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Radius Vector শব্দের বাংলা অর্থ: ব্যাসার্ধ ভেক্টর
Radius Vector Meaning In Bengali ব্যাসার্ধ ভেক্টর
Radius Vector
দূরক,
Definition
1) In mathematics, a radius vector is a line segment between the origin and a point in three-dimensional space, used to describe the position of that point.
2) In physics, a radius vector is a vector that describes the position of a particle in a given coordinate system, typically originating from the origin.
3) In astronomy, a radius vector is a geometric concept that describes the position of a celestial body in its orbit relative to the point of reference, typically the focal point of its elliptical path.
Examples
Radius Vector Example in a sentence
1) The radius vector of the circle points directly from the center to any point on its circumference.
2) In physics, the displacement of an object can be represented by a radius vector.
3) The radius vector of a planet describes its position relative to the sun.
4) To find the area of a sector of a circle, you need the angle and the length of the radius vector.
5) The vector sum of two radius vectors can be used to find the resultant displacement.
6) The radius vector of a satellite in orbit around Earth changes as it moves.
7) The magnitude of a radius vector is equal to the distance from the origin.
8) The position of a ship at sea can be determined using a radius vector relative to a fixed point.
9) By analyzing the radius vector, astronomers can track the movement of celestial bodies.
10) The radius vector in polar coordinates is often denoted by the symbols (r, θ).
Part of Speech
Radius Vector (Noun)
Synonyms
Distal , Radius Vector - (SYNONYM) দূরক
Encyclopedia
In mathematics, a radius vector is a line segment between the origin and a point in three-dimensional space, used to describe the position of that point.
In physics, a radius vector is a vector that describes the position of a particle in a given coordinate system, typically originating from the origin.
In astronomy, a radius vector is a geometric concept that describes the position of a celestial body in its orbit relative to the point of reference, typically the focal point of its elliptical path.
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