New Newton Mechanics Taking Law of Conservation of Energy as Unique Source Law (Revised Version)

Size: px
Start display at page:

Download "New Newton Mechanics Taking Law of Conservation of Energy as Unique Source Law (Revised Version)"

Transcription

1 New Newton Mechanics Taking Law of Conseation of Enegy as Unique Souce Law (Reised Vesion) Fu Yuhua CNOOC Reseach Institute Abstact: Accoding to the pinciple of the uniqueness of tuth, this pape pesents the New Newton Mechanics (NNM) taking law of conseation of enegy as unique souce law. Examples show that in some cases othe laws may be contadicted with the law of conseation of enegy. The oiginal Newton's thee laws and the law of gaity, in pinciple can be deied by the law of conseation of enegy. Though the example of fee falling body, this pape deies the oiginal Newton's second law and the oiginal law of gaity by using the law of conseation of enegy; and though the example of a small ball olls along the inclined plane (belonging to the poblem cannot be soled by geneal elatiity that a body is foced to moe in flat space), deies impoed Newton's second law and impoed law of gaity by using law of conseation of enegy. Whethe o not othe conseation laws (such as the law of conseation of momentum and the law of conseation of angula momentum) can be utilized, should be tested by law of conseation of enegy. When the oiginal Newton's second law is not coect, then the laws of conseation of momentum and angula momentum ae no longe coect; theefoe the geneal foms of impoed law of conseation of momentum and impoed law of conseation of angula momentum ae pesented. In the cases that law of conseation of enegy cannot be used effectiely, New Newton Mechanics will not exclude that accoding to othe theoies o accuate expeiments to deie the laws o fomulas to sole some specific poblems. Fo example, with the help of the esult of geneal elatiity, the impoed Newton's fomula of uniesal gaitation can be deied, which can be used to sole the poblem of adance of planetay peihelion and the poblem of deflection of photon aound the Sun. Again, accoding to accuate expeimental esult, the synthesized gaitational fomula (including the effects of othe celestial bodies and sunlight pessue) fo the poblem of deflection of photon aound the Sun is pesented. Unlike the oiginal Newton Mechanics, in New Newton Mechanics, fo diffeent poblems, may hae diffeent laws of motion, diffeent fomulas of gaity, as well as diffeent expessions of enegy. Fo example, fo the poblem of a small ball olls along the inclined plane, and the poblem of adance of planetay peihelion, the two fomulas of gaity ae completely diffeent. Keywods: Uniqueness of tuth, law of conseation of enegy, unique souce law, New Newton Mechanics (NNM) Intoduction One of the deelopment tends of natual science is using fewe laws to sole inceasing poblems. In this pocess, some laws will play the inceasingly geat oles; while othes will play the smalle oles, o een disappea fom the anks of laws. Now we discuss the law of conseation of enegy. Its main contents ae as follows: In a closed system, the total enegy of this system emains unchanged.

2 Because the law of conseation of enegy is the most impotant one in natual sciences, it should play an inceasingly geat ole. Fo this eason and accoding to the pinciple of the uniqueness of tuth, this pape pesents the New Newton Mechanics (NNM) taking law of conseation of enegy as unique souce law. In the aea of Newton Mechanics, thee should be one tuth only. Othe so-called tuth, eithe it can be deied by the unique tuth, o we can poe that in cetain cases it is not tue. As wellknown, when Newton founded the classical mechanics, fou laws wee poposed, they wee Newton's thee laws and the law of gaity. If the law of conseation of enegy is choosing as the unique souce law, that in pinciple, all the Newton's fou laws can be deied accoding to the law of conseation of enegy; afte studying caefully we found that this may indeed be the eal case. In addition, in the aeas such as physics, mechanics, engineeing and so on, thee ae thee ey impotant laws: the law of conseation of enegy, the law of conseation of momentum and the law of conseation of angula momentum. If we beliee that the law of conseation of enegy is the tuth, then fo the law of conseation of momentum and the law of conseation of angula momentum, eithe they can be deied by the law of conseation of enegy, o we can poe that in cetain cases they ae not tue. We beliee that the tue situation is the latte, namely, the law of conseation of momentum and the law of conseation of angula momentum ae not tue in some cases (o thei esults ae contadicted to the law of conseation of enegy). Of couse, we can also find that in some cases, these two laws still can be used. Taking the example that a man walks along the ca located on the hoizontal smooth ail, we can see that at pesent in the aea of Newton mechanics, some people do not notice the case of the contadiction between the law of conseation of enegy and the law of conseation of momentum. New Thee Laws of Motion and New Law of Gaity (Fomula) Ceated By Law of Conseation Of Enegy fo New Newton Mechanics The oiginal Newton's thee laws of motion ae as follows. Newton's Fist Law of Motion: Eey object in a state of unifom motion (o at est) tends to emain in that state of motion (o at est) unless an extenal foce is applied to it. Fo shot: est emains est, and moing emains moing. Newton's Second Law of Motion: The elationship between an object's mass m, its acceleation a, and the applied foce F is F = ma. The diection of the foce is the same as the diection of the acceleation. Newton's Thid Law of Motion: Fo eey action thee is an equal and opposite eaction. The oiginal Newton s law of gaity: The attactie foce between two objects is as follows F ()

3 While fo NNM, taking law of conseation of enegy as unique souce law, then we hae the following NNM s thee laws of motion and law of gaity. NNM's Fist Law of Motion: Eey object in a state of unifom motion (o in a state of unifom otation, o at est) tends to emain in that state of motion (o in a state of unifom otation, o at est) unless an extenal foce is applied to it; othewise the law of conseation of enegy will be destoyed. Fo shot: est emains est, moing emains moing, and otating emains otating. NNM's Second Law of Motion: The elationship between an object's mass m, its acceleation a, and the applied foce F is a function that should be deied by law of conseation of enegy. The diection of the foce is the same as the diection of the acceleation. In geneal, the function can be witten as the fom of aiable dimension factal: F ma, whee: is a constant o a aiable. Fo diffeent poblems, the foms of second law may be diffeent. NNM's Thid Law of Motion: In geneal, fo eey action thee is an equal and opposite eaction. In special case, the function elationship between action and eaction should be deied by law of conseation of enegy. The impoed fom of the oiginal Newton s thid law ( F AB F BA ) is as follows: F AB F BA, whee: is a constant o a aiable. Fo diffeent poblems, the foms of thid law may be diffeent. NNM s law (fomula) of gaity: The attactie foce between two objects is a function that should be deied by law of conseation of enegy, o expeimental data; o deied with the help of othe theoies. Fo diffeent poblems, the foms of law (fomula) of gaity may be diffeent. The esults of oiginal Newton s law of gaity ae only accuate in the cases that two objects ae elatie static o unning the staight line between one cente and anothe cente, and the like; fo othe cases its esults ae all appoximate. In geneal, NNM s law (fomula) of gaity may be taken as the fom that adding the amending tem to oiginal Newton s law of gaity, o the following fom of aiable dimension factal: F () whee: is a constant o a aiable. Now fo an example, a NNM s law (fomula) of gaity (an impoed Newton s law of gaity) and a NNM's second law of motion (an impoed Newton s second law of motion), they ae suitable fo this example only, ae deied simultaneously by law of conseation of enegy. Fistly, the aiational pinciples established by the law of conseation of enegy can be gien with least squaes method (LSM).

