We just saw it. Another record breaker. This incredible explosion of a massive dying star is the brightest supernova ever observed. You may think you get how big this explosion was, but it was brighter than collective brightness of all the 400 Billion stars in the Milky Way. You may be asking why you can’t see it in the sky. Well even though it is incredibly bright, it is 3.8 Billion light years away in a distant galaxy, so the discovery needed a huge telescope. It may have been powered by a rare star called a magnetar, a star with such an...
You may have heard about the leaked rumour about the discovery of gravitational waves from earlier this week. It was from Lawrence Krauss, who is an amazing science communicator and author, as well as a darn good astrophysicist. My earlier rumor about LIGO has been confirmed by independent sources. Stay tuned! Gravitational waves may have been discovered!! Exciting. — Lawrence M. Krauss (@LKrauss1) January 11, 2016 It’s safe to say that as a guy with an inside scoop on a lot of the latest science news, this is something to get excited about. The ‘LIGO’ he is referring to stands...
The Crab Nebula, as it’s commonly known, is connected to one of the earliest recorded supernova explosions. In 1054 AD, Chinese Astronomers saw the explosion of this supernova as an incredibly bright star in the sky lasting about two weeks, before fading. Now, nearly 1000 years later, the explosion is still happening as an expanding shock front rich in heavy elements moves through the interstellar medium. When the shock front hits dust or gas it is slowed down, giving the resulting nebula a unique shape. In this case, it looks like a crab. The supernova wasn’t exactly the death of the original...
We know that galaxies like our Milky Way are far more massive than we can see. The dark matter in the Milky Way makes up 90% of it’s total mass. Another way of saying this is the Mass to Light ratio, comparing the total mass inferred by the rotation speed of the galaxy to the total mass of stars in the galaxy. This ratio, M/L, for the Milky Way, is about 10. But for a galaxy cluster, the M/L ratio is more like 100. Galaxy clusters are not just dense collections of stars and massive galaxies, they are also immense...
When Isaac Newton quantified gravity, his theory explained how everything in the world around us behaved in its presence. It opened a door to an understanding of something fundamental, yet elusive in explanation. Centuries later, Einstein came along and took a step back, finding a larger more comprehensive theory of gravity, one that explained the strange things that happen in the grand universe. His theory could even explain things that Newton’s theory of gravity could not, such as the odd orbit of Mercury around the Sun. But the greatest part of Einstein’s theory is that if you use it to...
For the first time in 30 years, the United States has the capability to produce fuel for deep space missions. Plutonium-238 is an isotope that produces thermal energy through radioactive decay. This energy can be converted into electricity and used to power spacecraft systems for decades of flight. Systems using this isotope include the Viking landers, the Voyager spacecraft, and more recent missions like the Mars Science Laboratory (Curiosity) and New Horizons. The Oak Ridge National Laboratory in Tennessee, run by the US Department of Energy, has produced 50 grams of the isotope, amounting to the size of a golf...
Gas giants, like Jupiter, Saturn, or some of the largest exoplanets, are mostly made of Hydrogen gas. The simplest and most abundant element in the universe, Hydrogen easily reacts to form compounds, especially at higher temperatures, making it hard to contain and work with. It’s essential to understand how it behaves across a range of temperatures and pressures so that we can understand the interiors of stars and planets. But there may also be applications closer to home, like the white whale of materials science, a room temperature superconductor. A team of researchers from Osaka University and Tokyo Institute of...
We are reaching the point in our study of exoplanets, planets orbiting other stars, where the atmospheres of distant worlds are within the limits of our technology. Once we could barely see the wobble of a star, the telltale sign of an exoplanet, and now we can see reflected starlight and study a distant atmosphere. Now we can probe deeper questions, are atmospheres of exoplanets similar to solar system planets? What are they made of? Do other solar systems have the same raw materials as ours? Do they have what we believe to be the raw materials for life? A...
The only reason we can see black holes in the universe is because some of them swallow up gas and dust. This heats up material that is spinning rapidly around the black hole as it falls in (called an accretion disk), and produces massive jets of material due to conservation of angular momentum that can be seen across the universe. The energy released in the jets and the energy given off in the accretion disk are proportional to how much gas and dust is being consumed by the black hole. More matter = more food = more energy released. But...
Our species is just now reaching the technology necessary to detect features of exoplanets, and not just the exoplanets themselves. We have seen atmospheres, aurorae, and magnetism on distant worlds, and now we can add incredibly fast winds to that list. A team of astronomers have discovered an exoplanet, classified as HD 189733b, that has wind speeds exceeding 8,500 km / h, or about 2 Km / s. Lead researcher Tom Louden, of the University of Warwick’s Astrophysics group, said: “This is the first ever weather map from outside of our solar system. Whilst we have previously known of Wind on...
