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In addition to the nominal observations, the Hope detector has also uncovered new observations. The latest release includes new observations from the Emirates Mars Ultraviolet Spectrometer (EMUS) to better cover the auroras. The EMUS instrument was also able to successfully observe solar energetic particles and galactic cosmic rays through detector background monitoring. Additionally, as part of the detector characterization experiments, EMUS observed the ability to operate at higher gains, making it more sensitive to observations.
Hope Probe’s Emirates Exploration Imager (EXI) camera also observed high-rhythm clouds on December 24, 2021; and January 7-25 this year.
EMM Program Director Eng. “The new observations are a testament to the quality of the Hope Probe in advancing critical research and insights into Mars and its atmosphere, and we are delighted to share the latest observations with the global scientific community,” said Omran Sharaf.
“As the probe continues its planned mission to orbit Mars, we will continue to find ways to enrich our discoveries and observations beyond our mission and further enhance the international community’s understanding and understanding of Mars’ orbit,” Sharaf noted. “The Red Planet and strengthen the UAE’s position in the global space sector. “
Hessa Al Matroushi, Head of Science at EMM, added: “The recent reporting by the Mars Hope rover is a huge feat, proving the limitless potential of our instrument to achieve science beyond what it was designed for. The latest on Mars and its atmosphere. The insights reaffirm that there is much to be discovered, and we look forward to seeing the mission’s goals of providing useful scientific data, enhancing national capabilities and fostering global collaboration blossom with each new data collected.”
According to EMM, Hope Probe’s orbit is between 20,000 and 43,000 kilometers, tilted 25 degrees toward Mars, giving it the unique ability to orbit Earth every 55 hours, capturing comprehensive data every 9 days.
The Hope rover is studying the current state of Mars’ atmosphere and weather, and why hydrogen and oxygen are escaping from its upper atmosphere. It is also studying the relationship between Mars’ upper and lower atmospheres and various other phenomena such as dust storms, weather variability and atmospheric dynamics.
The fourth batch of information and data is shared with the scientific community and astronomers from around the world through the data center on the project’s website, which is released every three months, after the data captured by the detector’s instruments is catalogued and processed by the project’s team .
The first, second and third batches of data have received great interest from scientists, researchers, experts and astronomy enthusiasts from all over the world. To date, 1.7 TB of data has been downloaded.
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