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Hypothetical signs of life on Venus: revising results of 1975-1982 TV experiments

机译：假设的生命迹象在金星上：修改1975-1982电视实验结果

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Extraterrestrial life may presumably be discovered not in worlds separated from Earth by tens of parsecs but on the surface of Earth's nearest planet neighbor in the Solar System, Venus. This conclusion follows from the newly processed archive data of the TV experiment that was performed in 1975 and 1982 on Venus's surface by the VENERA Soviet spacecraft missions. One of the main experiments, pioneering in situ TV scanning of the planet surface, has never been repeated by any other space mission. The unique archive data have been reprocessed using state-of-the-art technologies that enabled image details to be substantially improved. The new analysis of the VENERA television images has identified up to 18 hypothetical living objects that feature a complex regular structure and presumably are capable of very slow motion. The objects, whose dimensions are significant, may be indicative of the existence of life on a planet whose physical environment is crucially different from Earth's. Water, which is terrestrial life's basis, cannot exist in the liquid phase at temperatures of about 460 degrees C characteristic of the spacecraft landing sites. Water content in the gaseous state is also negligible (about 2 x 10(-5)). Both water and oxygen are virtually absent in Venus's atmosphere. Therefore, the question is: what matter may life on the planet be built on? We consider chemical compounds stable at high temperatures that may be a base for hypothetical Venusian life. We conclude that to explore Venus's hypothetical life, a new dedicated mission, much more advanced than the VENERA missions, should be sent to the planet.
机译：可能会在世界上没有被发现的外星生命，但在地球上分开的世界，而是在太阳系的地球最近的行星邻居的表面上，维纳斯。这一结论是从1975年和1982年在Venus苏联航天器任务的1975年和1982年进行的电视实验的新加工档案数据。地球表面的原位电视扫描的主要实验之一从未被任何其他空间任务重复过。唯一的存档数据已使用最先进的技术进行重新处理，使能够显着提高图像细节。 Venera电视图像的新分析已经识别出最多18个假设的活物对象，其具有复杂的常规结构，并且可能是能够非常慢的运动。尺寸是显着的物体，其尺寸可以指示在物理环境与地球中均关键不同的行星上的生命存在。作为陆地生活的水，在液相中不能存在于航天器着陆位点约460摄氏度的温度下的液相中。气态的水含量也可忽略不计（约2×10（-5））。在金星的气氛中几乎不存在水和氧气。因此，问题是：在这个星球上可能会建立什么问题？我们认为化合物在高温下稳定，这可能是假设的Venusian寿命的基础。我们得出结论，为了探索金星的假设生命，一个新的专用使命，比Venera任务更先进，应该被送到地球。

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