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The most powerful telescope ever be in your pocket
The most powerful telescope in my pocket
By Nathaniel Douglas
Reduction of the telescope – "Astronomers in the last 50 years have made discoveries wonderful, expanding our understanding of the universe and opened humanity's vision beyond the visible spectrum. Our knowledge of how the universe born and how its phenomena has grown exponentially in a single human life. Despite these advances are key issues that are largely unanswered. To further in our understanding of how our current universe was formed after the Big Bang needs a new kind of observatory with capabilities currently available in both telescopes in the soil or space. "
The bigger is better concept is then inserted into our consciousness, which comes from the idea of smaller telescope efficient seems to defy all laws of science. However, science is still compatible with miniature telescopes. It is, however, the block in understanding fundamental interests that deprives us through the centuries.
Research in this area has a full understanding of the science behind the operation optical telescope helped design the next generation of telescopes. The size of the introduction of miniature telescope will be the size of a viewer now used the telescopes today. However, this new generation of telescopes with a resolution higher than even the most powerful telescope largest known.
technical objectives and mirror manufacturing has improved considerably over the centuries. With the help of computers, lasers and robotics technologies, optics can be made with unprecedented accuracy. Finally, reduced-size telescopes as small instrument as a portable pair of glasses in the not too distant future. Soon telescopes composed of very small (a few centimeters long) tubes mounted on a harness. They have the advantage of precise movement and shock absorption provides man's head. Wide field of view similar to the naked eye, the focus stunning, infinite expansion (limited only light pollution and nuisance), and the brightness of the color flash photography and recording of live video.
Harness will be practical, efficient and versatile. The design has the potential to be upgraded and customized.
After nearly 400 years of development of the telescope, we finally have a breakthrough now in a position to reshape and create revolutionary science optical telescopes telescopes to reduce the size of football to a viewer, and finally a pair of glasses. Welcome to the new technological era of the telescope.
The impossible possible – As our technological achievements in training the future, find ways to make the impossible possible. We constantly improving existing technology, making them smaller and more efficient. In many cases, small drawings become more integrated in the broad category efficiency. We are now able to manufacture instruments in a microscopic scale, except optical telescopes.
optical telescope is the only instrument that actually grows in size rather than decrease. As we move forward in research and development of these instruments, which grow in size with each new generation.
Astronomer's all dream of having access to a powerful telescope resolution but small enough to be portable. However, it has its roots in our minds that we can not increase resolution in a small design unique. In this connection, engineers continue to build more instruments, creating monsters and giants.
The reason miniature telescope size is considered impossible, not only from the perspective of science, but also a misinterpretation of the principle of light. I still do not understand complex interactions involved in capturing and displaying images so far. It is this uncertainty, why are we using two different theories light. Light is considered as a particle is accelerated from point A to point B, and light transmission is also considered wave motion of the waves. If a theory does not make sense, others are applied. miniature telescope size is based on the "unification theory of light."
Science - Our eyes are very unique: a young pupil is dilated between 2 and 7 mm, however, the eye has the ability to display images of several thousand meters diameter. Our extensive field of view provides convincing evidence that we consider the non-convergence-ray image, parallel rays. Convergence of ray image obeys the law of inverse square of the electromagnetic radiation. describe the rays converge rays that become a point.
Therefore, the image conveyed by these beams to reduce cross section with the distance of travel. The images obtained through the telescope of greater openness, is actually a few millimeters in our eyes. small angle (Field of truth) in the second grade, so little brain has trouble isolating the information they contain for recognition when taken into account in our field of vision. These small angles too much information packed into this great field of vision, and seem to be only a snip or become invisible. However, the extension provides the means by which the angles are small converted larger.
A telescope with an aperture of 30 mm in length and 120 mm focal length (ratio focal length f / 4), which offers a 5x magnification times and has an exit pupil of 5 mm. This is a very light telescope, writing about a maximum of 7 mm aperture of the students. If a second telescope was built with the same aperture size of 30 mm, but have a focal length of 1200 mm (F / 40). The magnification is 50x times.
Instead an exit pupil of 5 mm, the telescope will now have an exit pupil of only 0.5 mm. The same formula, once the power of 50x and a pupil output of 5 mm, the required opening is 300 mm.
Refractor telescopes can not obtain an exit pupil of 7 mm without being affected by aberrations. To overcome this problem, designers attempt to allocate telescope a balance between expansion and brightness. resolution to describe this balance. The commitment is to reduce the brightness, but the power of higher magnification and image clarity at the same rate.
