Thursday, September 26, 2019

Prepare an Observing Proposal (See attachment) Essay

Prepare an Observing Proposal (See attachment) - Essay Example What is the information that could be reconstructed? What are the natural changes regarding M6 cluster that could be observed? These are the questions that the proposed study would seek to establish. Considering the fact that astronomy is central to modern scientific developments, this study would serve to reconstruct information in astronomy, informing further development in the field. Table Summary of Observation Run Proposed for the Project Run Presently observed Features No nights Optimal months Accept months 1 Keck telescope Jan-Feb Jan-Feb 2 MMT 2 Feb-March Jan-Feb 3 KP-4m 3x 0.5 June-April Jan-Feb 4 WTYN 5 Feb-Jul June-April 5 CT-1.5m 3 Feb-Jul Feb-Jul 6 GEM-SQ 1.8 Feb-July Feb-Jul Scheduling Constraints Avoid cloudy days: Days that are cloud may obstruct vision; hence, unfruitful examination. Only clear days of the season are favorable. Scientific Justification Technological and scientific discoveries are playing a crucial role in enhancing human life. These developments are not only enhancing human life but are also shunning human curiosity through discovery and reconstruction of new information. Astronomy has been one of the areas that are central to scientific discoveries, especially in earth and physical sciences. Its developments have been revolutionized by technological revolution, like other areas of science. ... Keck II telescope was utilized for astronomical observation in 1996, but its potential effectiveness was realized in 1999 following the installation of all large first adaptive optics. Furthermore, in 2004, the Keck Telescope was incorporated with laser guide star AO systems, creating the allowance for the Telescope to have a resolution equivalent to the Hubble Space Telescopes. In 2005, various technological developments were realized creating the allowance for the two Keck Telescopes to be operated together (Plotner 789). In the obvious way, the developments in the Keck Telescope are a reflection of its increasing capability to discover various astronomical phenomena. There is the need to utilize the revolutionized and the state-of-art Keck Telescope to test the accuracy of the available information, such as those of the Messier star clusters. One most notable advantage of Keck Telescopes is that they do not have distortions of the atmosphere because they are over the atmosphere. T his has resulted in much sharper images. Another merit is that it is not compromised by lights which are scattered in the atmosphere. These two factors are responsible for a condition called twinkling stars. One more advantage of Keck Telescopes is that they observe a variety of wavelengths on light easily, which are hard to use while on the ground because they are placed in the atmosphere. Keck Telescopes can detect frequencies in the atmosphere and ground without distorting the signal. Therefore, places with electromagnetic mediums such as ultraviolet, gamma and X-Ray are easily viewed from the space. One of the inherent challenges with the use of Keck Telescope is that Earth’s rotation implies that the scope must frequently compensate for its movement in order to align it on a

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