(* Content-type: application/mathematica *) (*** Wolfram Notebook File ***) (* http://www.wolfram.com/nb *) (* CreatedBy='Mathematica 6.0' *) (*CacheID: 234*) (* Internal cache information: NotebookFileLineBreakTest NotebookFileLineBreakTest NotebookDataPosition[ 145, 7] NotebookDataLength[ 61281, 1477] NotebookOptionsPosition[ 57682, 1356] NotebookOutlinePosition[ 58110, 1374] CellTagsIndexPosition[ 58067, 1371] WindowFrame->Normal ContainsDynamic->False*) (* Beginning of Notebook Content *) Notebook[{ Cell[CellGroupData[{ Cell["A little jaunt brought on by a seemingly reasonable claim", "Subtitle", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.4007910117256775`*^9, 3.4007910595147614`*^9}}], Cell[TextData[{ " ... the premise behind astrology is ridiculous ... the doctor or \ midwife or taxi driver who helped deliver you exerted a greater gravitational \ pull on you at your moment of birth than did the sun, the moon, or any of the \ planets.\n\nfrom ", StyleBox["The Canon: A Whirligig Tour of the Beautiful Basics of Science", FontSlant->"Italic"], " by Natalie Angier\n\nLet us calculate.\n\nThe gravitational force between \ two objects varies with their masses and inversely with the square of the \ distance between them" }], "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}}], Cell[BoxData[ RowBox[{ RowBox[{"F", "[", RowBox[{"m1_", ",", "m2_", ",", "r_"}], "]"}], ":=", RowBox[{"G", " ", FractionBox[ RowBox[{"m1", " ", "m2"}], SuperscriptBox["r", "2"]]}]}]], "Input", CellChangeTimes->{{3.400768529119486*^9, 3.400768529306892*^9}, { 3.400768711840892*^9, 3.400768763549487*^9}, {3.400769164521467*^9, 3.4007691658645463`*^9}}], Cell["We'll need the gravitational constant", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}}], Cell[BoxData[ RowBox[{"<<", "PhysicalConstants`"}]], "Input", CellChangeTimes->{{3.4007688769929357`*^9, 3.400768883099265*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{"G", "=", "GravitationalConstant"}]], "Input", CellChangeTimes->{{3.4007690776741347`*^9, 3.400769078298823*^9}, { 3.400769109330231*^9, 3.4007691202622776`*^9}}], Cell[BoxData[ FractionBox[ RowBox[{"6.673`*^-11", " ", SuperscriptBox["Meter", "2"], " ", "Newton"}], SuperscriptBox["Kilogram", "2"]]], "Output", CellChangeTimes->{3.4007691235731306`*^9, 3.400790813385351*^9}] }, Open ]], Cell["\<\ While the quote addresses a person and a baby, we'll consider two adults, \ each weighing, say, 100 kg. If they're 1/2 meter apart, the force between \ them is\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ SubscriptBox["F", "twopeople"], "=", RowBox[{"F", "[", RowBox[{ RowBox[{"100", "Kilogram"}], ",", RowBox[{"100", "Kilogram"}], ",", RowBox[{ FractionBox["1", "2"], "Meter"}]}], "]"}]}]], "Input", CellChangeTimes->{{3.400769285539259*^9, 3.4007693057635517`*^9}, { 3.4007711943333464`*^9, 3.400771227646922*^9}}], Cell[BoxData[ RowBox[{"2.6691999999999998`*^-6", " ", "Newton"}]], "Output", CellChangeTimes->{ 3.4007693072471857`*^9, {3.4007712033606606`*^9, 3.4007712282716503`*^9}, 3.4007908134478207`*^9}] }, Open ]], Cell["\<\ which is actually pretty large. For instance, this is equivalent to an \ amount of, say, salt, of mass\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.4007720827967205`*^9, 3.4007720834994946`*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ RowBox[{ SubscriptBox["m", "salt"], ":=", RowBox[{"Convert", "[", RowBox[{ FractionBox[ SubscriptBox["F", "twopeople"], "AccelerationDueToGravity"], ",", "Kilogram"}], "]"}]}], ";", SubscriptBox["m", "salt"]}]], "Input", CellChangeTimes->{{3.4007694676017585`*^9, 3.400769506894672*^9}, { 3.400769790409582*^9, 3.400769794813634*^9}, 3.400769837979613*^9, { 3.400770290878829*^9, 3.4007702931589403`*^9}, {3.400771208951972*^9, 3.4007712120756083`*^9}}], Cell[BoxData[ RowBox[{"2.721826515680686`*^-7", " ", "Kilogram"}]], "Output", CellChangeTimes->{ 3.400770294626963*^9, {3.4007712192131133`*^9, 3.4007712302083025`*^9}, 3.4007908146659765`*^9}] }, Open ]], Cell[TextData[{ "The density of salt is about ", Cell[BoxData[ FormBox[ RowBox[{"\[Rho]", " ", "=", RowBox[{"2150", " ", RowBox[{ StyleBox["kg", FontSlant->"Italic"], "/", SuperscriptBox["m", "3"]}]}]}], TraditionalForm]]], " so from ", Cell[BoxData[ FormBox[ RowBox[{"m", "=", RowBox[{"\[Rho]", " ", "V"}]}], TraditionalForm]]], ", the equivalent volume is" }], "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ RowBox[{ SubscriptBox["V", "salt"], ":=", FractionBox[ SubscriptBox["m", "salt"], RowBox[{"2150", FractionBox["Kilogram", SuperscriptBox["Meter", "3"]]}]]}], ";", SubscriptBox["V", "salt"]}]], "Input", CellChangeTimes->{{3.4007698058550067`*^9, 3.4007698859244614`*^9}}], Cell[BoxData[ RowBox[{"1.2659658212468307`*^-10", " ", SuperscriptBox["Meter", "3"]}]], "Output", CellChangeTimes->{3.4007698869395795`*^9, 3.400771234050371*^9, 3.400790818226727*^9}] }, Open ]], Cell[TextData[{ "or, since there are 1,000 millimeters per meter, 0.126 ", Cell[BoxData[ FormBox[ SuperscriptBox["mm", "3"], TraditionalForm]]], ", which is a cube about 1/2 mm on a side.