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Science & technology history
History of science and technilogy
History of science and technology
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Space: up until a few centuries ago astronomers knew little about the universe outside of our planet. But now, with vastly improved technology, astronomers are able to uncover so much more about what lies outside of Earth. While today’s observational technology is greatly superior to that of the past, we can’t disregard the accomplishments of astronomers in the past, because without their work our knowledge of space would far less than it is today. From Galileo’s first telescope to the Webb space telescope that has yet to be launched, there are so many observational technologies that made important contributions to the observation and exploration of space. The credit for the invention of the first telescope is given to a Dutch glasses maker, …show more content…
With new technology and machines gave people the ability to grind glass lenses, and mirrors to different shapes. James Gregory, a Scottish astronomer, created the parabolic mirror, a mirror that curved differently than a spherical mirror. With this type of mirror the light rays bounce off the mirror and meet in the same place, resulting in a clear image. Thus making reflectors the first type of telescope to have clear images. Astronomers started building larger reflecting telescopes, to accommodate a larger primary mirror. Larger mirrors allowed the telescopes to collect more light, which allows astronomers to see objects that are dimmer or further away. It used to be that size of the telescope showed how powerful it was, but now it is the size of the primary mirror. Glass lenses began to improve, but it was still easier to make mirrors. Glass lenses couldn’t have any imperfections or the image would be distorted, but mirrors just needed to be shiny. At this point reflecting telescopes began to be more popular than refracting telescopes. In the mid 1700s it was learned that when white light travels through glass it splits into a rainbow, which is what causes the circles of colour around bright objects. In 1729, Chester Moor Hall came up with a solution to this problem by combining a convex lens with a concave lens. From the late 1700s to early 1800s Pierre Louis Guinand worked with Joseph von Fraunhofer worked together on making glass lenses with less imperfections. In the 1800s as reflectors got larger, there started being a problem of the Earth’s atmosphere distorting the images. When light passes through air pockets it gets distorted and results in a blurry image.
Journal Eleven In “The Telescope Effect” Shankar Vedantam states his theories on why people are so willing to help a single person deal with tragedy. However, when it comes to mass tragedies or terror people seem to shy away from helping or lending a hand. Vedantam seems to bring to light some issues people have in their minds when it comes to who they provide help for. Vedantam in the beginning of the essay tells the story of a Dog named Hokget and how the puppy was abandoned by her owner on a big tanker lost at sea.
Shortly after college he began to study optics and the construction of telescopes, and wrote his first book, Optica Promota ^1. In 1663 James went to London where he published Optica Promota, which discussed topics such as lenses, mirrors, reflection and refraction, paralax and transits. Optica Promota also discussed Gregory's most famous invention, the reflective telescope. It later became known and the Gregorian Telescope. However, at the time the telescope was only discussed because the mirror polishers could not polish the mirrors properly, so it was never auctually made untill after Gregory's death. He laso invented the feflective burning mirror. In 1664 James went to Puda, Italy and studied under Stefano degli Angeli in geometry, mechanics, and astronomy. While he was there, the published two more worksVera circuli et hyperbolae in which James showed how to compute logarithms by finding the areas of inscribed parallelograms between a hyperbola and its asymptotes, thus leading to the term "hyperbolic logarithms" in 1667. ^2 And Geometriae para universalis where he attempted to prove that the (little shape thingy that i cant type ...looks like a n mixed with pi) and e are transcendual, unfortunatly, his arguments contained a subtle error which was published in 1668, right before he left Italy for London.
Who has not ever, even if just for a brief moment, looked up at a dark but vividly lit starry night sky and wondered how far those seemingly little lights reach, and if that beauty goes on forever, or if it ends at some point. I believe this question has been pondered by mankind since our creation, and early astronomers are proof of this pondering. Telescopes began as a way for these early astronomers to chart the stars and planets and their movements as they searched for more than what just the naked eye could offer them. In the early 17th century, craftsman began making telescopes, though the tools to invent them had been available for centuries before. Early telescope were called spyglasses and needed improvement. Galileo's Optic Tube, also known as the Galilean telescope is an example of the early creation of refracting telescopes. There were a few different makers and models of refractor telescopes but it was soon discovered they could make a better telescope. With the beginning of the 18th century came the reflecting telescope, which is also called a reflector; an optical telescope that uses either a single curved mirror, or a combination of curved mirrors. There are many types reflecting telescopes: there is the Gregorian telescope, the Cassegrain telescope, and the Ritchey–Chrétien telescope. But today, we are going to be talking about one telescope in particular; "the 200 inch Hale Telescope, which for decades stood as the largest telescope on the planet"(1), from 1948 to 1976. The Hale telescope opened up the skies in ways we never imagined.
