Home
Class 12
CHEMISTRY
The source of energy of stars is nuclear...

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about `10^(7) `. Energy released in the process of fusion is due to mass defect. It is also called `Q`-value. `Q = Delta mc^(2), Delta m =` mass defect.
Fusion reaction takes place at about a)`9 xx 10^(2) K` b)`3 xx 10^(3) K` c)`3 xx 10^(4) K` d)`3 xx 10^(4) K`

A

`3 xx 10^(2) K`

B

`3 xx 10^(3) K`

C

`3 xx 10^(4) K`

D

`3 xx 10^(6) K`

Text Solution

Verified by Experts

The correct Answer is:
d
Promotional Banner

Topper's Solved these Questions

  • RADIOACTIVITY AND NUCLEAR TRANSFORMATION

    OP TANDON|Exercise psg-VII|5 Videos
  • RADIOACTIVITY AND NUCLEAR TRANSFORMATION

    OP TANDON|Exercise psg-VIII|5 Videos
  • RADIOACTIVITY AND NUCLEAR TRANSFORMATION

    OP TANDON|Exercise psg-V|3 Videos
  • ORGANIC COMPOUNDS CONTAINING NITROGEN

    OP TANDON|Exercise Single integer|8 Videos
  • SATURATED ALIPHATIC HYDROCARBONS

    OP TANDON|Exercise SINGLE INTEGER ANSWER TYPE QUESTIONS|7 Videos

Similar Questions

Explore conceptually related problems

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. Mass equivalent to the energy 931 MeV is

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. A star has 10^(40) deutrons. It produes via the process ._(1)H^(2) + ._(1)H^(2) rarr ._(1)He^(3) + ._(1)H^(1) ._(1)H^(3) + ._(1)H^(3) rarr ._(2)He^(4) + ._(0)n^(1) If the average power radiated by the star is 10^(16) W , when the deutron supply of the star is exhausted in a time of the order of

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. In a nuclear reaction ._(1)H^(2) + ._(1)H^(2) rarr ._(2)He^(3) + ._(0)n^(1) If the masses of ._(1)H^(2) and ._(2)He^(3) are 2.014741 and 3.016977 amu, respectively. then the Q -value of the reaction is nearly.

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. The binding energy per nucleon of ._(1)H^(2) and ._(2)He^(4) are 1.1 MeV and 7 MeV , respectively. If two deuteron nuclei react to form a single helium nucleus, then the energy released is

In sun and other stars, where temperature is about 10^(7) K fusion, takes place dominatly by:

In botter star where the temperature is about 10^(8)K , fusion takes place3 and the cyclic is known as:

if in a nuclear fusion reaction, mass defect to 0.3% , then energy released in fusion of 1 kg mass

In a nuclear explosion, one kg uranium was used. The energy released during the explosion is E//2 xx 10^13 J if m ass defect involved in the fusion is 0.2%. Find the value of E/2.