Lab#1 ast

Name: Date: 1 Tools for Success in ASTR 105G 1.1 Introduction Astronomy is a physical science. Just like biology, chemistry, geology, and physics, astronomers collect data, analyze that data, attempt to understand the object/subject they are looking at, and submit their results for publication. Along the way astronomers use all of the mathematical techniques and physics necessary to understand the objects they examine. Thus, just like any other science, a large number of mathematical tools and concepts are needed to perform astronomical research. In today’s introductory lab, you will review and learn some of the most basic concepts necessary to enable you to successfully complete the various laboratory exercises you will encounter during this semester. When needed, the weekly laboratory exercise you are performing will refer back to the examples in this introduction—so keep the completed examples you will do today with you at all times during the semester to use as a reference when you run into these exercises later this semester (in fact, on some occasions your TA might have you redo one of the sections of this lab for review purposes). 1.2 The Metric System Like all other scientists, astronomers use the metric system. The metric system is based on powers of 10, and has a set of measurement units analogous to the English system we use in everyday life here in the US. In the metric system the main unit of length (or distance) is the meter , the unit of mass is the kilogram , and the unit of liquid volume is the liter. A meter is approximately 40 inches, or about 4” longer than the yard. Thus, 100 meters is about 111 yards. A liter is slightly larger than a quart (1.0 liter = 1.101 qt). On the Earth’s surface, a kilogram = 2.2 pounds. As you have almost certainly learned, the metric system uses prefixes to change scale. For example, one thousand meters is one “kilometer.” One thousandth of a meter is a “millimeter.” The prefixes that you will encounter in this class are listed in Table 1.2. In the metric system, 3,600 meters is equal to 3.6 kilometers; 0.8 meter is equal to 80 centimeters, which in turn equals 800 millimeters, etc. In the lab exercises this semester we will encounter a large range in sizes and distances. For example, you will measure the sizes of some objects/things in class in millimeters, talk about the wavelength of light in nanometers, and measure the sizes of features on planets that are larger than 1,000 kilometers. Table 1.1: Metric System Prefixes 1

Prefix Name Prefix Symbol Prefix Value Giga G 1,000,000,000 (one billion) Mega M 1,000,000 (one million) kilo k 1,000 (one thousand) centi c 0.01 (one hundreth) milli m 0.001 (one thousandth) micro µ 0.0000001 (one millionth) nano n 0.0000000001 (one billionth) 1.3 Beyond the Metric System When we talk about the sizes or distances to objects beyond the surface of the Earth, we begin to encounter very large numbers. For example, the average distance from the Earth to the Moon is 384,000,000 meters or 384,000 kilometers (km). The distances found in astronomy are usually so large that we have to switch to a unit of measurement that is much larger than the meter, or even the kilometer. In and around the solar system, astronomers use “Astronomical Units.” An Astronomical Unit is the mean (average) distance between the Earth and the Sun. One Astronomical Unit (AU) = 149,600,000 km. For example, Jupiter is about 5 AU from the Sun, while Pluto’s average distance from the Sun is 39 AU. With this change in units, it is easy to talk about the distance to other planets. It is more convenient to say that Saturn is 9.54 AU away than it is to say that Saturn is 1,427,184,000 km from Earth. 1.4 Changing Units and Scale Conversion Changing units (like those in the previous paragraph) and/or scale conversion is something you must master during this semester. You already do this in your everyday life whether you know it or not (for example, if you travel to Mexico and you want to pay for a Coke in pesos), so do not panic! Let’s look at some examples ( 2 points each ): 1. Convert 34 meters into centimeters: Answer: Since one meter = 100 centimeters, 34 meters = 3,400 centimeters. 2. Convert 34 kilometers into meters: 34 kilommeters = 34000 meters 3. If one meter equals 40 inches, how many meters are there in 400 inches? 2

Approx. 600 km 8. If you were to drive 100 km/hr (kph), how long would it take you to go from LasCruces to Albuquerque? Since it is 352 km and we are going 100 kph, 3 hours 52 min. 9. If one mile = 1.6 km, how many miles per hour (mph) is 100 kph? Divide by 1.6, 62.137 mph 4

Figure 1.1: Map of New Mexico. 1.5 Squares, Square Roots, and Exponents In several of the labs this semester you will encounter squares, cubes, and square roots. Let us briefly review what is meant by such terms as squares, cubes, square roots and exponents. The square of a number is simply that number times itself: 3 × 3 = 3 2 = 9. The exponent 5

