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They arrived at a figure for the solar parallax of 9. They were also the first astronomers to have access to an accurate and reliable value for the radius of Earth, which had been measured by their colleague Jean Picard in as 3 toises.
A better method for observing Venus transits was devised by James Gregory and published in his Optica Promata It was strongly advocated by Edmond Halley  and was applied to the transits of Venus observed in and , and then again in and Transits of Venus occur in pairs, but less than one pair every century, and observing the transits in and was an unprecedented international scientific operation including observations by James Cook and Charles Green from Tahiti.
Despite the Seven Years' War , dozens of astronomers were dispatched to observing points around the world at great expense and personal danger: several of them died in the endeavour.
Another method involved determining the constant of aberration. Simon Newcomb gave great weight to this method when deriving his widely accepted value of 8.
Newcomb also collaborated with A. Michelson to measure the speed of light with Earth-based equipment; combined with the constant of aberration which is related to the light time per unit distance , this gave the first direct measurement of the Earth—Sun distance in kilometres.
Newcomb's value for the solar parallax and for the constant of aberration and the Gaussian gravitational constant were incorporated into the first international system of astronomical constants in ,  which remained in place for the calculation of ephemerides until The discovery of the near-Earth asteroid Eros and its passage near Earth in — allowed a considerable improvement in parallax measurement.
Direct radar measurements of the distances to Venus and Mars became available in the early s. Along with improved measurements of the speed of light, these showed that Newcomb's values for the solar parallax and the constant of aberration were inconsistent with one another.
The unit distance A the value of the astronomical unit in metres can be expressed in terms of other astronomical constants:.
The Sun is constantly losing mass by radiating away energy,  so the orbits of the planets are steadily expanding outward from the Sun.
This has led to calls to abandon the astronomical unit as a unit of measurement. Hence, it is possible to construct ephemerides entirely in SI units, which is increasingly becoming the norm.
The measurements of the secular variations of the astronomical unit are not confirmed by other authors and are quite controversial.
Furthermore, since , the astronomical unit has not been estimated by the planetary ephemerides. The following table contains some distances given in astronomical units.
It includes some examples with distances that are normally not given in astronomical units, because they are either too short or far too long.
Distances normally change over time. Examples are listed by increasing distance. From Wikipedia, the free encyclopedia. This article is about the unit of length.
For constants, see astronomical constant. For units in astronomy, see astronomical system of units. Mean distance between Earth and the Sun, common length reference in astronomy.