Estimating ET
    Astronomy and Cosmologies - Spring 2004
    Goals
    Equipment
    Homework
    Predictions
    Activities
    Learning
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    This is an in-class workshop for week 1. Work in teams of about 4. Write your answers, ideas, and questions on your own copy. Summarize your team's results on your feedback form and hand it in at the end of class.  Save your workshop for your portfolio; you need not turn it in today. 

    GOALS

    SCIENCE: To think about the possibility of life in our galaxy.

    ESTIMATION: To learn to do order of magnitude estimates, a powerful technique in physics and astronomy.

    SCIENTIFIC NOTATION: To learn to use powers of ten notation to easily describe large and small quantities.

    SIGNIFICANT FIGURES: To learn to evaluate how much precision is necessary or possible, and to let go of unreal precision.

    UNCERTAINTY: To learn to quantify the precision of your estimates.

    EQUIPMENT: Your brain and pencil; NO CALCULATORS or computers.

    PREDICTIONS: First you and your team will make some guesses about the likelihood of conditions that could lead to intelligent life. Then you will use these to estimate the likelihood that an extraterrestrial intelligence (ET) might contact us. Before we start, make two guesses:

    1. What fraction of stars in our galaxy might have intelligent, communicating civilizations? _____

    2. How many intelligent, communicating civilizations might there be in our galaxy? _____

     

    ACTIVITIES

    A. Make an estimate for each question below. B. Explain your reasoning. C. Estimate the uncertainty in your guess. Could it be twice as big? 100 times smaller? More?

    (1) What fraction of the stars in our galaxy are similar to the Sun? S=____

    (1.b) Reason:

    (1.c) Uncertainty?

    (2) What fraction of those sun-like stars might have planets? fp = ____

    (2.b) Reason:

    (2.c) Uncertainty?

    (3) How many "earths" would the average planetary system have? Ne = ____

    (3.b) Reason:

    (3.c) Uncertainty?

    (4) On what fraction of those earth-like planets would life develop? fl = _____

    (4.b) Reason:

    (4.c) Uncertainty?


    (5) On what fraction of those planets with life would the life develop intelligence? fi = ____

    (5.b) Reason:

    (5.c) Uncertainty?

    (6) On what fraction of those planets with intelligent life would technology develop? fc = ____

    (6.b) Reason:

    (6.c) Uncertainty?


    (7) Estimate the fraction of the planet's lifetime during which the average communicating civilization survives: civilization's lifetime ____ / planet's lifetime ____ = ______ = L

    (7.b) Reason:

    (7.c) Uncertainty?

     

    Discuss your estimates with your teammates. You need not agree, but you should note the range of estimates and their justifications.


    D. Combine your guesses to estimate the number of communicative civilizations in our galaxy. First get back together with the whole class. One team will share its data at the board, and Zita will demonstrate how to easily calculate an order-of-magnitude estimate using scientific notation. Then you will practice the method with your own data.

    1. The fraction of stars in our galaxy with communicative civilizations = x = S* Fp * Ne * Fl * Fi * Fc * L

     

     

    How many stars would there have to be in our galaxy for there to be at least one communicating civilization? (Hint: invert x. Why?)

     

    2. If there are 100 billion stars in the Milky Way, how many communicating civilizations would there be? Call this N.

     


    E. Calculate the uncertainty in your estimate. The fractional uncertainty in N is equal to the sum of the fractional uncertainties in each factor. (Fractional uncertainties are unitless.)

     

     

    Then you can find the total uncertainty dN = N * f , which has units of number of civilizations.

     

    F. Now consider how much precision it is reasonable to retain in your estimate for N. Write your estimate +/- uncertainty:

    N +/- dN = _______ +/- ________

    Your uncertainty dN tells you how many decimal places you can reasonably keep in your N. For example, if you find N = 14.72836 and dN = 2, then you know N only to whole number precision: N = 15 +/- 2.

    Keep this in mind when you calculate in the future. Often in astronomy, our data is quite approximate, so even if your calculator gives you many decimal places, most of them are not significant. Retain only significant figures, and do not waste your time on meaningless precision. Order of magnitude estimates are often the best we can do, and they can be quite interesting and useful. As you develop your skill in making order-of-magnitude estimates, you can impress your friends with back-of-the envelope calculations


    G. Reflect on the meaning and consequences of your calculation. Can we expect to hear from ET? How certain are you of your answer? Are there other factors you might want to take into consideration?


     

    LEARNING

    Think about the key points you have learned. What surprised you? Compare your final results to your initial guesses 1. and 2. What is still unclear? Is there anything you need help with before you can meet your learning goals? What else would you like to learn, beyond this workshop?

    Please fill out a workshop feedback form and hand it in at the end of class. Everyone on your team should contribute to the feedback. Please summarize your team's results in your feedback form.

    Source and credits; example

    Maintained by: E.J. Zita