That would depend on how far the two points are seperated. Miles or meters BIG difference.
It would be VERY STUPID to measure ten miles using a 30cm ruler.
The distance between two points is the distance between them. It doesn't depend on the method an object uses to move between the two points. It also doesn't depend on what route an object follows between them, or even whether or not anything moves between the two points. The distance between the earth and the Orion Nebula is the distance, even though no object has ever moved between the earth and the Orion Nebula.
lengthThe distance between two points is called the displacement.
I assume you refer to the distance between the points.I assume you refer to the distance between the points.I assume you refer to the distance between the points.I assume you refer to the distance between the points.
Yes, the x-distance, y-distance, z-distance, or any combination of the three between any two points may be zero Not possible. If the distance between two points is zero then the points are the same.
the distance between two points is length
The distance between identical points on a wave is called wavelength.
In plane geometry, the shortest distance between two points is a line. In spherical geometry, the shortest distance between two points is a segment of a great circle. The distance between one point and another is known as the displacement.
The metric of a geometric space is defined as the distance between two points.
The distance between these two points is termed as a wavelength.
distance is the measure of the length between two points where as displacement is the shortest distance between the points.
In plane geometry, the shortest distance between two points is a line. In spherical geometry, the shortest distance between two points is a segment of a great circle. The distance between one point and another is known as the displacement.
The most accurate way to determine the distance to a nearby galaxy is by using the method of parallax, which involves measuring the slight shift in the position of the galaxy as observed from different points in Earth's orbit around the Sun. This method allows astronomers to calculate the distance based on the angle of the shift and the known distance between the observation points.