >1600K F.o.v. ~300 x 75 km 4 Loki Loki, March 4, 1979 Pele Loki as seen by NIMS Image A: Brightness temperatures in K; Image B: color temperatures in K Loki temps: lava flooding? Emakong Caldera Emakong 5 Lava channel Voyager Io Results Emakong Emakong ~70 km long Tupan Caldera Culann 6.

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    6 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us