What Caused the Lack of an Ice Sheet on Siberia During the Last Glacial Maximum?

In summary: The paper suggests the temperatures at the end of the Permian period were higher than previously thought, possibly higher than at any time in the past 600 million years. The Permian extinction, which was the largest ever, occurred at this time (251 mya). The authors believe that low oxygen levels in the ocean contributed to the loss of 90-95% of all marine species. The dinosaurs came later (215-65 mya).Based on available estimates, the authors believe that the mean global temperature was 6C higher than the present level over the past 600 million years.
  • #1
KTevolved
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I was just wondering when the last time the global average temperature was 90 degrees F? Also wondering what a temperature of this extream would do to todays environment and life it self?
 
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  • #2
What exactly is your intention with that question? Has there ever been a period when the global temperature was 90F? Reconstructing paleologic temperatures is something like solving N variables with maybe N-10 equations. or another comparison would be, trying to overview the complete ocean while looking through a porthole.

There are reasons to believe that Earth was somewhat warmer in the late Miocene a few million years ago, (http://www.nature.com/nature/journal/v486/n7401/full/nature11200.html), but certainly not 90F. It was probably a good bit warmer during the Paleocene especially the Paleocene Eocene Thermal Maximum but 90F as an average appears unlikely. Maybe at the at the time the Earth was formed.
 
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  • #3
Just wondering beause of global warming. I didnt realize it wouldn't have occurred since the beginning of Earth formation, i thought it would hae occurred when the dinosaurs were alive and there were no ice caps.
 
  • #4
This is not the place to discuss that. See why
 
  • #5
Alright so do you know of any forums that deal with this? I am getting into the topic.
 
  • #6
KTevolved said:
Alright so do you know of any forums that deal with this? I am getting into the topic.
Average temperature since records have been kept average ~57F. The sun is slowly getting hotter, eventually, it will be too hot for life as we know it.

Earth's fate

Earth's ultimate fate is precarious. As a red giant, the Sun will have a maximum radius beyond the Earth's current orbit, 1 AU (1.5×1011 m), 250 times the present radius of the Sun.[106] However, by the time it is an asymptotic giant branch star, the Sun will have lost roughly 30% of its present mass due to a stellar wind, so the orbits of the planets will move outward. If it were only for this, Earth would probably be spared, but new research suggests that Earth will be swallowed by the Sun owing to tidal interactions.[106] Even if Earth should escape incineration in the Sun, still all its water will be boiled away and most of its atmosphere will escape into space. Even during its current life in the main sequence, the Sun is gradually becoming more luminous (about 10% every 1 billion years), and its surface temperature is slowly rising. The Sun used to be fainter in the past, which is possibly the reason life on Earth has only existed for about 1 billion years on land. The increase in solar temperatures is such that in about another billion years the surface of the Earth will likely become too hot for liquid water to exist, ending all terrestrial life.[106][107]

http://en.wikipedia.org/wiki/Sun#Earth.27s_fate

You can easily search for information online.
 
  • #7
www.cgd.ucar.edu/ccr/aboutus/staff/kiehl/Kiehl-Shields.pdf

This paper suggests the temperatures at the end of the Permian period were higher than previously thought, possibly higher than at any time in the past 600 million years. The Permian mass extinction, which was the largest ever, occurred at this time (251 mya). The authors believe that low oxygen levels in the ocean contributed to the loss of 90-95% of all marine species. The dinosaurs came later (215-65 mya).

Temperature simulations indicate summer mean temperatures in parts of subtropical Pangaea (the single super-continent that existed at that time) to be in excess of 40C (104F). The overall simulated mean annual temperature for the planet at that time was about 8C higher than today.

EDIT: The paper seems to be unavailable right now, 0300 Aug 29 2012. Here's another study on late Permian climate: They are only estimating a mean global temperature 6C higher than the present level, at least with one of two models they're looking at. This paper is looking at the late Permian, but not necessarily at the end of the Permian (Permian-Triassic boundary) which is the subject of the first paper. In any case, there seems to be no evidence that the mean global temperature was ever much higher than 8C above the present level over the past 600 million years based on available estimates.

www.ipgp.fr/~fluteau/UIA/articles/7_fluteau-pangea-climate.pdf
 
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  • #8
SW VandeCarr said:
www.cgd.ucar.edu/ccr/aboutus/staff/kiehl/Kiehl-Shields.pdf

This paper suggests the temperatures at the end of the Permian period were higher than previously thought, possibly higher than at any time in the past 600 million years. The Permian extinction, which was the largest ever, occurred at this time (251 mya). The authors believe that low oxygen levels in the ocean contributed to the loss of 90-95% of all marine species. The dinosaurs came later (215-65 mya).

