Telescopes

The Hubble Space Telescope was flown into space aboard the Space Shuttle Discovery, mission STS-31, on April 24, 1990. On the subsequent servicing mission, in December, 1993, flaws in the original optics were corrected.

The resolution of the Hubble Space Telescope at a distance of 4.2 AU is about 207 km. At this distance, the smallest feature visible on Jupiter would need to be larger than 207 km to be resolved by the telescope based on its angular resolution of 0.05 arcseconds. Smaller features would appear blurred or indistinct.

The least important power of a telescope is likely the magnification power. While magnification allows you to zoom in on objects, other factors such as aperture size, optical quality, and clarity are more crucial for obtaining clear and detailed images.

The telescope was invented in 1608 not 2010.

See related question.

The size of a reflecting telescope is typically indicated by its aperture, which is the diameter of the primary mirror. Aperture size plays a crucial role in determining the light-gathering ability and resolving power of the telescope.

The Hubble Space Telescope has had a significant impact on society by advancing our understanding of the universe and providing breathtaking images that inspire people around the world. It has contributed to numerous scientific discoveries, education, and public outreach activities that have increased public interest in astronomy and space exploration. Additionally, it has helped to create new technologies and collaborations that benefit various fields of science and technology.

Hawaii is home to the most telescopes because of its ideal weather and high-altitude locations, offering clear and stable viewing conditions for astronomy research. Mauna Kea, in particular, is a popular site for astronomical observatories due to its high elevation and minimal light pollution.

The eye can distinguish very small objects, but it cannot see many microscopic creatures, such as dust mites, microcrustaceans, amoebas and bacteria. Microscopes open up this world to humans the way telescopes open up the night sky. There are many techniques scientists and students use to view the microscopic world. One of the easiest and most common techniques is making a wet mount slide. Wet mount slides are appropriate whenever the object of interest has aquatic origins or is itself a liquid.

The term "space" comes from the Latin word "spatium," which means an interval or gap. It's not named after the content of space itself, but rather describing the concept of the vast expanse that exists between celestial bodies.

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