Greenhouse and icehouse Earth
Throughout Earth's climate history (Paleoclimate) its climate has fluctuated between two primary states: greenhouse and icehouse Earth.[1] Both climate states last for millions of years and should not be confused with glacial and interglacial periods, which occur as alternate phases within an icehouse period and tend to last less than 1 million years.[2] There are five known Icehouse periods in Earth's climate history, which are known as the Huronian, Cryogenian, Andean-Saharan, Late Paleozoic, and Late Cenozoic glaciations.[1] The main factors involved in changes of the paleoclimate are believed to be the concentration of atmospheric carbon dioxide (CO2), changes in Earth's orbit, long-term changes in the solar constant, and oceanic and orogenic changes from tectonic plate dynamics.[3] Greenhouse and icehouse periods have played key roles in the evolution of life on Earth by directly and indirectly forcing biotic adaptation and turnover at various spatial scales across time.[4][5]
Greenhouse Earth
[edit]A "greenhouse Earth" is a period during which no continental glaciers exist anywhere on the planet.[6] Additionally, the levels of carbon dioxide and other greenhouse gases (such as water vapor and methane) are high, and sea surface temperatures (SSTs) range from 28 °C (82.4 °F) in the tropics to 0 °C (32 °F) in the polar regions.[7] Earth has been in a greenhouse state for about 85% of its history.[6]
The state should not be confused with a hypothetical runaway greenhouse effect, which is an irreversible tipping point that corresponds to the ongoing runaway greenhouse effect on Venus.[8] The IPCC states that "a 'runaway greenhouse effect'—analogous to [that of] Venus—appears to have virtually no chance of being induced by anthropogenic activities."[9]
Causes
[edit]There are several theories as to how a greenhouse Earth can come about. Geologic climate proxies indicate that there is a strong correlation between a greenhouse state and high CO2 levels.[1] However, it is important to recognize that high CO2 levels are interpreted as an indicator of Earth's climate, rather than as an independent driver. Other phenomena have instead likely played a key role in influencing global climate by altering oceanic and atmospheric currents[10] and increasing the net amount of solar radiation absorbed by Earth's atmosphere.[11] Such phenomena may include but are not limited to tectonic shifts that result in the release of greenhouse gases (such as CO2 and CH4) via volcanic activity,[12] Volcanoes emit massive amounts of CO2 and methane into the atmosphere when they are active, which can trap enough heat to cause a greenhouse effect. On Earth, atmospheric concentrations of greenhouse gases like carbon dioxide (CO2) and methane (CH4) are higher, trapping solar energy in the atmosphere via the greenhouse effect. Methane, the main component of natural gas, is responsible for more than a quarter of the current global warming. It is a formidable pollutant with an 80-fold higher global warming potential than CO2 in the 20 years after it has been introduced into the atmosphere. An increase in the solar constant increases the net amount of solar energy absorbed into Earth's atmosphere,[11] and changes in Earth's obliquity and eccentricity increase the net amount of solar radiation absorbed into Earth's atmosphere.[11]
Icehouse Earth
[edit]Earth is now in an icehouse state, and ice sheets are present in both poles simultaneously.[6] Climatic proxies indicate that greenhouse gas concentrations tend to lower during an icehouse Earth.[13] Similarly, global temperatures are also lower under Icehouse conditions.[14] Earth then fluctuates between glacial and interglacial periods, and the size and the distribution of continental ice sheets fluctuate dramatically.[15] The fluctuation of the ice sheets results in changes in regional climatic conditions that affect the range and the distribution of many terrestrial and oceanic species.[4][5][16] On scales ranging from thousands to hundreds of millions of years, the Earth's climate has transitioned from warm to chilly intervals within life-sustaining ranges. There have been three periods of glaciation in the Phanerozoic Eon (Ordovician, Carboniferous, and Cenozoic), each lasting tens of millions of years and bringing ice down to sea level at mid-latitudes. During these frigid "icehouse" intervals, sea levels were generally lower, CO2 levels in the atmosphere were lower, net photosynthesis and carbon burial were lower, and oceanic volcanism was lower than during the alternate "greenhouse" intervals. Transitions from Phanerozoic icehouse to greenhouse intervals coincided with biotic crises or catastrophic extinction events, indicating complicated biosphere-hydrosphere feedbacks.[39]
The glacial and interglacial periods tend to alternate in accordance with solar and climatic oscillation until Earth eventually returns to a greenhouse state.[15]
Earth's current icehouse state is known as the Quaternary Ice Age and began approximately 2.58 million years ago.[17] However, an ice sheet has existed in Antarctica for approximately 34 million years.[17] Earth is now in a clement interglacial period that started approximately 11,800 years ago.[17] Earth will likely phase into another interglacial period such as the Eemian, which occurred between 130,000 and 115,000 years ago, during which evidence of forest in North Cape, Norway, and hippopotamus in the Rhine and Thames Rivers can be observed.[16] Earth is expected to continue to transition between glacial and interglacial periods until the cessation of the Quaternary Ice Age and will then enter another greenhouse state.
