View source for Mars Express

{{Short description|European orbiter mission to Mars (2003–present)}}
{{Italic title}}
{{About|the space exploration mission|the film|Mars Express (film)}}
{{Infobox spaceflight
| name               = ''Mars Express''
| image              = Mars-express-volcanoes-sm.jpg
| image_caption      = CG image of ''Mars Express'' arriving at Mars
| mission_type       = [[Mars]] orbiter
| operator           = [[ESA]]
| website            = {{URL|exploration.esa.int/mars}}
| COSPAR_ID          = 2003-022A
| SATCAT             = 27816
| mission_duration   = Elapsed:<br />{{Age in years, months and days|year=2003|month=06|day=02}} since launch<br />{{Age in years, months and days|year=2003|month=12|day=25}} at Mars
| spacecraft_type    = 
| manufacturer       = 
| dry_mass           = {{convert|666|kg|lb|abbr=on}}
| launch_mass        = 1,123 kg<ref>{{cite web |url=https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=2003-022A |title=Mars Express |publisher=[[NASA Space Science Data Coordinated Archive]] |access-date=November 30, 2022 }}</ref>
| power              = 460&nbsp;watts
| launch_date        = {{start-date|June 2, 2003, 17:45|timezone=yes}}&nbsp;UTC
| launch_rocket      = [[Soyuz-FG]]/[[Fregat]]
| launch_site        = [[Baikonur Cosmodrome|Baikonur]] [[Baikonur Cosmodrome Site 31|31/6]]
| launch_contractor  = [[Starsem]]
| last_contact       = 
| decay_date         = 
| orbit_epoch        = 
| orbit_reference    = [[Areocentric orbit|Areocentric]]
| orbit_periapsis    = {{convert|298|km|mi|abbr=on}}
| orbit_apoapsis     = {{convert|10107|km|mi|abbr=on}}
| orbit_inclination  = 86.3&nbsp;degrees
| orbit_period       = 7.5&nbsp;hours
| orbit_eccentricity = 0.571
| apsis              = areion
| interplanetary     = {{Infobox spaceflight/IP
   |type                = orbiter
   |component           = ''Mars Express''
   |object              = [[Mars]]
   |orbits              = 
   |arrival_date        = December 25, 2003, 03:00 UTC<br /><small>[[Timekeeping on Mars|MSD]] 46206 08:27 [[Airy Mean Time|AMT]]</small>
}} 
 {{Infobox spaceflight/IP
   |type                = lander
   |component           = ''[[Beagle 2]]''
   |object              = [[Mars]]
   |site                = 
   |arrival_date        = December 25, 2003, 02:54 UTC
}}
| instruments_list   = {{Infobox spaceflight/Instruments
  |acronym1 = HRSC       |name1 = [[High Resolution Stereo Camera]]
  |acronym2 = OMEGA      |name2 = Visible and Infrared Mineralogical, Mapping Spectrometer
  |acronym3 = [[MARSIS]] |name3 = Sub-surface Sounding Radar Altimeter
  |acronym4 = PFS        |name4 = [[Planetary Fourier Spectrometer]]
  |acronym5 = SPICAM     |name5 = Ultraviolet and Infrared Atmospheric Spectrometer
  |acronym6 = ASPERA     |name6 = Energetic Neutral Atoms Analyser
  |acronym7 = MaRS       |name7 = Mars Radio Science Experiment
  |acronym8 = VMC        |name8 = [[Visual Monitoring Camera]] }}
| insignia           = File:Mars Express insignia.png
| insignia_caption   = ESA Solar System insignia for the ''Mars Express'' mission
| insignia_alt       = ''Mars Express'' mission insignia
}}
{{Use mdy dates|date=February 2024}}

'''''Mars Express''''' is a [[space exploration]] mission by the [[European Space Agency|European Space Agency (ESA)]] exploring the planet [[Mars]] and its moons since 2003, and the first planetary mission attempted by ESA.<ref name=":0">{{Cite web |last=Howell |first=Elizabeth |date=July 26, 2018 |title=European Space Agency's Mars Express |url=https://www.space.com/18206-mars-express.html |access-date=April 1, 2023 |website=Space.com }}</ref>