At this point, Galileo’s career took a dramatic turn. In spring of 1609 he heard that Netherlands this instrument was invented that showed things that are far as though they were nearby. After, few tries he quickly found out the secret of the invention is a three-powered spyglass from lenses for sale in spectacle makers shops. To improve this, he taught himself the art of lens grinding, and produced powerful
In 1608 Hans Lippershey looked at Jupiter through a thin tube shaped object similar to a telescope. Galileo improved the telescope made by Hans in 1609 by adding a convex lens in the front. The telescope was built with a concave eyepiece and convex lenses. Telescopes were used for improving maps and figuring out the positions and motions of stars early on. Scientists believed that the bigger the lens of a telescope the better, so a man named George E. Hale had created a 100 inch telescope which was finished in 1917. Around the 1920s Edwin Hubble had looked through the telescope towards the sky and had discovered that our galaxy, the Milky Way, was not the only galaxy. He also discovered that our galaxy was expanding. Fifty years later the Hubble was funded to be built. The Hubble was supposed to be launched in 1983, but didn’t end up going into space until 1990. NASA launched the Hubb...
Darrigol, Olivier. "The Analogy Between Light And Sound In The History Of Optics From The
Although telescopes has been around for several hundreds of years, there has been great discrepancy as to who invented it first. Here is one authors opinion. Lippershey was a Dutch spectacle marker during the early 17th century (approximately 1600). He was one of the first who created the "looker" (now called telescope) by placing two pieces of lenses together. The discovery that placing lenses together can magnify images were made by children who took Lippershey's spectacles and looked at a distant church tower.
The Hubble Telescope is the world’s first space-based optical telescope. The Hubble telescope received its name from American astronomer Dr. Edwin P. Hubble. Dr. Hubble confirmed an ever expanding universe which provided the basic foundation of the Big Bang theory. The first concept of the Hubble telescope came from Lyman Spitzer in 1946, who at that time was a professor and researcher at Yale University. In 1946, Professor Spitzer believed that Earth’s atmosphere blurs and distorts light, and a space orbited telescope would be able to overcome this problem.
When considering this topic, one might ask themselves why explore space? We explore space to compare other planets with the earth and to study the sun, to explore the universe while finding if intelligent life exists, for satellites to improve communications, weather forecasting, navigation, resource monitoring, and “to create a focal point for a new intellectual renaissance” (Ruzic).
The refracting telescope is one of many different types of telescope. Refracting telescopes work by refracting the light through an initial convex lens, (known as the objective lens), then through another convex lens (known as the eyepiece lens). These two lenses focus the light into the eyepiece so we can see the image clearly.
Even though we know a great amount more than the astronomers in the past, there is still an even larger amount we do not know about the universe to this day. Even our own solar system contains many questions yet to be answered. Some of these include the possibility of a planet beyond Pluto (Planet X), the means by which the system was created, and even the possibility of a sister star to the Sun named Nemesis. Another astronomical mystery is the creation of the universe. In time, many questions will be answered but some will always remain. Astronomy is something that will never be completely understood.
The earliest known telescope was created by Hans Lippershey in 1608. Others have claimed to have made the discovery of telescope but according to documents, he is the earliest who has applied for the patent. The telescope had an convex objective lens and a concave eyepiece.
The refractor telescope uses two glass lenses, the objective lens and the eyepiece len, to collect and refract parallel rays of light from distant objects in a specific way to produce a image that fits the size of our eyes pupil. The light rays are gathered through the opening of the telescope called the aperture, they then travel through the objective lens and refract onto a single point called the focal point. From here the light rays continue to travel in the same direction until they reach the eyepiece lens, which refracts the light back into parallel rays. Distant objects appear brighter, clearer and much more magnified than they really are because of this process. The magnification of a telescope can be calculated by using this formula
Ever since the beginning of time there have been stars. Not only stars in the sky, but moons, planets, and even galaxies! Astronomy is defined as the branch of science that deals with celestial objects, space, and the physical universe as a whole. In other words it is the study of space, planets, and stars. Throughout the ages, many people have used astronomy to help them learn about the universe, our own planet, and even make predictions about life itself. Understanding astronomy means understanding where it originated, the different groups/cultures that used it, and modern purposes of the science of the stars.
Space has always been a pivotal and utmost important subject for many years. In the past, scientists have made monumental advances in this field such as sending people into orbit and landing a man on the moon. Of course, this has only barely been explored and we still have a lot more to see of the ever-vast outer space. One of the most significant topics of all of science has only been touched and there’s still more to come.