Average acceleration  =  (change in speed)  /  (time for the change)
The missile's change in speed is  (5,000 - 0)  =  5,000 m/s
Average acceleration  =  (5,000 m/s)  /  (10 sec)
                                  =      500 m/s²       (about  51 Gs) 
Inconveniently, this isn't one of the choices on the list. Is there something wrong, either with the choices or with my solution ?
No. Relax. Everything is OK.
500 meters is the same thing as 0.5 kilometer.  So my answer can also be written as  0.5 km/s² .  That doesn't change anything, and it IS one of the listed choices.
The average acceleration is <em>0.5 km/sec²  (d)</em> .
 
        
                    
             
        
        
        
Answer:
As wind or an ocean current moves, the Earth spins underneath it. ... The Coriolis effect bends the direction of surface currents to the right in the Northern Hemisphere and left in the Southern Hemisphere.
Explanation:
The Coriolis effect causes winds and currents to form circular patterns.
 
        
             
        
        
        
Answer:
741 J/kg°C
Explanation:
Given that
Initial temperature of glass, T(g) = 72° C
Specific heat capacity of glass, c(g) = 840 J/kg°C
Temperature of liquid, T(l)= 40° C
Final temperature, T(2) = 57° C
Specific heat capacity of the liquid, c(l) = ?
Using the relation 
Heat gained by the liquid = Heat lost by the glass 
m(l).C(l).ΔT(l) = m(g).C(g).ΔT(g)
Since their mass are the same, then
C(l)ΔT(l) = C(g)ΔT(g)
C(l) = C(g)ΔT(g) / ΔT(l)
C(l) = 840 * (72 - 57) / (57 - 40)
C(l) = 12600 / 17
C(l) = 741 J/kg°C
 
        
             
        
        
        
Explanation:
It is given that,
Focal length of the concave mirror, f = -13.5 cm
Image distance, v = -37.5 cm (in front of mirror)
Let u is the object distance. It can be calculated using the mirror's formula as :



u = -21.09 cm
The magnification of the mirror is given by :


m = -1.77 
So, the magnification produced by the mirror is (-1.77). Hence, this is the required solution.
 
        
             
        
        
        
Answer:
Stellar black holes form when the center of a very massive star collapses in upon itself.