Answer:
Mp= 1.48×10^23 Kg and M = 4.47×10^30 Kg
Explanation:
Given that
Diameter of planet D = 1.8×10^6m
Radius of planet Rp = 0.9×10^6m
Period of rotation of planet = 22.3 hrs = 80280s
Radius of orbit r = 2.2 × 10^11 m
Period of revolution around star T =432days = 432×24×60×60 = 37324800s
Acceleration of gravity on the surface of planet gp = 12.2m/s^2
gp = GMp/(Rp)^2
Mp = gp×(Rp)^2 /G
= 12.2 * (0.9*10^6)^2 ÷ 6.67×10^-11
9.882×10^12 ÷ 6.67×10^-11
Mp= 1.4×10^23 Kg
To determine the mass of the star, we consider the revolution of the planet around the star with period T
T^2 = (4π^2/GM)r^3
M = 4π^2r^3 ÷ GT^2
M = 4π^2* (2.2×10^11)^3 ÷ 6.67×10^-11 × ( 37324800)^2
M= 4.47×10^30 Kg
Remember that the total
velocity of the motion is the vector sum of the velocity you would have in
still water and the stream. Always place the vectors carefully to be able to
come up with an accurate sum vector.
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Answer:
The last option is correct
ΔT1 = 4 sec ΔT2 = 4 sec ΔT3 = 4 sec
S = V0 t + 1/2 a t^2
S1 = 1/2 a t^2 = 8 a where V0 is the speed at the start of the interval
During any interval (of 4 sec) the particle travels 1/2 a t^2 = 8 a due to its acceleration - and you need to include the speed at the start of the interval
S1 = 8a
S2 = 8 a + 8 a = 16 a
S3 = 16 a + 8 a = 24 a
Note: V2 = V1 + a t for any interval
V2 - V1 = V1 + a t - V1 = a t
and a = (V2 - V1) / t = a the speed increase is constant during the interval
Yeah we always see the same side of the moon because it orbits around earth with that side constantly facing earth, if that's not your question than just comment and i'll try to answer...