Answer:
4 amps
Explanation: ohms law
B.Power is the force of work over a certain distance.
C.Power is the rate at which work is accomplished.
D.Power is the energy supplied in a force.
Answer:
Explanation:
Initial velocity , u = 27 m/s
displacement before stop, s = 41.5 m .
final velocity, v = 0
acceleration a = ?
v² = u² + 2 a s
0 = 27² + 2 x a x 41.5
a = - 27² / 2 x 41.5
= - 8.78 m /s
Answer:
The centripetal acceleration of Deimos is .
Explanation:
The centripetal acceleration is defined as:
(1)
Where v is the velocity of Deimos and r is the orbital distance.
Notice that is necessary to determine the velocity first.
The speed of the Deimos can be found by means of the Universal law of gravity:
(2)
Then, replacing Newton's second law in equation 2 it is gotten:
(3)
However, a is the centripetal acceleration since Deimos almost describes a circular motion around Mars:
(4)
Replacing equation 4 in equation 3 it is gotten:
(5)
Where v is the orbital speed, G is the gravitational constant, M is the mass of Mars, and r is the orbital radius.
Finally, equation 4 can be used:
Hence, the centripetal acceleration of Deimos is .
The centripetal acceleration of Deimos, one of Mars' moon, can be calculated using its orbital period and distance from Mars. Convert the time units to seconds and use the formulas for velocity and centripetal acceleration to get an answer of approximately 7.84x10^-5 m/s^2.
To find the centripetal acceleration of Deimos, we can use the formula for centripetal acceleration, which is a =v^2/r , where v is the velocity and r is the radius (distance from Mars to Deimos). The velocity can be found using the formula v = 2πr/T, where T is the period (time for one complete orbit).
First, convert the days into seconds because the SI unit of time in physics is second. So, 1.26 days = 1.26 * 24 * 60 * 60 = 108864 seconds.
Then, calculate the velocity: v = 2 * π * 2.35x10^7m / 108864s = 1.36 km/s.
Finally, substitute v and r into the centripetal acceleration formula: a = (1.36x10^3m/s)^2 / 2.35x10^7m = 7.84x10^-5 m/s^2.
The centripetal acceleration of Deimos is approximately 7.84x10^-5 m/s^2.
#SPJ3
Answer: cluster
Explanation:
There are four main shapes of galaxies: spiral, galaxies are divided into four main groups: spiral, lenticular, elliptical, and irregular, elliptical, and irregular.
The least common shape is cluster
Spiral galaxies- These are the most common. These have arms extending from a bright bulge in spiral shape.
Elliptical galaxy have ellipsoidal shape.
Lenticular galaxies - Intermediate between elliptical and spiral galaxies.
Irregular shape- No well defined shape
Spherical - Nearly spherical galaxies. These are least
cluster- group of galaxies having irregular shape is the least common shape.
Question: The least common shape for a galaxy _____.
Answer:Cluster
Answer:
10 seconds
Explanation:
Hope this is right and that it helps.
You see if the skier is going 250 meters a second 250 times 10 is 2500 so it would take the skier 10 seconds.
Answer:
Explanation:
distance = 2500 meters
velocity = 250 meter/second
time = distance / velocity
= 2500 meters
250 meter/second
= 10 sec.