Mars Exploration News  
MARSDAILY
Oxia Planum favoured for ExoMars surface mission
by Staff Writers
Paris (ESA) Nov 12, 2018

The two candidates for the landing site of the ESA-Roscosmos rover and surface science platform. The study area of each landing site is indicated by the black outline; the shape corresponds to the different landing ellipses defined by factors such as different launch dates within the launch window and, in the case of Mawrth Vallis, local topography constraints resulting in different landing ellipse centres depending on the launch date.

The map is colour-coded corresponding to elevation: whites and reds are higher than yellows and greens. The data was obtained by the Mars Orbiter Laser Altimeter onboard NASA's Mars Global Surveyor.

Both landing site candidates lie close to the transition between the cratered northern highlands and the southern lowlands of Mars. They lie just north of the equator, in a region with many channels cutting through from the southern highlands to the northern lowlands. As such, they preserve a rich record of geological history from the planet's wetter past, billions of years ago.

The ExoMars Landing Site Selection Working Group has recommended Oxia Planum as the landing site for the ESA-Roscosmos rover and surface science platform that will launch to the Red Planet in 2020.

The proposal will be reviewed internally by ESA and Roscosmos with an official confirmation expected mid-2019.

At the heart of the ExoMars programme is the quest to determine if life has ever existed on Mars, a planet that has clearly hosted water in the past, but has a dry surface exposed to harsh radiation today.

While the ExoMars Trace Gas Orbiter, launched in 2016, began its science mission earlier this year to search for tiny amounts of gases in the atmosphere that might be linked to biological or geological activity, the rover will drive to different locations and drill down to two metres below the surface in search of clues for past life preserved underground. It will relay its data to Earth through the Trace Gas Orbiter.

Both landing site candidates - Oxia Planum and Mawrth Vallis - preserve a rich record of geological history from the planet's wetter past, approximately four billion years ago. They lie just north of the equator, with several hundred kilometres between them, in an area of the planet with many channels cutting through from the southern highlands to the northern lowlands. Since life as we know it on Earth requires liquid water, locations like these include many prime targets to search for clues that may help reveal the presence of past life on Mars.

"With ExoMars we are on a quest to find biosignatures. While both sites offer valuable scientific opportunities to explore ancient water-rich environments that could have been colonised by micro-organisms, Oxia Planum received the majority of votes," says ESA's ExoMars 2020 project scientist Jorge Vago.

"An impressive amount of work has gone into characterising the proposed sites, demonstrating that they meet the scientific requirements for the goals of the ExoMars mission. Mawrth Vallis is a scientifically unique site, but Oxia Planum offers an additional safety margin for entry, descent and landing, and for traversing the terrain to reach the scientifically interesting sites that have been identified from orbit."

The Landing Site Selection Working Group also emphasised that the discoveries generated during the landing site selection process are essential to guide the science operations of the ExoMars rover.

The recommendation was made following a two-day meeting held at the National Space Centre in Leicester, UK, which saw experts from the Mars science community, industry, and ExoMars project present and discuss the scientific merits of the sites alongside the engineering and technical constraints.

The quest to find the perfect landing site began almost five years ago, in December 2013, when the science community was asked to propose candidate locations. Eight proposals were considered in the following April, with four put forward for detailed analysis in late 2014.

In October 2015, Oxia Planum was identified as one of the most compatible sites with the mission requirements - at that time with a 2018 launch date in mind - with a second option to be selected from Aram Dorsum and Mawrth Vallis. In March 2017, the down-selection identified Oxia Planum and Mawrth Vallis as the two candidates for the 2020 mission, with both undergoing a detailed evaluation over the last 18 months.

On the technical side, the landing site must be at a suitably low elevation level, so that there is sufficient atmosphere and time to help slow the landing module's parachute descent. Then, the 120 x 19 km landing ellipses should not contain features that could endanger the landing, the deployment of the surface platform ramps for the rover to exit, and the subsequent driving of the rover. This means scrutinising the region for steep slopes, loose material and large rocks.

On the science side, the analysis had to identify sites where the rover could use its drill to retrieve samples from below the surface, and to define possible traverses it could make up to 5 km from its touchdown point in order to reach the maximum number of interesting locations.

Oxia Planum lies at the boundary where many channels emptied into the vast lowland plains. Observations from orbit show that the region exhibits layers of clay-rich minerals that were formed in wet conditions some four billion years ago, likely in a large body of standing water.

The channels that transported material into the lower-elevation 'sink', where the landing ellipse is situated, cover an area of 212 000 square kilometres. Layers of material that have been recently exposed through erosion are accessible from any of the touchdown points, giving a window into the early history of this area.

The minerals in Oxia Planum are representative of those found in a wide area around the region and so would provide insight into the conditions experienced at a global scale, putting constraints on the climate and habitability potential of Mars in this period.

