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Unit of time From Wikipedia, the free encyclopedia
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 approximately 225 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]
The following list assumes that 1 galactic year is 225 million years.
Time | Event | |
---|---|---|
Galactic years (gal) |
Millions of years (Ma) | |
Past (years ago) | ||
About 61.32 gal | Big Bang | |
About 54 gal | Birth of the Milky Way | |
20.44 gal | Birth of the Sun | |
17–18 gal | 3937 Ma | Oceans appear on Earth |
16.889 gal | 3800 Ma | Life begins on Earth |
15.555 gal | 3500 Ma | Prokaryotes appear |
12 gal | 2700 Ma | Bacteria appear |
10 gal | 2250 Ma | Eukaryian period[5][6] first appearance of eukaryotes[7] Stable continents appear |
6.8 gal | 1530 Ma | Multicellular organisms appear |
2.4 gal | 540 Ma | Cambrian explosion occurs |
2 gal | 500 Ma | The first brain structure appears in worms |
1.11 gal | 250 Ma | Permian–Triassic extinction event |
0.2933 gal | Cretaceous–Paleogene extinction event | |
0.0013 gal | Emergence of anatomically modern humans | |
Future (years from now) | ||
0.15 gal | Mean time between impacts of asteroidal bodies in the order of magnitude of the K/Pg impactor has elapsed.[8] | |
1 gal | All the continents on Earth may fuse into a supercontinent. Three potential arrangements of this configuration have been dubbed Amasia, Novopangaea, and Pangaea Ultima.[9] | |
2–3 gal | Tidal acceleration moves the Moon far enough from Earth that total solar eclipses are no longer possible | |
4 gal | Carbon dioxide levels fall to the point at which C4 photosynthesis is no longer possible. Multicellular life dies out[10] | |
15 gal | Surface conditions on Earth are comparable to those on Venus today | |
22 gal | The Milky Way and Andromeda Galaxy begin to collide | |
25 gal | Sun ejects a planetary nebula, leaving behind a white dwarf | |
30 gal | The Milky Way and Andromeda complete their merger into a giant elliptical galaxy called Milkomeda or Milkdromeda[11] | |
500 gal | 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[12] | |
2000 gal | Local Group of 47 galaxies[13] coalesces into a single large galaxy[14] |
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