The eye has an important role in the completion of the apparent field image. Are capable influence the field of vision, expansion and exit pupil (brightness). A short focal length eyepiece will provide a great increase in energy, small field vision, and the exit pupil recently, a long focal length eyepiece will provide a small increase in power, wide field of vision, and student output long.
In this example, we can see that the increase is inversely proportional to the diameter of the exit pupil and exit pupil is directly proportional to brightness. In the most Bigger is better formula, we know that increasing openness, which can increase the exit pupil and therefore the brightness of the image.
There are several design aberrations set restrictions on optical telescope design of the modem. In the design of optical systems, optical engineer must make compromises in the fight against aberrations to achieve the desired result. Aberrations errors leading to the imperfection of the image. These errors can result from design or manufacturing or both. Lens achromatic have been developed to reduce chromatic aberration created when white light is refracted, but even with the best designs, no chromatic aberration can be completely eliminated. Chromatic aberration is also composed of a side effect called secondary spectrum. The higher the ratio of InFocus, the lowest spectrum becomes secondary. chromatic aberration limits the most resistant to a focal ratio of F/15. Reflectors, which is less affected by the aberration chromatic focal length of a portion of f / 5 f / 2.5 and commercial design for professional designers. In the design of telescopes known, the various conditions necessary to perfect the image is built, requiring engineers to make concessions to achieve a balance that will close the best possible picture.
What if the extension, the focus and brightness can be separated? The new formula of "miniature telescopes isolated from each of these factors and that each independently tuned for maximum efficiency.
The desire for expansion of energy "Most Large Telescope (OWL) is an exceptional project that requires an international effort. This huge telescope's primary mirror is over 100 meters in diameter and has a resolution 40 times better than the Hubble Space Telescope. This a telescope with a primary mirror size of a golf ball of the foot. "
The need for greater magnifying power began with the design of Galileo. Research and experiments to improve the telescope's magnification shows that increasing the power of increase is directly proportional to the difference in focal length and ocular (eye), where the focal length Eye is the shorter of the two.
The race to build the telescope Powerful began early in the development of the telescope. The brightest minds when they compete to dominate the development of this new technology. At that time, telescope tubes were very long. Sometimes, these tubes to the length that makes them unstable. In some cases, the tubes were removed from the instrument design. telescopes tubeless telescopes were called air.
As telescope engineers in the competition to develop more powerful telescopes, not realizing encountered a problem less than limits the length and the extension of these early creations of the telescope. They note that the images become darker with the expansion. Somehow, the expansion is to reduce the amount of light entering or leaving the lens and the telescope.
The explanation for this phenomenon is that the light was not quite out of the eyepiece of the telescope, enough light has not been included in the target. An increase in the size of the aperture increases the exit pupil and the problem of the dark image expansion is resolved.
At this stage of development in the telescope, refracting telescopes Kepler and Galileo were just invented. Lens is detected early and it was difficult to produce quality lenses. objectives were to open an even bigger challenge.
telescope will soon reach its size limit, but now that the second section of the formula of high resolving power is known, several versions reflecting telescope was born.
To date, almost 400 years later, the same formula is still used. improvements simply modem increase the quality of the optics now used, the amendment reduces the minimum aberration. Now we can build the biggest telescopes in resolving power and brightness never taught possible at the time of Galileo, but the formula used in the modem development of these instruments is the same as the first drawings, the bigger better.
The bigger is better the formula is not unlimited. For example, chromatic aberration limits the brightness of an astronomical telescope, that requires a focal ratio of f / I 5 to filter aberration secondary spectrum. The coordination relationship limits the light gathering capacity of the vessels. The reflectors are not affected by the side effect of radio spectrum. Ff2.5 focal ratio in the range is reasonable requires close exit pupil of 7 mm. No But any attempt to increase the magnification of these telescopes reflectors while maintaining the brightness should be increased in the diaphragm and reach the same proportion. These are the design features that makes the phrase "more is bigger, better" so compelling.
Previous limitations - understanding of the principle of light rewarded us with the development of modern optical technology. This article was written to provide a breakthrough in research and development of small powerful telescopes.
Most major manufacturers to inform you that the extension of the telescope is not of great importance, and full brightness is a concern a buyer should have to buy a telescope.
Expansion and brightness are as important for viewing and capturing images distant, but the most important factor in providing the details in an image is developed. Of all the basic principles involved in the capture of an image, the emphasis is less known. The conscience of a focal image and how to obtain a focused image can be easily calculated, but what are the interactions that will focus electrodynamics image remains unanswered.
