2778: Cuisine - Revision history

CalibansCreations: /* Explanation */

2025-03-19T08:57:07Z

‎Explanation

162.158.155.82: /* Explanation */

2023-09-23T12:48:34Z

‎Explanation

Pressforaction: /* Explanation */

2023-09-02T14:55:51Z

‎Explanation

172.69.22.71: /* Explanation */

2023-08-21T21:09:30Z

‎Explanation

DownGoer: I would argue that the mistake is more funny than unfortunate

2023-08-10T06:25:58Z

I would argue that the mistake is more funny than unfortunate

162.158.186.245: /* Explanation */ clarify

2023-06-29T00:31:00Z

‎Explanation: clarify

172.70.90.61: /* Explanation */ Very very minor tweaks. (Can't remember if US spelling is "fuzing", so leaving that. Works for me as it is, anyway.)

2023-05-31T07:55:35Z

‎Explanation: Very very minor tweaks. (Can't remember if US spelling is "fuzing", so leaving that. Works for me as it is, anyway.)

Kynde: Rewriting title text explanation which has nothing to do with stars as it is before stars.

2023-05-30T13:28:15Z

Rewriting title text explanation which has nothing to do with stars as it is before stars.

Kynde: /* Explanation */

2023-05-30T13:15:10Z

‎Explanation

Kynde: /* Explanation */

2023-05-30T13:14:06Z

‎Explanation

@@ Line 11: / Line 11: @@
 ==Explanation==
-[[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures{{Citation needed}}, such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
+[[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures,{{Citation needed}} such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
 The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions).

@@ Line 13: / Line 13: @@
 [[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures{{Citation needed}}, such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
-The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions)
+The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions).
 The title text refers to the time before {{w|stellar fusion}}, just after the Big Bang when most matter was hydrogen atoms. See [[2723: Outdated Periodic Table]] for more on what other atoms were present. These primordial hydrogen atoms formed clouds that eventually collapsed into galaxies, forming stars that then created all heavier elements in one way or another. It took a long time but eventually some of these hydrogen atoms created Cueball and everything else on Earth. See [[1123: The Universal Label]]. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, indicating that it is his atoms that are interested in this cuisine – not himself – as they were the ones around when his interest began. Actually mainly his protons. And it was because of their interest in fusing together that Cueball came to be.

@@ Line 13: / Line 13: @@
 [[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures{{Citation needed}}, such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
-The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium, and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions)
+The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions)
-The title text refers to the time before {{w|stellar fusion}}, just after the Big Bang when most matter was hydrogen atoms. See [[2723: Outdated Periodic Table]] for more on what other atoms where present. These primordial hydrogen atoms formed clouds that eventually collapsed into galaxies, forming stars that then created all heavier elements in one way or the other. It took a long time but eventually some of these hydrogen atoms created Cueball and everything else on Earth. See [[1123: The Universal Label]]. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, indicating that it is his atoms that are interested in this cuisine not himself, as they were the ones around when his interest began. Actually mainly his protons. And it was because of their interest in fusing together that Cueball came to be.
+The title text refers to the time before {{w|stellar fusion}}, just after the Big Bang when most matter was hydrogen atoms. See [[2723: Outdated Periodic Table]] for more on what other atoms were present. These primordial hydrogen atoms formed clouds that eventually collapsed into galaxies, forming stars that then created all heavier elements in one way or another. It took a long time but eventually some of these hydrogen atoms created Cueball and everything else on Earth. See [[1123: The Universal Label]]. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, indicating that it is his atoms that are interested in this cuisine – not himself – as they were the ones around when his interest began. Actually mainly his protons. And it was because of their interest in fusing together that Cueball came to be.
 ==Transcript==

@@ Line 11: / Line 11: @@
 ==Explanation==
-[[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures, such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
+[[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures{{Citation needed}}, such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
 The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium, and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions)

@@ Line 11: / Line 11: @@
 ==Explanation==
-[[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures, such as a combination of French and Chinese food, or Mexican and Korean food. Unfortunately, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
+[[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, typically used to describe a style of cuisine based on combining aspects of the cuisines of two or more cultures, such as a combination of French and Chinese food, or Mexican and Korean food. However, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
 The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium, and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions)

