You will need

- calculator;
- - radar;
- - stopwatch;
- - Handbook of astronomy.

Instruction

1

Radar is one of the modern methods of determining the distance from Earth to the planets (geocentric distance). It is based on a comparative analysis of the sent and reflected signal.Send a radio signal in the direction of interest

**of the planet**and turn on the stopwatch. When will the reflected signal to stop the clock. By the known velocity of propagation and the time during which the signal reaches**the planet**is reflected, calculate the**distance**to**the planet**. It is equal to the product of the speed at half the stopwatch.2

Before the advent of radar to determine the distance to objects in the Solar system using the method of the horizontal parallax. The error of this method is kilometer, and the measurement error of the distance using the radar centimeter.

3

The essence of the definition of the distances to the planets by the method of the horizontal parallax is to change the direction of the object when moving the observation point (parallax) – as a base is taken maximally spaced points together: the radius of the Earth. That is, the determination of distances to

**the planets**by the method of the horizontal parallax is a simple trigonometric problem. If you know all the data.4

Multiply 1 radian (the angle formed by the arc length is equal to radius expressed in seconds (206265) on the radius of the Earth (6370 km) and divide by the amount of parallax

**of the planet**at this time. The resulting value**is the distance**to**the planet**in astronomical units.5

At an annual or trigonometric parallax (base is the semimajor axis of earth's orbit) calculate distances to very distant planets and stars. By the way, parallax equal to one second determines

**the distance of**one parsec, and 1 PS = 206265 astronomical units. Divide 206265 seconds (1 radians) on the value of trigonometric parallax. The resulting quotient is**the distance of**to the interest**of the planet**.6

Finally,

**distance**to planets can be calculated using the third law of Kepler. The calculation is quite complicated, so let's proceed to the final part.Construct the squared value of the orbital period**of the planet**around the Sun. Calculate the cube root of this value. The resulting number is**the distance**from the interest**of the planet**to the Sun in astronomical units, or heliocentric**distance**. Knowing the heliocentric**distance**and the position of the planets (angular**distance****of the planet**from the Sun), you can easily calculate the geocentric**distance**.