I saw an article last night about gravitational waves, that a black hole merger was detected by not just the Laser Interferometer Gravitational Wave Observatory (LIGO), but by another project altogether, the Virgo collaboration. This is the first gravitational wave detection confirmed by two separate groups, and it marks the beginning of a new era of experimental science, the first in astronomy in over two decades. Around 1.8 Billion years ago, to black holes merged in a faroff galaxy. They had masses of 31 and 25 times that of the Sun, though with their incredible density they would each be...
The closest star to the Earth, aside from the Sun, is Proxima Centauri, a small red dwarf star that is part of the Alpha Centauri system, roughly 4 light years away. If you don’t know light years, the distance is a staggering 37,800,000,000,000 Km. Beyond that our stellar neighbourhood fills in as you move 20 light years in any direction, and by 100 light years, there are dozens of stars around us. This gives a stellar density of about 0.14 stars per cubic parsec (a parsec is about 3.26 light years), pretty normal in terms of the number of stars in a given...
Neutron stars are the most extreme objects in the universe that have been proven to exist. Black holes are very likely, but we’re still not 100% sure about them. A black hole is like a giant squid in the ocean. We’re pretty sure they exist, but nobody has caught one. The neutron star on the other hand is like a blue whale, everybody knows they exist, and they are massive, rare, and beautiful. Of course, once we know something exists, the next logical step is to figure out how it behaves, to characterize and generalize it, and to identify where it’s...
Black holes form when a massive star runs out of fuel. Gravity causes the core to collapse down to an object so dense that light itself can not escape. In the Milky Way galaxy, there are expected to be over 100 Million black holes, though of course we can’t see them. The one we can see is the supermassive black hole Sag A*, lying deep within the core of the galaxy. But how did Sag A* form? Was it from the merger of many smaller black holes? Or is there some other process forming the most enigmatic objects in the...
One of the first things you hear when learning about the states of matter is about good old H2O: Steam, Water, Ice. Naturally you are asked “Why does Ice float?” The answer is a simple matter of density, frozen water is less dense because water expands when it freezes. You can do a bit of an experiment by filling a balloon with water. Paint the balloon and put it in the freezer. When it freezes the water will expand, and so will the rubbery balloon, but the dried paint will crack at weak points. This is exactly the same thing...
A few hundred million years after the big bang, the first stars formed. We aren’t exactly sure how, but we do know that they contained Hydrogen, Helium, and a little bit of Lithium. These were the only elements in the entire universe at the time. Within these first stars, the fusion of heavier elements began. Oxygen, Nitrogen, Carbon, Iron, and all the other elements that make up everything we know formed Billions of years ago in these first stars and in their progenitors. It was a slow process to produce these elements and seed them throughout the cosmos, but over...
This past week, American astronaut Scott Kelly, currently on a one year stint aboard the International Space Station, broke the record of 363 days for most time logged in Space by an American. Kelly will continue to run up the tally, as he is just over halfway through his one year mission. His record comes from a total of four space missions, including two Shuttle missions and two ISS stays. While Kelly continues his mission to determine the long term effects of space flight on humans, his fellow ISS astronaut Andreas Mogensen has been testing a new skin suit developed...
It’s hard to do experiments in space. It costs a boatload of money, takes years of preparation, and even then we can’t get much further than low-Earth orbit. But there is a cheaper alternative to understanding the universe. We can perform experiments on Earth to simulate what happens far beyond our own planet. That’s just what scientists did at the Vertical Gun Range at NASA’s Ames Research Center in California. They found that Ceres is likely a mish-mash of celestial bodies from several billion years of bombardment. Until March of this year, when the Dawn spacecraft entered orbit of the...
For a long time, the scientific community has been hopeful for a mission to some of the most interesting moons of the solar system. Europa, Enceladus, and Ganymede all have subsurface oceans and will give substantial insights into the formation and evolution of life in the solar system and beyond. The only problem is that it costs an astronomical (literally) amount of money to get there. A bare bones mission to Europa would cost over 600 Million dollars, and if we are spending that much we had better be sure it will work. Money aside, the technology to get appropriate...
The Cosmic Microwave Background Radiation (CMBR) started out as static in a communications lab in New Jersey where it was discovered by Penzias and Wilson in 1964. Since then it has proven to be an extremely powerful tool for determining the structure and age of the Universe. It helps us constrain cosmological models, gives us insight into the inflationary period of the Universe, and tells us where to look for the largest and smallest structures of the Universe. The temperature fluctuations seen in the CMBR are so small they can only be quantified in millionths of a degree. Yet these...
