Safely Estimating the Size of Sunspots

PURPOSE

There's more than meets the eye to the little yellow ball in the sky! Sunspots are relatively cool areas that appear as dark blemishes on the face of the Sun. Looking at solar telescope imagery, it's difficult to get a sense of the actual size of sunspots. In this activity, you will estimate the actual size of these features.

MATERIALS

  1. Internet access via Web browser, e.g., Netscape Communicator or Microsoft Internet Explorer
  2. Pencil, metric ruler, and hardcopy of near-real-time solar telescope imagery (showing sunspots)
  3. Scientific calculator

PROCEDURE

  1. Use a Web browser to access The very latest SOHO images Web page. Download/print the latest MDI Continuum solar image.
  2. In the following data table, record the image date and time. [Note Date/Time format: Date = yy/mm/dd; Time = UTC. Refer to a Time Conversion Chart to convert UTC to EST/EDT.]
  3. Using a metric ruler and the hardcopy solar image, carefully measure the diameter of the Sun (mm) and the width (mm) of the largest sunspot (along major axis); record these data in the data table (below). Circle and label the largest sunspot (e.g., "largest").
  4. Answer the Activity Questions.

DATA

Date
(mm/dd/yy)
Time
(EST/EDT)


FeatureScale Model Size
(mm)
Actual Size
(km)
Diameter of Sun

Largest Sunspot

Sunspot No. 2

Sunspot No. 3

ACTIVITY QUESTIONS

  1. Use a proportion (two equivalent ratios) to solve for the actual size of the largest sunspot. Show your work (below); record your answer in the data table (above).

  2. Compare/contrast the size of the largest sunspot with the diameter of the Earth (12,735 km). Approximately how many Earth diameters would fit inside the Sun's diameter? Show your work; circle your answer.


  3. The hardcopy MDI Continuum solar image is really a scale model of the Sun. Use the Sun's scale model diameter and actual diameter to determine the scale of the image (you may need to refer to a brief tutorial on determining fractional scale). Show your work; circle your answer. Use the image scale to estimate the size of two other sunspots; record the estimated size of these sunspots in the data table (above). Circle and label the two sunspots (e.g., "No. 2," "No. 3").


APPENDICES

  1. The very latest SOHO images
    http://sohowww.nascom.nasa.gov/data/realtime-images.html
  2. Time Conversion Chart
    http://www.wsanford.com/~wsanford/activities/timeconv.html
  3. Determining the Fractional Scale of a Map or Scale Model
    http://www.wsanford.com/~wsanford/activities/scale.html
  4. Converting Metric Units - Use the following list of metric units to count the number of units change, then move the decimal point (in the same direction in which you were counting) one place for each unit of change: For example, convert 1,100 cm to m by moving the decimal point 2 places to the left: 1,100 cm = 11 m (approximately 36 feet).