A survey of data and publications relating to

Titan Atmospheric Chemistry Studies

Table 1: Titan Atmospheric Chemistry Simulation Experiments

Reference Pressure Initial Gas Mixture Discharge Temp System k-value at 0.5 mm C/N C/H Chemical properties
Khare et al., 1984a 0.20 hPa 10% CH4, 90% N2 DC glow 300 K flow 0.04 1.94a 0.6a Less aliphatic C-H, amines, nitriles (IR)
Aromatics and N heteroaromatics (Py-GC/MS)b
2-4 rings PAHs (L2MS)c
Khare et al., 1987 0.13 hPa 100% CH4 RF glow 300 K flow 0.00108 - 0.00375   0.71d Aliphatic C-H, (N-H or O-H due to leak?) (IR)
  0.13 hPa 7% CH4, 93%H2 RF glow 300 K flow 0.0014 - 0.0027   0.66d  
  0.13 hPa 3% CH4, 25%He, 72%H2 RF glow 300 K flow 0.0044 - 0.035   0.57d No CH, 1050 cm-1 (Si-O, glass contamination?) (IR)
McDonald et al.,1994 2 hPa 10% CH4, 90% N2 RF glow 300 K flow   1.5e 0.6e Aliphatic C-H, amines, nitrile, double bonds (IR)
  1 hPa 0.1% CH4, 99.9% N2 RF glow 300 K flow   0.75 0.6 No nitriles, weak C-H, amines, double bonds (IR)
Coll et al., 1995 900 hPa 11% CH4, 89% N2 spark ~100 K closedf   11 1  
McKay, 1996 103 hPa 10% CH4, 90% N2 spark 300 K flow   5.5 1  
Coll et al., 1999 ~2 hPa 2% CH4, 98% N2 DC glow 100 - 150 K flow   2.8 0.8 Aliphatic C-H, amines, nitriles (IR)
                  No aromatic except benzene (Py-GC/MS)
Ramirez et al., 2002 ~1 hPa 2% CH4, 98% N2 DC glow 300 K flow 0.0034      
Khare et al., 2002 71 hPa 10% CH4, 90% N2 RF discharge 300 K closedg       Aliphatic C-H, amine, nitrile double bonds, rings (IR)
Imanaka et al., 2004 0.13 hPa 10% CH4, 90% N2 RF glow 300 K flow 0.031 1.45 0.75 No aliphatic C-H, amines, nitriles (IR), abundant aromaticsh
Imanaka et al., 2004 0.26 hPa 10% CH4, 90% N2 RF glow 300 K flow 0.032 1.78 0.80 Less aliphatic C-H, amines, nitriles (IR), abundant aromaticsh
Imanaka et al., 2004 0.67 hPa 10% CH4, 90% N2 RF glow 300 K flow 0.014 1.85 0.80 Aliphatic C-H, amines, nitriles (IR), abundant aromaticsh
Imanaka et al., 2004 1.6 hPa 10% CH4, 90% N2 RF glow 300 K flow 0.0047 1.97 0.79 Aliphatic C-H, amines, nitriles (IR), less aromaticsh
Imanaka et al., 2004 23 hPa 10% CH4, 90% N2 RF glow 310 K flow 0.0018 2.76 0.73 Aliphatic C-H, amines, nitriles (IR), much less aromaticsh
a Sagan et al., 1984
b Khare et al., 1984b; Ehrenfreund et al., 1995
c Sagan et al., 1993
d Elemental analysis (Khare, unpublished data)
e Data from Sagan et al. (1984)
f CH4 partial pressure maintained as 13 hPa
g Periodic supply of N2/CH4 for every 2 hr
h Abundance and size of aromatics are inferred from IR and UV/VIS spectroscopy, Raman spectroscopy, mL2MS

 

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