Analyzing solar system elemental abundances:
(A) - Hydrogen (~73% by mass, ~92% by number) and Helium (~25% by mass, ~8% by number) are by far the most abundant elements in the solar system. Together they comprise about 98% of all matter. This reflects the primordial composition from the Big Bang and stellar nucleosynthesis.
(B) - There is a general exponential decrease in elemental abundance with increasing atomic number from H (Z=1) through the first 50 elements. This trend reflects:
(C) - This is false. Elements heavier than iron (Z=26) and certainly those above Z=50 are significantly less abundant than lighter elements. Heavy elements (>50) are produced through slow and rapid neutron capture processes (s-process and r-process) which are much rarer than the fusion processes creating lighter elements. The abundances continue to decrease for heavier elements.
(D) - This is the opposite of reality. The Oddo-Harkins rule states that elements with even atomic numbers are generally more abundant than their odd-numbered neighbors. This occurs because:
Answer: (A) and (B) are correct
| Group I | Group II | ||
| P | Iceland | 1 | Subduction Zone |
| Q | Indonesia | 2 | Transform Fault |
| R | Nepal | 3 | Mid-Oceanic Ridge |
| S | New Zealand | 4 | Continental Collision |