Position vector in spherical coordinates

In summary, a position vector in spherical coordinates is a way of representing the position of a point in space using three parameters: radius, inclination, and azimuth. It is commonly used in physics and mathematics to describe the location of objects in three-dimensional space. The radius represents the distance from the origin, while the inclination is the angle between the vector and the positive z-axis, and the azimuth is the angle between the projection of the vector onto the xy-plane and the positive x-axis. This coordinate system is useful for describing objects with spherical symmetry and is often used in celestial mechanics and astronomy.
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xoxomae
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Is the position vector r=xi+yj+zk just r=rerin spherical coordinates?
 
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Yes. Note however that, unlike in the Cartesian representation, we can't use that to tell us where the point is, because we first need to know where the point is to know what vector ##\mathbf e_r## is.
 
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Related to Position vector in spherical coordinates

1. What is a position vector in spherical coordinates?

A position vector in spherical coordinates is a mathematical representation of a point in three-dimensional space using three coordinates: radius (r), inclination (θ), and azimuth (φ). It is used to describe the location of a point relative to a fixed origin.

2. How is a position vector in spherical coordinates different from a position vector in Cartesian coordinates?

In Cartesian coordinates, a position vector is represented as (x, y, z), where x, y, and z are the distances from the origin in the x, y, and z directions respectively. In spherical coordinates, the position vector is represented as (r, θ, φ), where r is the distance from the origin, θ is the angle from the positive z-axis, and φ is the angle from the positive x-axis. So, while both systems use three coordinates, the way they are measured and represented is different.

3. How do you convert a position vector in spherical coordinates to Cartesian coordinates?

To convert a position vector in spherical coordinates to Cartesian coordinates, we use the following formulas:
x = r sinθ cosφ
y = r sinθ sinφ
z = r cosθ
Here, r is the distance from the origin, θ is the angle from the positive z-axis, and φ is the angle from the positive x-axis.

4. What is the range of values for the coordinates in a position vector in spherical coordinates?

The range of values for the coordinates in a position vector in spherical coordinates are as follows:
r: r ≥ 0 (r cannot be negative as it represents a distance)
θ: 0 ≤ θ ≤ π (θ is the inclination angle, so it ranges from 0 to 180 degrees)
φ: 0 ≤ φ ≤ 2π (φ is the azimuth angle, so it ranges from 0 to 360 degrees)

5. In what fields is the use of position vectors in spherical coordinates most common?

Position vectors in spherical coordinates are commonly used in fields such as astronomy, physics, and engineering. They are especially useful in situations where the location of a point needs to be described in a spherical system, such as the position of planets, stars, or satellites in space.

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