Causes
[edit]It is well established that there is strong correlation between low CO2 levels and an icehouse state.[18] However, that does not mean that decreasing atmospheric levels CO2 is a primary driver of a transition to the icehouse state.[11][18] Rather, it may be an indicator of other solar, geologic, and atmospheric processes at work.[18][10][11]
Potential drivers of previous icehouse states include the movement of the tectonic plates and the opening and the closing of oceanic gateways.[19] They seem to play a crucial part in driving Earth into an icehouse state, as tectonic shifts result in the transportation of cool, deep water, which circulates to the ocean surface and assists in ice sheet development at the poles.[7] Examples of oceanic current shifts as a result of tectonic plate dynamics include the opening of the Tasmanian Gateway 36.5 million years ago, which separated Australia and Antarctica,[20][21] and the opening of the Drake Passage 32.8 million years ago by the separation of South America and Antarctica,[21] both of which are believed to have allowed for the development of the Antarctic ice sheet. The closing of the Isthmus of Panama and of the Indonesian seaway approximately 3 to 4 million years ago may also be a contributor to Earth's current icehouse state.[22] One proposed driver of the Ordovician Ice Age was the evolution of land plants. Under that paradigm, the rapid increase in photosynthetic biomass gradually removed CO2 from the atmosphere and replaced it with increasing levels of O2, which induced global cooling.[23] One proposed driver of the Quaternary Ice age is the collision of the Indian Subcontinent with Eurasia to form the Himalayas and the Tibetan Plateau.[17] Under that paradigm, the resulting continental uplift revealed massive quantities of unweathered silicate rock CaSiO
3, which reacted with CO2 to produce CaCO
3 (lime) and SiO
2 (silica). The CaCO
3 was eventually transported to the ocean and taken up by plankton, which then died and sank to the bottom of the ocean, which effectively removed CO2 from the atmosphere.[17]
Glacials and interglacials
[edit]Within icehouse states are "glacial" and "interglacial" periods that cause ice sheets to build up or to retreat. The main causes for glacial and interglacial periods are variations in the movement of Earth around the Sun.[24] The astronomical components, discovered by the Serbian geophysicist Milutin Milanković and now known as Milankovitch cycles, include the axial tilt of Earth, the orbital eccentricity (or shape of the orbit), and the precession (or wobble) of Earth's rotation. The tilt of the axis tends to fluctuate from 21.5° to 24.5° and back every 41,000 years on the vertical axis. The change actually affects the seasonality on Earth since a change in solar radiation hits certain areas of the planet more often on a higher tilt, and a lower tilt creates a more even set of seasons worldwide. The changes can be seen in ice cores, which also contain evidence that during glacial times (at the maximum extension of the ice sheets), the atmosphere had lower levels of carbon dioxide. That may be caused by the increase or the redistribution of the acid-base balance with bicarbonate and carbonate ions that deals with alkalinity. During an icehouse period, only 20% of the time is spent in interglacial, or warmer times.[24] Model simulations suggest that the current interglacial climate state will continue for at least another 100,000 years because of CO2 emissions, including the complete deglaciation of the Northern Hemisphere.[25]
Snowball Earth
[edit]A "snowball Earth" is the complete opposite of greenhouse Earth in which Earth's surface is completely frozen over. However, a snowball Earth technically does not have continental ice sheets like during the icehouse state. "The Great Infra-Cambrian Ice Age" has been claimed to be the host of such a world, and in 1964, the scientist W. Brian Harland brought forth his discovery of indications of glaciers in the low latitudes (Harland and Rudwick). That became a problem for Harland because of the thought of the "Runaway Snowball Paradox" (a kind of Snowball effect) that once Earth enters the route of becoming a snowball Earth, it would never be able to leave that state. However, Joseph Kirschvink brought up a solution to the paradox in 1992. Since the continents were then huddled at the low and the middle latitudes, there was less ocean water available to absorb the higher amount solar energy hitting the tropics, and there was also an increase in rainfall because more land exposed to higher solar energy might have caused chemical weathering, which would contribute to removal of CO2 from the atmosphere. Both conditions might have caused a substantial drop in CO2 atmospheric levels which resulted in cooling temperatures and increasing ice albedo (ice reflectivity of incoming solar radiation), which would further increase global cooling (a positive feedback). That might have been the mechanism of entering Snowball Earth state. Kirschvink explained that the way to get out of Snowball Earth state could be