| タイトル | Radiolytic Impacts of Energetic Electron Irradiation on Enceladus and Mimas |
| 本文（外部サイト） | http://hdl.handle.net/2060/20110023338 |
| 著者（英） | Sturner, S. J.; Sittler, E. C.; Cooper, J. F. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2011-01-01
2011 |
| 言語 | eng |
| 内容記述 | Episodic overturn of the south polar terrain on Enceladus would convey radio lytic oxidants from surface irradiation by Saturn's inner magnetospheric electrons to the putative underlying polar sea and contribute to CO2 and other gas production driving the visibly active cryovolcanism. Low duty cycle of active episodes below 1 - 10 percent would raise the relative importance of the continuous radiolytic chemical energy input for mass and heat outflow, e.g. as compared to heating by gravitational tides. The "Pac-Man" thermal anomaly on Mimas most likely arises from leading-trailing asymmetry of electron irradiation and resultant radio lytic processing of the moon ice to a few centimeters of depth. The Mimas thermal anomaly distribution suggests a relatively stable surface unmodified by Enceladus-like geologic overturn or cryovolcanic activity. In both cases, the heavily irradiated skin depth corresponds to the sensible thermal layer probed by Cassini infrared measurements. Neutral gas and dust emissions from Enceladus limit energetic ion and plasma electron fluxes in the inner magnetosphere, thereby governing the irradiation of Mimas and other Saturn moons. |
| NASA分類 | Astronomy |
| レポートNO | GSFC.ABS.5450.2011 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
