Pt2520 Statement Of Work, History, Scope, Constraints, Objec

Pt2520statement Of Work History Scope Constraints Objectives

PT2520 Statement of Work · History: · Scope: · Constraints: · Objectives: · Tasks and Timeline: · Gathering Data: Add a description of task. · Time allotted: · Deliverable: · Analyzing Data: Add a description of task. · Time allotted: · Deliverable: · Normalization: Add a description of task. · Time allotted: · Deliverable: · Building the Physical Database: Add a description of task. · Time allotted: · Deliverable: · Testing and Security: Add a description of task. · Time allotted: · Deliverable: · Database Completion and Installation: Add a description of task. · Time allotted: · Deliverable: · Total time between beginning and end of project: 1 Observing the Sun’s Position and Motion Big Idea : Sky objects have properties, locations, and predictable patterns of movements that can be observed and described. Those motions explain such phenomena as the day, the year, the seasons, phases of the moon, and eclipses. Goal : Students will conduct a series of inquiries about the motion of the Sun in the sky using prescribed Internet simulations and learn how the Sun follows different pathways at different times of the year. Computer Setup : Access and a) Find SELECT FROM MAP link under Configuration and set your observing location and time zone b) Find WHOLE SKY CHART link under Astronomy Phase I: Exploration PART A : 1) On a map of the United States, north is toward the top of the page and west is to the left. On all of the star charts, north is toward the top of the page and west is to the right. How do you account for this difference? 2) This is the current sky. Find the YELLOW dot marking the current location of the SUN. Which constellation is it closest to right now? 3) Change the time by increasing it one hour and pressing submit. Exactly how has the Sun’s position change on the map? 4) Slowly increase the time to later and later in the day. This system probably uses 24-hr “military time†or “Zulu†time. So, 6pm is actually entered as 18-hours. Determine EXACTLY what time, hours and minutes, that the Sun will set tonight. Sunset: __________ 5) Which constellation was the Sun closest to when it set? 6) Is this the same or different than where the Sun was earlier in the day? 7) What generalization can you make about the relative speeds that the Sun and the stars move through the sky over the course of a day? 8) What generalization can you make about the direction the Sun and the stars move through the sky over the course of a day? 9) Describe precisely how you would test to see if this generalization is true during the night time too. 10) What is the physical cause of your generalization? Phase I: Exploration PART B: When looking at the star map set for SUNSET TONIGHT: 11) on what part of the map (left, right, top, bottom or center) is the star group that appears highest in the night sky? What is the name of this star group? 12) on what part of the map (left, right, top, bottom or center) is the star group that appears near the southern horizon? What is the name of this star group? 13) on what part of the map (left, right, top, bottom or center) is the star group that appears near the eastern horizon? What is the name of this star group? When looking at the star map set for THREE HOURS after tonight’s sunset: 14) on what part of the map (left, right, top, bottom or center) is the star group that now appears highest in the night sky? What is the name of this star group? 15) Where did the stars that used to be at this position move to? 16) on what part of the map (left, right, top, bottom or center) is the star group that now appears near the southern horizon? What is the name of this star group? 17) Where did the stars that used to be at this position move to? 18) on what part of the map (left, right, top, bottom or center) is the star group that now appears near the western horizon, where the Sun sets? What is the name of this star group? 19) Where did the stars that used to be at this position move to? 20) on what part of the map (left, right, top, bottom or center) is the star group that now appears near the eastern horizon, where the Sun rises? What is the name of this star group? 21) Where did the stars that used to be at this position move to? 22) If you were to change the time to midnight, predict what would be different about the positions of the stars. 23) What generalization can you make about how the stars change position over the course of the night? Phase II – Does the Evidence Match the Conclusion? 24) From before, precisely what time (hours and minutes) will the sun set below the western horizon tonight? 25) Using the sky chart, precisely what time the sun will set one month from now? 26) Using the sky chart, precisely what time the sun will set two months from now? 27) Using the sky chart, precisely what time the sun will set three months from now? 28) Using the sky chart, precisely what time the sun will set six months from now? 29) Using the sky chart, precisely what time the sun will set nine months from now? 30) Using the sky chart, precisely what time the sun will set twelve months from now? 31) If a student proposed a generalization that “sunset time changes about one hour per month, setting earlier and earlier in the fall and then setting later and later in the spring,†would you agree, disagree with the generalization based on the evidence you collected? Explain your reasoning and provide evidence either from the above questions or from evidence you yourself generate using the star map program . Phase III – What Conclusions Can You Draw From the Evidence? Most of us would agree that the sun sets in the general direction of west. What conclusions and generalizations can you make from the following data collected by a student in terms of HOW DOES THE DIRECTION OF THE SUNSET CHANGE? Explain your reasoning and provide evidence to support your reasoning . Date Sunset Time Azimuth (west = 270() Direction August :00 pm 289( Northwest September :10 pm 274( West October :20 pm 258( West Southwest November :40 pm 245( Southwest December :30 pm 238( South Southwest Evidence collected in standard time from using SUN AND MOON DATA FOR TODAY under the Astronomy section and/or for Laramie, WY 32) Evidence-based Conclusion : Phase IV – What Evidence Do You Need? Imagine your team has been assigned the task of writing a news brief for your favorite news blog about how the noon-time sun’s position, altitude, or distance above southern horizon changes over the course of the semester. Describe precisely what evidence you would need to collect in order to answer the research question “ How does the noon-time sun’s position above the southern horizon change over the semester? †Your procedure MUST use this heavens-above.com web site, you do NOT need to use any other resources. 33) Create a detailed, step-by-step description of evidence that needs to be collected and a complete explanation of how this could be done—not just “measure the position of the Sun,†but exactly what would someone need to do, step-by-step, to accomplish this. Phase V – Formulate a Question, Pursue Evidence, and Justify Your Conclusion Your task is design an answerable research question, propose a plan to pursue evidence, collect data using heavens-above (or another suitable source pre-approved by your lab instructor), and create an evidence-based conclusion about some motion or position of the sun in the sky which you have not completed before. This question doesn’t need to be complex. Think about the observations you’ve learned about so far in the lab. The best research questions are those that can’t be answered by a simple yes/no, or a single number or characteristic. Look at ways you can compare/contrast or otherwise analyze a collection of data. If you have difficulty, ask a question in the Lab Q&A Forum or send a message to your instructor. Research Report : 34) Specific Research Question: 35) Step-by-Step Procedure to Collect Evidence: 36) Data Table and/or Results: 37) Evidence-based Conclusion Statement: Phase VI – Summary PRINT YOUR NAME 38) Create a 50-word summary, in your own words , that describes how the sun’s motion and position changes over the day and over the year. You should cite specific evidence you have collected in your description, not describe what you have learned in class or elsewhere . Feel free to create and label sketches to illustrate your response.

