Tracking clouds on Venus
Tracking clouds on Venus

The fast winds of Venus are getting faster

18 June 2013

The most detailed record of cloud motion in the atmosphere of Venus chronicled by ESA’s Venus Express has revealed that the planet’s winds have steadily been getting faster over the last six years.

Venus is well known for its curious super-rotating atmosphere, which whips around the planet once every four Earth days. This is in stark contrast to the rotation of the planet itself – the length of the day – which takes a comparatively laborious 243 Earth days.

By tracking the movements of distinct cloud features in the cloud tops some 70 km above the planet’s surface over a period of 10 venusian years (6 Earth years), scientists have been able to monitor patterns in the long-term global wind speeds.

When Venus Express arrived at the planet in 2006, average cloud-top wind speeds between latitudes 50º on either side of the equator were clocked at roughly 300 km/h. The results of two separate studies have revealed that these already remarkably rapid winds are becoming even faster, increasing to 400 km/h over the course of the mission.

“This is an enormous increase in the already high wind speeds known in the atmosphere. Such a large variation has never before been observed on Venus, and we do not yet understand why this occurred,” says Igor Khatuntsev from the Space Research Institute in Moscow and lead author of the Russian-led paper to be published in the journal Icarus.

Increasing wind speeds on Venus
Increasing wind speeds on Venus

Dr Khatuntsev’s team determined the wind speeds by measuring how cloud features in images moved between frames: over 45 000 features were painstakingly tracked by hand and more than 350 000 further features were tracked automatically using a computer programme.

In a complementary study, a Japanese-led team used their own automated cloud tracking method to derive the cloud motions: their results are to be published in the Journal of Geophysical Research.

On top of this long-term increase in the average wind speed, however, both studies have also revealed regular variations linked to the local time of day and the altitude of the Sun above the horizon, and to the rotation period of Venus.

One regular oscillation occurs roughly every 4.8 days near the equator and is thought to be connected to atmospheric waves at lower altitudes.

But the research also unveiled some harder-to-explain curiosities.

“Our analysis of cloud motions at low latitudes in the southern hemisphere showed that over the six years of study the velocity of the winds changed by up 70 km/h over a time scale of 255 Earth days – slightly longer than a year on Venus,” says Toru Kouyama from the Information Technology Research Institute in Ibaraki, Japan.

The two teams also saw dramatic variations in the average wind speeds between consecutive orbits of Venus Express around the planet.

In some cases, wind speeds at low latitudes varied such that clouds completed one journey around the planet in 3.9 days, while on other occasions they took 5.3 days.

Scientists currently have no explanation for either of these variations, or for the long-term overall increase in wind speeds.

“Although there is clear evidence that the average global wind speeds have increased, further investigations are needed in order to explain what drives the atmospheric circulation patterns that are responsible, and to explain the changes seen in localised areas on shorter timescales,” says Håkan Svedhem, ESA’s Venus Express Project Scientist.

“The atmospheric super-rotation of Venus is one of the great unexplained mysteries of the Solar System. These results add more mystery to it, as Venus Express continues to surprise us with its ongoing observations of this dynamic, changing planet.”

Notes for Editors

Related papers:

“Cloud level winds from the Venus Express Monitoring Camera imaging,” by I. Khatuntsev et al., is accepted for publication in the journal Icarus. doi:10.1016/j.icarus.2013.05.018.

“Long-term variation in the cloud-tracked zonal velocities at the cloud top of Venus deduced from Venus Express VMC images,” by T. Kouyama et al. is accepted for publication in the Journal of Geophysical Research – Planets,118, 37–46, 2013 doi:10.1029/2011JE004013.

The observations were carried out using the Venus Monitoring Camera (VMC; principal investigator W. Markiewicz, MPI-Ae, Katlenburg-Lindau, Germany). The VMC is a wide-angle multichannel camera that takes images in the near-infrared, ultraviolet and visible wavelengths.

For further information, please contact:

Igor Khatuntsev
Space Research Institute of the Russian Academy of Sciences, Moscow, Russia
Email: khatuntsev@iki.rssi.ru

Toru Kouyama
Information Technology Research Institute, National Institute of Advanced Industrial Science and Technology, Ibaraki, Japan
Email: t.kouyama@aist.go.jp

Håkan Svedhem
Venus Express Project Scientist
Tel: +31 71 565 3370
Email: h.svedhem@esa.int

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