Authors: Jeffrey Joseph Wolynski
Ammonia is found in late stage stars such as Neptune and Uranus. It is also present in intermediate aged stars such as Jupiter and Saturn. Given the sheer amount of hydrogen and nitrogen available to chemically combine into ammonia, it is clear that production of ammonia is a natural process in stellar evolution/metamorphosis, and we can mimic this with the Haber Process. A naturally occurring Haber process runs counter to the establishment's false worldview that stars can not cool down enough to form huge amounts of organic and non-organic molecules. We know it happens because we have direct and indirect observational evidence of it happening.
Comments: 3 Pages. 2 diagrams
[v1] 2018-07-22 10:10:29
Unique-IP document downloads: 205 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.