REPORTS
15. N. Lühmann, R. Panisch, T. Müller, Appl. Organomet.
transform to the desired products 15 and 17. supports the observation that a more electron-rich
Additional silylium carborane and silane, plus arene accelerates the reaction.
Chem. 24, 533 (2010).
16. S. J. Blanksby, G. B. Ellison, Acc. Chem. Res. 36, 255
(2003).
extra hours of stirring, were required to achieve
The proton is likely the universe’s oldest cata-
a higher yield. Treatment of substrate 18 afforded lyst, and it is now available as a crystalline arenium
a yield of 51%; the lower yield was probably carborane (25). Coupled to a neutral silane as fuel,
17. Y.-R. Luo, Comprehensive Handbook of Chemical Bond
Energies (CRC Press, Boca Raton, FL, 2007).
18. S. Duttwyler et al., Angew. Chem. Int. Ed. 49, 7519
(2010).
caused by decomposition of the product (19).
arenium acids are competent catalysts for the long-
The terphenyl substrates containing a methyl sought phenyl cation–based Friedel-Crafts reac-
group on the nonfluorinated phenyl ring (10b and tivity. Such C–F activation for the formation of
12) showed a mixture of ortho and para products. arene-arene bonds complements transition metal–
The distribution was slightly in favor of the para based arene-arene couplings, particularly for the
position, which should be more accessible; how- formation of designed graphenes and higher-order
ever, the small preference for the para methyl in- polynuclear aromatic hydrocarbon–based mate-
dicates a very reactive intermediate that does not rials. Understanding the science of silyl cations
19. C. A. Reed, Z. Xie, R. Bau, A. Benesi, Science 262, 402
(1993).
20. J. B. Lambert, W. J. Schulz, J. A. McConnell, W. Schilf,
J. Am. Chem. Soc. 110, 2201 (1988).
21. C. Eaborn, J. Chem. Soc. (Resumed), 3148 (1953).
22. C. Eaborn, J. Chem. Soc. (Resumed), 4858 (1956).
23. C. Eaborn, J. Chem. Soc. 100, 43 (1975).
24. C. A. Reed, J. Chem. Soc. Chem. Commun. 2005, 1669
(2005).
25. See supporting material on Science Online.
26. J. B. Lambert, S. Zhang, S. M. Ciro, Organometallics 13,
2430 (1994).
27. S. Körbe, P. J. Schreiber, J. Michl, Chem. Rev. 106, 5208
(2006).
28. T. M. Douglas, E. Molinos, S. K. Brayshaw, A. S. Weller,
Organometallics 26, 463 (2007).
29. C. A. Reed, Acc. Chem. Res. 31, 133 (1998).
30. M. Juhasz, S. Hoffmann, E. Stoyanov, K. C. Kim,
C. A. Reed, Angew. Chem. Int. Ed. 43, 5352 (2004).
31. A. Nicolaides, D. M. Smith, F. Jensen, L. Radom, J. Am.
Chem. Soc. 119, 8083 (1997).
distinguish strongly between the two positions.
and phenyl cation–like intermediates at play here,
Additional studies enabled us to make a along with the design of tailored precursors, will
qualitative statement on the reaction rate. The certainly lead to a useful expansion of the syn-
terphenyl substrates (8, 10a, 10b, and 12) were thetic chemist’s tool box and the material chem-
used in competitive C–F activation reactions. ist’s objects of investigation.
Two substrates were added to the same reaction
mixture with only half an equivalent of reagent.
Gas chromatography–mass spectrometry (GC-
MS) consistently showed that substrates con-
taining methyl groups (at any of the two rings)
reacted faster than did the electron-poorer rings
without substituents. The tendency of reaction
rates for different substrates was found to be 8 >
10a ≈ 10b > 12 (25). This observation matches
with the proposed transition state A. Its positive
charge would be stabilized by an increased elec-
tron density of the fluorophenyl ring, provided by
an additional substituent such as the methyl group.
Methylation of the donor arene had the same ef-
fect on the reaction rate.
For the transformation of substrate 2, quan-
tum mechanical calculations predicted a transi-
tion state for the fluoride abstraction (Fig. 2) that
nearby aryl moieties can stabilize (18, 25). The
structural and activation parameters predicted
by the quantum chemical model (calculated Ea =
19.8 kcal mol–1; transition-state interatomic lengths,
C–F = 2.55 Å, C–C = 2.86 Å) fit well with the
experimental findings (34). The model further
References and Notes
1. G. A. Olah, Friedel-Crafts Chemistry (Wiley, New York,
1973).
2. R. M. Roberts, A. A. Khalaf, Friedel-Crafts Alkylation
Chemistry: A Century of Discovery (Dekker, New York,
1984).
3. H.-G. Franck, J. W. Stadelhofer, Industrial Aromatic
Chemistry (Springer-Verlag, Berlin, 1988).