3“√×”, as in3). The mathematical operation of a square root is usually represented by the symbol√9 = 3 . But mathematicians also represent square roots using a fractional exponent of one half: 9 1 / 2 = 3. Likewise, the cube root of a number is represented as 27 1 / 3 = 3 (3 × 3 × 3 = 27). The fourth root is written as 16 1 / 4 (= 2), and so on. Here are some example problems: √ 100 = 10 • • 10.5 3 = 10.5 × 10.5 × 10.5 = 1157.625 • Verify that the square root of 17 (√17= 17 1 / 2 ) = 4.123 1.6 Scientific Notation The range in numbers encountered in Astronomy is enormous: from the size of subatomic particles, to the size of the entire universe. You are certainly comfortable with numbers like ten, one hundred, three thousand, ten million, a billion, or even a trillion. But what about a number like one million trillion? Or, four thousand one hundred and fifty six million billion? Such numbers are too cumbersome to handle with words. Scientists use something called “Scientific Notation” as a short hand method to represent very large and very small numbers. The system of scientific notation is based on the number 10. For example, the number 100 = 10 × 10 = 10 2 . In scientific notation the number 100 is written as 1.0 × 10 2 . Here are some additional examples: • Ten = 10 = 1 × 10 = 1.0 × 10 1 • One hundred = 100 = 10 × 10 = 10 2 = 1.0 × 10 2 • One thousand = 1,000 = 10 × 10 × 10 = 10 3 = 1.0 × 10 3 • One million = 1,000,000 = 10 × 10 × 10 × 10 × 10 × 10 = 10 6 = 1.0 ×10 6 Ok, so writing powers of ten is easy, but how do we write 6,563 in scientific notation? 6,563 = 6563.0 = 6.563 × 10 3 . To figure out the exponent on the power of ten, we simply count the 7

numbers to the left of the decimal point, but do not include the left-most number. Here are some more examples: • 1,216 = 1216.0 = 1.216 × 10 3 • 8,735,000 = 8735000.0 = 8.735000 × 10 6 • 1,345,999,123,456 = 1345999123456.0 = 1.345999123456 × 10 12 ≈ 1.346 × 10 12 Note that in the last example above, we were able to eliminate a lot of the “unnecessary” digits in that very large number. While 1.345999123456 × 10 12 is technically correct as the scientific notation representation of the number 1,345,999,123,456, we do not need to keep all of the digits to the right of the decimal place. We can keep just a few, and approximate that number as 1.346 × 10 12 . Your turn! Work the following examples (2 points each): 13. 121 = 121.0 =1.21*10^2 14. 735,000 = 7.35000=7.35*10^5 15. 999,563,982 = 9.99563982 = 9.99563982*10^8 Now comes the sometimes confusing issue: writing very small numbers. First, lets look at powers of 10, but this time in fractional form. The number 0.1 = . In scientific notation we would write this as 1the fraction. How about 0.001? We can rewrite 0.001 as× 10 −1 . The negative number in the exponent is the way we write 10 −3 . Do you see where the exponent comes from? Starting at the decimal point, we simply count over to the right of the first digit that isn’t zero to determine the exponent. Here are some examples: • 0.121 = 1.21 × 10 −1 8

Entering numbers in scientific notation into your calculator depends on layout of your calculator; we cannot tell you which buttons to push without seeing your specific calculator. However, the “E” button described above is often used, so to enter 6.589need to type 6.589 “E” 7. ×10 7 , you may Verify that you can enter the following numbers into your calculator: • 7.99921 ×10 21 • 2.2951324 ×10 −6 1.7.2 Order of Operations When performing a complex calculation, the order of operations is extremely important. There are several rules that need to be followed: i. Calculations must be done from left to right. ii. Calculations in brackets (parenthesis) are done first. When you have more than oneset of brackets, do the inner brackets first. iii. Exponents (or radicals) must be done next.iv. Multiply and divide in the order the operations occur. v. Add and subtract in the order the operations occur. If you are using a calculator to enter a long equation, when in doubt as to whether the calculator will perform operations in the correct order, apply parentheses. Use your calculator to perform the following calculations (2 points each): 20. = 41/25 = 1 16/25 21. (4 2 + 5) − 3 = 18 22. 20 ÷ (12 − 2) × 3 2 − 2 = 16 10

