A Black Eye in a Black Sky

When Charles Messier catalogued 100 different objects in the night sky, he couldn’t have imagined the richness and detail of each one of his individual discoveries, or that we would ever see them in such incredible detail as to understand what they truly are and how they evolve.  But every time I see a new image of a well-known object, I not only see the new and amazing details revealed, I see the next level of technology that enables us to see it in a new light.  This image of Messier number 64 gives me that view. Messier 64 is...

Ghosts of Quasars Past Surround Distant Galaxies

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...

Supernova Remnant Sleuthing: The White Dwarf did it

There are multiple types of Supernovae that have been observed throughout the Universe.  Classifying them is difficult because the conditions of each one are not always similar.  There are now seven different classifications of these stellar explosions, that are divided (and subdivided) by their spectral characteristics.  By studying the light from supernovae, we can determine what type it is, and identify what kind of stellar environment led to its destruction. The supernova remnant 3C 397, shown above in the constellation Aquilla at a distance of 33,000 light years, has thought to have been expanding for 1-2 millennia. Originally thought to have...

Two Supermassive Black Holes are Merging

A vast number of Galaxies in the Universe have a central black hole that is incredibly massive.  The Black Hole at the centre of the Milky Way, dubbed Sag A*, is estimated to have a mass as high as three Million Suns.  We generally can’t see black holes, but when they start to pull in matter from surrounding gas and dust clouds, the material forms a disk around the star.  This accretion disk can heat up to incredible temperatures and emit X-rays and other high energy light, allowing us to see where the black holes are.  Sometimes the light from...

Stars do Collide! And We Saw It!

When I do Planetarium shows, one of the things I like to talk about during the Milky Way – Andromeda collision that will happen in 70 Mlllion years, is the fact that very few stars will actually hit each other.  Yet we still call it a ‘Galaxy collision.’  One of the questions I always get is “Will the Earth survive this?”  I usually ask the audience. The response is usually a unanimous ‘No way!” And then I tell them how big Galaxies are and they can’t believe how unlikely it is that the solar system will be affected.  Consider the...