Talk:Hydrogen/Archive 3
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Origin
Most hydrogen in the universe was created on the first seconds of the Big Bang, by a process named Big Bang nucleosynthesis. Hydrogen atoms also are created in nature by disintegration of heavier elements, or by an electron capture by a proton from a pair production process.
- It does not make sense to say that protium was created by BBN when protons were already around, no? Double sharp (talk) 02:01, 5 November 2016 (UTC)
Suggested update to broken link
The link in Reference 126 is no longer valid, new link should be https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19970033338.pdf to reach the document. Thanks. -Kyle — Preceding unsigned comment added by Ksinger4 (talk • contribs) 12:50, 12 July 2017 (UTC)
Semi-protected edit request on 17 July 2017
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In the third sentence of the first paragraph of section 5.3 Energy Carrier, please change "Elemental hydrogen from solar, biological, or electrical sources require more energy to make it than is obtained by burning it" to "Elemental hydrogen from solar, biological, or electrical sources require(s) more energy to make than is obtained by burning it", adding an "s" to "require" because its noun is "Elemental hydrogen" and removing "it" after "make" because it is not needed. Thanks! Mahde darmo (talk) 03:31, 17 July 2017 (UTC)
External links modified
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- Added archive https://web.archive.org/web/20080213144956/http://www.sc.doe.gov/bes/hydrogen.pdf to http://www.sc.doe.gov/bes/hydrogen.pdf
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Expansion on hydrogen fusion
@David Condrey: recently added the following material to the article . I don't think I object to the addition in principle (although i haven't reviewed the material in full), but it's very poorly formatted at the moment, and brings the quality of this Featured Article down. I've included the material below, so it can be edited / tightened, and debated:
Origin of hydrogen
This article, and any article about an elemental atom and particles needs a section about how the element was created.
I propose this text:
External links modified
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I have just modified 7 external links on Hydrogen. Please take a moment to review my edit. If you have any questions, or need the bot to ignore the links, or the page altogether, please visit this simple FaQ for additional information. I made the following changes:
- Added archive https://web.archive.org/web/20090213174645/http://usm.maine.edu/~newton/Chy251_253/Lectures/LewisStructures/Dihydrogen.html to http://www.usm.maine.edu/~newton/Chy251_253/Lectures/LewisStructures/Dihydrogen.html
- Added archive https://web.archive.org/web/20080224162206/http://hydpark.ca.sandia.gov/DBFrame.html to http://hydpark.ca.sandia.gov/DBFrame.html
- Added archive https://web.archive.org/web/20090810180658/http://www.astronautix.com/craft/marveyor.htm to http://www.astronautix.com/craft/marveyor.htm
- Added archive https://web.archive.org/web/20010509065844/http://www.noble.org/ag/Soils/NitrogenPrices/Index.htm to http://www.noble.org/Ag/Soils/NitrogenPrices/Index.htm
- Added archive https://web.archive.org/web/20080216050327/http://bellona.org/filearchive/fil_Hydrogen_6-2002.pdf to http://bellona.org/filearchive/fil_Hydrogen_6-2002.pdf
- Added archive https://web.archive.org/web/20080302193129/http://energyquest.ca.gov/story/chapter13.html to http://www.energyquest.ca.gov/story/chapter13.html
- Added archive https://web.archive.org/web/20080527233910/http://www.hydrogenandfuelcellsafety.info/resources/mdss/Praxair-LH2.pdf to http://www.hydrogenandfuelcellsafety.info/resources/mdss/Praxair-LH2.pdf
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HYDROGEN
Is the light gas in the air it is made up of 78pacent.the only thing i what to know is that what are the chemical and physical properties of hydrogem — Preceding unsigned comment added by 41.59.35.203 (talk) 13:04, 1 March 2018 (UTC)
- Most of these properties are listed in the infobox, right in top. Meaninful or special properties are also described in the article text. Is there a property you are missing? - DePiep (talk) 14:40, 1 March 2018 (UTC)
- Most of air is made of nitrogen. Only a small amount of hydrogen is found in the atmosphere, mostly in the form of water vapour. Graeme Bartlett (talk) 22:00, 1 March 2018 (UTC)
Charged ion
In the section "Natural occurrence", one can find this sentence: "A molecular form called protonated molecular hydrogen (H3+) is found in the interstellar medium, where it is generated by ionization of molecular hydrogen from cosmic rays. This charged ion has also been observed in the upper atmosphere of the planet Jupiter". Now, why charged ion? To my knowledge, any ion must have a charge.Ekisbares (talk) 14:54, 27 January 2019 (UTC)
- @Ekisbares: You are correct; the word charged is redundant here, as ions by definition have a nonzero charge. You can be bold and fix it! ComplexRational (talk) 20:56, 27 January 2019 (UTC)
I corrected it just now. Thank you for the attention.Ekisbares (talk) 09:40, 28 January 2019 (UTC)
74% of this Universe's and the Sun's mass is Hydrogen
It's important to be accurate in science. This article refers to "roughly 75% of this Universe's mass is hydrogen". It's 74% and there are many good websites that confirm this - do a google search. Also, the Sun's mass is 74% hydrogen. 73.46.49.164 (talk) 05:43, 14 November 2017 (UTC)
Regarding accuracy -- the Sun is constantly turning Hydrogen into Helium...so that 74 percent figure won't be true forever. It is an accident of being at the right time -- 5 billion years -- after the Sun's formation. So...on that basis...I think "roughly 75 percent" sounds right. Chesspride 172.164.0.124 (talk) 08:54, 30 July 2018 (UTC)
The amount of hydrogen decreases with an increase in global warming. So there will be a minimal amount left of hydrogen. Karaya Melissa (talk) 17:47, 1 February 2019 (UTC)
Monatomic?
