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Given that, relative to the geocentric equatorial frame, r=-6634.2 I - 1261.8 J -5230.9 K (km)...
Problem 4) (a bit tricky!) Given r= -50000,-10000, km 1 × ū2. (μ = where 1: 2: u3 form a right-handed coordinate system such that Uz = 398600 kins/s?) a) Find the true anomaly θ. b) Find the eccentricity vector e of the orbit c) Is the (û,coordinate set the same as the perifocal coordinate frame (p, 4. W)? Why or why not?
An object's position is given by r(t) = (150-t2 + 1/12t3)i + (200+5t-2.5t2, + 1/18t3)j where t is in seconds and r is in m. Determine the object's velocity at t = 4.0 s. Determine the object's acceleration any time t. The orbital speed of a satellite orbiting Mars at an altitude of 1.06 times 10'm above the surface was measured to be 1.75 km/s. The radius of Mars is 3.39 times 106 m Determine the mass of Mars A...
(1 point) Given R(t)=e4tcos(3t)i+e4tsin(3t)j+3e4tkR(t)=e4tcos(3t)i+e4tsin(3t)j+3e4tk Find the derivative R′(t)R′(t) and norm of the derivative. R′(t)=R′(t)= ∥R′(t)∥=‖R′(t)‖= Then find the unit tangent vector T(t)T(t) and the principal unit normal vector N(t)N(t) T(t)=T(t)= N(t)=N(t)= (1 point) Given R(t) = cos(36) i + e sin(3t) 3 + 3e"k Find the derivative R') and norm of the derivative. R'(t) = R' (t) Then find the unit tangent vector T(t) and the principal unit normal vector N() T(0) N() Note: Yn can can on the hom
Given the position vector r(t), determine v,lv. a, T,K : r = r(t) (1 + et)i + e Given the position vector r(t), determine v,lv. a, T,K : r = r(t) (1 + et)i + e
of meters. 30. Given these two vectors A (3.00)i + (7.00)j - (4. 00) k and B (2.00)i - (4.50)j + (3. 00) k: a. Calculate A. B Calculate A >< B b. Calculate the angle between A and B Determine by calculation if the vector c. is perpendicular to B. d. Calculate a unit vector that points in the direction of the vector-A
Given M 5 i +4- 3 k and N 6 i- 3 j - k, calculate the vector product M x N. 8 Review the definition of the cross product in term of components. i + Need Help? LReadIt 11 watch lt
(1 point) Given the acceleration vector a(t) = (-4 cos (2t))i + (-4 sin (2t))j + (-3t) k , an initial velocity of v (0) =i+ k, and an initial position of r (0)=i+j+ k, compute: A. The velocity vector v (t) = j+ . B. The position vector r(t) = j+ k
i+j+k A charge q moving with speed v enters a region of constant magnetic field given by B-B The unit vector in the i-23+3 direction of the velocity vector is given by n- If an electric feld E is applied such that the charge experiences zero resultant force while it is moving through the electric magnetic fields, then the unit vector in the direction of the electric field is B)-(4부) i+j+k i-2j+k
Table 13.1 Solar system data (in SI units and relative to Earth) Orbit eccentricity Mass Equatorial radius semimajor axis period (a^) (years) 30 Sun 2.0 X 10 3.3 × 10 Mercury 3.30 X 1023 Venus 4.87 X 1024 Earth Mars Jupiter 1.90 x 1027318 Saturn 5.68 × 1026 95.2 Uranus 8.68 X 1014.5 Neptune 1.02 x 102617.1 Pluto 2.440 ×106 6.052 X 106 6.378 X 106 3.396 × 106 5.79×1010 1.082 x 1011 1.496 × 1011 2.279 ×1011 11.2 7.783...
If C is the curve given by r (t) = (1 + 4 sin t)i + (1+2 sin2t)j + (1 + 3 sin3t) k, 0≤t≤π/2 and F is the radial vector field F(x, y, z) = xi + yj + zk, compute the work done by F on a particle moving along C.