Exoplanets are light years away, hidden by their parent stars, and barely detectable. Yet even though most have never been directly imaged, we can study the light from the parent star as the planet passes in front of it, and use this information to learn about the planet’s size and composition, especially if it has an atmosphere. Once you know a little bit about how big and dense a planet is, and the major elements that form it’s crust and atmosphere, you can do a lot of Chemistry to figure out what it should be made of and how these...
The Rosetta orbiter, currently studying comet 67P/Churyumov-Gerasimenko as it orbits the Sun, has been watching how the comet has changed as it moves toward its perihelion (point of closest approach to the Sun) in August of 2015. As the comet heats up from the increasing intensity of the Sun’s rays, it releases surface gases and dust into what eventually becomes the atmosphere-like coma surrounding the comet. As the comet moves the material produces the visible tail that we usually associate with a comet. With 67P specifically, Rosetta has recently made a surprising discovery: That the water and carbon dioxide streaming...
It’s been an amazing week for detection and study of water in our Solar system. Just last week we received the first results of the Rosetta mission’s analysis of water from comet 67P. Now we’ve received the latest breakthrough from the Curiosity Rover on Mars, results on Water, Methane, and even Organic material! The Sample Analysis at Mars instrument (SAM) took measurements of the Martian atmosphere over a period of 20 months, and for two of these months in late 2013 and early 2014, the Methane levels were 10 times as high as measurements before and after the spike. “This temporary...