''Mars Express'' consisted of two parts, the ''Mars Express Orbiter'' and ''[[Beagle 2]]'',<ref name=":1">{{Cite web |title=NASA - NSSDCA - Spacecraft - Details |url=https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=2003-022A |access-date=April 1, 2023 |website=nssdc.gsfc.nasa.gov |publisher=National Aeronautics and Space Administration}}</ref> a [[Lander (spacecraft)|lander]] designed to perform [[exobiology]] and geochemistry research. Although the lander failed to fully deploy after it landed on the Martian surface, the orbiter has been successfully performing scientific measurements since early 2004, namely, [[image resolution|high-resolution]] imaging and mineralogical mapping of the surface, radar sounding of the subsurface structure down to the permafrost, precise determination of the [[atmospheric circulation]] and composition, and study of the interaction of the [[Atmosphere of Mars|atmosphere]] with the [[interplanetary medium]].<ref name=":1" />

Due to the valuable science return and the highly flexible mission profile, ''Mars Express'' has been granted several mission extensions. The latest was approved on March 7, 2023, consisting of a confirmed operating period until December 31, 2026, and a further provisional extension to December 31, 2028.<ref>{{cite web |url=https://sci.esa.int/web/director-desk/-/extended-life-for-esa-s-science-missions |title=Extended life for ESA's science missions |publisher=[[ESA]] |date=March 7, 2023 |access-date=March 20, 2023}}</ref><ref>{{cite web |url=https://www.theregister.com/2023/12/24/mars_express_mission_extension/ |title=ESA's Mars Express continues to avoid retirement home |publisher=[[The Register]] |last=Speed |first=Richard |date=December 24, 2023 |access-date=January 6, 2024}}</ref> Arriving at Mars in 2003, {{Age in years, months and days| year=2003| month=12| day=25}} ago (and counting), it is the second longest surviving, continually active spacecraft in orbit around a planet other than Earth, behind only NASA's still active ''[[2001 Mars Odyssey]]''.

== Name ==
"Express" in the name originally referred to the speed and efficiency with which the [[spacecraft]] was designed and built.<ref>{{cite web |date=February 18, 2009 |title=Mars Express Frequently Asked Questions |url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Frequently_asked_questions2 |access-date=March 28, 2016 |publisher=[[ESA]]}}</ref> However, "Express" also describes the spacecraft's relatively short interplanetary voyage, a result of being launched when the orbits of Earth and Mars brought them closer than they had been in about 60,000 years.<ref>{{Cite journal |last1=Cardesin-Moinelo |first1=A. |last2=Godfrey |first2=J. |last3=Grotheer |first3=E. |last4=Blake |first4=R. |last5=Damiani |first5=S. |last6=Wood |first6=S. |last7=Dressler |first7=T. |last8=Bruno |first8=M. |last9=Johnstone |first9=A. |last10=Lucas |first10=L. |last11=Marin-Yaseli de la Parra |first11=J. |last12=Merritt |first12=D. |last13=Sierra |first13=M. |last14=Määttänen |first14=A. |last15=Antoja-Lleonart |first15=G. |date=2024 |title=Mars Express: 20 Years of Mission, Science Operations and Data Archiving |url=https://link.springer.com/10.1007/s11214-024-01059-0 |journal=Space Science Reviews |language=en |volume=220 |issue=2 |page=25 |doi=10.1007/s11214-024-01059-0 |bibcode=2024SSRv..220...25C |issn=0038-6308|hdl=10261/359596 |hdl-access=free }}</ref>

== Background ==
The ''Mars Express'' mission is dedicated to the study of the interior, subsurface, surface, atmosphere, and environment of the planet Mars. The spacecraft carried seven scientific instruments, a small lander, a lander relay, and a [[Visual Monitoring Camera]], all designed to contribute to solving the [[Water on Mars|mystery of Mars' missing water]].

Some of the instruments on the orbiter, including the camera systems and some [[spectrometers]], reuse designs from the failed launch of the Russian ''[[Mars 96]]'' mission in 1996<ref name=":0" /> (European countries had provided much of the instrumentation and financing for that unsuccessful mission). The scientific objectives of the ''Mars Express'' represent an attempt to fulfill in part the lost scientific goals of this failed Russian mission, complemented by exobiology research with Beagle-2.<ref>{{Cite web |title=Mars Express en route for the Red Planet |url=https://www.esa.int/Newsroom/Press_Releases/Mars_Express_en_route_for_the_Red_Planet |access-date=2025-05-20 |website=www.esa.int |language=en}}</ref>

The design of ''Mars Express'' is based on ESA's [[Rosetta space probe|''Rosetta'' mission]], on which a considerable sum was spent on development. The same design was also used for ESA's ''[[Venus Express]]'' mission in order to increase reliability and reduce development cost and time.

