The Story of Earth
The First 4.5 Billion Years, from Stardust to Living Planet
Robert M Hazen, Central, 550 H4299s 2012
p96 ZrSiO4 zircons durable, uranium atoms decay to lead with 4.5 GY halflife, dating the crystals
p97 Water lowers the temperature at which zircons grow, causes higher O18 to O16 ratio, surface water does also
- Jack Hills Australia, 4.4 GY old zircon, oldest known surviving solid fragment of Earth, so there were oceans then
- p98 ~100 MY after Tethys, global mile-deep ocean
- p126 smaller protocontinents 3 GYa
- p177 2/3 of the current 4500 mineral types require oxygen (from life, in subsurface waters) to form
- i.e. turquoise, azurite, malachite
- minerals deriving from copper, uranium, iron, manganese, nickel, mercury, molybdenum, and others
- p178 Mars does NOT have this mineral diversity, the scarce water is frozen
- surface oxidized iron is "like a coating of paint", oxidized by disassociated water and escaped hydrogen
- p179 continents significantly smaller 2 GYa, also rusty red
p190 United Plates of America, Laurentian supercraton a conglomeration of > 6 large cratons
- p226 Dominic Papineau, anoxic dead zones from fertilizer runoff
- p263 10ppm chance of death by asteroid impact
- 300 meter Apophis will cross close by in 2029
- 8 meter rock every year
- 30 meter rock 1e-3 per year, Tunguska
- 800 meter 2e-6/y
- 5000 m rock 1e-7/y
- 10000 m Chixulub
- p266 Mars colony as alternative (?), one way trip
- but where does the industry and minerals come from
- p268 Loihi submerged 2 mile high southwest of Hawaii, emerging in a million years