45
votes
Are we really star-stuff from the interior of collapsing stars?
The straightforward answer is, "Yes, we are made of star stuff."
Some of it will be from the interior of collapsing stars, some will be from supernovas, some from normal everyday fusion, and some ...
44
votes
Accepted
Is lithium considered a metal in astronomy?
The latter.
To astronomers, a metal is any element that is not hydrogen or helium, because these elements together constitute most of the elements in the Universe, by far.
This means that, in many ...
38
votes
Accepted
Why didn't the Big Bang produce heavier elements?
I think that your thought process is flawed in that you assume that by drastically increasing the temperature you are guaranteed to get heavy elements. As odd as this may sound, this isn't the case (...
29
votes
Why don’t supergiants at least start to fuse nickel into even heavier elements before going supernova?
The final stages of nucleosynthesis are a statistical equilibrium process. At the same time as nuclei are being built up, photodisintegration is breaking them down.
The temperatures required to ...
29
votes
Accepted
Formation of elements in the Sun other than helium
The Sun is currently turning hydrogen into helium. There are no other nuclear reactions taking place at any significant rate in the Sun. The Sun will not start to make heavier elements until it ...
27
votes
Do stars become more metal-rich as they evolve?
If the star is a solar mass or below it will not produce any metals (anything heavier than helium) within 10 billion years of birth. It will be on the main sequence, fusing hydrogen to helium via the ...
20
votes
Are we really star-stuff from the interior of collapsing stars?
Sagan's quote is half-correct. While some of these elements are created during or immediately prior to a supernova of some sort, others are either partially or entirely fused during normal stellar ...
19
votes
Does a star fuse helium to beryllium on the main sequence?
Does a star fuse helium to beryllium on the main sequence?
Stars don't fuse helium to beryllium except as a very, very short intermediate step toward carbon. Helium-helium fusion to form beryllium is ...
18
votes
What would the Sun be like if nuclear reactions could not proceed via quantum tunneling?
Short answer: Without tunnelling, stars like the Sun would never reach nuclear fusion temperatures; stars less massive than around $5M_{\odot}$ would become "hydrogen white dwarfs" supported by ...
18
votes
Accepted
Is oxygen an alpha element?
Two things.
The abundance of oxygen is a difficult thing to measure in optical spectra - much harder than Mg, Ca, and Si. So these latter are usually used to represent "the alpha elements". ...
17
votes
Can we compress any object to create black Holes?
Do you mean, "Can we in principle", or just, "Can we..." ?
The answer to the latter is no. We have no technology to create black holes. It was a remote possibility that was considered when creating ...
15
votes
What effects besides "mass defect" cause the alpha ladder beyond iron-56/nickel-56 to be endothermic?
There are plenty of misleading statements in Wikipedia and elsewhere on the internet about nucleosynthesis (I am busy searching to see if I have said something similar in the past!)
The reason that ...
15
votes
Do stars become more metal-rich as they evolve?
Yes, it will
Metals in astronomy, are simply elements that are heavier than hydrogen and helium. From that perspective, even oxygen and carbon are "metals" in a astronomical sense, although ...
11
votes
Accepted
Why does lithium fuse at lower temperatures than hydrogen?
The slowest reaction rate in the pp chain determines how quickly hydrogen can "burn" in the core of a sun-like star. That rate-determining step is actually the fusion of two protons to form ...
11
votes
Accepted
Does a star fuse helium to beryllium on the main sequence?
What defines the main sequence?
Main sequence stars are characterized by hydrogen fusion in their cores, either through the proton-proton chain (for lower-mass stars) or the CNO cycle (for stars more ...
9
votes
Accepted
Do we know how old the matter that makes us is?
The material (heavier than helium) that makes up the solar system was made in millions, if not hundreds of millions of stars that lived and died in the ~7 billion years between the formation of the ...
9
votes
Accepted
Why do stars usually stop fusion at iron, even though nickel-62 has the highest binding energy per nucleon?
Contrary to common myth, the addition of alpha particles to iron-peak nuclei is exothermic. However, in the nickel/iron core of a massive star, there are no free alpha particles, they must be broken ...
8
votes
Accepted
Why is it that lithium and deuterium are burned before hydrogen?
Deuterium burns first because its combination with a proton or another deuteron is a pure strong nuclear force interaction, with the minimum of Coulomb repulsion. It occurs at lower temperatures than ...
7
votes
Can we compress any object to create black Holes?
Kind of a quick answer, if you don't mind.
Can we compress any object to create black Holes?
The pressure at the bottom of the ocean is enormous, it would kill a person in a fraction of a second, ...
7
votes
Accepted
Does Oxygen-burning process produce Neon?
The pages you’re looking at describe fusion of two similar nuclei with each other (e.g. oxygen with oxygen). But fusion doesn’t have to involve identical nuclei, and reactions involving more abundant ...
7
votes
Accepted
Can I "see" nucleosynthesis in R Geminorum with a small telescope, a plastic diffraction grating and a cell phone? (famous technetium lines)
No, even if you could resolve the spectral lines, there is no way in your proposed experiment that you could distinguish the Technetium features from spectral lines due to many other chemical elements....
6
votes
Accepted
What is the length of time for each fusion process in a massive star?
My stellar astrophysics text, Francis LeBlanc's An Introduction to Stellar Astrophysics, gives the following quantities for the stages of burning in a $25M_{\odot}$ star (citing models by Arnould &...
6
votes
Why does iron consume more energy in the fusion process than it produces?
As can be seen in this question: What effects besides "mass defect" cause the alpha ladder beyond iron-56/nickel-56 to be endothermic? It is not so straightforward to explain why fusion ...
5
votes
Accepted
"Turn on point" for fusion?
I don't have detailed model calculations to hand and I'm not sure they have been done for the small range of metallicity you mention. However, in handwaving terms.
(1) Mass and composition are the ...
5
votes
Accepted
Does Alpha Process Produce Bismuth?
Bismuth is produced via the s-process.
It is the slow absorption of neutrons that can produce heavier elements beyond the peak of the binding energy per nucleon curve at iron. The alpha process isn't ...
5
votes
Accepted
In layman's terms, why does the cold C-N-O process end in Carbon?
Both 15N($p,\alpha$)12C and 15N($p,\gamma$)16O can and do take place. However, the former is a strong force interaction, whilst the latter is mediated by the electromagnetic force and is known as a &...
5
votes
In layman's terms, why does the cold C-N-O process end in Carbon?
This question has several misunderstandings.
The CNO cycles (there is more than one CNO cycle) in a main sequence star have nothing to do with the triple alpha process. A star that is using the triple ...
4
votes
Accepted
Would dropping a white dwarf or a "still-hot" stellar core into a large planet or brown dwarf create a star?
The issue is not whether the dense core can fuse, but what fusion processes can occur on its surface. Remember that novas happen when gas accumulate on the surface of white dwarf stars: the high ...
4
votes
Do the newly-created deuterons in our Sun release any photons? In addition to a positron and an electron neutrino?
Does the newly-formed deuteron then automatically release a photon?
Not directly. The initial step of the p-p chain is a weak interaction rather than an electromagnetic interaction. This initial step ...
3
votes
Formation of elements in the Sun other than helium
Pretty sure from my stellar nucleosynthesis days that the p-p I chain is the dominant form of nucleosynthesis in the sun, but the p-p II, p-p III, and p-p IV chains also occur, just to a much lesser ...
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