\n\nWhich means that the person \ sitting across the table from you is exerting a gravitation force on you \ equivalent to the weight of a grain or two of salt in the palm of your hand.\n\ \nSo, back to the planets. First, the Earth is clearly a planet and also \ clearly exerts quite a bit of force on you, far more than any taxi driver or \ midwife. But ignoring that, what about the other celestial bodies?\n\nLet's \ consider Jupiter. Jupiter is pretty big, but it's also pretty far away, so \ just knowing the form of the force law won't let us figure out if the force \ between you and Jupiter is large (we've got two competing effects, ", Cell[BoxData[ FormBox[ RowBox[{"F", "~", " ", SubscriptBox["m", "jup"]}], TraditionalForm]]], " and ", Cell[BoxData[ FormBox[ RowBox[{"F", "~", " ", SuperscriptBox[ SubscriptBox["r", "jup"], RowBox[{"-", "2"}]]}], TraditionalForm]]], ", one is big for Jupiter and one little). We'll need the actual numbers. \ Jupiter's mass is easy to get" }], "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007699010106897`*^9, 3.400769907038935*^9}, { 3.4007700336945424`*^9, 3.4007700561989517`*^9}, {3.400770099411784*^9, 3.400770229940457*^9}, {3.4007703343261795`*^9, 3.4007705736111073`*^9}, { 3.4007706218874073`*^9, 3.4007706419256926`*^9}, 3.400772157103524*^9, 3.400791329871116*^9}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ SubscriptBox["m", "jup"], "=", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], " ", "Kilogram"}]}]], "Input", CellChangeTimes->{{3.4007705768284965`*^9, 3.400770633616757*^9}, { 3.4007706944030733`*^9, 3.4007706958087177`*^9}}], Cell[BoxData[ RowBox[{"1.8988`5.000000000000002*^27", " ", "Kilogram"}]], "Output", CellChangeTimes->{{3.4007706739275446`*^9, 3.4007706968863745`*^9}, 3.4007908541310124`*^9}] }, Open ]], Cell["\<\ But how far away is it? This value is changing all the time, of course, but \ we can get a good idea of what it is by calculating the maximum, so whatever \ result we get, we'll know that the real answer is at least that but almost \ always more. The maximum occurs (approximately, since Jupiter and Earth move around the \ Sun in ellipses and not circles) when Jupiter is directly opposed to Earth, \ i.e. directly opposit with the Sun in the middle. We can estimate how far \ this is by taking the sum of the maximum distance of both Jupiter and the \ Earth from the Sun\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ SubscriptBox["r", "jup"], "=", RowBox[{ RowBox[{"(", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "+", RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}]}], ")"}], "Meter"}]}]], "Input", CellChangeTimes->{{3.4007709054564595`*^9, 3.400770970132537*^9}}], Cell[BoxData[ RowBox[{"9.68179156030210085443`8.848969037225423*^11", " ", "Meter"}]], "Output", CellChangeTimes->{{3.4007709419568624`*^9, 3.400770971272684*^9}, 3.4007908590348597`*^9}] }, Open ]], Cell["So what's the force between you and Jupiter?", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ SubscriptBox["F", "jup"], "=", RowBox[{"F", "[", RowBox[{ RowBox[{"100", "Kilogram"}], ",", SubscriptBox["m", "jup"], ",", SubscriptBox["r", "jup"]}], "]"}]}]], "Input", CellChangeTimes->{{3.4007711538040853`*^9, 3.4007711727021327`*^9}, { 3.4007712579929914`*^9, 3.4007712621005583`*^9}}], Cell[BoxData[ RowBox[{"0.000013517266959176376`", " ", "Newton"}]], "Output", CellChangeTimes->{3.4007711733893337`*^9, 3.400771262459775*^9, 3.400790862330122*^9}] }, Open ]], Cell["Comparing to the force between you and a taxi driver", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}}], Cell[CellGroupData[{ Cell[BoxData[ FractionBox[ SubscriptBox["F", "jup"], SubscriptBox["F", "twopeople"]]], "Input", CellChangeTimes->{{3.4007712639435005`*^9, 3.400771272470996*^9}}], Cell[BoxData["5.064164153745084`"], "Output", CellChangeTimes->{3.400771276313055*^9, 3.4007908654535894`*^9}] }, Open ]], Cell["\<\ Oops! Jupiter's force is five times as large. And since we took the largest \ distance, this is the lower limit. This raises the issue of what forces the other heavenly bodies exert on you. \ First, though, let's simplify the math we have to do. We're eventually going to be taking a ratio of two forces and some things are \ common to both numerator and denominator. Specifically, G appears in both as \ does the mass of the person, so these both cancel, leaving\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}}], Cell[BoxData[ RowBox[{ RowBox[{"Fratio", "[", RowBox[{"m2_", ",", "m3_", ",", "r12_", ",", "r13_"}], "]"}], ":=", RowBox[{ FractionBox["m2", "m3"], FractionBox[ SuperscriptBox["r13", "2"], SuperscriptBox["r12", "2"]]}]}]], "Input", CellChangeTimes->{{3.4007716602809334`*^9, 3.4007716864408073`*^9}, { 3.400771817083639*^9, 3.4007718823970337`*^9}}], Cell["\<\ Just to check, we can calculate the answer for Jupiter and a taxi driver \ again\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{"Fratio", "[", RowBox[{ SubscriptBox["m", "jup"], ",", RowBox[{"100", "Kilogram"}], ",", SubscriptBox["r", "jup"], ",", RowBox[{ FractionBox["1", "2"], "Meter"}]}], "]"}]], "Input", CellChangeTimes->{{3.400771968119361*^9, 3.4007720316971264`*^9}}], Cell[BoxData["5.0641641537450828382`4.999877034356897"], "Output", CellChangeTimes->{3.4007720002283955`*^9, 3.400772032477987*^9, 3.4007908734340553`*^9}] }, Open ]], Cell[TextData[{ "Now we need the masses and greatest distances to the varous planets. \n\n\ ", StyleBox["Mathematica", FontSlant->"Italic"], " reports the distance between the Moon and Earth in kilometers and all \ other Apoapses is meters, so we have to fix that below. We can also use the \ radius of the Earth for ", Cell[BoxData[ FormBox[ SubscriptBox["r", "earth"], TraditionalForm]]], " to get the relative force between it and a taxi driver." }], "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773329273526*^9}}], Cell[CellGroupData[{ Cell[BoxData[{ RowBox[{"celestialbodynames", "=", RowBox[{"Append", "[", RowBox[{ RowBox[{"AstronomicalData", "[", "\"\\"", "]"}], ",", "\"\\""}], "]"}]}], "\n", RowBox[{ RowBox[{"celestialbodies", "=", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{ RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "#", "]"}], ",", "\"\\""}], "]"}], "Kilogram"}], ",", RowBox[{ RowBox[{"Abs", "[", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "#", "]"}], ",", "\"\\""}], "]"}], "+", RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "\"\\"", "]"}], ",", "\"\\""}], "]"}]}], "]"}], "Meter"}]}], "}"}], "&"}], "/@", "celestialbodynames"}]}], ";"}], "\n", RowBox[{ RowBox[{ RowBox[{"celestialbodies", "[", RowBox[{"[", RowBox[{"3", ",", "2"}], "]"}], "]"}], "=", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}]}], ";"}], "\n", RowBox[{ RowBox[{ RowBox[{"celestialbodies", "[", RowBox[{"[", RowBox[{"10", ",", "2"}], "]"}], "]"}], "=", RowBox[{"1000", " ", RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}]}], ";"}], "\n", "celestialbodies", "\n"}], "Input", CellChangeTimes->{{3.4007726854033628`*^9, 3.4007726888860044`*^9}, { 3.400773032717845*^9, 3.4007730399330063`*^9}, {3.400773093047223*^9, 3.4007731026674433`*^9}, 3.4007743239218554`*^9}], Cell[BoxData[ RowBox[{"{", RowBox[{"\<\"Mercury\"\>", ",", "\<\"Venus\"\>", ",", "\<\"Earth\"\>", ",", "\<\"Mars\"\>", ",", "\<\"Jupiter\"\>", ",", "\<\"Saturn\"\>", ",", "\<\"Uranus\"\>", ",", "\<\"Neptune\"\>", ",", "\<\"Pluto\"\>", ",", "\<\"Moon\"\>"}], "}"}]], "Output", CellChangeTimes->{3.400772694679999*^9, 3.400773040838808*^9, 3.4007731047289147`*^9, 3.400774327404647*^9, 3.4007746846303744`*^9, 3.4007908813832865`*^9}], Cell[BoxData[ RowBox[{"{", RowBox[{ RowBox[{"{", RowBox[{ RowBox[{"3.30220000000000000000001`5.*^23", " ", "Kilogram"}], ",", RowBox[{"2.21914780178620896673`8.348551928624502*^11", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"4.869`5.000000000000003*^24", " ", "Kilogram"}], ",", RowBox[{"2.61039550199716744983`8.115741615399871*^11", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"5.9742`5.000000000000002*^24", " ", "Kilogram"}], ",", RowBox[{"6.37814`6.999999999999997*^6", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{ "6.4191000000000000000007`4.999999999999999*^23", " ", "Kilogram"}], ",", RowBox[{"4.01326430356498158743`8.797557519396388*^11", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"1.8988`5.000000000000002*^27", " ", "Kilogram"}], ",", RowBox[{"9.68179156030210085443`8.848969037225423*^11", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"5.685`5.000000000000002*^26", " ", "Kilogram"}], ",", RowBox[{ "1.656081150377106281648`7.321780242078527*^12", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"8.6625`5.*^25", " ", "Kilogram"}], ",", RowBox[{"3.15848710563095667999`9.235827628936157*^12", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"1.0278`5.000000000000002*^26", " ", "Kilogram"}], ",", RowBox[{ "4.688972025962583092653`8.077161784380886*^12", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{"1.314`3.999999999999989*^22", " ", "Kilogram"}], ",", RowBox[{ "7.528025632169552136949`8.683063088349025*^12", " ", "Meter"}]}], "}"}], ",", RowBox[{"{", RowBox[{ RowBox[{ "7.3459006322855173653772`4.995678626217362*^22", " ", "Kilogram"}], ",", RowBox[{"4.05695760000000009`3.8167530928501696*^8", " ", "Meter"}]}], "}"}]}], "}"}]], "Output", CellChangeTimes->{3.400772694679999*^9, 3.400773040838808*^9, 3.4007731047289147`*^9, 3.400774327404647*^9, 3.4007746846303744`*^9, 3.4007908816800165`*^9}] }, Open ]], Cell["\<\ So now all we need to do is calculate the forces.