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The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? for GMAT 2024 is part of GMAT preparation. The Question and answers have been prepared according to the GMAT exam syllabus. Information about The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? covers all topics & solutions for GMAT 2024 Exam. Find important definitions, questions, meanings, examples, exercises and tests below for The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer?.

Solutions for The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? in English & in Hindi are available as part of our courses for GMAT. Download more important topics, notes, lectures and mock test series for GMAT Exam by signing up for free.

Here you can find the meaning of The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? defined & explained in the simplest way possible. Besides giving the explanation of The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer?, a detailed solution for The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? has been provided alongside types of The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? theory, EduRev gives you an ample number of questions to practice The progress of astronomy has always been closely associated with the development and application of mechanical processes and skill. Before the seventeenth century, the size of the planets could not be measured, the satellites of the planets except the Earth’s moon were unknown, the phases of Mercury and Venus were merely conjectured, and accurate positions of the sun, moon, and planets among the stars, and of the stars among themselves, were impossible all because there were no telescopes. More than a half century elapsed after the invention of the telescope before Picard combined it with a graduated circle in such a way that the measurement of angles was greatly improved. Then arose the necessity for accurate time. Although Galileo had learned the principles governing the pendulum, astronomy had to wait for the mechanical genius of Huygens before a satisfactory clock was invented around 1657.Nearly all the large reflecting telescopes ever built were constructed by astronomers who possessed great facility in practical mechanics. The rapid and significant advances in nearly all departments of astronomy in the past century would not have been possible except through the skill and patience of glassmakers, opticians, and engineers. The principles of spectrum analysis as formulated by Kirchho allowed for the discovery of the elements composing every heavenly body. The deftness of Wollaston showed that light could not be analyzed unless it first passed through a very narrow slit. Even in our modern day the power of the telescope and spectroscope has been vastly extended by the optical skill and mechanical dexterity of individuals such as Rowland, Hastings and Brashear, all Americans.An observatory site should have a fairly unobstructed horizon, as much freedom from cloud as possible, good foundations for the instruments, and a very steady atmosphere. To understand the necessity of a steady atmosphere, look at some distant outdoor object through a window on a hot summer day. The object appears blurry and wavering. Similarly, currents of warm air continually rise from the earth to upper regions of the atmosphere, and colder air comes down and rushes underneath. Although these atmospheric movements are often invisible to the eye, their effect is plainly visible in the telescope as a blurry distortion. In order for an ideally-designed telescope to perform perfectly, it must be located in a perfect atmosphere. Otherwise its full power cannot be employed. All hindrances of atmosphere are most advantageously avoided in arid or desert regions of the globe, at elevations of 3000 to 10,000 feet above sea level. Higher mountains have as yet been only partially investigated, and it is not known whether difficulties of occupying them permanently would more than counterbalance the gain which greater elevation would afford.The primary purpose of this passage is toa)detail the advancement of a specific scientific fieldb)recontextualize the reader’s understanding of what it takes to develop a successful telescopec)explore the early contributions made in the field of astronomy, and some of the mechanical processes that contributed to that developmentd)advocate for more research into telescope placement and developmente)describe inventions that helped astronomy and the ideal use of the telescope.Correct answer is option 'E'. Can you explain this answer? tests, examples and also practice GMAT tests.