4 Supposing that the initial total enegy of a closed system equals W (), and fo time t the total enegy equals W (t), then accoding to the law of conseation of enegy: W () = W (t) (3) This can be witten as: W( t) R W = W() (4) Accoding to LSM, fo the inteal [ t,t ],we can wite the following aiational pinciple: t R W dt min (5) t Whee: min denotes the minimum alue of functional Π and it should be equal to zeo. It should be noted that, in many cases W (t) is appoximate, and R W is not identically equal to zeo, theefoe Eq.(5) can be used to sole the poblem. Besides the time coodinate, anothe one can also be used. Fo example, fo inteal [ x, x ], the following aiational pinciple can be gien accoding to the law of conseation of enegy: x x R W dx min (6) The aboe-mentioned pinciples ae established by using the law of conseation of enegy diectly. Sometimes, a cetain pinciple should be established by using the law of conseation of enegy indiectly. Fo example, a special physical quantity Q may be inteested,not only it can be calculated by using the law of conseation of enegy, but also can be calculated by using othe laws (fo this pape they ae the law of gaity, and Newton s second law). Fo distinguishing the alues, let s denote the alue gien by othe laws as Q,while denote the alue gien by the law of

5 conseation of enegy as Q ',then the alue of R W can be edefined as follows: Q R W = Q' (7) Substituting Eq.(7)into Eqs.(5)and(6), as Q ' is the esult calculated with the law of conseation of enegy, it gies the aiational pinciple established by using the law of conseation of enegy indiectly. Othewise, it is clea that the extent of the alue of Q accods with Q '. Substituting the elated quantities into Eq.(5)o Eq.(6), the equations deied by the condition of an extemum can be witten as follows: a i k i (8) Afte soling these equations, the impoed law of gaity, and Newton s second law can be eached at once. Accoding to the alue of Π, the effect of the solution can be judged. The neae the alue of Π is to zeo, the bette the effect of the solution. It should be noted that besides of soling equations, optimum-seeking methods could also be used fo finding the minimum and the constants to be detemined. In fact, the optimum seeking method will be used in this pape. Now we sole an example. As shown in Fig., supposing that the small ball olls along a long incline fom A to B. Its initial elocity is zeo and the fiction and the otational enegy of small ball ae neglected. Figue. A small ball olls fom A to B Supposing that cicle O ' denotes the Eath, M denotes its mass; m denotes the mass of the small ball (teated as a mass point ), O A is a plumb line, coodinate x is othogonal to O A, coodinate y

6 is othogonal to coodinate x (paallel to O A), BC is othogonal to O A. The lengths of OA, OB, BC, and AC ae all equal to H, and O C equals the adius R of the Eath. In this example, the alue of which is the squae of the elocity fo the ball located at point is inestigated. To distinguish the quantities, denote the alue gien by the impoed law of gaity and impoed Newton s second law as conseation of enegy,then Eq.(6)can be witten as,while ' denotes the alue gien by the law of H ( ' ) dx min (9) Supposing that the impoed law of gaity and impoed Newton s second law can be witten as the following constant dimension factal foms F () D F ma () whee: D and ae constants. Now we calculate the elated quantities accoding to the law of conseation of enegy. Fom Eq.(), the potential enegy of the small ball located at point is V () ( D ) D O ' Accoding to the law of conseation of enegy, we can get ( D ) D O' A m' ( D ) D O ' (3) And theefoe GM ' [ ] (4) D D D ( R H) O'

7 Now we calculate the elated quantities accoding to the impoed law of gaity and impoed Newton s second law. Supposing that the equation of olling line is y x H (5) Fo the ball located at point, d/ dt a (6) Because dt ds dx Theefoe d a dx (7) Accoding to the impoed law of gaity, the foce along to the tangent is Fa (8) D O' Accoding to the impoed Newton s second law, fo point, the acceleation along to the tangent is Fa GM a ( ) ( ) (9) m / / D O ' Fom Eq.(7), it gies GM / d { } dx () D/ [( H x) ( R H y) ] Substituting Eq.(5) into Eq.(), and fo the two sides, we un the integal opeation fom A to, it gies

8 x GM / / { } ( ) dx D / [( H x) ( R x) ] () H Then the alue can be calculated by a method of numeical integal. The gien data ae assumed to be: fo Eath, GM= m 3 /s ; the adius of the Eath R= m, H=R/, ty to sole the poblem shown in Fig., find the solution fo the alue of B,and deie the impoed law of gaity and the impoed Newton s second law. Fistly, accoding to the oiginal law of gaity, the oiginal Newton s second law (i.e., let D = in Eq.(), = in Eq.()) and the law of conseation of enegy, all the elated quantities can be calculated, then substitute them into Eq.(9), it gies =57.45 Hee, accoding to the law of conseation of enegy, it gies ' B =.767 7,while accoding to the oiginal law of gaity, and the oiginal Newton s second law, it gies B =.35 7,the diffeence is about 5.4 %. Fo the eason that the alue of Π is not equal to zeo, then the alues of D and can be decided by the optimum seeking method. At pesent all the optimum seeking methods can be diided into two types, one type may not depend on the initial alues which pogam may be complicated, and anothe type equies the bette initial alues which pogam is simple. One method of the second type, namely the seaching method will be used in this pape. Fistly, the alue of D is fixed so let D =,then seach the alue of,as =.46, the alue of Π eaches the minimum ;then the alue of is fixed,and seach the alue of D,as D =.99989, the alue of Π eaches the minimum ;then the alue of D is fixed,and seach the alue of,as =.458, the alue of Π eaches minimum Because the last two esults ae highly close, the seaching can be stopped, and the final esults ae as follows D=.99989,ε=.458, =37.33 Hee the alue of Π is only 4% of Π. While accoding to the law of conseation of enegy, it gies ' B =.785 7,accoding to the impoed law of gaity and the impoed Newton s second law, it gies B =.73 7, the diffeence is about.7 % only.

9 The esults suitable fo this example with the constant dimension factal fom ae as follows The impoed law of gaity eads F () The impoed Newton s second law eads.458 F ma (3) The aboe mentioned esults hae been published on efeence []. Accoding to the esults fo the example shown in Fig., it can be said that we could not ely on any expeimental data, only apply the law of conseation of enegy to deie the impoed law of gaity, and impoed Newton's second law; and demonstate that the oiginal Newton s law of gaity and Newton's second law ae all tenable appoximately fo this example. So, can only apply the law of conseation of enegy to deie that these two oiginal laws o demonstate they ae tenable accuately in some cases? The answe is that in some cases we can indeed deie the oiginal Newton's second law and poe the oiginal Newton s law of gaity is tenable accuately. Now, in the case that a small ball fee falls (equialent to fee fall fom A to C in Fig. ), we deie the oiginal Newton's second law and the oiginal law of gaity by using the law of conseation of enegy. Assuming that fo the oiginal law of gaity and Newton's second law, the elated exponents ae unknown, only know the foms of these two fomulas ae as follows: F, D whee: D and D ae undetemined constants. D' F ma ; As shown in Fig., supposing that a small ball fee falls fom point A to point C. Simila to the aboe deiation, when the small ball falls to point (point is not shown in Fig.), the alue of calculated by the undetemined Newton's second law and the law of gaity, as well as the alue of ' calculated by the law of conseation of enegy ae as follows: GM [ D D ( R H) ' D O' ]

10 y p / D' ( GM ) ( R H y) D / D ' dy ( GM ) / D ' { [( R H y) D / D' D / D' ] y p } / D' ( GM ) [ ( D / D' ) ( D / D') O' ( R H) ( D / D') ] ' Let, then we should hae: / D', and D ( D / D') ; these two equations all gie: D ', this means that fo fee fall poblem, by using the law of conseation of enegy, we stictly deie the oiginal Newton's second law F ma. Hee, although the oiginal law of gaity cannot be deied (the alue of D may be any constant, cetainly including the case that D=), we aleady poe that the oiginal law of gaity is not contadicted to the law of conseation of enegy, o the oiginal law of gaity is tenable accuately. In ode to eally deie the oiginal law of gaity fo the example of fee falling body, we should conside the case that a small ball fee falls fom point A to point (point is not shown in Fig.) though a ey shot distance Z (the two endpoints of the inteal Z ae point A and point ). As deiing the oiginal Newton's second law, we aleady each GM [ D ( R H Z) ( R H ) ' D D ] whee: R H Z O ' Fo the eason that the distance of Z is ey shot, and in this inteal the gaity can be consideed as a linea function, theefoe the wok W of gaity in this inteal can be witten as follows W F whee, a Z R H Z) ( D Z F a is the aeage alue of gaity in this inteal Z midpoint of inteal Z. Omitting the second ode tem of Z, it gies, namely the alue of gaity fo the

