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Viewing Objects

Updated:
May 04, 2004

Viewing Objects

 

You have just bought a new telescope. After several days of studying books, you decided it's time to try out your new toy. With great excitement, you set up the telescope as detailed in the instructions. Referencing one of the star charts you brought along, you swing the telescope to the location known to contains M57: The Ring Nebula. All the books and magazines you read shows the Ring Nebula as a colorful ringed object with a small dead star at its center. With great excitement, you put your eye to the eyepiece. Looking for that beautiful ring you see...a little fuzzy gray disk! Where is the color? What happened to the star in the center? WHAT THE #&%#$@ IS WRONG HERE!?!?

Unfortunately, the above scenario happens all too often. "I never see any color...is my scope broken?" "Am I not doing something?" "Did I buy the wrong telescope?" " What am I doing wrong?"

The facts are you are probably NOT doing anything wrong with your telescope. It is your expectations of what you are going to see that need adjusting. To help you understand, let's take a look at the following three pictures of M57- The Ring Nebula.

M57: the Ring NebulaThe first picture simulates a typical view of M57 using a popular model of an amateur astronomer's 8 inch telescope. The image has no color, is very small and very dim. Increasing the power of the telescope would make the image larger, but the image would also become dimmer. In the next picture, again we see an image taken by an amateur astronomer. The telescope used here was larger. In addition, a long time exposure camera was used. The over all cost of the equipment used to get this image was four times higher than the cost for the telescope used in the first picture.

The final picture was taken by professional astronomers using the 200 inch Hale telescope. The final image was computer enhanced to help bring out the image and colors. This is the image most likely to be seen in books or magazines.

Clearly the three images are not at all the same. More importantly, the first image is more representative of what anyone looking through an amateur's telescope would really see! Other factors also affect how clearly any astronomical object will be seen. Weather, light pollution, air pollution and the atmosphere all affect how clearly any object will be seen.

Aperture Size

The telescope's aperture size is directly proportional to how much light from any space object is need for you to see that object. In general, the larger the telescope's aperture, the dimmer the object that can be viewed. There is a condition among astronomers known as aperture fever. Aperture fever is the condition an astronomer gets when he or she wishes they had an even larger telescope aperture. This is an incurable disease! The plain truth is, the larger the telescope's aperture, the further into space you will see. It is also true that the larger one's aperture, the more money one has to give up. It is NOT true that a telescope with a lot of magnification power is better then one without. Aperture is much more important than magnification power.

Some thoughts

here are several factors that will effect how clearly you will see anything through any telescope. But you will never see those beautiful color images found in many books or magazines through an amateur telescope. Most all the images used by the media are taken using very large professional telescope using state of the art photographic systems. The final image is then run through computer imaging software to enhance the final colors and image quality.

This does not mean that you still can not experience the thrill of seeing, no matter how dim, an astronomical object using your own eyes. The light that finally ends up entering your eye, in many cases, has been traveling for over 2 million years. So what if the Ring Nebula might turn out to be a small, dim spot in the eyepiece. Not many people can say, "The Ring Nebula, oh I've seen that with my own eyes!" You might even consider taking your own impressive color images using a CCD or film camera mounted on your telescope.