论文标题
关于维纳斯水上海洋可能的进化史
On the Possible Evolutionary History of the Water Ocean on Venus
论文作者
论文摘要
我们已经研究了金星上水海的可能进化史，采用了一维辐射感染模型，包括参数为反照率和相对湿度。在此模型下，宜居区可能包括金星。它可以继续以$ \ sim 1 $ 1 $ gy的增加，在淡淡的年轻太阳通量中增加，带有反照率= 0.3，相对湿度（rh = 1）和$ p_ {n0} = 10^5 $ pa的适度参数。如果我们考虑三维计算的放宽参数，那么海洋可能存在的时间可能超过$ \ sim $ 4.6 Gy。在这种情况下，我们必须考虑造成失控的原因，而不仅仅是太阳发光度的增加。重要的是要研究地球未来的未来和对其历史可居住区域的外部活动的观察，这一点很重要。
We have investigated the possible evolutional history of the water ocean on Venus, adopting the one dimensional radiative-convective model,including the parameters as albedo and relative humidity. Under this model, it has the possibility that the habitable zone could include Venus. It could continue for $\sim 1$ Gy in faint young solar flux increasing, with modest parameters such as albedo = 0.3, relative humidity (RH=1), and $p_{n0}=10^5 $Pa. If we relax parameters considering the 3-Dimensional calculations, the ocean could exist there longer than $\sim$ 4.6 Gy. In such cases, we have to consider the cause of runaway other than just solar luminosity increasing. It is important to investigate Venus history for the coming future of Earth and observations of exoplanets for their historical habitable zones.
