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Nội dung text 8. GRAVITATION_KEY _ SOLUTIONS (132-143).pmd.pdf

Olympiad Class Work Book VIII – Physics (Vol – III) GRAVITATION WORK SHEET -1 KEY CUQ: 1) 3 2)4 3)1 4)1 5)2 6)2 7)3 8) 1 9)3 10)1 JEE MAINS AND ADVANCED: 1) 4 2)4 3)2 4)3 5)2 6)1 7)4 8)3 9) 1 10)2 11)2 12)3 13)1 14)3 15)1 16)3 17)3 18) 3 19)a-t;b-q;c-p;d-r 20)1,2,3 21)1,2,3 22)3 23)2 24)1 25)a-p;b-q;c-s;d-q SOLUTIONS 1. 2 mM F G d    2 2 3 ' G m M GmM F d d     2     3 1 4 GMm F xf d x  4 2. The gravitational force is maximum when the mass is divided into equal parts 3.   11   4 1 1 6.67 10 10 F      7 F N 6.67 10   4. 1 2 2 m m F G r  2 . . m m F G d  6. 2 1 F r  Force decreases by 4 times 1 2 F N  7. Intensity of gravitational field inside the follow spherical shell is zero 8. 1 2 E E E net              2 2 4 8 2 4 G G   2 G    G 2 G   2 net G E   9. The vectors 1 2 3 E E E , ,    Form a closed polygon (triangle) Hence resultant gravitational field E  0  10.   3 5 2 2 10 10 2 G G x x       2 2 2 1 10 x x 2    2 2 x x   2 100. 9 2 x   2 9 x   x x    2 10 11 2 x  2 11 x m  11. 11 G N 6.67 10   7 F N 6.67 10       2 1 4 10 m m F G  

Olympiad Class Work Book VIII – Physics (Vol – III) 23. F F F net  1 2             2 2 1 2 2 3 2 6 4 1 1      G G G G 11 11 4 6.67 10 26.68 10        N 24. F F F net  1 2           2 2 1 3 2 3 27 2 1 4    G G G 11 45.02 10 N    25.      2 2 2 4 3 3 2         net G m m Gm a F a a b F  net  0   2 2 c F F F F F F net     1 2 1 2 2 cos 3  2 2 3Gm a  d F  net  0 WORKSHEET-2 KEY CUQ: 1)3 2)1 3)2 4)3 5)1 6)1 7)1 8)2 JEE MAINS AND ADVANCED: 1) 3 2)1 3) 4 4) 1 5) 3 6) 1 7) 2 8) 2 9) 3 10) 3 11) 4 12) 4 13) 2 14) 3 15) 4 16) a-r;b-q;c-p;d-s 17) 1,3 18) 1,2,3,4 19) 1 20) 1 21) 2 22) 2 23) 3 24) 3 25) 1 26) 2,3 27) a-r;b-p;c-q;d-t SOLUTIONS 1.   2 2 g R ' g R h     2 2 1 ' 2 2     g R g R h   2 2 1 2 R R h    2 2 R h R   2 R h R   2 R h R h R       2 1 0.414  2. d 1 d g g R         4 d g g  1 4 g d g R         3 3 4 4   d R R   3 6400 3 1600 4800 4     km 3. 64 ' 100 g g     2 2 ' 64 100 g R g R h    8 10 R R h   10 8 8 R R h   2 8 R h
VIII – Physics (Vol – III) Olympiad Class Work Book 2 6400 1600 8 4 4     R R h km 4. | 2 2 g g R cos     1 2 2 g g R cos     3 2 2 2 R R cos 4     3 0 cos 30 2      5. 2 2 g g Rw cos     0 g    0, 45   2 2 g R w   cos 2 2 R g w  2g w R  6. w mg    2 2 2 2 ' 4 g R R g R R R    ' 4 g g  ' ' 4 4    mg w w mg 7. d 1 d g g R         2 R d  2 d g g  100 50 2 2 d mg mg N    8.   2 1 GM g R        1 2 2 5 4 g GM R            dividing 1 & 2     1 80 1 M m  9. d 1 d g g R         1 g d g n R         1 1      1 1 d d n R R n n 1 d R n         10. 2 2 2         P p GM GM g R D 2 4 p p GM g D  11.   2 2 g R ' g R h   ' 16 g g    2 2 1 16 R R h   1 4 R R h   4 3 R R h h R     12. 2 1 1 h d R R    d h  2

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