Space/Science — HabitableZone

Space/Science » in reply to Martian razorbacks solved

or not

Interesting hypothesis but optical spectra & Mossbauer tell a chemical story.
from VISIBLE/NEAR INFRARED SPECTRAL CHARACTERIZATION OF IN SITU ROCK OUTCROPS AT
MERIDIANI PLANUM AS OBSERVED BY THE MARS EXPLORATION ROVER OPPORTUNITY by Farrand et al (PSC , 2005, 2082.pdf) they state "Vein/coating materials were
observed at Endurance crater in association with such
features as “Razorback”... These
coating/fracture fill materials were characterized by a
shallow 900 nm absorption feature- very similar to that
observed in the “rind” material at Shoemakers Patio in
Eagle crater. Examples of these materials subjected to
in situ examination display a stronger inner Fe3+ doublet
in Mössbauer spectra . The same mineral
phase(s) could be responsible for both features; possibilities
include, but are not limited to, schwertmannite,
akaganeite or ferrihydrite." That to my mind suggests chemistry in involved, not jus physcal rearrangement of existing dust particles.

Log in or register to post.

The whole thread (2 posts)