connected again to carbon dioxide. A possible explanation is that during Snowball Earth, volcanic activity would not halt but accumulate atmospheric CO2. At the same time, global ice cover would prevent chemical weathering (particularly hydrolysis), responsible for removal of CO2 from the atmosphere. CO2 therefore accumulated in the atmosphere. Once the atmosphere accumulation of CO2 reached a threshold, temperature would rise enough for ice sheets to start melting. That would in turn reduce the ice albedo effect, which would in turn further reduce the ice cover and allow an exit from Snowball Earth. At the end of Snowball Earth, before the equilibrium "thermostat" between volcanic activity and the by then slowly resuming chemical weathering was reinstated, CO2 in the atmosphere had accumulated enough to cause temperatures to peak to as much as 60 °C, thrusting the Earth into a brief moist greenhouse state. Around the same geologic period of Snowball Earth (it is debated if it was the cause or the result of Snowball Earth), the Great Oxygenation Event (GOE) was occurring. The event known as the Cambrian Explosion followed and produced the beginnings of populous bilateral organisms, as well as a greater diversity and mobility in multicellular life.[26] However, some biologists claim that a complete snowball Earth could not have happened since photosynthetic life would not have survived under many meters of ice without sunlight. However, sunlight has been observed to penetrate meters of ice in Antarctica[citation needed]. Most scientists[citation needed] now believe that a "hard" Snowball Earth, one completely covered by ice, is probably impossible. However, a "slushball Earth," with points of opening near the equator, is considered to be possible.
Recent studies may have again complicated the idea of a snowball Earth. In October 2011, a team of French researchers announced that the carbon dioxide during the last speculated "snowball Earth" may have been lower than originally stated, which provides a challenge in finding out how Earth got out of its state and whether a snowball or a slushball Earth occurred.[27]
Transitions
[edit]Causes
[edit]The Eocene, which occurred between 56.0 and 33.9 million years ago, was Earth's warmest temperature period for 100 million years.[28] However, the "super-greenhouse" period had eventually become an icehouse period by the late Eocene. It is believed that the decline of CO2 caused the change, but mechanisms of positive feedback may have contributed to the cooling.
The best available record for a transition from an icehouse to greenhouse period in which plant life existed is for the Permian period, which occurred around 300 million years ago. A major transition took place 40 million years ago and caused Earth to change from a moist, icy planet in which rainforests covered the tropics to a hot, dry, and windy location in which little could survive. Professor Isabel P. Montañez of University of California, Davis, who has researched the time period, found the climate to be "highly unstable" and to be "marked by dips and rises in carbon dioxide."[29]
Impacts
[edit]The Eocene-Oligocene transition was the latest and occurred approximately 34 million years ago. It resulted in a rapid global cooling, the glaciation of Antarctica, and a series of biotic extinction events. The most dramatic species turnover event associated with the time period is the Grande Coupure, a period that saw the replacement of European tree-dwelling and leaf-eating mammal species by migratory species from Asia.[30]
Research
[edit]Paleoclimatology is a branch of science that attempts to understand the history of greenhouse and icehouse conditions over geological time. The study of ice cores, dendrochronology, ocean and lake sediments (varve), palynology, (paleobotany), isotope analysis (such as radiometric dating and stable isotope analysis), and other climate proxies allows scientists to create models of Earth's past energy budgets and the resulting climate. One study has shown that atmospheric carbon dioxide levels during the Permian age rocked back and forth between 250 parts per million, which is close to today's levels, up to 2,000 parts per million.[29] Studies on lake sediments suggest that the "hothouse" or "super-greenhouse" Eocene was in a "permanent El Niño state" after the 10 °C warming of the deep ocean and high latitude surface temperatures shut down the Pacific Ocean's El Niño-Southern Oscillation.[31] A theory was suggested for the Paleocene–Eocene Thermal Maximum on the sudden decrease of the carbon isotopic composition of the global inorganic carbon pool by 2.5 parts per million.[32] A hypothesis posed for this drop of isotopes was the increase of methane hydrates, the trigger for which remains a mystery. The increase of atmospheric methane, which happens to be a potent but short-lived greenhouse gas, increased the global temperatures by 6 °C with the assistance of the less potent carbon dioxide.[citation needed]
List of icehouse and greenhouse periods
[edit]- A greenhouse period ran from 4.6 to 2.4 billion years ago.
