#set document(title: "1.2 Physical Quantities and Units", author: "OpenStax / XYZ Homework") #set page(width: 8.5in, height: auto, margin: 1in) #import "@preview/cetz:0.5.2" #set text(font: ("STIX Two Text", "Libertinus Serif", "New Computer Modern"), size: 10.5pt, lang: "en") #show math.equation: set text(font: ("STIX Two Math", "New Computer Modern Math")) #set par(justify: true, leading: 0.62em, spacing: 0.9em) #set enum(spacing: 1.1em) // room between list items so tall inline fractions don't collide #set list(spacing: 1.1em) #set table(stroke: 0.5pt + rgb("#c7ccd3")) #let BLUE = rgb("#183B6F") // brand navy — section bars + example/solution labels (white on navy 11.09:1) #let ORANGE = rgb("#A94509") // brand primary-700 — AA-safe deep orange for TEXT (5.93:1 on white; raw brand #F37021 is 2.94:1 and must never carry text) #let RED = rgb("#DC2626") // brand error-600 #let GREEN = rgb("#059669") // brand success-600 (decoration only; small green text uses green-text #007942) #show heading.where(level: 1): it => block(width: 100%, above: 0pt, below: 16pt, fill: gradient.linear(BLUE, rgb("#2C5AA0")), inset: (x: 14pt, y: 12pt), radius: 3pt, text(fill: white, weight: "bold", size: 19pt, it.body)) #show heading.where(level: 2): it => block(width: 100%, above: 18pt, below: 10pt, fill: BLUE, inset: (x: 10pt, y: 6pt), radius: 2pt, text(fill: white, weight: "bold", size: 12pt, it.body)) #show heading.where(level: 3): it => text(fill: ORANGE, weight: "bold", size: 12.5pt, it.body) #show heading.where(level: 4): it => text(fill: BLUE, weight: "bold", size: 10.5pt, it.body) #let examplebox(label, title, body) = block(width: 100%, breakable: true, fill: rgb("#EFF1F5"), stroke: 0.5pt + rgb("#CFDDF0"), radius: 4pt, inset: 10pt, above: 12pt, below: 12pt)[ #block(below: 6pt)[#box(fill: BLUE, inset: (x: 6pt, y: 2pt), radius: 2pt, text(fill: white, weight: "bold", size: 8.5pt, label)) #h(0.4em) #strong[#title]] #body] // rail = decorative left rule (raw brand token); labelcolor = AA-safe label text shade #let notebox(label, rail, labelcolor, tint, body) = block(width: 100%, breakable: true, fill: tint, stroke: (left: 3pt + rail), inset: (left: 10pt, rest: 8pt), radius: (right: 4pt), above: 11pt, below: 11pt)[ #text(fill: labelcolor, weight: "bold", size: 7.5pt, tracking: 0.5pt)[#upper(label)] #linebreak() #body] #let solutionbox(body) = block(above: 4pt, below: 8pt)[ #text(fill: BLUE, weight: "bold", size: 8.5pt)[Solution] #linebreak() #body] #let figph(msg) = block(width: 100%, height: 60pt, fill: rgb("#f6f7f9"), stroke: (paint: rgb("#c7ccd3"), dash: "dashed"), radius: 4pt, inset: 10pt)[ #align(center + horizon, text(fill: rgb("#889"), style: "italic", size: 9pt, msg))] // Standardize inlined figure sizes: measure the natural CeTZ canvas, then scale to a // consistent envelope (aspect-aware; see build_typst.py FIG_* constants). Unlike the // print preamble, dimensions are FLOORED: in an editor a user can trim a figure to a // degenerate 1-D shape (a bare line), and w/h or tw/w would then divide by zero. #let _STD_W = 3.5 #let _WIDE_W = 5.6 #let _MAX_H = 3.4 #let _ASPECT_WIDE = 2.2 #let _UPSCALE_MAX = 1.15 #let stdfig(body) = context { let m = measure(body) let w = calc.max(m.width / 1in, 0.01) let h = calc.max(m.height / 1in, 0.01) let tw = if w / h > _ASPECT_WIDE { _WIDE_W } else { _STD_W } let s = calc.min(tw / w, _MAX_H / h, _UPSCALE_MAX) align(center, box(scale(x: s * 100%, y: s * 100%, reflow: true, body))) } #show figure: set block(breakable: false) #set figure(gap: 8pt) #show figure.caption: set text(size: 8.5pt, fill: rgb("#555")) == 1.2#h(0.6em)Physical Quantities and Units === Learning Objectives By the end of this section, you will be able to: - Perform unit conversions both in the SI and English units. - Explain the most common prefixes in the SI units and be able to write them in scientific notation. #figure(figph[A view of Earth from the Moon.], alt: "A view of Earth from the Moon.", caption: [The distance from Earth to the Moon may seem immense, but it is just a tiny fraction of the distances from Earth to other celestial bodies.]) The range of objects and phenomena studied in physics is immense. From the incredibly short lifetime of a nucleus to the age of the Earth, from the tiny sizes of sub-nuclear particles to the vast distance to the edges of the known universe, from the force exerted by a jumping flea to the force between Earth and the Sun, there are enough factors of 10 to challenge the imagination of even the most experienced scientist. Giving numerical values for physical quantities and equations for physical principles allows us to understand nature much more deeply than does qualitative description alone. To comprehend these vast ranges, we