\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{"ratios", "=", RowBox[{ RowBox[{ RowBox[{"(", RowBox[{"Fratio", "[", RowBox[{ RowBox[{"#", "[", RowBox[{"[", "1", "]"}], "]"}], ",", RowBox[{"100", "Kilogram"}], ",", RowBox[{"#", "[", RowBox[{"[", "2", "]"}], "]"}], ",", RowBox[{ FractionBox["1", "2"], "Meter"}]}], "]"}], ")"}], "&"}], "/@", "celestialbodies"}]}]], "Input", CellChangeTimes->{{3.4007730756808577`*^9, 3.4007730780390615`*^9}, { 3.400773671723419*^9, 3.4007736732227945`*^9}}], Cell[BoxData[ RowBox[{"{", RowBox[{ "0.0167637403207344577`4.999610894104642", ",", "0.178635248445922335`4.999335124681317", ",", "3.67139972167283694`4.991399828238082*^8", ",", "0.0099636537222891634`4.9998615835911355", ",", "5.0641641537450828382`4.999877034356897", ",", "0.5182117423948026849`4.995879289724357", ",", "0.0217082612650648087`4.999949538350009", ",", "0.0116867388227661726`4.999273410400315", ",", "5.7965981727893167516484`3.9999819805218655*^-7", ",", "1115.7942533964774180272`3.501573798148235"}], "}"}]], "Output", CellChangeTimes->{3.4007730789917135`*^9, 3.400773108992422*^9, 3.4007736738162975`*^9, 3.4007743349324684`*^9, 3.4007746878163853`*^9, 3.4007908867556524`*^9}] }, Open ]], Cell[TextData[{ "For the curious, this line uses what ", StyleBox["Mathematica", FontSlant->"Italic"], " calles a Pure Function (the ", Cell[BoxData[ FormBox[ RowBox[{ RowBox[{"(", "#", ")"}], "&"}], TraditionalForm]]], " bit) which is applied to each pair of masses and distances in turn (the ", Cell[BoxData[ FormBox["/@", TraditionalForm]]], " bit).\n\nSo, our answer in a more convenient form:" }], "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.400790918880539*^9, 3.4007909363095026`*^9}, {3.4007914793083916`*^9, 3.40079152368011*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", "ratios"}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]], "Input", CellChangeTimes->{{3.400773631693216*^9, 3.4007736789391527`*^9}}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "0.0167637403207344577`4.999610894104642"}, {"\<\"Venus\"\>", "0.178635248445922335`4.999335124681317"}, {"\<\"Earth\"\>", "3.67139972167283694`4.991399828238082*^8"}, {"\<\"Mars\"\>", "0.0099636537222891634`4.9998615835911355"}, {"\<\"Jupiter\"\>", "5.0641641537450828382`4.999877034356897"}, {"\<\"Saturn\"\>", "0.5182117423948026849`4.995879289724357"}, {"\<\"Uranus\"\>", "0.0217082612650648087`4.999949538350009"}, {"\<\"Neptune\"\>", "0.0116867388227661726`4.999273410400315"}, {"\<\"Pluto\"\>", "5.7965981727893167516484`3.9999819805218655*^-7"}, {"\<\"Moon\"\>", "1115.7942533964774180272`3.501573798148235"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{{3.400773650138677*^9, 3.4007736798450255`*^9}, 3.4007743412733297`*^9, 3.400790941962982*^9}] }, Open ]], Cell["\<\ Looks like the Earth, the Moon, and Jupiter all exert more force than your \ average taxi driver. But the taxi driver clearly 'out gravity's everything \ else. Though, we seem to be missing a rather large heavenly body\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.400774262808962*^9, 3.4007742711020794`*^9}, {3.40077435673503*^9, 3.400774385331337*^9}, { 3.400791549544034*^9, 3.400791554791783*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{"Fratio", "[", RowBox[{ RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Kilogram"}], ",", RowBox[{"100", "Kilogram"}], ",", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}], ",", RowBox[{ FractionBox["1", "2"], "Meter"}]}], "]"}]], "Input", CellChangeTimes->{{3.4007738577069364`*^9, 3.400773905217642*^9}}], Cell[BoxData["214885.0044637084505919394`6.989994005991709"], "Output", CellChangeTimes->{{3.400773890942576*^9, 3.4007739059985514`*^9}, 3.4007909465544844`*^9}] }, Open ]], Cell[TextData[{ "Bigger than anything but the Earth itself.\n\nWhich raises another issue, \ why does the Moon contribute more to the ocean tides than the Sun? The Sun's \ gravitational force on the water in the ocean is ~100 times larger than the \ Moon's.\n\nI leave that as an exercise for the reader. A hint: considering \ just the Earth and the Moon, do two identical rocks on opposit sides of the \ planet always have the same net 'weight'?\n\nBut before we go ...\n \nIt's \ frequently a good idea to see how the answers change as you vary the \ conditions somewhat. So let's consider what happens when we're as ", StyleBox["close", FontSlant->"Italic"], " as possible to the planet, instead of as far away as possible.