... – a gas that on Earth can only be produced artificially in a lab – in the clouds of Venus. Since then studies have either overturned the claim or added further intrigue to the finding. But now, a new study measuring water concentration in Venus...
... are shown in red with big features labelled. The red dappling shows the noise in the cube. Figure 4 - All of the discrete clouds detected. The black outline shows the gas disk of M33. All of the clouds are colour coded according to their velocity...
... these regions find it easy to leave the satellite and begin orbiting the host. As more stars leave the satellite, they leave a trace on the sky that reveals the satellite's orbit. "Stellar streams around the Clouds were predicted but never observed...
... of four filaments converging on a central hub, have captured the effects of gravity on ammonia gas moving within the cloud to show how the swirling motion of gas aids in the star formation process. It has been known for some time that stars...
... overly active star formation is that the clouds throughout the galaxy are very unstable, which is not normally the case. Gas clouds keep in equilibrium as long as the inward force of gravity is matched by the outward force of pressure. Once gravity...
... condensation of water), and gases and fresh cloud material dredged up from the deeper atmosphere. Once at the cloud tops, the new material is blown around the planet by the prevailing winds, creating a storm system that evolves from a single white...