All optical instruments focus on the design, so it will always be a priority to training a clear picture.
Expansion and brightness are of secondary importance, are the result after development. This is the critical distance of the importance of determining luminosity increase and temperature to which an image is seen clearly.
Extension describes the action of the conversion of smaller angles (Real field) in the largest (apparent field) that a change in the angle at which you receive the rays of the image, which, fooling the brain into believing that the object is close, then it is really.
If not for the need to focus, a single convex lens of a magnifying glass, a telescope would be capable of expansion infinite zoom through the action of simply changing the distance, it takes the eye.
Unfortunately, there is a critical distance that the images are the focus through a single lens or a lens system. This is also known that the critical distance development.
What is stress?
Webster: "fo-cus is the distinction or clarity with which an optical system of a picture.
Four Hundred Years of History – The discovery of the expansion was deleted by accident. Lens Manufacturer Lippershey early January experimented with two different objectives when it was discovered the effect of expansion away. Found keeping a close eye on negative lens, while maintaining a positive lens in alignment with the first, far eye, distant objects appear much closer than would at first sight. Since then, research to understand and explain the science behind these magical devices is always a temptation. Even with current technology, designers still face telescope design constraints and challenges to forge a compromise between the size of the telescope, the brightness and clarity.
Scientists have always been intrigued by the nature of light. Sir Isaac Newton to light what is referred to as a sequence of small particles travel in straight lines. Dutch scientist Christiaan Huygens, on the other hand, believed that light wave was a substance called ether, which is supposed to fill the space, including a vacuum. Huygens concept was accepted as the best theory of the two. Today however, scientists believe that light is composed of a sequence of wavelet pockets of energy called photons.
Bigger is better formula – "With a telescope that is 10 times the area of meeting all the telescopes ever built. You would be able to descend several thousand times smaller than the smallest thing to do with current telescopes. "
The formula that has shaped telescopes known in the centuries of development is pretty basic, well known and proven to be more is better.
It is the same as saying that greater openness offers a brighter image, while over the focal length allows a higher power. Still, this formula is written in stone?
Let the formula for the test.
Expansion can be obtained without lens focal length? The answer is yes. Microscopes provide a large increase in focal length lenses relatively short. Is it possible capture the light without opening large? Again, the answer is yes. Microscope shows too. So why is that they provide microscopes High magnification bright enough for a relatively small, while the telescope can not? This shows that this is not the law of expansion, or brightness, but the design limitations of instruments that emphasize the idea that bigger is better. Kepler telescope design base works like a microscope, viewed through the other end of the tube. Because the telescopes are essentially an inverted microscope, you can see the close relationship between the two.
An international student microscope Full size standard provides up to 400 increases, but as a microscope is a tube less than 20 inches in length. enough light is reflected by the mirror plainoconvex his "less than 7 inches in diameter. For identical brightness and expansion of a telescope focal ratio f / 2.5 is recommended for a pupil output of about 7 mm. This telescope will require an opening of 320 inches (3.2 meters) and a focal length of 800 centimeters (8 feet), the calculation more or less with a 20 mm eyepiece. This is an increase of almost 50 times in size. This shows that the brightness is not limited to open or limited expansion long focal length. No But the "bigger is better" formula is a design limitation that the surface in the range of increases.
Development of distance images is more difficult to focus images in the foreground. We can prove with a single magnifying glass held close to the eye. Other objects, then 2 / 3 length focal lens out of the question.
All optical systems design of the whole debate. To vary the expansion and brightness, the focus should be constant. May compromise the visa extension brightness and conversely, it can never compromise the development.
Therefore, instead of saying that enlargement M is inversely proportional to the light, it is also fair to say that M is equal to the extension point, divided by the brightness B, where the emphasis is a constant D.
M = D / B
Power magnification (M) = constant attention (D) / Brightness (B)
In the optical telescope design namely, the three factors are integrated. The approach has been the main factor to take a clear image, while the extension and brightness serves as a secondary factor in the development of a focused image. To find perspective, focus, brightness and magnification are inseparable. Resolving power is used to summarize the performance of a telescope. Set by telescope's ability to print details of an image. An image of the fingerprint of the individual points that meet to form a complete picture. Zooming an image involves the stretching of these points. Increases light is very different from image expansion, and magnified by changing the angle of light in the received image.
But is not the issue gap, and if these three important factors can be isolated and individually tuned? Hmmmm. Enginering telescope will not be the same, and the science of astronomy to explode.
Nathaniel Douglas
About the Author
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