Grade Level/Subject Unit Enduring Understanding SOL Objectives 11th/12th Astronomy The Sun Dynamic finite processes occurring in and around the Sun are responsible for creating all forms of electromagnetic radiation, and drive processes occurring on Earth and the forms of life that inhabit it. SOL 6.8 - The student will investigate and understand the organization of the solar system and the interactions among the various bodies that comprise it. d) revolution and rotation; Title Lesson Objective Sun Spotting Inquiry Level Sun spots are dynamic phenomena on the sun The sun rotates at different rates at different latitudes (differential rotation) 3 – Question given, methods open, solution open Materials Required Telescope with solar filter (Mylar or otherwise) or Binoculars and stiff screen to project images on Stiff piece of white poster board, roughly 8”x11.5” for the projector screen Magnetic Compass Sun Spotting In this lab, we will be investigating the motions of sunspots across the surface of the sun. 1. Before starting this lab, how do you think sunspots move and change across the surface of the sun? 2. What could cause sunspots to move on the surface of the sun? Sunspots on the Sun as seen by SOHO Source: NASA.gov 3. Looking at the sunspots in the image at the upper right, what do you notice about the size, clustering, and location of sunspots. a. Size: b. Clustering: c. Location: 4. If the sun had a solid surface as the earth does, how do you think sunspots would then move? 5. Knowing that the sun is more like a liquid, how do you think sunspots could move? 6. Do sunspots near the equator have a larger distance or smaller distance to travel compared to sunspots at 45 latitude (halfway to the northern pole)? Create a sunspot viewing station CAUTION: Looking directly at the sun can cause serious eye damage, even blindness. NEVER look directly at the sun. Never use binoculars to look at the sun. Follow the instructions at the following website to setup your sunspot viewing station. http://spaceweather.com/sunspots/doityourself.html Once you have obtained an image, identify sunspots. Place your sun coordinate grid under your image so that the north (N) is pointed towards cardinal south according to your compass. Images that project onto screens are inverted, so we have to flip our axes to better line up our sun’s image. Identify sunspots by numbering them. They will persist for a couple of days to weeks, so be sure you can identify the same spot day-to-day. Under Sunspot ID, insert the identifier you assigned to your sunspots. Under Day #, insert the date (for instance, 3/17 for March 17th). And at each day and sunspot, record the latitude and longitude. For instance, Lat: 15 N, Long 10 W. You should try to get seven data points for each sunspot. Some months, there may be very few to no sunspots, other months there may be dozens. Try to identify the most evident ones. Sunspot Day 1 Day 2 Day 3 Day 4 Day 5 Day 6 Day 7 ID _______ _______ _______ _______ _______ _______ _______ For each Sunspot listed in your table, plot the data on a separate piece of graph paper with the axes listed below. Plot each sunspot in a different color and make a legend so that they are easily identifiable. Make sure to properly label your axes, include units, and a title. 1. Plot Longitude versus time 2. Plot Latitude versus time Note four trends that you see in your graphs. 1. 2. 3. 4. By looking at sunspot movement, astronomers can pinpoint the rotation rate of the sun. Estimate the rotation rate at different latitudes from your data. For instance, if you notice that one sunspot moves from longitude 30 E to 20 W in 3 days, we can estimate the rotation rate using ratios: 𝑡 360° = 3 50° Therefore, 𝑡 = 21.6 days for one complete rotation. Use this information to fill in the table on the next page. Be sure to order your data from lowest latitude to highest. Latitude versus rotation period of the sun Latitude () Rotation Period (days) Discuss any trends you see in your data. From your data, does the sun seem to rotate like a solid (like the earth), or is there another type of rotation that appears to be happening?
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