One of the big questions in astrophysics is about variation of the laws of Physics. The laws we know and are familiar with; angular momentum, gravity, energy, are the same everywhere on Earth. But what about beyond Earth? The universe is so large and so vast, we may be in a local region where the laws of Physics are set, and our laws may be different from a distinct region somewhere else in the universe. The good news is that we can make predictions based on our understanding of physics. And with our powerful telescopes that allow us to view a variety of...
I love data visualization. If I didn’t love astronomy and explosions so much, I would probably be in the art form of visualizing data in fascinating ways. Who knows? I may change my life’s work some day. A recent APOD takes the art to a new level. By looking at time sensitive measurements of Gamma Rays from an incredible active galactic nucleus (AGN), we can get an idea of how a gamma ray burst comes at us from so far away, and what the difference is between the usual activity and a true burst of radiation. Each circle represents a...
If you could see through the lens of a very powerful telescope, to an area of sky the size of a grain of sand held at arm’s length, a new universe would be revealed to you. For in that tiny patch of seemingly empty sky, there are thousands of galaxies visible, albeit with many hours of light collection. Observing the most distant of these galaxies, at the edge of the universe, allows us to estimate the number of Galaxies present in the distant past, when the universe was very young. As our observations improve, and our ability to simulate the conditions of the...
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...
As we push the limits of our technology, we naturally will find the biggest, the brightest, the smallest, the most extreme, and of course the most distant objects in the universe. We are at the time in history where we are beginning to see the edges of our universe in unprecedented detail. Eventually will will stop finding the biggest, brightest, and most distant, after which point our technology will serve to improve our precision and allow us to peer within these unique objects. Astronomers have used this incredible technology to discover the most distant galaxy in the universe, forming only...
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...
When the first stars and galaxies started to form, it was like a spark of a massive chain reaction where the vast amounts of gas and dust that had clumped together were quickly converted into dense, luminous star clusters. This was the beginning of the formation of the heavier elements that would eventually make up all that we see on the planet Earth. But when did this massive tirade of star formation end? When we look at galaxies in the present epoch, most don’t form stars very rapidly at all, and giant elliptical galaxies are all but devoid of gas,...
The deeper we peer through the cosmos, the more we are looking into the distant past. Light from other galaxies takes millions of years to reach us, and so when that light has finally arrived at Earth, it is millions of years old, a snapshot in time of the distant galaxy. The furthest we can see is so far back in the history of the universe, that galaxies haven’t even formed yet. As we look at the large-scale structure of the Universe, we see it filled with a cosmic web of galaxy clusters, containing tens of thousands of galaxies each....
Our entire universe, from the tiniest atoms, to the structure of our experiential world, to the most massive galaxy clusters and the cosmic web, is dependent on a set of single properties, where small changes to these fundamental numbers would lead to a state where none of it could exist. Understanding these fundamental numbers is the key to unlocking the deepest secrets of the universe and answering the biggest questions of our existence. One of these numbers is the tiny difference in the masses of the proton and neutron. If it varied even a little bit in either direction, we...
The science of Astronomy goes far beyond what humans can see with our eyes. The visible part of the spectrum has taught us so much, but when we look at all photons across the spectrum of light, we find exponentially more powerful methods for discovering the mysteries of the universe. Radio waves, yes the same ones that bring you music in your car, are found throughout the universe in very interesting environments. Radio waves often trace the most powerful objects in the universe, such as super-massive black holes, quasars, and other types of active galactic nuclei. Humans see visible light...
