Chelen Johnson
Hertzsprung-Russel diagram for Active Galactic Nuclei (HR4AGN): Using space and ground based ultraviolet, optical, and infrared images to find a correlation between the color and luminosity of gas emission and dust emission around supermassive black holes at the centers of galaxies.
My NITARP experience has made me rethink my entire approach to science education. Many of my students expect me to do the work and pretty much hand it to them all wrapped up and neat. Science education must involve a great deal of discovery by the student and not a string of topics with definitions.
It was very special to be in the room when the announcement of planet Kepler 10b (an estimated 1.4 X the size of the Earth) was discovered. I turned to my student Inga and asked, "How does it feel to be one of the first people on planet Earth to know about this discovery?" She replied, "I never thought of it like that ... it's pretty cool."
I think the best part about the trip and NITARP as a whole is the chance to do authentic research and learn the methods and techniques used to tease as much information out of the data as possible. It still amazes me (and this is what I try to instill in the students in my astronomy classes) that we can learn so much from a tiny point of light if we are just clever enough to know how to look at it.