The authors' isothermal map indicates mean annual temperatures in tropical Pangaea (the single super-continent that existed at that time) to be as high as 32C (90F).
Can you point out for me where it says the average GLOBAL temperature was estimated to be that high, not just in some areas. I'm sure it's there, but I don't have time to look.

The map seems to show temperature variations in different locations.
 
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  • #9
Evo said:
Can you point out for me where it says the average GLOBAL temperature was estimated to be that high, not just in some areas. I'm sure it's there, but I don't have time to look.

The map seems to show temperature variations in different locations.

The last sentence before the RESULTS section says the simulated mean annual global surface temperature was 7.98 C higher than it is today. BTW, I edited the second paragraph.
 
  • #10
SW VandeCarr said:
The last sentence before the RESULTS section says the simulated mean annual global surface temperature was 7.98 C higher than it is today. BTW, I edited the second paragraph.
Thanks!

Then that would only bring the average temp then to 22.5C or 72.5F. And 7.98 C is very high, other estimates range from 5 to 6.5 C. I wonder if they goofed on their data for current world temperature?

Global Mean Annual Temperature

Average per Decade

2000s 14.51C 58.12F


About the Temperature Data

The temperature data are provided publicly by NASA's Goddard Institute for Space Studies (GISS), based in New York City. GISS has compiled and analyzed data from a thousand weather stations around the world, ship and satellite observations of sea temperatures, and measurements at Antarctic research stations to form a global temperature index. The annual averages go back in history only to 1880, when meteorologists began using modern scientific instruments to monitor temperatures precisely.

http://www.currentresults.com/Environment-Facts/changes-in-earth-temperature.php

I am only providing this to show what the current Global Mean Annual Temperature is.
 
  • #11
It appears that this Kiehl & Shields 2005 study is the result of a simulation model, which I guess would not have any higher status than a hypothesis.

Remarkable is the mentioning of the Siberian traps, the main suspect for the P-T extinction, remarkable because the last three known eruptions with high aerosol emissions, Agung 1963, El Chinon 1982 and Pinotubo 1991 were followed by a few years of cooler temperatures. Also following the largest eruption of modern times, the Tambora was followed by the year without summer (1816). All in all, and also giving the uncertainty of temperatures only several thousand years, due to conflicting evidence, it would suggest that their outcome may not be the most robust.
 
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  • #12
Andre said:
It appears that this Kiehl & Shields 2005 study is the result of a simulation model, which I guess would not have any higher status than a hypothesis.

Remarkable is the mentioning of the Siberian traps, the main suspect for the P-T extinction, remarkable because the last three known eruptions with high aerosol emissions, Agung 1963, El Chinon 1982 and Pinotubo 1991 were followed by a few years of cooler temperatures. Also following the largest eruption of modern times, the Tambora was followed by the year without summer (1816). All in all, and also giving the uncertainty of temperatures only several thousand years, due to conflicting evidence, it would suggest that their outcome may not be very robust.

I'm not an Earth scientist although I've had a lifelong interest in meteorology. Wouldn't the value of simulations depend on the quality of data? How much could one say about the climate of Pangaea in the late Permian without computer simulation? I guess we could say it would have an extreme continental climate with monsoons and a lot of deserts. Beyond that, it would depend on specific evidence from various parts of the supercontinent that are accessible today. Can we categorically say that computer simulations based on such evidence are not very useful in investigating paleoclimates?

BTW: Did you see the Fluteau, Besse et al paper I posted later?
 
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  • #13
SW VandeCarr said:
I'm not an Earth scientist although I've had a lifelong interest in meteorology. Wouldn't the value of simulations depend on the quality of data? How much could one say about the climate of Pangaea in the late Permian without computer simulation? I guess we could say it would have an extreme continental climate with monsoons and a lot of deserts. Beyond that, it would depend on specific evidence from various parts of the supercontinent that are accessible today. Can we categorically say that computer simulations based on such evidence are not very useful in investigating paleoclimates?

