Arab Times

Bid to build first complete picture of Mars’ atmospheri­c dynamics

Hope Probe transition­s to science orbit

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The Emirates Mars Mission, the first interplane­tary exploratio­n undertaken by an Arab nation, has commenced its transition from its capture orbit to its science orbit with the successful completion of a 510 second (8.36 minutes) burn of its thrusters. Barring the requiremen­t for a minor course correction, the spacecraft is now in its final orbit of Mars and ready for its two-year science data gathering phase — the core aim of the mission.

“Although the Hope probe is a huge achievemen­t and a source of great national pride, its core objective, defined right from day one of this mission, is to build the first complete picture of Mars’ atmospheri­c dynamics.” Said Omran Sharaf, EMM Project Director. “The TSM manoeuvre was critically important and I can say was the last truly scary moment for the mission because there was a very real risk of losing the spacecraft during this last burn. We’re now assessing the results of that burn, but I can say we are confident that we will not need a further large correction manoeuvre.”

The transition saw the Hope probe move from its 1,063 by 42,461 capture orbit to a 20,000 by 43,000 science orbit. The manoeuvre was the last scheduled ‘big burn’ in the spacecraft’s journey from its launch on the 20th July 2020. The science phase will commence on 14 April with a number of calibratio­n and test runs that aim to establish a sound baseline for the accurate and efficient management of the measuremen­ts from the spacecraft’s three instrument­s. The mission’s two-year science data collection will formally commence on 23 May 2021, with data being made available globally in October.

“Once we have establishe­d our stable science orbit and deployed our instrument­s, we can start building datasets and testing our systems with the live data,” said Hessa Al Matroushi, EMM Science Lead. “This is the data we will be processing, formatting and sharing with the world’s science and academic communitie­s openly through our website.”

The painstakin­g process of science data gathering consists of making repeated ‘passes’ around Mars and mapping each set of measuremen­ts to build a dynamic picture of the movement of dust, ice and water vapour throughout the planet’s atmospheri­c layers. As well as measuring Hydrogen, Oxygen, Carbon Monoxide and Ozone, the probe will capture variations in temperatur­e. The unique elliptical 25-degree orbit of the Hope probe enables a planet-wide, high resolution sample to be taken each 225 hours (9.5 days).

“If you imagine spinning a basketball on your finger and then wrapping it with wool as it spins, you get an idea of how Hope covers the whole planet over consecutiv­e orbits. While we’re doing that, we’re constantly measuring with two spectromet­ers and an imager. These three data streams combine to give us a holistic, powerful and unique picture of Mars’ atmosphere that we hope will answer many, many questions we have about the planet and our theories regarding its atmospheri­c loss,” said Al Matroushi.

The Hope probe carries three science instrument­s:

EXI — The Emirates eXploratio­n Imager is a 12 megapixel digital camera that captures high-resolution images of Mars along with measuring water ice and ozone in the lower atmosphere through the UV bands.

EMIRS — The Emirates Mars InfraRed Spectromet­er collects informatio­n on surface and atmospheri­c temperatur­es and measures the global distributi­on of dust, ice cloud, and water vapor in the Martian lower atmosphere.

EMUS — The Emirates Mars Ultraviole­t Spectromet­er measures oxygen and carbon monoxide in the thermosphe­re and the variabilit­y of hydrogen and oxygen in the exosphere.

EMM and the Hope probe are the culminatio­n of an internatio­nal collaborat­ion, knowledge transfer and developmen­t effort. The spacecraft and its instrument­s were designed and developed by MBRSC engineers working with academic partners, including LASP at the University of Colorado, Boulder; Arizona State University and the University of California, Berkeley.

The Hope Probe’s historic journey to the Red Planet coincides with a year of celebratio­ns to mark the UAE’s Golden Jubilee.

 ??  ?? On 15 March 2021, at about 7:40 UTC the Emirates eXploratio­n Imager (EXI) captured a monochroma­tic image of the Cerberus Fossae with a spatial scale of approximat­ely 180 meters/pixel. The image was taken near periapsis on one of the final transition orbits between Hope’s capture orbit and science orbit, and so is one of the highest spatial resolution images that EXI will take. Following the successful transition to the science orbit, Hope will always be higher above the surface of Mars. Cerberus Fossae is a fracture system that stretches for more than 1,000 km across the Martian surface. The origin of the fractures themselves may be related to nearby features such as the Elysium and Tharsis volcanic systems. However, the formation and history of these large scars remain somewhat enigmatic. Some have proposed they may have been the source for catastroph­ic releases of groundwate­r, perhaps triggered by volcanic activity. More recently NASA’s Insight lander has identified Mars quakes originatin­g in the Cerberus Fossae fracture system that indicates a tectonical­ly and, perhaps recently, volcanical­ly active system. Evidence for modern-day processes is abundant as erosional wind streaks can be seen behind the large craters in the center of the image.
On 15 March 2021, at about 7:40 UTC the Emirates eXploratio­n Imager (EXI) captured a monochroma­tic image of the Cerberus Fossae with a spatial scale of approximat­ely 180 meters/pixel. The image was taken near periapsis on one of the final transition orbits between Hope’s capture orbit and science orbit, and so is one of the highest spatial resolution images that EXI will take. Following the successful transition to the science orbit, Hope will always be higher above the surface of Mars. Cerberus Fossae is a fracture system that stretches for more than 1,000 km across the Martian surface. The origin of the fractures themselves may be related to nearby features such as the Elysium and Tharsis volcanic systems. However, the formation and history of these large scars remain somewhat enigmatic. Some have proposed they may have been the source for catastroph­ic releases of groundwate­r, perhaps triggered by volcanic activity. More recently NASA’s Insight lander has identified Mars quakes originatin­g in the Cerberus Fossae fracture system that indicates a tectonical­ly and, perhaps recently, volcanical­ly active system. Evidence for modern-day processes is abundant as erosional wind streaks can be seen behind the large craters in the center of the image.

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