Our sun is not the centre of the universe but is rather part of a giant, disc-shaped cluster of stars that floats through space.

  • Who discovered it?: Thomas Wright and William Herschel
  • Year of Discovery: 1750
How was it discovered?

For thousands of years, scientist believed that the universe consisted of a vast spherical 220px-William_Herschel01shell of stars, with Earth at its centre. Nothing existed in the immense void between Earth and that shell of stars except the few planets and the sun.

By the mid-1600s, most scientists acknowledged that the sun, not the earth, sat at the centre of the spherical universe. Some prominent scientists (Christian Huygens, for example) believed that stars were really holes in the black sphere of space where light from a luminous region of perpetual day beyond shined through.

Two men’s discoveries combined to establish the existence of dense clusters of stars called galaxies. Born in 1711, English man Thomas Wright taught mathematics and navigation but was a passionate amateur astronomer. As had many astronomers before him, Wright observed that the stars were not evenly spread across the sky. A seeming cloud of faint stars was densely packed along the band called the Milky Way.


This bothered Wright considered that the stars might be spread along the surfaces of a field of giant bubbles. If we were packed along one of those rings of stars, looking along the ring would cause us to see more stars than if we looked straight out from it. He then considered the rings of Saturn and proposed that the stars might be packed into wide rings or a thin disk. If we were on that disc, it would account for the uneven distribution of stars we saw—even if the stars were really evenly spaced across that disk.

In 1750 Wright published a book, An Original Theory on New Hypothesis of the Universe, in which he proposed this theory. He was the first to use the word galaxy to describe a giant cluster of stars.

Five years later, famed astronomer and mathematician Immanuel Kant
proposed a similar arrangement of the stars into a giant disk-shaped cluster.
English astronomer William Hershel (born in 1738) read with interest Wright’s theory.

In 1785 Herschel decided to use statistical methods to count the stars. He surely couldn’t count them all. So he randomly picked 683 small regions of the sky and set about counting the stars in each region using a 48-inch telescope—considered a giant scope at the time.

Herschel quickly realized that the number of stars per unit area of sky rose steadily as he approached the Milky Way and spiked in regions in the Milky Way. (The number of stars per unit area of sky reached a minimum in directions at right angles to the Milky Way.) This made Herschel think of Wright’s and Kant’s theories. Hershel concluded that his counting results could only be explained if most of the stars were compacted into a lens-shaped mass and that the sun was buried in this lens. Herschel was the first to add statistical measurement to Wright’s discovery of the existence and shape of galaxies.