Maybe the quality of suppositions is even more important. You're looking at the end of the line of a lot of them, for instance the temperature supposition are based on stable oxygen isotopes (18O), for instance http://smu.edu/Earth'sciences/people/faculty/tabor/Tabor%26Montanez2005.pdf , if you have worked your way through the isotopes in the water cycle textbook and the GNIP database for isotopes in precipitation, you'll find a plethora of variables that has to be accounted for. You just have to make a lot of suppositions, that might be wrong.
 
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  • #14
Andre said:
Maybe the quality of suppositions is even more important. You're looking at the end of the line of a lot of them, for instance the temperature supposition are based on stable oxygen isotopes (18O), for instance http://smu.edu/Earth'sciences/people/faculty/tabor/Tabor%26Montanez2005.pdf[/URL], if you have worked your way through the isotopes in the water cycle textbook and the [url=http://www-naweb.iaea.org/napc/ih/index.html]GNIP database[/url] for isotopes in precipitation, you'll find a plethora of variables that has to be accounted for. You just have to make a lot of suppositions, that might be wrong.[/QUOTE]

Maybe I should elaborate on those suppositions. Tabora & Montanez 2005 state:

[quote]The dD values of the phyllosilicates range from -69promil to -55promil. The d18O values range from 19.5mil to 22.7mil. If these samples preserve a record of equilibrium with paleo-meteoric waters, the isotopic compositions of the phyllosilicates correspond to paleotemperatures of phyllosilicate crystallization ranging from 22.3 °C to 35.3 °C.[/quote]

There is already one 'if'. Obviously during chemical processes there will be some isotopic fractination because of physical differences between heavy and light isotopes, these processes are temperature dependent, hence it's use as paleo thermometer. Unfortunately there are also many other (often unknown) factors to take into account. Let's just confine ourselfs to one of them "meteoric water", if I read that correctly it would suggest that they assume the original isotope ratio of the rain water in contact with the rocks would be consistent with water of those temperature.

However have a look at the isotope in precipitation chart of [url=http://www-naweb.iaea.org/napc/ih/IHS_resources_gnip.html]GNIP[/url]:

[ATTACH=full]154744[/ATTACH]

Although there is a clear temperature dependence for isotope in precipitation, there are also abberations. You can't see the cold winters in Argentine or the hot summers in China, based on the isotopes.

[URL]http://www.nature.com/ngeo/journal/v4/n4/full/ngeo1106.html[/URL]:

[ATTACH=full]154745[/ATTACH]

These isotopes would suggest that the temps of Greece and Belgium are about equal. The locals will tell you that this is not really the case, also when yellow here is the same yellow in the upper chart, then Shri Lanka would be as cold as The Netherlands. That would be hard to sell too.

The main reason for this abbaration is the [url=http://wwwrcamnl.wr.usgs.gov/isoig/isopubs/itchch2.html#2.3.4]Rayleigh process or Rayleigh fractionation[/url]. As condensation in clouds prefers heavy isotopes (deuterium and 18O) the cloud gets gradually depleted from heavy isotopes. The further the clouds move away from the source, the lighter the remaining isotopes are. This spoils the effectiviness of many isotope thermometers, if the rayleigh factor is unknown, which is obviously the case for the Permian past. So the isotope values of that meteoric water is not a very reliable isotope thermometer.
 

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  • #15
Andre said:
It appears that this Kiehl & Shields 2005 study is the result of a simulation model, which I guess would not have any higher status than a hypothesis.

The value of simulations can be tested against current climates. One takes a set variables that are believed to be correlated with various climate parameters and sees how well the simulation based on these variables predicts known climates. The problem arises in how well this set of variables can be measured or assessed in paleo-environments. One big set of assumptions regards solar output and axial tilt. For late Permian Pangaea, the assumption in the Kiehl paper was that these variables were essentially the same as today. Again, I'm saying it's the quality and relevance of the data or lack of data that determines the value of a simulation. A simulation that works well in the current environment does so because the variables and correlations are well known. But but a good simulation model will nevertheless pass or fail based on the quality and relevance of the data available for paleo-environments.
 