The total initial ''Mars Express'' budget excluding the lander was [[euro|€]]150 million.<ref name="esa31021">{{cite web |date=March 29, 2011 |title=Mars Express: Summary |url=http://sci.esa.int/mars-express/31021-summary/ |publisher=European Space Agency}}</ref><ref name="nasa2003-022A">{{cite web |title=Mars Express |url=https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=2003-022A |access-date=December 7, 2018 |work=NSSDC ID: 2003-022A |publisher=NASA}}</ref> The prime contractor for the construction of ''Mars Express'' orbiter was [[EADS Astrium Satellites]].

== Orbiter and subsystems ==

=== Structure ===
The ''Mars Express'' orbiter is a cube-shaped spacecraft with two [[Photovoltaic module|solar panel]] wings extending from opposite sides. The launch mass of 1223&nbsp;kg includes a main bus with 113&nbsp;kg of payload, the 60&nbsp;kg lander, and 457&nbsp;kg of propellant. The main body is 1.5 m × 1.8 m × 1.4 m in size, with an aluminium honeycomb structure covered by an aluminium skin. The solar panels measure about 12 m tip-to-tip. Two 20 m long wire [[dipole antenna]]s extend from opposite side faces perpendicular to the solar panels as part of the radar sounder.<ref name="ref1">{{cite web |url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/The_spacecraft |title=The spacecraft / Mars Express |publisher=[[ESA]] |date=October 10, 2005 |access-date=March 29, 2016 }}</ref>

=== Propulsion ===
The Soyuz/Fregat launcher provided most of the thrust ''Mars Express'' needed to reach Mars. The final stage of the Soyuz, Fregat was jettisoned once the probe was safely on a course for Mars. The spacecraft's on-board means of propulsion was used to slow the probe for Mars orbit insertion and subsequently for orbit corrections.<ref name="ref1" />

The body is built around the main propulsion system, which consists of a [[Bipropellant rocket|bipropellant]] 400 [[Newton (unit)|N]] main engine. The two 267-liter propellant tanks have a total capacity of 595&nbsp;kg. Approximately 370&nbsp;kg are needed for the nominal mission. Pressurized helium from a 35-liter tank is used to force fuel into the engine. Trajectory corrections will be made using a set of eight 10 N thrusters, one attached to each corner of the spacecraft bus. The spacecraft configuration is optimized for a Soyuz/Fregat, and was fully compatible with a [[Delta II]] launch vehicle.

=== Power ===
Spacecraft power is provided by the solar panels which contain 11.42 square meters of silicon cells. The originally planned power was to be 660{{nbsp}}[[Watt|W]] at 1.5{{nbsp}}[[astronomical unit|AU]] but a faulty connection has reduced the amount of power available by 30%, to about 460{{nbsp}}W. This loss of power does not significantly affect the science return of the mission. Power is stored in three [[lithium ion battery|lithium-ion batteries]] with a total capacity of 64.8{{nbsp}}Ah for use during eclipses. The power is fully regulated at 28{{nbsp}}[[Volt|V]], and the [[Terma A/S|Terma]] power module (also used in ''[[Rosetta (spacecraft)|Rosetta]]'') is redundant.<ref>{{cite news |url=http://ing.dk/artikel/terma-elektronik-vaekker-rumsonde-fra-aarelang-dvale-165600 |title=Terma-elektronik vækker rumsonde fra årelang dvale|newspaper=[[Ingeniøren]] |first=Mie |last=Stage |date=January 19, 2014 |access-date=March 29, 2016 }}</ref><ref>{{Cite journal |title=Power Conditioning Unit for Rosetta/Mars Express |journal = Space Power |volume=502 |page=249 |publisher=[[Astrophysics Data System]] |last1=Jensen |first1=H. |last2=Laursen |first2=J. |bibcode=2002ESASP.502..249J |date=2002 }}</ref> During routine phase, the spacecraft's power consumption is in the range of 450–550{{nbsp}}W.<ref>{{cite web |url=http://www.asi-proc.it/missions/mex |title=MEX — ASI-PROC|publisher=Planetary Radar Operational Center |date=March 29, 2016 |access-date=March 29, 2016 |archive-url=https://web.archive.org/web/20160413141724/http://www.asi-proc.it/missions/mex |archive-date=April 13, 2016 }}</ref>

=== Attitude control - avionics ===
Attitude control (3-axis stabilization) is achieved using two 3-axis inertial measurement units, a set of two [[star camera]]s and two [[Sun sensor]]s, [[gyroscope]]s, [[accelerometer]]s, and four 12&nbsp;N·m·s [[reaction wheel]]s. Pointing accuracy is 0.04 degree with respect to the inertial reference frame and 0.8 degree with respect to the Mars orbital frame. Three on-board systems help ''Mars Express'' maintain a very precise pointing accuracy, which is essential to allow the spacecraft to use some of the science instruments.

