I really enjoy looking at images of the Sun from one of the several round-the-clock monitoring systems. It’s fascinating that the public can get access to almost real time images of the Sun and see what’s going on in several wavelengths. I’ve always hoped to see what other stars look like in the future, and today, that future is one step closer. Here’s a brand new picture of another star! This is a real image of distant star π1Gruis, a star 350 times as massive as the Sun, in the southern hemisphere constellation Grus. The star is 530 light years...
I’ve written many times about the power of looking at different wavelengths of light to study different properties of the universe. From a visualization standpoint, there are other techniques that give you additional power when imaging. More than just the wavelength of light you’re using to show the detail, you can choose the range of wavelengths to bring forward certain features while suppressing others. The aptly-named spaghetti nebula, shown above, is a great example of this. A supernova remnant that covers the constellations Taurus and Auriga, the nebula is very large in the sky, covering three full moons worth (love that unit...
A supernova is the death blast of a giant star, far larger than our Sun. Massive stars go out with a bang, outshining entire galaxies, allowing us to see them across the universe. A supernova observed in 2013 occurred in a distant galaxy and took over 30 Million years to reach Earth, where the timing was perfect for us to observe and study it. And now that it’s been studied, the explosion was truly the death of a giant. The supernova, named 2013 ej, was discovered in June 2013 in the galaxy M74 in the constellation Pisces. It was the closest supernova...
Remember last week when I was talking about the evidence for some ancient-but-astronomically-recent supernovae? It turns out there is other evidence! Evidence that has helped scientists narrow down the potential source locations. Data from the Cosmic Ray Isotope Spectrometer (CRIS), an instrument aboard NASA’s Advanced Composition Explorer (ACE) spacecraft, has helped us figure out where the recent supernovae might have come from. CRIS measures what we call cosmic rays, atomic nuclei that have been accelerated across the galaxy at close to the speed of light. CRIS has been around for a while, and through 17 years of cosmic ray observations,...
If a supernova were to go off somewhere in our galaxy, the minimum safe distance for Earthbound life would be about 50 light years. Any closer than that, and we would experience an intense blast of high energy radiation and an eventual shower of radioactive particles. It would be like nuclear bombs were set off all around the Earth, causing little destruction but a lot of radioactive fallout. Supernovae are incredibly powerful to be able to cause such damage at 50 light years, but even at larger distances, we can see evidence of their effects here on Earth. A team of...
I saw this pop up on Reddit yesterday, where user /u/bubbleweed posted a video to r/astronomy showing Jupiter with a clear sign of an impactor. It was independently observed in Austria at the exact same time. Notice that both videos show the exact same thing. In the reddit thread, users encourage the original poster to report it to the Planetary Virtual Observatory and Laboratory in hopes of getting follow up from the Hubble telescope. It is strikingly similar to a 2010 confirmed impact event. The ‘explosion’ of the potential impactor might make you think it’s fake, that it couldn’t explode because...
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....
The most violent single event in the universe is the death of a massive star, a supernova. We have seen several different types, though the common element is a massive explosion, taking a star hiding amongst the background into an eruption that outshines it’s entire host galaxy. We have seen the brightness grow and fade over the duration of a supernova event, but we have never seen one just as it’s starting. Until now. Would you ever have thought that the Kepler space telescope, a planet hunter that continuously observes stars, could see supernovae? The key is in the words ‘continuously observed.’ By keeping...
Today, the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) is expected to announce a monumental discovery that is 100 years in the making. Theorized by Einstein’s general relativity in 1915, gravitational waves are ripples in space-time, similar to sound waves, but much tinier. The search has been ongoing for decades, with no results. Until now. LIGO has the most sensitive gravitational wave detector ever conceived – in two interferometer facilities in Livingston, Louisiana and Hanford, Washington. They use a laser split along two axes to give an in-phase beam. If gravitational waves along one of the axes affect the beam, it...
If you listen to an astronomer talk about a supernova, you’ll probably hear something along the lines of ‘A massive explosion of a massive star that is bright enough to outshine an entire galaxy.’ You can imagine how bright it might be, but it doesn’t really give you enough context to get the wow factor from it. Carl Sagan always said ‘When you make the finding yourself – even if you’re the last person on Earth to see the light – you’ll never forget it.’ Now you, dear reader, have the chance to make the discovery yourself. A series of images of galaxy...
