|
gptkb:K-electron_capture
|
gptkb:Auger_electron_emission
|
|
gptkb:GRB_980425
|
~10^48 ergs
|
|
gptkb:Solar_Flare
|
10^20 to 10^25 joules
|
|
gptkb:Type_Ib/c_supernova
|
~10^51 ergs
|
|
gptkb:Type_Ic_supernova
|
~10^51 ergs
|
|
gptkb:Type_II-P_supernova
|
~10^51 ergs
|
|
gptkb:Solar_flares
|
10^20 to 10^25 Joules
|
|
gptkb:FRBs
|
~10^38 joules
|
|
gptkb:Meteor_Strike
|
can be equivalent to nuclear explosion
|
|
gptkb:Type_II-L_supernova
|
~10^51 ergs
|
|
gptkb:Operation_Prayer_Power
|
for humanitarian crises
|
|
gptkb:GRB_221009A
|
among the most energetic GRBs observed
|
|
gptkb:Type_IIP_supernova
|
~10^51 ergs
|
|
gptkb:Type_Ib_supernova
|
~10^51 ergs
|
|
gptkb:K-electron_capture
|
X-ray emission
|
|
gptkb:High_Explosives
|
Very rapid
|
|
gptkb:GRB_970228
|
~10^52 ergs
|