The Anatomy of a Nucleus
Imagine you are zooming into the heart of an atom, past the swirling clouds of electrons, right into the dense, compact core known as the nucleus. What do you see? You see a tightly packed cluster of particles: protons and neutrons. These particles are collectively called nucleons.
To describe this nucleus, physicists use two fundamental numbers. The first is the atomic number, denoted by Z. This is simply the count of protons. It is the identity badge of the element. If Z=1, you have Hydrogen. If Z=6, you have Carbon.
The second number is the mass number, denoted by A. This is the total count of all nucleons—both protons and neutrons. If we let N represent the number of neutrons, we can write a very simple but powerful equation:
The Mathematical Constraint
Now, let's look at this equation logically. The number of neutrons, N, represents a physical count of particles. You can have zero neutrons, one neutron, or a hundred neutrons, but you can never have a negative number of neutrons.
Mathematically, this means N≥0.
If we substitute this logic back into our equation, we get a strict constraint:
This tells us that the mass number A will always be greater than or equal to the atomic number Z. It can never, ever be less. This immediately eliminates option (a) from our question.
The Lone Exception
Protium
You might wonder, is the mass number ever exactly equal to the atomic number? For this to happen, N must be exactly zero. Does such a nucleus exist?
Yes, it does! Look at the most abundant element in the universe: Hydrogen. Specifically, its most common isotope, Protium (11H). The nucleus of Protium consists of a single, lonely proton and absolutely zero neutrons.
For Protium:
Z=1
N=0
A=1+0=1
Here, A=Z. This proves that the mass number is sometimes equal to the atomic number.
The General Rule
Heavier Nuclei
What about literally every other isotope in the universe? Let's take another isotope of Hydrogen, called Deuterium (12H). This nucleus contains one proton and one neutron.
For Deuterium:
Z=1
N=1
A=1+1=2
Here, A>Z. As we move to heavier elements, the number of neutrons not only equals the number of protons but eventually exceeds it to keep the nucleus stable against electrostatic repulsion. For example, Uranium-238 has 92 protons and 146 neutrons!
The Final Verdict
By analyzing the physical reality of the nucleus, we have discovered that the mass number is sometimes exactly equal to the atomic number (as in the case of Protium) and sometimes strictly greater than the atomic number (as in Deuterium and all other heavier nuclei).
Therefore, both statements (c) and (d) perfectly describe the relationship between the mass number and the atomic number.