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you contract in length in the direction of travel, an --------=_MB8CB8ECBE-A1B7-41E7-A8ED-E5DC5A50F02E Content-Type: text/plain; format=flowed; charset=utf-8 Content-Transfer-Encoding: quoted-printable Hello Larry & All, Thanks Larry, my question about being able to determine "c" using=20 electrical hardware goes back at least 35 years. I did read Maxwell's=20 equations then and, step by step, could follow the derivation of them=20 but felt none the wiser when finished. But I can now at least cross that=20 off of my bucket list. It seemed too easy to be true and perhaps low=20 precision of this electrical method accounts for official determinations=20 of "c" by other more expensive methods. I now see, on the internet, some=20 lab demonstrations of this. Dave W Hello Patrick & All,, Thanks for the explanation. I did read General Relativity in part=20 shortly after it came out but did not absorb much. Perhaps with your=20 explanation in hand it will make more sense. So, if I understand=20 correctly, space between A and B can expand at speeds greater than the=20 speed of light; strange. And I suppose any expansion between A and B at=20 rates slower than the speed of light would increase the wavelength of=20 light. Dave W ------ Original Message ------ From: "Patrick Kelly" <Patrick.Kelly@dal.ca> To: "naturens@chebucto.ns.ca" <naturens@chebucto.ns.ca> Sent: 2/25/2019 6:28:29 PM Subject: Re: Re[2]: [NatureNS] Big Bang? >Two other points worth noting: Shortly after the Big Bang there was a=20 >period of cosmic inflation. This was originally an entirely theoretical=20 >concept to deal with issues such as why is the universe so flat. and=20 >the horizon problem (how can the cosmic microwave background be almost=20 >exactly the same in opposite directions when there has not been enough=20 >time in the universe for them to have been in contact with each other.=20 >Cosmic inflation, which now has some observational evidence to back it=20 >up, was a brief period when the size of the universe expanded=20 >exponentially, and much faster than the speed of light. This is not a=20 >problem as relativity theory does not prohibit space-time from=20 >expanding faster than the speed of light. Cosmic inflation carried the=20 >vast majority of the universe so far from us that its light has not yet=20 >reached us. Thus, the term "observable universe". At the end of the=20 >cosmic inflationary period, the expansion took on the rate that we see=20 >now (less the effects of mass slowing it and dark energy accelerating=20 >it. > >It is also worth noting that special relativity deals only with the=20 >speed of light. For the universe to be logically consistent, all=20 >observers, regardless of their relative motion (hence the term=20 >"relativity") see the speed of light in a vacuum as the "speed of=20 >light". As Carl Sagan said, Thou shalt not add the speed to the speed=20 >of light. Special relativity is what makes strange things appear to=20 >happen to other observers as you near the speed of light. Your clocks=20 >(biological and mechanical) slow down, you contract in length in the=20 >direction of travel, and your mass increases. Unless you are making=20 >really precise measurements, such as with an atomic clock or the GPS=20 >satellites, these effect do not really start to show up until you get=20 >near 50% of the speed of light. At "human" speeds, the equations=20 >simplify to Newton's laws of motion. When you add gravity to special=20 >relativity you get general relativity, which, when Einstein first=20 >worked it out, had him puzzled as it predicted that the universe should=20 >be either expanding or contracting! General relativity also says that=20 >"gravity" is the warping of space-time caused by the presence of mass.=20 >All moving objects, including light respond to the warping of=20 >space-time by changing their velocity, so that even light, passing near=20 >a massive object, will change direction. This effect is responsible for=20 >gravitational lenses.