You can solve this using Kepler's 3rd law. T is proportional to r^1.5. T(J) = T(E)*5.2^1.5 = 11.86 years.
<span>You can also solve it the hard way: Find M (sun's mass) and r(Jupiter's orbital radius) in m. Then use Kepler's equation T = 2pi*r^1.5/sqrt(GM).</span>
The particles released during alpha decay are called alpha particles. Alpha particles have greater mass and charge than other emitted particles.
- Radioactive emissions are the transfer of energy through the flow of particles or waves in a medium
- There are 3 types of radioactive emissions which are alpha, beta and gamma
- In alpha radiation, the nucleus emits an alpha particle which is equivalent to a helium nucleus
- In beta radiation, an electron is emitted to convert a neutron to a proton
- In gamma radiation, the nucleus just loses energy
Since alpha particles have more mass and charge, they are more ionising and lose more energy at a faster rate and can be blocked easily.
Learn more about alpha decay emissions here:
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Here is the answer to the given question above. <span>The majority of supercell thunderstorms move to the right of the mean layer wind. This tendency is the result of differences in barometric pressure that develop as vertical wind shear interacts with the storm's updraft. In response to this vertical wind shear, an area of low pressure develops in the upper region of the down shear (right) side of the storm's updraft. In contrast, a region of relatively higher pressure forms on the other side of the updraft in the up shear portion of the storm. The region of low pressure on the right side of the updraft creates a favorable environment for propagation of the storm and, in response, it moves to the right.</span>
Answer:
Nuclear energy is not limited to the generation of electricity, but may equally well be used for such important tasks as desalination, production of hydrogen, space heating and process-heat applications in industry as well as for extraction of carbon from CO2 to combine with hydrogen to create synthetic liquid fuels.
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