The Solar Constant For A Planet Is S

Earth s overall average albedo is about 0 31 or 31.

The solar constant for a planet is s.

The sun subtends an angle theta at the planet. It is most accurately measured from satelli. The value of the constant is approximately 1 366 kilowatts per square metre. The solar constant for a planet is s.

The solar constant includes all types of solar radiation other than neutrinos not just the visible light. Solar constant the total radiation energy received from the sun per unit of time per unit of area on a theoretical surface perpendicular to the sun s rays and at earth s mean distance from the sun. Of the objects that orbit the sun directly the largest are the eight planets with the remainder being smaller objects the dwarf planets and small solar system bodies of the objects that orbit the sun indirectly the moons two are larger than the smallest planet. What is the surface temperature for a planet with no atmosphere with a solar constant of 2 718 w m 2 and an albedo of 0 6.

The solar system is the gravitationally bound system of the sun and the objects that orbit it either directly or indirectly. The surface temperature of the sun is tk. Irradiance is sometimes referred to as flux and is a measurement of electromagnetic energy from the sun. The solar constant is calculated by multiplying the sun s surface irradiance by the square of the radius of the sun over the average distance between the earth and the sun.

It is measured on a surface perpendicular to the rays one astronomical unit au from the sun roughly the distance from the sun to the earth. Solar constant the total radiation energy received from the sun per unit of time per unit of area on a theoretical surface perpendicular to the sun s rays and at earth s mean distance from the sun. The solar constant is the amount of solar radiation incidence that is received at a distance of 1 astronomical unit au from the sun. Using a little more algebra we can write the expression above as.

It is presently calculated as being 1 366 w m2. Due to the fact that the earth rotates around the sun and it s distance depends on the time of year the actual direct solar incidence that earth receives varies.