must also have accepted units in which to express them. And we shall find that (even in the potentially mundane discussion of meters, kilograms, and seconds) a profound simplicity of nature appears—most physical quantities can be expressed as combinations of only four fundamental physical quantities: length, mass, time, and electric current. We define a #strong[physical quantity] either by #emph[specifying how it is measured] or by #emph[stating how it is calculated] from other measurements. For example, we define distance and time by specifying methods for measuring them, whereas we define #emph[average speed] by stating that it is calculated as distance traveled divided by time of travel. Measurements of physical quantities are expressed in terms of #strong[units], which are standardized values. For example, the length of a race, which is a physical quantity, can be expressed in units of meters (for sprinters) or kilometers (for distance runners). Without standardized units, it would be extremely difficult for scientists to express and compare measured values in a meaningful way. () #figure(figph[A boy looking at a map and trying to guess distances with unit of length mentioned as cables between two points.], alt: "A boy looking at a map and trying to guess distances with unit of length mentioned as cables between two points.", caption: [Distances given in unknown units are maddeningly useless.]) There are two major systems of units used in the world: #strong[SI units] (also known as the metric system) and #strong[English units] (also known as the customary or imperial system). #emph[English units] were historically used in nations once ruled by the British Empire and are still widely used in the United States. Virtually every other country in the world now uses SI units as the standard; the metric system is also the standard system agreed upon by scientists and mathematicians. The acronym “SI” is derived from the French #emph[Système International]. === SI Units: Fundamental and Derived Units gives the fundamental SI units that are used throughout this textbook. This text uses non-SI units in a few applications where they are in very common use, such as the measurement of blood pressure in millimeters of mercury (mm Hg). Whenever non-SI units are discussed, they will be tied to SI units through conversions. #figure(table( columns: 4, align: left, inset: 6pt, table.header([#emph[Length]], [#emph[Mass]], [#emph[Time]], [#emph[Electric Current]]), [meter (m)], [kilogram (kg)], [second (s)], [ampere (A)], )) It is an intriguing fact that some physical quantities are more fundamental than others and that the most fundamental physical quantities can be defined #emph[only] in terms of the procedure used to measure them. The units in which they are measured are thus called #strong[fundamental units]. In this textbook, the fundamental physical quantities are taken to be length, mass, time, and electric current. (Note that electric current will not be introduced until much later in this text.) All other physical quantities, such as force and electric charge, can be expressed as algebraic combinations of length, mass, time, and current (for example, speed is length divided by time); these units are called #strong[derived units]. === Units of Time, Length, and Mass: The Second, Meter, and Kilogram ==== The Second The SI unit for time, the #strong[second] (abbreviated s), has a long history. For many years it was defined as 1/86,400 of a mean solar day. More recently, a new standard was adopted to gain greater accuracy and to define the second in terms of a non-varying, or constant, physical phenomenon (because the solar day is getting longer due to very gradual slowing of the Earth’s rotation). Cesium atoms can be made to vibrate in a very steady way, and these vibrations can be readily observed and counted. In 1967 the second was redefined as the time required for 9,192,631,770 of these vibrations. () Accuracy in the fundamental units is essential, because all measurements are ultimately expressed in terms of fundamental units and can be no more accurate than are the fundamental units themselves. #figure(figph[A top view of an atomic fountain is shown. It measures time using the vibration of the cesium atom.], alt: "A top view of an atomic fountain is shown. It measures time using the vibration of the cesium atom.", caption: [An atomic clock such as this one uses the vibrations of cesium atoms to keep time to a precision of better than a microsecond per year. The fundamental unit of time, the second, is based on such clocks. This image is looking down from the top of an atomic fountain nearly 30 feet tall!]) ==== The Meter The SI unit for length is the #strong[meter] (abbreviated m); its definition has also changed over time to become more accurate and precise. The meter was first defined in 1791 as 1/10,000,000 of the distance from the equator to the North Pole. This measurement was improved in 1889 by redefining the meter to be the distance between two engraved lines on a platinum-iridium bar now kept near Paris. By 1960, it had become possible to define the meter even more accurately in terms of the wavelength of light, so it was again redefined as 1,650,763.73 wavelengths of orange light emitted by krypton atoms. In 1983, the meter was given its present definition (partly for greater accuracy) as the distance light travels in a vacuum in 1/299,792,458 of a second. () This change defines the speed of light to be exactly 299,792,458 meters per second. The length of the meter will change if the speed of light is someday measured with greater accuracy. #figure(figph[Beam of light from a flashlight is represented by an arrow pointing right, traveling the length of a meter stick.], alt: "Beam of light from a flashlight is represented by an arrow pointing right, traveling the length of a meter stick.", caption: [The meter is defined to be the distance light travels in 1/299,792,458 of a second in a vacuum. Distance traveled is speed multiplied by time.]) ==== The Kilogram The SI unit for mass is the #strong[kilogram] (abbreviated kg); it was previously defined to be the mass of a platinum-iridium cylinder kept with the old meter standard at the International Bureau of Weights and Measures near Paris. Exact replicas of the previously defined kilogram are also kept at the United States’ National Institute of Standards and Technology, or NIST, located in Gaithersburg, Maryland outside of Washington D.C., and at other locations around the world. The determination of all other masses could be ultimately traced to a comparison with the standard mass. Even though the platinum-iridium cylinder was resistant to corrosion, airborne contaminants were able to adhere to its surface, slightly changing its mass over time. In May 2019, the scientific community adopted a more stable definition of the kilogram. The kilogram is now defined in terms of the second, the meter, and Planck's constant, #emph[h] (a quantum mechanical value that relates a photon's energy to its frequency). Electric current and its accompanying unit, the ampere, will be introduced in Electric Current, Resistance, and Ohm's Law when electricity and magnetism are covered. The initial modules in this textbook are concerned with mechanics, fluids, heat, and waves. In these subjects all pertinent physical quantities can be expressed in terms of the fundamental units of length, mass, and time. === Metric Prefixes SI units are part of the #strong[metric system]. The metric system is convenient for scientific and engineering calculations because the units are categorized by factors of 10. gives metric prefixes and symbols used to denote various factors of 10. Metric systems have the advantage that conversions of units involve only powers of 10. There are 100 centimeters in a meter, 1000 meters in a kilometer, and so on. In nonmetric systems, such as the system of U.S. customary units, the relationships are not as simple—there are 12 inches in a foot, 5280 feet in a mile, and so on. Another advantage of the metric system is that the same unit can be used over extremely large ranges of values simply by using an appropriate metric prefix. For example, distances in meters are suitable in construction, while distances in kilometers are appropriate for air travel, and the tiny measure of nanometers are convenient in optical design. With the metric system there is no need to invent new units for particular applications. The term #strong[order of magnitude] refers to the scale of a value expressed in the metric system. Each power of #math.equation(block: false, alt: "10")[$"10"$], and so forth are all different orders of magnitude. All quantities that can be expressed as a product of a specific power of #math.equation(block: false, alt: "10")[$"10"$] are said to be of the #emph[same] order of magnitude. For example, the number #math.equation(block: false, alt: "800")[$"800"$] can be written as #math.equation(block: false, alt: "8 times 10 squared")[$8 × "10"^(2)$], and the number #math.equation(block: false, alt: "450")[$"450"$] can be written as #math.equation(block: false, alt: "4. 5 times 10 squared .")[$4. 5 × "10"^(2) .$] Thus, the numbers #math.equation(block: false, alt: "800")[$"800"$] and #math.equation(block: false, alt: "450")[$"450"$] are of the same order of magnitude: #math.equation(block: false, alt: "10 squared .")[$"10"^(2) .