Ocean and Earth Science, National Oceanography Centre Southampton, University of Southampton, Southampton SO14 3ZH, UK.
Department of Earth and Environmental Sciences, Wesleyan University, Middletown, Connecticut 06459, USA.
Nat Commun. 2017 Apr 4;8:14845. doi: 10.1038/ncomms14845.
The evolution of Earth's climate on geological timescales is largely driven by variations in the magnitude of total solar irradiance (TSI) and changes in the greenhouse gas content of the atmosphere. Here we show that the slow ∼50 Wm increase in TSI over the last ∼420 million years (an increase of ∼9 Wm of radiative forcing) was almost completely negated by a long-term decline in atmospheric CO. This was likely due to the silicate weathering-negative feedback and the expansion of land plants that together ensured Earth's long-term habitability. Humanity's fossil-fuel use, if unabated, risks taking us, by the middle of the twenty-first century, to values of CO not seen since the early Eocene (50 million years ago). If CO continues to rise further into the twenty-third century, then the associated large increase in radiative forcing, and how the Earth system would respond, would likely be without geological precedent in the last half a billion years.
在地质时间尺度上,地球气候的演化主要是由总太阳辐射(TSI)强度的变化和大气温室气体含量的变化驱动的。在这里,我们表明,在过去的大约 4.2 亿年中,TSI 缓慢增加了约 50 Wm(辐射强迫增加了约 9 Wm),但这一增长几乎被大气 CO 浓度的长期下降所抵消。这可能是由于硅酸盐风化的负反馈和陆地植物的扩张,这两者共同确保了地球的长期可居住性。如果人类不减少化石燃料的使用,那么到二十一世纪中叶,我们将面临自始新世(5000 万年前)以来从未见过的 CO 浓度。如果 CO 浓度在二十一世纪进一步上升,那么相关的辐射强迫的大幅增加,以及地球系统的反应,在过去的 5 亿年中可能没有地质先例。