Prepare an Observing Proposal (See attachment) Essay

Prepargon an spy Proposal (See attachment) - Essay ExampleWhat is the information that could be reconstructed? What ar the natural changes regarding M6 cluster that could be observed? These are the questions that the proposed workplace 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 programing Constraints Avoid cloudy days Days that are cloud may obstruct vision hence, unsuccessful examination. Only clear days of the season are favorable. Scientific Justification Technological and scientific discoveries are playi ng a crucial role in enhancing compassionate 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 visible sciences. Its developments have been revolutionized by technological revolution, like other areas of science. ... Keck II telescope was utilized for astronomical comment in 1996, but its potential effectiveness was realized in 1999 following the installation of all bounteous first adaptive optics. Furthermore, in 2004, the Keck squeeze was incorporated with laser guide star AO systems, creating the honorarium 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 reflectivity 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 sieve 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. This has resulted in much sharper images. Another virtue is that it is not compromised by lights which are scattered in the atmosphere. These two factors are responsible for a delineate called twinkling stars. One more advantage of Keck Telescopes is that they observe a variety of wavelengths on light intimately, which are hard to use while on the ground because they are placed in the atmosphere. Keck Telescopes can light upon 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 Earths rotation implies that the scope must ofttimes compensate for its movement in order to align it on a