Size Matters: Telescope Aperture Explained Quiz

If sagging is a problem for lenses held at the edges (refractors), but mirrors can be supported across their entire back surface, then reflectors do not have the same size limits as lens telescopes.

If aperture determines both brightness and detail, and if seeing the universe requires both, then a larger aperture is the most important feature for a powerful telescope.

If mirrors avoid the weight and color-distortion problems of lenses and can be built in segments (like the James Webb), then they are the only practical choice for giant telescopes.

If the f-number (or focal ratio) describes how "fast" or "slow" a telescope is at taking pictures, and if this is a ratio of length to width, then the denominator is the aperture.

If the primary mirror bounces light back up toward the opening, and if the observer's head would block the light if they looked there, then a secondary mirror is used to bounce the light to an eyepiece.

If the ability to see detail (resolution) is tied to the width of the aperture, and if a larger aperture allows for higher resolution, then a small aperture is actually less capable of seeing fine details.

If Telescope B has twice the diameter of Telescope A, and if light-gathering power follows the square of the diameter (2² = 4), then Telescope B collects 4 times more light.

If a reflector uses mirrors to gather light, then it needs a primary mirror and a secondary mirror; because mirrors are glass, they need a shiny coating like aluminum. Lenses are for refractors.

If a telescope has multiple mirrors, the first and largest mirror that catches the incoming light is defined as the primary mirror.

If the Earth's atmosphere distorts light, and if a large aperture collects more photons from distant galaxies, then placing a large-aperture telescope in space provides the clearest and deepest views possible.

If the aperture is the opening that lets light into a telescope, and if that light is collected by the primary optical part, then the width of that lens or mirror is defined as the aperture.

If a nebula is faint, it requires a high light-gathering power; if a 10-inch aperture is much larger than a small lens or binoculars, then it is the best tool for the job.

If the mirror is designed to bring parallel rays of starlight together to a single point, and if a "bowl-shaped" curve is required for this, then the scientific term for that shape is concave.

If more light is collected, the image is brighter and fainter stars appear; if a wider aperture is used, the physics of light allows for more detail (resolution), which requires a wider physical tube.

If magnification only stretches out an image that is already bright enough to see, and if many galaxies are too dim to be seen at all, then collecting enough light to make them visible is the first priority.

If reflection is the bouncing of light and refraction is the bending of light, and if "reflectors" use mirrors, then the mechanism for focusing starlight must be reflection off a curved mirror.

If the light-gathering area is a circle calculated by pi * r², and if the radius (r) is doubled (2r), then (2)² equals 4; therefore, the area and light-gathering power increase by 4 times.

If the light enters the front of a reflector and must reflect off a surface to be focused, and if the largest mirror is positioned at the far end, then that primary mirror is at the bottom.

If a reflecting telescope uses a mirror instead of a lens to gather light, and if the aperture is the diameter of the primary gathering surface, then the size of the primary mirror is the aperture.

If starlight is spread out like rain, and if a larger bucket catches more raindrops than a smaller one, then a telescope with a wider aperture will catch more light from distant stars.