=20 >(https://en.wikipedia.org/wiki/Gravitational_lens) Some exoplanets have=20 >been found using gravitational lens. > >Pat > > >On Feb 25, 2019, at 2:08 PM, Larry Bogan wrote: > >>David, >> Maxwell's equations summarize the laws of electric and magnetic=20 >>fields. Their solutions for an oscillating electric charge describes=20 >>the electromagnetic wave (light, radio, xray, microwave, etc) and in=20 >>the solution the speed of those waves in a vacuum is determined by two=20 >>constants, the permittivity and permeability of free space. These two=20 >>constants are determined separately by the laws of electric and=20 >>magnetic fields. >> >>All this was known in the late 19th century. >>https://en.wikipedia.org/wiki/Maxwell%27s_equations >>-- >>Larry Bogan >><larry@bogan.ca> >>Brooklyn Corner, Nova Scotia >> >> >> >>On Mon, 25 Feb 2019 14:22:37 +0000 >>David <dwebster@glinx.com> wrote: >> >>>Hi Burkhard, Lois, Don & All, >>> The more I hear about the big bang, which seems to be heavy on >>>speculation and light on certainty, the more I am inclined to turn to >>>the present and try to understand it. >>> One puzzle to which I have found no clear answer is a statement=20 >>>in a >>>text on Electricity and Magnetism (G.R. Noakes,1950); (page 322)=20 >>>that >>>ratios of such measurements as capacity in electromagnetic units and >>>capacity in electrostatic units is "...the simplest direct way of >>>determining c, the speed of light. It would be inconvenient to do so=20 >>>but >>>this suggests that the speed of light (in air ?) could be measured in >>>the dark. >>> Does this imply that c is determined by the interaction of >>>electrostatic and electromagnetic forces (possible because light=20 >>>waves >>>involve both) or is this just a coincidence of ratios between two >>>independently developed systems of measurement ? >>>YT, DW, Kentville >>> > > >Patrick Kelly > >159 Town Road > >Falmouth NS B0P 1L0 > >Canada > > > >(902) 472-2322 > > --------=_MB8CB8ECBE-A1B7-41E7-A8ED-E5DC5A50F02E Content-Type: text/html; charset=utf-8 Content-Transfer-Encoding: quoted-printable <html><head> <style id=3D"css_styles" type=3D"text/css">blockquote.cite { margin-left: 5= px; margin-right: 0px; padding-left: 10px; padding-right:0px; border-left:= 1px solid #cccccc } blockquote.cite2 {margin-left: 5px; margin-right: 0px; padding-left: 10px;= padding-right:0px; border-left: 1px solid #cccccc; margin-top: 3px; padding= -top: 0px; } a img { border: 0px; } li[style=3D'text-align: center;'], li[style=3D'text-align: right;'] { list= -style-position: inside;} body { font-family: Segoe UI; font-size: 12pt; }</style></head> <body><div>Hello Larry & All,</div><div>=C2=A0 =C2=A0 Thanks Larry, my= question about being able to determine "c" using electrical hardware goes b= ack at least 35 years. I did read Maxwell's equations then and, step by ste= p, could follow the derivation of them but felt none the wiser when finishe= d. But I can now at least cross that off of my bucket list. It seemed too e= asy to be true and perhaps low precision of this electrical method accounts = for official determinations of "c" by other more expensive methods. I now= see, on the internet, some lab demonstrations of this.</div> <div>Dave W</div><div><br /></div><div>Hello Patrick & All,,</div><div>= =C2=A0 =C2=A0 Thanks for the explanation. I did read General Relativity in= part shortly after it came out but did not absorb much. Perhaps with your e= xplanation in hand =C2=A0it will make more sense. So, if I understand corre= ctly, space between A and B can expand at speeds greater than the speed of= light; strange. And I suppose any expansion between A and B at rates slower = than the speed of light would increase the wavelength of light.=C2=A0</div= ><div>Dave W</div> <div>------ Original Message ------</div> <div>From: "Patrick Kelly" <<a href=3D"mailto:Patrick.Kelly@dal.ca">Patr= ick.Kelly@dal.ca</a>></div> <div>To: "naturens@chebucto.ns.ca" <<a href=3D"mailto:naturens@chebucto.= ns.ca">naturens@chebucto.ns.ca</a>></div> <div>Sent: 2/25/2019 6:28:29 PM</div> <div>Subject: Re: Re[2]: [NatureNS] Big Bang?</div><div><br /></div> <div id=3D"x2a9d804c0f1441b" style=3D"word-wrap: break-word; -webkit-nbsp-m= ode: space; -webkit-line-break: after-white-space; "><blockquote cite=3D"8E= 34287A-B259-46CE-95A6-DF59515F9736@dal.ca" type=3D"cite" class=3D"cite2"> Two other points worth noting: Shortly after the Big Bang there was a perio= d of cosmic inflation. This was originally an entirely theoretical concept= to deal with issues such as why is the universe so flat. and the horizon pr= oblem (how can the cosmic microwave background be almost exactly the same in opposite directions when there ha= s not been enough time in the universe for them to have been in contact wit= h each other. Cosmic inflation, which now has some observational evidence t= o back it up, was a brief period when the size of the universe expanded exponentially, and