Charon ResearchMay 2, 2008
Another semester nearly done and I have hardly posted at all. I’ll do a full summary once grades are in. For now, my classes are essentially done (one more on Monday night). Now I just have to finish writing up the journal/log for my research project, which I just realized I have not actually talked about before. Fairly briefly, then…
My last research project (with advisor Dr. Shobita Satyapal), done in Spring 2007, was based predominantly on Spitzer Space Telescope (and some older) infrared observations of a variety of galaxies. In that project I did a fairly rough, low sample comparison of various methods of determining star formation rate in galaxies (infrared, UV, visible light, etc.). Ultimately, I determined that infrared was the way to go for a variety of reasons. I am not sure how valid my results were (this was all new to me), but I got some interesting reactions from Shobita and one of her grad students, so that’s a plus.
This time around, I am working with Dr. Michael Summers, as I mentioned in an earlier post. He is working up a paper discussing the possibility of Charon having an atmosphere and the composition, density and lifespan of that atmosphere, if present. While the great bulk of the work (and all the theory) is his (and a collaborator’s), he has had me running some mathematical models using the IDL programming language. Technically-speaking, I am not really doing Charon research for much of it, because a lot of the models I am running (like determining equilibrium vapor pressures for a variety of gases at very low temperatures) has nothing to do with Charon specifically. Some of it, my earlier work (I actually started this work last May), used Charon parameters, however, so that qualifies. (Current direction of conclusions: yes, Charon most likely does have an atmosphere, which is picks up in part from Pluto’s evaporation while it is near enough to the sun.)
Since it is not really a full research project (I have no theory, no position, not much of anything), I am not sure how he will be grading it – hopefully just grading the quality of the programming output I did plus whatever journal I write up talking about my adventures making the models. He has used at least one of my output plots in a talk he gave to other atmospheric sciences, so I can’t be too far off in my models.
One thing I have learned about doing this research is that advisors are very hard to contact! Both of my advisors have been very out of the loop with my daily activities. In Shobita’s case, she delegated pretty much all of my handling to one of her post-docs. She was out of it enough that my conclusions were a surprise to her – she had not inquired as to my progress for many weeks prior to the final paper. I still have not gotten my graded paper back from her after almost a year of asking. In Mike’s case, he is a very busy man – two active NASA missions (New Horizons, AIM), one hopefully soon-to-be-approved mission (ARES) as well as papers he is working on and his class time. It is lucky for me I am sitting in on his atmospheric physics class this semester – it gives me 10 minutes each week to talk to him on our way to the parking lot after class! He apparently has a good number of grad students (like 6-8) working for him, although I only know two of them – neither of which gets much face time either, so at least I know it is not just me.