en.wikipedia.org/wiki/Nuclear_transmutation
6 corrections found
iron, which is produced by an endothermic reaction (one that consumes energy).
This reverses the usual stellar-fusion rule: fusion up to iron releases energy, while fusing iron or heavier nuclei requires energy input.
Full reasoning
In stellar nucleosynthesis, iron is the endpoint because fusion to iron does not yield increasing energy beyond that point. Authoritative NASA explanations say stars build elements up to iron, and that iron requires more energy to fuse than it creates. NASA Goddard likewise explains that elements lighter than iron generally emit energy if fused and that iron releases no energy when fused. So the problem is not that iron itself is produced by an endothermic reaction; rather, fusion of iron (or of heavier nuclei) is energetically unfavorable. The article's wording incorrectly states that producing iron is endothermic.
2 sources
- NASA Science – Big Idea 3.2
Many layers of fusion create more elements, up to iron, as iron requires more energy to fuse than it creates.
- NASA GSFC – What is Your Cosmic Connection to the Elements?
Fusion continues in red supergiants until iron is formed. Unlike the elements before it, iron releases no energy when fused. Elements lighter than iron generally emit energy if fused.
The first artificial transmutation was accomplished in 1925 by Patrick Blackett
Standard histories credit Rutherford’s 1919 nitrogen-bombardment experiment as the first artificial transmutation; Blackett’s 1925 work confirmed and clarified that reaction.
Full reasoning
This sentence conflicts with standard historical accounts of nuclear physics. A 1934 Nature summary states that the first artificial transmutation was accomplished in 1919, when nitrogen was disintegrated by alpha-particle bombardment. The American Institute of Physics’ chronology likewise records that Rutherford caused transmutation from one stable chemical element into another in 1919. Blackett’s later cloud-chamber work was important because it provided clearer experimental evidence and identified the residual oxygen nucleus, but that is different from saying he accomplished the first artificial transmutation.
2 sources
- Artificial Nuclear Transmutations | Nature
The first of such transmutations was accomplished in 1919, when nitrogen was disintegrated by a-particle bombardment with the liberation of fast protons.
- Discovery of Fission - Moments of Discovery
1919 Rutherford causes transmutation from one stable chemical element into another, by bombardment with alpha particles.
when a uranium atom is bombarded with slow neutrons, fission takes place.
This is only true for certain uranium isotopes, especially U-235. Most uranium in reactor fuel is U-238, which does not fission with slow (thermal) neutrons.
Full reasoning
The statement is too broad because uranium is not a single nuclear species. The U.S. Nuclear Regulatory Commission explains that uranium-235 fissions with low-energy thermal neutrons, but uranium-238 does not; for U-238, a neutron must have additional energy for fission to occur. NRC’s reactor explainer likewise says the chain reaction depends on U235, and that U238 cannot sustain the fission process without the help of an elevated concentration of U235. So the sentence is inaccurate as written: it should specify uranium-235 (or another fissile isotope), not “a uranium atom” in general.
2 sources
- Fissionable material | Nuclear Regulatory Commission
Uranium-235 fissions with low-energy thermal neutrons... By contrast, the binding energy released by uranium-238 absorbing a thermal neutron is less than the critical energy, so the neutron must possess additional energy for fission to be possible.
- What is a Chain Reaction? | Nuclear Regulatory Commission
The primary active ingredient in the fuel for a nuclear reactor is... U235... The majority of the uranium in the reactor is in the form of... U238, which cannot sustain the fission process without the help of an elevated concentration of the isotope U235.
discovered that radioactive thorium was converting itself into radium.
Rutherford and Soddy’s thorium work did not show thorium turning directly into radium. Their 1902 result was that thorium produced new radioactive substances, notably thorium X and a gaseous emanation.
Full reasoning
This sentence misstates Rutherford and Soddy’s discovery. The American Institute of Physics’ Rutherford exhibit says that their work on thorium in 1901 and 1902 provided chemical evidence for a change from thorium to “thorium X”, establishing that radioactive decay produced a new atom. Frederick Soddy’s own later summary in Scientific American says their 1902 conclusion about thorium was that one product was the thorium emanation, a gas, formed from thorium through the intermediary thorium-X. Those sources do support that Rutherford and Soddy recognized radioactive transmutation, but not that they discovered thorium converting itself into radium.
2 sources
- Rutherford's Nuclear World: Exploring Radioactivity | American Institute of Physics
His best known chemical colleague was Frederick Soddy... who worked with him on thorium and its decay products in 1901 and 1902. Chemical evidence provided the decisive proof that the change from thorium to the purposefully vaguely named 'thorium X' did not occur at the molecular level, but at the atomic level.
- What is a Chemical Element? | Scientific American
The conclusion in 1902 by Sir Ernest Rutherford and myself with regard to the element thorium was of this direct and simple character... One of the constituents, the thorium emanation, is a gas... It is formed from thorium through the intermediary of another constituent, thorium-X.
Nuclides with mass number greater than 64 are predominantly produced by neutron capture processes—the s-process and r-process–in supernova explosions and neutron star mergers.
This mixes up the sites of the two neutron-capture processes. The r-process is associated with explosive events such as neutron-star mergers, but the s-process mainly occurs in asymptotic giant branch (AGB) stars.
Full reasoning
The sentence incorrectly groups the s-process with supernova explosions and neutron-star mergers. Physics Today explains that in asymptotic giant branch (AGB) stars, neutron-capture events are separated by long intervals, which is the defining condition for the slow neutron-capture (s-) process. By contrast, in cataclysmic environments such as supernovae a nucleus can capture several neutrons within seconds, corresponding to the rapid neutron-capture (r-) process. A separate NASA explanation of heavy-element production likewise describes r-process elements as forming in environments with enormous neutron densities, such as neutron-star collisions or some supernova explosions. So the article’s wording is wrong because it places both s- and r-process nucleosynthesis in explosive events, when the s-process is primarily an AGB-star process.
2 sources
- Particle storage ring enables a role reversal in proton capture - Physics Today
In so-called asymptotic giant branch stars, neutron-capture events can be separated by decades... In cataclysmic environments such as supernovae, on the other hand, a nucleus may capture several neutrons within seconds. Together, those two versions of the mechanism, called the s- and r-processes...
- NASA@SC20: Understanding How Violent Cosmic Events Create Heavy Elements
These so-called 'r-process' elements... are thought to be created in an astrophysical environment with an enormously high neutron density, such as those resulting from the collisions of neutron stars or supernova explosions.
In 2022, CERN's ISOLDE team reported producing 18 gold nuclei from proton bombardment of a uranium target.
The 2022 ISOLDE paper was about 18 radioactive gold ion beams (i.e., 18 gold isotopes/beams), not just 18 individual gold nuclei.
Full reasoning
This sentence appears to misread the underlying paper. The 2022 article “Producing gold at ISOLDE-CERN” does not report creating only 18 nuclei total. Its abstract says the researchers measured the yield of 18 ion beams of radioactive gold nuclei produced in a thick uranium target bombarded by 1.4-GeV protons. In other words, the paper concerns 18 gold radioactive ion beams / isotopic species, not merely 18 individual nuclei.
1 source
- Producing gold at ISOLDE-CERN - The University of Liverpool Repository
Abstract: The yield of 18 ion beams of radioactive gold nuclei produced in the thick uranium target at ISOLDE (CERN) by 1.4-GeV protons was measured.