NEWTON S THEORY OF GRAVITY

Size: px
Start display at page:

Download "NEWTON S THEORY OF GRAVITY"

Transcription

1 NEWTON S THEOY OF GAVITY 3 Concptual Qustions 3.. Nwton s thid law tlls us that th focs a qual. Thy a also claly qual whn Nwton s law of gavity is xamind: F / = Gm m has th sam valu whth m = Eath and m = sun o vic vsa. Mm s Mm s 3.. Th foc of th sta on plant is F = G. Th foc of th sta on plant is F = G. Sinc m = m, and =, M ( m ) G s ( ) F = = = F Mm G 4 s Mm Mm 3.3. (a) Th foc of th Eath on th fist satllit is F = G whil F = G. Sinc =, F m 000 kg = = =. F m 000 kg (b) With Fnt = ma, F = ma and F = ma, so, a F m 000 kg = = = a F m 000 kg Th f-fall acclation is th sam fo objcts of diffnt mass Th astonauts can b wightlss at any distanc bcaus an objct is said to b wightlss if it is in f fall (as in obit). Fo th gavitational foc to bcom zo, th spaccaft would hav to b an infinit distanc away Th hamm will not fall to th Eath. Th astonaut, shuttl, and hamm a all in f fall aound th Eath (in an obit), so th hamm has th sam acclation as th astonaut and dos not mov away fom him Th acclation du to gavity is M g = G. With g = 0 m/s, M = M, and =, M ( M ) M g = G = G = G = g = 0 m/s ( ) Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist. 3-

2 3- Chapt Th gavitational potntial ngy is ngativ bcaus w choos to plac th zo point of potntial ngy at infinity ( U = 0). With this choic, th gavitational potntial ngy is ngativ bcaus th consvativ foc of at gavity is attactiv. Th two masss will gain kintic ngy as thy appoach ach oth Th scap spd fom Plant X is v scap X GM X = = 0,000 m/s. Plant Y is twic as dns as Plant X but th sam siz so has twic th mass. Thfo v scap Y X X G( MX) = = vscap X = 4,4 m/s 3.9. Th Eath s nw obital piod would b about.9 yas. Fo cicula obits, Kpl s thid law lats obital 4π 3 piod to adius and can b wittn T =. H M is th mass of th body bing obitd (th Sun in this GM poblm.) Th obital piod is indpndnt of th mass of th obiting body Fo a cicula obit, v = GM/ (Equation 3.). As dcass, v incass, so th satllit spds up as th satllit spials inwad. Exciss and Poblms Sction 3.3 Nwton s Law of Gavity 3.. Modl: Modl th sun (s) and th ath () as sphical masss. Du to th lag diffnc btwn you siz and mass and that of ith th sun o th ath, a human body can b tatd as a paticl. GMsM y GMM y Solv: Fs on you = and F on you = s- Dividing ths two quations givs 30 6 s on y s kg m -4 = = = on y s kg m F M F M 3.. Modl: Assum th two lad balls a sphical masss. Gmm on F on ( N m /kg )(0 kg)(0. 00 kg) 9 Solv: (a) F = = = = N (0. 0 m) (b) Th atio of th abov gavitational foc to th gavitational foc on th 00 g ball is N = (0. 00 kg)(9. 8 m/s ) Assss: Th answ in pat (b) shows how small is th gavitational foc btwn two lad balls spaatd by 0 cm compad to th gavitational foc on th 00 g ball Modl: Modl th sun (s), th moon (m), and th ath () as sphical masss. GMsM m GMM m Solv: Fs on m = and F on m = s-m -m 9 Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

3 Nwton s Thoy of Gavity 3-3 Dividing th two quations and using th astonomical data fom Tabl 3., 30 8 s on m s -m kg m 4 on m s-m kg m F M = = =. 8 F M Not that th sun-moon distanc is not noticably diffnt fom th tabulatd sun-ath distanc Solv: F sph on paticl Dividing th two quations, GM M GM M = = s p p and F ath on paticl s-p 6 sph on paticl s 5900 kg m -7 = = =. ath on paticl s-p kg m F M F M 3.5. Modl: Modl th woman (w) and th man (m) as sphical masss o paticls. Solv: F - GM wm m. w on m Fm on w m-w (. 0 m) ( N m /kg )(50 kg)(70 kg) -7 = = = =. 3 0 N 3.6. Modl: Modl th ath () as a sph Th spac shuttl o a.0 kg sph (s) in th spac shuttl is + s = m m = m away fom th cnt of th ath. Solv: (a) 4 GMMs on s 6 ( + s) ( m) F ( N m /kg )( kg)(. 0 kg) = = = 9. 0 N Sction 3.4 Littl g and Big G 3.7. Modl: Modl th sun (s) as a sphical mass. 30 GMs.. gsun sufac 8 s ( m) - 30 GMs ( N m /kg )( kg) sun at ath s- ( m) Solv: (a) (b) g ( N m /kg )( 99 0 kg) = = = 74 m/s -3 = = = m/s 3.8. Modl: Modl th moon (m) and Jupit (J) as sphical masss. Solv: (a) g GM m.. moon sufac 6 m ( m) ( N m /kg )( kg) = = =. 6 m/s Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

4 3-4 Chapt 3 (b) g 7 GM J.. Jupit sufac 7 J ( m) ( N m /kg )( 90 0 kg) = = = 5. 9 m/s 3.9. Modl: Modl th ath () as a sphical mass. Th acclation du to gavity at sa lvl is Tabl 3.) m/s (s Tabl 3.) and = m (s 6 Solv: H g GM GM g = = = = ( ) m/s ath gobsvatoy ( + h) ( + h / ) ( + h / ) ath GM/ = is th acclation du to gavity on a non-otating ath, which is why w v usd th valu m/s. Solving fo h, h= =. 4 km Modl: Modl th ath () as a sphical mass. Solv: Lt th acclation du to gavity b 30g. whn th ath is shunk to a adius of x. Thn, g sufac sufac GM GM = = and 3.0g sufac x 3 GM GM = = = x x. Th ath s adius would nd to b 0.58 tims its psnt valu. 3.. Modl: Modl Plant Z as a sphical mass. Z ( N m /kg ) M Z 4 M 6 Z Z ( m) GM Solv: (a) gz sufac = 8. 0 m/s = = kg (b) Lt h b th hight abov th noth pol. Thus, g GM Z GM Z gz sufac 8. 0 m/s abov N pol 6 Z + h Z + hz + hz = = = = = m/s ( ) ( / ) ( / ) m m Sction 3.5 Gavitational Potntial Engy 3.. Modl: Modl Mas (M) as a sphical mass. Igno ai sistanc. Also consid Mas and th ball as an isolatd systm, so mchanical ngy is consvd. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

5 Nwton s Thoy of Gavity 3-5 Solv: A hight of 5 m is vy small in compaison with th adius of ath o Mas. W can us flat-ath gavitational potntial ngy to find th spd with which th astonaut can thow th ball. On ath, with y i = 0 m and v = 0 m/s, ngy consvation givs f mvf mgyf mvi mgy i vi gyf + = + = = (9. 8 m/s )(5 m) = 7. m/s Engy is also consvd on Mas, but th acclation du to gavity is diffnt. g 3 GM M.. Ma s sufac 6 M ( m) ( N m /kg )(6 4 0 kg) = = = m/s On Mas, with y i = 0 m and v f = 0 m/s, ngy consvation is vi (7. m/s) mv f mgyf mv i mgyi yf g m. + = + = = = 39 m (3 77 m/s ) 3.3. Modl: Modl Jupit as a sphical mass and th objct as a point paticl. Th objct and Jupit fom an isolatd systm, so mchanical ngy is consvd. Th minimum launch spd fo scap, which is calld th scap spd, allows an objct to scap to an infinit distanc fom Jupit (o, in gnal, fom its patn objct). Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

6 3-6 Chapt 3 Solv: Th ngy consvation quation K + U = K+ U is wh J and GM m GM m J o J o mv o = mv o J M J a th adius and mass of Jupit. Using th asymptotic condition v = 0 m/s as, 7 GM Jmo GM J ( N m /kg )( kg) 4 mv o v 7 J J m 0 J = = = = m/s Thus, th scap vlocity fom Jupit is 60. km/s Modl: Modl th ath () as a sphical mass. Compad to th ath s siz and mass, th ockt () is modld as a paticl. This is an isolatd systm, so mchanical ngy is consvd. Solv: Th ngy consvation quation K + U = K+ U is In th psnt cas,, so GM m GM m mv = mv GM m GM mv = mv v= v ( N m /kg )( kg) v = (. 5 0 m/s) = 0 km/s m 3.5. Modl: Th pob and th sun fom an isolatd systm, so mchanical ngy is consvd. Th minimum launch spd fo scap, which is calld th scap spd, allows an objct to scap to an infinit distanc fom th sun, wh th objct will hav slowd to zo spd with spct to th sun. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

7 Nwton s Thoy of Gavity 3-7 W dnot by m p th mass of th pob. M s is th sun s mass, and sun and th pob. Solv: Th consvation of ngy quation K + U = K+ U is GM m mv Using th condition v = 0 m/s asymptotically as, s p s p p- = mv p- s-p s-p is th spaation btwn th cnts of th GM m GM m ( N m /kg )( 99 0 kg) mv 50 0 m - 30 s p GMs.. 4 p scap = vscap = = =. s-p s-p. 4 0 m/s 3.6. Modl: Modl th distant plant (p) and th ath () as sphical masss. Bcaus both a isolatd, th mchanical ngy of th objct on both th plant and th ath is consvd. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

8 3-8 Chapt 3 Lt us dnot th mass of th plant by gavity on th sufac of th plant is M p and that of th ath by and th ath, spctivly. Solv: (a) W a givn that M = M and g = g. Sinc g p p g p and on th sufac of th ath is g. P p 4 GM p GM = and g =, w hav GM GM G( M / ) M. You mass is m 0. Also, acclation du to p and p p 6 7 = = p = =. =. p 4 4 (b) Th consvation of ngy quation K + U = K+ U is Using v = 0 m/s as, w hav mv 0 scap GM m = p 0 p GM m mv p 0 p 0 0 = mv 0 p 8 8( m) 80 0 m GM m 4 p ( ) 4( N m /kg )( kg) scap 7 p p m v a th adii of th plant GM G M = = = = 9. 4 km/s Sction 3.6 Satllit Obits and Engis 3.7. Modl: Modl th sun (s) as a sphical mass and th astoid (a) as a point paticl. Th astoid, having mass m a and vlocity v a, obits th sun in a cicl of adius a. Th astoid s tim piod is T a = 50. ath yas = s. 8 Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

