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1997 BC Exam
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1.5 Functions and Logarithms Greg Kelly, Hanford High School, Richland, WashingtonPhoto by Vickie Kelly, 2004 Golden Gate Bridge San Francisco, CA
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A relation is a function if: for each x there is one and only one y. A relation is one-to-one if also: for each y there is one and only one x. In other words, a function is one-to-one on domain D if: whenever
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To be one-to-one, a function must pass the horizontal line test as well as the vertical line test. one-to-onenot one-to-onenot a function (also not one-to-one)
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Inverse functions: Given an x value, we can find a y value. Switch x and y : (eff inverse of x) Inverse functions are reflections about y = x. Solve for x :
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example 3: Graph: for a parametrically: 3 menu 3 enter 1 menu 4 Zoom to [-1,7] x [-1,3] menu 4 Zoom Square B
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b Find the inverse function: Switch x & y: Graph the curves as functions. example 3: Graph: for Clear the previous graph. ctrl =
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Consider This is a one-to-one function, therefore it has an inverse. The inverse is called a logarithm function. Example: Two raised to what power is 16? The most commonly used bases for logs are 10: and e : is called the natural log function. is called the common log function.
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is called the natural log function. is called the common log function. In calculus we will use natural logs exclusively. We have to use natural logs: Common logs will not work.
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English translation by Edward Wright A Few Historical Notes: Logarithm is the combination of two Greek roots, Logos (reason or ratio) + artihmus (number). The word logarithm was introduced in Napier’s 1614 work, Mirifici Logarithmorum canonis descriptio, (description of the wonderful canon of logarithms), originally published in Latin. Logarithms were "invented" by a Scottish nobleman named John Napier (1550-1617).
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Astronomer Johannes Kepler read Napier’s work in 1616, and used logarithms in developing his Third Law of Planetary Motion. Kepler published the third law in 1620 in a book titled Euphemerides, dedicated to Napier. He later published his own work on logarithms. Kepler’s Third Law states: The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
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Surprisingly, the notation ln for natural logs was not first used until 1893 by an American, Washington Irving Stringham (1847-1909). The term “natural logarithm” (actually “logarithm Ephemerides us naturalis”) was first used by an Italian mathematician, Pietro Mengoli (1626- 1686). “In place of e log we shall henceforth use the shorter symbol ln, made up of the initial letters of logarithm and of natural or Napierian”
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Even though we will be using natural logs in calculus, you may still need to find logs with other bases occasionally. On the TI-nspire you can find the log of any base by using. ctrl log If you leave the base blank, it assumes you want a common log. For example: Or you can specify the base:
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Here are shortcuts for accessing the various symbol palettes on the TI-inspire: ctrl Characters/Symbols: Expression Templates: Trig Symbols: trig Symbols (, etc): Equalities & Inequalities: ctrl = Punctuation Mark: ?!
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Properties of Logarithms Since logs and exponentiation are inverse functions, they “un-do” each other. Product rule: Quotient rule: Power rule: Change of base formula:
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Example 6: $1000 is invested at 5.25 % interest compounded annually. How long will it take to reach $2500? We use logs when we have an unknown exponent. 17.9 years In real life you would have to wait 18 years.
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