Slurries Of Mud May Have Flowed In Martian Gullies. The Australia Broadcasting Corporation (11/2, Catchpole) reports, “Martian water most likely flowed as slurries of mud rather than trickling streams, according to a recent NASA report.” Jennifer Heldmann of the Ames Research Center analyzed pictures of the Terra Sirenum and the Centauri Montes regions of Mars, comparing them to similar patches of gully deposits in the Atacama Desert in South America. “This data revealed the light tone was caused by the difference in the size of the particles in the mudflows compared to the coarser-grained surrounding terrain.” Scientists “say this indicates the best way to look for water on Mars is not to look for differences in the composition of the sediments, but in the size of the particles.
- Icarus publication: Heldmann, J.L., Conley, C.A., Brown, A.J., Fletcher, L., Bishop, J.L., and C.P. McKay, Possible Liquid Water Origin for Atacama Desert Mudflow and Recent Gully Deposits on Mars, Icarus, doi:10.1016/j.icarus.2009.09.013 (2009).
- Radio interview with Dave Schlom regarding LCROSS on Northstate Public Radio, KCHO, 91.7 and KFPR, 88.9 FM (November 3, 2009).
- Mentor for student team from the Lego Robotics Club in Haslett, Michigan (sponsored by MSU College of Engineering), competing the FIRST Lego League Smart Move competition and working on a project related to LCROSS.
- Girl Scout Day at the SETI Institute: giving a talk on Planetary Science and helping mentor the students during afternoon science activities (November 7, 2009).