1.8 Graphing and/or Plotting Now we want to discuss graphing data. You probably learned about making graphs in high school. Astronomers frequently use graphs to plot data. You have probably seen all sorts of graphs, such as the plot of the performance of the stock market shown in Fig. 1.2. A plot like this shows the history of the stock market versus time. The “x” (horizontal) axis represents time, and the “y” (vertical) axis represents the value of the stock market. Each place on the curve that shows the performance of the stock market is represented by two numbers, the date (x axis), and the value of the index (y axis). For example, on May 10 of 2004, the Dow Jones index stood at 10,000. Plots like this require two data points to represent each point on the curve or in the plot. For comparing the stock market you need to plot the value of the stocks versus the date. We call data of this type an “ordered pair.” Each data point requires a value for x (the date) and y (the value of the Dow Jones index). Table 1.2 contains data showing how the temperature changes with altitude near the Earth’s surface. As you climb in altitude, the temperature goes down (this is why high mountains can have snow on them year round, even though they are located in warm areas). The data points in this table are plotted in Figure 1.3. 1.8.1 The Mechanics of Plotting When you are asked to plot some data, there are several things to keep in mind. Figure 1.2: The change in the Dow Jones stock index over one year (from April 2003 to July 2004). Table 1.2: Temperature vs. Altitude 11

Figure 1.3: The change in temperature as you climb in altitude with the data from Table 1.2. At sea level (0 ft altitude) the surface temperature is 59 o F. As you go higher in altitude, the temperature goes down. 1.8.2 Plotting and Interpreting a Graph Table 1.3 contains hourly temperature data on January 19, 2006, for two locations: Tucson and Honolulu. 23. On the blank sheet of graph paper in Figure 1.4, plot the hourly temperatures measured for Tucson and Honolulu on 19 January 2006. ( 10 points ) 24. Which city had the highest temperature on 19 January 2006? ( 2 points ) Honolulu 13

25. Which city had the highest average temperature? ( 2 points ) Honolulu Table 1.3: Hourly Temperature Data from 19 January 2006 Time Tucson Temp. Honolulu Temp. hh:m m o F o F 00:00 49.6 71.1 01:00 47.8 71.1 02:00 46.6 71.1 03:00 45.9 70.0 04:00 45.5 72.0 05:00 45.1 72.0 06:00 46.0 73.0 07:00 45.3 73.0 08:00 45.7 75.0 09:00 46.6 78.1 10:00 51.3 79.0 11:00 56.5 80.1 12:00 59.0 81.0 13:00 60.8 82.0 14:00 60.6 81.0 15:00 61.7 79.0 16:00 61.7 77.0 17:00 61.0 75.0 18:00 59.2 73.0 19:00 55.0 73.0 20:00 53.4 72.0 21:00 51.6 71.1 22:00 49.8 72.0 23:00 48.9 72.0 24:00 47.7 72.0 26. Which city heated up the fastest in the morning hours? ( 2 points ) Honolulu rose more steadily While straight lines and perfect data show up in science from time to time, it is actually quite rare for real data to fit perfectly on top of a line. One reason for this is that all 14

that the Moon is a lot closer to the Earth than Mars is. So if you are asked to calculate the Earth-Moon distance and you get an answer of 4.5 AU, this should alarm you! That would imply that the Moon is three times farther away from Earth than Mars is! And you know that’s not right. Use your intuition to answer the following questions. In addition to just giving your answer, state why you gave the answer you did. ( 5 points each ) 27. Earth’s diameter is 12,756 km. Jupiter’s diameter is about 11 times this amount. Which makes more sense: Jupiter’s diameter being 19,084 km or 139,822 km? 139,822 km. 28. Sound travels through air at roughly 0.331 kilometers per second. If BX 102 suddenly exploded, which would make more sense for when people in Mesilla (almost 5 km away) would hear the blast? About 14.5 seconds later, or about 6.2 minutes later? About 14.5 seconds 29. Water boils at 100 ◦ C. Without knowing anything about the planet Pluto other than the fact that is roughly 40 times farther from the Sun than the Earth is, would you expect the surface temperature of Pluto to be closer to -100 ◦ or 50 ◦ ? 16

-100 degrees 1.10 Putting it All Together We have covered a lot of tools that you will need to become familiar with in order to complete the labs this semester. Now let’s see how these concepts can be used to answer real questions about our solar system. Remember, ask yourself does this make sense? for each answer that you get! 30. To travel from Las Cruces to New York City by car, you would drive 3585 km. Whatis this distance in AU? ( 10 points ) 0.000024 31. The Earth is 4.5 billion years old. The dinosaurs were killed 65 million years ago dueto a giant impact by a comet or asteroid that hit the Earth. If we were to compress the history of the Earth from 4.5 billion years into one 24-hour day, at what time would the dinosaurs have been killed? ( 10 points ) 11:40 pm 17