Attractive Force Potentials per unit Mass for Sun Solution

STEP 0: Pre-Calculation Summary
Formula Used
Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)/Distance of Point
Vs = (f*Msun)/rS/MX
This formula uses 4 Variables
Variables Used
Attractive Force Potentials for Sun - Attractive Force Potentials for Sun is referred to the gravitational force exerted by the Sun on an object and can be described by the gravitational potential.
Universal Constant - Universal Constant is a physical constant that is thought to be universal in its application in terms of Radius of the Earth and Acceleration of Gravity.
Mass of the Sun - (Measured in Kilogram) - Mass of the Sun defined as the total amount of matter that the Sun contains. This includes all of its components, such as hydrogen, helium, and trace amounts of heavier elements.
Distance of Point - (Measured in Meter) - Distance of Point refers to the point located on the surface of the Earth to the center of the Sun or the Moon.
STEP 1: Convert Input(s) to Base Unit
Universal Constant: 2 --> No Conversion Required
Mass of the Sun: 1.989E+30 Kilogram --> 1.989E+30 Kilogram No Conversion Required
Distance of Point: 256 Kilometer --> 256000 Meter (Check conversion ​here)
STEP 2: Evaluate Formula
Substituting Input Values in Formula
Vs = (f*Msun)/rS/MX --> (2*1.989E+30)/256000
Evaluating ... ...
Vs = 1.55390625E+25
STEP 3: Convert Result to Output's Unit
1.55390625E+25 --> No Conversion Required
FINAL ANSWER
1.55390625E+25 1.6E+25 <-- Attractive Force Potentials for Sun
(Calculation completed in 00.004 seconds)

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Created by Mithila Muthamma PA
Coorg Institute of Technology (CIT), Coorg
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Attractive Force Potentials Calculators

Attractive Force Potentials per unit Mass for Moon
​ LaTeX ​ Go Attractive Force Potentials for Moon = (Universal Constant*Mass of the Moon)/Distance of Point
Mass of Moon given Attractive Force Potentials
​ LaTeX ​ Go Mass of the Moon = (Attractive Force Potentials for Moon*Distance of Point)/Universal Constant
Attractive Force Potentials per unit Mass for Sun
​ LaTeX ​ Go Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)/Distance of Point
Mass of Sun given Attractive Force Potentials
​ LaTeX ​ Go Mass of the Sun = (Attractive Force Potentials for Sun*Distance of Point)/Universal Constant

Attractive Force Potentials per unit Mass for Sun Formula

​LaTeX ​Go
Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)/Distance of Point
Vs = (f*Msun)/rS/MX

What do you mean by Tidal Force?

The Tidal Force is a gravitational effect that stretches a body along the line towards the center of mass of another body due to a gradient (difference in strength) in gravitational field from the other body; it is responsible for diverse phenomena, including tides, tidal locking, breaking apart of celestial bodies.

How to Calculate Attractive Force Potentials per unit Mass for Sun?

Attractive Force Potentials per unit Mass for Sun calculator uses Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)/Distance of Point to calculate the Attractive Force Potentials for Sun, The Attractive Force Potentials per unit Mass for Sun formula is defined as to make potential energy of system decrease. As atoms first begin to interact, attractive force is stronger than repulsive force and so potential energy of system decreases. Attractive Force Potentials for Sun is denoted by Vs symbol.

How to calculate Attractive Force Potentials per unit Mass for Sun using this online calculator? To use this online calculator for Attractive Force Potentials per unit Mass for Sun, enter Universal Constant (f), Mass of the Sun (Msun) & Distance of Point (rS/MX) and hit the calculate button. Here is how the Attractive Force Potentials per unit Mass for Sun calculation can be explained with given input values -> 1.6E+25 = (2*1.989E+30)/256000.

FAQ

What is Attractive Force Potentials per unit Mass for Sun?
The Attractive Force Potentials per unit Mass for Sun formula is defined as to make potential energy of system decrease. As atoms first begin to interact, attractive force is stronger than repulsive force and so potential energy of system decreases and is represented as Vs = (f*Msun)/rS/MX or Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)/Distance of Point. Universal Constant is a physical constant that is thought to be universal in its application in terms of Radius of the Earth and Acceleration of Gravity, Mass of the Sun defined as the total amount of matter that the Sun contains. This includes all of its components, such as hydrogen, helium, and trace amounts of heavier elements & Distance of Point refers to the point located on the surface of the Earth to the center of the Sun or the Moon.
How to calculate Attractive Force Potentials per unit Mass for Sun?
The Attractive Force Potentials per unit Mass for Sun formula is defined as to make potential energy of system decrease. As atoms first begin to interact, attractive force is stronger than repulsive force and so potential energy of system decreases is calculated using Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)/Distance of Point. To calculate Attractive Force Potentials per unit Mass for Sun, you need Universal Constant (f), Mass of the Sun (Msun) & Distance of Point (rS/MX). With our tool, you need to enter the respective value for Universal Constant, Mass of the Sun & Distance of Point and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.
How many ways are there to calculate Attractive Force Potentials for Sun?
In this formula, Attractive Force Potentials for Sun uses Universal Constant, Mass of the Sun & Distance of Point. We can use 2 other way(s) to calculate the same, which is/are as follows -
  • Attractive Force Potentials for Sun = (Universal Constant*Mass of the Sun)*((1/Distance of Point)-(1/Distance)-(Mean Radius of the Earth*cos(Angle made by the Distance of Point)/Distance^2))
  • Attractive Force Potentials for Sun = Universal Constant*Mass of the Sun*(Mean Radius of the Earth^2/Distance^3)*Harmonic Polynomial Expansion Terms for Sun
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