Investigating Venus Runaway Greenhouse Effect: Limestone Burning Temperature

  • Thread starter Andre
  • Start date
  • Tags
    Venus
In summary, the runaway greenhouse effect on Venus is caused by high atmospheric CO2 pressure. The lower temperature limit for this reaction is around 1,200 degrees Fahrenheit (900 degrees Celsius). The process of liberating carbon dioxide from limestone can happen at room temperature, although it is more likely to happen at higher temperatures.
  • #1
Andre
4,311
74
Working on my point paper of the https://www.physicsforums.com/showthread.php?t=2974 and I need to address the runaway greenhouse effect ideas. Now we have this:

http://www.vt-2004.org/Background/Infol2/EIS-D7.html

Another runaway effect occurs when high temperature chemical reactions begin to drive carbon dioxide from the rocks into the atmosphere

I thought this would occur not below 900-1100 degrees celsius as in http://www.brocross.com/iwps/pages/lime.htm :

Limestone is a sedimentary rock composed principally of calcium carbonate and it can be calcined by heating it in a kiln. The heating process chemically converts the stone to burnt lime (quicklime, calcium oxide, CaO). To do this the stone must be heated to a temperature of between 900° and 1100°C. This causes the limestone to dissociate yielding burnt lime and carbon dioxide gas.

So my questions are:

What would be the lower temperature limit for " at high temperature chemical reactions begin to drive carbon dioxide from the rocks into the atmosphere"

What would be the effect of high atmospheric CO2 pressure on that temperature?

Any experts on lime burning?
 
Last edited by a moderator:
Chemistry news on Phys.org
  • #2
completely off topic. but have found out why venus though being smaller than Earth has a denser atmosphere than our planet.co2 ,the chief constituent of venetian atmosphere is has greater molecular mass than either o2 or n2 . hence gravity of venus can support a more thicker atmosphere than Earth where the lighter gases are dominant.however not sure how one can explain such a large amount of CO2 in the first place.
 
  • #3
Hi Sage, Yes we have been there.

Assuming that the abundance of elements of both Earth and Venus are comparable, within the same order of magnitude, Earth and Venus should have comparable amounts of carbon in the lithosphere.

The back side of my envellope says that Venus has about the same amount of carbon in the atmosphere as the Earth has in the crust, forming variations of limestone type rox.

The greenhouse hypothesis for Venus (Kasting, Pollack, Ackerman. Icarus. 1984;57:335-55.) assumes that Venus had an Earthlike appareance in the early days including oceans and weathering processes that bonded CO2 to limestone. How get all the limestone of Earth in the atmosphere?

quoting again:
Another runaway effect occurs when high temperature chemical reactions begin to drive carbon dioxide from the rocks into the atmosphere

seems highly inadequate if we need all the CO2 to get out the crust and we need 900-1200 degrees celcius to begin with:

The material needs to reach a temperature of 2,200 degrees Fahrenheit (1,200 degrees Celsius). At 1,650 degrees Fahrenheit (900 degrees Celsius), carbon dioxide (CO2) is driven off, and 2,200 degrees Fahrenheit (1,200 degrees Celsius) is required for the heat to penetrate through to the center of the stone.

http://oikos.com/library/naturalbuilding/lime.html

So I was looking for a chemical specialist who could confirm if the processes are possible under lower temperatures.
 
  • #4
You don't necessarily need high temperatures for limestone to give off CO2 - acid rain will also do the trick, through the reaction CaCO3 + 2H+ -> Ca++ +H2O +CO2. This will take place at room temperature, and is the reason why all the old limestone statues and monuments are being ruined. So if Venus in the early days had an acid rain problem (and it certainally does now!), this could have liberated considerable amounts of CO2.
 
  • #5
some new developments.the key point it seems is the presence of liquid water.venus in its early days was too hot(unlike earth)to hold liquid water. so all its water (comparable to the entire volume of water present in Earth's oceans today) was in the form of steam in the atmosphere. now absence of a strong venetian magnetic field meant that deadly solar radiations could easily prey on venus's atmosphere breaking down water vapour into hydrogen and oxygen. hydrogen , of course escaped while oxygen quickly combined with carbon containing compounds in venetian crust and venetian atmosphere to produce C02. this process continued relentlessly until todays venetian atmosphere with nearly 90% CO2 was formed.also consider that since early venus had so much water vapour in its atmosphere, the greenhouse effect would be extreme. venus was in the past far hotter than it is today.
 
  • #6
What would be the lower temperature limit for " at high temperature chemical reactions begin to drive carbon dioxide from the rocks into the atmosphere"


If you're asking for the specific lower limit temperature for the reaction to occur appreciably, you can find a resonable estimate simply by using the free energy-Gibbs-equation. You'll need to find the specific reaction and perhaps a bit of research at your local university science library.
 
  • #7
Thanks for the tips.

Sage, back later, but my back of the envellope gestimation using Stefan Bolzmann law with Temperature in Kelvin proportional to the 1/4 power to the insolation flux and Venus at about 0.7 AU's (so double flux) I would roughly guestimate the black blody temperature of Venus at some 300K (Earth 255K). That's the ideal temperature of a summer afternoon here. No problem with liquid water.
 

What is the Venus runaway greenhouse effect?

The Venus runaway greenhouse effect is a phenomenon where the planet's atmosphere traps heat from the sun, causing the surface temperature to rise to extreme levels. This is due to the high levels of carbon dioxide in the atmosphere, which absorbs and retains heat.

Why is it important to investigate the Venus runaway greenhouse effect?

Studying the Venus runaway greenhouse effect can provide insights into the potential effects of climate change on Earth. It can also help us better understand the conditions that can lead to a planet becoming inhospitable to life.

What role does limestone burning temperature play in the Venus runaway greenhouse effect?

Limestone burning temperature is an important factor in the Venus runaway greenhouse effect because it affects the amount of carbon dioxide that is released into the atmosphere. Higher burning temperatures result in more carbon dioxide being released, which can contribute to the greenhouse effect.

How is the limestone burning temperature on Venus different from Earth?

The limestone burning temperature on Venus is significantly higher than on Earth, due to the planet's extreme surface temperatures and atmospheric pressure. This results in a greater amount of carbon dioxide being released into the atmosphere, further contributing to the runaway greenhouse effect.

What are the potential solutions to the Venus runaway greenhouse effect?

Some proposed solutions to the Venus runaway greenhouse effect include reducing the amount of carbon dioxide in the atmosphere through carbon capture and storage, or introducing reflective particles into the atmosphere to reflect sunlight and cool the planet. However, these solutions are currently theoretical and would require further research and development.

Similar threads

  • Sci-Fi Writing and World Building
Replies
21
Views
993
  • Earth Sciences
6
Replies
186
Views
74K
  • Astronomy and Astrophysics
Replies
6
Views
5K
Replies
17
Views
3K
Replies
59
Views
9K
Replies
4
Views
3K
Replies
12
Views
4K
Replies
9
Views
27K
  • Earth Sciences
Replies
3
Views
3K
Back
Top