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...
Ever heard the term ‘champagne flow?’ I’m not talking about a celebration, it’s actually a term in astronomy. When a cluster of massive stars form and ionize the surrounding hydrogen cloud, the hot gas propels itself through the layers of cooler gas at the cluster outskirts. When the hot gas finally bursts through to the vacuum of space, it flows rapidly like a newly opened bottle of champagne. This is exactly what’s happening in the cluster RCW 34, a young, gaseous cluster in the southern constellation Vela. The interesting thing about this cluster is that its nearly invisible in optical...
Have you ever heard of an object called ‘Hanny’s Voorwerp?’ It’s a thin wispy ghost-like blob at the edge of a Galaxy. It was discovered by Dutch schoolteacher Hanny van Arkel in 2007 as she was classifying galaxies as part of the Galaxy Zoo project. Since then, astronomers have been studying its origin, as it was the first of a brand new phenomenon in astronomy. This past week, a new data set of wispy trails at the edge of Galaxies have been released as part of a Hubble study by Bill Keel of the University of Alabama, Tuscaloosa. The new Hubble...
A few months ago I talked about Astronomers seeing the gas cloud known as G2 passing the central black hole of the Milky Way, called Sagittarius A*, and how we had hoped to watch the black hole destroy it in order to learn about the behaviour of supermassive black holes. As we all sat and watched the passage of the cloud over the course of a few months, we were surprised to find that the cloud remained intact and passed straight by Sag A*. When we last checked in, the leading theory was that the ‘cloud’ actually was a dense...
The Sun is the driving force behind our planetary system. It’s energy warms our planet, drives weather and climate patterns, and fuels the aurorae that surround our magnetic poles. The Sun also has a much grander sphere of influence beyond the orbit of the Earth, stretching into the vast space between itself and the other members of the stellar neighbourhood. The charged particles that are released from the Sun, called the solar wind, stretch out to 120 Astronomical Units, about 18 Billion Km. The bubble of the Sun’s influence is known as the Heliosphere, though it is anything but a...
Have you ever heard of the Van Allen belts? If not you really should learn about them. After all, without them the majority of life on Earth could not survive. So what are they and how do they keep us alive? The Van Allen Belts are a collection of charged particles, held in place by the magnetic field of Earth, that act as a barrier to prevent the most harmful radiation from the Sun from reaching the surface of the Earth. They shift according to the incoming energy of the Sun, and if there is a large enough swell of...
Twenty Years of exoplanet research has seen incredible advances in detecting planets orbiting distant stars, as well as their size, orbit period, orbit distance, and even atmospheric composition. But the next step in understanding exoplanets is to learn about their magnetic fields. We know that many exoplanets should have magnetic fields. It makes sense, since nearly every world in our own solar system has some sort of magnetism. But for the first time, an international team of Astronomers, led by Kristina Kislyakova of the Space Research Institute of the Austrian Academy of Sciences, have discovered a way to detect magnetic fields...