I'm not seeing backing for the claim that monatomic hydrogen is nearly as common as suggested in the article. Is that correct? Pinging Graeme Bartlett, who removed the {{fv}} tag, and DePiep, who reverted the removal of the claim. Best, Kevin (aka L235 · t · c) 01:36, 7 April 2019 (UTC)
- I reverted that edit because the editor was blocked at that time, and the statement did not have sourcing. Did not see the fv notice. If people think this is too strong a verdict, reentry can be OK. -DePiep (talk) 07:12, 7 April 2019 (UTC)
- Hi, I made that change. I included my logic in the edit summary. I can't cite it because nothing in google mentions anything about monatomic Hydrogen being the most abundant. I asked around in ##chemistry and ##physics who claim it's plausible because the hydrogen present in stars would be in plasma state but no citation on any numbers were produced. From the same NASA link, there seems to be more hydrogen outside stars unless I am misunderstanding it. "This is an interesting question. It is known that most of the hydrogen now in the galaxy is within stars. One estimate I found (Gene Smith's Astonomy Tutorial: http://casswww.ucsd.edu/public/tutorial/ISM.html is that only about 5% of hydrogen in the galaxy is in the form of interstellar gas. That's within a galaxy. Outside of a galaxy, but within a galaxy cluster, the density of hydrogen is about a thousand times less, but clusters are millions of times larger than galaxies, so there is likely much more hydrogen in intergalactic gas than there is in stars. " https://web.archive.org/web/20170216110630/https://imagine.gsfc.nasa.gov/ask_astro/stars.html . Sincerely, Itchyjunk (talk) 10:12, 7 April 2019 (UTC)
- Well the source supplied had turned into a dead link, so I changed the reference to a page from the same work on the website. The numbers did not match, but the article said "about" and that was close enough. Graeme Bartlett (talk) 11:04, 7 April 2019 (UTC)
- But that's talking about hydrogen in stars, right? The issue is around the claim that monatomic Hydrogen (H) as opposed to diatomic Hydrogen (H2) is the most abundant in the Universe. The NASA link also says there is a lot more Hydrogen outside of stars than in stars. That begs the question, "Why are 2 monatomic hydrogen floating around and not forming diatomic hydrogen?" I am not saying it correct or incorrect. But you need some citation to keep the claim. And as far as I could find, no source makes such a claim. "Hydrogen is most abundant?", sure. "Monatomic Hydrogen is most abundant?", citation needed. — Preceding unsigned comment added by Itchyjunk (talk • contribs) 20:56, 7 April 2019 (UTC)
- Well the source supplied had turned into a dead link, so I changed the reference to a page from the same work on the website. The numbers did not match, but the article said "about" and that was close enough. Graeme Bartlett (talk) 11:04, 7 April 2019 (UTC)
- Why not simply drop "monatomic" altogether? For instance
Its monatomic form (H) is the most abundant chemical substanceHydrogen (H) is the most abundant atom in the Universe, constituting roughly 75% of all baryonic mass.
- I think it is awkward to describe hydrogen in a plasma state as "monoatomic" - a plasma of H2 and a plasma of H look exactly the same: a soup of electrons and protons (and maybe a couple neutrons with some protons). TigraanClick here to contact me 09:52, 8 April 2019 (UTC)
Monatomic?
"When bonded to fluorine, oxygen, or nitrogen, hydrogen can participate in a form of medium-strength noncovalent bonding with the hydrogen of other similar molecules, a phenomenon called hydrogen bonding that is critical to the stability of many biological molecules."
Hydrogen bonding doesn't mean the hydrogens are bonding. They have a partial positive charge and the fluorine, oxygen and nitrogen have a partial negative charge, so the hydrogen is attracted to the negative charge on the other molecule.~~Syd Henderson~~ — Preceding unsigned comment added by 2600:8803:B402:FA00:CDE2:6F82:11E:FADA (talk) 00:36, 3 July 2019 (UTC)
- Replaced with "When bonded to a more electronegative element, particularly fluorine, oxygen, or nitrogen, hydrogen can participate in a form of medium-strength noncovalent bonding with another electronegative element with a lone pair, a phenomenon called hydrogen bonding that is critical to the stability of many biological molecules." Thank you for spotting the error! Double sharp (talk) 03:39, 3 July 2019 (UTC)
