Available online 7 March 2018The concentration of atmospheric oxygen (pO2) is thought to have increased throughout Earth history, punctuated by rapid increases ca. 2.4 and 0.8 billion years ago near the beginning and end of the Proterozoic Eon. As photosynthesis is the largest source of free O2, the reigning paradigm of rising O2 levels centres around biologic metabolism. Here we show that the phosphorus content of igneous rocks correlates, in a first-order sense, with secular increases in O2 through time, suggesting that rising O2 levels are affected by long-term mantle cooling and its effect on the continental phosphorus inventory. Because phosphorus is the limiting nutrient for primary productivity, its availability has fundamental contr...
The question of whether rising oxygen levels through Earth history have driven the evolution of life...
Oxygenation of Earth’s atmosphere and oceans occurred across three major steps during the Paleoprote...
Several lines of geologic evidence have pointed to a significant increase in P sub O2 about 2,000 m....
Stepwise increases in oxygen abundance have been recognised as some of the most significant events t...
There is no direct geologic record of the level of free oxygen in the atmosphere over Earth history....
© 2016 Macmillan Publishers Limited.Earth owes its oxygenated atmosphere to its unique claim on life...
The macronutrient phosphorus is thought to limit primary productivity in the oceans on geological ti...
The macronutrient phosphorus is thought to limit primary productivity in the oceans on geological ti...
Atmospheric oxygen was maintained at low levels throughout huge swathes of Earth's early history. Es...
A shift toward higher atmospheric oxygen concentration during the late Proterozoic has been inferred...
Terrestrial weathering releases phosphorus and other essential nutrients that fuel life in Earth...
Terrestrial weathering releases phosphorus and other essential nutrients that fuel life in Earth...
Terrestrial weathering releases phosphorus and other essential nutrients that fuel life in Earth...
Abstract Oxygen is a potential biosignature for terrestrial Earth-like planets. The primary source o...
This article examines the geological evidence for the rise of atmospheric oxygen and the origin of o...
The question of whether rising oxygen levels through Earth history have driven the evolution of life...
Oxygenation of Earth’s atmosphere and oceans occurred across three major steps during the Paleoprote...
Several lines of geologic evidence have pointed to a significant increase in P sub O2 about 2,000 m....
Stepwise increases in oxygen abundance have been recognised as some of the most significant events t...
There is no direct geologic record of the level of free oxygen in the atmosphere over Earth history....
© 2016 Macmillan Publishers Limited.Earth owes its oxygenated atmosphere to its unique claim on life...
The macronutrient phosphorus is thought to limit primary productivity in the oceans on geological ti...
The macronutrient phosphorus is thought to limit primary productivity in the oceans on geological ti...
Atmospheric oxygen was maintained at low levels throughout huge swathes of Earth's early history. Es...
A shift toward higher atmospheric oxygen concentration during the late Proterozoic has been inferred...
Terrestrial weathering releases phosphorus and other essential nutrients that fuel life in Earth...
Terrestrial weathering releases phosphorus and other essential nutrients that fuel life in Earth...
Terrestrial weathering releases phosphorus and other essential nutrients that fuel life in Earth...
Abstract Oxygen is a potential biosignature for terrestrial Earth-like planets. The primary source o...
This article examines the geological evidence for the rise of atmospheric oxygen and the origin of o...
The question of whether rising oxygen levels through Earth history have driven the evolution of life...
Oxygenation of Earth’s atmosphere and oceans occurred across three major steps during the Paleoprote...
Several lines of geologic evidence have pointed to a significant increase in P sub O2 about 2,000 m....