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Mars Science Lab Detects Solar Burst’s Effects

January 30, 2012

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The largest solar particle event since 2005 hit the Earth, Mars and the Mars Science Laboratory spacecraft travelling in-between, allowing the onboard Radiation Assessment Detector to measure the radiation a human astronaut could be exposed to en route to the Red Planet.

On Sunday, a huge coronal mass ejection erupted from the surface of the sun, spewing a cloud of charged particles in our direction, causing a strong “S3″ solar storm. A NASA Goddard Space Weather Lab animation of the CME illustrates how the disturbance impacts Earth, Mars and several spacecraft. Solar storms can affect the Earth’s aurorae, satellites, air travel and GPS systems; no harmful effects to the Mars Science Laboratory have been detected from this solar event.

“We only have a few hours of data downloaded from the RAD so far, but we clearly see the event, said RAD Principal Investigator Don Hassler, science program director in the Space Studies Department at Southwest Research Institute. The Mars Science Laboratory, launched Nov. 26, will land a sophisticated car-sized rover called Curiosity on the surface of the planet in August. Loaded with 10 instruments including RAD, Curiosity will traverse the landing site looking for the building blocks of life and characterizing factors that may influence life, such as the harsh radiation environment expected on Mars. “This SPE encounter is particularly exciting in light of the alignment between the Earth, MSL and Mars right now and for the next few months. It will be very interesting to compare the RAD data, collected from inside the capsule, with the data from other spacecraft.”

This event has also been seen by the Solar Dynamics Observatory, Geostationary Operational Environment Satellites, the Advanced Composition Explorer, and the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft in Earth orbit as well as the Solar Heliospheric Observatory (SOHO) flying between Earth and the sun.

“RAD was designed to characterize radiation levels on the surface of Mars, but an important secondary objective is measuring the radiation during the almost nine-month journey through interplanetary space to prepare for future human exploration,” said Hassler. “RAD is an important bridge between the science and exploration sides of NASA.

“Not only will this give us insight into the physics of these giant clouds, but like an astronaut, RAD is tucked inside the MSL ‘spacecraft,’” Hassler continued. “Measurements from RAD will give us insight about the shielding provided by spacecraft for future manned missions in deep space.”

RAD will collect data nearly continuously during cruise and will downlink data every 24 hours. Positioned in the front-left corner of the rover, the instrument is about the size of a coffee can and weighs about three pounds, but has capabilities of an Earth-bound instrument nearly 10 times its size. When MSL arrives at Mars, RAD will detect charged particles arriving from space and will measure neutrons and gamma rays coming from Mars’ atmosphere above, or the surface material below, the rover.

SwRI, together with Christian Albrechts University in Kiel, Germany, built RAD with funding from the NASA Human Exploration and Operations Mission Directorate and Germany’s national aerospace research center, Deutsches Zentrum für Luft- und Raumfahrt.

The Mars Science Laboratory is a project of NASA’s Science Mission Directorate. The mission is managed by NASA’s Jet Propulsion Laboratory, a division of Caltech. The mission’s rover was designed, developed and assembled at JPL.

Image Caption: This is an artist’s concept of NASA’s Mars Science Laboratory spacecraft during its cruise phase between launch and final approach to Mars. The spacecraft includes a disc-shaped cruise stage (on the left) attached to the aeroshell. The spacecraft’s rover (Curiosity) and descent stage are tucked inside the aeroshell. Image credit: NASA/JPL-Caltech

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Source: Southwest Research Institute



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