Shock Breakout Visualized

I just released a post about the Kepler Space Telescope and its observation of the shock breakout of an exploding star, the exact moment when it’s considered a supernova.  Further to this I wanted to show some of the great visualizations of the event, and to show you just how energetic and luminous a supernova really is, compared to our Sun.   The video shows the shock breakout, the bright flash lasting an hour, before the star rapidly increases in brightness to it’s maximum.  Not shown is the gradual fading of the supernova, which can take days or even weeks....

Solar Burp

We know that the giant bright light in the sky that keeps us warm is so much more than we can see.  A star, like countless others in the sky, close enough to outshine all of them.  The Sun is a dynamic object, endlessly churning and burping plasma beyond it’s boundaries into the solar system and beyond.  NASA spacecraft and ground-based telescopes have been keeping eyes on the Sun for years to characterize its 11-year magnetic cycle.  And every so often they have a front-row seat to the massive blasts that just can’t be seen with human eyes. The first...

New Gamma Source

Gamma rays are the highest energy photons on the electromagnetic spectrum.  Their wavelength is similar to the size of an atom, and when two of them collide they tend to produce a matter-antimatter particle pair.  They represent energy high enough to synthesize the fundamental particles of matter, and are produced in the highest energy environments in the cosmos.  The interchange of matter and energy works both ways, so one of the ways gamma rays are generated is through annihilation of a matter-antimatter particle pair.  Looking back to the beginning of the universe it gives us the earliest ‘chicken or egg’...

Constellation Series: Orion

Since the dawn of human history, we have looked up into the night sky and found patterns in the stars.  Some of us saw animals, others saw gods and heroes, but we all agreed that they were greater than our simple existence. In this blog series, we will take a deeper look into the constellations that Astronomers use to map today’s night sky.  We will look into the history of each of the 88 constellations and the stars and objects that form them, to discover more about our culture, and our connection with the universe. Our first constellation on the list is bright, large,...

Still More Hidden Galaxies

I’ve covered a few ‘hidden galaxy’ stories lately, from the ultra high resolution see-through of Andromeda, to dark dust in front of M81 and M82.  Now, hundreds of new hidden galaxies have been revealed by a team of astronomers who are looking straight through the Milky Way for the first time ever, shedding light on the structure of new galaxy clusters and the enigmatic pull of the ‘great attractor.’ The Earth is not stationary in space.  It orbits the Sun, which in turn orbits the Milky Way galaxy, which then moves through the Universe as part of a galaxy cluster. ...

Gamma Rays Point to Pulsars, Not Dark Matter

Gamma rays are the most powerful form of electromagnetic radiation in the universe.  With wavelengths as small at atoms, they usually result from the most powerful interactions known, such as the collision of two particles, or the release of energy from the accretion disk of a black hole.  But there is another potential source of gamma rays that has not yet been confirmed: Dark Matter. The leading candidate for dark matter is the theorized Weakly Interacting Massive Particle (WIMP), though it is not as wimpy as its namesake suggests, making up 5 times as much mass as the visible matter...

Potential Ninth Planet!

Sadly no, this time we are NOT talking about Pluto. Astronomer Mike Brown from Caltech, heralded as the ‘man who killed planet Pluto’ has done some new work that might replace Pluto with a better fit for a true ninth planet, one that is ten times the mass of Earth.  Now the only problem is finding it. But wait, if we haven’t seen it, how do we know it’s there? Well it certainly showcases the power of science, that an understanding of the true laws of nature can give us incredible predictive power.  It started out as a ‘that’s strange’...

First Light For Black Hole Observatory

A newly installed instrument on the European Southern Observatory’s (ESO) Very Large Telescope (VLT) has just taken it’s first images, what we call ‘first light’ in the astronomy world.  The instrument, called GRAVITY, uses four different 8m telescopes to perform what we call ‘Baseline Interferometry.’  It is expected that tis is the instrument that will allow humanity to take the first ever direct picture of a black hole. Interferometry is a technique that uses multiple small telescopes all collecting light at a specific wavelength.  These telescopes form a line that we call the baseline.  The combination of these telescopes and...

Dark Matter in a Galaxy Cluster

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...

How You Can See A Black Hole!

Black holes are the most extreme phenomena known in the universe.  They are the absolute limit of what gravity and space-time can be twisted into.  It’s no surprise that some of the most massive and advanced telescopes in the world are tasked with studying their properties and how they interact with their environment.  But maybe there’s a way for you and I to see what a black hole can do, and all we need is a moderate 8 inch telescope and our eyes! Even though black holes generally give off tons of radiation, we need to observe them in the...