$] Order of magnitude can be thought of as a ballpark estimate for the scale of a value. The diameter of an atom is on the order of #math.equation(block: false, alt: "10 to the power minus 10 m,")[$"10"^(− 10) " m,"$] while the diameter of the Sun is on the order of #math.equation(block: false, alt: "10 to the power 9 m.")[$"10"^(9) " m."$] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #emph[The Quest for Microscopic Standards for Basic Units] The fundamental units described in this chapter are those that produce the greatest accuracy and precision in measurement. There is a sense among physicists that, because there is an underlying microscopic substructure to matter, it would be most satisfying to base our standards of measurement on microscopic objects and fundamental physical phenomena such as the speed of light. A microscopic standard has been accomplished for the standard of time, which is based on the oscillations of the cesium atom. The standard for length was once based on the wavelength of light (a small-scale length) emitted by a certain type of atom, but it has been supplanted by the more precise measurement of the speed of light. If it becomes possible to measure the mass of atoms or a particular arrangement of atoms such as a silicon sphere to greater precision than the kilogram standard, it may become possible to base mass measurements on the small scale. There are also possibilities that electrical phenomena on the small scale may someday allow us to base a unit of charge on the charge of electrons and protons, but at present current and charge are related to large-scale currents and forces between wires. ] #figure(table( columns: 7, align: left, inset: 6pt, [Prefix], [Symbol], [Value], [Example (some are approximate)], [], [], [], [exa], [E], [#math.equation(block: false, alt: "10 to the power 18")[$"10"^("18")$]], [exameter], [Em], [#math.equation(block: false, alt: "10 to the power 18 m")[$"10"^("18") " m"$]], [distance light travels in a century], [peta], [P], [#math.equation(block: false, alt: "10 to the power 15")[$"10"^("15")$]], [petasecond], [Ps], [#math.equation(block: false, alt: "10 to the power 15 s")[$"10"^("15") " s"$]], [30 million years], [tera], [T], [#math.equation(block: false, alt: "10 to the power 12")[$"10"^("12")$]], [terawatt], [TW], [#math.equation(block: false, alt: "10 to the power 12 W")[$"10"^("12") " W"$]], [powerful laser output], [giga], [G], [#math.equation(block: false, alt: "10 to the power 9")[$"10"^(9)$]], [gigahertz], [GHz], [#math.equation(block: false, alt: "10 to the power 9 Hz")[$"10"^(9) " Hz"$]], [a microwave frequency], [mega], [M], [#math.equation(block: false, alt: "10 to the power 6")[$"10"^(6)$]], [megacurie], [MCi], [#math.equation(block: false, alt: "10 to the power 6 Ci")[$"10"^(6) " Ci"$]], [high radioactivity], [kilo], [k], [#math.equation(block: false, alt: "10 cubed")[$"10"^(3)$]], [kilometer], [km], [#math.equation(block: false, alt: "10 cubed m")[$"10"^(3) " m"$]], [about 6/10 mile], [hecto], [h], [#math.equation(block: false, alt: "10 squared")[$"10"^(2)$]], [hectoliter], [hL], [#math.equation(block: false, alt: "10 squared L")[$"10"^(2) " L"$]], [26 gallons], [deka], [da], [#math.equation(block: false, alt: "10 to the power 1")[$"10"^(1)$]], [dekagram], [dag], [#math.equation(block: false, alt: "10 to the power 1 g")[$"10"^(1) " g"$]], [teaspoon of butter], [—], [—], [#math.equation(block: false, alt: "10 to the power 0")[$"10"^(0)$] (=1)], [], [], [], [], [deci], [d], [#math.equation(block: false, alt: "10 to the power minus 1")[$"10"^(− 1)$]], [deciliter], [dL], [#math.equation(block: false, alt: "10 to the power minus 1 L")[$"10"^(− 1) " L"$]], [less than half a soda], [centi], [c], [#math.equation(block: false, alt: "10 to the power minus 2")[$"10"^(− 2)$]], [centimeter], [cm], [#math.equation(block: false, alt: "10 to the power minus 2 m")[$"10"^(− 2) " m"$]], [fingertip thickness], [milli], [m], [#math.equation(block: false, alt: "10 to the power minus 3")[$"10"^(− 3)$]], [millimeter], [mm], [#math.equation(block: false, alt: "10 to the power minus 3 m")[$"10"^(− 3) " m"$]], [flea at its shoulders], [micro], [µ], [#math.equation(block: false, alt: "10 to the power minus 6")[$"10"^(− 6)$]], [micrometer], [µm], [#math.equation(block: false, alt: "10 to the power minus 6 m")[$"10"^(− 6) " m"$]], [detail in microscope], [nano], [n], [#math.equation(block: false, alt: "10 to the power minus 9")[$"10"^(− 9)$]], [nanogram], [ng], [#math.equation(block: false, alt: "10 to the power minus 9 g")[$"10"^(− 9) " g"$]], [small speck of dust], [pico], [p], [#math.equation(block: false, alt: "10 to the power minus 12")[$"10"^(− "12")$]], [picofarad], [pF], [#math.equation(block: false, alt: "10 to the power minus 