Telescopes

A mirror in a telescope reflects and focuses light to create images of distant objects. It is the primary optical element in a reflecting telescope, where it gathers and concentrates light to produce sharper and brighter views of celestial bodies. Mirrors are essential for collecting and directing light to the eyepiece or camera in a telescope.

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 Hubble Space Telescope takes pictures of various celestial objects in space, including stars, galaxies, nebulae, and planets in our own solar system. It has provided stunning images that have helped astronomers better understand the universe and phenomena like black holes, distant galaxies, and planetary atmospheres.

No, ancient Egyptian astronomers did not have telescopes. They relied on naked-eye observations of the sky and developed impressive astronomical knowledge and calendars based on these observations. Telescopes were not invented until much later in history.

The fundamental limit on a telescope's resolution is determined by the wave phenomenon called diffraction. Diffraction causes light waves to spread out as they pass through an aperture or around an obstacle, limiting the ability of a telescope to distinguish fine details in an image.

There are 3 syllables in the word "telescope."

Yes, Galileo used a telescope to observe the phases of Jupiter in 1610. He discovered that the planet showed different phases similar to the Moon, which supported the heliocentric model of the solar system.

The first time electronic scoreboard was used in a Wembley international match in 1955.

FAST, or the Five hundred meter Aperture Spherical Telescope, first proposed in 1994, is a radio telescope to be built by 2013 in a natural basin in Pingtang County near Duyun, capital of the Qiannan Buyei and Miao Autonomous Prefecture, Guizhou Province , southwest China As of June 2011 construction should be complete by September 2016.

A spectroscope is a device for producing and recording spectra for examination. When light given off by a simple burning substance is viewed through a spectroscope, a certain color will appear.

Yes, telescopes can be improved through advancements in technology and engineering. For example, larger and more precise mirrors, better imaging sensors, and improved stabilization systems can all enhance the capabilities of telescopes for better image quality and detection of celestial objects. Additionally, innovations in data processing and analysis can further improve the scientific output of telescopes.

You stay where the telescope is, and open up your spy phone. It is blue, and located in the left hand side of the screen. Click on it, and it will go to the centre of your screen. Now, click the red button at the top of the phone, and three tools will come out. A comb (pretty dam well pointless), a pair of scissors and A WRENCH!

Telescopes collect and focus electromagnetic radiation, such as visible light or radio waves, to create images of objects in space. Different telescopes are designed to detect specific wavelengths of radiation to study various astronomical phenomena, from stars and planets to galaxies and black holes.

An observer on Earth can recognize waxing and waning phases of the Moon based on the illuminated portion of the Moon's surface visible from Earth. During the waxing phase, the illuminated portion increases from right to left, while during the waning phase, the illuminated portion decreases from right to left. To remember this, you can think of the letter "D" for waxing (like the shape of the letter as it increases in size) and the letter "C" for waning (like the shape of the letter as it decreases in size).

Well the name of the game in telescopes is to collect as much light as possible. The more light you capture and concentrated the better and clearer the image. Multi-segment telescopes are designed to capture larges amount of light ad different optimal angles and channel them to a central focal point. Parabolic mirrors work efficiently at this naturally. However they are expensive and difficult to make properly, especially at large sizes. So having a multi-section mirror is cheaper and allows for a greater light concentration.

Hope this helps

Well that depends on what kind of telescope you are talking about. I have a masters degree in space studies and I am currently working at Cambridge University so if you would like any help in your future, please be sure to email me at doomlad1232011@hotmail.ca I'am here to help!

Improve

The benefits for science have been that we have seen further into space than ever before, we have looked at stars close up, we have given ourselves a bright future thanks to this telescope

As we can see now ,in modern days many people are discovering such as new gadgets or instruments that can help to recognize or to study more about celestial bodies.Stars are one of the specific celestial bodies that are so small to see in our naked eyes. Scientist Mr.Isaas Newton made an instrument to see more,the little organism /the stars clearly with the use of telescope.Such Mr.Isaac Newton is not the 1 who was discovered this idea but he is the 1 who improvised or made this gadget.Now a days,all of the gadgets are improvised by other person,so its now easy to study about stars,moon,sun and other celestial body..

-Vincent Michael Brillo-

roxas city capiz.

The optical axis maintains the correct distance between the lenses in a light microscope. This is the imaginary line that passes through the center of each lens in the system. Keeping the optical axis aligned ensures proper focus and clarity of the specimen being observed.

No, you can change the magnification of the telescope by simply changing the eyepiece. The two most important powers of the telescope, light-gathering power and resolving power, depend on the diameter of the telescope, but it does not control the magnification.

Galileo was unable to resolve the rings of Saturn as individual objects with his telescope. They appeared to him as "ears" or handles attached to the planet. The true nature of Saturn's rings was not understood until later observations with more powerful telescopes.

Mirrors in reflecting telescopes are used to gather and focus light. The primary mirror collects incoming light, and then reflects it to a secondary mirror, which in turn directs the light to the eyepiece or imaging instrument. This design allows for larger apertures and better light-gathering capabilities than refracting telescopes.

The word "telescope" comes from the Greek words "tele" (far) and "skopein" (to look or see), which together mean "far-seeing" or "seeing far off." The telescope was invented by the Dutch eyeglass maker Hans Lippershey in the early 17th century.