A Cosmic Zoom

Visualizing the Universe, one pixel at a time.

Earth's Location in the Universe

A slideshow, graphics from Wikipedia Author: Andrew Colvin

Earth's Location In Space

Knowledge of Earth's location in the universe has been shaped by 400 years of telescopic observations, and has expanded radically in the last century. Initially, Earth was believed to be the center of the universe, which consisted only of those planets visible with the naked eye and an outlying sphere of fixed stars.

After the acceptance of the heliocentric model in the 17th century, observations by William Herschel and others showed that Earth's Sun lay within a vast, disc-shaped galaxy of stars, later revealed to be suns like our own.

By the 20th century, observations of spiral nebulae revealed that our galaxy was only one of billions in an expanding universe, grouped into clusters and superclusters. By the 21st century, the overall structure of the visible universe was becoming clearer, with superclusters forming into a vast web of filaments and voids.

Superclusters, filaments and voids are likely the largest coherent structures that exist in the Universe. At still larger scales (over 1000 megaparsecs)[e] the Universe becomes homogeneous meaning that all its parts have on average the same density, composition and structure.[1]

Since there is believed to be no "center" or "edge" of the universe, there is no particular reference point with which to plot the overall location of the Earth in the universe.[2] The Earth is at the center of the observable universe because its observability is determined by its distance from Earth. Reference can be made to the Earth's position with respect to specific structures, which exist at various scales.

It is still undetermined whether the universe is infinite, and there is speculation that our universe might only be one of countless trillions within a larger multiverse, itself contained within the omniverse.

More Details and Notes

The Solar System

     
Planet Mean Distance from the Sun (km) Diameter (km) Diameter Relative to Earth
Mercury 58 x 106 4,880 0.38
Venus 108 x 106 12,100 0.95
Earth 150 x 106 12,760 1.0
Mars 228 x 106 6,800 0.53
Jupiter 778 x 106 143,800 11.27
Saturn 1,427 x 106 120,000 9.44
Uranus 2,870 x 106 52,300 4.10
Neptune 4,497 x 106 49,500 3.88
Pluto (dwarf planet) 5,900 x 106 3,000 0.20

SS Scale Size and distance

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The Milky Way

milkyway614px-Milky_Way_Arms.svg

How Big is the Universe?

The age of the universe is about 13.75 billion years, but due to the expansion of space we are observing objects that were originally much closer but are now considerably farther away (as defined in terms of cosmological proper distance, which is equal to the co-moving distance at the present time) than a static 13.75 billion light-years distance.

The diameter of the observable universe is estimated to be about 28 billion parsecs (93 billion light-years).

putting the edge of the observable universe at about 46–47 billion light-years away.