|
gptkb:Type_II_supernovae
|
~10^44 joules
|
|
gptkb:Fast_Radio_Burst
|
~10^38 joules
|
|
gptkb:Beta_plus_decay
|
Q-value
|
|
gptkb:Naked-eye_burst
|
~10^54 ergs
|
|
gptkb:potassium-40_decay
|
1.311 MeV (beta minus)
|
|
gptkb:2013_Russian_meteor_event
|
~470 kilotons of TNT
|
|
gptkb:Type_Ia_Supernova
|
~10^44 joules
|
|
gptkb:Alpha_decay
|
Typically 4-8 MeV
|
|
gptkb:GW170817_detection
|
~10^53 ergs
|
|
gptkb:potassium-40_decay
|
1.505 MeV (electron capture)
|
|
gptkb:The_Zorro_Burst
|
extremely high
|
|
gptkb:March_5,_1979_gamma-ray_burst
|
~10^44 joules
|
|
gptkb:Fast_Radio_Bursts
|
~10^38 joules
|
|
gptkb:GW150914_observation
|
~3 solar masses converted to gravitational waves
|
|
gptkb:1908_Tunguska_event
|
10–15 megatons of TNT
|
|
gptkb:Type_II_supernova
|
~10^44 joules
|
|
gptkb:Great_East_Japan_Earthquake
|
about 600 million times Hiroshima bomb
|
|
gptkb:GRB_080916C
|
8.8×10^54 ergs
|
|
gptkb:Chicxulub_asteroid_impact
|
~10^23 joules
|
|
gptkb:binary_black_hole_merger_GW150914
|
~3 solar masses converted to gravitational waves
|