Lia1228
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\begin{tabular}{|c|c|c|c|}
\hline
\begin{tabular}{l}
Exoplanet \\
Name
\end{tabular} & \begin{tabular}{l}
Mass of \\
Host Star \\
(solar \\
masses)
\end{tabular} & \begin{tabular}{l}
Period of \\
Revolution \\
(Earth \\
years)
\end{tabular} & \begin{tabular}{l}
Average \\
Distance from \\
Host Star \\
(AU)
\end{tabular} \\
\hline
\begin{tabular}{l}
Kepler 79 \\
b
\end{tabular} & 1.165 & 0.0369 & 0.116 \\
\hline
\begin{tabular}{l}
Kepler 36 \\
b
\end{tabular} & 1.071 & 0.0379 & [tex][tex]$0.115$[/tex][/tex] \\
\hline
\begin{tabular}{l}
Kepler 18 \\
b
\end{tabular} & 0.972 & 0.00962 & [tex][tex]$0.0448$[/tex][/tex] \\
\hline
\begin{tabular}{l}
Kepler \\
186 b
\end{tabular} & 0.544 & 0.356 & [tex][tex]$\sim 0.116$[/tex][/tex] \\
\hline
\begin{tabular}{l}
Kepler \\
[tex][tex]$442 f$[/tex][/tex]
\end{tabular} & 0.61 & 0.3075 & [tex][tex]$\sim 0.442$[/tex][/tex] \\
\hline
\begin{tabular}{l}
HD \\
17156 b
\end{tabular} & 1.275 & 0.05813 & [tex][tex]$\sim 1.7156$[/tex][/tex] \\
\hline
\begin{tabular}{l}
HD 20782 \\
b
\end{tabular} & 1.43 & 1.605 & [tex][tex]$\sim 2.0782$[/tex][/tex] \\
\hline
\begin{tabular}{l}
Trappist 1 \\
b
\end{tabular} & 0.089 & 0.0252 & [tex][tex]$\sim 1.0$[/tex][/tex] \\
\hline
\end{tabular}



Answer :

Certainly! Let's analyze and compile the provided data on the exoplanets in a structured manner.

### 1. Data Compilation

We need to compile a structured table containing the following columns:
- Exoplanet Name
- Mass of Host Star (in solar masses)
- Period of Revolution (in Earth years)
- Average Distance from Host Star (in Astronomical Units, AU)

### 2. Extracting and Arranging Data

Based on the provided data, we compile the table as follows:

#### Kepler 79 b
- Mass of Host Star: 1.165 solar masses
- Period of Revolution: 0.0369 Earth years
- Average Distance from Host Star: 0.116 AU

#### Kepler 36 b
- Mass of Host Star: 1.071 solar masses
- Period of Revolution: 0.0379 Earth years
- Average Distance from Host Star: 0.115 AU

#### Kepler 18 b
- Mass of Host Star: 0.972 solar masses
- Period of Revolution: 0.00962 Earth years
- Average Distance from Host Star: 0.0448 AU

#### Kepler 186 b
- Mass of Host Star: 0.544 solar masses
- Period of Revolution: 0.356 Earth years
- Average Distance from Host Star: Not Available (None)

#### Kepler 442 f
- Mass of Host Star: 0.61 solar masses
- Period of Revolution: 0.3075 Earth years
- Average Distance from Host Star: Not Available (None)

#### HD 17156 b
- Mass of Host Star: 1.275 solar masses
- Period of Revolution: 0.05813 Earth years
- Average Distance from Host Star: Not Available (None)

#### HD 20782 b
- Mass of Host Star: 1.43 solar masses
- Period of Revolution: 1.605 Earth years
- Average Distance from Host Star: Not Available (None)

#### Trappist 1 b
- Mass of Host Star: 0.089 solar masses
- Period of Revolution: 0.0252 Earth years
- Average Distance from Host Star: Not Available (None)

### 3. Compiled Table

[tex]\[ \begin{array}{|c|c|c|c|} \hline \text{Exoplanet Name} & \text{Mass of Host Star (solar masses)} & \text{Period of Revolution (Earth years)} & \text{Average Distance from Host Star (AU)} \\ \hline \text{Kepler 79 b} & 1.165 & 0.0369 & 0.116 \\ \hline \text{Kepler 36 b} & 1.071 & 0.0379 & 0.115 \\ \hline \text{Kepler 18 b} & 0.972 & 0.00962 & 0.0448 \\ \hline \text{Kepler 186 b} & 0.544 & 0.356 & \text{None} \\ \hline \text{Kepler 442 f} & 0.61 & 0.3075 & \text{None} \\ \hline \text{HD 17156 b} & 1.275 & 0.05813 & \text{None} \\ \hline \text{HD 20782 b} & 1.43 & 1.605 & \text{None} \\ \hline \text{Trappist 1 b} & 0.089 & 0.0252 & \text{None} \\ \hline \end{array} \][/tex]

### Explanation of Table
- Exoplanet Name: This column lists the names of various exoplanets.
- Mass of Host Star (solar masses): This column indicates the mass of the star hosting the exoplanet, measured in solar masses.
- Period of Revolution (Earth years): This column specifies the period it takes for the exoplanet to complete one orbit around its host star, measured in Earth years.
- Average Distance from Host Star (AU): This column shows the average distance of the exoplanet from its host star, measured in astronomical units (AU). If the distance data is unavailable, it is marked as "None".

We have now successfully compiled and explained the tabulated data based on the provided information.

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