\n \nWe'll \ just change the + to a ", Cell[BoxData[ FormBox["-", TraditionalForm]]], " " }], "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007765250231895`*^9, 3.4007765272720737`*^9}}], Cell[CellGroupData[{ Cell[BoxData[{ RowBox[{ RowBox[{"celestialbodies", "=", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{ RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "#", "]"}], ",", "\"\\""}], "]"}], "Kilogram"}], ",", RowBox[{ RowBox[{"Abs", "[", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "#", "]"}], ",", "\"\\""}], "]"}], "-", RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "\"\\"", "]"}], ",", "\"\\""}], "]"}]}], "]"}], "Meter"}]}], "}"}], "&"}], "/@", "celestialbodynames"}]}], ";"}], "\n", RowBox[{ RowBox[{ RowBox[{"celestialbodies", "[", RowBox[{"[", RowBox[{"3", ",", "2"}], "]"}], "]"}], "=", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}]}], ";"}], "\n", RowBox[{ RowBox[{ RowBox[{"celestialbodies", "[", RowBox[{"[", RowBox[{"10", ",", "2"}], "]"}], "]"}], "=", RowBox[{"1000", " ", RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{"ratiosclose", "=", RowBox[{ RowBox[{ RowBox[{"(", RowBox[{"Fratio", "[", RowBox[{ RowBox[{"#", "[", RowBox[{"[", "1", "]"}], "]"}], ",", RowBox[{"100", "Kilogram"}], ",", RowBox[{"#", "[", RowBox[{"[", "2", "]"}], "]"}], ",", RowBox[{ FractionBox["1", "2"], "Meter"}]}], "]"}], ")"}], "&"}], "/@", "celestialbodies"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", "ratiosclose"}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]}], "Input", CellChangeTimes->{{3.400774492157262*^9, 3.400774509211893*^9}, { 3.400774555393651*^9, 3.400774560781779*^9}, {3.400774639307777*^9, 3.4007746437744455`*^9}}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "0.1219405800864283187`4.998951359519842"}, {"\<\"Venus\"\>", "6.5358248778338690632`4.995993781180876"}, {"\<\"Earth\"\>", "3.67139972167283694`4.991399828238082*^8"}, {"\<\"Mars\"\>", "0.1700975945726079562`4.999428375654292"}, {"\<\"Jupiter\"\>", "10.7672382817164511378`4.999820710896011"}, {"\<\"Saturn\"\>", "0.7776613195701439679`4.994957429667835"}, {"\<\"Uranus\"\>", "0.0265819321887153508`4.999944160758405"}, {"\<\"Neptune\"\>", "0.013364529512908529`4.999223048057803"}, {"\<\"Pluto\"\>", "6.2950663510876911397407`3.9999812217382704*^-7"}, {"\<\"Moon\"\>", "1115.7942533964774180272`3.501573798148235"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{3.40077450327713*^9, 3.4007745616876097`*^9, 3.4007746446021833`*^9, 3.4007909528014193`*^9}] }, Open ]], Cell["\<\ Big difference. Venus now wins over the taxi driver and Jupiter doubled its \ effect. And look at the relative change of Mars\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007745754468484`*^9, 3.400774615069066*^9}, { 3.400774652239251*^9, 3.4007746663732767`*^9}, {3.4007747412132635`*^9, 3.400774751364749*^9}}], Cell[CellGroupData[{ Cell[BoxData[ RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", RowBox[{"ratiosclose", "/", "ratios"}]}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]], "Input", CellChangeTimes->{{3.400774668466049*^9, 3.400774729156413*^9}}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "7.2740675859554130567`4.698251005949277"}, {"\<\"Venus\"\>", "36.5875432463287779892`4.6966312438516455"}, {"\<\"Earth\"\>", "1.`4.6903698325741"}, {"\<\"Mars\"\>", "17.0718091288230553972`4.69861492994322"}, {"\<\"Jupiter\"\>", "2.1261629668449421609`4.698818876049403"}, {"\<\"Saturn\"\>", "1.5006632539362222442`4.694388119432585"}, {"\<\"Uranus\"\>", "1.2245076592796383957`4.698916853881902"}, {"\<\"Neptune\"\>", "1.1435636335839012594`4.698218232835052"}, {"\<\"Pluto\"\>", "1.0859932262750778983`3.698951605465922"}, {"\<\"Moon\"\>", "1.0000000000000000215`3.200543802484254"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{{3.4007746729951878`*^9, 3.400774729718649*^9}, 3.4007909585642204`*^9}] }, Open ]], Cell["\<\ We can conclude from this that Mercury's, Venus', and Mar's gravitational \ effect is dominated by its distance from us, while the force due to the \ larger planets depends mostly on their mass. But we're not done yet. Other things that vary a lot are the mass of the \ person and their distance from us. Looking at the equation, we can easily see \ that a 50kg (110lb) person will exert half the force. But what about, say, \ the taxi driver's hands holding a new born baby? Here the distance is quite \ a bit closer. Will that change anything? I think a good estimate of the mass of a person's hand is about a pound, so \ two hands is about a kilogram. What of the distance? Before we could be \ cavalier about that since the planets are so far away, any little change we \ make at human scales is irrelevent to the final answer. Now however, we have \ to be more careful. The distance isn't zero, since the distance in the force \ equation is the distance between two centers of mass. For a baby's head \ that's about 5cm from the surface and for your hand about another centimeter, \ for six centimeters total.