Wednesday, 22 July 2015

1. where did the elements heavier than hydrogen and helium come from

Top sites by search query "1. where did the elements heavier than hydrogen and helium come from"

  http://www.chem4kids.com/files/elem_intro.html
Element 1: Hydrogen Element 2: Helium Element 3: Lithium Element 4: Beryllium Element 5: Boron Element 6: Carbon Element 7: Nitrogen Element 8: Oxygen Element 9: Fluorine Element 10: Neon Element 11: Sodium Element 12: Magnesium Element 13: Aluminum Element 14: Silicon Element 15: Phosphorus Element 16: Sulfur Element 17: Chlorine Element 18: Argon As we move past the first eighteen elements, you can start to learn about transition elements in the fourth period (row) of the periodic table

Case Study: The Natural Abundance of Elements - Chemwiki


  http://chemwiki.ucdavis.edu/Inorganic_Chemistry/Case_Studies/Case_Study%3A_The_Natural_Abundance_of_Elements
Indeed, this process called the solar nebula theory has validity because we are able to see distantly forming solar systems with a dim central protostar surrounded by gas. Sign In Forgot Password Register username password If you like us, please share us on social media, tell your friends, tell your professor or consider building or adopting a Wikitext for your course

  http://www.armaghplanet.com/blog/the-star-older-than-the-universe.html
Reply Cameron Reed Posted November 4, 2014 at 6:15 PM Well how do you know that the big bang theory is correct you can say you have proof but you do not have a reliable source if so. Reply Cameron Reed Posted November 4, 2014 at 6:21 PM Well how do you know that the big bang theory is correct you can say you have proof but you do not have a reliable source if so

  http://scienceline.ucsb.edu/getkey.php?key=24
So - to summarize, your question has two parts: the abundance of iron and silicon is greater than the heavier elements in the universe in general, and the earth is at the right distance from the Sun so that when it condensed out of the solar nebula, the ligher elements were either bound up in compounds or blown away to the farther reaches of the solar system.Click Here to return to the search form. Back to the early solar nebula: In the center of this swirling gas cloud, or nebula, the density and temperature got high enough for a star to form and begin thermonuclear reactions in its core and shine

  http://m.teachastronomy.com/astropedia/article/The-Creation-of-Heavy-Elements
Stellar iron is actually denser than terrestrial iron, but the electrons have been stripped from all the atoms and the nuclei are not held together in a lattice. Those of around 8 solar masses will have hot enough cores to further ignite the carbon and fuse it into heavier elements such as oxygen, neon, and magnesium

  http://www.webelements.com/aluminium/
Aluminium was first isolated by Hans Christian Oersted in 1825 who reacted aluminium chloride (AlCl3) with potassium amalgam (an alloy of potassium and mercury). until 1925, at which time the American Chemical Society decided to revert back to aluminum, and to this day Americans still refer to aluminium as "aluminum"

Periodic Table of Elements - Elements Database


  http://www.elementsdatabase.com/
Mendeleev's Periodic Table It was only in 1869 when Dmitri Mendeleev, an inventor and chemist of Russian origin, discovered the Periodic Law and organized all chemical elements in columns and rows. Origins of the Periodic Table of Elements The Periodic Table displays all known chemical elements which are grouped by chemical properties and atomic structure

  http://scienceblogs.com/startswithabang/2012/12/12/why-the-world-will-run-out-of-helium/
assuming we get fusion reactors working within the next decade or so we will be converting mass amounts of hydrogen into helium, every country every continent. It would be released to the atmosphere when the natural gas is burnt.So, not filling a balloon with helium would not slow down (or speed up) the depletion of helium from the underground reservoirs

  http://startswithabang.com/?p=1762
But you also make a lot of heavier elements, like Carbon, Oxygen, and Nitrogen, and sometimes Silicon, Neon, and sometimes even Iron, Cobalt, and Nickel. Fortunately that people who sadly are overweight and also suffering from various diseases can help to eliminate the severity of the illnesses by simply losing weight

The Photographic Periodic Table of the Elements


  http://www.periodictable.com/
Newest samples 2 September, 2013 What you'll find on this site My Popular Science Column Buy Posters, Card Decks and Books! Don't miss the mostBeautiful periodic tableposters and card decks plusreal elements and displaysfrom the creators of this site

  http://www.rsc.org/periodic-table/element/1/hydrogen
The RSC makes no representations whatsoever about the suitability of the information contained in the documents and related graphics published on this Site for any purpose. Here's Brian Clegg.Brian CleggForget 10 Downing Street or 1600 Pennsylvania Avenue, the most prestigious address in the universe is number one in the periodic table, hydrogen

  http://web.lemoyne.edu/~giunta/EA/MENDELEEVann.HTML
Mendeleev's formulation was clearly superior in several respects to the work of contemporary classifiers: it was the clearest, most consistent, and most systematic formulation, and Mendeleev made several testable predictions based on it. Therefore, in the study of compounds, not only the quantities and properties of the elements and their reciprocal behavior is to be taken into consideration, but also the atomic weight of the elements

WMAP Big Bang Elements Test


  http://map.gsfc.nasa.gov/universe/bb_tests_ele.html
One second after the Big Bang, the temperature of the universe was roughly 10 billion degrees and was filled with a sea of neutrons, protons, electrons, anti-electrons (positrons), photons and neutrinos. The important prediction that the cosmic microwave background (CMB) exists, and has a blackbody spectrum with a temperature of about 5 degrees above absolute zero, was a by-product of this work

  http://mysite.du.edu/~jcalvert/phys/helium.htm
When alpha particles were allowed to enter a vacuum through a thin screen, the characteristic spectrum of helium was soon observed when an electrical discharge was produced. These lamps are supplied with a high-voltage transformer with large leakage reactance so that the voltage is high for striking, and decreases when current flows

  http://scienceblogs.com/startswithabang/2013/07/05/why-did-the-universe-start-off-with-hydrogen-helium-and-not-much-else/
It was once so hot that the Universe was filled with nearly equal amount of matter and antimatter: protons and antiprotons, neutrons and antineutrons, electrons and positrons, neutrinos and antineutrinos, and of course photons (which are their own antiparticle), among others. The brain just fills in a bunch of details because it decided that event took much longer than it really did, and therefore you should have been able to see a lot more than you normally would

No comments:

Post a Comment