Q3: (a) Determined kind of motion for the following motion from between brattices. (1) n (q,)= n(Fredumd deg res) is (Holonomial, Sikleronomial , reuohonomia l) (2) Y= a sin 0 is (Holonomial, Sikleronomial, reuohonomial) (3) Y= a sin ot + 6t is (Holonomial, Sikleronomial , reuohonomial) (b) Lagrange equation of motion for the sun around the arts as ()i-ro- %3D (2)r+ ro. 2µ 0. dt (3)r-ro = 0. (c) Lagrange equation of motion for the simple pendulum as. (1) 0.= -E sin e (2) 0. =-4 cos e (3) 0.= = -2 tan e.
Q3: (a) Determined kind of motion for the following motion from between brattices. (1) n (q,)= n(Fredumd deg res) is (Holonomial, Sikleronomial , reuohonomia l) (2) Y= a sin 0 is (Holonomial, Sikleronomial, reuohonomial) (3) Y= a sin ot + 6t is (Holonomial, Sikleronomial , reuohonomial) (b) Lagrange equation of motion for the sun around the arts as ()i-ro- %3D (2)r+ ro. 2µ 0. dt (3)r-ro = 0. (c) Lagrange equation of motion for the simple pendulum as. (1) 0.= -E sin e (2) 0. =-4 cos e (3) 0.= = -2 tan e.
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![Q3: (a) Determined kind of motion for the following motion from between brattices.
(1) n (q,)= n(Fredumd deg res) is (Holonomial, Sikleronomial , reuohonomia l)
(2) Y= a sin 0 is (Holonomial, Sikleronomial, reuohonomial)
(3) Y= a sin ot + 6t is (Holonomial, Sikleronomial , reuohonomial)
(b) Lagrange equation of motion for the sun around the arts as
(1)i-ro
0.
%3D
(2)r+ ro.
2µ
0.
dt
(3)-ro
-学,)-。
= 0.
(c) Lagrange equation of motion for the simple pendulum as.
(1) 0.= -B sin e
(2) ö.
=-4
(3) д.-
= -2 tan e.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F22a6d1fc-3f76-4cab-9306-603fbaee2deb%2F14da57b7-b192-441a-811d-1c258b6de0ea%2Fzoz7hp_processed.jpeg&w=3840&q=75)
Transcribed Image Text:Q3: (a) Determined kind of motion for the following motion from between brattices.
(1) n (q,)= n(Fredumd deg res) is (Holonomial, Sikleronomial , reuohonomia l)
(2) Y= a sin 0 is (Holonomial, Sikleronomial, reuohonomial)
(3) Y= a sin ot + 6t is (Holonomial, Sikleronomial , reuohonomial)
(b) Lagrange equation of motion for the sun around the arts as
(1)i-ro
0.
%3D
(2)r+ ro.
2µ
0.
dt
(3)-ro
-学,)-。
= 0.
(c) Lagrange equation of motion for the simple pendulum as.
(1) 0.= -B sin e
(2) ö.
=-4
(3) д.-
= -2 tan e.
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