Earth's location in the universe

Earth's location in the universe

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.[1] After the acceptance of the heliocentric model in the 17th century, observations by William Herschel and others showed that the Sun lay within a vast, disc-shaped galaxy of stars.[2] By the 20th century, observations of spiral nebulae by Edwin Hubble revealed that our galaxy was one of billions in an expanding universe,[3][4] grouped into clusters and superclusters. By the end of the 20th century, the overall structure of the visible universe was becoming clearer, with superclusters forming into a vast web of filaments and voids.[5] Superclusters, filaments and voids are the largest coherent structures in the Universe that we can observe.[6] At still larger scales (over 1000 megaparsecs)[b] the Universe becomes homogeneous meaning that all its parts have on average the same density, composition and structure.[7]

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.[8] Because the observable universe is defined as that region of the universe visible to terrestrial observers, Earth is, by definition, the center of the observable universe.[9] 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. There have been numerous hypotheses that our universe may be only one such example within a higher multiverse; however, no direct evidence of any sort of multiverse has ever been observed, and some have argued that the hypothesis is not falsifiable.[10][11]

A diagram of our location in the observable universe.
Feature Diameter Notes Sources
Earth 12,756.2 km
(equatorial)
Measurement comprises just the solid part of the Earth; there is no agreed upper boundary for Earth's atmosphere.
The geocorona, a layer of UV-luminescent hydrogen atoms, lies at 100,000 km.
The Kármán line, defined as the boundary of space for astronautics, lies at 100 km.
[12][13][14][15]
Orbit of the Moon 768,210 km[a] The average diameter of the orbit of the Moon relative to the Earth. [16]
Geospace 6,363,000–
12,663,000 km
(110-210 Earth radii)
The space dominated by Earth's magnetic field and its magnetotail, shaped by the solar wind. [17]
Earth's orbit 299.2 million km[a]
AU[b]
The average diameter of the orbit of the Earth relative to the Sun.
Encompasses the Sun, Mercury and Venus.
[18]
Inner Solar System ~6.54 AU Encompasses the Sun, the inner planets (Mercury, Venus, Earth, Mars) and the asteroid belt.
Cited distance is the 2:1 resonance with Jupiter, which marks the outer limit of the asteroid belt.
[19][20][21]
Outer Solar System 60.14 AU[a] Includes the outer planets (Jupiter, Saturn, Uranus, Neptune).
Cited distance is the orbital diameter of Neptune.
[22]
Kuiper belt ~96 AU Belt of icy objects surrounding the outer solar system. Encompasses the dwarf planets Pluto, Haumea and Makemake.
Cited distance is the 2:1 resonance with Neptune, generally regarded as the outer edge of the main Kuiper belt.
[23]
Heliosphere 160 AU Maximum extent of the solar wind and the interplanetary medium. [24][25]
Scattered disk 195.3 AU Region of sparsely scattered icy objects surrounding the Kuiper belt. Encompasses the dwarf planet Eris.
Cited distance is derived by doubling the aphelion of Eris, the farthest known scattered disk object
As of now, Eris's aphelion marks the farthest known point in the scattered disk.
[26]
Oort cloud 100,000–200,000 AU
0.613–1.23 pc [c]
Spherical shell of over a trillion (1012) comets. Existence is currently hypothetical, but inferred from the orbits of long-period comets. [27]
Solar System 1.23 pc The Sun and its planetary system. Cited diameter is that of the Sun's Hill sphere; the region of its gravitational influence. [28]
Local Interstellar Cloud 9.2 pc Interstellar cloud of gas through which the Sun and a number of other stars are currently travelling. [29]
Local Bubble 2.82–250 pc Cavity in the interstellar medium in which the Sun and a number of other stars are currently travelling.
Caused by a past supernova.
[30][31]
Gould Belt 1,000 pc Ring of young stars through which the Sun is currently travelling. [32]
Orion Arm 3000 pc
(length)
The spiral arm of the Milky Way Galaxy through which the Sun is currently travelling.
[33]
Orbit of the Solar System 17,200 pc The average diameter of the orbit of the Solar System relative to the Galactic Center.
The Sun's orbital radius is roughly 8,600 parsecs, or slightly over half way to the galactic edge.
One orbital period of the Solar System lasts between 225 and 250 million years.
[34][35]
Milky Way Galaxy 30,000 pc Our home galaxy, composed of 200 billion to 400 billion stars and filled with the interstellar medium. [36][37]
Milky Way subgroup 840,500 pc The Milky Way and those satellite dwarf galaxies gravitationally bound to it.
Examples include the Sagittarius Dwarf, the Ursa Minor Dwarf and the Canis Major Dwarf.
Cited distance is the orbital diameter of the Leo T Dwarf galaxy, the most distant galaxy in the Milky Way subgroup.
[38]
Local Group 3 Mpc[c] Group of at least 47 galaxies of which the Milky Way is a part.
Dominated by Andromeda (the largest), the Milky Way and Triangulum; the remainder are dwarf galaxies.
[39]
Local Sheet 7 Mpc Group of galaxies including the Local Group moving at the same relative velocity towards the Virgo Cluster and away from the Local Void. [40][41]
Virgo Supercluster 30 Mpc The supercluster of which our Local Group is a part.
It comprises roughly 100 galaxy groups and clusters, centred on the Virgo Cluster.
Our Local Group is located on the outer edge of the Virgo Supercluster.
[42][43]
Laniakea 160 Mpc A group connected with the superclusters of which our Local Group is a part.
Comprises roughly 300 to 500 galaxy groups and clusters, centred on the Great Attractor in the Hydra-Centaurus Supercluster.
[44][45][46][47]
Observable universe 28,000 Mpc More than 100 billion galaxies, arranged in millions of superclusters, galactic filaments, and voids, creating a foam-like superstructure. [48][49]
Universe Minimum 28,000 Mpc Beyond the observable universe lie the unobservable regions from which no light has reached the Earth yet.
No information is available, as light is the fastest travelling medium of information.
However, uniformitarianism argues that the universe is likely to contain more galaxies in the same foam-like superstructure.
[50]
a Semi-major and semi-minor axes
b 1 AU or astronomical unit is the distance between the Earth and the Sun, or 150 million km. Earth's orbital diameter is twice its orbital radius, or 2 AU.
c A parsec (pc) is the distance at which a star's parallax as viewed from Earth is equal to one second of arc, equal to roughly 206,000 AU or 3.0857×1013 km.
One megaparsec (Mpc) is equivalent to one million parsecs.

