This week we created two new programs, one of which calculates the total stellar flux by sorting through a list of stars and their data. This program also lets us calculate at what distance surrounding a star would a planet be in the liquid water habitable zone. Our second program is the starting point of our newest model, which is getting the temperature of a star based solely on two data point, the B and the V stellar flux filters. 
Semper Discemus
BASIS Tucson North Senior Project Blog 