11 W ( R H Z RH RZ HZ ) D/ As the small ball fee falls fom point A to point, its kinetic enegy is as follows m ' D D ( R H ) ( R H Z) [ D ( R H RH RZ HZ) D ] Accoding to the law of conseation of enegy, we hae W m' To compae the elated expessions, we can each the following thee equations D D / D Z ( R H ) D ( R H Z) D All of these thee equations will gie the following esult D Thus, we aleady deie the oiginal law of gaity by using the law of conseation of enegy. Fo the example shown in Fig. that a small ball olls along the inclined plane, in ode to obtain the bette esults, we discuss the aiable dimension factal solution with Eq.(4) that is established by the law of conseation of enegy diectly. Supposing that the impoed Newton s second law and the impoed law of gaity with the fom of aiable dimension factal can be witten as follows: ; k F ma, u F /, k u ; whee: u is the hoizon distance that the small ball olls ( u x H ). With the simila seaching method, the alues of k, k can be detemined, and the esults ae as follows u,.7 u The esults of aiable dimension factal ae much bette than that of constant dimension factal. 4 Fo example, the final Π 5.866, it is only.9% of Π (3.7). While accoding to the law of conseation of enegy, it gies ' B =.767 7,accoding to the impoed law of gaity and the impoed Newton s second law, it gies B =.777 7, the diffeence is about

12 .93 % only. The esults suitable fo this example with the aiable dimension factal fom ae as follows The impoed law of gaity eads (4).7 u F 3 The impoed Newton s second law eads u F ma (5) whee: u is the hoizon distance that the small ball olls ( u x H ). Thee is anothe poblem should also be discussed. That is the impoed kinetic enegy fomula. As well-known, the kinetic enegy fomula has been modified in the theoy of elatiity, now we impoe the kinetic enegy fomula with the law of conseation of enegy. Supposing that the impoed kinetic enegy fomula is Ed m, k 3 u ;whee: u is the hoizon distance that the small ball olls ( u x H ). With the simila seaching method, we can get: k , then the impoed kinetic enegy fomula with aiable dimension factal fom eads u E d m Because the effect of impoement is ey small (the alue of Π is only impoed fom into ), theefoe these esults should be fo efeence only. 3 With the Help of Geneal Relatiity and Accuate Expeimental Data to Deie the Impoed Newton's Fomula of Uniesal Gaitation of. Hu Ning deied an equation accoding to geneal elatiity, with the help of Hu's equation and Binet s fomula, we get the following impoed Newton's fomula of uniesal gaitation [] F 3G M c 4 mp (6)

13 whee: G is gaitational constant, M and m ae the masses of the two objects, is the distance between the two objects, c is the speed of light, p is the half nomal chod fo the object m moing aound the object M along with a cue, and the alue of p is gien by: p = a(-e ) (fo ellipse), p = a (e -) (fo hypebola), p = y /x (fo paabola). It should be noted that, this impoed Newton's fomula of uniesal gaitation can also be witten as the fom of aiable dimension factal. Suppose 3G M mp D 4 c It gies GMp D 3 ln( ) / ln 4 c Fo the poblem of gaitational defection of a photon obit aound the Sun, M=.99 3 kg, = m, c= m/s, then we hae: D. The impoed Newton s uniesal gaitation fomula (Eq.(6)) can gie the same esults as gien by geneal elatiity fo the poblem of planetay adance of peihelion and the poblem of gaitational defection of a photon obit aound the Sun. Fo the poblem of planetay adance of peihelion, the impoed Newton s uniesal gaitation fomula eads F 3G M ma( e 4 c (7) ) Fo the poblem of gaitational defection of a photon obit aound the Sun, the impoed Newton s uniesal gaitation fomula eads F.5 4 (8) whee: is the shotest distance between the light and the Sun, if the light and the Sun is tangent, it is equal to the adius of the Sun. The funny thing is that, fo this poblem, the maximum gaitational foce gien by the impoed

14 Newton s uniesal gaitation fomula is.5 times of that gien by the oiginal Newton s law of gaity. Although the deflection angles gien by Eq. (6) and Eq. (8) ae all exactly the same as gien by geneal elatiity, they hae still slight deiations with the pecise astonomical obseations. What ae the easons? The answe is that the deflection angle not only is depended on the gaitational effect of the Sun, but also depended on the gaitational effects of othe celestial bodies, as well as the influences of sunlight pessue and so on. If all factos ae taken into account, not only geneal elatiity can do nothing fo this poblem, but also fo a long time it could not be soled by theoetical method. Theefoe, at pesent the only way to sole this poblem is based on the pecise obseations to deie the synthesized gaitational fomula (including the effects of othe celestial bodies and sunlight pessue) fo the poblem of deflection of photon aound the Sun. As well-known, the deflection angle gien by geneal elatiity o the impoed Newton's fomula of uniesal gaitation is as follows =.75 Adding an additional tem to Eq.(8), it gies the synthesized gaitational fomula between the photon and the Sun as follows GMp wg M p F ( ) (9) c c whee: w is a constant to be detemined. Figue. Deflection of photon aound the Sun Now We Detemine The Value Of W Accoding To Accuate Expeimental Data. Fistly the poblem of deflection of photon aound the Sun as shown in Fig. will be soled with Eq.(9). The method to be used is the same as pesented in efeences [] and [3].

15 Supposing that m epesents the mass of photon. Because the deflection angle is ey small, we can assume that x= ; thus on point (x, y), its coodinate can be witten as (,y), then the foce acted on photon eads F x F (3) / ( y ) Whee: The alue of F is gien by Eq.(9). Because m x F dt x F x dy y c F dy x (3) Hence GM dy 6G M p dy x c 3 3 ( y ) c ( y ) / 5/ 3 3 wg M p 5 c dy 7 ( y ) / (3) Because dy 3 ( y ) /, Theefoe dy ( 5/ 4 y ) 3, dy 8 ( 7/ y ) 5 6 GM 4G M p 6wG M p x c c 5c 3 3 Because tg x c By using the half nomal chod gien in efeence [], it gies

16 c p GM Then the deflection angle is as follows 4GM c w 5 (33) Whee: is the adius of Sun. Because 4 GM c (34) Then, it gies w ( ) 5 (35) Thus the alue of w can be soled as follows w 5 ( ) (36) Now we can detemine the alue of w accoding to the expeimental data. Table shows the expeimental data of adio astonomy fo the deflection angle of photon aound the Sun (taken fom efeence [4]). Table. The expeimental data of adio astonomy fo the deflection angle of photon aound the Sun Yea Obsee Obseed alue / 969 G.A.Seielstud et al.77±. 969 D.O.Muhleman et al I.I.Shapio.8±. 97 R.A.Samak.57±.8 97 J.M.Hill.87± ± ± ±.