much faster than = the speed of light. This is not a problem as relativity theory does not pr= ohibit space-time from expanding faster than the speed of light. Cosmic inf= lation carried the vast majority of the universe so far from us that its light has not yet reached us. Thus= , the term "observable universe". At the end of the cosmic inflationary per= iod, the expansion took on the rate that we see now (less the effects of ma= ss slowing it and dark energy accelerating it. <div><br /> </div> <div>It is also worth noting that special relativity deals only with the sp= eed of light. For the universe to be logically consistent, all observers, r= egardless of their relative motion (hence the term "relativity") see the sp= eed of light in a vacuum as the "speed of light". As Carl Sagan said, Thou shalt not add the speed to the= speed of light. Special relativity is what makes strange things appear to h= appen to other observers as you near the speed of light. Your clocks (biolo= gical and mechanical) slow down, you contract in length in the direction of travel, and your mass increases= . Unless you are making really precise measurements, such as with an atomic = clock or the GPS satellites, these effect do not really start to show up u= ntil you get near 50% of the speed of light. At "human" speeds, the equations simplify to Newton's laws of mo= tion. When you add gravity to special relativity you get general relativity= , which, when Einstein first worked it out, had him puzzled as it predicted = that the universe should be either expanding or contracting! General relativity also says that "gravity" is t= he warping of space-time caused by the presence of mass. All moving objects= , including light respond to the warping of space-time by changing their ve= locity, so that even light, passing near a massive object, will change direction. This effect is responsible f= or gravitational lenses. (<a href=3D"https://en.wikipedia.org/wiki/Gravitat= ional_lens">https://en.wikipedia.org/wiki/Gravitational_lens</a>) Some exop= lanets have been found using gravitational lens.</div> <div><br /> </div> <div>Pat</div> <div><br /> </div> <div><br /> <div> <div>On Feb 25, 2019, at 2:08 PM, Larry Bogan wrote:</div> <br class=3D"Apple-interchange-newline" /> <blockquote type=3D"cite" class=3D"cite"> <div>David,<br /> =C2=A0Maxwell's equations summarize the laws of electric and magnetic field= s. Their solutions for an oscillating electric charge describes the electro= magnetic wave (light, radio, xray, microwave, etc) and in the solution the= speed of those waves in a vacuum is determined by two constants, the permittivity and permeability of free space. These t= wo constants are determined separately by the laws of electric and magnetic = fields.<br /> <br /> All this was known in the late 19th century.<br /> <a href=3D"https://en.wikipedia.org/wiki/Maxwell%27s_equations">https://en.= wikipedia.org/wiki/Maxwell%27s_equations</a><br /> -- <br /> Larry Bogan <br /> <larry@bogan.ca><br /> Brooklyn Corner, Nova Scotia<br /> <br /> <br /> <br /> On Mon, 25 Feb 2019 14:22:37 +0000<br /> David <dwebster@glinx.com>= wrote:<br /> <br /> <blockquote type=3D"cite" class=3D"cite">Hi Burkhard, Lois, Don & All,<= br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">=C2=A0=C2=A0=C2=A0=C2=A0The more I = hear about the big bang, which seems to be heavy on <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">speculation and light on certainty= , the more I am inclined to turn to <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">the present and try to understand= it.<br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">=C2=A0=C2=A0=C2=A0=C2=A0One puzzle = to which I have found no clear answer is a statement in a <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">text on Electricity and Magnetism= (G.R. Noakes,1950); =C2=A0(page 322) that <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">ratios of such measurements as cap= acity in electromagnetic units and <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">capacity in electrostatic units is = "...the simplest direct way of <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">determining c, the speed of light. = It would be inconvenient to do so but <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">this suggests that the speed of li= ght (in air ?) could be measured in <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">the dark.