Home
Class 12
CHEMISTRY
In the nuclear reaction ""(3) Li^(7) + "...

In the nuclear reaction `""_(3) Li^(7) + ""_(1) H^(1) to 2""_(2) He^(4)` . The mass loss is nearly 0.02 amu . Hence the energy released in the process is `x xx 10^(2)` million kcal l mole . (nearly) . Then 'x' is ____

Text Solution

Verified by Experts

The correct Answer is:
4

`Q = ((0.02 xx 931.5 xx 10^(6) xx 1 .602 xx 10^(-19) xx 6 xx 10^(23))/(4 .18 xx 1000)) = 42.84 xx 10^(3+ 4)`
`= 4.284 xx 10^(8)` Kcal/mole = `4.28 xx (10^(8))/(10^(6))` million Kcal/mole = `4 xx 10^(2)` million Kcal/mole
Promotional Banner

Topper's Solved these Questions

  • NUCLEAR CHEMISTRY

    AAKASH SERIES|Exercise PRACTICE SHEET - 2 (Single or more than one option questions)|14 Videos
  • NUCLEAR CHEMISTRY

    AAKASH SERIES|Exercise PRACTICE SHEET - 2 (Linked Comprehension type questions )|6 Videos
  • NUCLEAR CHEMISTRY

    AAKASH SERIES|Exercise PRACTICE SHEET - 1 (Match the following questions)|2 Videos
  • NOBLE GASES

    AAKASH SERIES|Exercise PRACTICE SHEET - 2 (Single more than one option questions)|5 Videos
  • PERIODIC TABLE

    AAKASH SERIES|Exercise QUESTIONS FOR DESCRIPTIVE ANSWERS|37 Videos

Similar Questions

Explore conceptually related problems

It has been estimated that the total power radiated by the sun is 3.8 xx 10^(26) J per second . The source of energy of stars is a thermonucleur fission reaction . Energy released in the process of fusion is due to mass defect . Q = Delta mc^(2) In a nuclear reaction , ""_(1)^(2) H + ""_(1)^(2) H to ""_(2)^(3) He + ""_(0)^(1)n . if the masses of ""_(1)^(2) H & ""_(2)^(3) He are 2.014741 amu and 3.016977 amu respectively . then the Q-value of the reaction is nearly :

The binding energy par nucleon for deuterium (""_(1)^(2)H) and helium (""_(4)^(2)He) are 1.1 MeV and 7.0 MeV respectively. The energy released when two deutrons fuse to form a helium nucleus (""_(4)^(2)He) is K(10^(7)) MeV, where K= ……… (nearly)

It has been estimated that the total power radiated by the sun is 3.8 xx 10^(26) J per second . The source of energy of stars is a thermonucleur fission reaction . Energy released in the process of fusion is due to mass defect . Q = Delta mc^(2) B.E. per nucleon of ""_(1)^(2) H and ""_(2)^(4) He and 1.1 MeV and 7 MeV respectively . If two deutrons nuclei react to form a single helium nucleus , then the energy released is :

Consider the D - T reaction (deuterium - tritium fusion) ._(1)^(2)H+ ._(1)^(3)H to ._(2)^(4)He + n Calculate the energy released in MeV in this reaction from the data : m(._(1)^(2)H)=2.014102 u m(._(1)^(3)H)=3.016049 u

The mass defect in a particular nuclear reaction is 0.3 g. The amount of energy liberated, in kWh is (velocity of light = 3 xx 10^(8) ms^(-1) .