=== Communications ===
The communications subsystem is composed of three antennas: A 1.6&nbsp;m diameter parabolic dish [[high-gain antenna]] and two omnidirectional antennas. The first one provide links (telecommands uplink and telemetry downlink) in both [[X-band]] (8.4&nbsp;GHz) and [[S-band]] (2.1&nbsp;GHz) and is used during nominal science phase around Mars. The low gain antennas are used during launch and early operations to Mars and for eventual contingencies once in orbit. Two Mars lander relay UHF antennas are mounted on the top face for communication with the ''Beagle 2'' or other landers, using a Melacom transceiver.<ref name="melacom">{{cite web |url=http://apps.qinetiq.com/perspectives/micro_news_article7.asp |title=QinetiQ to put Mars in the picture |archive-url=https://web.archive.org/web/20060831063330/http://apps.qinetiq.com/perspectives/micro_news_article7.asp |archive-date=August 31, 2006 |quote=Consisting of a lightweight bespoke transponder and transceiver weighing less than 650 grams, the system will provide the 10,000-kilometre UHF radio communications link between the ''Mars Express'' orbiter and Beagle-2 lander. |publisher=[[Qinetiq]] |access-date=March 29, 2016 }}</ref>

==== Earth stations ====
Although communications with Earth were originally scheduled to take place with the ESA 35-meter wide Ground Station in New Norcia (Australia) [[New Norcia Station]], the mission profile of progressive enhancement and science return flexibility have triggered the use of the ESA [[ESTRACK]] Ground Stations in [[Cebreros Station]], [[Madrid]], Spain and [[Malargüe Station]], [[Argentina]].

In addition, further agreements with NASA [[Deep Space Network]] have made possible the use of American stations for nominal mission planning, thus increasing complexity but with a clear positive impact in scientific returns.

This inter-agency cooperation has proven effective, flexible and enriching for both sides. On the technical side, it has been made possible (among other reasons) thanks to the adoption of both Agencies of the Standards for Space Communications defined in [[CCSDS]].

=== Thermal ===
Thermal control is maintained through the use of radiators, [[multi-layer insulation]], and actively controlled heaters. The spacecraft must provide a benign environment for the instruments and on-board equipment. Two instruments, PFS and OMEGA, have infrared detectors that need to be kept at very low temperatures (about −180&nbsp;°C). The sensors on the camera (HRSC) also need to be kept cool. But the rest of the instruments and on-board equipment function best at room temperatures (10–20&nbsp;°C).

The spacecraft is covered in gold-plated aluminium-tin alloy thermal blankets to maintain a temperature of 10–20&nbsp;°C inside the spacecraft. The instruments that operate at low temperatures to be kept cold are thermally insulated from this relatively high internal temperature, and emit excess heat into space using attached radiators.<ref name="ref1" />

=== Control unit and data storage ===
The spacecraft is run by two Control and Data management Units with 12 gigabits<ref name="ref1" /> of solid state mass memory for storage of data and housekeeping information for transmission. The on-board computers control all aspects of the spacecraft functioning including switching instruments on and off, assessing the spacecraft orientation in space and issuing commands to change it.