9 Nwton s Thoy of Gavity 3-9 Solv: Th gavitational foc btwn th sun (mass = M ) and th astoid povids th cntiptal acclation quid fo cicula motion. Substituting s a a a s π a s a a a a a Ta 4π GM m m v GM GM T = = = G = N m /kg, a = m. Th vlocity of th astoid in its obit will thfo b s 30 M s = kg, and th tim piod of th astoid, w obtain πa π a T 8 a (4.4 0 m) 4 v = = =.7 0 m/s.58 0 s Solv: W giv th answ to two significant figus bcaus th astoid piod is givn to two significant figus Modl: Modl th sun (s) and th ath () as sphical masss. Th ath obits th sun with vlocity v in a cicula path with a adius dnotd by s-. Th sun s and th ath s masss a dnotd by M s and m, spctivly. Solv: Th gavitational foc povids th cntiptal acclation quid fo cicula motion. M Assss: Th tabulatd valu is isn t xactly cicula. s ( π s-) = = s- s- s-t GM m m v m 3 3 4π s- 4 π ( m) s - GT ( N m /kg )( s) = = =. 0 0 kg kg. Th slight diffnc can b ascibd to th fact that th ath s obit 3.9. Fom Kpl s thid law, th obital piod squad is popotional to th obital adius cubd: T y x 3 3 y (4 x) 64 x (8 x) / Thus, at = 4, T = T. Thfo T = 8T. A ya on Plant Y is 8 00 = 600 ath days long Modl: Modl th sta (s) and th plant (p) as sphical masss. Solv: Fom th plant s acclation du to gavity, w find its mass to b M g p g 6 p p (. m/s )( m) 5 p = = =. G N m /kg y GM = (b) Fom th plant s obital piod, w find th mass of th sta Omga to b M p p 4π T = GM s x 5 0 kg 4π 4 π (. 0 m) 30 = = = 5. 0 kg GT ( N m /kg )( s) s 3.. Modl: Modl th plant and satllits as sphical masss. Plas f to Figu EX3.. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

10 3-0 Chapt 3 3 / Solv: (a) Th piod of a satllit in a cicula obit is T = [4 π /( GM )] This is indpndnt of th satllit s mass, so w can find th atio of th piods of two satllits a and b: T T a b 3 a = b Satllit has =, so T = T= 50 min. Satllit 3 has 3 = (3/), so T 3/ 3 T = (3/) = 459 min. (b) Th foc on a satllit is F = GMm/. Thus th atio of th focs on th two satllits a and b is Satllit has = and m = m, so m = so F = (/3) () F = 4440 N. 3 m, 3 a b a F m = Fb a mb F F = () () = 0,000 N. Similaly, satllit 3 has 3 = (3/) and (c) Th spd of a satllit in a cicula obit is v = ( GM/), so its kintic ngy is atio of th kintic ngy of two satllits a and b is Ka b ma = Kb a mb Satllit 3 has 3 = (3/) and m 3 = m, so K/ K 3 = (3/)(/) = 3/ =. 50. K = mv = GMm/. Thus th 3.. Modl: Modl th sun (S) as a sphical mass and th satllit (s) as a point paticl. Th satllit, having mass m s and vlocity v s, obits th sun with a mass M S in a cicl of adius s. Solv: Th gavitational foc btwn th sun and th satllit povids th ncssay cntiptal acclation fo cicula motion. Nwton s scond law givs S s msvs = s s GM m Bcaus vs = π s/ Ts wh T s is th piod of th satllit, this quation simplifis to 30 S ( π s) 3 S s ( N m /kg )( kg)( s) 9 = s = = s =. s Ts s 4π 4π GM GM T 9 0 m 3.3. Modl: Modl th ath () as a sphical mass and th satllit (s) as a point paticl. Th satllit has a mass is m s and obits th ath with a vlocity v s. Th adius of th cicula obit is dnotd by s and th mass of th ath by M. Solv: Th satllit xpincs a gavitational foc that povids th cntiptal acclation quid fo cicula motion: 4 s s s.. s s s vs (5500 m/s) 7 πs π(. 3 0 m) 4 Ts = = =. 5 0 s = 4. h vs 5500 m/s GM m m v GM ( N m / kg )( kg) 7 = = = =. 3 0 m 3.4. Modl: Modl Mas (m) as a sphical mass and th satllit (s) as a point paticl. Th gosynchonous satllit whos mass is m s and vlocity is v s obits in a cicl of adius s aound Mas. Lt us dnot mass of Mas by M m. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

11 Nwton s Thoy of Gavity 3- Solv: Th gavitational foc btwn th satllit and Mas povids th cntiptal acclation ndd fo cicula motion: Using G = N m /kg, s 7 = m. Thus, altitud piod, o GM mms msvs ms( π s) GM mt s = = s = s s T s s 4 π 3 M = kg, and T s = (4. 8 hs) = (4. 8)(3600) s = 89,80 s, w obtain s m m 7 = =. 7 0 m. Th spd is th obital cicumfnc dividd by th πs π( m/s) vs = = =. 44 km/s T 89,80 s s 3.5. Solv: W a givn M+ M = 50 kg which mans M= 50 kg M. W also hav 6 6 ( N)(0. 0 m) = N MM = = 4798 kg GM M (0. 0 m) N m /kg Thus, (50 kg M ) M = 4798 kg o M (50 kg) M + (4798 kg ) = 0. Solving this quation givs M = kg and kg. Th two masss a 04 and 46 kg W placd th oigin of th coodinat systm on th 0.0 kg mass ( m ) so that th 5.0 kg mass ( m 3) is on th y-axis and th 0.0 kg mass ( m ) is on th x-axis. 7 /3 Solv: (a) Th focs acting on th 0.0 kg mass ( m ) a Thus th foc is F i i i gmm ˆ ( N m /kg )(0.0 kg)(0.0 kg) ˆ 6 ˆ m on m = = =.33 0 N (0.0 m) gmm 3 ˆ ( N m /kg )(0.0 kg)(5.0 kg) ˆ 7 ˆ m3 on m = = =.67 0 N 3 (0.0 m) 6 Fon m = Fm on m + F ˆ -7 ˆ -6 m on m = i j Fon m = F j j j.33 0 N N.34 0 N 3 ( 6 Fon m ) x.33 0 N θ = tan = tan 83 ( F 7 on m ) =.67 0 N y 6 Fon m =. 3 0 N, 83 cw fom th +y-axis Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

12 3- Chapt 3 (b) Th focs acting on th 5.0 kg mass ( m 3) a 7 F = F =.67 0 ˆj N Thus 3 F m on m m on m 3 3 gmm3 m on m3 3 (0.0 m) + (0.0 m) 8 ˆ 8 m on m = ( N)sin φ ( N) cos 3 ( N m /kg )(0.0 kg)(5.0 kg) 8 = = = N F i φˆj 8 0 cm 8 = ( N) ˆ 0 cm i ( N) ˆj.36 cm.36 cm 8 ˆ 8 = ( N) i ( N) ˆj 8ˆ 7 F = F + F = i N.64 0 ˆj N F 7 m on m m on m m on m on m = ( N) + (.64 0 N) =.84 0 N 3 ( F 8 on m ) x N = tan = tan 7.5 ( F 7 on m ) =.64 0 N 3 y θ 3 F on =. 3 0 N, 7. 5 ccw fom th -y-axis Solv: Th angl θ = tan = Th distanc = = ( m) + (0. 00 m) = m. Th focs 0 on th 0.0 kg mass a Mm F ˆ ˆ = G ( sinθi + cos θ j) Mm F = G (sinθiˆ+ cos θ ˆj) 5 Not m= mand =. Thus, th nt foc on th 0.0 kg mass is Mm F F F G ˆj nt = + = cosθ ( N m /kg )(0. 0 kg)(5. 0 kg)cos(4. 04 ) = ˆ j (0. 06 m) 7 = ˆj N Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

13 Nwton s Thoy of Gavity Solv: Th total gavitational potntial ngy is th sum of th potntial ngis du to th intactions of th pais of masss. U = U + U + U 3 3 mm mm m m = G G G With m m m = 0. 0 kg, = 0. 0 kg, = 5. 0 kg, = 0. 0 m, = 0. 0 m, and 3 = m, 7 U = J Assss: Th gavitational potntial ngy is ngativ bcaus th masss attact ach oth. It is a scala, so th a no vcto calculations quid Solv: Th total gavitational potntial ngy is th sum of th potntial ngis du to th intactions of th pais of masss. U = U + U + U 3 3 mm mm m m = G G G Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

14 3-4 Chapt 3 With m = 0. 0 kg, m = m = 0. 0 kg, = = ( m) + (0. 00 m) = m, and 3 = m, U = J Assss: Th gavitational potntial ngy is ngativ bcaus th masss attact ach oth. It is a scala, so th a no vcto calculations quid Bcaus of th gavitational foc of attaction btwn th lad sphs, th cabls will mak an angl of θ with th vtical. Th distanc btwn th sph cnts is thfo going to b lss than m. Th fbody diagam shows th focs acting on th lad sph. Solv: W can s fom th diagam that th distanc btwn th cnts is d =. 000 m Lsinθ. Each sph is in static quilibium, so Nwton s scond law is F = F Tsinθ = 0 Tsinθ = F x gav F = T cosθ mg = 0 T cosθ = mg Dividing ths two quations to liminat th tnsion T yilds y Fgav Gmm/d Gm sinθ tanθ cosθ = = mg = mg = d g W know that d is going to b only vy, vy slightly lss than.00 m. Th vy slight diffnc is not going to b nough to affct th valu of F gav, th gavitational attaction btwn th two masss, so w ll valuat th ight sid of this quation by using.00 m fo d. This givs ( N m /kg )(00 kg) 0 8 tanθ = = θ = ( ) (. 00 m) (9. 8 m/s ) gav This small angl causs th two sphs to mov clos by th distanc btwn thi cnts is d = m. 7 Lsinθ =. 4 0 m = m. Consquntly, 3.3. W placd th oigin of th coodinat systm on th 0 kg sph ( m ). Th sph ( m ) with a mass of 0 kg is 0 cm away on th x-axis. Th point at which th nt gavitational foc is zo must li btwn th masss m Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