12 F")[$"10"^(− "12") " F"$]], [small capacitor in radio], [femto], [f], [#math.equation(block: false, alt: "10 to the power minus 15")[$"10"^(− "15")$]], [femtometer], [fm], [#math.equation(block: false, alt: "10 to the power minus 15 m")[$"10"^(− "15") " m"$]], [size of a proton], [atto], [a], [#math.equation(block: false, alt: "10 to the power minus 18")[$"10"^(− "18")$]], [attosecond], [as], [#math.equation(block: false, alt: "10 to the power minus 18 s")[$"10"^(− "18") " s"$]], [time light crosses an atom], )) === Known Ranges of Length, Mass, and Time The vastness of the universe and the breadth over which physics applies are illustrated by the wide range of examples of known lengths, masses, and times in . Examination of this table will give you some feeling for the range of possible topics and numerical values. (See and .) #figure(figph[A magnified image of tiny phytoplankton swimming among the crystal of ice.\[], alt: "A magnified image of tiny phytoplankton swimming among the crystal of ice.[", caption: [Tiny phytoplankton swims among crystals of ice in the Antarctic Sea. They range from a few micrometers to as much as 2 millimeters in length.]) #figure(figph[A view of Abell Galaxy with some bright stars and some hot gases.], alt: "A view of Abell Galaxy with some bright stars and some hot gases.", caption: [Galaxies collide 2.4 billion light years away from Earth. The tremendous range of observable phenomena in nature challenges the imagination.]) === Unit Conversion and Dimensional Analysis It is often necessary to convert from one type of unit to another. For example, if you are reading a European cookbook, some quantities may be expressed in units of liters and you need to convert them to cups. Or, perhaps you are reading walking directions from one location to another and you are interested in how many miles you will be walking. In this case, you will need to convert units of feet to miles. Let us consider a simple example of how to convert units. Let us say that we want to convert 80 meters (m) to kilometers (km). The first thing to do is to list the units that you have and the units that you want to convert to. In this case, we have units in #emph[meters] and we want to convert to #emph[kilometers]. Next, we need to determine a #strong[conversion factor] relating meters to kilometers. A conversion factor is a ratio expressing how many of one unit are equal to another unit. For example, there are 12 inches in 1 foot, 100 centimeters in 1 meter, 60 seconds in 1 minute, and so on. In this case, we know that there are 1,000 meters in 1 kilometer. Now we can set up our unit conversion. We will write the units that we have and then multiply them by the conversion factor so that the units cancel out, as shown: #math.equation(block: true, alt: "80 m times the fraction 1 km over 1000 m equals 0 .080 km.")[$80 cancel("m") × frac("1 km", 1000 cancel("m")) = 0 ".080 km."$] Note that the unwanted m unit cancels, leaving only the desired km unit. You can use this method to convert between any types of unit. Click Appendix C for a more complete list of conversion factors. #figure(table( columns: 6, align: left, inset: 6pt, [Lengths in meters], [Masses in kilograms (more precise values in parentheses)], [Times in seconds (more precise values in parentheses)], [], [], [], [#math.equation(block: false, alt: "10 to the power minus 18")[$"10"^(− "18")$]], [Present experimental limit to smallest observable detail], [#math.equation(block: false, alt: "10 to the power minus 30")[$"10"^(− "30")$]], [Mass of an electron #math.equation(block: false, alt: "9 . 11 times 10 to the power minus 31 kg")[$9 "." "11" × "10"^(− "31") #h(0.25em) " kg"$]], [#math.equation(block: false, alt: "10 to the power minus 23")[$"10"^(− "23")$]], [Time for light to cross a proton], [#math.equation(block: false, alt: "10 to the power minus 15")[$"10"^(− "15")$]], [Diameter of a proton], [#math.equation(block: false, alt: "10 to the power minus 27")[$"10"^(− "27")$]], [Mass of a hydrogen atom #math.equation(block: false, alt: "1 . 