The method called "parallax.
India astronomers recognized that the earth was a sphere.
"Libra" is a constellation ... a group of stars that seem to join in a pattern when viewed by humans on Earth, in a region of the sky defined by human astronomers on Earth. The stars in Libra are totally unrelated to each other, and each of them is at a different distance from Earth.
The distance from the Sun to the Earth varies about 3% over the course of a year, from a minimum or "perihelion" distance of about 91,500,000 miles to a maximum or "aphelion" distance of about 94,500,000 miles. 93 million miles is a good average figure. Details of how to measure this distance are given later. The speed of light is approximately 186,000 miles per second, or 300,000 kilometers per second. With an average distance of 93 million miles and an approximate speed of light of 186,000 miles per second, the math becomes really easy; it takes light 500 seconds to reach the Earth. Here's one method of how to measure the distance to the Sun, using radar technology: (You can't use radar to measure the distance to the Sun directly because of the nature of the Sun's surface.) 1) Wait for Earth, Venus and the Sun to line up with Venus (more or less) directly between us and the Sun. 2) Measure the distance to Venus using radar. 3) Knowing the Earth to Venus distance, use Kepler's Third Law to find the Earth to Sun distance. (Kepler's Third Law will give the ratio of the distances of Earth and Venus from the Sun. Thus, knowing the Earth to Venus distance, you can find the Earth to Sun distance.) See the "Related Link" below for more about measuring the distance to the Sun.
Light years are used to measure distance from Earth to distant stars and planets.
A "light year" is a measure of distance, derived from "how far light can travel in one Earth year". Thus, if you shine a torch for the amount of time it takes the Earth to orbit the sun exactly once, that light would have travelled the distance of a "light year".
Parallax is the method that astronomers use to measure the distance from the sun to the earth.
Astronomers use a method called parallax to measure the distance to nearby stars. Astronomers can measure parallax by measuring the position of a nearby star with respect to the distant stars behind it. Then, they measure the same stars again six months later when the Earth is on the opposite side of its orbit.
Stellar Parallax Astronomers estimate the distance of nearby objects in space by using a method called stellar parallax, or trigonometric parallax. Simply put, they measure a star's apparent movement against the background of more distant stars as Earth revolves around the sun.
The average distance between the Earth and sun, in round figures, is 93 million miles. Astronomers tend to maintain the same distance from the sun that ordinary people do.
Not calipers. Astronomers snap a photo, wait six months, then snap another. The apparent change in position with respect to much further background stars gives them a decent estimate, using the diameter of Earth's solar orbit as one leg of an extremely long isosceles triangle. We gauge distances to further stars using apparent brightness of Cepheid variables, and so on.
I believe that it is all to do with margin of error. The further away the planet, the greater the margin of error in the observations and therefore the greater the uncertainty in their distance from Earth.
Well, they clearly aren't for closer stars, astronomers measure the angle the star's light hits the Earth at 6 month intervals - as the Earth rotates around the sun at a known distance, it's simple geometry given the two angles and the diameter of the Earth's orbit to calculate the distance of the star in question and the distance varies.
The unit used is usually the Astronomical Unit (AU), which is the average distance from the earth to the sun, and is approx 150 million km.
Parallax is the apparent change in position of an object when you look at it from different angles. Astronomers often us parallax to measure distances to nearby stars. This method can be used to determine stars' distances up to 400 light-years from Earth.
Celsius is a measure of temperature, not distance.
The mathematical equation which describes how to measure the distance from Earth to the moon using Earth's diameter as a unit of measure is d = Dcot(p/2)/2 Where d is the distance from Earth to the moon, D is the diameter of the Earth and p is the angle of parallax subtended at moon by the diameter of the Earth.
The simplest method is parallax - measure the angle to the sun from opposite sides of the earth and construct a triangle. Using the diameter of the earth as a base line, calculate the altitude (height) of the triangle formed.