Sample Size Solves Problems

Science and technology benefit one another.  New scientific theories afford new opportunities to create technology that can harness the laws of nature.  Conversely, new technologies allow for better instrumentation and unprecedented efficiency in scientific progress.  It’s a continual feedback loop, and some of the greatest challenges in science are solved simply by throwing more resources at them, or in other words, gathering more data. A good example of this is a relatively old problem for astronomers – determining how the spin of a galaxy affects it’s shape.  We certainly don’t want for analogies on Earth, spinning pizza, driving on a...

Juno’s New Jupiter

The Juno spacecraft began its long journey to Jupiter in 2011.  Waking up in 2016 it underwent a successful orbit injection on July 4th. Now after nearly a year of waiting, the public finally gets to see the first fruits of the mission. It has certainly been worth the wait.   A new Jupiter, seen from a distance of 52,000 Km, has a vivid and chaotic southern pole in the above image.  Swirling storms thousands of kilometres across whirl around one another in a sea of gaseous ammonia clouds.  Will the system remain chaotic? Or will it change a year from...

A Direct Black Hole

How did supermassive black holes form in the early epochs of the universe? More importantly, how did they have enough time to grow as large as they did? The answer requires a very different universe.  And back then, conditions were much different than they are now.  There was a lot of gas, little dust, no stars, and a plethora of dark matter. Astronomers have spent decades observing early quasars, massive active galaxies powered by huge black holes feeding on surrounding gas.  But these galaxies are seen so early in the universe’s history, one starts to wonder how a black hole finds sufficient...

Reproducible Results and Baby Planets

When I report science news, discuss new discoveries, and get excited about new results, it can be difficult to hear that little voice in the back of my mind that says ‘reproducible results.’  It’s the voice of the pure scientist that reminds me to be critical of the things I read, and be open to critical review for the things I write and say. Any result isn’t worth the paper it’s printed on unless it can be independently reproduced.  This is a key to scientific advancement.  If the result can’t be reproduced, then something is wrong.  It may be an error with...

Seeding The Supermassive

In the early Universe, things were quite different.  The first stars were much more massive than stars today, and contained mostly Hydrogen.  Astronomers have good ideas about how they formed, but other objects from around this time, namely black holes, are much tougher to account for.  Early black holes were huge, with no explanation for how they grew so large.  “Early” means “first Billion years after the Big Bang,” but even in that time, it’s hard to determine how observed black holes could grow as large as 100,000 solar masses. I say 100,000 solar masses, because that is the mass of two ‘seed’ black holes, discovered...

The How and Why of Planet Nine

It hasn’t been found yet – let me make that clear.  But with evidence that it should exist, astronomers are looking more closely at the proposed planet nine and how it might have formed, and how it could have ended up in such a distant orbit. When you start to think about how a planet ten times the mass of Earth could have ended up more than ten times as far from the Sun as Neptune, a few scenarios pop into mind: It was formed in the inner solar system, where interactions with gas giants or another star pulled it out It formed...

Martian Water is Quick-Boil

At this stage of our understanding of the planet Mars, we have seen salty water flowing (recurring slope lineae), found evidence of ancient riverbeds, and seen seasonal changes in the polar caps.  But an important question is how does water behave on Mars? A bit of science here on Earth gives some insight. Water at sea level on Earth boils at 100 degrees Celsius, which actually defined the Celsius scale.  But as pressure changes, liquids boil at different temperatures.  As the atmosphere gets thinner, the boiling temperature of water decreases.  On Mars, with it’s extremely thin atmosphere, this means that water...

History of a Made-Up Planet

There are eight planets in the Solar System.  This statement makes a lot of people angry for several different reasons.  The obvious group to respond with anger is the ‘people for Pluto,’ who have an unwavering dedication to the little planet that could.  It’s scientifically recognized as a dwarf Planet, and is still one step up from a Kuiper Belt Object (KBO), so it’s doing well.  Far beyond Pluto, in the outer recesses of our Solar system, you may have heard of a potential Super-Earth-sized Planet recently theorized by Konstantin Batygin and Mike Brown.  This is the other reason people would...

Journey to the Center

As I’ve said before, the most powerful, most energetic, most intense processes happen in the center.  The gravitational center of the Earth, the Sun, and the galaxy are all places where temperature, pressure, and interactions of matter and energy are pushed to their limits.  When you look up to the sky it’s easy to see the Milky Way (unless you live in an urban center).  Do you ever wonder where the middle of it is? Where that supermassive black hole lies? Astronomers know where it is, but you need infrared cameras to see it past the thick dust that blocks...

Nature Outshines CERN

The gravitational center of most objects and clusters in the universe are the place where the most massive and high energy interactions take place.  For the solar system, the Sun’s core is hot and energetic.  For star clusters, central regions host the most massive and brightest stars.  For galaxy clusters, the most massive galaxies in the universe are seen in the center.  And for individual galaxies, the Milky Way included, the core is where the fun happens. In the core of our galaxy, there are many massive and powerful objects, not limited to a supermassive star cluster, pulsars, supernova remnants,...