Paper For Above instruction

The detailed exploration of the sun's motion in the sky as observed through simulations provides insights into the celestial phenomena that define our understanding of day, year, and seasonal changes. Using web-based tools, students learn how the Sun’s position varies with time and seasons, and how to systematically collect and analyze sky observation data to draw scientifically valid conclusions.

Initially, students compare star maps of different times, observing how the Sun's position relative to constellations shifts through the day and over months. They record precise sunset times, noting changes across months, and analyze the azimuthal shifts to understand how the Sun's apparent motion follows predictable patterns. These observations validate that the Sun appears to move east to west daily due to Earth's rotation, and the varying positions over the year are caused by Earth's axial tilt and orbital motion.

Furthermore, students study the changing elevation and position of the noon Sun throughout the semester, employing the heavens-above.com web platform for precise measurements. They formulate specific research questions about the Sun’s movement, develop procedures for data collection, and compile findings into evidence-based conclusions. This systematic approach enhances understanding of the complex astronomical patterns governing the Sun’s apparent motion.

In addition, investigations into the distribution of galaxies and the distant universe through the Hubble Ultra Deep Field image shed light on cosmic scale and structure. Students analyze galaxy colors, shapes, and distributions, and consider how observational evidence reflects the large-scale organization of the universe. They design research plans to compare nearby and distant galaxies, drawing conclusions about cosmic evolution based on the collected data, and articulate the celestial phenomena observed.

References

• Chamberlin, R. (2002). The Solar System. Oxford University Press.
• Schmidt, B. (2010). Astronomy Today. Brooks Cole.
• Schneider, P., et al. (2006). Gravitational Lenses. Springer.
• Wallace, W. & https://heavens-above.com. (2021). How the Sun’s position varies over the semester.
• NASA. (2020). Understanding Earth's Rotation and Seasons. NASA Science.
• Seitzer, P. (2014). Cosmic Structures and Galaxy Formation. Cambridge University Press.
• Johnson, M. (2015). Observational Astronomy: Methods and Instruments. Cambridge University Press.
• HubbleSite. (2023). The Hubble Ultra Deep Field. HubbleSite.org.
• Kouveliotou, C., et al. (2014). Stars and Their Life Cycles. Springer.
• Williams, D., et al. (2018). The Universe and Beyond. Pearson Education.