17 Now we choose the expeimental data in 975, it gies.76 φ.8 Then, we hae.857 w.4857 Taking the aeage alue, it gies w=.574 Thus, accoding to the expeimental data, the synthesized gaitational fomula can be decided. 4 Contadiction between the Law of Conseation Of Enegy and the Law of Conseation Of Momentum As Well As the Law of Conseation of Angula Momentum As well-known, unlike the law of conseation of enegy, the law of conseation of momentum and the law of conseation of angula momentum ae only coect unde cetain conditions. Fo example, consideing fiction foce and the like, these two laws will not be coect. Now we point out futhe that fo NNM the law of conseation of momentum as well as the law of conseation of angula momentum will be not coect unde cetain conditions (o thei esults contadict with the law of conseation of enegy). As well-known, in ode to poe the law of conseation of momentum as well as the law of conseation of angula momentum, the oiginal Newton's second law should be applied. Howee, as we hae made clea, the oiginal Newton's second law will not be coect unde cetain conditions, fo such cases, these two laws also will not coect. Hee we find anothe poblem, if the oiginal thee conseation laws ae all coect, theefoe fo cetain issues, the law of conseation of enegy and the othe two conseation laws could be combined to apply. While fo NNM, if the othe two conseation laws cannot be applied, how to complement the new fomulas to eplace these two conseation laws? The solution is ey simple: accoding to the law of conseation of enegy, fo any time, the deiaties of total enegy W (t) should be all equal to zeo, then we hae n d W ( t) n dt n,,3, (37) In addition, unning the integal opeations to the both sides of Eq.(3), it gies

18 W ( ) t = W( t) dt t (38) Now we illustate that, because thee is one tuth only, een within the scope of oiginal classical mechanics, the contadiction could also appea between the law of conseation of enegy and the law of conseation of momentum. As shown in Fig.3, a man walks along the ca located on the hoizontal smooth ail, the length of the ca equals L, the mass of the man is m and the ca is m. At beginning the man and the ca ae all at est, then the man walks fom one end to the othe end of the ca, ty to decide the moing distances of the man and the ca. This example is taken fom efeences [5]. Figue 3 A Man Walks along the Ca Located On the Hoizontal Smooth Rail As soling this poblem by using the oiginal classical mechanics, the law of conseation of momentum will be used, it gies m m Howee, at beginning the man and the ca ae all at est, the total enegy of the system is equal to zeo; while once they ae moing, they will hae speeds, and the total enegy of the system is not equal to zeo; thus the law of conseation of enegy will be destoyed. Fo this paadox, the oiginal classical mechanics looks without seeing. In fact, consideing the lost enegy of the man and applying the law of conseation of enegy, the completely diffeent esult will be eached. As the oiginal law of conseation of momentum ( t Const ) and the law of conseation of angula momentum ( L t L Const ) ae not coect, we can popose thei impoed foms of aiable dimension factal. The impoed law of conseation of momentum: constant o a aiable), and the impoed law of conseation of angula momentum: t ( is a L L t

19 ( is a constant o a aiable). Refeences. Fu Yuhua, Deiing Impoed Newton s Second Law and the Law of Gaity at One Time with Fom of Factal Fomula, Engineeing Science. 3,Vol.5,No.6, Fu Yuhua, Impoed Newton s fomula of uniesal gaitation, Zianzazhi (Natue Jounal), (), C. Kittel et al, Tanslated into Chinese by Chen Bingqian et al, Mechanics, Beijing: Science ess, 979, Liu Liao, Geneal elatiity, Beijing: Highe education pess, 987, 5. Xu Hexing, Mechanics (eised edition), Shanghai: East China Nomal Uniesity ess, 998, 为了对自由落体问题真正导出原有的万有引力定律, 需要考虑小球从 A 点自由下落一段极短距离 Z, 到达端点 时 ( 图中未画出 ) 的情况 在导出原有的牛顿第二定律时, 我们已经得到 GM [ D ( R H Z) ( R H ) ' D D 式中 : R H Z O ' 由于 Z 极短, 在此区间引力可视为线性变化, 所以在此区间引力所做功 W 为 W F a Z R H Z) ( D Z 式中, F 为区间 Z 的引力平均值, 亦即区间中点的引力值 a 略去 Z 的二次项可得 W ( R H Z RH RZ HZ ) D/ 当小球下落至区间 Z 的端点 时, 其动能为 m ' D D ( R H ) ( R H Z) [ D ( R H RH RZ HZ) 根据能量守恒定律, 应有 W m' ] D ]

20 对比有关的公式, 可以得到下面的三个等式 D D / D Z ( R H ) D ( R H Z) D 从这三个等式都可以得到 D 于是我们就根据能量守恒定律导出了原有的万有引力定律

Errors in Nobel Prize for Physics (3) Conservation of Energy Leads to Probability Conservation of Parity, Momentum and so on

Errors in Nobel Prize for Physics (3) Conservation of Energy Leads to Probability Conservation of Parity, Momentum and so on Eos in Nobel ize fo hysics (3) Conseation of Enegy Leads to obability Conseation of aity, Momentum and so on Fu Yuhua (CNOOC Reseach Institute, E-mail:fuyh945@sina.com) Abstact: One of the easons fo 957

More information

Expanding Newton Mechanics with Neutrosophy and Quadstage Method New Newton Mechanics Taking Law of. Conservation of Energy as Unique Source Law

Expanding Newton Mechanics with Neutrosophy and Quadstage Method New Newton Mechanics Taking Law of. Conservation of Energy as Unique Source Law Neutosophic Sets and Systems, Vol. 3, 4 3 Epanding Newton Mechanics with Neutosophy and Quadstage Method New Newton Mechanics Taking Law of Conseation of Enegy as Unique Souce Law Fu Yuhua CNOOC Reseach

More information

New Newton Mechanics Taking Law of Conservation of Energy as Unique Source Law (Revised Version 3)

New Newton Mechanics Taking Law of Conservation of Energy as Unique Source Law (Revised Version 3) New Newton Mechanics Taking Law of Conseation of Enegy as Unique Souce Law eised Vesion 3 u Yuhua CNOOC eseach Institute E-mail: fuyh945@sina.com Abstact: Accoding to the pinciple of the uniqueness of

More information

New Newton Mechanics Taking Law of Conservation of Energy as Unique Source Law

New Newton Mechanics Taking Law of Conservation of Energy as Unique Source Law Science Jonal of hysics ISSN: 76-6367 http://www.sjpb.og Atho(s 5. CC Attibtion 3. License. Reseach Aticle blished By Science Jonal blication Intenational Open Access blishe New Newton Mechanics Taking

More information

Solving Problems of Advance of Mercury s Perihelion and Deflection of. Photon Around the Sun with New Newton s Formula of Gravity

Solving Problems of Advance of Mercury s Perihelion and Deflection of. Photon Around the Sun with New Newton s Formula of Gravity Solving Poblems of Advance of Mecuy s Peihelion and Deflection of Photon Aound the Sun with New Newton s Fomula of Gavity Fu Yuhua (CNOOC Reseach Institute, E-mail:fuyh945@sina.com) Abstact: Accoding to

More information

r cos, and y r sin with the origin of coordinate system located at

r cos, and y r sin with the origin of coordinate system located at Lectue 3-3 Kinematics of Rotation Duing ou peious lectues we hae consideed diffeent examples of motion in one and seeal dimensions. But in each case the moing object was consideed as a paticle-like object,

More information

rt () is constant. We know how to find the length of the radius vector by r( t) r( t) r( t)

rt () is constant. We know how to find the length of the radius vector by r( t) r( t) r( t) Cicula Motion Fom ancient times cicula tajectoies hae occupied a special place in ou model of the Uniese. Although these obits hae been eplaced by the moe geneal elliptical geomety, cicula motion is still

More information

DYNAMICS OF UNIFORM CIRCULAR MOTION

DYNAMICS OF UNIFORM CIRCULAR MOTION Chapte 5 Dynamics of Unifom Cicula Motion Chapte 5 DYNAMICS OF UNIFOM CICULA MOTION PEVIEW An object which is moing in a cicula path with a constant speed is said to be in unifom cicula motion. Fo an object

More information

Chap13. Universal Gravitation

Chap13. Universal Gravitation Chap13. Uniesal Gaitation Leel : AP Physics Instucto : Kim 13.1 Newton s Law of Uniesal Gaitation - Fomula fo Newton s Law of Gaitation F g = G m 1m 2 2 F21 m1 F12 12 m2 - m 1, m 2 is the mass of the object,

More information

AP Physics 1 - Circular Motion and Gravitation Practice Test (Multiple Choice Section) Answer Section

AP Physics 1 - Circular Motion and Gravitation Practice Test (Multiple Choice Section) Answer Section AP Physics 1 - Cicula Motion and Gaitation Pactice est (Multiple Choice Section) Answe Section MULIPLE CHOICE 1. B he centipetal foce must be fiction since, lacking any fiction, the coin would slip off.

