NASA is now preparing its Mars Atmosphere and Volatile Evolution (MAVEN) and InSight missions to research the planet’s atmosphere and rock. Meanwhile, the European Space Agency and Russia’s Roskosmos space agency also plan a detailed probe into Martian atmosphere to possibly answer if there is life on the planet.
The DAN spectrometer was switched on in mid-August and though it is still in test flight mode, the experiments have already begun.
Their first results have been reported at the third Moscow international Solar System Symposium arranged by the Space Research Institute of the Russian Academy of Sciences. The data were presented by Maxim Litvak, the head of the space gamma-ray spectroscopy lab at the Space Research Institute.
DAN revealed that the amount of hydrogen in Mars rock where the rover landed was surprisingly small- corresponding to the mass of 1-2% of water. These results contradict the previously obtained data by Russia’s HAD High Energy Neutron Detector HEND installed at the2001 Mars Odyssey robotic spacecraft.
The HEND-generated maps show that the rover’s landing area in the Gale Crater could rather be considered humid (5-6% of water).
However, the new results could be explained. HEND’s spatial resolution is hundreds of kilometers while DAN is able to measure hydrogen level directly under the rover.
This shows that water ice distribution in Mars rock is more complex than it was thought, so finer research methods are needed, like the Curiosity mission.
New projects also take this necessity into account - MAVEN, InSight, ExoMars
(collaboration between the European Space Agency and Roskosmos) as well as projects by other countries.
Their scientific goals are somewhat common – to research the planet’s development and find out why it lost its magnetic field and water and is or was there any life on the planet.
The answers lie in the planet’s atmosphere and geology, the distribution of water ice and minerals on the surface and upper layers of the rock.
All researchers dream of landing on the planet and expect to do it in the 2020s. Now, space agencies are working on less complicated projects to bring rock from the Red Planet to Earth.
Russia puts a stake on the ExoMars project that is to be sealed this November. The ExoMars Trace Gas Orbiter (TGO) is joint project to send a robotic orbiter-carrier to Mars in 2016.. The TGO would deliver the ExoMars EDM stationary lander and then proceed to map the sources of methane and other gases on Mars
Russia will equip the lander with two Atmospheric Chemistry Suite (ACS) spectrometers and fine resolution neutron detector (FREND) spectrometer for the search of subsurface water on the planet.
The first stage of the project will also feature a demo Entry Descent and Landing (MEDLI) Suite. It was also planned to have Russian equipment but plans the idea was dropped due to limited timeframe.
The instrument is to test out soft touchdown technologies and though it has equipment to study Mars’ atmosphere and life it can’t be called a full-fledge research space craft as its equipment will not last longer than 2-4 days.
The second stage of the mission is the launch of Pasteur payload in 2018. Russia will supply Proton booster for to deliver the ExoMars rover onto the Martian surface and another set of instruments on the stationary landing platform
Pasteur will also be equipped with Infrared Surface Emissivity Model(ISEM) and ADRON (Active Detector of gamma Rays and Neutrons). The engineers are open for other suggestions.
According to head of the Institute for Space Research Lev Zelyony, ExoMars is also a great chance to practice joint mission control for further collective missions which is also crucial for the research.
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