3. Look up the densities of white dwarfs. neutron stars, and black holes. Sort them by increasing mass. Low-Mass Star Energy Production The following equations show the first energy production process in low-mass stars like our Sun. The symbols are as follows: H 2 hydrogen, He = helium, e + is a positron, v is a neutrino, and y is a photon (gamma-ray). The numerical superscripts on the upper-left corner of the symbols represent the atomic mass (aka number of protons and neutrons in the nucleus). Study it and answer the questions that follow. 1H+1H>2H+e++v 2H+1H>3He+y 3He+ 3He >4He+ 1H + 1H 4. What fuel (input) appears on the left-hand side of the first equation? 5. What type of energy is released on the right-hand side of the second equation? 6. What atom other than hydrogen is released on the right side of the third equation? 7. Fill-in the table using your answers from #4, #5. and #6: Name of Energy Production Process Shown NI IPIPI Ic: Fnrmnrl