✪ Will They Really “Cancel” You?! 🙅‍♂️ ✪

Here are the plain facts and nothing but the facts. [Easy Way To Trade header]( Dear Subscriber, You've probably heard about angry online mobs calling for people to be "cancelled" … Socially blacklisted … Even fired from their jobs. All because they don't conform to a particular ideology … Or because they disagree with this or that government decision — from the left, the right, or in-between. This public shaming (and worse!) is an unfortunate dark side of the Internet … And an especially unfortunate symptom of the new hyperpolitical world we live in today. But if you think that's concerning … Suppose you discovered an obscure official plan that will give the U.S. Federal Reserve the power to do some "canceling" of its own … Closely monitor — and even control — their checking accounts … Closely monitor — and even control — nearly all their financial transactions. Imagine a scenario in which … You're checking account is restricted or even frozen … You're unable to buy or sell anything from your bank account or credit card … You're unable to pay your mortgage or fill up your gas tank. I know it sounds like a chapter from a dystopian novel. But it could soon be a reality. [Click here]( for the facts and nothing but the facts. Good luck and God bless! [Signature] Martin D. Weiss, PhD Founder of Weiss Ratings Helium (from Greek: ἥλιος, romanized: helios, lit. 'sun') is a chemical element with the symbol He and atomic number 2. It is a colorless, odorless, tasteless, non-toxic, inert, monatomic gas and the first in the noble gas group in the periodic table.[a] Its boiling point is the lowest among all the elements, and it does not have a melting point at standard pressure. It is the second lightest and second most abundant element in the observable universe, after hydrogen. It is present at about 24% of the total elemental mass, which is more than 12 times the mass of all the heavier elements combined. Its abundance is similar to this in both the Sun and in Jupiter, due to the very high nuclear binding energy (per nucleon) of helium-4, with respect to the next three elements after helium. This helium-4 binding energy also accounts for why it is a product of both nuclear fusion and radioactive decay. The most common isotope of helium in the universe is helium-4, the vast majority of which was formed during the Big Bang. Large amounts of new helium are created by nuclear fusion of hydrogen in stars. Helium was first detected as an unknown, yellow spectral line signature in sunlight during a solar eclipse in 1868 by Georges Rayet,[12] Captain C. T. Haig,[13] Norman R. Pogson,[14] and Lieutenant John Herschel,[15] and was subsequently confirmed by French astronomer Jules Janssen.[16] Janssen is often jointly credited with detecting the element, along with Norman Lockyer. Janssen recorded the helium spectral line during the solar eclipse of 1868, while Lockyer observed it from Britain. Lockyer was the first to propose that the line was due to a new element, which he named after the sun. The formal discovery of the element was made in 1895 by chemists Sir William Ramsay, Per Teodor Cleve, and Nils Abraham Langlet, who found helium emanating from the uranium ore, cleveite, which is now not regarded as a separate mineral species, but as a variety of uraninite.[17][18] In 1903, large reserves of helium were found in natural gas fields in parts of the United States, by far the largest supplier of the gas today. Liquid helium is used in cryogenics (its largest single use, consuming about a quarter of production), and in the cooling of superconducting magnets, with its main commercial application in MRI scanners. Helium's other industrial uses—as a pressurizing and purge gas, as a protective atmosphere for arc welding, and in processes such as growing crystal to make silicon wafers—account for half of the gas produced. A small but well-known use is as a lifting gas in balloons and airships.[19] As with any gas whose density differs from that of air, inhaling a small volume of helium temporarily changes the timbre and quality of the human voice. In scientific research, the behavior of the two fluid phases of helium-4 (helium I and helium II) is important to researchers studying quantum mechanics (in particular the property of superfluidity) and to those looking at the phenomena, such as superconductivity, produced in matter near absolute zero. On Earth, it is relatively rare—5.2 ppm by volume in the atmosphere. Most terrestrial helium present today is created by the natural radioactive decay of heavy radioactive elements (thorium and uranium, although there are other examples), as the alpha particles emitted by such decays consist of helium-4 nuclei. This radiogenic helium is trapped with natural gas in concentrations as great as 7% by volume, from which it is extracted commercially by a low-temperature separation process called fractional distillation. Terrestrial helium is a non-renewable resource because once released into the atmosphere, it promptly escapes into space. Its supply is thought to be rapidly diminishing.[20][21] However, some studies suggest that helium produced deep in the earth by radioactive decay can collect in natural gas reserves in larger than expected quantities,[22] in some cases, having been released by volcanic activity.[2 [-------------------] Sometimes, colleagues of Easy Way To Trade share special offers with us that we think our readers should be made aware of. Below is one such special opportunity that we believe deserves your attention. The first evidence of helium was observed on August 18, 1868, as a bright yellow line with a wavelength of 587.49 nanometers in the spectrum of the chromosphere of the Sun. The line was detected by French astronomer Jules Janssen during a total solar eclipse in Guntur, India.[24][25] This line was initially assumed to be sodium. On October 20 of the same year, English astronomer, Norman Lockyer, observed a yellow line in the solar spectrum, which, he named the D3 because it was near the known D1 and D2 Fraunhofer line lines of sodium.[26][27] He concluded that it was caused by an element in the Sun unknown on Earth. Lockyer and English chemist Edward Frankland named the element with the Greek word for the Sun, ἥλιος (helios).[28][29] In 1881, Italian physicist Luigi Palmieri detected helium on Earth for the first time through its D3 spectral line, when he analyzed a material that had been sublimated during a recent eruption of Mount Vesuvius.[30] Sir William Ramsay, the discoverer of terrestrial helium The cleveite sample from which Ramsay first purified helium[31] On March 26, 1895, Scottish chemist Sir William Ramsay isolated helium on Earth by treating the mineral cleveite (a variety of uraninite with at least 10% rare-earth elements) with mineral acids. Ramsay was looking for argon but, after separating nitrogen and oxygen from the gas, liberated by sulfuric acid, he noticed a bright yellow line that matched the D3 line observed in the spectrum of the Sun.[27][32][33][34] These samples were identified as helium by Lockyer and British physicist William Crookes.[35][36] It was independently isolated from cleveite, in the same year, by chemists, Per Teodor Cleve and Abraham Langlet, in Uppsala, Sweden, who collected enough of the gas to accurately determine its atomic weight.[37][38][25][39] Helium was also isolated by the American geochemist, William Francis Hillebrand, prior to Ramsay's discovery, when he noticed unusual spectral lines while testing a sample of the mineral uraninite. Hillebrand, however, attributed the lines to nitrogen.[40] His letter of congratulations to Ramsay offers an interesting case of discovery, and near-discovery, in science.[41] [Easy Way To Trade Logo]( You are receiving this e-mail because you have expressed an interest in the Financial Education niche on one of our landing pages or sign-up forms on our website. 11780 US Highway 1 Palm Beach Gardens, FL 33408-3080 Would you like to [edit your e-mail notification preferences or unsubscribe]( from our mailing list? Copyright © 2023 Weiss Ratings. All rights reserved. To ensure you keep receiving our emails, be sure to [whitelist us.]( 655 15th St NW, Washington, DC 20005, United States Copyright © 2023 Easy Way To Trade. All Rights Reserved[.]( [Privacy Policy]( l [Terms & Conditions]( l [Unsubscribe]( [Easy Way To Trade](