15 Nwton s Thoy of Gavity 3-5 and m. This is bcaus on such a point, th gavitational focs du to m and m a in opposit dictions. As th gavitational foc is dictly popotional to th two masss and invsly popotional to th squa of distanc btwn thm, th mass m must b clos to th 0-kg mass. Th small mass m, if placd ith to th lft of m o to th ight of m, will xpinc gavitational focs fom m and m pointing in th sam diction, thus always lading to a nonzo foc. Solv: mm mm 0 0 Fm on m = Fm on m G = G = x (0. 0 x) x (0. 0 x) 0x 8x = 0 x= m and 0. 7 m Th valu x = cm is unphysical in th cunt situation, sinc this point is not btwn m and m. Thus, th mass should b placd.7 cm to th ight of th lag mass. To two significant figus, this is cm Modl: Modl th ath () as a sphical mass and th satllit (s) as a point paticl. Lt h b th hight fom th sufac of th ath wh th acclation du to gavity of th sufac valu ( g sufac). Solv: (a) Sinc galtitud = (0. 0) gsufac, w hav GM GM = (0. 0) ( + h) ( + h) = h=. 6 h= (. 6)( m) = m =. 4 0 m ( g altitud) is 0% (b) Fo a satllit obiting th ath at a hight h abov th sufac of th ath, th gavitational foc btwn th ath and th satllit povids th cntiptal acclation ncssay fo cicula motion. Fo a satllit obiting with vlocity v s, 4 GMms msvs GM ( N m /kg )( kg) = v s = = = 4. 5 km/s ( ) 6 7 ( + h) + h + h ( m m) Modl: Modl th ath as a sphical mass and th objct (o) as a point paticl. Igno ai sistanc. This is an isolatd systm, so mchanical ngy is consvd. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

16 3-6 Chapt 3 Solv: (a) Th consvation of ngy quation K + Ug = K + Ug is v = GM + y GM m mv GM m o o o = mv o + y 4 = ( N m /kg )( kg) 3 0 km/s 6 6 = m m (b) In th flat-ath appoximation, Ug = mgy. Th ngy consvation quation thus bcoms m v m gy m v m gy o+ o = o+ o 5 v = v + g( y y ) = (9. 8 m/s )( m 0 m) = 3. 3 km/s (c) Th pcnt o in th flat-ath calculation is 330 m/s 300 m/s 3. 6% 300 m/s Modl: Consid th objct as a paticl and tak th plant to b a sphical mass. Solv: Consvation of mchanical ngy of th objct givs Mm Mm G = mv G + h Th objct s mass dops out. Solving fo th spd as it hits th gound, + h GMh v = GM = GM = + h ( + h) ( + h) Assss: Compa this to GMh v = gh =, which is th sult if th potntial U = mgh is usd Modl: Modl th ath and th pojctil as sphical masss. Igno ai sistanc. This is an isolatd systm, so mchanical ngy is consvd. A pictoial psntation of th bfo-and-aft vnts is shown. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

17 Nwton s Thoy of Gavity 3-7 Solv: Aft using v = 0 m/s, th ngy consvation quation K + U = K+ U is Th pojctil mass cancls. Solving fo h, w find GM m GM m 0 J = h p p mv p + v 5 h= = 4. 0 m GM Modl: Modl th ath as a sphical mass and th mtooids as point masss. Solv: (a) Th ngy consvation quation K + U = K+ Ugivs GM m mv = mv v = v + GM m m (000 m/s) ( N m /kg )( kg) m m 4 =. 0 m/s = km/s GM m Th spd dos not dpnd on th mtooid s mass. / (b) This pat diffs in that = km = m. Th shap of th mtooid s tajctoy is not impotant fo using ngy consvation. Thus GM m GM m mv = mv v = v + GM km m km m 3 = m/s = 8. 9 km/s 7 / / Modl: Modl th two stas as sphical masss, and th comt as a point mass. This is an isolatd systm, so mchanical ngy is consvd. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

18 3-8 Chapt 3 In th initial stat, th comt is fa away fom th two stas and thus it has nith kintic ngy no potntial ngy. In th final stat, as th comt passs though th midpoint conncting th two stas, it posssss both kintic ngy and potntial ngy. Solv: Th consvation of ngy quation Kf + Uf = Ki + Ui givs mv f f f 30 f f. GMm GMm = 0 J + 0 J 4GM 4( N m /kg )( kg) v = = = 3,600 m/s = 33 km/s m Assss: Not that th final vlocity of 33 km/s dos not dpnd on th mass of th comt Modl: Modl th astoid as a sphical mass and youslf as a point mass. This is an isolatd systm, so mchanical ngy is consvd. Th adius of th astoid is M a and its mass is a. Solv: Th consvation of ngy quation Kf + Uf = Ki + Ui fo th astoid givs GM m GMam mv = a f mvi a + Th minimum spd fo scap is th on that will caus you to stop only whn th spaation btwn you and th astoid bcoms vy lag. Noting that vf 0 m/s as, w hav a i a v 4 GM ( N m /kg )(. 0 0 kg) = = v 3 i =. 58 m/s. 0 0 m That is, you nd a spd of.58 m/s to scap fom th astoid. W can now calculat you jumping spd on th ath. Th consvation of ngy quation givs 0 J mvi mg(0 50 m) vi (9 8 m/s )(0 50 m) 3 3 m/s =. =.. =. This mans you can scap fom th astoid Modl: Th pojctil is a paticl. Th ath and moon a sphical masss. Solv: Th pojctil is attactd to both th moon and ath. Its final vlocity and potntial ngy a zo. Sinc th pojctil is fid fom th fa sid of th moon, its initial distanc fom th cnt of th ath is th ath-moon a Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

19 Nwton s Thoy of Gavity 3-9 distanc -m plus th adius of th moon m. Lt th pojctil hav mass m. Th consvation of mchanical ngy quation is Fom Tabl 3., givs scap v =. 78 km/s. Mm M m mv -G - G = 0 J + 0 J ( ) m scap -m + m m M M v G m scap = + -m + m m m m = m, = m, M = kg, and Assss: Th scap vlocity dos not dpnd on th mass of th objct which is tying to scap. m M = kg, which Modl: Th two astoids mak an isolatd systm, so mchanical ngy is consvd. W will also us th law of consvation of momntum fo ou systm. Solv: Th consvation of momntum quation pfx = pix is M( v ) + M( v ) = 0 kg m/s ( v ) = ( v ) fx fx fx fx Th quation fo mchanical ngy consvation Kf + Uf = Ki + Ui is GM ( )( M) GM ( )( M) 0. 8GM M( vfx) + ( M)( vfx) = [( vfx) ] + ( vfx) = 0 GM ( vfx) = ( vfx) = ( vfx) =. 03 / Th havi astoid has a spd of 0. 56( GM/ ) and th light on a spd of. 03( GM/ ) Modl: Gavity is a consvativ foc, so w can us consvation of ngy. GM / Th plants will b pulld togth by gavity and ach will hav spd v as thy cash and th spaation btwn thi cnts will b. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

20 3-0 Chapt 3 Solv: Th plants bgin with only gavitational potntial ngy. Whn thy cash, thy hav both potntial and kintic ngy. Thus, Bcaus th plant is Jupit-siz, w ll us GMM K U Mv Mv K U + = + = + = 0 J v = GM 7 M = M Jupit =. 9 0 kg and GMM = =. 4 0 m. Insting Jupit ths valus into th xpssion abov givs th cash spd of ach plant as v = m/s. Assss: Not that th foc is not constant, bcaus it vais with distanc, so th motion is not constant acclation motion. Th fomulas fom constant-acclation kinmatics do not wok fo poblms such as this Modl: Modl th distant plant (P) as a sphical mass. Solv: Th acclation at th sufac of th plant and at th altitud h a GM M GM g g g G ( + h) P P P sufac = and altitud = sufac = ( + h) = + h= h= ( ) = That is, th staship is obiting at an altitud of Modl: Th stas a sphical masss. 4 8 Solv: Th stats a idntical, so thi final spds v f a th sam. Thy collid whn thi cnts a apat. Fom ngy consvation, M M 3 G = 3 Mv 9 f 3 G (5 0 0 m). vf = GM m v = m/s f Modl: Th stas a sphical masss. Thy ach otat about th systm s cnt of mass. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

21 Nwton s Thoy of Gavity 3- Solv: (a) Th stas otat about th systm s cnt of mass with th sam piod: T = T = T. W can locat th cnt of mass by ltting th oigin b at th small-mass sta. Thn (. 0 0 kg)(0 m) + ( kg)(. 0 0 m) = cm = =. 5 0 m kg kg Mass m undgos unifom cicula motion with adius = m du to th gavitational foc of mass m at distanc =. 0 0 m. Th gavitational foc is sponsibl fo th cntiptal acclation, so Gmm mv m p 4p m Fgav = = ma cntiptal = = = T T / / p 8 30 ( N m /kg )(.0 0 kg) 4p 4 (0.5 0 m)(0.5 0 m) T= = = s = 4 yas Gm (b) Th spd of ach sta is v= ( π )/ T. Thus π π. 8 ( 5 0 m) v = = =. 3 km/s T s π π. 8 (0 5 0 m) v = = = 4. km/s T s Modl: Modl th moon (m) as a sphical mass and th land (l) as a paticl. This is an isolatd systm, so mchanical ngy is consvd. Th initial position of th luna land (mass = m ) is at a distanc = m + 50 km fom th cnt of th moon. Th final position of th luna land is th obit whos distanc fom th cnt of th moon is = km. m Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

22 3- Chapt 3 Solv: Th xtnal wok don by th thusts is xt = mch = g W E U wh w usd E = U fo a cicula obit. Th chang in potntial ngy is fom th initial obit at mch g i = m + 50 km to th final obit f = m km. Thus W xt GM mm GM mm GM mm = = f i i f ( N m /kg )( kg)(4000 kg) = m m 8 = J Modl: Modl th ath () as a sphical mass and th spac shuttl (s) as a point paticl. This is an isolatd systm, so th mchanical ngy is consvd. Th spac shuttl (mass = m ) is at a distanc of = + 50 km. s Solv: Th xtnal wok don by th thusts is xt = mch = g W E U wh w usd E = U fo a cicula obit. Th chang in potntial ngy is fom th initial obit at mch g = + 50 km to th final obit f = + 60 km. Thus W xt GMm GMm GMm = = f i i f 4 ( N m /kg )( kg)(75,000 kg) = m m =. 0 J This much ngy must b supplid by buning th on-boad ful Modl: Assum a sphical astoid and a point mass modl fo th satllit. This is an isolatd systm, so mchanical ngy is consvd. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

23 Nwton s Thoy of Gavity 3-3 Th obital adius of th satllit is Solv: (a) Th spd of a satllit in a cicula obit is = a + h= 8,800 m + 5,000 m = 3,800 m 6 GM ( N m /kg )(. 0 0 kg) v = = = 7. 0 m/s 3,800 m (b) Th minimum launch spd fo scap ( v i ) will caus th satllit to stop asymptotically ( v f = 0 m/s) as. Using th ngy consvation quation K + U = K + U, w gt f GM m GM m GM mv mv v v a s a s a s f = s i 0 J 0 J = scap f a a scap a / 6 GMa ( N m /kg )(. 0 0 kg) = = = m/s 8800 m Modl: Modl th moon as a sphical mass and th satllit as a point mass. Th otational piod of th satllit is th sam as th otational piod of th moon aound its own axis. This tim happns to b 7.3 days. Solv: Th gavitational foc btwn th moon and th satllit povids th cntiptal acclation ncssay fo cicula motion aound th moon. Thfo, Sinc = m + h, thn GM mm ω m m T π = = 3 GM mt ( N m /kg )( kg)( s) = = 4π 4π 7 = m h= m = m m = m Modl: Modl th ath as a sphical mass and th satllit as a point mass. Th satllit is dictly ov a point on th quato onc vy two days. Thus, s = s. T = T = 4 Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

