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Atmospheric Chemistry of Titan
Juramike
post May 2 2010, 03:38 AM
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Here is a "Benzene-O-Vision" graphic showing the amount of benzene and phenyl radicals at high altitudes on Titan. This is based on detections of benzene and phenyl radical (which recombined in the sample chamber to make benzene) using the INMS instrument during closest approach. The numbers are normalized to constant pressure altitude, roughly 1000 km.

Attached Image


The data was taken from Table 1 in: Vuitton et al, Journal of Geophysical Research 113 (2008) E05007. "Formation and distribution of benzene on Titan". doi: 10.1029/2007JE002997 [EDIT 5/24/10: Article freely available here] and overlaid on a map of Titan.

The authors mentioned that the errors in these measurements are 20%.

These detections are well above the detached haze layer. Most are at the same sun azimuth angle. (T23 observation had the lowest angle.) Assuming that the temporal difference is minimal (each dot is from a different flyby), there doesn't appear to be an obvious correlation with latitude.

This graphic does show that benzene is present even waaaay up in the thermosphere and ionosphere.


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scalbers
post Dec 11 2011, 08:39 PM
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I saw a talk given at the AGU conference last week mentioning that far infra-red spectral observations suggest that the atmospheric hazes probably have different composition than the traditional Titan tholins. More lab work will be helpful in comparing various compositions to the observations. This is related to post #79 I believe. Here is the abstract...

ABSTRACT FINAL ID: P33F-0
TITLE: Spectral and vertical distribution properties of Titan’s particulates from thermal-IR CIRS data: Physical Implications
SESSION TYPE: Oral
SESSION TITLE: P33F. Titan: An Earth-Like World II
AUTHORS (FIRST NAME, LAST NAME): Carrie M Anderson1, Robert Samuelson2, 1, Sandrine Vinatier3
INSTITUTIONS (ALL): 1. Solar System Exploration Divis, NASA---GSFC, Greenbelt, MD, United States.
2. Astronomy, University of Maryland, College Park, MD, United States.
3. LESIA , Observatoire de Paris-Meudon, Meudon , France.
Title of Team:
ABSTRACT BODY: Analyses of far-IR spectra between 20 and 560 cm-1 (500 and 18 μm) recorded by the Cassini Composite Infrared Spectrometer (CIRS) yield the spectral dependence and the vertical distribution of Titan’s photochemical aerosol and stratospheric ice clouds. Below the stratopause (~300 km) the aerosol appears to be incompletely mixed for the following reasons: 1) the altitude dependence of the aerosol mass absorption coefficient is larger at higher altitudes than at lower altitudes, 2) the aerosol scale height varies with altitude, which implies some kind of layering effect, and 3) the aerosol abundance varies with latitude.

The spectral shape of the aerosol opacity appears to be independent in altitude and latitude below the stratopause, even though inhomogeneities in the abundance appear to be prevalent throughout this altitude region. This implies that aerosol chemistry is restricted to altitude regions above the stratopause, where pressures are less than ~0.1 mbar. The aerosol exhibits an extremely broad emission feature with a spectral peak at 140 cm-1 (71 μm), which is not evident in laboratory simulated Titan aerosols (tholin) that are created at pressures greater than 0.1 mbar.

A strong broad emission feature centered roughly around 160 cm-1 corresponds very closely to those found in nitrile ice spectra. This feature is pervasive throughout the region from high northern to high southern latitudes. The inference of nitrile ices is consistent with the highly restricted altitude ranges over which these features are observed, and appear to be dominated by HCN and HC3N. At low and moderate latitudes these clouds are observed to be located between 60 and 100 km, whereas at high northern latitudes during northern winter these clouds are observed at altitudes between 150 and 165 km. The ubiquitous nature of these nitrile ice clouds is inconsistent with a simple meridional circulation concept, suggesting that the true dynamical situation is more complex.



KEYWORDS: [6281] PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS / Titan, [5405] PLANETARY SCIENCES: SOLID SURFACE PLANETS / Atmospheres, [5422] PLANETARY SCIENCES: SOLID SURFACE PLANETS / Ices.
(No Image Selected)
(No Table Selected)
SPONSOR NAME: Carrie Anderson

Additional Details
Previously Presented Material: Most of the material was published in Icarus 212, 762-778 in 2011.