\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007745754468484`*^9, 3.400774615069066*^9}, { 3.400774652239251*^9, 3.4007746663732767`*^9}, {3.4007747412132635`*^9, 3.4007752425558243`*^9}, {3.4007752810211*^9, 3.4007753184087877`*^9}, { 3.400775415719839*^9, 3.400775434335597*^9}, {3.4007764989892397`*^9, 3.400776506797862*^9}, {3.400791127160886*^9, 3.4007911286133013`*^9}, { 3.4007916883589454`*^9, 3.4007917438658876`*^9}}], Cell[CellGroupData[{ Cell[BoxData[{ RowBox[{"celestialbodynames", "=", RowBox[{"Append", "[", RowBox[{ RowBox[{"AstronomicalData", "[", "\"\\"", "]"}], ",", "\"\\""}], "]"}]}], "\n", RowBox[{ RowBox[{"celestialbodies", "=", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{ RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "#", "]"}], ",", "\"\\""}], "]"}], "Kilogram"}], ",", RowBox[{ RowBox[{"Abs", "[", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "#", "]"}], ",", "\"\\""}], "]"}], "+", RowBox[{"AstronomicalData", "[", RowBox[{ RowBox[{"ToString", "[", "\"\\"", "]"}], ",", "\"\\""}], "]"}]}], "]"}], "Meter"}]}], "}"}], "&"}], "/@", "celestialbodynames"}]}], ";"}], "\n", RowBox[{ RowBox[{ RowBox[{"celestialbodies", "[", RowBox[{"[", RowBox[{"3", ",", "2"}], "]"}], "]"}], "=", RowBox[{ RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}]}], ";"}], "\n", RowBox[{ RowBox[{ RowBox[{"celestialbodies", "[", RowBox[{"[", RowBox[{"10", ",", "2"}], "]"}], "]"}], "=", RowBox[{"1000", " ", RowBox[{"AstronomicalData", "[", RowBox[{"\"\\"", ",", "\"\\""}], "]"}], "Meter"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{"ratioshand", "=", RowBox[{ RowBox[{ RowBox[{"(", RowBox[{"Fratio", "[", RowBox[{ RowBox[{"#", "[", RowBox[{"[", "1", "]"}], "]"}], ",", RowBox[{"1", "Kilogram"}], ",", RowBox[{"#", "[", RowBox[{"[", "2", "]"}], "]"}], ",", RowBox[{ FractionBox["6", "100"], "Meter"}]}], "]"}], ")"}], "&"}], "/@", "celestialbodies"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", "ratioshand"}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]}], "Input", CellChangeTimes->{{3.4007753314648*^9, 3.4007753784727125`*^9}}], Cell[BoxData[ RowBox[{"{", RowBox[{"\<\"Mercury\"\>", ",", "\<\"Venus\"\>", ",", "\<\"Earth\"\>", ",", "\<\"Mars\"\>", ",", "\<\"Jupiter\"\>", ",", "\<\"Saturn\"\>", ",", "\<\"Uranus\"\>", ",", "\<\"Neptune\"\>", ",", "\<\"Pluto\"\>", ",", "\<\"Moon\"\>"}], "}"}]], "Output", CellChangeTimes->{{3.4007753600131283`*^9, 3.400775379519065*^9}, 3.400790965029805*^9}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "0.0241397860618576191`4.999610894104641"}, {"\<\"Venus\"\>", "0.2572347577621281624`4.999335124681315"}, {"\<\"Earth\"\>", "5.2868155992088852`4.991399828238086*^8"}, {"\<\"Mars\"\>", "0.0143476613600963954`4.999861583591135"}, {"\<\"Jupiter\"\>", "7.2923963813929184787`4.9998770343568975"}, {"\<\"Saturn\"\>", "0.746224909048515776`4.995879289724358"}, {"\<\"Uranus\"\>", "0.0312598962216933245`4.999949538350007"}, {"\<\"Neptune\"\>", "0.0168289039047832886`4.999273410400314"}, {"\<\"Pluto\"\>", "8.3471013688166161224037`3.9999819805218673*^-7"}, {"\<\"Moon\"\>", "1606.7437248909274820075`3.501573798148236"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{{3.4007753600131283`*^9, 3.400775379519065*^9}, 3.40079096506104*^9}] }, Open ]], Cell["\<\ Not much change. How about one more: a car passing you on the freeway.\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007745754468484`*^9, 3.400774615069066*^9}, { 3.400774652239251*^9, 3.4007746663732767`*^9}, {3.4007747412132635`*^9, 3.4007752425558243`*^9}, {3.4007752810211*^9, 3.4007753184087877`*^9}, { 3.400775405677952*^9, 3.400775460291459*^9}, {3.4007911698139544`*^9, 3.400791171266453*^9}}], Cell[CellGroupData[{ Cell[BoxData[{ RowBox[{ RowBox[{"ratioscar", "=", RowBox[{ RowBox[{ RowBox[{"(", RowBox[{"Fratio", "[", RowBox[{ RowBox[{"#", "[", RowBox[{"[", "1", "]"}], "]"}], ",", RowBox[{"1000", "Kilogram"}], ",", RowBox[{"#", "[", RowBox[{"[", "2", "]"}], "]"}], ",", RowBox[{"2", "Meter"}]}], "]"}], ")"}], "&"}], "/@", "celestialbodies"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", "ratioscar"}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]}], "Input", CellChangeTimes->{{3.4007754840452895`*^9, 3.400775500708889*^9}}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "0.0268219845131751323`4.9996108941046415"}, {"\<\"Venus\"\>", "0.285816397513475736`4.9993351246813145"}, {"\<\"Earth\"\>", "5.87423955467653911`4.9913998282380865*^8"}, {"\<\"Mars\"\>", "0.0159418459556626615`4.9998615835911355"}, {"\<\"Jupiter\"\>", "8.1026626459921380394`4.999877034356898"}, {"\<\"Saturn\"\>", "0.8291387878316841956`4.995879289724359"}, {"\<\"Uranus\"\>", "0.0347332180241036939`4.999949538350009"}, {"\<\"Neptune\"\>", "0.0186987821164258762`4.999273410400315"}, {"\<\"Pluto\"\>", "9.2745570764629068026371`3.999981980521864*^-7"}, {"\<\"Moon\"\>", "1785.2708054343638688483`3.501573798148235"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{3.400775503113944*^9, 3.4007909697930975`*^9}] }, Open ]], Cell["\<\ Jupiter still wins. OK, I can't resist, one more: you're visiting an \ aircraft carrier and standing on the dock looking up at it (from Wikipedia, \ the mass of an Essex class WWII aircraft carrier is 27200 tons and it's width \ is ~30m)\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007745754468484`*^9, 3.400774615069066*^9}, { 3.400774652239251*^9, 3.4007746663732767`*^9}, {3.4007747412132635`*^9, 3.4007752425558243`*^9}, {3.4007752810211*^9, 3.4007753184087877`*^9}, { 