A star wiggles thrice

By Michael on April 25, 2007 at 5:12 pm | In Astrophysics, Blog Posts | No Comments

If you are even moderately interested in astronomy you’ve heard about the latest discovery of a near-Earth-sized planet. Our buddy The Bad Astronomer lays it out very nicely for us.

The image at right shows the gravitational effect of each of the 3 planets on the star of this system. The y-axis shows the star alternately coming towards us and away from us as it orbits the barycenter of the system. (Our Sun does this too, mainly from the tug of Jupiter.) Note the units are in meters per second (m/s), this is 1/1000th of the unit astronomers generally use (km/s).

This is accomplished by measuring emission and absorption lines in the spectrum of the star. Each of these three sine waves is superimposed on the measurements. The error in these measurements is reported at about 1 m/s, so astronomers are looking for very small movements of the lines.

Thus, the trick is to first get ridiculously high-resolution observations, then measure the spectra with exquisite precision and finally untangle the influence of all of the orbiting bodies on the data. The end result of all of that work is a plot like that at right: proof that something is orbiting that star. Using other physics we can determine the masses and the size of the orbits. Even more recent technology is allowing us to probe the atmospheres of these planets spectroscopically.

I suspect there will be a lot more amazing discoveries along these lines.