World Institute for Scientific Exploration (WISE)
Question
Asked 22 August 2014
Looking for an advise on nebulae (molecular clouds, globules, protoplanetary disks)?
Our group of geochemists, geologists and chemists is looking for a astrophysicists or astronomer who will be interested to participate in our research. We discovered the correlation between ionization potential of elements and their abundance in planets and other bodies. This correlation could be explained by a simple termochemical equation. Predictions by this equation correlate impressively well with observed chemical composition of surface of planets. We propose a theoretical process which could explain observed facts. Details of our work are described in this document http://arxiv.org/abs/1208.2909
We are looking for a person who could help us (in collaboration way) to improve and connect our theoretical model with observations of nebulae.
All Answers (2)
Natural Hydrogen Energy LLC
It is correct. In our work we tested it on new data from space probes then interpreted the observed correlation as a Boltzmann distribution depending on the distance from the Sun. We tested our model on factual data for Moon, Mars, Venus and Meteorites. We find that predictions force of the model is excellent. Then, we made surface-to-volume analysis for elements. We find periodical trends, related with affinity of elements to hydrogen and with their mass. This suggests that radial differentiation of elements inside the planet was chemically- and gravity-driven. We have far more interesting results, which are out of scope of this paper.
Similar questions and discussions
If you are a specialist in protoplanetary disks, would you like to collaborate with us?
Our group believes it has discovered an important correlation between the ionization potential of elements and their abundance in planets and other Solar System objects. This correlation can be explained with a simple thermochemical equation and the predictions made with this equation correlate impressively well with the observed surface chemical compositions of planets.
Details of our work are described in the following document: https://arxiv.org/abs/1208.2909v2
Since the time of this preprint, our model has been experimentally tested by an independent team of researchers using geoneutrino measurements and the Earth’s heat flux. Their conclusions are at favor of our model. Also, it has been shown that our anoxic Earth model matches geophysical PREM data very well.
Now we are looking for an astrophysicist or astronomer with a good understanding of protoplanetary disks to collaborate with our group of geochemists, geologists and chemists to improve our theoretical model with observations of protoplanetary disks.
UPD Oct 12: we are still interested, please contact us.
Related Publications
Examination of ˜2000 sun--like stars has revealed 97 planets (as
of 2002 Nov), all residing within our Milky Way Galaxy and within
˜200 light years of our Solar System. They have masses between
0.1 and 10 times that of Jupiter, and orbital sizes of 0.05--5 AU. Thus
planets occupy the entire detectable domain of mass and orbits. News
&summaries abou...
We calculate the probability of injection of SRs by a nearby SN into a young protoplanetary disk to be of a few per mil. We simulate the formation of molecular clouds via turbulent converging flows to estimate the expected abundance of 60Fe in the early solar system.