4. R. F. Heck, J. Am. Chem. Soc. 90, 5518 (1968).
5. Z. Rappoport, P. Stang, Eds., Dicoordinated Carbocations
(Wiley, New York, 1997).
6. J. Hassan, M. Sévignon, C. Gozzi, E. Schulz, M. Lemaire,
Chem. Rev. 102, 1359 (2002).
7. D. Alberico, M. E. Scott, M. Lautens, Chem. Rev. 107, 174
(2007).
8. N. Miyaura, A. Suzuki, Chem. Rev. 95, 2457 (1995).
9. H. Amii, K. Uneyama, Chem. Rev. 109, 2119 (2009).
10. V. P. W. Böhm, C. W. K. Gstottmayr, T. Weskamp,
W. A. Herrmann, Angew. Chem. Int. Ed. 40, 3387 (2001).
11. The action of SbF5 on perfluorinated naphthalene forms
radical cations capable of coupling with pentafluorinated
benzene, albeit with limited substrate scope; see (35).
12. Flash vacuum pyrolysis appears to facilitate the lysis of
C(aryl)–F bonds and thereby promote arene-arene
coupling; see (36).
32. R. Scholl, C. Seer, R. Weitzenbock, Chem. Ber. 43, 2202
(1910).
33. R. Scholl, C. Seer, Justus Liebigs Ann. Chem. 394, 111 (1912).
34. Specific coordination of solvent or counterion is
estimated to have an effect of <5 kcal/mol on activation
parameters, such that the model is still consistent with
a reaction at 80°C over several hours.
35. B. A. Selivanov, Y. V. Pozdnyakovich, T. V. Chuikova,
O. I. Osina, V. D. Steingarts, Zh. Org. Khim. 16, 1910
(1980).
36. K. Y. Amsharov, M. A. Kabdulov, M. Jansen, Eur. J. Org.
Chem. 2009, 6328 (2009).
Acknowledgments: We thank the Swiss National Science
Foundation for financial support.
Supporting Online Material
Materials and Methods
Table S1
References 37 to 45
13. C. Douvris, O. V. Ozerov, Science 321, 1188 (2008).
14. C. Douvris, C. M. Nagaraja, C. H. Chen, B. M. Foxman,
O. V. Ozerov, J. Am. Chem. Soc. 132, 4946 (2010).
3 January 2011; accepted 16 March 2011
10.1126/science.1202432
veals upper cloud features at ~70 to 75 km
altitude (11), thermal infrared observations reveal
cloud structures at slightly lower altitudes of 65
to 70 km and show that the center of the southern
polar vortex has a brightness temperature ~15 K
warmer than a surrounding cold collar (15). The
mean cloud-top altitude is close to 74 km up to
mid-latitudes in both hemispheres but decreases
Venus’s Southern Polar Vortex
Reveals Precessing Circulation
D. Luz,1* D. L. Berry,2 G. Piccioni,3 P. Drossart,4 R. Politi,3 C. F. Wilson,5 S. Erard,4 F. Nuccilli6
Initial images of Venus’s south pole by the Venus Express mission have shown the presence of a
bright, highly variable vortex, similar to that at the planet’s north pole. Using high-resolution infrared
measurements of polar winds from the Venus Express Visible and Infrared Thermal Imaging
Spectrometer (VIRTIS) instrument, we show the vortex to have a constantly varying internal structure,
with a center of rotation displaced from the geographic south pole by ~3 degrees of latitude and that
drifts around the pole with a period of 5 to 10 Earth days. This is indicative of a nonsymmetric and
varying precession of the polar atmospheric circulation with respect to the planetary axis.
1Centro de Astronomia e Astrofísica da Universidade de Lisboa,
Observatório Astronómico de Lisboa, 1349-018 Lisboa, Portugal.
2Departamento de Física, Universidade de Évora, 7002-554
Évora, Portugal. 3Istituto Nazionale di Astrofisica, Istituto
Nazionale di Astrofisica– Istituto di Astrofisica Spaziale e
Fisica Cosmica (INAF-IASF) Rome, 00133 Rome, Italy. 4Labo-
ratoire d’Études Spatiales et d’Instrumentation en Astrophysique,
Observatoire de Paris, CNRS, Université Pierre et Marie Curie,
Université Paris-Diderot, F-92195 Meudon Cedex, France.
5Department of Physics, University of Oxford, Oxford OX1 3PU,
UK. 6INAF–Istituto di Fisica dello Spazio Interplanetario (IFSI)
Rome, 00133 Rome, Italy.
enus has the most extreme atmospheric polar regions in hemispheric spiral-like patterns
circulation of the terrestrial planets, with of clouds (11), where it results in fast rotating,
V
the cloud-level atmosphere spinning on infrared-bright central vortices (12–15).
average 60 times faster than the planet’s surface Although the spiral hemispheric patterns can
*To whom correspondence should be addressed. E-mail:
(1). This superrotation (2–10) extends to both be seen in ultraviolet dayside imagery, which re- dluz@oal.ul.pt
577