10

10

10

10

and so forth.

You'll notice how the power on the 10 equals the number of zeros after the 1. How do you write 560,000,000? You might notice that this number is also equal to 5.6 x 100,000,000, which can be written as 5.6 x 10

10^{0} = 1 (any number to the power of 0 = 1)

10^{-1} = 0.1

10^{-2} = 0.01

10^{-3} = 0.001

and so forth.

Let's try some more. How would you write the following numbers?

- 0.00045
- 345000
- 0.066
- -0.000102
- -53000

The next thing that you might have to do with numbers in scientific
notation is to multiply or divide them. Generally this is pretty easy
with a calculator. One of the things people don't know about their
calculators is that there is usually a built in key that allows you to represent
numbers in scientific notation in your calculator. The key is usually labeled with **EE**
or **Exp** - what it actually is called will depend upon the type of
calculator you have.

Let's go through an example of how you put a number into your calculator. Let's say you want to do the following problem -

4.5 x 10^{-5} x 3.3 x 10^{6}.

1. Put in the front part of the first number, 4.5 in this case.

2. Press the EE or Exp key. This usually causes a "00" or a "x10" to show up.

3. Enter the power on the 10, in this case -5. You don't want to use the subtraction key; use a key labeled ± or +/-. Don't put a "10" in since your calculator already has taken care of that.

4. Now press the multiply key.

5. Enter the second number, first the 3.3.

6. Press the EE or Exp key.

7. Put the power that is operating on the 10 in, which is 6 in this case.

8. Now press the equals or enter key to finish off the calculation.

If everything went all right, you should have gotten 148.5 (or 1.485 x 10

Here are some examples to try out - try to get the correct answer in each case

- 9.9 x 10
^{-5}x 4.5 x 10^{-8} - 1.02 x 10
^{4}/ 3.3 x 10^{-9} - 4.0 x 10
^{-2}x 1.0 x 10^{8} - 8.2 x 10
^{9}x 5.3 x 10^{8} - 9.8 x 10
^{19}+ 4.2 x 10^{-9}

In case you don't have a calculator, you can still do the math,
mainly the multiplication and division, by following these rules -

- Multiplication: multiply the two front numbers, and then add the powers.
- Division: divide the two front numbers, and then subtract the powers.

If you don't believe this, try the practice problems above without a calculator or without using the EE/EXP key. You should get the same answers. Actually, you will only want to do this with problems 1-4 since the last one is an addition.

**WORD OF WARNING:** If you use a calculator to work with numbers
in scientific notation, your calculator may write them in a way that
they are not normally written. For example, the number 3.4 x 10^{22}
could appear in your calculator like **3.4 22**
or **3.4 ^{22}**. The "x 10"
part is often excluded to save space. If you were to do a
calculation and your calculator gives an answer similar to that shown
above (without the "x 10" part), make sure you write the number out
correctly - don't forget to write out the "x 10" part.

Why? There is a big difference between those numbers. If
your calculator displays 3.4 ^{22}, and you write on your
answer sheet 3.4 ^{22}, you'll lose points, since 3.4 ^{22}
means 3.4 taken to the power of 22, not what it is supposed to mean (3.4
x 10^{22}). That's a big difference - don't be lazy;
write out the number properly.

**When do you use scientific notation?** This is one of those questions that
doesn't have a solid answer. If you have a number like -0.2, or 123, you really don't need
to write them in scientific notation, since that would be a bit silly and make the number
harder to read. In general it is best to use scientific notation if the number is in the
millions or greater, or if it is smaller than 0.001. While these are only guidelines
you should do whatever you are comfortable with.

