Helpful Scripts
- Signal to Noise Calculator - This script will calculate the bandwidth and signal to noise ratio for an NEO of known size, distance, and rotation period.
Manuscript Pre-Prints
- Revisiting the Phoenix TECP data: Implications for regolith control of near-surface humidity on Mars
- Constraints on planetesimal disk mass from the cratering and equatorial ridge on Iapetus
- Estimating the size of late veneer impactors from impact-induced mixing on Mercury
- Impact-induced compositional variations on Mercury
Data Products
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Fun gif of Iapetus being bombarded overtime. The colors represent the number of times an area on the surface has been excavated by an impact. Red is 10 times while dark blue is 0 times. This simulation is for a classic Nice Model bombardment of Iapetus. |
Map of the thermal inertia of Iapetus (Rivera-Valentin et al., 2011). The colors represent the magnitude of the thermal inertia in J m-2 K-1 s-1/2. Thermal inertia is a property of a material and characterizes how efficiently it holds onto thermal energy (i.e, heat).