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For thousands of years, very little was known about Venus. It appeared on the sky in the morning and in the evening. The way it, like Mercury, swiftly moved against the background of static stars suggested it was a planet. And, it's brightness, third after the Sun and the Moon, meant that it was bound to be of decent size, and rather close to us. The first person to look at Venus through a telescope was Galileo, in 1609. All he could see, however, was a featureless disk. As optical telescopes got bigger and more widespread, that was all anybody could see. No surface, no details. Venus, it seemed, was completely enveloved in an opaque layer of thick clouds. For a few centuries more, this was all we had. How thick are those clouds? What do they consist of? What lies beneath them? Nobody knew. In general though, ideas and suggestions were benign in nature. Since Venus is so close to us and of almost of the same size and mass as Earth, we nurtured the idea of Venus being a kind of sister planet. A balmy, summery Earth, where things were a little warmer and a little greener due to it being closer to the Sun. With the arrival of spectroscopic analysis, though, it became possible for us to, without going there, measuring the properties of the Venusian atmosphere. This was done in the 1920's, and the result showed carbon dioxide. Lots and lots of it, without as much as a hint of any water vapour. As it turned out, we would have to wait for an answer until the 1960's, when Russia launched its Venera program. The first probe aimed to touch down onto the surface of venus, Venera 3, was designed for an atmosphere somewhat like our own, and was subsequently crushed like a tin can before returning any data. Venera 4, 5 and 6 came in various states of reinforcement, but none of them lasted even an hour. They did get a chance to sample the Venusian atmosphere however. It was, as predicted, full of carbon dioxide, while the clouds themselves turned out to be, not water, but yellow-stained masses of concentrated sulphuric acid. It turned out that temperatures on the surface of Venus were as high as 740K (~470°C), hotter than any household oven, and hot enough to melt lead. The pressure of the Venusian atmosphere is 90 times that on Earth (about the same as the pressure at a depth of thousand metres in an Earth ocean). The air is so thick that to an observer on the surface of Venus, the ground, although solid and rocky, would seem to ripple, and distort. If unprotected, the very same observer would be boiled in the heat, fried by the acidic air, and crushed by the pressure in less than a second. Of all the known places in the solar system, this beautiful evening and morning star is the one that most closely resembles our idea of hell. So what happened to Venus? It's twice as far from the Sun as Mercury, but hotter still. It is due to a phenomenon very well known on Earth today: the greenhouse effect. The Venusian atmosphere, full of carbon dioxide, lets in the visible light from the Sun, but will not let the infrared heat-radiation generated by the surface escape. So the temperature keeps climbing, until what little infrared radiation that manages to get out just balances the sunlight absorbed by the surface. |