Projects per year
Abstract
Titan's atmospheric inventory of oxygen compounds (H2O, CO2, CO) are thought to result from photochemistry acting on externally supplied oxygen species (O+, OH, H2O).
These species potentially originate from two main sources: (1)
cryogenic plumes from the active moon Enceladus and (2) micrometeoroid
ablation. Enceladus is already suspected to be the major O+ source, which is required for CO creation. However, photochemical models also require H2O and OH influx to reproduce observed quantities of CO2 and H2O.
Here, we exploit sulphur as a tracer to investigate the oxygen source
because it has very different relative abundances in micrometeorites
(S/O ~ 10−2) and Enceladus' plumes (S/O ~ 10−5).
Photochemical models predict most sulphur is converted to CS in the
upper atmosphere, so we use Atacama Large Millimeter/submillimeter Array
(ALMA) observations at ~340 GHz to search for CS emission. We
determined stringent CS 3σ stratospheric upper limits of
0.0074 ppb (uniform above 100 km) and 0.0256 ppb (uniform above 200 km).
These upper limits are not quite stringent enough to distinguish
between Enceladus and micrometeorite sources at the 3σ level and a
contribution from micrometeorites cannot be ruled out, especially if
external flux is toward the lower end of current estimates. Only the
high-flux micrometeorite source model of Hickson et al. can be rejected
at 3σ. We determined a 3σ stratospheric upper limit for CH2NH
of 0.35 ppb, which suggests cosmic rays may have a smaller influence in
the lower stratosphere than predicted by some photochemical models.
Disk-averaged C3H4 and C2H5CN profiles were determined and are consistent with previous ALMA and Cassini/CIRS measurements.
Original language | English |
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Article number | 251 |
Number of pages | 8 |
Journal | Astronomical Journal |
Volume | 155 |
Early online date | 25 May 2018 |
DOIs | |
Publication status | Published - Jun 2018 |
Keywords
- planets and satellites: atmospheres
- planets and satellites: individual (Titan)
- radiative transfer
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Dive into the research topics of 'The Origin of Titan’s External Oxygen: Further Constraints from ALMA Upper Limits on CS and CH2NH'. Together they form a unique fingerprint.Projects
- 4 Finished
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Research into planetary formation at Bristol.
Elliott, T. (Principal Investigator)
1/04/15 → 28/02/19
Project: Research
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Nick Teanby's Leverhulme Prize
Teanby, N. A. (Principal Investigator)
1/03/11 → 1/03/14
Project: Research