24 3-4 Chapt 3 Solv: Fom Kpl s laws applid to a cicula obit: 4π GMT ( N m /kg )( kg)( ) = = 4π 4π T = GM 7 = m Assss: Th adius of th obit is lag than th gosynchonous obit Plas f to Figu P3.50. Solv: Th gavitational foc on on of th masss is du to th sta and th oth plant. Thus Mm Gmm mv m π GM Gm 4π G + = = + = 4 ( ) T T 3 G m 4π 4π M + = T 4 = T G ( M + m/4) 3.5. Solv: (a) Taking th logaithm of both sids of v But p q = Cu givs p q q logc [log( v ) = plog v] = [log( Cu ) = logc + qlog u] logv = logu + p p x= logu and y = log v, so x and y a latd by q logc y = x+ p p (b) Th pvious sult shows th is a lina lationship btwn x and y, so th is a lina lationship btwn log u and log v. Th gaph of a lina lationship is a staight lin, so th gaph of log v-vsus-log u will b a staight lin. (c) Th slop of th staight lin psntd by th quation y= ( qp / ) x+ log Cp / is qp. / Thus, th slop of th log v- vsus-log u gaph will b qp. / (d) Th pdictd y-intcpt of th gaph is log C/p, and th xpimntally dtmind valu is Equating ths, w can solv fo M. Bcaus th plants all obit th sun, th mass w a finding is M = M. 4π 4π logc = log = = 0 = GMsun GMsun 0 M sun Th tabulatd valu, to th significant figus, is wigh th sun! 4π = (0 ) = kg G 3.5. Solv: (a) Dividing th cicumfnc of th obit by th piod givs (b) Using th fomula fo th acclation at th sufac, g sum 30 / M = kg. W hav usd th obits of th plants to πs π(. 0 0 m) 4 v = = = m/s T. 0 s 30 GMs.. sufac 4 s (. 0 0 m) 4 ( N m /kg )( 99 0 kg) = = =. 3 0 m/s sun Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

25 Nwton s Thoy of Gavity 3-5 (c) Th mass of an objct on th ath will b th sam as its mass on th sta. Th gavitational foc is (d) Th adius of th obit of th satllit is T G sta sufac ( F ) = mg =. 3 0 N = 0 m m =. 0 m. Th piod is π 4 π (. 0 m) 4 = = T =. GM 30 s ( N m /kg )( kg) This mans th a 589 volutions p scond o obits p minut. () Applying Equation 3.5 fo a gosynchonous obit, s 30 3 GMs ( N m /kg )( kg)(. 0 s) 6 = = =. T 4π 4π 5 0 m Modl: Assum th sola systm is a point paticl. Solv: (a) Th adius of th obit of th sola systm in th galaxy is 5,000 light yas. This mans = 5,000 light yas = 500( m/s)(365 d/y)(4 h/d)(3600 s/h)( y) = m π π( m) 5 8 T = = = s =. 0 yas v m/s yas (b) Th numb of obits = = 4 obits yas (c) Applying Nwton s scond law yilds GM m mv v G g cnt ss ss ( m/s) ( m) 4 = M g cnt = = =. (d) Th numb of stas in th cnt of th galaxy is kg = kg Modl: Assum th th stas a sphical masss N m /kg kg Th stas otat about th cnt of mass, which is th cnt of th tiangl and qual distanc fom all th stas. Th gavitational foc btwn any two stas is th sam. On a givn sta th two focs fom th oth stas mak an angl of 60. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

26 3-6 Chapt 3 Solv: Th valu of can b found as follows: Th gavitational foc btwn any two stas is L/ L. 0 0 m = cos(30 ) = = = m cos(30 ) cos(30 ) 30 GM ( N m /kg )( kg) 6 Fg = = = N L (. 0 0 m) Th componnt of this foc towad th cnt is c g 6 6 F = F cos(30 ) = ( N)cos(30 ) =. 9 0 N Th nt foc on a sta towad th cnt is twic this foc, and that foc quals 6 π. 9 0 N = Mω = M T 30 Mω. This mans 4π M 4 π ( kg)( m) 8 T = = = s = 0 yas N N Modl: Angula momntum is consvd fo a paticl following a tajctoy of any shap. Fo a paticl in an lliptical obit, th paticl s angula momntum is L = mvt = mvsin β, wh v is th vlocity tangnt to th tajctoy and β is th angl btwn and v. Solv: At th distanc of closst appoach ( min ) and also at th most distant point, β = 90. Sinc th is no tangntial foc (th only foc bing th adial foc) th is no toqu, so angula momntum must b consvd: min max m v = m v Pluto min Pluto max 3 v = v ( / ) = (6. 0 m/s)(( m)/( m) = 3. 7 km/s Modl: Angula momntum is consvd fo a paticl following a tajctoy of any shap. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

27 Nwton s Thoy of Gavity 3-7 Fo a paticl in an lliptical obit, th paticl s angula momntum is L = mvt = mvsin β, wh v is th vlocity tangnt to th tajctoy, and β is th angl btwn and v. Solv: At th distanc of closst appoach ( min ) and also at th most distant point, β = 90. Sinc th is no tangntial foc (th only foc bing th adial foc) th is no toqu, so angula momntum must b consvd: m v = m v Mcuy min 0 Mcuy max ( m)(38. 8 km/s) 0 min = maxv/ v = = m km/s Modl: Fo th sun + comt systm, th mchanical ngy is consvd. Solv: Th consvation of ngy quation Kf + Uf = Ki + Ui givs Using G = Nm /kg, w gt v = km/s. GM M Mv GM M s c s c c = Mv c 30 M s = kg, 0 = m, = m, and v = km/s, Modl: Modl th plant (p) as a sphical mass and th spacship (s) as a point mass. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

28 3-8 Chapt 3 Solv: (a) Fo th cicula motion of th spacship aound th plant, GM m GM p s mv0 p = v 0 = Immdiatly aft th ockts w fid v = v 0 / and = 0. Thfo, v = (b) Th spacship s maximum distanc is max = 0. Its minimum distanc occus at th oth nd of th llips. Th ngy at th fiing point is qual to th ngy at th oth nd of th lliptical tajctoy. That is, GM GM m mv p s p s s = mv s Sinc th angula momntum at ths two nds is consvd, w hav 0 p GM m mv = mv v = v ( / ) With this xpssion fo v, th ngy quation simplifis to Using = 0 and v GM p = v / =, 0 0 GM v v GM p p = ( / ) GM GM GM GM p p p 0 p 0 = = = 0 + = Th solutions a = 0 (th initial distanc) and = 0 /7. Thus th minimum distanc is min = 0 / Solv: (a) At what distanc fom th cnt of Satun is th acclation du to gavity th sam as on th sufac of th ath? Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

29 Nwton s Thoy of Gavity 3-9 (b) (c) Th distanc is m. This is. 06Satun Solv: (a) A 000 kg satllit obits th ath with a spd of 997 m/s. What is th adius of th obit? (b) (c) Th adius of th obit is payload 4 GM E ( N m /kg )( kg) 8 = = = m ( v ) (997 m/s) 3.6. Solv: (a) A 00 kg objct is lasd fom st at an altitud abov th moon qual to th moon s adius. At what spd dos it impact th moon s sufac? (b) Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

30 3-30 Chapt 3 (c) Th spd is v = 680 m/s Solv: (a) Kpl s thid law fo cicula obits is 4π 3 4π T = T = GM GM 4π 3 Ltting a =, th fist satllit obys T = a. Fo th scond satllit, which obits th sam mass, GM 3 3 T + T = a( + ) = a + n Sinc, w can us th appoximation ( ± x) ± nx. Thus 3 3 T + T a + Subtacting th quation 3 T a = fo th fist satllit fom this, 3 3 T = a Dividing this by th quation fo th fist satllit, T 3 = T (b) Th satllits obit th ath. Th factional diffnc in thi piods is T 3 km = = T 6700 km Aft = 4467 piods thy will mt again. Fo th inn satllit, 4π 6 T = ( m) 4 G( kg) = 5456 s =. 5 hs So th satllits will mt again in hs = 6770 hs = 8 days. Assss: A communications satllit has an obital piod of aound.5 h. Th supising lngth of tim btwn th two satllits mting is du to th small diffncs in thi piods Modl: Modl th ath and sun as sphical masss, th satllit as a point mass. Assum th satllit s distanc fom th ath is vy small compad to th ath s (and satllit s) distanc to th sun Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

31 Nwton s Thoy of Gavity 3-3 Solv: Th nt foc on th satllit is th sum of th gavitational foc towad th sun and th gavitational foc towad th ath. This nt foc is sponsibl fo cicula motion aound th sun. W want to chos th distanc d to mak th piod T match th piod T with which th ath obits th sun. Th ath s obital piod is givn by 3 (4 π / s) T = GM. Thus Using s p 4p s cntiptal T 3 GM m GM m mv m GM Fnt = = ma = = = m = m d T = d and cancling th Gm tm givs M M = M ( d ) ( d) d s s 3 This quation can t b solvd xactly, but w can mak us of th fact that d to us th binomial appoximation. Facto th out of th xpssions d to gt M M M = ( d / ) d d s s ( / ) If w think of d / = x, w can simplify th fist tm by using ( ± x) ± nx. H n =, so w gt Thus d = [ M /(3 M )] = m. Assss: M M M M M /3 9 s d / = 0. 00, so ou assumption that s s s [ ( ) d / ] = ( d / ) = 3 d d d / is justifid. n Modl: Th ath and sun a sphical masss. Th ath is in a cicula obit aound th sun. Th pojctil is a paticl. Th ffct of th ath s otation on th pojctil s vlocity is ignod. Th ath and sun a so massiv compad to th ockt that thy a unaffctd by th ockt s motion (no coil). Th ockt scaps fom th influnc of th ath s gavitation in a distanc small in compaison with th distanc fom th ath to th sun, so that th chang in sola potntial of th ockt as it scaps th ath is ngligibl. Solv: To scap th sun s gavitational pull at th ath s distanc fom th sun, a pojctil must hav spd v Th ngy consvation quation fo th pojctil is scap. mv Mm - = 0 J s scap G -s 30 Ms.. scap -s ( m) - ( N m /kg )( 99 0 kg) 4 v = G = = m/s Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

