For a long time, the scientific community has been hopeful for a mission to some of the most interesting moons of the solar system. Europa, Enceladus, and Ganymede all have subsurface oceans and will give substantial insights into the formation and evolution of life in the solar system and beyond. The only problem is that it costs an astronomical (literally) amount of money to get there. A bare bones mission to Europa would cost over 600 Million dollars, and if we are spending that much we had better be sure it will work. Money aside, the technology to get appropriate...
Eight minutes after launching from the Baikonur Cosmodrome, a Russian Proton-M rocket experienced a catastrophic failure in its third stage rocket, resulting in the complete atmospheric burn-up of the rocket and its payload, a Mexican Communications Satellite. After launching at 11:47am local time in Kazakhstan, the rocket experienced an emergency situation 497 seconds into the flight, reported as a failure in the rocket’s Breeze-M third stage. The carrier rocket was launching the Mexsat 1 communications satellite, known as Centenario, into orbit, in a contract with the Mexican government. After reaching a 161 Km altitude, the rocket failed and fell back to...
I always love to chat about stories by close-to-home scientists. I just talked recently about some University of Waterloo cosmological work, but today I can follow it up with a very close to home scientist that I’ve run into a few times. Something about seeing the achievements of those you know makes you feel pride too – it gives us all a good reason to support friends, colleagues, and even acquaintances, since we can share in their passion. Astronomer Lisa Esteves, a PhD candidate from the University of Toronto, has been watching exoplanets carefully with the Kepler Space Telescope, seeing...
That’s right it is not always Polaris. Over a human lifetime Polaris will always be our north star, but in the year 14,000, it will be the bright star Vega. This is due to the tilt of the Earth’s axis, which precesses like a spinning top, albeit much more slowly, over a 32,000 year period.
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...
Space Junk is a growing problem. Even though there is a lot of room in low Earth orbit, it’s estimated that 3,000 tons of space debris is floating around at different altitudes and speeds, posing a significant threat to present and future orbital infrastructure. The number of objects classed as space junk doubled in 2014 to 4000 individual pieces, mostly due to collisions between objects already in space. Most of this space junk is old derelict satellites and rocket bodies and engines leftover from 50 years of space exploration. Because of the wide variety of altitudes, trajectories, and speeds, it can...
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,...
We are fairly confident about the idea that the Moon formed when a Mars sized object hit the young Earth over 4 Billion years ago. The resulting debris cloud condensed to form the Moon, giving the Earth a surprisingly large Moon for its size. Next to Charon and Pluto, the Earth’s Moon is the largest relative to the size of its planet. It’s also the third largest of all moons in the Solar System, next to Ganymede and Titan, #1 and #2 respectively. but there is one problem with this theory of the Moons formation: The Earth and Moon are...
On the York Universe radio show this past Monday evening on astronomy.fm, I was having a discussion with another host about how so many things in Astronomy can take Millions or even Billions of years, yet there are still all kinds of phenomena that happen in seconds, hours, weeks, years, or on the scale of human lifetimes. Stars live for hundreds of Millions of years at the low end, yet the intense brightening from the Supernova death of a massive star lasts for only a few days or weeks. It’s as if the Universe is piquing our interest with short...
Mercury, the smallest planet in the solar system, and closest to the Sun, is only a little bit bigger than Earth’s Moon. But the Moon is comparatively reflective object. Mercury is thought to be made of the same rock as the Moon, so what is the difference? Why do objects in our Solar system have different brightnesses? The key is in a property called albedo. It’s basically how much light an object reflects, measured as a fraction. For example, the Moon reflects 12% of the light the Sun shines on it, so it has an albedo of 0.12. The albedo...
