Answer:
D. Z, X, Y
Hydrogen fusion in the sun occurs in the following three steps:
1. Fusion of Hydrogen into Deuterium.
Here two protons collide, one proton turns into a neutron emitting an antielectron and a neutrino.
The remaining proton is bound to the neutron forming a heavy Hydrogen (Deuterium) nucleus while the antielectron just produced will annihilate with an electron generating two high-energy photons.
2. The Formation of Helium-3
A proton is captured by a nucleus of Deuterium emitting a photon and forming then a 3He nucleus.
3. The Recombination of Two Helium-3 Into One Nucleus of Helium With The Emission of Two Protons
Note that steps 1 and 2 each happen twice for each time step 3 occurs. In this process, the total net energy released is up to 26 MeV.
I got this from:
"The Hydrogen Fusion Process - Windows to the Universe" https://www.windows2universe.org/?page=/sun/Solar_interior/Nuclear_Reactions/Fusion/Fusion_in_stars/H_fusion.html&edu=high#:~:text=The%20basic%20Hydrogen%20fusion%20cycle%20involves%20four%20Hydrogen,a%20neutron%20emitting%20an%20antielectron%20and%20a%20neutrino.
I hope this helps. Have a great day or night!