32 3-3 Chapt 3 Th ath s spd in its obit is found by considing Equation 3.: GMs 4 v = = m/s -s Th pojctil must also scap fom th ath s gavitational pull. Fa fom th ath, th pojctil s total spd is th sum of its spd lativ to th ath fa fom th influnc of ath s gavity, v p, and th ath s spd. v = v + v scap p vp = vscap v = m/s m/s =. 3 0 m/s. To obtain th spd v p fa fom th ath, th pojctil must b launchd fom th ath with spd v launch. Using ngy consvation, Mm M mv G mv v G v launch = p launch = + p 4 4 ( N m /kg )( kg) = + (. 3 0 m/s) 6 ( m) 4 = m/s Assss: Th pojctil must attain a spd of 6.6 km/s if launchd in th diction of ath s motion. This is about a facto of 7 tims lss than what is quid fom st. Not that th spd of th ath in its obit about th sun v diffs fom th scap spd fom th sun vscap by a facto of Modl: Modl th 400 kg satllit and th 00 kg satllit as point masss and modl th ath as a sphical mass. Momntum is consvd duing th inlastic collision of th two satllits. 6 6 Solv: Fo th givn obit, 0 = + 0 m = m. Th spd of a satllit in this obit is GM v0 = = 7357 m/s 0 Th two satllits collid, stick togth, and mov with vlocity v. Th quation fo momntum consvation fo th pfctly inlastic collision givs (400 kg + 00 kg) v = (400 kg)(7357 m/s) (00 kg)(7357 m/s) v = 444 m/s Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

33 Nwton s Thoy of Gavity 3-33 Th nw satllit s adius immdiatly aft th collision is still = 0 = m. Now it is moving in an lliptical obit. W nd to dtmin if th minimum distanc is lag o small than th ath s adius = m. 6 Th combind satllits will continu moving in an lliptical obit. Th momntum of th combind satllit is L = mv sin β (s Equation 3.6) and is consvd in a tajctoy of any shap. Th angl β is 90 whn v = 444 m/s and whn th satllit is at its closst appoach to th ath. Fom consvation of angula momntum, w hav 0 0 v = v = (444 m/s) = m /s m /s = v Using th consvation of ngy quation at positions and, GM(500 kg) GM(500 kg) (500 kg)(444 m/s) = (500 kg) v m Using th abov xpssion fo, w can simplify th ngy quation to A vlocity of 0,07 m/s fo v yilds v 4 7 ( m/s) v + ( m /s ) = 0 m /s v = 0,07 m/s and 444 m/s m /s 6 = =. 6 0 m 0,07 m/s 6 Sinc 6 < = m, th combind mass of th two satllits will cash into th ath Modl: Plant Physics is a sphical mass. Th cuis ship is in a cicula obit. Solv: (a) At th sufac, th f-fall acclation is 0 g = GM/. Fom kinmatics, y = y + v t g( t) 0 m = 0 m + ( m/s)(. 5 s) g(. 5 s) f i g =. 0 m/s Th piod of th cuis ship s obit is = 3,800 s. Fo th cicula obit of th cuis ship, Th mass is thus M= ( / Gg ) = kg. (b) Fom pat (a), 4π 3 T T = ( ) = = GM 3π GM g (. 0 m/s )(3,800 s) 6 = = m. 3π 6 =. 3 0 m Modl: Th moon is a sphical mass. Th moon land is oiginally in a cicula obit. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

34 3-34 Chapt 3 Solv: Engy and momntum a consvd btwn points and in th lliptical obit. Also, at both points GM β = 90, so L = mvsin β = mv. Lt h = 000 km. Th oiginal spd of th land is m v = m/s + h =. v m + h Consvation of angula momntum quis m v = mv = =. Th ngy consvation qua- v tion givs m + h Substituting v = v, m m m + M m Mmm mv G = mv G h Mm m + h Mm = m h m m v G v G + m h v + = GM m m m + h m 6 = m = m m 39 0 m /s ( ) =. m m + h [( m + h)/ m] ( m + h) m + h v GM h GM v = 80 m/s Th factional chang in spd quid to just gaz th moon at point is 338 m/s 80 m/s =. 8% 338 m/s Assss: A duction in spd by almost % is asonabl Modl: Modl th ath as a sphical mass and th satllit as a point mass. This is an isolatd systm, so mchanical ngy is consvd. Also, th angula momntum of th satllit is consvd. Plas f to Figu CP3.68. Solv: (a) Angula momntum is L = mvsin β. Th angl β = 90 at points and, so consvation of angula momntum quis Th ngy consvation quation is m v m v v v = = GMm GMm mv ( ) = mv ( ) ( v ) ( v ) = GM m m m Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

35 Nwton s Thoy of Gavity 3-35 Using th angula momntum sult fo v givs (b) Fo th cicula obit, Fo th lliptical obit, = = ( v ) ( v ) GM ( v ) GM GM ( / ) GM ( / ) v = and v = v = GM ( N m /kg )( kg) v = = = 7730 m/s ( m 3 0 m) = km = m m = m = + 35,900 km = m m = m GM ( / ) v = v = 0, 60 m/s 0 (c) Fom th wok-kintic ngy thom, W = K = mv mv =. 7 0 J GM ( (d) / ) v = + Using th sam valus of and as in (b), v = 600 m/s. Fo th cicula obit, 9 () W = mv mv = J 0 GM v = = 3070 m/s (f) Th total wok don is. 5 0 J. This is th sam as in Exampl 3.6, but h w v land how th wok has to b dividd btwn th two buns Modl: Th od is thin and unifom. Solv: (a) Th od is not sphical so must b dividd into thin sctions ach d wid and having mass dm. Sinc th od is unifom, dm d M = dm = d M L L Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

36 3-36 Chapt 3 Th width of th od is small nough so that all of dm is distanc away fom m. Th gavitational potntial ngy of dm and m is m dm m( M/L) d du = G = G Th total potntial ngy of th od and mass m is found by adding th contibutions du fom vy point along th od in an intgal: Not is incasing with th limits chosn as thy a. (b) Th foc on m whn at x is L x+ GMm d GMm x + L/ U = du = ln L = L x L/ L x du GMm d L L GMm F = = ln x ln x dx L dx + = L x + L/ x L/ 4 L = GMm, x 4x L Assss: Th diction of th foc is towad th x diction, as xpctd. Th foc magnitud appoachs as th mass m appoachs th nd of th od, but gos to zo lik away th od looks lik a point mass. x as x gts lag. This is xpctd sinc fom fa Modl: Th ing is unifom and is so thin that vy point on it may b considd to b th sam distanc fom m. Solv: (a) W must dtmin th gavitational potntial (du) btwn m and an abitay pat of th ing dm, thn add using an intgal all th contibutions to U. Sinc th ing is unifom, Th distanc fom m to dm is Th total gavitational potntial is dm dl M = dm = dl M π π = x +. Th gavitational potntial btwn m and dm is m dm mm dl du = G = G π x + GmM U = du = dl π x + ing Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

37 Nwton s Thoy of Gavity 3-37 Not that x and do not chang fo any location of dm. Th intgal is just th lngth of th ing. ing dl = π Thus GmM U = x + (b) Th foc on m whn at x is du d 3 Fx = = GmM [( x + ) ] = GmM ( x + ) ( x) dx dx x = GmM 3 ( x + ) Thus th magnitud of th foc is x F = GmM ( x + ) Assss: Th foc is zo at th cnt of th ing. Elswh its diction is towad th oigin. As x gts lag, th foc dcass lik x This is xpctd sinc fom fa away th ing looks lik a point mass. 3. Copyight 03 Pason Education, Inc. All ights svd. This matial is potctd und all copyight laws as thy cuntly xist.

38

GRAVITATION. (d) If a spring balance having frequency f is taken on moon (having g = g / 6) it will have a frequency of (a) 6f (b) f / 6

GRAVITATION. (d) If a spring balance having frequency f is taken on moon (having g = g / 6) it will have a frequency of (a) 6f (b) f / 6 GVITTION 1. Two satllits and o ound a plant P in cicula obits havin adii 4 and spctivly. If th spd of th satllit is V, th spd of th satllit will b 1 V 6 V 4V V. Th scap vlocity on th sufac of th ath is

More information

GRAVITATION 4) R. max. 2 ..(1) ...(2)

GRAVITATION 4) R. max. 2 ..(1) ...(2) GAVITATION PVIOUS AMCT QUSTIONS NGINING. A body is pojctd vtically upwads fom th sufac of th ath with a vlocity qual to half th scap vlocity. If is th adius of th ath, maximum hight attaind by th body

More information

8 - GRAVITATION Page 1

8 - GRAVITATION Page 1 8 GAVITATION Pag 1 Intoduction Ptolmy, in scond cntuy, gav gocntic thoy of plantay motion in which th Eath is considd stationay at th cnt of th univs and all th stas and th plants including th Sun volving

More information

CHAPTER 5 CIRCULAR MOTION

CHAPTER 5 CIRCULAR MOTION CHAPTER 5 CIRCULAR MOTION and GRAVITATION 5.1 CENTRIPETAL FORCE It is known that if a paticl mos with constant spd in a cicula path of adius, it acquis a cntiptal acclation du to th chang in th diction

More information

STATISTICAL MECHANICS OF DIATOMIC GASES

STATISTICAL MECHANICS OF DIATOMIC GASES Pof. D. I. ass Phys54 7 -Ma-8 Diatomic_Gas (Ashly H. Cat chapt 5) SAISICAL MECHAICS OF DIAOMIC GASES - Fo monatomic gas whos molculs hav th dgs of fdom of tanslatoy motion th intnal u 3 ngy and th spcific

More information

Get Solution of These Packages & Learn by Video Tutorials on GRAVITATION

Get Solution of These Packages & Learn by Video Tutorials on  GRAVITATION FEE Download Study Packag fom wbsit: www.tkoclasss.com & www.mathsbysuhag.com Gt Solution of Ths Packags & an by Vido Tutoials on www.mathsbysuhag.com. INTODUCTION Th motion of clstial bodis such as th

More information

CHAPTER 5 CIRCULAR MOTION AND GRAVITATION

CHAPTER 5 CIRCULAR MOTION AND GRAVITATION 84 CHAPTER 5 CIRCULAR MOTION AND GRAVITATION CHAPTER 5 CIRCULAR MOTION AND GRAVITATION 85 In th pious chapt w discussd Nwton's laws of motion and its application in simpl dynamics poblms. In this chapt

More information

5-9 THE FIELD CONCEPT. Answers to the Conceptual Questions. Chapter 5 Gravity 63

5-9 THE FIELD CONCEPT. Answers to the Conceptual Questions. Chapter 5 Gravity 63 Chapt 5 Gavity 5-9 THE FIELD CONCEPT Goals Intoduc th notion of a fild. (Pobl Solvin) Calculat th Sun's avitational fild at Eath's location. Contnt Th psnc of a ass odifis spac. A valu can b assind to