67 times 10 to the power minus 27 kg")[$1 "." "67" × "10"^(− "27") #h(0.25em) " kg"$]], [#math.equation(block: false, alt: "10 to the power minus 22")[$"10"^(− "22")$]], [Mean life of an extremely unstable nucleus], [#math.equation(block: false, alt: "10 to the power minus 14")[$"10"^(− "14")$]], [Diameter of a uranium nucleus], [#math.equation(block: false, alt: "10 to the power minus 15")[$"10"^(− "15")$]], [Mass of a bacterium], [#math.equation(block: false, alt: "10 to the power minus 15")[$"10"^(− "15")$]], [Time for one oscillation of visible light], [#math.equation(block: false, alt: "10 to the power minus 10")[$"10"^(− "10")$]], [Diameter of a hydrogen atom], [#math.equation(block: false, alt: "10 to the power minus 5")[$"10"^(− 5)$]], [Mass of a mosquito], [#math.equation(block: false, alt: "10 to the power minus 13")[$"10"^(− "13")$]], [Time for one vibration of an atom in a solid], [#math.equation(block: false, alt: "10 to the power minus 8")[$"10"^(− 8)$]], [Thickness of membranes in cells of living organisms], [#math.equation(block: false, alt: "10 to the power minus 2")[$"10"^(− 2)$]], [Mass of a hummingbird], [#math.equation(block: false, alt: "10 to the power minus 8")[$"10"^(− 8)$]], [Time for one oscillation of an FM radio wave], [#math.equation(block: false, alt: "10 to the power minus 6")[$"10"^(− 6)$]], [Wavelength of visible light], [#math.equation(block: false, alt: "1")[$"1"$]], [Mass of a liter of water (about a quart)], [#math.equation(block: false, alt: "10 to the power minus 3")[$"10"^(− 3)$]], [Duration of a nerve impulse], [#math.equation(block: false, alt: "10 to the power minus 3")[$"10"^(− 3)$]], [Size of a grain of sand], [#math.equation(block: false, alt: "10 squared")[$"10"^(2)$]], [Mass of a person], [#math.equation(block: false, alt: "1")[$"1"$]], [Time for one heartbeat], [#math.equation(block: false, alt: "1")[$"1"$]], [Height of a 4-year-old child], [#math.equation(block: false, alt: "10 cubed")[$"10"^(3)$]], [Mass of a car], [#math.equation(block: false, alt: "10 to the power 5")[$"10"^(5)$]], [One day #math.equation(block: false, alt: "8 . 64 times 10 to the power 4 s")[$8 "." "64" × "10"^(4) #h(0.25em) "s"$]], [#math.equation(block: false, alt: "10 squared")[$"10"^(2)$]], [Length of a football field], [#math.equation(block: false, alt: "10 to the power 8")[$"10"^(8)$]], [Mass of a large ship], [#math.equation(block: false, alt: "10 to the power 7")[$"10"^(7)$]], [One year (y) #math.equation(block: false, alt: "3 . 16 times 10 to the power 7 s")[$3 "." "16" × "10"^(7) #h(0.25em) "s"$]], [#math.equation(block: false, alt: "10 to the power 4")[$"10"^(4)$]], [Greatest ocean depth], [#math.equation(block: false, alt: "10 to the power 12")[$"10"^("12")$]], [Mass of a large iceberg], [#math.equation(block: false, alt: "10 to the power 9")[$"10"^(9)$]], [About half the life expectancy of a human], [#math.equation(block: false, alt: "10 to the power 7")[$"10"^(7)$]], [Diameter of the Earth], [#math.equation(block: false, alt: "10 to the power 15")[$"10"^("15")$]], [Mass of the nucleus of a comet], [#math.equation(block: false, alt: "10 to the power 11")[$"10"^("11")$]], [Recorded history], [#math.equation(block: false, alt: "10 to the power 11")[$"10"^("11")$]], [Distance from the Earth to the Sun], [#math.equation(block: false, alt: "10 to the power 23")[$"10"^("23")$]], [Mass of the Moon #math.equation(block: false, alt: "7 . 35 times 10 to the power 22 kg")[$7 "." "35" × "10"^("22") #h(0.25em) " kg"$]], [#math.equation(block: false, alt: "10 to the power 17")[$"10"^("17")$]], [Age of the Earth], [#math.equation(block: false, alt: "10 to the power 16")[$"10"^("16")$]], [Distance traveled by light in 1 year (a light year)], [#math.equation(block: false, alt: "10 to the power 25")[$"10"^("25")$]], [Mass of the Earth #math.equation(block: false, alt: "5 . 97 times 10 to the power 24 kg")[$5 "." "97" × "10"^("24") #h(0.25em) " kg"$]], [#math.equation(block: false, alt: "10 to the power 18")[$"10"^("18")$]], [Age of the universe], [#math.equation(block: false, alt: "10 to the power 21")[$"10"^("21")$]], [Diameter of the Milky Way galaxy], [#math.equation(block: false, alt: "10 to the power 30")[$"10"^("30")$]], [Mass of the Sun #math.equation(block: false, alt: "1 . 99 times 10 to the power 30 kg")[$1 "." "99" × "10"^("30") #h(0.25em) " kg"$]], [], [], [#math.equation(block: false, alt: "10 to the power 22")[$"10"^("22")$]], [Distance from the Earth to the nearest large galaxy (Andromeda)], [#math.equation(block: false, alt: "10 to the power 42")[$"10"^("42")$]], [Mass of the Milky Way galaxy (current upper limit)], [], [], [#math.equation(block: false, alt: "10 to the power 26")[$"10"^("26")$]], [Distance from the Earth to the edges of the known universe], [#math.equation(block: false, alt: "10 to the power 53")[$"10"^("53")$]], [Mass of the known universe (current upper limit)], [], [], )) #examplebox("Example 1")[Unit Conversions: A Short Drive Home][ Suppose that you drive the 10.0 km from your school to home in 20.0 min. Calculate your average speed (a) in kilometers per hour (km/h) and (b) in meters per second (m/s). (Note: Average speed is distance traveled divided by time of travel.) Strategy First we calculate the average speed using the given units. Then we can get the average speed into the desired units by picking the correct conversion factor and multiplying by it. The correct conversion factor is the one that cancels the unwanted unit and leaves the desired unit in its place. Solution for (a) (1) Calculate average speed. Average speed is distance traveled divided by time of travel. (Take this definition as a given for now—average speed and other motion concepts will be covered in a later module.) In equation form, #math.equation(block: true, alt: "average speed = the fraction distance over time .")