Contact Details
CONTACT (NAME ONLY): Carrie Anderson
CONTACT (E-MAIL ONLY): carrie.m.anderson@nasa.gov


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Posts in this topic
- Juramike   Atmospheric Chemistry of Titan   May 2 2010, 03:38 AM
- - Juramike   Into the Wierdness: Ion-neutral chemistry (A maj...   May 5 2010, 02:59 AM
- - ngunn   Thanks for that very interesting explanation Mike....   May 6 2010, 11:20 AM
- - Juramike   The radical cationic, carbonium, and carbenium spe...   May 6 2010, 01:50 PM
|- - Littlebit   QUOTE (Juramike @ May 6 2010, 06:50 AM) T...   May 11 2010, 09:22 PM
|- - ngunn   QUOTE (Littlebit @ May 11 2010, 10:22 PM)...   May 11 2010, 09:56 PM
- - Juramike   Cute. To be really, really anal, a radical shoul...   May 12 2010, 12:30 AM
- - Juramike   Purple Haze or Where It’s At A paper by Lavvas et...   May 12 2010, 11:46 PM
|- - rlorenz   QUOTE (Juramike @ May 12 2010, 06:46 PM) ...   May 20 2010, 07:17 PM
- - Juramike   Titan's organic chemistry is driven by photoch...   May 16 2010, 09:52 PM
- - Juramike   Titan's Chaotic Chemistry Titan is a syntheti...   May 18 2010, 12:30 AM
- - Juramike   Many ways to fall Below is a graphic showing an e...   May 20 2010, 04:17 AM
- - Juramike   I agree that the reality is probably a lot more co...   May 21 2010, 05:42 PM
- - Juramike   It turns out that the methane is only part of the ...   May 31 2010, 04:57 AM
- - Juramike   In the presence of N2 or Ar, ionization occurs fir...   Jun 1 2010, 03:36 AM
|- - Littlebit   QUOTE (Juramike @ May 31 2010, 08:36 PM) ...   Jun 1 2010, 07:59 PM
- - Juramike   Nitrogen does get incorporated. It is primarily i...   Jun 1 2010, 08:34 PM
- - Juramike   So what does CH5+ do? Basically(!), not much....   Jun 2 2010, 04:15 AM
- - Juramike   Even on electron quenching of the CH5+ radical, it...   Jun 3 2010, 03:32 AM
- - ngunn   About Titan chemistry, not necessarily atmospheric...   Jun 3 2010, 09:01 PM
- - Juramike   Great catch!! From the press release: ...   Jun 4 2010, 12:38 AM
- - Bill Harris   Mike, This has been a good discussion of the chem...   Jun 4 2010, 10:02 PM
- - Juramike   The low temperatures at the surface and lower atmo...   Jun 4 2010, 10:49 PM
- - Juramike   For the moment, the Clark et al. paper can be foun...   Jun 4 2010, 10:52 PM
- - Juramike   Article in press: Strobel, D.F. Icarus (2010) Art...   Jun 6 2010, 07:58 PM
- - Juramike   H2 is the key reagent that shunts the pathway to t...   Jun 8 2010, 12:43 AM
- - Juramike   Titan’s atmospheric chemistry is driven by sunligh...   Jun 9 2010, 02:16 AM
- - remcook   Starting on Monday: http://fd147.univ-rennes1.fr/a...   Jun 9 2010, 07:04 AM
- - Juramike   Very cool! Here is an EXCEL conditional forma...   Jun 10 2010, 02:58 AM
|- - rlorenz   QUOTE (Juramike @ Jun 9 2010, 09:58 PM) H...   Jun 12 2010, 01:00 AM
|- - Juramike   As requested (twice now) here is a comparison of s...   Aug 25 2010, 01:41 AM
- - Bill Harris   This is mindboggling. The potential scope of the...   Jun 10 2010, 02:31 PM
- - Shaka   Will the final exam be essay or multiple choice?   Jun 10 2010, 11:59 PM
- - Juramike   I'm gonna give away the answers!   Jun 11 2010, 12:30 AM
- - Juramike   Enter the mechanism Over the next several graphic...   Jun 11 2010, 05:51 AM
- - Bill Harris   QUOTE (Juramike @ Jun 10 2010, 07:30 PM) ...   Jun 11 2010, 04:13 PM
- - Juramike   Ethane (C2H6) [CH3CH3] Almost all ethane is for...   Jun 12 2010, 03:40 AM
- - Juramike   Ethylene (C2H4) [H2C=CH2] Ethylene is a key inter...   Jun 13 2010, 03:21 AM
- - Juramike   Acetylene (C2H2) [HCCH] Acetylene has several for...   Jun 14 2010, 02:52 AM
- - Juramike   Methyl acetylene (1-propyne) (C3H4) [CH3CCH] This...   Jun 15 2010, 02:58 AM
- - jekbradbury   QUOTE (Juramike @ Jun 14 2010, 10:58 PM) ...   Jun 15 2010, 07:35 PM
- - Juramike   Whoops. You are right, it is allene not cumene. ...   Jun 15 2010, 10:39 PM