More information

Kinetics. Central Force Motion & Space Mechanics

Kinetics. Central Force Motion & Space Mechanics Kintics Cntal Foc Motion & Spac Mcanics Outlin Cntal Foc Motion Obital Mcanics Exampls Cntal-Foc Motion If a paticl tavls un t influnc of a foc tat as a lin of action ict towas a fix point, tn t motion

More information

Physics 240: Worksheet 15 Name

Physics 240: Worksheet 15 Name Physics 40: Woksht 15 Nam Each of ths poblms inol physics in an acclatd fam of fnc Althouh you mind wants to ty to foc you to wok ths poblms insid th acclatd fnc fam (i.. th so-calld "won way" by som popl),

More information

GAUSS PLANETARY EQUATIONS IN A NON-SINGULAR GRAVITATIONAL POTENTIAL

GAUSS PLANETARY EQUATIONS IN A NON-SINGULAR GRAVITATIONAL POTENTIAL GAUSS PLANETARY EQUATIONS IN A NON-SINGULAR GRAVITATIONAL POTENTIAL Ioannis Iaklis Haanas * and Michal Hany# * Dpatmnt of Physics and Astonomy, Yok Univsity 34 A Pti Scinc Building Noth Yok, Ontaio, M3J-P3,

More information

Physics 111. Lecture 38 (Walker: ) Phase Change Latent Heat. May 6, The Three Basic Phases of Matter. Solid Liquid Gas

Physics 111. Lecture 38 (Walker: ) Phase Change Latent Heat. May 6, The Three Basic Phases of Matter. Solid Liquid Gas Physics 111 Lctu 38 (Walk: 17.4-5) Phas Chang May 6, 2009 Lctu 38 1/26 Th Th Basic Phass of Matt Solid Liquid Gas Squnc of incasing molcul motion (and ngy) Lctu 38 2/26 If a liquid is put into a sald contain

More information

5.61 Fall 2007 Lecture #2 page 1. The DEMISE of CLASSICAL PHYSICS

5.61 Fall 2007 Lecture #2 page 1. The DEMISE of CLASSICAL PHYSICS 5.61 Fall 2007 Lctu #2 pag 1 Th DEMISE of CLASSICAL PHYSICS (a) Discovy of th Elcton In 1897 J.J. Thomson discovs th lcton and masus ( m ) (and inadvtntly invnts th cathod ay (TV) tub) Faaday (1860 s 1870

More information

Hydrogen atom. Energy levels and wave functions Orbital momentum, electron spin and nuclear spin Fine and hyperfine interaction Hydrogen orbitals

Hydrogen atom. Energy levels and wave functions Orbital momentum, electron spin and nuclear spin Fine and hyperfine interaction Hydrogen orbitals Hydogn atom Engy lvls and wav functions Obital momntum, lcton spin and nucla spin Fin and hypfin intaction Hydogn obitals Hydogn atom A finmnt of th Rydbg constant: R ~ 109 737.3156841 cm -1 A hydogn mas

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

The angle between L and the z-axis is found from

The angle between L and the z-axis is found from Poblm 6 This is not a ifficult poblm but it is a al pain to tansf it fom pap into Mathca I won't giv it to you on th quiz, but know how to o it fo th xam Poblm 6 S Figu 6 Th magnitu of L is L an th z-componnt

More information

II.3. DETERMINATION OF THE ELECTRON SPECIFIC CHARGE BY MEANS OF THE MAGNETRON METHOD

II.3. DETERMINATION OF THE ELECTRON SPECIFIC CHARGE BY MEANS OF THE MAGNETRON METHOD II.3. DETEMINTION OF THE ELETON SPEIFI HGE Y MENS OF THE MGNETON METHOD. Wok pupos Th wok pupos is to dtin th atio btwn th absolut alu of th lcton chag and its ass, /, using a dic calld agnton. In this

More information

Physics 202, Lecture 5. Today s Topics. Announcements: Homework #3 on WebAssign by tonight Due (with Homework #2) on 9/24, 10 PM

Physics 202, Lecture 5. Today s Topics. Announcements: Homework #3 on WebAssign by tonight Due (with Homework #2) on 9/24, 10 PM Physics 0, Lctu 5 Today s Topics nnouncmnts: Homwok #3 on Wbssign by tonight Du (with Homwok #) on 9/4, 10 PM Rviw: (Ch. 5Pat I) Elctic Potntial Engy, Elctic Potntial Elctic Potntial (Ch. 5Pat II) Elctic

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

E F. and H v. or A r and F r are dual of each other.

E F. and H v. or A r and F r are dual of each other. A Duality Thom: Consid th following quations as an xampl = A = F μ ε H A E A = jωa j ωμε A + β A = μ J μ A x y, z = J, y, z 4π E F ( A = jω F j ( F j β H F ωμε F + β F = ε M jβ ε F x, y, z = M, y, z 4π

More information

Ch 13 Universal Gravitation

Ch 13 Universal Gravitation Ch 13 Univesal Gavitation Ch 13 Univesal Gavitation Why do celestial objects move the way they do? Keple (1561-1630) Tycho Bahe s assistant, analyzed celestial motion mathematically Galileo (1564-1642)

More information

Escape Velocity. GMm ] B

Escape Velocity. GMm ] B 1 PHY2048 Mach 31, 2006 Escape Velocity Newton s law of gavity: F G = Gm 1m 2 2, whee G = 667 10 11 N m 2 /kg 2 2 3 10 10 N m 2 /kg 2 is Newton s Gavitational Constant Useful facts: R E = 6 10 6 m M E

More information

Solid state physics. Lecture 3: chemical bonding. Prof. Dr. U. Pietsch

Solid state physics. Lecture 3: chemical bonding. Prof. Dr. U. Pietsch Solid stat physics Lctu 3: chmical bonding Pof. D. U. Pitsch Elcton chag dnsity distibution fom -ay diffaction data F kp ik dk h k l i Fi H p H; H hkl V a h k l Elctonic chag dnsity of silicon Valnc chag

More information

Aakash. For Class XII Studying / Passed Students. Physics, Chemistry & Mathematics

Aakash. For Class XII Studying / Passed Students. Physics, Chemistry & Mathematics Aakash A UNIQUE PPRTUNITY T HELP YU FULFIL YUR DREAMS Fo Class XII Studying / Passd Studnts Physics, Chmisty & Mathmatics Rgistd ffic: Aakash Tow, 8, Pusa Road, Nw Dlhi-0005. Ph.: (0) 4763456 Fax: (0)

More information

Using the Hubble Telescope to Determine the Split of a Cosmological Object s Redshift into its Gravitational and Distance Parts

Using the Hubble Telescope to Determine the Split of a Cosmological Object s Redshift into its Gravitational and Distance Parts Apion, Vol. 8, No. 2, Apil 2001 84 Using th Hubbl Tlscop to Dtmin th Split of a Cosmological Objct s dshift into its Gavitational and Distanc Pats Phais E. Williams Engtic Matials sach and Tsting Cnt 801

More information

Fourier transforms (Chapter 15) Fourier integrals are generalizations of Fourier series. The series representation

Fourier transforms (Chapter 15) Fourier integrals are generalizations of Fourier series. The series representation Pof. D. I. Nass Phys57 (T-3) Sptmb 8, 03 Foui_Tansf_phys57_T3 Foui tansfoms (Chapt 5) Foui intgals a gnalizations of Foui sis. Th sis psntation a0 nπx nπx f ( x) = + [ an cos + bn sin ] n = of a function

More information

Physics 4A Chapter 8: Dynamics II Motion in a Plane

Physics 4A Chapter 8: Dynamics II Motion in a Plane Physics 4A Chapte 8: Dynamics II Motion in a Plane Conceptual Questions and Example Poblems fom Chapte 8 Conceptual Question 8.5 The figue below shows two balls of equal mass moving in vetical cicles.

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

10. Force is inversely proportional to distance between the centers squared. R 4 = F 16 E 11.

10. Force is inversely proportional to distance between the centers squared. R 4 = F 16 E 11. NSWRS - P Physics Multiple hoice Pactice Gavitation Solution nswe 1. m mv Obital speed is found fom setting which gives v whee M is the object being obited. Notice that satellite mass does not affect obital

More information

ORBITAL TO GEOCENTRIC EQUATORIAL COORDINATE SYSTEM TRANSFORMATION. x y z. x y z GEOCENTRIC EQUTORIAL TO ROTATING COORDINATE SYSTEM TRANSFORMATION

ORBITAL TO GEOCENTRIC EQUATORIAL COORDINATE SYSTEM TRANSFORMATION. x y z. x y z GEOCENTRIC EQUTORIAL TO ROTATING COORDINATE SYSTEM TRANSFORMATION ORITL TO GEOCENTRIC EQUTORIL COORDINTE SYSTEM TRNSFORMTION z i i i = (coωcoω in Ωcoiinω) (in Ωcoω + coωcoiinω) iniinω ( coωinω in Ωcoi coω) ( in Ωinω + coωcoicoω) in icoω in Ωini coωini coi z o o o GEOCENTRIC

More information

ω = θ θ o = θ θ = s r v = rω

ω = θ θ o = θ θ = s r v = rω Unifom Cicula Motion Unifom cicula motion is the motion of an object taveling at a constant(unifom) speed in a cicula path. Fist we must define the angula displacement and angula velocity The angula displacement

More information

Recap. Centripetal acceleration: v r. a = m/s 2 (towards center of curvature)

Recap. Centripetal acceleration: v r. a = m/s 2 (towards center of curvature) a = c v 2 Recap Centipetal acceleation: m/s 2 (towads cente of cuvatue) A centipetal foce F c is equied to keep a body in cicula motion: This foce poduces centipetal acceleation that continuously changes

More information

Physics 201 Homework 4

Physics 201 Homework 4 Physics 201 Homewok 4 Jan 30, 2013 1. Thee is a cleve kitchen gadget fo dying lettuce leaves afte you wash them. 19 m/s 2 It consists of a cylindical containe mounted so that it can be otated about its

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

Chapter 13: Gravitation

Chapter 13: Gravitation v m m F G Chapte 13: Gavitation The foce that makes an apple fall is the same foce that holds moon in obit. Newton s law of gavitation: Evey paticle attacts any othe paticle with a gavitation foce given

More information

Mon. Tues. Wed. Lab Fri Electric and Rest Energy

Mon. Tues. Wed. Lab Fri Electric and Rest Energy Mon. Tus. Wd. Lab Fi. 6.4-.7 lctic and Rst ngy 7.-.4 Macoscoic ngy Quiz 6 L6 Wok and ngy 7.5-.9 ngy Tansf R 6. P6, HW6: P s 58, 59, 9, 99(a-c), 05(a-c) R 7.a bing lato, sathon, ad, lato R 7.b v. i xal