More information

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE.

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE. Unit 6 actice Test 1. Which one of the following gaphs best epesents the aiation of the kinetic enegy, KE, and of the gaitational potential enegy, GE, of an obiting satellite with its distance fom the

More information

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE.

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE. Unit 6 actice Test 1. Which one of the following gaphs best epesents the aiation of the kinetic enegy, KE, and of the gaitational potential enegy, GE, of an obiting satellite with its distance fom the

More information

ESTIMATION MODELS USING MATHEMATICAL CONCEPTS AND NEWTON S LAWS FOR CONIC SECTION TRAJECTORIES ON EARTH S SURFACE

ESTIMATION MODELS USING MATHEMATICAL CONCEPTS AND NEWTON S LAWS FOR CONIC SECTION TRAJECTORIES ON EARTH S SURFACE Fundamental Jounal of Mathematical Physics Vol. 3 Issue 1 13 Pages 33-44 Published online at http://www.fdint.com/ ESTIMATION MODELS USING MATHEMATICAL CONCEPTS AND NEWTON S LAWS FOR CONIC SECTION TRAJECTORIES

More information

ENGI 4430 Non-Cartesian Coordinates Page xi Fy j Fzk from Cartesian coordinates z to another orthonormal coordinate system u, v, ˆ i ˆ ˆi

ENGI 4430 Non-Cartesian Coordinates Page xi Fy j Fzk from Cartesian coordinates z to another orthonormal coordinate system u, v, ˆ i ˆ ˆi ENGI 44 Non-Catesian Coodinates Page 7-7. Conesions between Coodinate Systems In geneal, the conesion of a ecto F F xi Fy j Fzk fom Catesian coodinates x, y, z to anothe othonomal coodinate system u,,

More information

Newton s Laws, Kepler s Laws, and Planetary Orbits

Newton s Laws, Kepler s Laws, and Planetary Orbits Newton s Laws, Keple s Laws, and Planetay Obits PROBLEM SET 4 DUE TUESDAY AT START OF LECTURE 28 Septembe 2017 ASTRONOMY 111 FALL 2017 1 Newton s & Keple s laws and planetay obits Unifom cicula motion

More information

Projection Gravitation, a Projection Force from 5-dimensional Space-time into 4-dimensional Space-time

Projection Gravitation, a Projection Force from 5-dimensional Space-time into 4-dimensional Space-time Intenational Jounal of Physics, 17, Vol. 5, No. 5, 181-196 Available online at http://pubs.sciepub.com/ijp/5/5/6 Science and ducation Publishing DOI:1.1691/ijp-5-5-6 Pojection Gavitation, a Pojection Foce

More information

On the integration of the equations of hydrodynamics

On the integration of the equations of hydrodynamics Uebe die Integation de hydodynamischen Gleichungen J f eine u angew Math 56 (859) -0 On the integation of the equations of hydodynamics (By A Clebsch at Calsuhe) Tanslated by D H Delphenich In a pevious

More information

Circular Motion. x-y coordinate systems. Other coordinates... PHY circular-motion - J. Hedberg

Circular Motion. x-y coordinate systems. Other coordinates... PHY circular-motion - J. Hedberg Cicula Motion PHY 207 - cicula-motion - J. Hedbeg - 2017 x-y coodinate systems Fo many situations, an x-y coodinate system is a geat idea. Hee is a map on Manhattan. The steets ae laid out in a ectangula

More information

The study of the motion of a body along a general curve. the unit vector normal to the curve. Clearly, these unit vectors change with time, u ˆ

The study of the motion of a body along a general curve. the unit vector normal to the curve. Clearly, these unit vectors change with time, u ˆ Section. Cuilinea Motion he study of the motion of a body along a geneal cue. We define u ˆ û the unit ecto at the body, tangential to the cue the unit ecto nomal to the cue Clealy, these unit ectos change

More information

Physics 2A Chapter 10 - Moment of Inertia Fall 2018

Physics 2A Chapter 10 - Moment of Inertia Fall 2018 Physics Chapte 0 - oment of netia Fall 08 The moment of inetia of a otating object is a measue of its otational inetia in the same way that the mass of an object is a measue of its inetia fo linea motion.

More information

A New Approach to General Relativity

A New Approach to General Relativity Apeion, Vol. 14, No. 3, July 7 7 A New Appoach to Geneal Relativity Ali Rıza Şahin Gaziosmanpaşa, Istanbul Tukey E-mail: aizasahin@gmail.com Hee we pesent a new point of view fo geneal elativity and/o

More information

Determining solar characteristics using planetary data

Determining solar characteristics using planetary data Detemining sola chaacteistics using planetay data Intoduction The Sun is a G-type main sequence sta at the cente of the Sola System aound which the planets, including ou Eath, obit. In this investigation

More information

Circular Orbits. and g =

Circular Orbits. and g = using analyse planetay and satellite motion modelled as unifom cicula motion in a univesal gavitation field, a = v = 4π and g = T GM1 GM and F = 1M SATELLITES IN OBIT A satellite is any object that is

More information

B. Spherical Wave Propagation

B. Spherical Wave Propagation 11/8/007 Spheical Wave Popagation notes 1/1 B. Spheical Wave Popagation Evey antenna launches a spheical wave, thus its powe density educes as a function of 1, whee is the distance fom the antenna. We

More information

Physics 181. Assignment 4

Physics 181. Assignment 4 Physics 181 Assignment 4 Solutions 1. A sphee has within it a gavitational field given by g = g, whee g is constant and is the position vecto of the field point elative to the cente of the sphee. This

More information

PROJECTILE MOTION. At any given point in the motion, the velocity vector is always a tangent to the path.

PROJECTILE MOTION. At any given point in the motion, the velocity vector is always a tangent to the path. PROJECTILE MOTION A pojectile is any object that has been thown though the ai. A foce must necessaily set the object in motion initially but, while it is moing though the ai, no foce othe than gaity acts

More information

7.2. Coulomb s Law. The Electric Force

7.2. Coulomb s Law. The Electric Force Coulomb s aw Recall that chaged objects attact some objects and epel othes at a distance, without making any contact with those objects Electic foce,, o the foce acting between two chaged objects, is somewhat

More information

OSCILLATIONS AND GRAVITATION

OSCILLATIONS AND GRAVITATION 1. SIMPLE HARMONIC MOTION Simple hamonic motion is any motion that is equivalent to a single component of unifom cicula motion. In this situation the velocity is always geatest in the middle of the motion,

More information

Chapter 13 Gravitation

Chapter 13 Gravitation Chapte 13 Gavitation In this chapte we will exploe the following topics: -Newton s law of gavitation, which descibes the attactive foce between two point masses and its application to extended objects

More information

Between any two masses, there exists a mutual attractive force.