Another key aspect of the ''Mars Express'' mission is its [[artificial intelligence]] tool (MEXAR2).<ref name="ESA1">{{cite web |title=Artificial Intelligence Boosts Science from Mars |url=http://www.esa.int/Our_Activities/Operations/Artificial_intelligence_boosts_science_from_Mars |publisher=ESA |date=April 29, 2008 |access-date=March 29, 2016 }}</ref> The primary purpose of the AI tool is the scheduling of when to download various parts of the collected scientific data back to Earth, a process which used to take ground controllers a significant amount of time. The new AI tool saves operator time, optimizes [[Bandwidth (signal processing)|bandwidth]] use on the [[Deep Space Network|DSN]], prevents data loss, and allows better use of the DSN for other space operations as well. The AI decides how to manage the spacecraft's 12 gigabits of storage memory, when the DSN will be available and not be in use by another mission, how to make the best use of the DSN bandwidth allocated to it, and when the spacecraft will be oriented properly to transmit back to Earth.<ref name="ESA1" /><ref>{{cite journal |doi=10.1109/MIS.2007.75 |url=http://mexar.istc.cnr.it/mexar2/publications/mexar2-ieee-intsys.pdf |title=Mexar2: AI Solves Mission Planner Problems |journal=IEEE Intelligent Systems |volume=22 |issue=4 |pages=12–19 |first=Amedeo |last=Cesta |date=2007 |s2cid=14477705 |access-date=December 7, 2011 |archive-date=March 5, 2012 |archive-url=https://web.archive.org/web/20120305230348/http://mexar.istc.cnr.it/mexar2/publications/mexar2-ieee-intsys.pdf }}</ref>

== Lander ==
[[File:Beagle 2 replica.jpg|thumb|A replica of the ''[[Beagle 2]]'' lander component of ''Mars Express'' at the [[Science Museum, London]]]]

The ''[[Beagle 2]]'' lander objectives were to characterize the landing site geology, mineralogy, and geochemistry, the physical properties of the atmosphere and surface layers, collect data on Martian meteorology and climatology, and search for possible signatures of [[life on Mars]]. However, the landing attempt was unsuccessful and the lander was declared lost. 

A Commission of Inquiry on ''Beagle 2'' identified several possible causes, including airbag problems, severe shocks to the lander's electronics which had not been simulated adequately before launch, and problems with parts of the landing system colliding; but was unable to reach any firm conclusions.<ref name="inquiry">{{cite web|url=http://forum.nasaspaceflight.com/index.php?action=dlattach;topic=36541.0;attach=631766|title=Beagle 2 ESA/UK Commission of Inquiry|website=[[NASASpaceFlight.com]]|date=April 5, 2004|access-date=March 29, 2016}}</ref>

The spacecraft's fate remained a mystery until it was announced in January 2015 that NASA's [[Mars Reconnaissance Orbiter]], using [[HiRISE]], had found the probe intact on the surface of Mars. It was then determined that an error had prevented two of the spacecraft's four solar panels from deploying, blocking the spacecraft's communications.{{Attribution needed|date=May 2025}} ''Beagle 2'' was the first British and first European probe to achieve a landing on Mars.

== Scientific instruments ==
The scientific objectives of the ''Mars Express'' payload are to obtain global high-resolution photo-geology (10 m resolution), mineralogical mapping (100 m resolution) and mapping of the atmospheric composition, study the subsurface structure, the global atmospheric circulation, and the interaction between the atmosphere and the subsurface, and the atmosphere and the interplanetary medium. The total mass budgeted for the science payload is 116&nbsp;kg.<ref>{{cite book
| title = ESA SP-1240: Mars Express: the scientific payload
|first1=Andrew |last1=Wilson |first2=Agustin |last2=Chicarro |place=Noordwijk, Netherlands
| publisher = ESA Publications Division
| date = 2004
| isbn = 978-92-9092-556-9
| url = http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=34885}}
</ref> The payload scientific instruments are:<ref>{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Mars_Express_instruments|title=Mars Express orbiter instruments|publisher=[[ESA]]|date=November 30, 2005|access-date=March 29, 2016}}</ref>