<br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">=C2=A0=C2=A0=C2=A0=C2=A0Does this= imply that c is determined by the interaction of <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">electrostatic and electromagnetic= forces (possible because light waves <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">involve both) or is this just a co= incidence of ratios between two <br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">independently developed systems of = measurement ?<br /> </blockquote> <blockquote type=3D"cite" class=3D"cite">YT, DW, Kentville<br /> </blockquote> <blockquote type=3D"cite" class=3D"cite"><br /> </blockquote> </div> </blockquote> </div> <br /> <div><span class=3D"Apple-style-span" style=3D"border-collapse: separate; f= ont-family: Helvetica; border-spacing: 0px;"><span class=3D"Apple-style-spa= n" style=3D"border-collapse: separate; color: rgb(0, 0, 0); font-family: He= lvetica; font-size: 12px; font-style: normal; font-variant: normal; font-we= ight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text= -indent: 0px; text-transform: none; white-space: normal; widows: 2; word-sp= acing: 0px; -webkit-border-horizontal-spacing: 0px; -webkit-border-vertical= -spacing: 0px; -webkit-text-decorations-in-effect: none; -webkit-text-size-= adjust: auto; -webkit-text-stroke-width: 0px; "> <div style=3D"word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line= -break: after-white-space; "> <span class=3D"Apple-style-span" style=3D"border-collapse: separate; color: = rgb(0, 0, 0); font-family: Helvetica; font-size: 12px; font-style: normal; = font-variant: normal; font-weight: normal; letter-spacing: normal; line-he= ight: normal; orphans: 2; text-indent: 0px; text-transform: none; white-spa= ce: normal; widows: 2; word-spacing: 0px; -webkit-border-horizontal-spacing= : 0px; -webkit-border-vertical-spacing: 0px; -webkit-text-decorations-in-ef= fect: none; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; = "> <div style=3D"word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line= -break: after-white-space; "> <span class=3D"Apple-style-span" style=3D"border-collapse: separate; color: = rgb(0, 0, 0); font-family: Helvetica; font-size: 12px; font-style: normal; = font-variant: normal; font-weight: normal; letter-spacing: normal; line-he= ight: normal; orphans: 2; text-indent: 0px; text-transform: none; white-spa= ce: normal; widows: 2; word-spacing: 0px; -webkit-border-horizontal-spacing= : 0px; -webkit-border-vertical-spacing: 0px; -webkit-text-decorations-in-ef= fect: none; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; = "> <p style=3D"margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-= left: 0px; "> <font face=3D"Courier" size=3D"3" style=3D"font-style: normal; font-variant= : normal; font-stretch: normal; font-size: 12px; line-height: normal; font-= family: Courier;"><br class=3D"Apple-interchange-newline" /> Patrick Kelly</font></p> <p style=3D"margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-= left: 0px; "> <font face=3D"Courier" size=3D"3" style=3D"font-style: normal; font-variant= : normal; font-stretch: normal; font-size: 12px; line-height: normal; font-= family: Courier;">159 Town Road</font></p> <p style=3D"margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-= left: 0px; "> <font face=3D"Courier" size=3D"3" style=3D"font-style: normal; font-variant= : normal; font-stretch: normal; font-size: 12px; line-height: normal; font-= family: Courier;">Falmouth NS<span class=3D"Apple-converted-space">=C2=A0<s= pan class=3D"Apple-converted-space">=C2=A0</span></span>B0P 1L0</font></p> <p style=3D"margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-= left: 0px; "> <font face=3D"Courier" size=3D"3" style=3D"font-style: normal; font-variant= : normal; font-stretch: normal; font-size: 12px; line-height: normal; font-= family: Courier;">Canada</font></p> <p style=3D"margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-= left: 0px; font: normal normal normal 12px/normal Courier; min-height: 14px= ; "> <br /> </p> <p style=3D"margin-top: 0px; margin-right: 0px; margin-bottom: 0px; margin-= left: 0px; "> <font face=3D"Courier" size=3D"3" style=3D"font-style: normal; font-variant= : normal; font-stretch: normal; font-size: 12px; line-height: normal; font-= family: Courier;">(902) 472-2322</font></p> </span></div> </span></div> </span></span></div> <br /> </div> </blockquote></div> </body></html> --------=_MB8CB8ECBE-A1B7-41E7-A8ED-E5DC5A50F02E--
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