@@ Line 14: / Line 14: @@
 [[Cueball]] is explaining a recipe to [[White Hat]], describing it as {{w|Fusion cuisine}}, a style of cuisine based on combining aspects of the cuisines of two or more cultures, such as a combination of French and Chinese food, or Mexican and Korean food. Unfortunately, he conflates this with {{w|nuclear fusion}}, combining atomic nuclei to create new kinds of atoms.
-The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium, and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron star spiral into each other (but they are remnants of super nova explosions)
+The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize atoms heavier than iron, such as copper, zinc, selenium, and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein. Most heavier elements are probably created when two Neutron stars spiral into each other (but they are remnants of super nova explosions)
-The title text refers to the time before {{w|stellar fusion}}, just after the Big Bang when most matter was hydrogen atoms. See [[2723: Outdated Periodic Table]] for more on what other atoms where present. These primordial hydrogen atoms formed clouds that eventually collapsed into galaxies, forming stars that then created all heavier elements in one way or the other. It took a long time but eventually some of these hydrogen atoms created Cueball and everything else on Earth. See [[1123: The Universal Label]]. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, indicating that it is his atoms that are interested in this cuisine not him self, as they where the ones around when his interest began. Actually mainly his protons. And it was because of their interest in fusing together that Cueball came to be.
+The title text refers to the time before {{w|stellar fusion}}, just after the Big Bang when most matter was hydrogen atoms. See [[2723: Outdated Periodic Table]] for more on what other atoms where present. These primordial hydrogen atoms formed clouds that eventually collapsed into galaxies, forming stars that then created all heavier elements in one way or the other. It took a long time but eventually some of these hydrogen atoms created Cueball and everything else on Earth. See [[1123: The Universal Label]]. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, indicating that it is his atoms that are interested in this cuisine not himself, as they were the ones around when his interest began. Actually mainly his protons. And it was because of their interest in fusing together that Cueball came to be.
 ==Transcript==

@@ Line 16: / Line 16: @@
 The recipe is described as the initiation of {{w|deuterium}} fusion in a kilogram ("four cups") of {{w|heavy water}} and allowing the reaction to continue to its endpoint, {{w|iron}}. The "very high heat" specified in the recipe would start at the four million-plus Kelvin at which {{w|deuterium fusion}} is initiated in stars, and could possibly reach the billions of Kelvin at which {{w|supernova}}s synthesize all atoms heavier than iron, such as copper, zinc, selenium, and iodine, which are essential in trace quantities for mammals. Unfortunately, heating a saucepan to even four million Kelvin would likely vaporize even the largest of kitchens, and any cooks therein.
-The title text refers to {{w|stellar fusion}} as responsible for at least one atom in each molecule of every living thing (excepting a tiny proportion of {{w|lithium hydride}}[https://academic.oup.com/mnras/article/476/2/1826/4848311][https://www.cdc.gov/niosh/docs/81-123/pdfs/0371.pdf?id=10.26616/NIOSHPUB81123]), all our food and water, and indeed everything but primordial [[2719: Hydrogen Isotopes|hydrogen isotopes]] and the tiny proportions of helium and lithium that were synthesized at the end of the {{w|radiation-dominated era}}; thus Cueball's personal interest in "fusion" cuisine. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, which is unusual.{{fact}}
+The title text refers to {{w|stellar fusion}} as responsible for at least one atom in each molecule of every living thing (excepting a tiny proportion of {{w|lithium hydride}}[https://academic.oup.com/mnras/article/476/2/1826/4848311][https://www.cdc.gov/niosh/docs/81-123/pdfs/0371.pdf?id=10.26616/NIOSHPUB81123]), all our food and water, and indeed everything but primordial [[2719: Hydrogen Isotopes|hydrogen isotopes]] and the tiny proportions of helium and lithium that were synthesized at the end of the {{w|radiation-dominated era}}; thus Cueball's personal interest in "fusion" cuisine. People often say that an interest of theirs goes back to their "early days", referencing their childhood, but in this case it appears that Cueball's interest goes back to several billions of years before he was born, indicating that it is his atoms that are interested in this cuisine not him self.
 ==Transcript==