Q 01/05
A) Their resonant frequency
B) Their temperature
C) Their radioactive decay rate
D) Their mass
Answer · why
Transitions between quantised energy levels are driven by very specific frequencies of radiation, which is what the clock locks onto.
Q 02/05
A) A hyperfine transition
B) A nuclear isomer transition
C) A rotational transition
D) A vibrational transition
Answer · why
It is the tiny energy split in the atom's ground state, driven by microwaves at about 9.19 GHz.
Q 03/05
A) 299,792,458
B) 1,420,405,752
C) 6,834,682,611
D) 9,192,631,770
Answer · why
The other numbers are rubidium's frequency, hydrogen's 21-cm line and the speed of light in metres per second.
Q 04/05
A) The mean solar day of 1950
B) The lunar month
C) The tropical year 1900
D) A sidereal day
Answer · why
There were deemed to be 31,556,925.9747 seconds in that year.
Q 05/05
A) Heinrich Hertz
B) Michael Faraday
C) Lord Kelvin
D) James Clerk Maxwell
Answer · why
He argued it would beat the Earth's rotation, which then defined the mean solar second.
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