Venus Atmosphere Temperature and Pressure ProfilesShade Tree Physics
Installed 04 Feb 2001 - Latest update 10 Nov 2013.
A reviewer of the article (Influenza 1918, A Venus Connection?) stated that influenza viruses are designed to grow at 37 degrees C (Celsius) [98.6 degrees F (Fahrenheit)] and to replicate using mammalian cell enzymes and that a long period of host and pathogen co-evolution is required.
The following graphs are provided as a first step in checking up on whether or not a suitable temperature, pressure, and chemically friendly environment for the production or replication of viruses exists in the Venusian atmosphere.
These first two graphs (before my additions and extensions), were originally published by J.M. Jenkins, P. G. Steffes, D.P. Hinson, J.D. Twicken, and G.L. Tyler in their article, Radio Occultation Studies of the Venus Atmosphere with the Magellan Spacecraft, Icarus, Vol. 110, 79-94, 1994. (The kind permission to use the graphs does not constitute endorsement of the hypothesis under evaluation in this article.) See: Other Temperature and Pressure Profiles. [Thanks to the visitors from Gprs Pune, Maharashtra, India and Skylogic Germany Gmbh for finding that this link needed updating. 7 Jun 2013]
The stated 37 degrees C (which is the average human body temperature prior to viral attack) corresponds to 310 Kelvin (K) (Celsius temp plus 273). If we enter the Venus altitude-versus-temperature graph at 310 K and go straight up (red line) to the temperature profile, and then horizontally to the left axis we find a corresponding altitude of 52.5 kilometers (33 miles).
Now, as a rough cross-check, we enter the Venus altitude-versus-atmospheric
pressure graph at 1000 millibars (the Earth's
average sea level atmospheric
pressure) and go up to intersect the altitude-pressure profile line, and
across to the left axis where we find the corresponding altitude of
49.5 kilometers (31 miles). This altitude is only three kilometers
(or six percent) different than we found from the temperature graph.
So, in spite of the surface temperature of Venus being on the order of 864 degrees Fahrenheit, there is a region in the Venusian atmosphere which approximates that of Earth with respect to temperature and pressure. But there may be problems.
52.5 kilometers above the Venusian surface turns out to be in the middle of the Venusian cloud blanket which is made up largely of sulfuric acid droplets. (The cloud bottoms are estimated to be 30 to 35 km above the surface and the tops are estimated to be from 60 to 75 km above the Venusian surface.) This upper altitude limit is perhaps a fuzzy estimate. The cloud tops temperature has been reported to be 260 K (-13 degrees C or 9 degrees F). According to the temperature profile above (green line) this temperature corresponds to an altitude of 58 km (36 miles) for the cloud tops. (For stratus clouds there will be thermal equilibrium between the atmosphere and the cloud tops.)
Is this acidic cloud environment good or bad for the formation of viral precursors and/or virus building processes? (a) Do sulfuric acid (H2SO4) droplets in a reducing atmosphere assist or preclude the formation or preservation of amino acids and other RNA building blocks? (b) Can sufficient solar ultraviolet energy penetrate the clouds to this depth? If either answer is harmful to the hypothesis then we can ask whether or not the Venusian atmosphere above the clouds, say 60 km (37 miles) and up, could be (or not be) a candidate region for the biological processes in question. The lack of sufficient ultraviolet penetration will not be a problem above the clouds. So, what are the lowest temperature and pressure constraints for reasonable biological activity?
Here is a chart showing temperature versus pressure for the Venusian atmosphere. It is derived from the two graphs above.
[Installed on 16 Aug 2011.]
The Digital Dutch 1976 Standard
Atmosphere Calculator was used in plotting Earth's standard atmosphere curve.
What about the surface of Venus?