ScienceDaily (Sep. 5, 2008) — Venus is a planet similar in size to the Earth. Nevertheless, it is quite different in other aspects. On the one hand, it spins very slowly on its axis, taking 224 terrestrial days and, moreover, it does so in the opposite direction to that of our planet, i.e. from East to West.

Its dense atmosphere of carbon dioxide with surface pressures 90 times that of Earth (equivalent to what we find at 1000 metres below the surface of our oceans), causes a runaway greenhouse effect that raises the surface temperatures up to 450ºC, to such as extent that metals like lead are in a liquid state on Venus. At a height of between 45 km and 70 km above the surface there are dense layers of sulphuric acid clouds totally covering the planet.

It was in the 1960s that they discovered, by means of telescopic observations, that the top level of cloud layers moved very rapidly, orbiting the planet in only four days, compared to the planet’s own orbit of 224 days. This phenomenon was baptised the “superotation” of Venus: the winds carrying these clouds travel at 360 km/h.

The various space missions that explored the planet in the 70s and 80s showed that the “superotation” was a permanent phenomenon and, moreover the probes that descended through its atmosphere indicated that, in a number of places, the winds decreased in speed to zero at Venus’s surface. New observations carried out with the Venus Express mission of the European Space Agency, in orbit around Venus since April 2006, have enabled the team of scientists from the University of the Basque Country (UPV/EHU) to determine in detail the global structure of the winds on Venus at the cloud level while, at the same time, to observe unexpected changes in the wind speeds, which have helped in the interpretation of this mysterious phenomenon.

The team was led by Agustín Sánchez Lavega with team members being Ricardo Hueso, Santiago Pérez Hoyos and Javier Peralta, from the Planetary Sciences Group at the Higher Technical Engineering School of Bilbao.

Novel aspects of the rotation

Using images recorded by both day and night on Venus with the VIRTIS spectral camera on board the Venus Express, the UPV/EHU scientists have succeeded in measuring these clouds over several months and have discovered new aspects of the “superotation”. Firstly, between the equator and the median latitudes of the planet there dominates a superotation with constant winds blowing from East to West, within the clouds decreasing speed with height from 370 km/h to 180 km/h. At these median latitudes, the winds decrease to a standstill at the pole, where an immense vortex forms.

Other aspects of the superrotation that observations with VIRTIS have made possible are that the meridional (North – South) movements are very weak, about 15 km/h, and, secondly, unlike what was previously believed, the superotation appears to be not so constant over time: “We have detected fluctuations in its speed that we do not yet understand”, stated the scientists. Moreover, for the first time they observed “the solar thermal tide” effect at high latitudes on Venus. “The relative movement of the Sun on the clouds and the intense heat deposited on them makes the superotation more intense at sunset than at sunrise”, they stated.

“Despite all the data brought together, we are still not able to explain why a planet than spins so slowly has hurricane global winds that are much more intense than terrestrial ones and are, moreover, concentrated at the top of its clouds” stated Mr Sánchez Lavega. This study has enabled advances to be made in a precise explanation of the origin of superotation in Venusian winds as well as in the knowledge of the general circulation of planetary atmospheres.

Journal reference:

1. Sánchez-Lavega et al. Variable winds on Venus mapped in three dimensions. Geophysical Research Letters, 2008; 35 (13): L13204 DOI: 10.1029/2008GL033817

enlarge

Scientists have determined in detail the global structure of the winds on Venus at the level of the clouds while, at the same time, observing unexpected changes in the wind speeds. (Credit: Image courtesy of Basque Research)

Related Stories

Did A Mega-collision Alter Venus? (Feb. 27, 2008) — A mega-collision between two large embryonic planets could have created Venus as we know it, according to a new paper by a Cardiff University scientist. Venus is a sister planet to Earth. It is ...  > read more

Evolution Of Venus: First Too Fast, Then Too Slow (Apr. 6, 2008) — Scientists analyzing the data from the European Venus Express spacecraft now orbiting Earth's prodigal twin planet have been piecing together an understanding of why the climate on both worlds is so ...  > read more

Tracking Alien Turbulences With Venus Express (Apr. 4, 2007) — New images and data from ESA's mission to Venus provide new insights into the turbulent and noxious atmosphere of Earth's sister planet. What causes violent winds and turbulences? Is the surface ...  > read more

And Now, The Weather: Complex Meteorology On Venus (Oct. 15, 2006) — In its relentless probing of Venus's atmosphere, ESA's Venus Express keeps revealing new details of the Venusian cloud system. Meteorology at Venus is a complex matter, scientists ...  > read more

Climate Catastrophes In The Solar System (Apr. 30, 2007) — Earth sits between two worlds that have been devastated by climate catastrophes. In the effort to combat global warming, our neighbors can provide valuable insights into the way climate catastrophes ...  > read more

Search ScienceDaily

Discovering A New Earth 430 Light Years Away