2.64 x 10 K and a radius Teegarden b orbits around has a surface temperature of Ttar = star (as we did in the class for Sun). Also, you do not need to consider any atmospheric equal to 3.78 x 10° m. As a hint it may help to calculate first the radiation power of that distance of Teegarden b from its star to be 0.0252 au ("astronomical units") which is Ratar of 8.9 x 10" m. Take the emissivity of that star to be e = 1. Take the (averaged) temperature on the surface of Teegarden b is over the course of its year? The star that may be hosted. An interesting candidate is "Teegarden b". Calculate what the averaged 3. We are searching for planets outside our Solar System (exoplanets), where life a. a. conditions on Teegarden b '. 2.3 x 102 K 2.9 x 102 K 4.1 x 102 K 5.4 x 102 K a. b. C. d.

2.64 x 10 K and a radius Teegarden b orbits around has a surface temperature of Ttar = star (as we did in the class for Sun). Also, you do not need to consider any atmospheric equal to 3.78 x 10° m. As a hint it may help to calculate first the radiation power of that distance of Teegarden b from its star to be 0.0252 au ("astronomical units") which is Ratar of 8.9 x 10" m. Take the emissivity of that star to be e = 1. Take the (averaged) temperature on the surface of Teegarden b is over the course of its year? The star that may be hosted. An interesting candidate is "Teegarden b". Calculate what the averaged 3. We are searching for planets outside our Solar System (exoplanets), where life a. a. conditions on Teegarden b '. 2.3 x 102 K 2.9 x 102 K 4.1 x 102 K 5.4 x 102 K a. b. C. d.