Venus puts on variety show among its cloud-tops
September 19, 2019

Studies of the cloud-tops of Venus by JAXA’s Akatsuki spacecraft show striking variety in wind speeds year-on-year and between the planet’s northern and southern hemispheres. The first fine-scale observations of cloud-top temperatures have also revealed a tendency for clouds to converge towards the equator at night, in contrast to poleward circulation seen previously in daytime studies. 

The results, which have been presented today at the EPSC-DPS Joint Meeting 2019 in Geneva, provide new insights into the mystery of why the Venusian atmosphere rotates much faster than the planet itself.

Prof Masato Nakamura, Project Manager of Akatsuki at JAXA, said: “The Venusian ‘super-rotation’ is most pronounced at the tops of Venus’s clouds, making this an important region for understanding the dynamics of the planet’s atmosphere. The Akatsuki mission is in a highly elliptical orbit around Venus that enables the spacecraft to image both the north and south hemispheres of the planet simultaneously.”

An international team of researchers has used advanced cloud-tracking and quality control techniques to analyse with high accuracy the direction and speed of cloud top winds using data collected by the Ultraviolet Imager (UVI) instrument over three years.

The study, led by Prof Takeshi Horinouchi of Hokkaido University, Japan, and Dr Yeon Joo Lee of JAXA/ISAS and TU Berlin, found that the super-rotation speed at the cloud tops not only changes over time but is different in the northern and southern hemispheres. The team also detected planetary-scale atmospheric waves at the cloud tops, which may interact with the super-rotation.

The degree of difference between the hemispheres, or ‘asymmetry’, may be linked to a second mystery at Venus: an as-yet unidentified chemical species in the atmosphere that strongly absorbs ultraviolet radiation from the Sun. 

Prof Horinouchi said: “The asymmetry in super-rotation speeds in cloud tops in the northern and southern hemispheres might be caused by variability in the distribution of the so-called ‘unknown’ ultraviolet absorber, which plays a key role in regulating how much radiation from the Sun that Venus can absorb. Our results provide new questions about the atmosphere of Venus, as well as revealing the richness of variety of the Venus atmosphere over space and time.” 

A separate study has revealed a detailed picture of Venus’s cloud temperatures for the first time on both the dayside and nightside of the planet. A team from the University of Tokyo, Rikkyo University and the National Institute of Advanced Industrial Science and Technology in Japan tracked the development over time of mottled clouds and streaky features in imagery from Akatsuki’s LIR infrared camera. 

The observation of cloud motions throughout the day and night has enabled the team to determine the average circulation in north-south directions and to detect thermally driven tides that create waves in the atmosphere and could play a key role in maintaining the super-rotation.

Mr Kiichi Fukuya of the University of Tokyo, who presented the results at the EPSC-DPS Joint Meeting 2019, said: “The most exciting discovery is the frequent occurrence of equatorward motions on the nightside – this is in contrast to the strong poleward circulation on the dayside we have observed previously at other wavelengths.” 

The findings suggest that there are as-yet unknown processes that are affecting cloud formation and atmospheric dynamics.“Akatsuki team members have been presenting their hottest topics today at the EPSC-DPS Joint Meeting 2019. The main goal of Akatsuki is to understand the Venusian atmospheric dynamics and cloud physics, which is quite different from that of the Earth. As the culmination of these studies, we believe that we will give a definitive answer how the super-rotation is maintained at Venus very near future,” said Prof Nakamura.

Images

Venus dayside synthesized false color image by UVI and IR1 (2016 Apr 25) No.1 A synthesized false color image of Venus using 283-nm and 365-nm images taken by UVI plus 0.90-µm (900-nm) image taken by IR1. Images are colorized as follows: 283 nm → blue; 365 nm → green; 0.90 µm → red. In the 283 nm band observed by UVI, there is an absorption band of sulfur dioxide (SO2). Also, there is an absorption band of an unidentified chemical substance in the 365 nm band. For example, it can be said that the amount of SO2 is relatively low in the bluish areas in this image. © PLANET-C Project Team
Equator-wards motion of clouds on night side. Credit: University of Tokyo.
Pole-wards motion of clouds on day side. Credit: University of Tokyo.
Artist’s impression of the Akatsuki mission. Credit: ISAS/JAXA

Science contacts

Takehiko Satoh
Project Scientist of Akatsuki
satoh.takehiko@jaxa.jp

Masato Nakamura
Project Manager of Akatsuki
nakamura.masato@jaxa.jp

Media contacts

Anita Heward
EPSC Press Officer
+44 7756 034243
anita.heward@europlanet-eu.org
epsc-dps-press@europlanet-society.org

Livia Giacomini
EPSC Press Officer
epsc-dps-press@europlanet-society.org

Adriana Postiglione
EPSC Press Officer
epsc-dps-press@europlanet-society.org

Shantanu Naidu
DPS Press Officer
dpspress@aas.org

During the meeting, the EPSC-DPS Press Office can be contacted on +41 22 791 9617.

Notes for Editors

Europlanet
The Europlanet Society, launched in September 2018, is an organization for individual and corporate members to promote the advancement of planetary science and related fields in Europe. The Society provides Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science. The Europlanet Society is the parent organisation of the European Planetary Science Congress (EPSC).

Europlanet Society website: www.europlanet-society.org
EPSC-DPSC 2019 Joint Meeting 2019 website: www.epsc-dps2019.eu

DPS
The Division for Planetary Sciences (DPS), founded in 1968, is the largest special-interest Division of the American Astronomical Society (AAS). Members of the DPS study the bodies of our own solar system, from planets and moons to comets and asteroids, and all other solar-system objects and processes. With the discovery that planets exist around other stars, the DPS has expanded its scope to include the study of extrasolar planetary systems as well.

The AAS, established in 1899, is the major organization of professional astronomers in North America. The membership (approx. 7,500) also includes physicists, mathematicians, geologists,
engineers, and others whose research interests lie within the broad spectrum of subjects now comprising contemporary astronomy. The mission of the AAS is to enhance and share humanity’s scientific understanding of the universe, which it achieves through publishing, meeting organization, education and outreach, and training and professional development.

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