3.400775405677952*^9, 3.400775460291459*^9}, {3.4007755330209694`*^9, 3.40077557496889*^9}, {3.400775840571381*^9, 3.400775877422882*^9}}], Cell[CellGroupData[{ Cell[BoxData[{ RowBox[{ RowBox[{"ratioscarrier", "=", RowBox[{ RowBox[{ RowBox[{"(", RowBox[{"Fratio", "[", RowBox[{ RowBox[{"#", "[", RowBox[{"[", "1", "]"}], "]"}], ",", RowBox[{"Convert", "[", RowBox[{ RowBox[{"27200", " ", "2000", "Pound"}], ",", "Kilogram"}], "]"}], ",", RowBox[{"#", "[", RowBox[{"[", "2", "]"}], "]"}], ",", RowBox[{"50", "Meter"}]}], "]"}], ")"}], "&"}], "/@", "celestialbodies"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", "ratioscarrier"}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]}], "Input", CellChangeTimes->{{3.4007754840452895`*^9, 3.400775500708889*^9}, { 3.400775584542262*^9, 3.4007755857916403`*^9}, {3.400775716539215*^9, 3.4007757166641536`*^9}, {3.400775749366665*^9, 3.400775804932826*^9}, { 3.4007758865277357`*^9, 3.400775900817514*^9}}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "0.0006793704280277686`"}, {"\<\"Venus\"\>", "0.007239404982159495`"}, {"\<\"Earth\"\>", "1.4878782137235038`*^7"}, {"\<\"Mars\"\>", "0.0004037888660002516`"}, {"\<\"Jupiter\"\>", "0.2052312492861346`"}, {"\<\"Saturn\"\>", "0.021001144524072916`"}, {"\<\"Uranus\"\>", "0.0008797529945715342`"}, {"\<\"Neptune\"\>", "0.0004736189301650757`"}, {"\<\"Pluto\"\>", "2.3491400525227925`*^-8"}, {"\<\"Moon\"\>", "45.218883436371335`"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{ 3.4007758058854775`*^9, {3.4007758896355667`*^9, 3.4007759023167686`*^9}, 3.4007909733850884`*^9}] }, Open ]], Cell["\<\ OK, we finally overcame Jupiter but only by a factor of five. If you're 110 \ meters from its center of gravity then\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007745754468484`*^9, 3.400774615069066*^9}, { 3.400774652239251*^9, 3.4007746663732767`*^9}, {3.4007747412132635`*^9, 3.4007752425558243`*^9}, {3.4007752810211*^9, 3.4007753184087877`*^9}, { 3.400775405677952*^9, 3.400775460291459*^9}, {3.4007755330209694`*^9, 3.40077557496889*^9}, {3.400775823767223*^9, 3.4007758371355844`*^9}, { 3.400775942999693*^9, 3.4007759574612627`*^9}, {3.400791176170581*^9, 3.4007911772950974`*^9}, 3.4007918041049585`*^9}], Cell[CellGroupData[{ Cell[BoxData[{ RowBox[{ RowBox[{"ratioscarrier", "=", RowBox[{ RowBox[{ RowBox[{"(", RowBox[{"Fratio", "[", RowBox[{ RowBox[{"#", "[", RowBox[{"[", "1", "]"}], "]"}], ",", RowBox[{"Convert", "[", RowBox[{ RowBox[{"27200", " ", "2000", "Pound"}], ",", "Kilogram"}], "]"}], ",", RowBox[{"#", "[", RowBox[{"[", "2", "]"}], "]"}], ",", RowBox[{"110", "Meter"}]}], "]"}], ")"}], "&"}], "/@", "celestialbodies"}]}], ";"}], "\[IndentingNewLine]", RowBox[{ RowBox[{ RowBox[{"{", RowBox[{"celestialbodynames", ",", "ratioscarrier"}], "}"}], "//", "Transpose"}], "//", "MatrixForm"}]}], "Input", CellChangeTimes->{{3.4007754840452895`*^9, 3.400775500708889*^9}, { 3.400775584542262*^9, 3.4007755857916403`*^9}, {3.400775716539215*^9, 3.4007757166641536`*^9}, {3.400775749366665*^9, 3.400775804932826*^9}, { 3.4007758865277357`*^9, 3.4007759367996454`*^9}}], Cell[BoxData[ TagBox[ RowBox[{"(", "\[NoBreak]", GridBox[{ {"\<\"Mercury\"\>", "0.0032881528716544`"}, {"\<\"Venus\"\>", "0.03503872011365195`"}, {"\<\"Earth\"\>", "7.201330554421757`*^7"}, {"\<\"Mars\"\>", "0.0019543381114412177`"}, {"\<\"Jupiter\"\>", "0.9933192465448915`"}, {"\<\"Saturn\"\>", "0.10164553949651292`"}, {"\<\"Uranus\"\>", "0.004258004493726225`"}, {"\<\"Neptune\"\>", "0.0022923156219989663`"}, {"\<\"Pluto\"\>", "1.1369837854210315`*^-7"}, {"\<\"Moon\"\>", "218.8593958320372`"} }, GridBoxAlignment->{ "Columns" -> {{Left}}, "ColumnsIndexed" -> {}, "Rows" -> {{Baseline}}, "RowsIndexed" -> {}}, GridBoxSpacings->{"Columns" -> { Offset[0.27999999999999997`], { Offset[0.7]}, Offset[0.27999999999999997`]}, "ColumnsIndexed" -> {}, "Rows" -> { Offset[0.2], { Offset[0.4]}, Offset[0.2]}, "RowsIndexed" -> {}}], "\[NoBreak]", ")"}], Function[BoxForm`e$, MatrixForm[BoxForm`e$]]]], "Output", CellChangeTimes->{{3.4007759203390713`*^9, 3.400775937174461*^9}, 3.400790977554921*^9}] }, Open ]], Cell["\<\ Its gravitational force on you is equivalent to Jupiter's. Note also that \ we're closing in on the Moon. One might consider doing the calculation for \ the Sears Tower. As a final observation, all this is relevent to why G, the gravitational \ constant, is the least well measured fundamental constant. There's so much \ mass around that it's hard to know where it all is.