Helium-3

to get hired for this trip. Though some of them may seem strict or even a little harsh, it is all for the well being of the entire mission and crew. If we did not have these requirements than we would not be able to survive this two year hunt for helium 3. There are five key characteristics that an astronaut needs in order to be successful on our mission. The first characteristic is resiliency. A resilient person has a what you may call a“Can Do” attitude, because this person is always persevering

fuel. Envision a society that can harness the same process that powers the sun. Skeptics may say that this is impossible. In fact, an alternate source of energy exists, and so does the process to create it. Nuclear fusion, a process in which the Helium 3 isotope is utilized is the rapture in which the U.S.A., and the world, could produce a great amount of energy as an alternative to petroleum. Whether nuclear fusion produces a substantial amount of energy for the U.S. may not matter. All good

Proposal for a Homemade Fusion Reactor Table of Contents Introduction Dangers Project Overview - Parts (a page for each part) Part List Cost Research Competitions Future Uses To Add Cost List Electrical System Design Calculations for Radiation List of safety procedures Introduction Nuclear fusion is a form of nuclear reaction which occurs when two or more atomic nuclei collide at a very high speed and as a result, join to form a new type of atomic nucleus. During this process

Helium is the first noble gas on the Periodic Table. The symbol of Helium is “He”, and the Atomic number is 2. This element has a atomic mass of 4.00g. Helium was first discovered on the sun as a cooler gas by Sir William Ramsay. The noble gas helium was given it’s name referring to the Greek goddess “Helios”,on August 18, 1868. Helium is the second top element on planet Earth. Also, it is the gas that scientist found that was leaking from Mt. Vesuvius in Italy. The Gas that can give a weird reaction

on the mass of the star, they can reach different types of fusion. Normal stars that have a mass of up to 4 times the sun can only have hydrogen fusion, helium fusion, and carbon fission. Stars with a bigger mass is classified as a massive star, and they undergo multiple stages. They start out similar to the normal stars with hydrogen fusion, helium fusion and carbon fission, but continue over to oxygen fusion, and silicon fusion. The end product of Silicon is Iron. No star can fuse Iron, it will die

Helium (Greek helios,"sun"), symbol He, inert, colorless, odorless gas element. In group 18 of the periodic table, helium is one of the noble gases. The atomic number of helium is 2. Pierre Janssen discovered helium in the spectrum of the corona of the sun during an eclipse in 1868. Shortly after it was identified as an element and named by the chemist Sir Edward Frankland and the British astronomer Sir Joseph Norman Lockyer. The gas was first isolated from terrestrial sources in 1895

Palacios 1 Kimberly Palacios English 1A-60 Professor Kathleen Gurnett 29 October 2015 Just Like Humans If a person was to be asked to describe our life stages, they would probably say something like “people are born, they live, and then they die.” Of course, they aren’t wrong, but we humans go through beautiful stages before reaching death. We go through stages such as infancy, childhood, adolescence, and adulthood. In many ways, Stars are just like humans. They also go through astonishing

No matter when we consider the beginning of time, there will always be the question of origin. "And before then- what?" The origin of the universe remains a mystery, but extrapolation from current working models can be used to speculate about the universe 's early development. The leading theory on the early development of the universe is the Big Bang theory, which puts forth the idea that the universe expanded from a singularity, or a single point.[1] The Big Bang laid the seeds that lead to the

paper discusses liquid helium, its discovery, properties applications and limitations. INTRODUCTION The discovery of what are known as “superfluids” was made relatively simultaneously in 1937 by two independent factions on opposite sides of the world. One was Pyotr Kapitsa in Moscow, and the other was John F. Allen and Donald Misener

Task 1.2- Properties (Part of P1) Describe the properties of . . . and. Radiation. Things should be including: • Their range in air • What they are stopped by • Their penetrating and ionising powers • How they are affected by electrical and magnetic fields. • How they are commonly detected. • Any other properties. Alpha, beta and gamma come from nuclear of an atom and they called radioactive, because it gives off radiation. These radiations absorb by different thickness of materials such as: Alpha