Titan's Wind and Unanticipated Temperature Asymmetry

T. Kostiuk; T. A. Livengood; T. Hewagama; G. Sonnabend; K. E. Fast; K. Murakawa; A. T. Tokunaga; J. Annen; D. Buhl; F. Schmuelling

arXiv · astro-ph/0412664

Titan's Wind and Unanticipated Temperature Asymmetry

T. Kostiuk·T. A. Livengood·T. Hewagama·G. Sonnabend·K. E. Fast·K. Murakawa·A. T. Tokunaga·J. Annen·D. Buhl·F. Schmuelling

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Abstract

Saturn's largest satellite, Titan, has stratospheric wind speeds that may be up to ~210 m/sec [1], circling Titan in about a day compared to Titan's slow 16-day rotation. Theoretical models to explain such super-rotating winds are not well constrained [2,3,4,5,6] by observations of Titan or a similar slow rotator, Venus. Titan's stratospheric temperature and the abundance of the important constituent ethane (C2H6) should be zonally invariant due to long photochemical and radiative lifetimes and rapid transport and mixing by high zonal winds. Here, we report new measurements of zonal wind in Titan's equatorial region, including the Cassini Huygens probe entry latitude [7]. Prograde zonal winds of 190+/-90 m/sec are found from Doppler-shifted ethane gas infrared emission near 12 micron wavelength, confirming high wind velocity even near the equator. Surprisingly, we find a temperature difference of 6+/-3 K between the East and West hemispheres of Titan at ~240 km altitude. Common direct processes such as diurnal heating by sunlight do not adequately explain the asymmetry, suggesting other processes, such as unknown atmospheric dynamics, may be responsible. The origin of the temperature difference is enigmatic and currently unexplained.

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T. Kostiuk, T. A. Livengood, T. Hewagama, G. Sonnabend, K. E. Fast, K. Murakawa, A. T. Tokunaga, J. Annen, D. Buhl, F. Schmuelling. 2004-12-29. Titan's Wind and Unanticipated Temperature Asymmetry. https://arxiv.org/abs/astro-ph/0412664

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