Galactic Year

Approximate orbit of the Sun (yellow circle) around the Galactic Centre

The galactic year, also known as a cosmic year, is the duration of time required for the Sun to orbit once around the center of the Milky Way Galaxy.^[1] One galactic year is 230 million Earth years.^[2] The Solar System is traveling at an average speed of 230 km/s (828,000 km/h) or 143 mi/s (514,000 mph) within its trajectory around the galactic center,^[3] a speed at which an object could circumnavigate the Earth's equator in 2 minutes and 54 seconds; that speed corresponds to approximately 1/1300 of the speed of light.

The galactic year provides a conveniently usable unit for depicting cosmic and geological time periods together. By contrast, a "billion-year" scale does not allow for useful discrimination between geologic events, and a "million-year" scale requires some rather large numbers.^[4]

Timeline of the universe and Earth's history in galactic years

The orientation of the Solar System's motion

The following list assumes that 1 galactic year is 225 million years.

Time	Event
Past
About 61.32 galactic years ago	Big Bang
About 54 galactic years ago	Birth of the Milky Way
20.44 galactic years ago	Birth of the Sun
17–18 galactic years ago	Oceans appear on Earth
16.889 galactic years ago	Life begins on Earth
15.555 galactic years ago	Prokaryotes appear
12 galactic years ago	Bacteria appear
10 galactic years ago	Stable continents appear
6.8 galactic years ago	Multicellular organisms appear
6.666 galactic years ago	Eukaryotes appear
2.4 galactic years ago	Cambrian explosion occurs
2 galactic years ago	The first brain structure appears in worms
1.11 galactic year ago	Permian–Triassic extinction event
0.2933 galactic years ago	Cretaceous–Paleogene extinction event
0.0013 galactic years ago	Emergence of anatomically modern humans
Future
0.15 galactic year from now	Mean time between impacts of asteroidal bodies in the order of magnitude of the K/Pg impactor has elapsed.^[5]
1 galactic year from now	All the continents on Earth may fuse into a supercontinent. Three potential arrangements of this configuration have been dubbed Amasia, Novopangaea, and Pangaea Ultima.^[6]
2–3 galactic years from now	Tidal acceleration moves the Moon far enough from Earth that total solar eclipses are no longer possible
4 galactic years from now	Carbon dioxide levels fall to the point at which C4 photosynthesis is no longer possible. Multicellular life dies out^[7]
15 galactic years from now	Surface conditions on Earth are comparable to those on Venus today
22 galactic years from now	The Milky Way and Andromeda Galaxy begin to collide
25 galactic years from now	Sun ejects a planetary nebula, leaving behind a white dwarf
30 galactic years from now	The Milky Way and Andromeda complete their merger into a giant elliptical galaxy called Milkomeda or Milkdromeda^[8]
500 galactic years from now	The Universe's expansion causes all galaxies beyond the Milky Way's Local Group to disappear beyond the cosmic light horizon, removing them from the observable universe^[9]
2000 galactic years from now	Local Group of 47 galaxies^[10] coalesces into a single large galaxy^[11]

Visualisation of the orbit of the Sun (yellow dot and white curve) around the Galactic Centre (GC) in the last galactic year. The red dots correspond to the positions of the stars studied by the European Southern Observatory in a monitoring programme.^[12]

References

^ Cosmic Year Archived 2014-04-12 at the Wayback Machine, Fact Guru, University of Ottawa
^ Leong, Stacy (2002). "Period of the Sun's Orbit around the Galaxy (Cosmic Year)". The Physics Factbook.
^ http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question18.html NASA – StarChild Question of the Month for February 2000
^ Geologic Time Scale – as 18 galactic rotations
^ Lunar and Planetary Institute (2010), https://www.lpi.usra.edu/features/chicxulub/
^ Williams, Caroline; Nield, Ted (2007-10-17). "Pangaea, the comeback". New Scientist. Retrieved 2014-01-02.
^ Franck, S.; Bounama, C.; von Bloh, W. (2005-11-07). "Causes and timing of future biosphere extinction". Biogeosciences Discussions. Copernicus GmbH. 2 (6): 1665-1679. Bibcode: 2006BGeo....3...85F. doi: 10.5194/bgd-2-1665-2005. S2CID 3619702.
^ Cox, T. J.; Loeb, Abraham (2008-05-01). "The collision between the Milky Way and Andromeda". Monthly Notices of the Royal Astronomical Society. Oxford University Press (OUP). 386 (1): 461–474. arXiv: 0705.1170. Bibcode: 2008MNRAS.386..461C. doi: 10.1111/j.1365-2966.2008.13048.x. ISSN 0035-8711. S2CID 14964036.
^ Loeb, Abraham (2011-04-18). "Cosmology with hypervelocity stars". Journal of Cosmology and Astroparticle Physics. IOP Publishing. 2011 (4): 023. arXiv: 1102.0007. Bibcode: 2011JCAP...04..023L. doi: 10.1088/1475-7516/2011/04/023. ISSN 1475-7516. S2CID 118750775.
^ Frommert, Hartmut; Kronberg, Christine (2007-06-05). "The Local Group of Galaxies". University of Arizona. Students for the Exploration and Development of Space. Archived from the original on 2009-09-07. Retrieved 2009-10-02.
^ Adams, Fred C.; Laughlin, Gregory (1997-04-01). "A dying universe: the long-term fate and evolutionof astrophysical objects". Reviews of Modern Physics. 69 (2): 337–372. arXiv: astro-ph/9701131. Bibcode: 1997RvMP...69..337A. doi: 10.1103/revmodphys.69.337. ISSN 0034-6861. S2CID 12173790.
^ "Milky Way Past Was More Turbulent Than Previously Known". ESO News. European Southern Observatory. 2004-04-06. After more than 1,000 nights of observations spread over 15 years, they have determined the spatial motions of more than 14,000 solar-like stars residing in the neighbourhood of the Sun.

