When NASA’s Mars rover Curiosity touched down inside Gale Crater in August 2012, it did so in dramatic fashion. In the final stages of its daring descent, the rover’s rocket-powered landing platform — known as a sky crane — lit up and blasted the dusty surface, carving out darkened divots before separating from the rover and flying out of harms way.
Over the months and years after landing, the High-Resolution Imaging Science Experiment (HiRISE) camera on board NASA’s Mars Reconnaissance Orbiter has been keeping track of changes around Curiosity’s landing zone (named “Bradbury Landing”), the crash site of the sky crane and the parachute-endowed back-shell that slowed the rover’s entry into the Martian atmosphere.
After disturbing the ruddy regolith on the Martian surface, usually, over time, the darkened area is expected to fade, slowly returning to its natural state. But recent HiRISE imagery of four components of Curiosity’s landing have faded inconsistently, potentially revealing a previously unknown Mars surface dynamic.
“Spacecraft like Curiosity create these dark blast zone patterns where bright dust is blown away by the landing,” said Ingrid Daubar, a HiRISE team scientist at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “We expected to see them fade as the wind moved the dust around during the months and years after landing, but we’ve been surprised to see that the rate of change doesn’t appear to be consistent.”
These followup observations are, in part, useful for NASA’s next Mars mission, InSight, that will launch in 2016. The InSight lander will deploy a probe that will be hammered a few meters into the ground to measure the heat traveling through the planet’s crust.
Any darkening of the surface is therefore really important for planetary scientists to understand. The darker the surface, the more sunlight that surface will absorb. The brighter the surface is, the more light is reflected and therefore less heating occurs.
From Discovery News
No comments:
Post a Comment