See also

References

  1. ^
  2. ^
  3. ^
  4. ^
  5. ^
  6. ^
  7. ^
  8. ^ . P. 55.
  9. ^
  10. ^
  11. ^
  12. ^
  13. ^ World Geodetic System (WGS-84). Available online from National Geospatial-Intelligence Agency Retrieved 27 April 2015.
  14. ^
  15. ^
  16. ^ NASA Moon Factsheet and NASA Solar System Exploration Moon Factsheet NASA Retrieved on 17 November 2008
  17. ^
  18. ^ NASA Earth factsheet and NASA Solar System Exploration Earth Factsheet NASA Retrieved on 17 November 2008
  19. ^
  20. ^
  21. ^
  22. ^ NASA Neptune factsheet and NASA Solar System Exploration Neptune Factsheet NASA Retrieved on 17 November 2008
  23. ^
  24. ^
  25. ^ See Figures 1 and 2.
  26. ^
  27. ^
  28. ^
  29. ^ Mark Anderson, "Don't stop till you get to the Fluff", New Scientist no. 2585, 6 January 2007, pp. 26–30
  30. ^
  31. ^
  32. ^
  33. ^ Harold Spencer Jones, T. H. Huxley, Proceedings of the Royal Institution of Great Britain, Royal Institution of Great Britain, v. 38–39
  34. ^
  35. ^
  36. ^
  37. ^
  38. ^
  39. ^
  40. ^
  41. ^
  42. ^
  43. ^
  44. ^
  45. ^
  46. ^
  47. ^
  48. ^
  49. ^
  50. ^