Editing Outer space (section)

== History of discovery ==
{{Further|Timeline of knowledge about galaxies, clusters of galaxies, and large-scale structure}}
In 350 BCE, Greek philosopher [[Aristotle]] suggested that ''nature abhors a vacuum'', a principle that became known as the ''[[Horror vacui (physics)|horror vacui]]''. This concept built upon a 5th-century BCE [[Ontology|ontological]] argument by the Greek philosopher [[Parmenides]], who denied the possible existence of a void in space.{{sfn|Grant|1981|p=10}} Based on this idea that a vacuum could not exist, in the West it was widely held for many centuries that space could not be empty.{{sfn|Porter|Park|Daston|2006|p=27}} As late as the 17th century, the French philosopher [[René Descartes]] argued that the entirety of space must be filled.{{sfn|Eckert|2006|p=5}}

In [[ancient China]], the 2nd-century astronomer [[Zhang Heng]] became convinced that space must be infinite, extending well beyond the mechanism that supported the Sun and the stars. The surviving books of the Hsüan Yeh school said that the heavens were boundless, "empty and void of substance". Likewise, the "sun, moon, and the company of stars float in the empty space, moving or standing still".{{sfn|Needham|Ronan|1985|pp=82–87}}

The Italian scientist [[Galileo Galilei]] knew that air has mass and so was subject to gravity. In 1640, he demonstrated that an established force resisted the formation of a vacuum. It would remain for his pupil [[Evangelista Torricelli]] to create an apparatus that would produce a partial vacuum in 1643. This experiment resulted in the first mercury [[barometer]] and created a scientific sensation in Europe. Torricelli suggested that since air has weight, then [[air pressure]] should decrease with altitude.<ref name=West_2013/> The French mathematician [[Blaise Pascal]] proposed an experiment to test this hypothesis.{{sfn|Holton|Brush|2001|pp=267–268}} In 1648, his brother-in-law, Florin Périer, repeated the experiment on the [[Puy de Dôme]] mountain in central France and found that the column was shorter by three inches. This decrease in pressure was further demonstrated by carrying a half-full balloon up a mountain and watching it gradually expand, then contract upon descent.{{sfn|Cajori|1917|pp=64–66}}

[[File:Magedurger Halbkugeln Luftpumpe Deutsches Museum.jpg|thumb|upright|left|The original [[Magdeburg hemispheres]] (left) used to demonstrate Otto von Guericke's vacuum pump (right)|alt=A glass display case holds a mechanical device with a lever arm, plus two metal hemispheres attached to draw ropes.]]

In 1650, German scientist [[Otto von Guericke]] constructed the first [[vacuum pump]]: a device that would further refute the principle of ''horror vacui''. He correctly noted that the atmosphere of the Earth surrounds the planet like a shell, with the density gradually declining with altitude. He concluded that there must be a vacuum between the Earth and the Moon.{{sfn|Genz|2001|pp=127–128}}

In the 15th century, German theologian [[Nicolaus Cusanus]] speculated that the universe lacked a center and a circumference. He believed that the universe, while not infinite, could not be held as finite as it lacked any bounds within which it could be contained.{{sfn|Tassoul|Tassoul|2004|p=22}} These ideas led to speculations as to the infinite dimension of space by the Italian philosopher [[Giordano Bruno]] in the 16th century. He extended the Copernican [[heliocentric]] cosmology to the concept of an infinite universe filled with a substance he called [[Aether (classical element)|aether]], which did not resist the motion of heavenly bodies.{{sfn|Gatti|2002|pp=99–104}} English philosopher [[William Gilbert (astronomer)|William Gilbert]] arrived at a similar conclusion, arguing that the stars are visible to us only because they are surrounded by a thin aether or a void.{{sfn|Kelly|1965|pp=97–107}} This concept of an aether originated with ancient Greek philosophers, including Aristotle, who conceived of it as the medium through which the heavenly bodies move.{{sfn|Olenick|Apostol|Goodstein|1986|p=356}}

The concept of a universe filled with a [[luminiferous aether]] retained support among some scientists until the early 20th century. This form of aether was viewed as the medium through which light could propagate.{{sfn|Hariharan|2003|p=2}} In 1887, the [[Michelson–Morley experiment]] tried to detect the Earth's motion through this medium by looking for changes in the [[speed of light]] depending on the direction of the planet's motion. The [[null result]] indicated something was wrong with the concept. The idea of the luminiferous aether was then abandoned. It was replaced by [[Albert Einstein]]'s theory of [[special relativity]], which holds that the speed of light in a vacuum is a fixed constant, independent of the observer's motion or [[frame of reference]].{{sfn|Olenick|Apostol|Goodstein|1986|pp=357–365}}{{sfn|Thagard|1992|pp=206–209}}

The first professional astronomer to support the concept of an infinite universe was the Englishman [[Thomas Digges]] in 1576.{{sfn|Maor|1991|p=195}} But the scale of the universe remained unknown until the [[List of the most distant astronomical objects#Timeline of most distant astronomical object recordholders|first successful measurement of the distance]] to a nearby star in 1838 by the German astronomer [[Friedrich Bessel]]. He showed that the star system [[61 Cygni]] had a [[stellar parallax|parallax]] of just 0.31&nbsp;[[arcsecond]]s (compared to the modern value of 0.287″). This corresponds to a distance of over 10 [[light year]]s.{{sfn|Webb|1999|pp=71–73}} In 1917, [[Heber Doust Curtis|Heber Curtis]] noted that [[nova]]e in spiral nebulae were, on average, 10 magnitudes fainter than galactic novae, suggesting that the former are 100 times further away.<ref name=Curtis1988/> The distance to the [[Andromeda Galaxy]] was determined in 1923 by American astronomer [[Edwin Hubble]] by measuring the brightness of [[cepheid variable]]s in that galaxy, a new technique discovered by [[Henrietta Leavitt]].<ref name=csiro_20041025/> This established that the Andromeda Galaxy, and by extension all galaxies, lay well outside the Milky Way.{{sfn|Tyson|Goldsmith|2004|pp=114–115}} With this Hubble formulated the [[Hubble constant]], which allowed for the first time a calculation of the age of the Universe and size of the Observable Universe, starting at 2 billion years and 280 million light-years. This became increasingly precise with better measurements, until 2006 when data of the [[Hubble Space Telescope]] allowed a very accurate calculation of the age of the Universe and size of the Observable Universe.<ref name="p537"/>

The modern concept of outer space is based on the [[Big Bang cosmology|"Big Bang" cosmology]], first proposed in 1931 by the Belgian physicist [[Georges Lemaître]].<ref name=nature127_3210_706/> This theory holds that the universe originated from a state of extreme energy density that has since undergone [[Hubble's law|continuous expansion]].<ref name=Big_Bang/>

The earliest known estimate of the temperature of outer space was by the Swiss physicist [[Charles Édouard Guillaume|Charles É. Guillaume]] in 1896. Using the estimated radiation of the background stars, he concluded that space must be heated to a temperature of 5–6&nbsp;K. British physicist [[Arthur Eddington]] made a similar calculation to derive a temperature of 3.18&nbsp;K in 1926. German physicist [[Erich Regener]] used the total measured energy of [[cosmic ray]]s to estimate an intergalactic temperature of 2.8&nbsp;K in 1933.<ref name="Apeiron2_3_79"/> American physicists [[Ralph Alpher]] and [[Robert Herman]] predicted 5&nbsp;K for the temperature of space in 1948, based on the gradual decrease in background energy following the then-new [[Big Bang]] theory.<ref name="Apeiron2_3_79"/>