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Taking the distance to the Crab pulsar to be 2000 pc and the bolometric magnitude at maximum brightness of the respective type Il supernovae explosion to be Mbol=-17, estimate the peak apparent magnitude. Compare this to the maximum brightness of Venus (m- -4), which can sometimes be seen during daytime.

Taking the distance to the Crab pulsar to be 2000 pc and the bolometric magnitude at maximum brightness of the respective type Il supernovae explosion to be Mbol=-17, estimate the peak apparent magnitude. Compare this to the maximum brightness of Venus (m- -4), which can sometimes be seen during daytime.

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Taking the distance to the Crab pulsar to be 2000 pc and the bolometric magnitude at maximum brightness of the respective type II supernovae explosion to be M_bol = -17, estimate the peak apparent magnitude. Compare this to the maximum brightness of Venus (m ≈ -4), which can sometimes be seen during daytime.
Transcribed Image Text:Taking the distance to the Crab pulsar to be 2000 pc and the bolometric magnitude at maximum brightness of the respective type II supernovae explosion to be M_bol = -17, estimate the peak apparent magnitude. Compare this to the maximum brightness of Venus (m ≈ -4), which can sometimes be seen during daytime.
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