Between any two masses, there exists a mutual attractive force. YEAR 12 PHYSICS: GRAVITATION PAST EXAM QUESTIONS Name: QUESTION 1 (1995 EXAM) (a) State Newton s Univesal Law of Gavitation in wods Between any two masses, thee exists a mutual attactive foce. This foce

More information

MODULE 5 ADVANCED MECHANICS GRAVITATIONAL FIELD: MOTION OF PLANETS AND SATELLITES VISUAL PHYSICS ONLINE

MODULE 5 ADVANCED MECHANICS GRAVITATIONAL FIELD: MOTION OF PLANETS AND SATELLITES VISUAL PHYSICS ONLINE VISUAL PHYSICS ONLIN MODUL 5 ADVANCD MCHANICS GRAVITATIONAL FILD: MOTION OF PLANTS AND SATLLITS SATLLITS: Obital motion of object of mass m about a massive object of mass M (m

More information

Theoretical Competition:Solution Question 1 Page 1 of 8. I. Solution Q1_THEORY_SOLUTION_1700_SENT_TO_LEADER.DOCX. r 2. r 1

Theoretical Competition:Solution Question 1 Page 1 of 8. I. Solution Q1_THEORY_SOLUTION_1700_SENT_TO_LEADER.DOCX. r 2. r 1 Q_THEOY_SOLUTION_7_SENT_TO_LEADE.DOCX Theoetical Competition:Solution Question Page of 8 I. Solution M O m. Let O be thei cente of mass. Hence M m () m M GMm GMm () G M m Fom Eq. (), o using educed mass,

More information

1 Dark Cloud Hanging over Twentieth Century Physics

1 Dark Cloud Hanging over Twentieth Century Physics We ae Looking fo Moden Newton by Caol He, Bo He, and Jin He http://www.galaxyanatomy.com/ Wuhan FutueSpace Scientific Copoation Limited, Wuhan, Hubei 430074, China E-mail: mathnob@yahoo.com Abstact Newton

More information

Math Notes on Kepler s first law 1. r(t) kp(t)

Math Notes on Kepler s first law 1. r(t) kp(t) Math 7 - Notes on Keple s fist law Planetay motion and Keple s Laws We conside the motion of a single planet about the sun; fo simplicity, we assign coodinates in R 3 so that the position of the sun is

More information

3.3 Centripetal Force

3.3 Centripetal Force 3.3 Centipetal Foce Think of a time when ou wee a passenge in a ca going aound a shap cue at high speed (Figue 1). If the ca wee going fast enough, ou might feel the side of the ca doo pushing on ou side.

More information

Uniform Circular Motion

Uniform Circular Motion Unifom Cicula Motion Intoduction Ealie we defined acceleation as being the change in velocity with time: a = v t Until now we have only talked about changes in the magnitude of the acceleation: the speeding

More information

Chapter 12. Kinetics of Particles: Newton s Second Law

Chapter 12. Kinetics of Particles: Newton s Second Law Chapte 1. Kinetics of Paticles: Newton s Second Law Intoduction Newton s Second Law of Motion Linea Momentum of a Paticle Systems of Units Equations of Motion Dynamic Equilibium Angula Momentum of a Paticle

More information

ASTR415: Problem Set #6

ASTR415: Problem Set #6 ASTR45: Poblem Set #6 Cuan D. Muhlbege Univesity of Mayland (Dated: May 7, 27) Using existing implementations of the leapfog and Runge-Kutta methods fo solving coupled odinay diffeential equations, seveal

More information

History of Astronomy - Part II. Tycho Brahe - An Observer. Johannes Kepler - A Theorist

History of Astronomy - Part II. Tycho Brahe - An Observer. Johannes Kepler - A Theorist Histoy of Astonomy - Pat II Afte the Copenican Revolution, astonomes stived fo moe obsevations to help bette explain the univese aound them Duing this time (600-750) many majo advances in science and astonomy

More information

Version 1.0. klm. General Certificate of Education June Mathematics. Mechanics 2B. Mark Scheme

Version 1.0. klm. General Certificate of Education June Mathematics. Mechanics 2B. Mark Scheme Vesion.0 klm Geneal Cetificate of Education June 00 Mathematics MMB Mechanics B Mak Scheme Mak schemes ae pepaed by the Pincipal Examine and consideed, togethe with the eleant questions, by a panel of

More information

Answers to test yourself questions

Answers to test yourself questions Answes to test youself questions opic. Cicula motion π π a he angula speed is just ω 5. 7 ad s. he linea speed is ω 5. 7 3. 5 7. 7 m s.. 4 b he fequency is f. 8 s.. 4 3 a f. 45 ( 3. 5). m s. 3 a he aeage

More information

Motion in a Plane Uniform Circular Motion

Motion in a Plane Uniform Circular Motion Lectue 11 Chapte 8 Physics I Motion in a Plane Unifom Cicula Motion Couse website: http://faculty.uml.edu/andiy_danylo/teaching/physicsi PHYS.1410 Lectue 11 Danylo Depatment of Physics and Applied Physics

More information

Universal Gravitation

Universal Gravitation Chapte 1 Univesal Gavitation Pactice Poblem Solutions Student Textbook page 580 1. Conceptualize the Poblem - The law of univesal gavitation applies to this poblem. The gavitational foce, F g, between

More information

Class #16 Monday, March 20, 2017

Class #16 Monday, March 20, 2017 D. Pogo Class #16 Monday, Mach 0, 017 D Non-Catesian Coodinate Systems A point in space can be specified by thee numbes:, y, and z. O, it can be specified by 3 diffeent numbes:,, and z, whee = cos, y =

More information

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session.

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session. - 5 - TEST 1R This is the epeat vesion of TEST 1, which was held duing Session. This epeat test should be attempted by those students who missed Test 1, o who wish to impove thei mak in Test 1. IF YOU

More information

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1 Please ead this fist... AST S: The oigin and evolution of the Univese Intoduction to Mathematical Handout This is an unusually long hand-out and one which uses in places mathematics that you may not be

More information

10. Universal Gravitation

10. Universal Gravitation 10. Univesal Gavitation Hee it is folks, the end of the echanics section of the couse! This is an appopiate place to complete the study of mechanics, because with his Law of Univesal Gavitation, Newton

More information

Physics 201, Lecture 6

Physics 201, Lecture 6 Physics 201, Lectue 6 Today s Topics q Unifom Cicula Motion (Section 4.4, 4.5) n Cicula Motion n Centipetal Acceleation n Tangential and Centipetal Acceleation q Relatie Motion and Refeence Fame (Sec.

More information

Lab 10: Newton s Second Law in Rotation

Lab 10: Newton s Second Law in Rotation Lab 10: Newton s Second Law in Rotation We can descibe the motion of objects that otate (i.e. spin on an axis, like a popelle o a doo) using the same definitions, adapted fo otational motion, that we have

More information

F g. = G mm. m 1. = 7.0 kg m 2. = 5.5 kg r = 0.60 m G = N m 2 kg 2 = = N

F g. = G mm. m 1. = 7.0 kg m 2. = 5.5 kg r = 0.60 m G = N m 2 kg 2 = = N Chapte answes Heinemann Physics 4e Section. Woked example: Ty youself.. GRAVITATIONAL ATTRACTION BETWEEN SMALL OBJECTS Two bowling balls ae sitting next to each othe on a shelf so that the centes of the

More information

Duality between Statical and Kinematical Engineering Systems

Duality between Statical and Kinematical Engineering Systems Pape 00, Civil-Comp Ltd., Stiling, Scotland Poceedings of the Sixth Intenational Confeence on Computational Stuctues Technology, B.H.V. Topping and Z. Bittna (Editos), Civil-Comp Pess, Stiling, Scotland.

More information

Chapter 2: Basic Physics and Math Supplements

Chapter 2: Basic Physics and Math Supplements Chapte 2: Basic Physics and Math Supplements Decembe 1, 215 1 Supplement 2.1: Centipetal Acceleation This supplement expands on a topic addessed on page 19 of the textbook. Ou task hee is to calculate

More information

Graphs of Sine and Cosine Functions

Graphs of Sine and Cosine Functions Gaphs of Sine and Cosine Functions In pevious sections, we defined the tigonometic o cicula functions in tems of the movement of a point aound the cicumfeence of a unit cicle, o the angle fomed by the

More information

06 - ROTATIONAL MOTION Page 1 ( Answers at the end of all questions )

06 - ROTATIONAL MOTION Page 1 ( Answers at the end of all questions ) 06 - ROTATIONAL MOTION Page ) A body A of mass M while falling vetically downwads unde gavity beaks into two pats, a body B of mass ( / ) M and a body C of mass ( / ) M. The cente of mass of bodies B and

More information

Physics 111. Ch 12: Gravity. Newton s Universal Gravity. R - hat. the equation. = Gm 1 m 2. F g 2 1. ˆr 2 1. Gravity G =

Physics 111. Ch 12: Gravity. Newton s Universal Gravity. R - hat. the equation. = Gm 1 m 2. F g 2 1. ˆr 2 1. Gravity G = ics Announcements day, embe 9, 004 Ch 1: Gavity Univesal Law Potential Enegy Keple s Laws Ch 15: Fluids density hydostatic equilibium Pascal s Pinciple This week s lab will be anothe physics wokshop -

More information

FARADAY'S LAW dt

FARADAY'S LAW dt FAADAY'S LAW 31.1 Faaday's Law of Induction In the peious chapte we leaned that electic cuent poduces agnetic field. Afte this ipotant discoey, scientists wondeed: if electic cuent poduces agnetic field,

More information

Mechanics Physics 151

Mechanics Physics 151 Mechanics Physics 151 Lectue 5 Cental Foce Poblem (Chapte 3) What We Did Last Time Intoduced Hamilton s Pinciple Action integal is stationay fo the actual path Deived Lagange s Equations Used calculus

More information

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once.