1. Digits other than zero are always significant.

2. Zeros between other SF are significant. For example, 4003 has four SF.

3. Zeros to the

4. When a number

5. When a number ends in zeros that are to the left of the decimal point location, the zeros are not necessarily significant. For example, 440 certainly has at least two SF, but the 0 may or may not be significant. You'd probably have to know more about the number, particularly how it was determined. One way to remove the ambiguity is to include the decimal point in the number. If I wrote "440." then I would want to include the zero as a SF, so there are now three SF in the number. Writing just "440" doesn't make it clear as to whether the zero is significant or not. Including a decimal point will help. So "329000" has three clearly SF, but the rest are uncertain. The number "329000." has six SF.

Sometimes a zero is included after a decimal to show that there is a need for greater accuracy, so that 3.20 has three SF, while 3.2 only has two. For some reason the person who wrote 3.20 wanted greater accuracy when the number is used in further calculations, and the rounding rules for significant figures takes effect (we'll get to those later).

Here are some for you to try - determine the number of SF in each number

- 6.751
- 0.157
- 28.0
- 2500
- 0.070
- 30.07
- 0.0067
- 6.02 x 10
^{23}

Now to actually use SF. If the numbers you are using are measurements of some sort, odds are they are not exactly accurate, and the level of accuracy is given by the number of SF. In the case of addition and subtraction, your final answer should have the same number of decimal places as the value with the least number of decimal places. If you were to take 9.221 - 7.01 your answer should be 2.21, not 2.211. It is best to determine the number of SF when you get to the end of all of your mathematical steps - so when you are ready to write down the final answer, double check to see how many SF you should write down.

For multiplication and division, the answer can’t be more accurate than the least accurate part. If you were to multiply 3.209 by 2.2 your answer should have only two SF in it since that is the least number of SF in the values you were given. You should write the answer as 7.1, not as 7.0598, which is the number your calculator spits out.

A word of warning - if you are using a number that is not a measured quantity like a constant that has an exact value, you should not use it to decide the number of SF in your final answer. Exact values or constants are considered to have an infinite number of SF. For example to calculate the circumference of a circle, you use the formula 2 r, where =3.14 (or more SF) and r is the radius of the circle. How many SF will your answer have? Should there be only 1 SF, since that is how many are in the 2? No. The 2 is not a measurement but a constant, a part of the formula. The same rule applies to the The number of SF would depend upon the number of SF in the r, so depending upon the value of r, the number of SF in your answer can vary.

Here are some examples to try - determine the answer for each using the proper number of SF.

- 3.4 + 0.00344
- 4.50 x 3.3005
- 9.01/7.88
- 4.510 x 10
^{12}x 3.401 x 10^{-11} - 607.1 x 4.4

grams - gm

kilometers - km

centimeters - cm

millimeters - mm

Ångstroms - Å

The trickiest thing is trying to remember what each of these things are in case you have to convert from one unit to another. Here is a listing if you need to convert from one value to another.

1 kg = 1000 gm

1 gm = 0.001 kg

1 meter = 100 cm = 1000 mm = 0.001 km = 10^{10} Å

1 cm = 10 mm = 0.00001 km (10^{-5} km) = 0.01 m = 10 ^{8}
Å

1 mm = 0.000001 km (10^{-6} km) = 0.001 m = 0.1 cm = 10 ^{7}Å

1 km = 1000 m = 100,000 cm = 1,000,000 mm = 10^{13} Å

1 Å = 10^{-10 }m = 10^{-8} cm = 10^{-7} mm
= 10 ^{-13} km

There are also some non-metric distances that are set up just for
convenience. For example, there is the distance between the Earth and
the Sun, which is defined as 1 **A. U.** (**Astronomical Unit**).
This is useful for measuring distances within the solar system. There is
also the distance of a** light-year** - the distance light travels in
one year. **Parsec** is another distance which is often used
interchangeably with light-year. These are often used to indicate the
distances between stars. For even greater distances there are
kiloparsecs and kilo light-years (1 kiloparsec = 1000 parsecs, 1 kilo
light-year = 1000 light-years) and for very great distances there is the
mega parsec (a million parsecs) and mega light-years (a million
light-years). The actual values for these distances and other common
units of measure can be found in the table of constants.