Helium and Neon
Helium and Neon
复制标题
氦气和氖气
作者：
B. Brauner
Collie教授和Patterson先生最近向化学会通报的实验、J. J. Thomson爵士的讲座以及《自然》杂志上关于化学元素可能合成的讨论引起了英国以外的极大兴趣。据我所知，意见分歧很大。就我个人而言，也许可以允许我说，我一直认为氦族元素可能通过整合从其他气体中形成，就像其他元素通过分解形成氦族元素一样（参见Chemical News，1896和Berichte，1899）。当我提出这个观点时，有人提出反对意见，认为 4H 大于 He，4.032，而不是 3.99，今天也可能提出同样的反对意见，认为 He + O，或 3.9 + 16，小于 Ne，20.2（除非 Ne 是气体混合物）。
THE experiments communicated to the Chemical Society recently by Prof. Collie and Mr. Patterson, the lectures delivered by Sir J. J. Thomson, and the discussions which have taken place in NATURE, on the possible synthesis of the chemical elements have aroused great interest outside England. So far as I can ascertain, opinion is much divided. For my own part I may perhaps be permitted to say that I have always entertained the idea of a possible formation of elements of the helium group from other gases by integration, just as these are formed from other elements by disintegration (see Chemical News, 1896, and Berichte, 1899). When I put forward this view objection was taken that 4H is greater than He, 4.032 instead of 3.99, and the same kind of objection may be raised to-day that He + O, or 3.9 + 16, is less than Ne, 20.2 (unless Ne is a mixture of gases).