- - Juramike   [Well, whaddya know...cyclopropenone has been dete...   Jun 16 2010, 09:28 PM
- - Juramike   Ethyl radical (.C2H5) [.CH2CH3] - key intermediate...   Jun 17 2010, 01:46 AM
- - Bill Harris   Mike, one thing I notice is that many of the react...   Jun 17 2010, 02:47 AM
- - Juramike   H+?? Dangit. Those should all be H. hydrogen r...   Jun 17 2010, 03:03 AM
- - Bill Harris   Oh, H-radical as in "H-dot"? They look...   Jun 17 2010, 05:08 AM
- - Juramike   Alright y'all, I'm real sorry about this, ...   Jun 19 2010, 03:06 AM
- - Juramike   Propane (C3H8) [CH3CH2CH3] The straightforward ...   Jun 19 2010, 03:21 AM
- - Juramike   Went back and fixed all diagrams in the different ...   Jun 19 2010, 12:45 PM
- - Bill Harris   Looks good, Mike. Sorry to have tossed a monkey w...   Jun 20 2010, 07:18 PM
- - Juramike   Diacetylene (C4H2) [HCC-CCH] - also known as Buta...   Jun 22 2010, 10:59 PM
- - Juramike   1,3-Butadiene (C4H6) [H2C=CHCHCH=CH2] The forma...   Jun 25 2010, 04:39 AM
- - PDP8E   Mike, you had me at H2O pdp8e   Jun 25 2010, 04:52 AM
|- - Juramike   QUOTE (PDP8E @ Jun 25 2010, 12:52 AM) Mik...   Jun 26 2010, 05:00 AM
- - Juramike   1-Butene (C4H8) [H2C=CHCH2CH3] 1-Butene is 1,3-...   Jun 26 2010, 04:57 AM
- - Juramike   n-Butane (C4H10) [CH3CH2CH2CH3] Boring butane c...   Jun 29 2010, 04:03 AM
- - Juramike   Benzene (C6H6) At lower altitudes, benzene is f...   Jun 30 2010, 03:56 AM
- - Juramike   Benzene (C6H6) high altitude ion route At highe...   Jul 1 2010, 12:31 AM
- - Juramike   Structure of Benzenium (C6H7+) This is one of t...   Jul 2 2010, 12:46 AM
- - Juramike   Beyond Benzene - PAH's and Polyphenyls Polyar...   Jul 4 2010, 01:46 AM
- - Bill Harris   The genesis of Titan's atmosphere may be more ...   Jul 8 2010, 12:44 PM
- - Juramike   HCN The incorporation of nitrogen into Titan’s ...   Jul 13 2010, 12:00 AM
- - Juramike   .CN radical - key intermediate The formation of...   Jul 14 2010, 12:11 AM
- - Juramike   Cyanomethlyene carbene [:CH(CN)] A very recent...   Jul 19 2010, 12:03 AM
- - GEmin   QUOTE The first experimental evidence showing how ...   Jul 19 2010, 06:36 AM
- - Juramike   Acetonitrile (CH3CN) There are multiple ways to...   Jul 21 2010, 02:08 AM
- - Juramike   Cyanoacetylene (HC3N) [HCC-CN] The dominant mec...   Jul 22 2010, 01:13 AM
- - Juramike   Cyanogen (C2N2) [NC-CN] According to the Krasno...   Jul 23 2010, 12:17 PM
- - Juramike   Dicyanoacetylene (C4N2) [NC-CC-CN] Two differen...   Jul 25 2010, 04:04 PM
- - Juramike   Acrylonitrile (C2H3CN) [H2C=CHCN] This molecule...   Jul 29 2010, 10:42 PM
- - Juramike   I’ve tried to represent Titan’s chemistry in a sli...   Aug 2 2010, 03:02 AM
- - Juramike   The graphic below shows the pattern of dominant re...   Aug 22 2010, 08:06 PM
- - Juramike   Estimated depths solids vs. liquids from the vario...   Aug 25 2010, 02:25 AM
- - Juramike   A recent DPS abstract discusses some possibilities...   Oct 8 2010, 02:26 PM
- - titanicrivers   Thanks for the discussion and the link Mike. One ...   Oct 8 2010, 03:46 PM
- - Juramike   Most of the formation chemistry seems to be happen...   Oct 8 2010, 05:21 PM
- - Juramike   LPSC 2011 abstract describes continuing efforts to...   Jan 30 2011, 04:07 AM
- - Juramike   Detection of high altitude cirrus clouds in Titan...   Feb 3 2011, 07:01 PM
- - centsworth_II   This gives hope of much greater understanding of T...   Feb 9 2011, 04:32 PM
- - ngunn   Interesting link posted on the Cassini Huygens Yah...   May 10 2011, 10:56 AM
- - Juramike   The Cool Way to PAH's in Titan's Upper Atm...   Jul 3 2011, 12:55 AM
- - scalbers   I saw a talk given at the AGU conference last week...   Dec 11 2011, 08:39 PM
- - Paolo   not sure this is the best topic to post it to, thi...   Jan 5 2012, 10:51 AM


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