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Venus spot continues to puzzle DR EMILY BALDWIN ASTRONOMY NOW Posted: August 05, 2009 Over two weeks ago a bright white spot appeared in the atmosphere of Venus, but where did it come from? A new report from the Venus Express team sheds some light on the matter. In our initial report of the discovery, amateur observer Frank Melillo who first spied the marking on 19 July commented: "I have seen bright spots before but this one is an exceptionally bright and quite intense area."
Amateur images taken on 19 July by Frank Melillo (top) and George Tasourdis (bottom) show a bright marking in ultraviolet. NB. Tasourdis' image is oriented with south towards the top of the picture, opposite to Melillo's. The spot, thirty percent brighter than 'normal' and 1,000 kilometres wide was soon confirmed by other amateurs, and fortunately the Venus Express Monitoring Camera (VMC) was also looking in the right place at the right time to examine the spot close-up and to monitor its evolution over the coming days. Venus' atmosphere is permanently smeared with white clouds, and the new bright region stuck its head up in one of the southern streaks, which typically spirals in towards the pole as part of the vortex-like circulation pattern that is centred there – rather like water spinning down a plug hole. In the spot's location at a latitude of 50 degrees south, the atmosphere rotates around the planet once every four days – a fair lick compared with Venus' somewhat lethargic 243 day long turn about its own axis. Interestingly, the VMC images reveal the white spot in images captured by the spacecraft four days earlier, albeit dimmer, brightening by the 19 July and suggesting that the event causing the confined marking occurred one atmospheric rotation earlier than Melillo and others first noticed it.
A montage of Venus Express images taken between 11 and 23 July. Image: MPS/ESA. But what caused the cloud properties to change so dramatically? In a new report released last night, and lead by Sanjay Limaye of the University of Wisconsin and Dimitri Titov of the Max Planck Institute in Germany, four possible scenarios are presented: a volcanic eruption, solar wind interaction, an icy comet impact or a previously unseen weather phenomenon.
Volcanic eruption?
A false colour VMC image taken of Venus in 2007, showing a bright confined spot similar to the most recent offering. Image: MPS/ESA.
Solar activity?
Impact?
A composite view of a segment of the hemispheric vortex on Venus (false colour, left) and an Atlantic cyclone (right).
Weather? As it stands with the current information available, it seems that the most likely and natural explanation for the local brightening was caused by perturbations in the atmospheric circulation. "In other words, the observers witnessed Venus weather," concludes the report. |
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