Galactic year
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 is 230 million 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 following list assumes that 1 galactic year is 225 million years.
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 |
0.2935 galactic years ago | Cretaceous–Paleogene extinction event |
Present day | |
---|---|
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] |
See also[]
- Geologic time scale
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 (20 October 2007). "Pangaea, the comeback". New Scientist. Retrieved 2 January 2014.
- ^ 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:2005BGD.....2.1665F. doi:10.5194/bgd-2-1665-2005.
- ^ 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.tmp..333C. 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.
- ^ "The Local Group of Galaxies". University of Arizona. Students for the Exploration and Development of Space. Retrieved 2 October 2009.
- ^ 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.
- Milky Way
- Types of year