Task 2: Calculating the Average Distance from Kepler 452b to its Star
Scientists work hard to get unedited data like this:
Into a form that’s easier to read like this:
Can you identify the signature “bucket” shape of a transiting planet around the red line in the graph above? Check the image below for an example of the “bucket” shape.


As you may remember from the light curve video, we need “periodic and consistent dips in the light curve” to study our planet. Simply observing one transit is not enough because it could be an outlier. The more transits we observe, the more accurate our scientific findings will be.

This is a graph of the same star taken over several years during the Kepler mission. Each red line indicates a mid-transit point.
Using the multi-transit graph above, follow the same steps we used in the practice to find the period of your planet and distance from its star.
Input the values for each transit in cells B2, B3, B4, and B5 of the Google Sheet. The period of the planet will be calculated automatically in cell B6 in units of Earth years.
Using the multi-transit graph above, follow the same steps we used in the practice to find the period of your planet and distance from its star.
Input the values for each transit in cells B2, B3, B4, and B5 of the Google Sheet. The period of the planet will be calculated automatically in cell B6 in units of Earth years.
You will share the planet period with the following team:
If the Mass team has already requested the planet period, send it in the chat now. If the Mass team has not yet sent a request, be prepared to send the information when the request arrives.

Receive Mass of Star from Host Star Team

Now that we have the period, we are ready to calculate the distance of the exoplanet from its host star using Kepler’s Third Law. We will use the following variables:

First, check in with the Host Star team to get the mass of the star Kepler 452.
Send the following message in the chat.

Wait here until you receive the star mass.
While you wait... did you know?

Once you receive the star mass, send the following message to the Host Star team.
“Period team to Host Star team. Data received. Thank you.”
Then, input the value you received for star mass in cell B3 of the Google Sheet below. Kepler 452b’s distance from its host star will be calculated automatically in units of AU in cell B4 of the Google Sheet.
Then, input the value you received for star mass in cell B3 of the Google Sheet below. Kepler 452b’s distance from its host star will be calculated automatically in units of AU in cell B4 of the Google Sheet.


Great work! Now that we have the distance of the planet, Kepler 452b, from its star, Kepler 452, it is time to determine if the planet is in the habitable zone.