Slope Streaks in Acheron Fossae on Mars
Explanation:
What creates these picturesque dark streaks on Mars?
No one knows for sure.
A leading hypothesis is that streaks like these are caused by
fine grained
sand sliding down the banks of troughs and craters.
Pictured above,
dark sand appears to have flowed hundreds of meters down the slopes of
Acheron Fossae.
The sand appears to
flow
like a liquid around boulders, and, for some reason,
lightens significantly over time.
This
sand flow process is one of several which can rapidly change the surface of
Mars, with other processes including
dust devils,
dust storms, and the freezing and
melting of areas of ice.
The
above image
was taken by the
HiRise camera on board the
Mars Reconnaissance Orbiter which has been orbiting Mars since 2006.
Acheron Fossae
is a 700 kilometer long
trough in the
Diacria quadrangle
of Mars.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
