Mean distance between sun or star and earth or planet Calculator

✖The Radius of the Sun is the distance from the center of the Sun to its surface, playing a crucial role in understanding solar radiation and its effects on the solar system.ⓘ Radius of the Sun [r]			+10% -10%
✖The Effective Surface Temperature is the temperature of a surface that accounts for the effects of radiation and heat transfer in the atmosphere.ⓘ Effective Surface Temperature [T_s]			+10% -10%
✖The Total Solar Irradiance is the total amount of solar energy received per unit area at the top of the Earth's atmosphere, influencing climate and weather patterns.ⓘ Total Solar Irradiance [G_s]			+10% -10%

✖The Mean Distance between Sun and Planet is the average space separating a planet from the Sun, influencing solar radiation and climate conditions on the planet.ⓘ Mean distance between sun or star and earth or planet [L]

⎘ Copy

👎

Formula

LaTeX

Reset

👍

Download Heat and Mass Transfer Formula PDF PDF Image

Mean distance between sun or star and earth or planet Solution

STEP 0: Pre-Calculation Summary

Formula Used

Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5
L = (((r^2)*[Stefan-BoltZ]*(T_s^4))/G_s)^0.5
This formula uses 1 Constants, 4 Variables

Constants Used

[Stefan-BoltZ] - Stefan-Boltzmann Constant Value Taken As 5.670367E-8

Variables Used

Mean Distance between Sun and Planet - (Measured in Meter) - The Mean Distance between Sun and Planet is the average space separating a planet from the Sun, influencing solar radiation and climate conditions on the planet.
Radius of the Sun - (Measured in Meter) - The Radius of the Sun is the distance from the center of the Sun to its surface, playing a crucial role in understanding solar radiation and its effects on the solar system.
Effective Surface Temperature - (Measured in Kelvin) - The Effective Surface Temperature is the temperature of a surface that accounts for the effects of radiation and heat transfer in the atmosphere.
Total Solar Irradiance - (Measured in Watt per Square Meter) - The Total Solar Irradiance is the total amount of solar energy received per unit area at the top of the Earth's atmosphere, influencing climate and weather patterns.

STEP 1: Convert Input(s) to Base Unit

Radius of the Sun: 700000000 Meter --> 700000000 Meter No Conversion Required
Effective Surface Temperature: 5774.461 Kelvin --> 5774.461 Kelvin No Conversion Required
Total Solar Irradiance: 1373 Watt per Square Meter --> 1373 Watt per Square Meter No Conversion Required

STEP 2: Evaluate Formula

Substituting Input Values in Formula

L = (((r^2)*[Stefan-BoltZ]*(T_s^4))/G_s)^0.5 --> (((700000000^2)*[Stefan-BoltZ]*(5774.461^4))/1373)^0.5

Evaluating ... ...

L = 150000000546.705

STEP 3: Convert Result to Output's Unit

150000000546.705 Meter --> No Conversion Required

FINAL ANSWER

150000000546.705 ≈ 1.5E+11 Meter <-- Mean Distance between Sun and Planet

(Calculation completed in 00.004 seconds)

You are here -

Home » Physics » Heat and Mass Transfer » Radiation » Mechanical » Atmospheric and Solar Radiation » Mean distance between sun or star and earth or planet

Credits

Created by Sai Venkata Phanindra Chary Arendra

Vallurupalli Nageswara Rao Vignana Jyothi Institute of Engineering and Technology (VNRVJIET), Hyderabad

Sai Venkata Phanindra Chary Arendra has created this Calculator and 100+ more calculators!

Verified by Rajat Vishwakarma

University Institute of Technology RGPV (UIT - RGPV), Bhopal

Rajat Vishwakarma has verified this Calculator and 400+ more calculators!

< Atmospheric and Solar Radiation Calculators

Effective surface temperature of sun given solar constant

LaTeX Go Effective Surface Temperature = (((Mean Distance between Sun and Planet^2)*Total Solar Irradiance)/((Radius of the Sun^2)*[Stefan-BoltZ]))^0.25

Radius of sun given total solar irradiance

LaTeX Go Radius of the Sun = (((Mean Distance between Sun and Planet^2)*Total Solar Irradiance)/([Stefan-BoltZ]*(Effective Surface Temperature^4)))^0.5

Mean distance between sun or star and earth or planet

LaTeX Go Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5

Total solar irradiance or solar constant

LaTeX Go Total Solar Irradiance = ((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/(Mean Distance between Sun and Planet^2)

Mean distance between sun or star and earth or planet Formula

LaTeX Go

Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5
L = (((r^2)*[Stefan-BoltZ]*(T_s^4))/G_s)^0.5

What is total solar irradiance?

The total solar irradiance (also called the solar constant) represents the rate at which solar energy is incident on a surface normal to the sun’s rays at the outer edge of the atmosphere when the earth is at its mean distance from the sun.

How to Calculate Mean distance between sun or star and earth or planet?

Mean distance between sun or star and earth or planet calculator uses Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5 to calculate the Mean Distance between Sun and Planet, Mean distance between sun or star and earth or planet formula is defined as the average distance between the center of the sun or star and the center of the earth or planet, which is a critical parameter in understanding the radiation and energy exchange between the two celestial bodies. Mean Distance between Sun and Planet is denoted by L symbol.

How to calculate Mean distance between sun or star and earth or planet using this online calculator? To use this online calculator for Mean distance between sun or star and earth or planet, enter Radius of the Sun (r), Effective Surface Temperature (T_s) & Total Solar Irradiance (G_s) and hit the calculate button. Here is how the Mean distance between sun or star and earth or planet calculation can be explained with given input values -> 1.5E+11 = (((700000000^2)*[Stefan-BoltZ]*(5774.461^4))/1373)^0.5.

FAQ

What is Mean distance between sun or star and earth or planet?

Mean distance between sun or star and earth or planet formula is defined as the average distance between the center of the sun or star and the center of the earth or planet, which is a critical parameter in understanding the radiation and energy exchange between the two celestial bodies and is represented as L = (((r^2)*[Stefan-BoltZ]*(T_s^4))/G_s)^0.5 or Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5. The Radius of the Sun is the distance from the center of the Sun to its surface, playing a crucial role in understanding solar radiation and its effects on the solar system, The Effective Surface Temperature is the temperature of a surface that accounts for the effects of radiation and heat transfer in the atmosphere & The Total Solar Irradiance is the total amount of solar energy received per unit area at the top of the Earth's atmosphere, influencing climate and weather patterns.

How to calculate Mean distance between sun or star and earth or planet?

Mean distance between sun or star and earth or planet formula is defined as the average distance between the center of the sun or star and the center of the earth or planet, which is a critical parameter in understanding the radiation and energy exchange between the two celestial bodies is calculated using Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5. To calculate Mean distance between sun or star and earth or planet, you need Radius of the Sun (r), Effective Surface Temperature (T_s) & Total Solar Irradiance (G_s). With our tool, you need to enter the respective value for Radius of the Sun, Effective Surface Temperature & Total Solar Irradiance and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.

Home

FREE PDFs

🔍 Search