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  • #16
SW VandeCarr said:
The value of simulations can be tested against current climates. ...

Exactly, so let us see how the modelers are doing in a setting that is well known. This is a copy paste from what I wrote in a discussion elsewhere.

It's now common knowledge now that there was no ice sheet on Siberia during the last glacial maximum, a phenomonon that appears to contradict the current understanding of ice ages and interglacials. Hence such an anomaly begs for an explanation. Krinner et al 2006 assume that it had been very cold in Siberia, in accordance with the assumed glacial regime and they propose that the impact of wind blown dust deposition on snow has decreased the reflectivity of the ice and caused it to melt again, thus preventing the accumulation of an ice sheet, especially in the arid conditions. They model this event and sure enough, manage to simulate that. To validate their work they refer to Hubberten et al 2004 which abstract indeed suggest that this might be correct.

Evidently they did not study their whole reference, otherwise they would have noticed (page 1340) :

Most of the Late Weichselian (Sartanian), namely from about 24 to 15 ka BP, was characterizedby the lowest levels of xerophilic insects, virtual disappearance of steppe species, and dominance of Arctic tundra inhabitants (Fig. 6). That definitely indicates lower summer temperatures than in the Middle Weichselian, but still warmer temperatures than today are indicated by the occurrence of some thermophilic plant species (Kienast, 2002).

Reason enough for the ice to melt during the summer, no need for aeolian dust. On the contrary, the reconstructed biotope of North Siberia during the Last Glacial Maximum was a combination of an arid grassy steppe and tundra vegetations, supporting a mega fauna (Hubberten et al 2004, Kienast et al 2005, Mol et al 2004, 2006).

Refs:

Hubberten et (21) al 2004 The periglacial climate and environment in northern Eurasia during the Last Glaciation, Quaternary Science Reviews 23 (2004) 1333–1357

Kienast, F., Schirrmeister, L., Siegert, C., Tarasov, P., 2005. Palaeobotanical evidence
for warm summers in the East Siberian Arctic during the last cold stage.
Quaternary Research 63, 283e300.

Krinner G. et al 2006; Ice-free glacial northern Asia due to dust deposition on snow, Climate Dynamics (2006) 27:613–625 DOI 10.1007/s00382-006-0159-z 123

Mol, D., L et al, 2004 Brief history , 14C dates, individual age, gender and size of the Yukagir mammoth. Symposium: The Yukagir mammoth: outcome of the first stageof research work. Academy of Sciences of the Republicof Sahka .(Yakutsk) p. 51-55

Mol, D., et al, 2006. Results of theCERPOLEX/Mammuthus Expeditions on the Taimyr Peninsula, Arctic Siberia. Russian Federation Quaternary International,January volumes 142-143 pp. 186-202.
 

FAQ: What Caused the Lack of an Ice Sheet on Siberia During the Last Glacial Maximum?

1. What causes changes in Earth's temperature over time?

The Earth's temperature has fluctuated throughout its history due to a combination of natural factors, such as changes in the Earth's orbit and volcanic activity, and human activities, such as greenhouse gas emissions.

2. How do scientists measure temperature in Earth's history?

Scientists use a variety of methods to measure temperature in Earth's history, including ice core samples, tree ring data, and sediment analysis. These methods can provide insights into Earth's temperature dating back thousands or even millions of years.

3. What is the current state of Earth's temperature compared to the past?

Currently, the Earth's temperature is rising at an alarming rate due to human-caused climate change. The Earth's average temperature has increased about 1 degree Celsius since the Industrial Revolution, and if left unchecked, could have devastating consequences for our planet.

4. How does Earth's temperature affect the environment?

Changes in Earth's temperature can have a significant impact on the environment, including sea level rise, changes in weather patterns, and the extinction of certain species. It can also lead to more frequent and severe natural disasters, such as hurricanes and wildfires.

5. Can Earth's temperature change naturally without human influence?

Yes, Earth's temperature has fluctuated naturally over its history, but the current rate of warming is far beyond what would occur naturally. The overwhelming scientific consensus is that human activities, such as burning fossil fuels, are the primary cause of the current rapid rise in Earth's temperature.

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