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

Extra notes for circular motion: Circular motion : v keeps changing, maybe both speed and

Extra notes for circular motion: Circular motion : v keeps changing, maybe both speed and Exta notes fo cicula motion: Cicula motion : v keeps changing, maybe both speed and diection ae changing. At least v diection is changing. Hence a 0. Acceleation NEEDED to stay on cicula obit: a cp v /,

More information

Mon. Tues. 6.2 Field of a Magnetized Object 6.3, 6.4 Auxiliary Field & Linear Media HW9

Mon. Tues. 6.2 Field of a Magnetized Object 6.3, 6.4 Auxiliary Field & Linear Media HW9 Fi. on. Tus. 6. Fild of a agntid Ojct 6.3, 6.4 uxiliay Fild & Lina dia HW9 Dipol t fo a loop Osvation location x y agntic Dipol ont Ia... ) ( 4 o I I... ) ( 4 I o... sin 4 I o Sa diction as cunt B 3 3

More information

Chapter 5. Uniform Circular Motion. a c =v 2 /r

Chapter 5. Uniform Circular Motion. a c =v 2 /r Chapte 5 Unifom Cicula Motion a c =v 2 / Unifom cicula motion: Motion in a cicula path with constant speed s v 1) Speed and peiod Peiod, T: time fo one evolution Speed is elated to peiod: Path fo one evolution:

More information

Lecture 22. PE = GMm r TE = GMm 2a. T 2 = 4π 2 GM. Main points of today s lecture: Gravitational potential energy: Total energy of orbit:

Lecture 22. PE = GMm r TE = GMm 2a. T 2 = 4π 2 GM. Main points of today s lecture: Gravitational potential energy: Total energy of orbit: Lectue Main points of today s lectue: Gavitational potential enegy: Total enegy of obit: PE = GMm TE = GMm a Keple s laws and the elation between the obital peiod and obital adius. T = 4π GM a3 Midtem

More information

Frictional effects, vortex spin-down

Frictional effects, vortex spin-down Chapt 4 Fictional ffcts, votx spin-down To undstand spin-up of a topical cyclon it is instuctiv to consid fist th spin-down poblm, which quis a considation of fictional ffcts. W xamin fist th ssntial dynamics

More information

Central Force Motion

Central Force Motion Cental Foce Motion Cental Foce Poblem Find the motion of two bodies inteacting via a cental foce. Examples: Gavitational foce (Keple poblem): m1m F 1, ( ) =! G ˆ Linea estoing foce: F 1, ( ) =! k ˆ Two

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

= 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

PH672 WINTER Problem Set #1. Hint: The tight-binding band function for an fcc crystal is [ ] (a) The tight-binding Hamiltonian (8.

PH672 WINTER Problem Set #1. Hint: The tight-binding band function for an fcc crystal is [ ] (a) The tight-binding Hamiltonian (8. PH67 WINTER 5 Poblm St # Mad, hapt, poblm # 6 Hint: Th tight-binding band function fo an fcc cstal is ( U t cos( a / cos( a / cos( a / cos( a / cos( a / cos( a / ε [ ] (a Th tight-binding Hamiltonian (85

More information

Chapter 4. Newton s Laws of Motion

Chapter 4. Newton s Laws of Motion Chapte 4 Newton s Laws of Motion 4.1 Foces and Inteactions A foce is a push o a pull. It is that which causes an object to acceleate. The unit of foce in the metic system is the Newton. Foce is a vecto

More information

ALLEN. è ø = MB = = (1) 3 J (2) 3 J (3) 2 3 J (4) 3J (1) (2) Ans. 4 (3) (4) W = MB(cosq 1 cos q 2 ) = MB (cos 0 cos 60 ) = MB.

ALLEN. è ø = MB = = (1) 3 J (2) 3 J (3) 2 3 J (4) 3J (1) (2) Ans. 4 (3) (4) W = MB(cosq 1 cos q 2 ) = MB (cos 0 cos 60 ) = MB. at to Succss LLEN EE INSTITUTE KT (JSTHN) HYSIS 6. magntic ndl suspndd paalll to a magntic fild quis J of wok to tun it toug 60. T toqu ndd to mata t ndl tis position will b : () J () J () J J q 0 M M

More information

PHYS 272H Spring 2011 FINAL FORM B. Duration: 2 hours

PHYS 272H Spring 2011 FINAL FORM B. Duration: 2 hours PHYS 7H Sing 11 FINAL Duation: hous All a multil-choic oblms with total oints. Each oblm has on and only on coct answ. All xam ags a doubl-sidd. Th Answ-sht is th last ag. Ta it off to tun in aft you finish.

More information

PHYS 272H Spring 2011 FINAL FORM A. Duration: 2 hours

PHYS 272H Spring 2011 FINAL FORM A. Duration: 2 hours PHYS 7H Sing 11 FINAL Duation: hous All a multil-choic oblms with total oints. Each oblm has on and only on coct answ. All xam ags a doubl-sidd. Th Answ-sht is th last ag. Ta it off to tun in aft you finish.

More information

Chapter. s r. check whether your calculator is in all other parts of the body. When a rigid body rotates through a given angle, all

Chapter. s r. check whether your calculator is in all other parts of the body. When a rigid body rotates through a given angle, all conveted to adians. Also, be sue to vanced to a new position (Fig. 7.2b). In this inteval, the line OP has moved check whethe you calculato is in all othe pats of the body. When a igid body otates though

More information

Gravitation. AP/Honors Physics 1 Mr. Velazquez

Gravitation. AP/Honors Physics 1 Mr. Velazquez Gavitation AP/Honos Physics 1 M. Velazquez Newton s Law of Gavitation Newton was the fist to make the connection between objects falling on Eath and the motion of the planets To illustate this connection

More information

Practice. Understanding Concepts. Answers J 2. (a) J (b) 2% m/s. Gravitation and Celestial Mechanics 287

Practice. Understanding Concepts. Answers J 2. (a) J (b) 2% m/s. Gravitation and Celestial Mechanics 287 Pactice Undestanding Concepts 1. Detemine the gavitational potential enegy of the Eath Moon system, given that the aveage distance between thei centes is 3.84 10 5 km, and the mass of the Moon is 0.0123

More information

Potential Energy and Conservation of Energy

Potential Energy and Conservation of Energy Potential Enegy and Consevation of Enegy Consevative Foces Definition: Consevative Foce If the wok done by a foce in moving an object fom an initial point to a final point is independent of the path (A

More information

Molecules and electronic, vibrational and rotational structure

Molecules and electronic, vibrational and rotational structure Molculs and ctonic, ational and otational stuctu Max on ob 954 obt Oppnhim Ghad Hzbg ob 97 Lctu ots Stuctu of Matt: toms and Molculs; W. Ubachs Hamiltonian fo a molcul h h H i m M i V i fs to ctons, to

More information

Q Q N, V, e, Quantum Statistics for Ideal Gas and Black Body Radiation. The Canonical Ensemble

Q Q N, V, e, Quantum Statistics for Ideal Gas and Black Body Radiation. The Canonical Ensemble Quantum Statistics fo Idal Gas and Black Body Radiation Physics 436 Lctu #0 Th Canonical Ensmbl Ei Q Q N V p i 1 Q E i i Bos-Einstin Statistics Paticls with intg valu of spin... qi... q j...... q j...

More information

Experiment 09: Angular momentum

Experiment 09: Angular momentum Expeiment 09: Angula momentum Goals Investigate consevation of angula momentum and kinetic enegy in otational collisions. Measue and calculate moments of inetia. Measue and calculate non-consevative wok

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

CDS 101/110: Lecture 7.1 Loop Analysis of Feedback Systems

CDS 101/110: Lecture 7.1 Loop Analysis of Feedback Systems CDS 11/11: Lctu 7.1 Loop Analysis of Fdback Systms Novmb 7 216 Goals: Intoduc concpt of loop analysis Show how to comput closd loop stability fom opn loop poptis Dscib th Nyquist stability cition fo stability

More information

Extinction Ratio and Power Penalty

Extinction Ratio and Power Penalty Application Not: HFAN-.. Rv.; 4/8 Extinction Ratio and ow nalty AVALABLE Backgound Extinction atio is an impotant paamt includd in th spcifications of most fib-optic tanscivs. h pupos of this application

More information

From Newton to Einstein. Mid-Term Test, 12a.m. Thur. 13 th Nov Duration: 50 minutes. There are 20 marks in Section A and 30 in Section B.

From Newton to Einstein. Mid-Term Test, 12a.m. Thur. 13 th Nov Duration: 50 minutes. There are 20 marks in Section A and 30 in Section B. Fom Newton to Einstein Mid-Tem Test, a.m. Thu. 3 th Nov. 008 Duation: 50 minutes. Thee ae 0 maks in Section A and 30 in Section B. Use g = 0 ms in numeical calculations. You ma use the following epessions

More information

SPH4U Unit 6.3 Gravitational Potential Energy Page 1 of 9

SPH4U Unit 6.3 Gravitational Potential Energy Page 1 of 9 SPH4 nit 6.3 Gavitational Potential negy Page of Notes Physics ool box he gavitational potential enegy of a syste of two (spheical) asses is diectly popotional to the poduct of thei asses, and invesely

More information

kg 2 ) 1.9!10 27 kg = Gm 1

kg 2 ) 1.9!10 27 kg = Gm 1 Section 6.1: Newtonian Gavitation Tutoial 1 Pactice, page 93 1. Given: 1.0 10 0 kg; m 3.0 10 0 kg;. 10 9 N; G 6.67 10 11 N m /kg Requied: Analysis: G m ; G m G m Solution: G m N m 6.67!10 11 kg ) 1.0!100

More information

F 12. = G m m 1 2 F 21 = F 12. = G m 1m 2. Review. Physics 201, Lecture 22. Newton s Law Of Universal Gravitation

F 12. = G m m 1 2 F 21 = F 12. = G m 1m 2. Review. Physics 201, Lecture 22. Newton s Law Of Universal Gravitation Physics 201, Lectue 22 Review Today s Topics n Univesal Gavitation (Chapte 13.1-13.3) n Newton s Law of Univesal Gavitation n Popeties of Gavitational Foce n Planet Obits; Keple s Laws by Newton s Law

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

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law AY 7A - Fall 00 Section Woksheet - Solutions Enegy and Keple s Law. Escape Velocity (a) A planet is obiting aound a sta. What is the total obital enegy of the planet? (i.e. Total Enegy = Potential Enegy

More information

c) (6) Assuming the tires do not skid, what coefficient of static friction between tires and pavement is needed?

c) (6) Assuming the tires do not skid, what coefficient of static friction between tires and pavement is needed? Geneal Physics I Exam 2 - Chs. 4,5,6 - Foces, Cicula Motion, Enegy Oct. 10, 2012 Name Rec. Inst. Rec. Time Fo full cedit, make you wok clea to the gade. Show fomulas used, essential steps, and esults with

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

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

Chap 5. Circular Motion: Gravitation

Chap 5. Circular Motion: Gravitation Chap 5. Cicula Motion: Gavitation Sec. 5.1 - Unifom Cicula Motion A body moves in unifom cicula motion, if the magnitude of the velocity vecto is constant and the diection changes at evey point and is

More information

Uniform Circular Motion

Uniform Circular Motion Unifom Cicula Motion constant speed Pick a point in the objects motion... What diection is the velocity? HINT Think about what diection the object would tavel if the sting wee cut Unifom Cicula Motion

More information

EE243 Advanced Electromagnetic Theory Lec # 22 Scattering and Diffraction. Reading: Jackson Chapter 10.1, 10.3, lite on both 10.2 and 10.