- Huronian glaciation – an icehouse period that ran from 2.4 billion to 2.1 billion years ago
- A greenhouse period ran from 2.1 billion to 720 million years ago.
- Cryogenian – an icehouse period that ran from 720 to 635 million years ago during which the entire Earth was at times frozen over
- A greenhouse period ran from 635 million years ago to 450 million years ago.
- Andean-Saharan glaciation – an icehouse period that ran from 450 million to 420 million years ago
- A greenhouse period ran from 420 million years ago to 360 million years ago.
- Late Paleozoic Ice Age – an icehouse period that ran from 360 million to 260 million years ago
- A greenhouse period ran from 260 million years ago to 33.9 million years ago.
- Late Cenozoic Ice Age – the current icehouse period, which began 33.9 million years ago
Modern conditions
[edit]Currently, Earth is in an icehouse climate state. About 34 million years ago, ice sheets began to form in Antarctica; the ice sheets in the Arctic did not start forming until 2 million years ago.[33] Some processes that may have led to the current icehouse may be connected to the development of the Himalayan Mountains and the opening of the Drake Passage between South America and Antarctica, but climate model simulations suggest that the early opening of the Drake Passage played only a limited role, and the later constriction of the Tethys and Central American Seaways is more important in explaining the observed Cenozoic cooling.[34] Scientists have tried to compare the past transitions between icehouse and greenhouse, and vice versa, to understand what type of climate state Earth will have next.
Without the human influence on the greenhouse gas concentration, a glacial period would be the next climate state. Predicted changes in orbital forcing suggest that in absence of human-made global warming, the next glacial period would begin at least 50,000 years from now[35] (see Milankovitch cycles), but the ongoing anthropogenic greenhouse gas emissions mean the next climate state will be a greenhouse Earth period.[33] Permanent ice is actually a rare phenomenon in the history of Earth and occurs only in coincidence with the icehouse effect, which has affected about 20% of Earth's history.
See also
[edit]References
[edit]- ^ a b c Summerhayes, Colin P.. (8 September 2020). Palaeoclimatology : from snowball earth to the anthropocene. John Wiley & Sons. ISBN 978-1-119-59138-2. OCLC 1236201953. Archived from the original on 18 April 2021. Retrieved 17 April 2021.
- ^ Paillard, D. (2006-07-28). "ATMOSPHERE: What Drives the Ice Age Cycle?". Science. 313 (5786): 455–456. doi:10.1126/science.1131297. ISSN 0036-8075. PMID 16873636. S2CID 128379788. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ P., Summerhayes, C. (13 July 2015). Earths evolving climate : a geological perspective. John Wiley & Sons. ISBN 978-1-118-89737-9. OCLC 907811494. Archived from the original on 21 November 2021. Retrieved 17 April 2021.
{{cite book}}
: CS1 maint: multiple names: authors list (link) - ^ a b Godfrey, Laurie R.; Samonds, Karen E.; Baldwin, Justin W.; Sutherland, Michael R.; Kamilar, Jason M.; Allfisher, Kristen L. (2020-08-08). "Mid-Cenozoic climate change, extinction, and faunal turnover in Madagascar, and their bearing on the evolution of lemurs". BMC Evolutionary Biology. 20 (1): 97. doi:10.1186/s12862-020-01628-1. ISSN 1471-2148. PMC 7414565. PMID 32770933.
- ^ a b Nge, Francis J.; Biffin, Ed; Thiele, Kevin R.; Waycott, Michelle (2020-01-22). "Extinction pulse at Eocene–Oligocene boundary drives diversification dynamics of two Australian temperate floras". Proceedings of the Royal Society B: Biological Sciences. 287 (1919): 20192546. doi:10.1098/rspb.2019.2546. ISSN 0962-8452. PMC 7015341. PMID 31964242.
