Density of Venus' atmosphere - historical

In summary: This suggests the atmospheric pressure at the surface was much higher than the estimated 30 atmospheres.
  • #1
PhilDSP
643
15
Hello!

I'd like to know when the high density of the atmosphere of Venus was first determined or suspected. Was it with the Russian probes that the first evidence came that the atmosphere was much more dense than the Earth's? Or had there been other indications earlier in time that such was the case?
 
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  • #3
I've been unable to find any published reference that anyone had suspected that the atmosphere of Venus differed substantially from the Earth's in density prior to 1967.

The Russian Venera 4 probe was the first to survive (partially) the entry into the atmosphere and take density measurements. It measured a density of about 22 Earth atmospheres but had a hull strength of only 25 atmospheres and was later found to be faulty. All of the early Venera probes that entered the atmosphere were eventually crushed by the atmospheric pressure.

http://en.wikipedia.org/wiki/Venera

Shortly afterward in 1967, data from the American Mariner 5 gave a calculation of 75 to 100 Earth atmospheres, far higher than had been expected.However, here is a very interesting and relevant site:

http://www.mentallandscape.com/V_Lavochkin1.htm

In 1967, most astrophysicists in America and Russia believed that Venus was extremely hot, but one MIT paper that year suggested the planet could be experiencing an Ice Age! Surface pressure on Venus was even more of a scientific guessing game at that time, with published estimates ranging from 3 to 1000 atmospheres. This uncertainty resulted from the inaccuracy of spectrographic methods, which measured conditions at the cloud tops, and from uncertainty about the depth of the atmosphere and the radius of the planet's hard surface. Estimates of 10 to 30 atmospheres of pressure at the surface were commonly believed.

That's a bit perplexing as the author earlier states that the barometer aboard Venera 4 had a range of 0.13-6.9 ± 0.2 atmospheres.
 
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1. What is the density of Venus' atmosphere?

The density of Venus' atmosphere is about 67 times greater than Earth's atmosphere. It has a density of 67 kg/m^3, compared to Earth's 1.2 kg/m^3.

2. How was the density of Venus' atmosphere historically measured?

The density of Venus' atmosphere was historically measured using a technique called radio occultation. This involved measuring the slight changes in radio waves as they passed through the atmosphere of Venus.

3. Has the density of Venus' atmosphere changed over time?

Yes, the density of Venus' atmosphere has changed over time. It has been decreasing due to the loss of gases such as hydrogen and helium. This loss is believed to be caused by the solar wind and the lack of a strong magnetic field on Venus.

4. How does the density of Venus' atmosphere compare to other planets?

The density of Venus' atmosphere is much higher than that of other planets in our solar system. It is second only to the planet Saturn, which has a density of 700 kg/m^3. This is due to Venus' thick atmosphere composed mainly of carbon dioxide.

5. Why is the density of Venus' atmosphere important to study?

The density of Venus' atmosphere is important to study because it can provide insight into the planet's evolution and its potential habitability. It also helps scientists understand the dynamics of planetary atmospheres and how they can change over time. Additionally, studying the density of Venus' atmosphere can aid in the development of future missions to the planet.

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