Origin and Evolution of Hydrogen Isotope in Solar System

Introduction

The solar system is amazing. From the eyes of the astronauts and the spectators, the universe is so vast that it managed the classical dance of the meteors being choreographed by the other celestial bodies. One of the most popular systems in the universe is the Solar System which managed to support the planets. From the previous scientists and astrologers, the life of the solar system came from various hypotheses which most are being supported by the discoveries of the isotopes. The purpose of the study is to give the details regarding the origin and the evolution of one of the isotopes that have been proved present in the solar system, the hydrogen isotope.

Background of the Study and Significance

The abundance of the isotopes in the solar system has been discovered to be the important elements. Moreover, the isotopes such as hydrogen and helium are incorporated in the nature of the sun processes. Many scientists/astrologers believed that the solar system has many other secrets and is yet to discover. Solar system is formed from a homogenous nebula with other elements producing into excess (Nolte and Lietz, 2000). The importance of the learning the origin and evolution of the hydrogen isotopes is high valued in the astrological profession, most especially in knowing the extent of the production of the hydrogen in the solar system which might trigger to the global warming. Through observing the chemical reactions and the irregularities of the isotopic elements, there are several crunches that might appear in determining the life in the solar system.

Literature Review

In the solar system, the experts suggested that the values or ratios of the isotopic elements are different from each other. Also in the nebular model that forms the solar system, there are significant productions of hydrogen isotopes that are burned in the sun. Accordingly, the hydrogen and the helium gases are formed in the solar wind through the continuous burning, and it is easier to burn when the elements are in lighter mass. Large isotopic hydrogen elements are expected to have the chemical and physical reactions on the other elements (Nolte and Lietz, 2000). Solar system, as we all know, is composed of countless stars and other celestial bodies and the system in which the eight planets are orbiting around the sun, the biggest star. Other than that, there is bulk composition of gases and elements namely hydrogen and noble gases that make up the vast majority of the solar material. The isotope compositions are professed to be the controversial interpretation of the supernova or be the supernova material. The corresponding supernova like isotope composition may have formed through the process of mixing and unmixing of the isotopes. The model of the photochemical dissociation of the hydrogen and the other elements are close to the reaction they receive from the sun (Russell, 2007). The continuous process of the hydrogen in the solar system can be the original case of the climate or global warming. Between the processes of the photochemical dissociation, the polarization arises. Aside from the past variations in the carbon cycle and the human intervention, and the uncertainties inherited in the climatic change, there is a significant hunch that the sudden climate change is from the burning reaction of too much hydrogen isotopes and deposited in the solar winds (Veizer, 2002).

Research Problems

The study understands the difficulty in analyzing the various phases that might trace the origin and evolution of the hydrogen isotope in the solar system. Therefore, there are several questions that can help the study in organizing the information.

1. What are the factors that might affect the evolution of the hydrogen isotopes?

2. What are the consequences of the excessive hydrogen isotopes in the solar system?

3. Is there are available clues regarding the origin of the hydrogen isotopes?

Methodology

The applied method in the study is the use of the secondary information which is all related to the solar system and other astrological elements. Through the use of the secondary information, the study can identify or link the relevant data pertaining to the origin and evolution of the hydrogen isotopes in the solar system. In addition, the secondary information is a great advantage for the study for it may deliver the differences or effects of the other isotopes that are all present in the solar system.

References:

Nolte, A., & Lietz, C., 2000. Abundances of Hydrogen and Helium Isotopes in Jupiter [Online] Available at: http://www.omatumr.com/abstracts/nolte_lietz.pdf [Accessed 29 March 2010].

Russell, S.S., 2007. The Formation of the Solar System, Journal of the Geological Society, Vol. 164.

Veizer, J., 2002. Global Warming: Armageddon or Bust? Some Scientists See the Possibility of Global Warming as the Precursor to a Global Armageddon, to Others It Is Merely Hype; the Truth Lies Somewhere in Between, Forum for Applied Research and Public Policy, Vol. 16, No. 4.