[$"average speed = " frac("distance", "time") "."$] (2) Substitute the given values for distance and time. #math.equation(block: true, alt: "average speed = the fraction 10 . 0 km over 20 . 0 min equals 0 . 500 the fraction km over min .")[$"average speed = " frac("10" "." 0 " km", "20" "." 0 " min") = 0 "." "500" frac(" km", " min") "."$] (3) Convert km/min to km/h: multiply by the conversion factor that will cancel minutes and leave hours. That conversion factor is #math.equation(block: false, alt: "60 min/hr")[$"60 min/hr"$] Discussion for (a) To check your answer, consider the following: (1) Be sure that you have properly cancelled the units in the unit conversion. If you have written the unit conversion factor upside down, the units will not cancel properly in the equation. If you accidentally get the ratio upside down, then the units will not cancel; rather, they will give you the wrong units as follows: #math.equation(block: true, alt: "the fraction km over min times the fraction 1 hr over 60 min equals the fraction 1 over 60 the fraction km times hr over min squared ,")[$frac(" km", "min") × frac(1 " hr", "60" " min") = frac(1, "60") frac(" km" ⋅ "hr", attach(" min", t: 2)) ","$] which are obviously not the desired units of km/h. (2) Check that the units of the final answer are the desired units. The problem asked us to solve for average speed in units of km/h and we have indeed obtained these units. (3) Check the significant figures. Because each of the values given in the problem has three significant figures, the answer should also have three significant figures. The answer 30.0 km/hr does indeed have three significant figures, so this is appropriate. Note that the significant figures in the conversion factor are not relevant because an hour is #emph[defined] to be 60 minutes, so the precision of the conversion factor is perfect. (4) Next, check whether the answer is reasonable. Let us consider some information from the problem—if you travel 10 km in a third of an hour (20 min), you would travel three times that far in an hour. The answer does seem reasonable. Solution for (b) There are several ways to convert the average speed into meters per second. (1) Start with the answer to (a) and convert km/h to m/s. Two conversion factors are needed—one to convert hours to seconds, and another to convert kilometers to meters. (2) Multiplying by these yields #math.equation(block: true, alt: "Average speed equals 30 . 0 the fraction km over h times the fraction 1 h over 3,600 s times the fraction 1, 000 m over 1 km ,")[$"Average speed" = "30" "." 0 frac("km", "h") × frac(1 #h(0.25em) "h", "3,600 s") × frac(1"," "000" #h(0.25em) "m", "1 km") ","$] #math.equation(block: true, alt: "Average speed equals 8 . 33 the fraction m over s .")[$"Average speed" = 8 "." "33" frac("m", "s") "."$] Discussion for (b) If we had started with 0.500 km/min, we would have needed different conversion factors, but the answer would have been the same: 8.33 m/s. You may have noted that the answers in the worked example just covered were given to three digits. Why? When do you need to be concerned about the number of digits in something you calculate? Why not write down all the digits your calculator produces? The module Accuracy, Precision, and Significant Figures will help you answer these questions. ] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #emph[Nonstandard Units] While there are numerous types of units that we are all familiar with, there are others that are much more obscure. For example, a #emph[firkin] is a unit of volume that was once used to measure beer. One firkin equals about 34 liters. To learn more about nonstandard units, use a dictionary or encyclopedia to research different “weights and measures.” Take note of any unusual units, such as a barleycorn, that are not listed in the text. Think about how the unit is defined and state its relationship to SI units. ] Some hummingbirds beat their wings more than 50 times per second. A scientist is measuring the time it takes for a hummingbird to beat its wings once. Which fundamental unit should the scientist use to describe the measurement? Which factor of 10 is the scientist likely to use to describe the motion precisely? Identify the metric prefix that corresponds to