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Venus Vortices Go For Chaotic Multi-Storey Strolls Around The Poles
Venus Vortices Go For Chaotic Multi-Storey Strolls Around The Poles
24 Mar 2013
(Source: Universidad Del Pais)

The South Polar Vortex of Venus changes its shape day-to-day. The upper panels of the figure show the upper clouds at 63km above the surface and the lower panels present the vortex as observed in the lower clouds at 42km altitude level. Credit: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA/Universidad del País Vasco (I. Garate-Lopez)
The South Polar Vortex of Venus changes its shape day-to-day. The upper panels of the figure show the upper clouds at 63km above the surface and the lower panels present the vortex as observed in the lower clouds at 42km altitude level. Credit: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA/Universidad del País Vasco (I. Garate-Lopez)
Animation constructed from VIRTIS infrared images on orbit 474, showing the short-term morphological evolution of the South Polar Vortex at the lower clouds level, about 42km above the surface. Credit: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA/Universidad del País Vasco (I. Garate-Lopez)
Animation constructed from VIRTIS infrared images on orbit 474, showing the short-term morphological evolution of the South Polar Vortex at the lower clouds level, about 42km above the surface. Credit: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA/Universidad del País Vasco (I. Garate-Lopez)

A detailed study of Venus' south polar vortex shows a much more chaotic and unpredictable cyclone than previously thought. The analysis reveals that the center of rotation of the vortex wanders around the pole differently at different altitude levels in the clouds of Venus. In its stroll around the Pole, in layers separated by 20 km, the vortex experiences unpredictable changes in its morphology. The results of this study are published online in Nature Geoscience today.

The study, entitled "A chaotic long-lived vortex at the southern pole of Venus," used infrared images from the VIRTIS instrument onboard the European Space Agency's Venus Express spacecraft. VIRTIS provides spectral images at different levels of the atmosphere and allows the observation of the lower and upper clouds of Venus.

Atmospheric vortices are common in the atmospheres of different planets of the Solar System, although they have different behaviors. Venus is a planet similar to Earth in size, but very different in other aspects. It rotates slowly around its axis, with a day on Venus lasting 243 Earth-days, and it spins in the opposite direction to Earth. Its dense carbon dioxide atmosphere, with surface pressures of 90 times that of Earth, causes a runaway greenhouse effect that raises the surface temperatures up to 450 degrees C. Between 45 and 70km above the surface there is a dense layer of sulfuric acid clouds that completely covers the planet and moves at speeds of 360km/h in a phenomenon named superrotation, where the atmosphere rotates much faster than the surface of the planet. The origin of this effect is still unknown.

At the poles of Venus, the atmospheric circulation forms intense and permanent vortices that change shape and size on a daily basis. In the new analysis published today, researchers report that the winds in the vortex, which were tracked by studying images obtained by the Venus Express orbiter, change chaotically from day-to-day. This unpredictable nature of the Venus polar vortices make them different from polar vortices found on other planets, like Earth or Saturn, which are much more stable and predictable.

The large-scale cyclone extends vertically in Venus' atmosphere over more than 20 kilometers, through a region of highly turbulent, permanent clouds. However, the centers of rotation at two different altitude levels (42 and 62 km above the surface) are not aligned and both wander around the south pole of the planet with no established pattern at velocities of up to 55km/h. The study also finds that even when averaged cross-winds are roughly the same at both altitudes, there is still a strong vertical gradient, with winds increasing by as much as 3km/h for every kilometer of height and leading to possible atmospheric instabilities

The vortices are fed by the atmospheric superrotation and are trapped in polar regions by a wide, shallow collar of cold air in subpolar latitudes. The eye at the centre of the vortex covers an average area of 2200 kilometres by 1400 kilometres. Despite several years of observations, it is not possible to explain why the vortex is variable enough to alter its shape in just one day, or remain stable for weeks. Thus, along with the origin of the superrotation of the atmosphere, identification of a mysterious source of ultraviolet absorption in the clouds, Venus polar vortices are one of the great mysteries of our twin planet. This study will help for a more precise explanation of the vortex and its relationship with the atmospheric superrotation.

Animation constructed from VIRTIS infrared images obtained over six subsequent days, showing the motion of the South Polar Vortex of Venus around the pole at the upper clouds altitude level, about 63km above the surface. Credit: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA/Universidad del País Vasco (I. Garate-Lopez)
Animation constructed from VIRTIS infrared images obtained over six subsequent days, showing the motion of the South Polar Vortex of Venus around the pole at the upper clouds altitude level, about 63km above the surface. Credit: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA/Universidad del País Vasco (I. Garate-Lopez)

REFERENCE

I. Garate-Lopez, R. Hueso, A. Sánchez-Lavega, J. Peralta, G. piccioni, P. Drossart. A chaotic long-lived vortex at the southern pole of Venus. Nature Geoscience, 24 March 2013, DOI: 10.1038/NGEO1764.

CONTACTS

Itziar Garate-Lopez
Escuela Técnica Superior de Bilbao
Universidad del País Vaso, Spain
Email: itziar.garate@ehu.es
Tel: 00 34 94 601 7389

Ricardo Hueso
Escuela Técnica Superior de Bilbao
Universidad del País Vaso, Spain
Email: ricardo.hueso@ehu.es

Agustín Sánchez-Lavega
Escuela Técnica Superior de Bilbao
Universidad del País Vaso, Spain
Email: agustin.sanchez@ehu.es

Javier Peralta
Observatorio Astronómico de Lisboa (CAAUL)
Instituto de Astrofísica de Andalucía (CSIC)
Email: peralta@iaa.es

Giuseppe Piccioni
VIRTIS-Venus Express PI
Istituto Nazionale di Astrofisica-IASF, Italy
Email: giuseppe.piccioni@iaps.inaf.it

Pierre Drossart
VIRTIS-Venus Express PI
LESIA, Observatoire de Paris, France
Email: pierre.drossart@obspm.fr

FURTHER INFORMATION

Venus Express: http://www.esa.int/Our_Activities/Space_Science/Venus_Express

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Last Updated: 25 Mar 2013