Four.
Hydrogen has one proton in its nucleus.
Each isotope of hydrogen has 1 proton in the nucleus. The difference between the isotopes lies in the number of neutrons: hydrogen-1 has 0 neutrons, hydrogen-2 (deuterium) has 1 neutron, and hydrogen-3 (tritium) has 2 neutrons.
There are three known naturally occurring isotopes of hydrogen; hydrogen-1 with one proton and no neutrons, hydrogen-2 with one proton and one neutron, and hydrogen-3 with one proton and two neutrons.
All hydrogen atoms, regardless of the number of neutrons in its isotope (zero neutrons for protium, one for deuterium, two for tritium), would have only one proton.
A star is made up primarily of hydrogen atoms. Hydrogen atoms consist of one proton and one electron. So, a star contains a very large number of hydrogen particles corresponding to the total mass and volume of the star, with each hydrogen atom having one proton.
For each full cycle of the proton-proton chain, four hydrogen nuclei combine to form one helium nucleus. This results in a net loss of four hydrogen nuclei, which is equivalent to the mass of the helium nucleus produced. This process is the primary fusion reaction that powers the Sun and other main-sequence stars.
Hydrogen has one proton in its nucleus.
Hydrogen-1 is fused into helium-4. This happens at high temperatures - somewhere around 14 million kelvin (which, at such high temperatures, is the same as 14 million degrees Celsius, for all practical purposes). There are two main reaction chains that in stars: the proton-proton chain reaction, and the CNO cycle. I suggest you read the corresponding Wikipedia articles, if you want more details about each of the reaction chains. Anyway, in our Sun, the predominant reaction chain is the proton-proton chain reaction.
A gas with one proton would be hydrogen gas (H2), which consists of two hydrogen atoms, each with one proton.
An isotope of hydrogen will always have 1 proton.
Each isotope of hydrogen has 1 proton in the nucleus. The difference between the isotopes lies in the number of neutrons: hydrogen-1 has 0 neutrons, hydrogen-2 (deuterium) has 1 neutron, and hydrogen-3 (tritium) has 2 neutrons.
There are three known naturally occurring isotopes of hydrogen; hydrogen-1 with one proton and no neutrons, hydrogen-2 with one proton and one neutron, and hydrogen-3 with one proton and two neutrons.
The overall result of the proton-proton chain is the fusion of four protons to form a helium nucleus (two protons and two neutrons) along with releasing energy in the form of gamma rays and neutrinos. This process is the main energy source for stars like our Sun.
Hydrogen is made up of one proton and one electron. It is the lightest and most abundant element in the universe.
All hydrogen atoms, regardless of the number of neutrons in its isotope (zero neutrons for protium, one for deuterium, two for tritium), would have only one proton.
The positively charged subatomic particles that remain when a hydrogen atom loses an electron are protons. Each hydrogen atom normally contains one proton, and when an electron is lost, the proton remains with a net positive charge.
The most common isotope of hydrogen has one proton, and one electron.The most common isotope of hydrogen has one proton, and one electron.The most common isotope of hydrogen has one proton, and one electron.The most common isotope of hydrogen has one proton, and one electron.