Partill: Modeling the Sun (20 points) Now it's time to construct your two models. Carry out the plans you described in Part II. Then, write a
report that includes the following: (20 points)
• A description of the processes and/or stages illustrated in each model
• A list of the materials and references you used to design and construct each model
• An explanation of how you can use your models to explain how changes in the proportions of
hydrogen and helium affect the Sun's life cycle
• An evaluation of how well you incorporated evidence into each model
• A suggestion of how you might improve each model
Submit this completed worksheet, your models, and your report to your teacher on or before the due
date.

part 1: the half-life of the element is 22 years.

part 2: it will take 132.02 year for the sample to decay from 308.0 g to 4.8125 g.

explanation:

part 1: there are two ways to determine the half life time.

first way: the half life time can be determined directly from its definition as it is the time required for the sample to decay to its half concentration.

from the data the initial concentration was 45.0 g and decayed to its half value (22.5 g) in 22.0 years.

second way: the radio active decay is considered first order reaction so we can use the laws of first order reactions.

k = (1/t) ln (a/a-x), where k is the rate constant of the reaction,

t is the time of the reaction

a is the initial concentration of the reactant

a-x is the remaining concentration at time (t)

a = 45.0 g the initial concentration at t = 0 year.

at t = 22 year, a-x = 22.5 g

then k = (1/22 year) ln (45.0 g/ 22.5 g) = 0.0315 year-1.

the half-life time (t1/2) = ln 2/ k = 0.693/ k =0.693/ 0.0315 = 22 years.

part 2:

using the same law k = (1/t) ln (a/a-x),

using the given data; a = 308.0 g and a-x = 4.8125 g and the calculated k from the part 1 (k = 0.0315 year-1)

t = (1/k) ln (a/a-x) = (1/0.0315) ln (308.0/ 4.8125) = 132.02 years

i'm wiling to try and you : )