\ \>", "Text", CellChangeTimes->{{3.400768528057516*^9, 3.4007685731131763`*^9}, { 3.4007686750935884`*^9, 3.4007687083582554`*^9}, {3.400768894031314*^9, 3.400768906571938*^9}, {3.400769204111101*^9, 3.400769278980028*^9}, { 3.400769397277443*^9, 3.4007694422862577`*^9}, {3.400769529352225*^9, 3.4007695398157616`*^9}, {3.400769652525196*^9, 3.400769781960665*^9}, 3.4007698665434976`*^9, {3.4007707086312857`*^9, 3.4007709026607485`*^9}, { 3.4007711005458183`*^9, 3.4007711050438824`*^9}, {3.4007711367801976`*^9, 3.400771151523822*^9}, {3.4007712423748465`*^9, 3.400771254510143*^9}, { 3.400771319840706*^9, 3.400771374644483*^9}, {3.400771518080063*^9, 3.400771658328702*^9}, {3.400771951596328*^9, 3.4007719663546124`*^9}, { 3.4007722328315*^9, 3.400772254305195*^9}, {3.400773166994834*^9, 3.400773351934136*^9}, {3.400773383262308*^9, 3.4007736120607166`*^9}, { 3.4007736974938755`*^9, 3.4007738433068895`*^9}, {3.4007739228818383`*^9, 3.4007740129830275`*^9}, {3.4007741148129234`*^9, 3.40077424575417*^9}, { 3.4007743944833994`*^9, 3.4007744647324*^9}, {3.400774511570174*^9, 3.4007745453826604`*^9}, {3.4007745754468484`*^9, 3.400774615069066*^9}, { 3.400774652239251*^9, 3.4007746663732767`*^9}, {3.4007747412132635`*^9, 3.4007752425558243`*^9}, {3.4007752810211*^9, 3.4007753184087877`*^9}, { 3.400775405677952*^9, 3.400775460291459*^9}, {3.4007755330209694`*^9, 3.40077557496889*^9}, {3.400775823767223*^9, 3.4007758371355844`*^9}, { 3.400775942999693*^9, 3.400776145196167*^9}, {3.4007911905549817`*^9, 3.4007912051892605`*^9}, {3.4007918260015154`*^9, 3.4007918417601523`*^9}}] }, Open ]] }, WindowSize->{660, 639}, WindowMargins->{{0, Automatic}, {Automatic, 4}}, PrintingCopies->1, PrintingPageRange->{Automatic, Automatic}, CellLabelAutoDelete->True, FrontEndVersion->"6.0 for Microsoft Windows (32-bit) (June 19, 2007)", StyleDefinitions->"Default.nb" ] (* End of Notebook Content *) (* Internal cache information *) (*CellTagsOutline CellTagsIndex->{} *) (*CellTagsIndex CellTagsIndex->{} *) (*NotebookFileOutline Notebook[{ Cell[CellGroupData[{ Cell[590, 23, 251, 3, 77, "Subtitle"], Cell[844, 28, 679, 12, 191, "Text"], Cell[1526, 42, 381, 10, 46, "Input"], Cell[1910, 54, 223, 3, 29, "Text"], Cell[2136, 59, 130, 2, 31, "Input"], Cell[CellGroupData[{ Cell[2291, 65, 188, 3, 31, "Input"], Cell[2482, 70, 222, 5, 51, "Output"] }, Open ]], Cell[2719, 78, 400, 7, 47, "Text"], Cell[CellGroupData[{ Cell[3144, 89, 366, 10, 45, "Input"], Cell[3513, 101, 202, 4, 30, "Output"] }, Open ]], Cell[3730, 108, 495, 8, 29, "Text"], Cell[CellGroupData[{ Cell[4250, 120, 522, 13, 48, "Input"], Cell[4775, 135, 201, 4, 30, "Output"] }, Open ]], Cell[4991, 142, 817, 22, 31, "Text"], Cell[CellGroupData[{ Cell[5833, 168, 329, 10, 54, "Input"], Cell[6165, 180, 192, 4, 30, "Output"] }, Open ]], Cell[6372, 187, 1933, 37, 215, "Text"], Cell[CellGroupData[{ Cell[8330, 228, 322, 8, 31, "Input"], Cell[8655, 238, 182, 3, 30, "Output"] }, Open ]], Cell[8852, 244, 1045, 17, 137, "Text"], Cell[CellGroupData[{ Cell[9922, 265, 418, 11, 72, "Input"], Cell[10343, 278, 196, 4, 30, "Output"] }, Open ]], Cell[10554, 285, 612, 8, 29, "Text"], Cell[CellGroupData[{ Cell[11191, 297, 339, 9, 31, "Input"], Cell[11533, 308, 169, 3, 30, "Output"] }, Open ]], Cell[11717, 314, 668, 8, 29, "Text"], Cell[CellGroupData[{ Cell[12410, 326, 169, 4, 50, "Input"], Cell[12582, 332, 111, 1, 30, "Output"] }, Open ]], Cell[12708, 336, 1193, 20, 137, "Text"], Cell[13904, 358, 378, 10, 49, "Input"], Cell[14285, 370, 852, 13, 29, "Text"], Cell[CellGroupData[{ Cell[15162, 387, 294, 8, 45, "Input"], Cell[15459, 397, 159, 2, 30, "Output"] }, Open ]], Cell[15633, 402, 1321, 24, 101, "Text"], Cell[CellGroupData[{ Cell[16979, 430, 1750, 49, 212, "Input"], Cell[18732, 481, 455, 8, 30, "Output"], Cell[19190, 491, 2227, 61, 231, "Output"] }, Open ]], Cell[21432, 555, 919, 14, 29, "Text"], Cell[CellGroupData[{ Cell[22376, 573, 554, 16, 45, "Input"], Cell[22933, 591, 752, 15, 55, "Output"] }, Open ]], Cell[23700, 609, 1428, 27, 83, "Text"], Cell[CellGroupData[{ Cell[25153, 640, 233, 6, 31, "Input"], Cell[25389, 648, 1355, 27, 182, "Output"] }, Open ]], Cell[26759, 678, 1339, 21, 83, "Text"], Cell[CellGroupData[{ Cell[28123, 703, 487, 13, 72, "Input"], Cell[28613, 718, 167, 2, 30, "Output"] }, Open ]], Cell[28795, 723, 2040, 32, 263, "Text"], Cell[CellGroupData[{ Cell[30860, 759, 2148, 64, 226, "Input"], Cell[33011, 825, 1353, 27, 182, "Output"] }, Open ]], Cell[34379, 855, 1454, 21, 47, "Text"], Cell[CellGroupData[{ Cell[35858, 880, 267, 7, 31, "Input"], Cell[36128, 889, 1302, 27, 176, "Output"] }, Open ]], Cell[37445, 919, 2705, 40, 227, "Text"], Cell[CellGroupData[{ Cell[40175, 963, 2227, 67, 246, "Input"], Cell[42405, 1032, 385, 7, 30, "Output"], Cell[42793, 1041, 1329, 27, 182, "Output"] }, Open ]], Cell[44137, 1071, 1547, 22, 29, "Text"], Cell[CellGroupData[{ Cell[45709, 1097, 680, 20, 72, "Input"], Cell[46392, 1119, 1305, 26, 182, "Output"] }, Open ]], Cell[47712, 1148, 1761, 25, 47, "Text"], Cell[CellGroupData[{ Cell[49498, 1177, 987, 26, 92, "Input"], Cell[50488, 1205, 1173, 28, 182, "Output"] }, Open ]], Cell[51676, 1236, 1768, 25, 29, "Text"], Cell[CellGroupData[{ Cell[53469, 1265, 990, 26, 92, "Input"], Cell[54462, 1293, 1134, 27, 182, "Output"] }, Open ]], Cell[55611, 1323, 2055, 30, 101, "Text"] }, Open ]] } ] *) (* End of internal cache information *)