Diverse aqueous episodes were followed by late volcanic activity, covering over the clay-rich deposits. Some lava material has resisted erosion until today, so the underlying materials may only have been exposed recently, initially protecting them from space radiation and later making them accessible to the rover and its analytical tools.

The landing ellipse has low elevation and contains very few topographic obstacles or challenging slopes.

The ESA-led rover and Roscosmos-led surface science platform will launch in the 25 July-13 August 2020 launch window on a Proton-M rocket from Baikonur, Kazakhstan, and cruise to Mars in a carrier module containing a single descent module, arriving at Mars 19 March 2021.

The descent module will separate from the carrier shortly before reaching the martian atmosphere, and will use two large parachutes, along with thrusters and a damping system, to slow its descent to land on the Red Planet. While the rover will drive to different locations to analyse the surface and subsurface, the stationary platform will provide context imaging at the landing site, and long-term climate monitoring and atmospheric investigations.

The test campaign for preparing the rover for Mars is in full swing. The rover structural and thermal model test campaign has been successfully completed, and a six-week qualification test on the Analytical Laboratory Drawer - the onboard laboratory where the rover's drill samples will be processed and analysed - is also nearing completion. The test included verifying the functionality of the sample processing mechanisms using Mars analogue samples under simulated Mars environment conditions - a low pressure, carbon dioxide atmosphere and a range of temperatures.

Tests to characterise the rover's ability to tackle different types of terrain are also ongoing with the locomotion verification model. The delivery of flight hardware has also started, including the rover's computer, battery and deployable mast, along with the majority of science instruments.

"Our ExoMars mission combines extreme performance with the novel design features of the rover, and we are looking forward to operating the first European mission on the surface of Mars," says Francois Spoto, ExoMars Programme team leader.

"Landing on Mars has a long chain of risks, but thanks to the combined skills and expertise of European and Russian industries working with reliable technologies, we are focused on a safe landing."

More information about the Landing Site Selection Working Group is available here.


Related Links
ExoMars at ESA
Mars News and Information at MarsDaily.com
Lunar Dreams and more


Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Contributor
$5 Billed Once


credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly


paypal only


MARSDAILY
ExoMars orbiter highlights radiation risk for Mars astronauts
Berlin, Germany (ESA) Sep 19, 2018
Astronauts on a mission to Mars would be exposed to at least 60% of the total radiation dose limit recommended for their career during the journey itself to and from the Red Planet, according to data from the ESA-Roscosmos ExoMars Trace Gas Orbiter being presented at the European Planetary Science Congress, EPSC, in Berlin, Germany, this week. The orbiter's camera team are also presenting new images of Mars during the meeting. They will also highlight the challenges faced from the recent dust stor ... read more

Comment using your Disqus, Facebook, Google or Twitter login.



Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

MARSDAILY
European-built Service Module arrives in US for first Orion lunar mission

Roscosmos to Study Possibility to 3D Print Lunar Soil Details for Space Repairs

First moon walk's commemorative plaque sold for $468,500

Neil Armstrong's huge souvenir collection to be auctioned

MARSDAILY
China unveils new 'Heavenly Palace' space station as ISS days numbered

China's space programs open up to world

China's commercial aerospace companies flourishing

China launches Centispace-1-s1 satellite

MARSDAILY
Aboard the first spacecraft to the Trojan asteroids

Scientists push back against Harvard 'alien spacecraft' theory

Cosmic Detective Work: Why We Care About Space Rocks

New insights on comet tails are blowing in the solar wind

MARSDAILY
SwRI team makes breakthroughs studying Pluto orbiter mission

ALMA maps temperature of Jupiter's icy moon Europa

NASA's Juno Mission Detects Jupiter Wave Trains

WorldWide Telescope looks ahead to New Horizons' Ultima Thule glyby

MARSDAILY
Saturn's Moon Dione Covered by Mysterious Stripes

Cutting through the mystery of Titan's atmospheric haze

Surprising chemical complexity of Saturn's rings changing planet's upper atmosphere

Latest insights into Saturn's weird magnetic field only make things weirder

MARSDAILY
Ozone hole in northern hemisphere to recover completely by 2030

Orbit Logic delivers Landsat mission planning system

Illegal emissions threaten to undermine UN's optimistic ozone report

Europe's third polar-orbiting weather satellite lofted into orbit

MARSDAILY
From Quantum Optics to Increased Risk Posture: Student Innovations at NASA

'Dust up' on International Space Station hints at sources of structure

Computer on Russian segment of ISS rebooted after glitch

Russia's Roscosmos confirms computer glitch on board ISS

MARSDAILY
Laboratory experiments probe the formation of stars and planets

Laser tech could be fashioned into Earth's 'porch light' to attract alien astronomers

NASA retires Kepler Space Telescope, passes planet-hunting torch

Rocky and habitable - sizing up a galaxy of planets









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.