QUESTION: How do astronomers estimate or try to count the number of stars in the Milky Way? ANSWER from Jim Sweitzer on 27 October 1995: This is an interesting question because the same method is used to measure the mass of our earth and sun. Astronomers don't actually count the stars in the galaxy, they really just try and figure out how much matter there is in the galaxy. Then, from studying how many stars are of different types, they can guess what the average mass is for a typical star in the galaxy. Dividing the average mass into the total mass for the galaxy gives a rough idea of how many stars there are. The most important thing is to get the mass of the galaxy. How is that done? Well, have you ever spun something on a string around in a circle? If you have, you probably know that the faster you spin the object, the stronger you feel the string pull on your hand. If you've never done this, you should try it by tying something attaching a small rubber ball to a few feet of string and giving it a whirl. Well, the faster the ball moves in a circle, the stronger the force you should feel on the string. Basically the same thing happens with stars orbiting in our galaxy. The stars are like the ball and the "string" holding the stars in the galaxy is the gravity of the rest of the stars in the galaxy. The same thing happens with the Space Shuttle orbiting the earth, but in this case, it is the earth's gravity that keeps it from zooming off into space. The circle the whirling ball travels in is the same thing as an orbit. It's just that for stars in the galaxy, the orbits are enormous. Where it takes a fraction of a second for the ball on the string to whirl around your head, it takes about ninety minutes for the space shuttle to orbit the earth. For a star that orbits the galaxy out where we live, it takes about 250 million years! And the radius of our sun's orbit in the galaxy is about 600,000,000,000,000,000 miles! The law of gravity says that the amount of force that keeps something in orbit depends on how much mass is pulling on the star and how far the star is from the center of all this mass. I won't go through it here, but when astronomers work backward from the orbit of the sun and its speed in the galaxy, they know that there needs to be about 100,000,000,000 times the mass of our sun to keep it on a steady orbit. They also know that the sun is a pretty average star. So, if you divide the mass of the sun (=1 in these units) into the number above, you get that there are about 100,000,000,000 stars (or 100 billion). Now this answer is very, very approximate, but is certainly accurate to within a factor of ten either way. At one time McDonalds resturants used to list how many hamburgers they have sold. I remember one time seeing one that said 100 billion sold and I thought of the number of stars in our galaxy. Now I think they just say, "billions sold." I hope all this makes some sense. Thanks for asking.