- ^ a b c Understanding Earth's Deep Past. 2011-08-02. doi:10.17226/13111. ISBN 978-0-309-20915-1. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ a b Stella., Woodard (2012). Oceanic and atmospheric response to climate change over varying geologic timescales. [Texas A & M University]. OCLC 805585971. Archived from the original on 2021-04-18. Retrieved 2021-04-17.
- ^ Steffen, Will; Rockström, Johan; Richardson, Katherine; Lenton, Timothy M.; Folke, Carl; Liverman, Diana; Summerhayes, Colin P.; Barnosky, Anthony D.; Cornell, Sarah E.; Crucifix, Michel; Donges, Jonathan F.; Fetzer, Ingo; Lade, Steven J.; Scheffer, Marten; Winkelmann, Ricarda; Schellnhuber, Hans Joachim (2018-08-06). "Trajectories of the Earth System in the Anthropocene". Proceedings of the National Academy of Sciences. 115 (33): 8252–8259. Bibcode:2018PNAS..115.8252S. doi:10.1073/pnas.1810141115. ISSN 0027-8424. PMC 6099852. PMID 30082409.
- ^ "Archived copy" (PDF). Archived from the original (PDF) on 2018-11-09. Retrieved 2018-11-02.
{{cite web}}
: CS1 maint: archived copy as title (link) - ^ a b Young, Grant M. (March 2019). "Aspects of the Archean-Proterozoic transition: How the great Huronian Glacial Event was initiated by rift-related uplift and terminated at the rift-drift transition during break-up of Lauroscandia". Earth-Science Reviews. 190: 171–189. Bibcode:2019ESRv..190..171Y. doi:10.1016/j.earscirev.2018.12.013. ISSN 0012-8252. S2CID 134347305. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ a b c d e Haigh, Joanna D.; Cargill, Peter (2015-06-23). The Sun's Influence on Climate. Princeton University Press. doi:10.23943/princeton/9780691153834.001.0001. ISBN 978-0-691-15383-4. S2CID 128666503. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ Schmidt, Anja; Fristad, Kirsten E.; Elkins-Tanton, Linda T., eds. (2015). Volcanism and Global Environmental Change. Cambridge University Press. doi:10.1017/cbo9781107415683. ISBN 9781107415683. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ "Review of "Global mean surface temperature and climate sensitivity of the EECO, PETM and latest Paleocene"". 2020-02-14. doi:10.5194/cp-2019-167-rc1.
{{cite journal}}
: Cite journal requires|journal=
(help) - ^ Zhang, Laiming (2019). "The evolution of latitudinal temperature gradients from the latest Cretaceous through the Present". Earth-Science Reviews. 189: 147–158. Bibcode:2019ESRv..189..147Z. doi:10.1016/j.earscirev.2019.01.025. S2CID 134433505. Archived from the original on 2021-11-21. Retrieved 2021-04-17 – via Science Direct.
- ^ a b Summerhayes, C. P. (2020). Palaeoclimatology : from snowball earth to the anthropocene. Chichester, West Sussex. ISBN 978-1-119-59138-2. OCLC 1145913723. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
{{cite book}}
: CS1 maint: location missing publisher (link) - ^ a b van Kolfschoten, Th. (August 2000). "The Eemian mammal fauna of central Europe". Netherlands Journal of Geosciences. 79 (2–3): 269–281. doi:10.1017/s0016774600021752. ISSN 0016-7746.
- ^ a b c d e Rose, James (January 2010). "Quaternary climates: a perspective for global warming". Proceedings of the Geologists' Association. 121 (3): 334–341. Bibcode:2010PrGA..121..334R. doi:10.1016/j.pgeola.2010.07.001. ISSN 0016-7878. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ a b c Woodard, S. C., & Thomas, D. J. (2012). Oceanic and atmospheric response to climate change over varying geologic timescales. by Stella C. Woodard. [Texas A&M University].
- ^ SMITH, ALAN G.; PICKERING, KEVIN T. (May 2003). "Oceanic gateways as a critical factor to initiate icehouse Earth". Journal of the Geological Society. 160 (3): 337–340. Bibcode:2003JGSoc.160..337S. doi:10.1144/0016-764902-115. ISSN 0016-7649. S2CID 127653725. Archived from the original on 2007-11-30. Retrieved 2021-04-17.
- ^ The Tasmanian Gateway Between Australia and Antarctica: Paleoclimate and Paleoceanography. ODP Preliminary Report. Vol. 189. Ocean Drilling Program. June 2000. doi:10.2973/odp.pr.189.2000. Archived from the original on 2021-11-21. Retrieved 2021-04-17.