[akb-1] Cosmic Year Archived 2014-04-12 at the Wayback Machine, Fact Guru, University of Ottawa

[biblio-2] Leong, Stacy (2002). "Period of the Sun's Orbit around the Galaxy (Cosmic Year)". The Physics Factbook.

[StarChild-3] ttp://starchild.gsfc.nasa.gov/docs/StarChild/questions/question18.html NASA – StarChild Question of the Month for February 2000

[timeline-4] Geologic Time Scale – as 18 galactic rotations

[5] Lunar and Planetary Institute (2010), https://www.lpi.usra.edu/features/chicxulub/

[6] Williams, Caroline; Nield, Ted (2007-10-17). "Pangaea, the comeback". New Scientist. Retrieved 2014-01-02.

[7] Franck, S.; Bounama, C.; von Bloh, W. (2005-11-07). "Causes and timing of future biosphere extinction". Biogeosciences Discussions. Copernicus GmbH. 2 (6): 1665-1679. Bibcode: 2006BGeo....3...85F. doi: 10.5194/bgd-2-1665-2005. S2CID 3619702.

[8] Cox, T. J.; Loeb, Abraham (2008-05-01). "The collision between the Milky Way and Andromeda". Monthly Notices of the Royal Astronomical Society. Oxford University Press (OUP). 386 (1): 461–474. arXiv: 0705.1170. Bibcode: 2008MNRAS.386..461C. doi: 10.1111/j.1365-2966.2008.13048.x. ISSN 0035-8711. S2CID 14964036.

[9] Loeb, Abraham (2011-04-18). "Cosmology with hypervelocity stars". Journal of Cosmology and Astroparticle Physics. IOP Publishing. 2011 (4): 023. arXiv: 1102.0007. Bibcode: 2011JCAP...04..023L. doi: 10.1088/1475-7516/2011/04/023. ISSN 1475-7516. S2CID 118750775.

[10] Frommert, Hartmut; Kronberg, Christine (2007-06-05). "The Local Group of Galaxies". University of Arizona. Students for the Exploration and Development of Space. Archived from the original on 2009-09-07. Retrieved 2009-10-02.

[11] Adams, Fred C.; Laughlin, Gregory (1997-04-01). "A dying universe: the long-term fate and evolutionof astrophysical objects". Reviews of Modern Physics. 69 (2): 337–372. arXiv: astro-ph/9701131. Bibcode: 1997RvMP...69..337A. doi: 10.1103/revmodphys.69.337. ISSN 0034-6861. S2CID 12173790.

[12] "Milky Way Past Was More Turbulent Than Previously Known". ESO News. European Southern Observatory. 2004-04-06. After more than 1,000 nights of observations spread over 15 years, they have determined the spatial motions of more than 14,000 solar-like stars residing in the neighbourhood of the Sun.

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v t e Time measurement and standards
Chronometry Orders of magnitude Metrology
International standards	Coordinated Universal Time offset UT ΔT DUT1 International Earth Rotation and Reference Systems Service ISO 31-1 ISO 8601 International Atomic Time 12-hour clock 24-hour clock Barycentric Coordinate Time Barycentric Dynamical Time Civil time Daylight saving time Geocentric Coordinate Time International Date Line IERS Reference Meridian Leap second Solar time Terrestrial Time Time zone 180th meridian
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Astronomical chronology	Galactic year Nuclear timescale Precession Sidereal time
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Related topics	Chronology Duration music Mental chronometry Decimal time Metric time System time Time metrology Time value of money Timekeeper

Timeline of the universe and Earth's history in galactic years

See also

References