OptionProbability
1687 K (melting point of silicon)
5800 K (solar photosphere i.e. Sun's visible surface, slightly hotter than Earth's core)
28,000 K (lightning strike)
15,000,000 K (15 million K, solar core)
300,000,000 K (300 million K, thermonuclear bomb)
100,000,000,000 K (100 billion K, supernova)
1.416784(16) x 10^32 K (Planck temperature, Big Bang)
27
8
7
6
3
Other
Mars
Europa
Titan
Enceladus
Venus
K2-18 b
Earth
The Big Bang
Ceres
Pluto/Charon
Triton
Luna (presumably in a shaded crater/magma tube)
Pluto
Charon
TRAPPIST-1d
Proxima Centauri b
Unknown
58
18
5
1
0
OptionVotes
YES
NO
1325
922
229
122
It has or may continue to vary over time at times after the first 1 billion years after the Big Bang
It varied over time during the first 1 billion years after the Big Bang
At the current time it varies across space
25
24
14
300
33
Systematic errors in stellar abundance observations
Varying fundamental constants
Stellar depletion (astrophysical solution)
Nuclear physics: Unknown/revised BBN reaction rates
Sterile neutrinos
Inhomogeneous cosmology
Decaying or annihilating dark matter
59
56
53
50
35
26