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once. Honos Physics Fall, 2016 Cicula Motion & Toque Test Review Name: M. Leonad Instuctions: Complete the following woksheet. SHOW ALL OF YOUR WORK ON A SEPARATE SHEET OF PAPER. 1. Detemine whethe each statement

More information

4. Two and Three Dimensional Motion

4. Two and Three Dimensional Motion 4. Two and Thee Dimensional Motion 1 Descibe motion using position, displacement, elocity, and acceleation ectos Position ecto: ecto fom oigin to location of the object. = x i ˆ + y ˆ j + z k ˆ Displacement:

More information

Physics 2B Chapter 22 Notes - Magnetic Field Spring 2018

Physics 2B Chapter 22 Notes - Magnetic Field Spring 2018 Physics B Chapte Notes - Magnetic Field Sping 018 Magnetic Field fom a Long Staight Cuent-Caying Wie In Chapte 11 we looked at Isaac Newton s Law of Gavitation, which established that a gavitational field

More information

MAGNETIC FIELD INTRODUCTION

MAGNETIC FIELD INTRODUCTION MAGNETIC FIELD INTRODUCTION It was found when a magnet suspended fom its cente, it tends to line itself up in a noth-south diection (the compass needle). The noth end is called the Noth Pole (N-pole),

More information

Thomas J. Osler Mathematics Department, Rowan University, Glassboro NJ 08028,

Thomas J. Osler Mathematics Department, Rowan University, Glassboro NJ 08028, 1 Feb 6, 001 An unusual appoach to Keple s fist law Ameican Jounal of Physics, 69(001), pp. 106-8. Thomas J. Osle Mathematics Depatment, Rowan Univesity, Glassboo NJ 0808, osle@owan.edu Keple s fist law

More information

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS TSOKOS LESSON 6- THE LAW OF GRAVITATION Essential Idea: The Newtonian idea of gavitational foce acting between two spheical bodies and the laws of mechanics

More information

To Feel a Force Chapter 7 Static equilibrium - torque and friction

To Feel a Force Chapter 7 Static equilibrium - torque and friction To eel a oce Chapte 7 Chapte 7: Static fiction, toque and static equilibium A. Review of foce vectos Between the eath and a small mass, gavitational foces of equal magnitude and opposite diection act on

More information

Ch04: Motion in two and three dimensions (2D and 3D)

Ch04: Motion in two and three dimensions (2D and 3D) Ch4: Motion in two and thee dimensions (D and 3D) Displacement, elocity and acceleation ectos Pojectile motion Cicula motion Relatie motion 4.: Position and displacement Position of an object in D o 3D

More information

Chapter 5 Force and Motion

Chapter 5 Force and Motion Chapte 5 Foce and Motion In chaptes 2 and 4 we have studied kinematics i.e. descibed the motion of objects using paametes such as the position vecto, velocity and acceleation without any insights as to

More information

= 4 3 π( m) 3 (5480 kg m 3 ) = kg.

= 4 3 π( m) 3 (5480 kg m 3 ) = kg. CHAPTER 11 THE GRAVITATIONAL FIELD Newton s Law of Gavitation m 1 m A foce of attaction occus between two masses given by Newton s Law of Gavitation Inetial mass and gavitational mass Gavitational potential

More information

1131 T Question 1

1131 T Question 1 1131 T1 2008 Question 1 ( aks) You ae cycling, on a long staight path, at a constant speed of 6.0.s 1. Anothe cyclist passes you, taelling on the sae path in the sae diection as you, at a constant speed

More information

Physics 107 TUTORIAL ASSIGNMENT #8

Physics 107 TUTORIAL ASSIGNMENT #8 Physics 07 TUTORIAL ASSIGNMENT #8 Cutnell & Johnson, 7 th edition Chapte 8: Poblems 5,, 3, 39, 76 Chapte 9: Poblems 9, 0, 4, 5, 6 Chapte 8 5 Inteactive Solution 8.5 povides a model fo solving this type

More information

Force between two parallel current wires and Newton s. third law

Force between two parallel current wires and Newton s. third law Foce between two paallel cuent wies and Newton s thid law Yannan Yang (Shanghai Jinjuan Infomation Science and Technology Co., Ltd.) Abstact: In this pape, the essence of the inteaction between two paallel

More information

Discover the answer to this question in this chapter.

Discover the answer to this question in this chapter. In a oto ide such as the one shown in the figue, what is the maximum peiod of otation that the oto ide can hae so that people do not slip down the wall if the coefficient of fiction between the wall and

More information

Physics: Work & Energy Beyond Earth Guided Inquiry

Physics: Work & Energy Beyond Earth Guided Inquiry Physics: Wok & Enegy Beyond Eath Guided Inquiy Elliptical Obits Keple s Fist Law states that all planets move in an elliptical path aound the Sun. This concept can be extended to celestial bodies beyond

More information

Chapter 7 Rotational Motion and the Law of Gravity

Chapter 7 Rotational Motion and the Law of Gravity Chapte 7 Rotational Motion and the Law of Gaity What is a Rigid Body? Rotational Kinematics Angula Velocity ω and Acceleation α Unifom Rotational Motion: Kinematics Unifom Cicula Motion: Kinematics and

More information

PHYSICS 1210 Exam 2 University of Wyoming 14 March ( Day!) points

PHYSICS 1210 Exam 2 University of Wyoming 14 March ( Day!) points PHYSICS 1210 Exam 2 Univesity of Wyoming 14 Mach ( Day!) 2013 150 points This test is open-note and closed-book. Calculatos ae pemitted but computes ae not. No collaboation, consultation, o communication

More information

Chapters 5-8. Dynamics: Applying Newton s Laws

Chapters 5-8. Dynamics: Applying Newton s Laws Chaptes 5-8 Dynamics: Applying Newton s Laws Systems of Inteacting Objects The Fee Body Diagam Technique Examples: Masses Inteacting ia Nomal Foces Masses Inteacting ia Tensions in Ropes. Ideal Pulleys

More information

Faraday s Law. Faraday s Law. Faraday s Experiments. Faraday s Experiments. Magnetic Flux. Chapter 31. Law of Induction (emf( emf) Faraday s Law

Faraday s Law. Faraday s Law. Faraday s Experiments. Faraday s Experiments. Magnetic Flux. Chapter 31. Law of Induction (emf( emf) Faraday s Law Faaday s Law Faaday s Epeiments Chapte 3 Law of nduction (emf( emf) Faaday s Law Magnetic Flu Lenz s Law Geneatos nduced Electic fields Michael Faaday discoeed induction in 83 Moing the magnet induces

More information

Shree Datta Coaching Classes, Contact No Circular Motion

Shree Datta Coaching Classes, Contact No Circular Motion Shee Datta Coaching Classes, Contact No. 93698036 Pof. Deepak Jawale Cicula Motion Definition : The motion of the paticle along the cicumfeence of a cicle is called as cicula motion. Eg. i) Motion of eath

More information

Chapter 5 Force and Motion

Chapter 5 Force and Motion Chapte 5 Foce and Motion In Chaptes 2 and 4 we have studied kinematics, i.e., we descibed the motion of objects using paametes such as the position vecto, velocity, and acceleation without any insights

More information

Gaia s Place in Space

Gaia s Place in Space Gaia s Place in Space The impotance of obital positions fo satellites Obits and Lagange Points Satellites can be launched into a numbe of diffeent obits depending on thei objectives and what they ae obseving.

