Astronomy is the poster child for big science. The observable universe is growing beyond comprehension. Gigantic instruments are needed to see most of it. Amateur telescopes are much smaller, but the advantages of increased aperture for seeing detail in faint fuzzies are a hard facts of physics. For amateurs, advice to buy the largest aperture that you can afford and aperture fever, are entrenched wisdom in the hobby. However, there are good reasons to do the opposite.
If you have a dedicated observatory, the weight of equipment isn't a problem. If you don't have your own, remote observatories are becoming more accessible to amateurs. Observatories with publicly accessible data like the LSST, which will generate a high resolution near-live movie of the night sky, will capture more data than all the astronomers in the world will ever be able to see. In spite of these resources, observing with your own equipment under a dark sky is wonderful fun for many. Unless you use a dedicated observatory, your equipment must be moved to an observing site and set up for each observation. Size and weight matter when you must carry and set up your own equipment.
Optical physics dictate that resolution of a telescope increases with the aperture of a telescope and light gathering with the square of the aperture. Let's consider the physics of the mass of the telescope itself. Increasing the size of a physical object, increases it's weight by between the square (e.g., hollow sphere) and the cube (e.g., solid sphere) of the dimension. Let's see how this applies to a telescope that might be used for astrophotography. The table below lists some typical weights for telescopes with camera, mount, and tripod by aperture.
|aperture||kind||weight||square law weight|
Our sample shows that the expected weight of a telescope will vary roughly as the square of it's aperture. Exact weights vary by type, e.g., refractors are heavier and Newtonians a bit lighter, but increasing aperture always costs significantly in weight. Mounts and tripods, especially for astrophotography, must be heavier to give steady support to a heavier telescope.
Many astronomers have also observed that the heavier and the more complicated the setup for a telescope, the less often it is used. My experience is that the frequency with which a telescope will be used is inversely proportional to its weight. Put together with the square law growth in weight - we expect, other things being equal, use of a portable telescope will decrease with the square of its aperture. I call this the inverse square law of observing frequency.
Of course other things are never equal:
The ultimate small telescope for many targets which require more than a degree or so in field of view may be a camera lens. With a tripod and small tracking mount many deep sky objects are well suited to astrophotography with a camera and lens. Detailed images of solar system objects require long focal lenghts that are best achieved with a telescope.
Example image taken with a camera, telephoto lens, and star tracker:
Omega Centauri from Terlingua
Camera weight matters too. The heavier the payload the heavier the mount and tripod that are required for sharp images. Astrophotographers often use these kinds of cameras:
Digital astrophotography techniques can make small equipment much more useful. Modern sensors are more sensitive and have lower noise than older sensors or film. Image stacking techniques capture more light and reduce noise in the final image. Image deconvolution processing recovers resolution lost to diffraction. Using new technology sensors and processing techniques, it's possible to take images that once would have required a telescope with twice the aperture to take.
Stacking images gathers additional light for an image just as a larger telescope objective does. By taking a stack of images with a longer exposure time an astrophotographer can gather as much light as with a larger telescope (e.g. 4X more exposure is the same as a 2X larger objective with 4X the weight). Stacks of images have advantages over single long exposures. Transient events like a gust of wind or a passing plane only spoil one short image. Noise is also easier to reduce in a stacked image.
These techniques don't help visual observers. With a small telescope, very faint objects will require a large objective telescope to be seen by eye. Dark skies, far from city lights, increase contrast and make dim targets easier to see in a small telescope.
If you double the size of your telescope, you can expect the weight to increase by four times. There's a lot to be said for starting out in astrophotography with just a camera and a then adding a small telescope suitable for astrophotography. Spending time using your equipment to take beautiful images is a lot more fun than lugging it around and setting it up. You can compensate for the smaller aperture size by taking more images. Stacking images and processing them to decrease noise and increase resolution can produce beautiful images without a large telescope. You will learn image processing skills that will make the best of image data from any size instrument.
Mars can look pretty big through a small scope! Example images taken with this small telescope follow:
Saturn with five moons 2016-06-09
January Earthshine Crescent Moon
Content created: 2017-02-19
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