a grosophone
no you cant see image its appers in waves
A refracting telescope is a type of optical telescope. It was used in astronomical telescopes and spy glasses. Objective lens are used to produce the image.
An optical telescope is a telescope that gathers and focuses light, mainly from the visible part of the electromagnetic spectrumcreate a magnified image for direct view, making a photograph, or collecting data through electronic image sensors.
A magnifying glass is an optical instrument that produces a virtual image. The virtual image appears behind the magnifying glass and is larger than the object being viewed.
The surface of a radio telescope doesn't have to be as flawless as the surface of an optical telescope because the radio telescope is collecting radio waves, something that will not be affected by faults in the glass. Optical telescopes, on the other hand, are collecting light, where faults in the surface can interfere with the image.
The main lens or mirror produces a virtual image of the obect being looked at, and it occurs at a distance behind the lens (or in front of the mirror) equal to the focal length. The telescope also has an eyepiece whose function is to allow the oberver to see the virtual image. Many telescopes come with a range of different eyepieces that give different amounts of magnification.
a reflecting telescope can help us because it is an optical telescope which uses a single or combination of curved mirrors that reflect light and form an image.
The main optical element of a refracting telescope is the objective lens. This lens collects and focuses light from distant objects, forming an image that can be magnified and observed through an eyepiece.
No, the images produced by a radio telescope and an optical telescope are not the same. Optical telescopes capture visible light and produce images that resemble what we see with the naked eye, revealing details of celestial objects in visible wavelengths. In contrast, radio telescopes detect radio waves, which can provide different information about astronomical objects, often revealing structures and phenomena that are invisible in optical wavelengths. The resulting images from both types of telescopes represent different aspects of the universe and require different methods of interpretation.
A telescope ray diagram can be used to show how light rays enter and are focused by the lenses or mirrors in a telescope. This helps illustrate how the telescope magnifies distant objects and forms an image for the viewer to see. By analyzing the paths of the light rays in the diagram, one can understand how the optical principles of the telescope work to enhance our ability to observe objects in space.
You can insert a corrective lens or a prism in the telescope optical system to produce an upright image. Another option is to use a diagonal mirror that reflects the light path and flips the image vertically, resulting in an upright orientation.
The most important part of a telescope is the telescope tube. Other parts are the viewfinder or optical finderscope, eyepiece, focuser, reflecting mirrors, refracting lenses, and the mount assembly.