Jupiter loses a stripe – 11 May 2010 – New Scientist.
Losing a stripe seems rather careless for a Giant Planet, but that’s what Jupiter has done. Why? First let’s look at what Jupiter’s bands are made of. The white, almost featureless cloud deck that has replaced the stripe is composed probably of ammonia ice-clouds and virtually all the cloud on Jupiter is the same. Neither hydrogen or helium can condense as clouds on Jupiter so most of the atmosphere is actually clear gas. The small fraction of gases that can condense do all the colouring and feature-making on all the gas giants.
Neptune & Uranus generally show very few clouds because they’re too cold for hydrogen compounds like methane, ammonia and water to condense at visible levels – only occasional methane ice clouds provide most of the visible features. Saturn is a bit warmer, but it seems to be “blanded out” because of the cold too. More visible clouds appear, but deeper in the atmosphere and so they’re more obscure.
Jupiter has a richer palette because it is warmer. We’ve met the immense ammonia ice-cloud canvas, but adding colour are trace organic, phosphorus and sulfur compounds. These produce the sometime vivid colours dredged up from deep down in Jupiter’s innards. Now it seems the source of colour has shifted or has been depleted and one of Jupiter’s colour bands is gone.
SO why the shift? We really don’t know. Jupiter is being mysterious and any “explanation” is currently just speculation, informed or otherwise. No doubt wacky theories will emerge to ‘muddy’ the picture, but there’s no way of knowing without actually going…