- ^ a b Stant, S.A.; Lara, J.; McGonigal, K.L.; Ladner, B.C. (2004-04-22), "Quaternary Nannofossil Biostratigraphy from Ocean Drilling Program Leg 189, Tasmanian Gateway", Proceedings of the Ocean Drilling Program, 189 Scientific Results, Proceedings of the Ocean Drilling Program, vol. 189, Ocean Drilling Program, doi:10.2973/odp.proc.sr.189.109.2004, archived from the original on 2021-11-21, retrieved 2021-04-15
- ^ Smith, Alan G.; Kevin T. Pickering (2003). "Oceanic gateways as a critical factor to initiate icehouse Earth". Journal of the Geological Society. 160 (3): 337–340. Bibcode:2003JGSoc.160..337S. doi:10.1144/0016-764902-115. S2CID 127653725.
- ^ Lenton, Timothy M.; Crouch, Michael; Johnson, Martin; Pires, Nuno; Dolan, Liam (February 2012). "First plants cooled the Ordovician". Nature Geoscience. 5 (2): 86–89. Bibcode:2012NatGe...5...86L. doi:10.1038/ngeo1390. ISSN 1752-0894. Archived from the original on 2021-03-20. Retrieved 2021-04-17.
- ^ a b Broecker, Wallace S.; George H. Denton (January 1990). "What Drives Glacial Cycles". Scientific American. 262: 49–56. Bibcode:1990SciAm.262a..49B. doi:10.1038/scientificamerican0190-48.
- ^ A. Ganopolski; R. Winkelmann; H. J. Schellnhuber (2016). "Critical insolation–CO2 relation for diagnosing past and future glacial inception". Nature. 529 (7585): 200–203. Bibcode:2016Natur.529..200G. doi:10.1038/nature16494. PMID 26762457. S2CID 4466220.
- ^ Maruyama, S.; M. Santosh (2008). "Models on Snowball Earth and Cambrian explosion: A synopsis". Gondwana Research. 14 (1–2): 22–32. Bibcode:2008GondR..14...22M. doi:10.1016/j.gr.2008.01.004.
- ^ CNRS, Delegation Paris Michel-Ange. "Snowball Earth's hypothesis challenged". ScienceDaily. Archived from the original on 19 October 2011. Retrieved 24 November 2011.
- ^ Herath, Anuradha K. "From Greenhouse to icehouse". Astrobio. Archived from the original on 14 October 2011. Retrieved 28 October 2011.
- ^ a b University of California-Davis. "A Bumpy Shift from Ice House to Greenhouse". ScienceDaily. Archived from the original on 10 June 2013. Retrieved 4 November 2011.
- ^ Prothero, D. R. (1994-01-01). "The Late Eocene-Oligocene Extinctions" (PDF). Annual Review of Earth and Planetary Sciences. 22 (1): 145–165. Bibcode:1994AREPS..22..145P. doi:10.1146/annurev.ea.22.050194.001045.
- ^ Huber, Matthew; Rodrigo Caballero (7 February 2003). "Eocene El Nino: Evidence for Robust Tropical Dynamics in the "Hothouse"". Science. 299 (5608): 877–881. Bibcode:2003Sci...299..877H. doi:10.1126/science.1078766. PMID 12574626. S2CID 19838005.
- ^ Higgins, John A.; Daniel P. Schrag (2006). "Beyond Methane: Towards a theory for the Paleocene-Eocene Thermal Maximum". Earth and Planetary Science Letters. 245 (3–4): 523–537. Bibcode:2006E&PSL.245..523H. doi:10.1016/j.epsl.2006.03.009.
- ^ a b Montanez, Isabel; G.S. Soreghan (March 2006). "Earth's Fickle Climate: Lessons Learned from Deep-Time Ice Ages". Geotimes. 51: 24–27.
- ^ "Zhang, Zhongshi & Nisancioglu, Kerim & Flatøy, F. & Bentsen, M. & Bethke, I. & Wang, H.. (2009). Did the opening of the Drake Passage play a significant role in Cenozoic cooling?". Archived from the original on 2021-11-21. Retrieved 2020-09-14.
- ^ Berger A, Loutre MF (August 2002). "Climate. An exceptionally long interglacial ahead?". Science. 297 (5585): 1287–8. doi:10.1126/science.1076120. PMID 12193773. S2CID 128923481.