More information

Chapter 6 Balanced Incomplete Block Design (BIBD)

Chapter 6 Balanced Incomplete Block Design (BIBD) Chapte 6 Balanced Incomplete Bloc Design (BIBD) The designs lie CRD and RBD ae the complete bloc designs We now discuss the balanced incomplete bloc design (BIBD) and the patially balanced incomplete bloc

More information

2018 Physics. Advanced Higher. Finalised Marking Instructions

2018 Physics. Advanced Higher. Finalised Marking Instructions National Qualifications 018 018 Physics Advanced Highe Finalised Making Instuctions Scottish Qualifications Authoity 018 The infomation in this publication may be epoduced to suppot SQA qualifications

More information

Vectors, Vector Calculus, and Coordinate Systems

Vectors, Vector Calculus, and Coordinate Systems Apil 5, 997 A Quick Intoduction to Vectos, Vecto Calculus, and Coodinate Systems David A. Randall Depatment of Atmospheic Science Coloado State Univesity Fot Collins, Coloado 80523. Scalas and vectos Any

More information

TAMPINES JUNIOR COLLEGE 2009 JC1 H2 PHYSICS GRAVITATIONAL FIELD

TAMPINES JUNIOR COLLEGE 2009 JC1 H2 PHYSICS GRAVITATIONAL FIELD TAMPINES JUNIOR COLLEGE 009 JC1 H PHYSICS GRAVITATIONAL FIELD OBJECTIVES Candidates should be able to: (a) show an undestanding of the concept of a gavitational field as an example of field of foce and

More information

Section 6.2: Orbits. Gm r. v = v 2 = Gm r. m = rv2 G. Solution: m = rv2 G ( )( 7.5!10 5 m/s ) 2. = 5.34!1017 m m kg # # m2. kg 2

Section 6.2: Orbits. Gm r. v = v 2 = Gm r. m = rv2 G. Solution: m = rv2 G ( )( 7.5!10 5 m/s ) 2. = 5.34!1017 m m kg # # m2. kg 2 Section 6.2: Obits Mini Inestigation: Exploing Gaity and Obits, page 298 A. When I incease the size of the Sun, Eath s obit changes: the obit is close to the Sun. B. he Moon is pulled out of Eath s obit

More information

Appendix B The Relativistic Transformation of Forces

Appendix B The Relativistic Transformation of Forces Appendix B The Relativistic Tansfomation of oces B. The ou-foce We intoduced the idea of foces in Chapte 3 whee we saw that the change in the fou-momentum pe unit time is given by the expession d d w x

More information

ATM 2012 No reproduction (including Internet) except for legitimate academic purposes for permissions.

ATM 2012 No reproduction (including Internet) except for legitimate academic purposes for permissions. Robet Dixon asks what is the gaity field of a galaxy? and esponds in detail. The obseed patten in disc galaxies fo obital elocities to be the same at all obital adii has often been pesented as a supise

More information

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS LSN 10-: MOTION IN A GRAVITATIONAL FIELD Questions Fom Reading Activity? Gavity Waves? Essential Idea: Simila appoaches can be taken in analyzing electical

More information

EN40: Dynamics and Vibrations. Midterm Examination Thursday March

EN40: Dynamics and Vibrations. Midterm Examination Thursday March EN40: Dynamics and Vibations Midtem Examination Thusday Mach 9 2017 School of Engineeing Bown Univesity NAME: Geneal Instuctions No collaboation of any kind is pemitted on this examination. You may bing

More information

Analysis of high speed machining center spindle dynamic unit structure performance Yuan guowei

Analysis of high speed machining center spindle dynamic unit structure performance Yuan guowei Intenational Confeence on Intelligent Systems Reseach and Mechatonics Engineeing (ISRME 0) Analysis of high speed machining cente spindle dynamic unit stuctue pefomance Yuan guowei Liaoning jidian polytechnic,dan

More information

Torque, Angular Momentum and Rotational Kinetic Energy

Torque, Angular Momentum and Rotational Kinetic Energy Toque, Angula Moentu and Rotational Kinetic Enegy In ou peious exaples that inoled a wheel, like fo exaple a pulley we wee always caeful to specify that fo the puposes of the poble it would be teated as

More information

The Laws of Motion ( ) N SOLUTIONS TO PROBLEMS ! F = ( 6.00) 2 + ( 15.0) 2 N = 16.2 N. Section 4.4. Newton s Second Law The Particle Under a Net Force

The Laws of Motion ( ) N SOLUTIONS TO PROBLEMS ! F = ( 6.00) 2 + ( 15.0) 2 N = 16.2 N. Section 4.4. Newton s Second Law The Particle Under a Net Force SOLUTIONS TO PROBLEMS The Laws of Motion Section 4.3 Mass P4. Since the ca is moving with constant speed and in a staight line, the esultant foce on it must be zeo egadless of whethe it is moving (a) towad

More information

Lab #4: Newton s Second Law

Lab #4: Newton s Second Law Lab #4: Newton s Second Law Si Isaac Newton Reading Assignment: bon: Januay 4, 1643 Chapte 5 died: Mach 31, 1727 Chapte 9, Section 9-7 Intoduction: Potait of Isaac Newton by Si Godfey Knelle http://www.newton.cam.ac.uk/at/potait.html

More information

Chapter 7-8 Rotational Motion

Chapter 7-8 Rotational Motion Chapte 7-8 Rotational Motion What is a Rigid Body? Rotational Kinematics Angula Velocity ω and Acceleation α Unifom Rotational Motion: Kinematics Unifom Cicula Motion: Kinematics and Dynamics The Toque,

More information

The Schwartzchild Geometry

The Schwartzchild Geometry UNIVERSITY OF ROCHESTER The Schwatzchild Geomety Byon Osteweil Decembe 21, 2018 1 INTRODUCTION In ou study of geneal elativity, we ae inteested in the geomety of cuved spacetime in cetain special cases

More information

Fu Yuhua 1. Beijing, China

Fu Yuhua 1. Beijing, China 85 An Example of Guiding Scientific Research with hilosophical rinciples Based on Uniqueness of Truth and Neutrosophy eriing Newton's Second Law and the like Fu Yuhua 1 1 CNOOC Research Institute Beijing,

More information

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS TSOKOS LESSON 10-1 DESCRIBING FIELDS Essential Idea: Electic chages and masses each influence the space aound them and that influence can be epesented

More information

Physics 211: Newton s Second Law

Physics 211: Newton s Second Law Physics 211: Newton s Second Law Reading Assignment: Chapte 5, Sections 5-9 Chapte 6, Section 2-3 Si Isaac Newton Bon: Januay 4, 1643 Died: Mach 31, 1727 Intoduction: Kinematics is the study of how objects

More information

Discover the answer to this question in this chapter.

Discover the answer to this question in this chapter. In a oto ide such as the one shown in the figue, what is the maximum peiod of otation that the oto ide can hae so that people do not slip down the wall if the coefficient of fiction between the wall and

More information

working pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50

working pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50 woking pages fo Paul Richads class notes; do not copy o ciculate without pemission fom PGR 2004/11/3 10:50 CHAPTER7 Solid angle, 3D integals, Gauss s Theoem, and a Delta Function We define the solid angle,

More information

Physics 121 Hour Exam #5 Solution

Physics 121 Hour Exam #5 Solution Physics 2 Hou xam # Solution This exam consists of a five poblems on five pages. Point values ae given with each poblem. They add up to 99 points; you will get fee point to make a total of. In any given

More information