EE243 Advanced Electromagnetic Theory Lec # 22 Scattering and Diffraction. Reading: Jackson Chapter 10.1, 10.3, lite on both 10.2 and 10. Appid M Fa 6, Nuuth Lctu # V //6 43 Advancd ctomagntic Thoy Lc # Scatting and Diffaction Scatting Fom Sma Obcts Scatting by Sma Dictic and Mtaic Sphs Coction of Scatts Sphica Wav xpansions Scaa Vcto Rading:

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

PHYSICS 220. Lecture 08. Textbook Sections Lecture 8 Purdue University, Physics 220 1

PHYSICS 220. Lecture 08. Textbook Sections Lecture 8 Purdue University, Physics 220 1 PHYSICS 0 Lectue 08 Cicula Motion Textbook Sections 5.3 5.5 Lectue 8 Pudue Univesity, Physics 0 1 Oveview Last Lectue Cicula Motion θ angula position adians ω angula velocity adians/second α angula acceleation

More information

HW Solutions # MIT - Prof. Please study example 12.5 "from the earth to the moon". 2GmA v esc

HW Solutions # MIT - Prof. Please study example 12.5 from the earth to the moon. 2GmA v esc HW Solutions # 11-8.01 MIT - Pof. Kowalski Univesal Gavity. 1) 12.23 Escaping Fom Asteoid Please study example 12.5 "fom the eath to the moon". a) The escape velocity deived in the example (fom enegy consevation)

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 1114: Unit 5 Hand-out Homework (Answers)

Physics 1114: Unit 5 Hand-out Homework (Answers) Physics 1114: Unit 5 Hand-out Homewok (Answes) Poblem set 1 1. The flywheel on an expeimental bus is otating at 420 RPM (evolutions pe minute). To find (a) the angula velocity in ad/s (adians/second),

More information

13.10 Worked Examples

13.10 Worked Examples 13.10 Woked Examples Example 13.11 Wok Done in a Constant Gavitation Field The wok done in a unifom gavitation field is a faily staightfowad calculation when the body moves in the diection of the field.

More information

School of Electrical Engineering. Lecture 2: Wire Antennas

School of Electrical Engineering. Lecture 2: Wire Antennas School of lctical ngining Lctu : Wi Antnnas Wi antnna It is an antnna which mak us of mtallic wis to poduc a adiation. KT School of lctical ngining www..kth.s Dipol λ/ Th most common adiato: λ Dipol 3λ/

More information

b) (5) What average force magnitude was applied by the students working together?

b) (5) What average force magnitude was applied by the students working together? Geneal Physics I Exam 3 - Chs. 7,8,9 - Momentum, Rotation, Equilibium Nov. 3, 2010 Name Rec. Inst. Rec. Time Fo full cedit, make you wok clea to the gade. Show fomulas used, essential steps, and esults

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

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 235 Chapter 5. Chapter 5 Gravitation

Physics 235 Chapter 5. Chapter 5 Gravitation Chapte 5 Gavitation In this Chapte we will eview the popeties of the gavitational foce. The gavitational foce has been discussed in geat detail in you intoductoy physics couses, and we will pimaily focus

More information

PHYSICS NOTES GRAVITATION

PHYSICS NOTES GRAVITATION GRAVITATION Newton s law of gavitation The law states that evey paticle of matte in the univese attacts evey othe paticle with a foce which is diectly popotional to the poduct of thei masses and invesely

More information

Objects usually are charged up through the transfer of electrons from one object to the other.

Objects usually are charged up through the transfer of electrons from one object to the other. 1 Pat 1: Electic Foce 1.1: Review of Vectos Review you vectos! You should know how to convet fom pola fom to component fom and vice vesa add and subtact vectos multiply vectos by scalas Find the esultant

More information

θ θ φ EN2210: Continuum Mechanics Homework 2: Polar and Curvilinear Coordinates, Kinematics Solutions 1. The for the vector i , calculate:

θ θ φ EN2210: Continuum Mechanics Homework 2: Polar and Curvilinear Coordinates, Kinematics Solutions 1. The for the vector i , calculate: EN0: Continm Mchanics Homwok : Pola and Cvilina Coodinats, Kinmatics Soltions School of Engining Bown Univsity x δ. Th fo th vcto i ij xx i j vi = and tnso S ij = + 5 = xk xk, calclat: a. Thi componnts

More information

Motion in Two Dimensions

Motion in Two Dimensions SOLUTIONS TO PROBLEMS Motion in Two Dimensions Section 3.1 The Position, Velocity, and Acceleation Vectos P3.1 x( m) 0!3 000!1 70!4 70 m y( m)!3 600 0 1 70! 330 m (a) Net displacement x + y 4.87 km at

More information

Q Q N, V, e, Quantum Statistics for Ideal Gas. The Canonical Ensemble 10/12/2009. Physics 4362, Lecture #19. Dr. Peter Kroll

Q Q N, V, e, Quantum Statistics for Ideal Gas. The Canonical Ensemble 10/12/2009. Physics 4362, Lecture #19. Dr. Peter Kroll Quantum Statistics fo Idal Gas Physics 436 Lctu #9 D. Pt Koll Assistant Pofsso Dpatmnt of Chmisty & Biochmisty Univsity of Txas Alington Will psnt a lctu ntitld: Squzing Matt and Pdicting w Compounds:

More information

PS113 Chapter 5 Dynamics of Uniform Circular Motion

PS113 Chapter 5 Dynamics of Uniform Circular Motion PS113 Chapte 5 Dynamics of Unifom Cicula Motion 1 Unifom cicula motion Unifom cicula motion is the motion of an object taveling at a constant (unifom) speed on a cicula path. The peiod T is the time equied

More information

Sections and Chapter 10

Sections and Chapter 10 Cicula and Rotational Motion Sections 5.-5.5 and Chapte 10 Basic Definitions Unifom Cicula Motion Unifom cicula motion efes to the motion of a paticle in a cicula path at constant speed. The instantaneous

More information

Physics C Rotational Motion Name: ANSWER KEY_ AP Review Packet

Physics C Rotational Motion Name: ANSWER KEY_ AP Review Packet Linea and angula analogs Linea Rotation x position x displacement v velocity a T tangential acceleation Vectos in otational motion Use the ight hand ule to detemine diection of the vecto! Don t foget centipetal

More information

F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces.

F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces. 4.8. Cental foces The most inteesting poblems in classical mechanics ae about cental foces. Definition of a cental foce: (i) the diection of the foce F() is paallel o antipaallel to ; in othe wods, fo

More information

4.4 Linear Dielectrics F

4.4 Linear Dielectrics F 4.4 Lina Dilctics F stal F stal θ magntic dipol imag dipol supconducto 4.4.1 Suscptiility, mitivility, Dilctic Constant I is not too stong, th polaization is popotional to th ild. χ (sinc D, D is lctic

More information

b) (5) What is the magnitude of the force on the 6.0-kg block due to the contact with the 12.0-kg block?

b) (5) What is the magnitude of the force on the 6.0-kg block due to the contact with the 12.0-kg block? Geneal Physics I Exam 2 - Chs. 4,5,6 - Foces, Cicula Motion, Enegy Oct. 13, 2010 Name Rec. Inst. Rec. Time Fo full cedit, make you wok clea to the gade. Show fomulas used, essential steps, and esults with

More information

Free carriers in materials

Free carriers in materials Lctu / F cais in matials Mtals n ~ cm -3 Smiconductos n ~ 8... 9 cm -3 Insulatos n < 8 cm -3 φ isolatd atoms a >> a B a B.59-8 cm 3 ϕ ( Zq) q atom spacing a Lctu / "Two atoms two lvls" φ a T splitting

More information

Gravitation. Chapter 12. PowerPoint Lectures for University Physics, Twelfth Edition Hugh D. Young and Roger A. Freedman. Lectures by James Pazun

Gravitation. Chapter 12. PowerPoint Lectures for University Physics, Twelfth Edition Hugh D. Young and Roger A. Freedman. Lectures by James Pazun Chapte 12 Gavitation PowePoint Lectues fo Univesity Physics, Twelfth Edition Hugh D. Young and Roge A. Feedman Lectues by James Pazun Modified by P. Lam 5_31_2012 Goals fo Chapte 12 To study Newton s Law

More information

Overview. 1 Recall: continuous-time Markov chains. 2 Transient distribution. 3 Uniformization. 4 Strong and weak bisimulation

Overview. 1 Recall: continuous-time Markov chains. 2 Transient distribution. 3 Uniformization. 4 Strong and weak bisimulation Rcall: continuous-tim Makov chains Modling and Vification of Pobabilistic Systms Joost-Pit Katon Lhstuhl fü Infomatik 2 Softwa Modling and Vification Goup http://movs.wth-aachn.d/taching/ws-89/movp8/ Dcmb

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

CBSE-XII-2013 EXAMINATION (MATHEMATICS) The value of determinant of skew symmetric matrix of odd order is always equal to zero.

CBSE-XII-2013 EXAMINATION (MATHEMATICS) The value of determinant of skew symmetric matrix of odd order is always equal to zero. CBSE-XII- EXAMINATION (MATHEMATICS) Cod : 6/ Gnal Instuctions : (i) All qustions a compulso. (ii) Th qustion pap consists of 9 qustions dividd into th sctions A, B and C. Sction A compiss of qustions of

More information

Chapter 5: Uniform Circular Motion

Chapter 5: Uniform Circular Motion Chapte 5: Unifom Cicula Motion Motion at constant speed in a cicle Centipetal acceleation Banked cuves Obital motion Weightlessness, atificial gavity Vetical cicula motion Centipetal Foce Acceleation towad

More information