Category Archives: planetary science

Recipe for a Planet

Did you ever stand outside looking up at the stars, and then down at the ground, and then wonder to yourself, “How did this planet come into being?”

Of course we all know the standard “theory” about how planets are formed—a star begins to coalesce out of a cloud of gas and dust. Over millions of years this action goes on until things get hot enough in the center to turn on the nuclear furnace that stokes the burning “machine” we call a star. The leftovers are where planets come into being. There’s LOTS of stuff left over after a star forms— grains of dust and chunks of ice and clouds of gases and so on. The ice and clouds nearest the star are pretty much “burned off” by the heat from the newborn stellar creation, but the rocks and dust grains stick around. In fact, they start to stick together. IF this goes on for long enough you get bigger and bigger “hunks” of stuff out there trundling around the stars. Eventually these hunks form worlds.

Courtesy The Spitzer Space Telescope
Courtesy the Spitzer Space Telescope

That’s the “potted” history of planetary formation. But, how do we observe this going on in other stellar systems today? The Spitzer Space Telescope has just released some observations that reveal large dust clouds around several stars. They likely formed when rocky, embryonic planet “seeds” crashed together, sending debris flying out through space.

It’s a chaotic scenario, but a plausible one. And, the scientists using Spitzer are looking for such dusty disks around many nearby stars to see just where collisions are affecting planetary formation in the neighborhood. Before Spitzer, only a few dozen planet-forming discs had been observed around stars older than a few million years. Spitzer’s uniquely sensitive infrared vision allows it to sense the dim heat from thousands of discs of various ages.

So, the next time you find yourself out there gazing at the stars and marveling at their seeming serenity, remember this: it’s not all as serene as you think. Somewhere around a newborn star is a scene of remarkable chaos. And born out of that chaos in a few million or billion years might be another Earth, and maybe another being to gaze skyward and wonder what’s happening “out there.”

Remote Sensing the Earth’s Surface

A satellite view of Mount St. Helens volcano sending out a steam and ash plume. Taken at 1 p.m. EDT on Oct. 5, 2004, about an hour after being released by the volcano. Courtesy NOAA.
A satellite view of Mount St. Helens volcano sending out a steam and ash plume. Taken at 1 p.m. EDT on Oct. 5, 2004, about an hour after being released by the volcano. Courtesy NOAA.

We don’t always think of our home planet as a target for space exploration, but of course it is. Satellites lofted into orbit by the National Oceanic and Atmospheric Administration give us near-constant views of the Earth’s surface and its weather. Most of us are familiar with the weather sats that give us our daily, weekly, and monthly forecasts, so it’s not a big stretch to think of those types of instruments sensing things like volcanic eruptions or other changes on the Earth’s surface.

Mt. St. Helens, the volcano in Washington state, is putting on quite a show. You can, if you want to watch it all day long, open up a webcam view of the mountain, taken from an observation post about 5 miles way from the summit of the mountain. If you’re really into it, open up NOAA’s eye in the sky and follow the action from geosynchronous orbit.

It’s kind of cool to think that while we monitor Mars using the rovers and orbiters, we can do the same at Earth, using near-real-time satellite imagery and in-situ cameras on the ground.