Charlie Warzel: "THIS is what google's self driving car can see. So basically this thing is going to destroy us all." [via Matt Buchanan]

There's a dark cloud hanging over the science of climate change, quite literally. Scientists today have access to supercomputers capable of running advanced simulations of Earth's climate hundreds of years into the future, accounting for millions of tiny variables. But even with all that equipment and training, they still can't quite figure out how clouds work.

Sometime between 1956-1958 an unknown IBM employee wrote a punchcard program that displayed the above pin-up girl on the screens of the US military's two billion dollar Semi-Automatic Ground Environment (SAGE) computers. Some say that the program was a diagnostic tool that showed the pin-up as a data transfer test. Others contend that it was just geek fun. The Atlantic's Benj Edwards tells the story of what was one of the first pieces of figurative computer art. "The Never-Before-Told Story of the World's First Computer Art (It's a Sexy Dame)"

Invented in 1801, Jacquard looms are really an add-on to already existent mechanical loom systems, which allowed those looms to create patterns more complex and intricate than anything that had been done before. The difference: Punch cards.

When you weave, the pattern comes from changes in thread position — which threads were exposed on the surface of the cloth and which were not. But prior to the Jacquard loom, there were only so many threads that any weaver could control at one time, so patterns were simple and blocky. Essentially, the Jacquard system vastly increased the pixels available in any weaving pattern, by automatically controlling lots and lots of threads all at once. Punch cards told the machine which threads were in play at any given time.

It's a really cool process, and I wanted to share a couple of videos that give you a good idea of how these looms work and how they changed the textiles industry. You can watch them below. But probably the best example is the image above. It's a picture of Joseph-Marie Jacquard, woven in silk on the loom he invented — a fantastic demonstration of the design power that loom offered. In just a few years, people went from weaving simple stars and knots, to weaving patterns that almost look like they were spit out of a printer.

Possibly, according to some scientists who are trying to understand the early days of Sol and friends.

One way that researchers study events like the creation of the solar system is to model what might have happened using computer software. The basic idea works like this: We know a decent amount about the physical laws (like gravity) that govern the creation of planets and the formation of a solar system. So scientists can take those laws, and program them into a virtual universe that also includes other real-world data ... like what we know about the make-up of the Sun and the planets orbiting it. Then, they recreate history. Then they do it again. Over and over and over, thousands of times, the scientists witness the creation of our solar system.

It doesn't happen the same way each time. Just like you can get a very different loaf of bread out of multiple attempts and baking the same general recipe. But those recreations start to give us an idea of which scenarios were more likely to have happened, and why. If our solar system tends to form in one way and resist forming in another, we have a stronger basis for assuming that the former way was more likely to be what really happened.

That's what you're seeing in this study, which Charles Q. Choi writes about for Scientific American.

Computer models showing how our solar system formed suggested the planets once gravitationally slung one another across space, only settling into their current orbits over the course of billions of years. During more than 6,000 simulations of this planetary scattering phase, planetary scientist David Nesvorny at the Southwest Research Institute in Boulder, Colo., found that a solar system that began with four giant planets [as ours currently has] only had a 2.5 percent chance of leading to the orbits presently seen now. These systems would be too violent in their youth to end up resembling ours, most likely resulting in systems that have less than four giants over time, Nesvorny found.

Instead, a model about 10 times more likely at matching our current solar system began with five giants, including a now lost world comparable in mass to Uranus and Neptune. This extra planet may have been an "ice giant" rich in icy matter just like Uranus and Neptune, Nesvorny explained.

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