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∙ 14y agoSince a billion light years is 1000 times a million, that means that you simply have to multiply 1000 x 22 km/sec, with a result of 22,000 km/sec.
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∙ 14y agoThe recessional velocity of a galaxy at a distance of 1 billion light years would be calculated using Hubble's Law by multiplying the Hubble constant (H0) with the distance.
Recessional velocity = H0 x distance = 22 km/s/Mly x 1,000 Mly = 22,000 km/s
Therefore, the recessional velocity of a galaxy at 1 billion light years would be 22,000 km/s.
Two different distance-time graphs have matching velocity-time graphs when the slope of the distance-time graph represents the velocity in the velocity-time graph, as velocity is the derivative of distance with respect to time. This means that the steeper the distance-time graph, the greater the velocity on the velocity-time graph at that point.
Velocity is in distance/time, so multiplied by 1/distance would give you 1/time. Hope this helps!
To calculate distance with velocity and weight, you can use the equation for work: Work = Force x Distance. The force can be calculated by multiplying the weight with gravity. Velocity can then be used to determine the time it takes for the object to travel that distance using the equation Distance = Velocity x Time.
Velocity is the rate of change of distance over time. This relationship is described by the equation velocity = distance/time, where velocity is measured in units like meters per second, distance is measured in units like meters, and time is measured in units like seconds. As velocity increases, the distance covered in a given amount of time also increases.
The equation that relates the distance traveled by a constantly accelerating object to its initial velocity, final velocity, and time is the equation of motion: [ \text{distance} = \frac{1}{2} \times (\text{initial velocity} + \text{final velocity}) \times \text{time} ] This equation assumes constant acceleration.
The recession velocity of a galaxy at a distance of 200 Mpc (mega-parsecs) would depend on Hubble's Law and the rate of expansion of the universe. For a rough estimate, assuming a Hubble constant of 70 km/s/Mpc, the recession velocity would be around 14,000 km/s.
To find the time when you know the distance and velocity but not the time, you should divide distance by velocity. This is because time equals distance divided by velocity (time = distance/velocity).
Velocity = distance / unit of time
Simple, velocity = distance by time ,which probably means distance = velocity X times.
distance/velocity = time
Velocity is the rate at which an object changes its position, regardless of the distance it has traveled. Velocity considers both speed and direction, so a change in direction can affect velocity even if distance remains constant. Distance is the total length of the path traveled, whereas velocity focuses on the rate of change in position.
The formula for uniform velocity is: Velocity = Distance / Time.
Velocity includes direction. And it's the 'difference', not the 'distance'.
velocity = distance travelled/time taken to travel that distance
velocity = distance/time
Velocity is distance / time
Distance Traveled is directly proportional to velocity. This is because velocity is the change in position over a period of time. The greater the velocity, the greater the distance traveled. For you calculus junkies, integrate velocity to get displacement.