Position Vector Formula

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Position vector is often used to represent the location of a satellite in space. The position vector provides information about the satellite's position relative to a reference point. Check FAQs
rpos=amajor(1-e2)1+ecos(v)
rpos - Position Vector?amajor - Major Axis?e - Eccentricity?v - True Anomaly?

Position Vector Example

With values
With units
Only example

Here is how the Position Vector equation looks like with Values.

Here is how the Position Vector equation looks like with Units.

Here is how the Position Vector equation looks like.

9.6936Edit=10.75Edit(1-0.12Edit2)1+0.12Editcos(0.684Edit)
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Position Vector Solution

Follow our step by step solution on how to calculate Position Vector?

FIRST Step Consider the formula
rpos=amajor(1-e2)1+ecos(v)
Next Step Substitute values of Variables
rpos=10.75m(1-0.122)1+0.12cos(0.684s)
Next Step Prepare to Evaluate
rpos=10.75(1-0.122)1+0.12cos(0.684)
Next Step Evaluate
rpos=9.69363246830535m
LAST Step Rounding Answer
rpos=9.6936m

Position Vector Formula Elements

Variables
Functions
Position Vector
Position vector is often used to represent the location of a satellite in space. The position vector provides information about the satellite's position relative to a reference point.
Symbol: rpos
Measurement: LengthUnit: m
Note: Value should be greater than 0.
Major Axis
The Major Axis refers to the longer dimension or principal axis of an elliptical coverage area or beam pattern.
Symbol: amajor
Measurement: LengthUnit: m
Note: Value should be greater than 0.
Eccentricity
Eccentricity refers to a characteristic of the orbit followed by a satellite around its primary body, typically the Earth.
Symbol: e
Measurement: NAUnit: Unitless
Note: Value should be between 0 to 1.
True Anomaly
True Anomaly is an angular parameter that defines the position of a body moving along a keplerian orbit.
Symbol: v
Measurement: TimeUnit: s
Note: Value should be greater than 0.
cos
Cosine of an angle is the ratio of the side adjacent to the angle to the hypotenuse of the triangle.
Syntax: cos(Angle)

Other formulas in Satellite Orbital Characteristics category

​Go Anomalistic Period
TAP=2πn
​Go Local Sidereal Time
LST=GST+Elong
​Go Mean Anomaly
M=E-esin(E)
​Go Mean Motion of Satellite
n=[GM.Earth]asemi3

How to Evaluate Position Vector?

Position Vector evaluator uses Position Vector = (Major Axis*(1-Eccentricity^2))/(1+Eccentricity*cos(True Anomaly)) to evaluate the Position Vector, The Position Vector formula specify the motion of the satellite in the orbital plane and only the magnitude of position vector is used for measurements. Position Vector is denoted by rpos symbol.

How to evaluate Position Vector using this online evaluator? To use this online evaluator for Position Vector, enter Major Axis (amajor), Eccentricity (e) & True Anomaly (v) and hit the calculate button.

FAQs on Position Vector

What is the formula to find Position Vector?
The formula of Position Vector is expressed as Position Vector = (Major Axis*(1-Eccentricity^2))/(1+Eccentricity*cos(True Anomaly)). Here is an example- 11.96237 = (10.75*(1-0.12^2))/(1+0.12*cos(0.684)).
How to calculate Position Vector?
With Major Axis (amajor), Eccentricity (e) & True Anomaly (v) we can find Position Vector using the formula - Position Vector = (Major Axis*(1-Eccentricity^2))/(1+Eccentricity*cos(True Anomaly)). This formula also uses Cosine (cos) function(s).
Can the Position Vector be negative?
No, the Position Vector, measured in Length cannot be negative.
Which unit is used to measure Position Vector?
Position Vector is usually measured using the Meter[m] for Length. Millimeter[m], Kilometer[m], Decimeter[m] are the few other units in which Position Vector can be measured.
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