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Taking out the Twinkle

Week of August 30, 1999

Last week I talked about why stars twinkle. Briefly, it's because little packets of air bend the light from stars in random ways, making the image dance. It's very pretty, and many poems have been written about it.

Unfortunately, science is often not so poetic. While pretty, this twinkling (what astronomers call ``seeing'', an old and confusing term that has unfortunately stuck) plays havoc with astronomical observations. Since telescopes tend to take images that have long exposure times, the seeing smears out the object in the image. Seeing is measured by how much the light from a star is smeared out, and the usual unit is an arcsecond (one arcsecond is very small; it's 1/3600 of a degree). This is then a fundamental limit to how small an object we can see. Imagine two objects, one half the sized of the other, but both smaller than the seeing. Because of seeing, they will both get blurred out to the same size, meaning we cannot tell which object is larger! Even worse, two objects that are close together get blurred together, and we cannot distinguish them. That really puts the brakes on how small an object we can detect.

Luckily, there are ways around seeing, but they cost. One solution is to get above the atmosphere. That's what Hubble does. It is not limited by atmospheric seeing, and so it can see objects with very high resolution. This is a nice solution, and it works very well indeed for space telescopes, but it's expensive.

Another method is to take very fast exposures of an object; in effect taking images faster than the seeing can blur the image. This only works with really bright objects, if you think about it. You can't see faint ones in such short exposures. Still, this method has been used to actually detect the size of the star Antares, a red giant that's so big it actually has a measurable (but very tiny) disk this way.

image of star before and after adaptive optics A third, relatively new method, is to try to detect just how the seeing is affecting the image, and actually warp the telescope mirror to compensate. Amazingly, this method, called ``adaptive optics'', works extremely well. It has been in use for a few years, and is now used on the world's largest telescopes. It means that ground based telescopes can have nearly as good resolution (that is, the ability to see very small things) as Hubble. It's also cheaper than launching a 'scope into orbit, and can be used on very large mirrors (the image at left is from the Canada France Hawaii Telescope, and shows a before-and-after image of a double star; you can see how much better the resolution is after the adaptive optics is switched on).

VLT image of its own name It's used by the VLT (which stands for ``Very Large Telescopes'', believe it or not) in Chile run by the European Southern Observatory (Note: the ESO website is located in Germany, and I have experienced very slow connections there. I suggest patience when trying to connect there). There are two methods for adaptive optics. One is that the main mirror is set on a series of actuators, little rods with pistons that press against the back of the mirror. A sensor figures out just how much and in what direction the starlight is getting bent by seeing, and the actuators distort the mirror shape to compensate. The other method is to use a series of smaller, usually hexagonal mirrors all fitted together, each with their own actuators. The advantage of the second method is that it's easier to make many small mirrors than one big one.

Either way, the control over the mirror is amazing. The distortions must be compensated on timescales of fractions of a second! Some amazing computer and engineering wizardry is needed for this.

But the results are astounding. By distorting the mirror in a known way, one of the VLT 'scopes was able to write its name on the sky! Those letters in the image are actually stars, wiggled around by the actuators in the VLT mirror. You can read more about how they made that image on their adaptive optics press release page.

It's not all fun and games. The images taken by the VLT array are astonishing and beautiful, some of the most dramatic and gorgeous astronomical images I have ever seen. Take a look for yourself! You can find them at their image index page. You can even order posters of some of the better images too. You can bet that at least one of these will be hanging in my house soon!

©2008 Phil Plait. All Rights Reserved.

This page last modified Saturday, 05-Mar-2011 18:03:22 UTC

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