... through the cloud, yielding clues to the chemical composition of the cloud. Combined ultraviolet and radio observations correlate to the cloud's infall velocities, providing solid evidence that the spectral features link to the cloud's dynamics...
...a structure has been seen in a molecular cloud. And, after reconstructing the chemical state and the evolutionary history of the cloud, the team, whose lead author on the research paper is Pei Zuo from the Chinese Academy of Sciences in Beijing, have...
... patchy ones, are present in its cool atmosphere. However for an object as cool as 700 K, the origin of the cloud coverage has been somewhat puzzling to scientists. 51 Eri b orbits 51 Eridani, a pre-main-sequence F dwarf that is only 20 ...
... – 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...
... radio waves that can penetrate through the thick cloud layers. The data from Hubble and Gemini can tell us how thick the clouds are and how deep we are seeing into the clouds," Simon explained. By mapping lightning flashes detected...
... 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...