this factor of 10. #solutionbox[ The scientist will measure the time between each movement using the fundamental unit of seconds. Because the wings beat so fast, the scientist will probably need to measure in milliseconds, or #math.equation(block: false, alt: "10 to the power minus 3")[$"10"^(− 3)$] seconds. (50 beats per second corresponds to 20 milliseconds per beat.) ] One cubic centimeter is equal to one milliliter. What does this tell you about the different units in the SI metric system? #solutionbox[ The fundamental unit of length (meter) is probably used to create the derived unit of volume (liter). The measure of a milliliter is dependent on the measure of a centimeter. ] === Summary - Physical quantities are a characteristic or property of an object that can be measured or calculated from other measurements. - Units are standards for expressing and comparing the measurement of physical quantities. All units can be expressed as combinations of four fundamental units. - The four fundamental units we will use in this text are the meter (for length), the kilogram (for mass), the second (for time), and the ampere (for electric current). These units are part of the metric system, which uses powers of 10 to relate quantities over the vast ranges encountered in nature. - The four fundamental units are abbreviated as follows: meter, m; kilogram, kg; second, s; and ampere, A. The metric system also uses a standard set of prefixes to denote each order of magnitude greater than or lesser than the fundamental unit itself. - Unit conversions involve changing a value expressed in one type of unit to another type of unit. This is done by using conversion factors, which are ratios relating equal quantities of different units. === Conceptual Questions Identify some advantages of metric units. === Problems & Exercises The speed limit on some interstate highways is roughly 100 km/h. (a) What is this in meters per second? (b) How many miles per hour is this? #solutionbox[ (a) #math.equation(block: false, alt: "27 . 8 m/s")[$"27" "." "8 m/s"$] (b) #math.equation(block: false, alt: "62 . 1 mph")[$"62" "." "1 mph"$] ] A car is traveling at a speed of #math.equation(block: false, alt: "33 m/s")[$"33 m/s"$]. (a) What is its speed in kilometers per hour? (b) Is it exceeding the #math.equation(block: false, alt: "90 km/h")[$"90 km/h"$] speed limit? Show that #math.equation(block: false, alt: "1 . 0 m/s equals 3 . 6 km/h")[$1 "." "0 m/s" = 3 "." "6 km/h"$]. Hint: Show the explicit steps involved in converting #math.equation(block: false, alt: "1 . 0 m/s equals 3 . 6 km/h.")[$1 "." "0 m/s" = 3 "." "6 km/h."$] #solutionbox[ #math.equation(block: true, alt: "the fraction 1.0 m over s equals the fraction 1 . 0 m over s times the fraction 3600 s over 1 hr times the fraction 1 km over 1000 m")[$frac("1.0 m", s) = frac(1 "." "0 m", s) × frac("3600 s", "1 hr") × frac(1 "km", "1000 m")$] #math.equation(block: true, alt: "equals 3 . 6 km/h")[$= 3 "." "6 km/h"$]. ] American football is played on a 100-yd-long field, excluding the end zones. How long is the field in meters? (Assume that 1 meter equals 3.281 feet.) Soccer fields vary in size. A large soccer field is 115 m long and 85 m wide. What are its dimensions in feet and inches? (Assume that 1 meter equals 3.281 feet.) #solutionbox[ length: #math.equation(block: false, alt: "377 ft")[$"377 ft"$]; #math.equation(block: false, alt: "4 . 53 times 10 cubed in .")[$4 "." "53" × "10"^(3) " in" "."$] width: #math.equation(block: false, alt: "280 ft")[$"280 ft"$]; #math.equation(block: false, alt: "3 . 3 times 10 cubed in")[$3 "." 3 × "10"^(3) " in"$]. ] What is the height in meters of a person who is 6 ft 1.0 in. tall? (Assume that 1 meter equals 39.37 in.) Mount Everest, at 29,028 feet, is the tallest mountain on the Earth. What is its height in kilometers? (Assume that 1 kilometer equals 3,281 feet.) #solutionbox[ #math.equation(block: true, alt: "8 . 847 km")[$8 "." "847 km"$] ] The speed of sound is measured to be #math.equation(block: false, alt: "342 m/s")[$"342 m/s"$] on a certain day. What is this in km/h? Tectonic plates are large segments of the Earth’s crust that move slowly. Suppose that one such plate has an average speed of 4.0 cm/year. (a) What distance does it move in 1 s at this speed? (b) What is its speed in kilometers per million years? #solutionbox[ (a) #math.equation(block: false, alt: "1 . 3 times 10 to the power minus 9 m")[$1 "." 3 × "10"^(− 9) " m"$] (b) #math.equation(block: false, alt: "40 km/My")[$"40 km/My"$] ] (a) Refer to to determine the average distance between the Earth and the Sun. Then calculate the average speed of the Earth in its orbit in kilometers per second. (b) What is this in meters per second?