* Visible and Infrared Mineralogical Mapping Spectrometer (OMEGA) (Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité) – France – Determines mineral composition of the surface up to 100 m resolution. Is mounted inside pointing out the top face.<ref>{{cite journal
| title = Global mineralogical and aqueous mars history derived from OMEGA/Mars express data|author5-link=Raymond Arvidson|author3-link=John F. Mustard
|vauthors=Bibring JP, Langevin Y, Mustard JF, Poulet F, Arvidson R, Gendrin A, Gondet B, Mangold N, Pinet P, Forget F |journal=[[Science (journal)|Science]]
| volume = 312
| issue = 5772
| date = 2006
| pages = 400–404
| doi=10.1126/science.1122659
| pmid = 16627738 |bibcode = 2006Sci...312..400B |s2cid=13968348 }}
</ref> Instrument mass: 28.6&nbsp;kg<ref name="chicarro">{{Cite report |url=http://mars.jpl.nasa.gov/mgs/sci/fifthconf99/6111.pdf |title=Mars Express Mission: Overview and Scientific Observations|last1= Chicarro|first1=A.F.|year=2003|access-date=March 29, 2016}}</ref>
* Ultraviolet and Infrared Atmospheric Spectrometer (SPICAM) – France – Assesses elemental composition of the atmosphere. Is mounted inside pointing out the top face. Instrument mass: 4.7&nbsp;kg<ref name="chicarro" />
* Sub-Surface Sounding Radar Altimeter ([[MARSIS]]) – Italy – A radar [[altimeter]] used to assess composition of sub-surface aimed at search for frozen water. Is mounted in the body and is nadir pointing, and also incorporates the two 20 m antennas. Instrument mass: 13.7&nbsp;kg<ref name="chicarro" />
* Planetary Fourier Spectrometer ([[Planetary Fourier Spectrometer|PFS]]) – Italy – Makes observations of atmospheric temperature and pressure (observations suspended in September 2005). Is mounted inside pointing out the top face<ref>{{cite journal|url=http://www.nature.com/news/2005/050905/full/news050905-10.html|title=Martian methane probe in trouble|journal=News@nature|publisher=[[Nature (journal)|Nature]]|doi=10.1038/news050905-10|first1=Mark|last1=Peplow|date=September 7, 2005|pages=news050905–10 |access-date=March 29, 2016|url-access=subscription}}</ref> and is currently working. Instrument mass: 30.8&nbsp;kg<ref name="chicarro" />
* Analyzer of Space Plasmas and Energetic Atoms (ASPERA) – Sweden – Investigates interactions between upper atmosphere and solar wind. Is mounted on the top face. Instrument mass: 7.9&nbsp;kg<ref name="chicarro" />
* [[High Resolution Stereo Camera]] (HRSC) – Germany – Produces color images with up to 2 m resolution. Is mounted inside the spacecraft body, aimed through the top face of the spacecraft, which is nadir pointing during Mars operations. Instrument mass: 20.4&nbsp;kg<ref name="chicarro" />
* Mars Express Lander Communications (MELACOM) – UK – Allows ''Mars Express'' to act as a communication relay for landers on the Martian surface. (Has been used on both [[Mars Exploration Rovers]], and was used to support the landing of NASA's ''Phoenix'' mission)
* Mars Radio Science Experiment (MaRS) – Uses radio signals to investigate atmosphere, surface, subsurface, gravity and solar corona density during solar conjunctions. It uses the communications subsystem itself.
* [[Visual Monitoring Camera]], a small camera to monitor the lander ejection.

== Operations of the spacecraft ==
{{more citations needed section|date=June 2011}}
Operations for ''Mars Express'' are carried out by a multinational team of engineers from ESA's Operation Centre ([[European Space Operations Centre|ESOC]]) in [[Darmstadt]]. The team began preparations for the mission about 3 to 4 years prior to the actual launch. This involved preparing the ground segment and the operational procedures for the whole mission.

The Mission Control Team is composed of the Flight Control Team, Flight Dynamics Team, Ground Operations Managers, Software Support and Ground Facilities Engineers. All of these are located at ESOC but there are additionally external teams, such as the Project and Industry Support teams, who designed and built the spacecraft. The Flight Control Team currently consists of:

* The Spacecraft Operations Manager
* Six Operations Engineers (including three Mission Planners)
* One Spacecraft Analyst
* Six spacecraft controllers (SpaCons), shared with [[ExoMars Trace Gas Orbiter]], [[BepiColombo]] and [[Solar Orbiter]].

The team build-up, headed by the Spacecraft Operations Manager, started about four years before launch. He was required to recruit a suitable team of engineers that could handle the varying tasks involved in the mission. For ''Mars Express'' the engineers came from various other missions. Most of them had been involved with Earth orbiting satellites.
== Mission profile ==
{{more citations needed section|date=June 2011}}

=== Mission preparation ===
In the years preceding the launch of a spacecraft numerous teams of experts distributed over the contributing companies and organisations prepared the space and ground segments. Each of these teams focussed on the area of its responsibility and interfacing as required. A major additional requirement raised for the Launch and Early Orbit Phase (LEOP) and all critical operational phases was that it was not enough merely to interface; the teams had to be integrated into one Mission Control Team. All the different experts had to work together in an operational environment and the interaction and interfaces between all elements of the system (software, hardware and human) had to run smoothly for this to happen:

* the flight operations procedures had to be written and validated down to the smallest detail;
* the [[control system]] had to be validated;
* system Validation Tests (SVTs) with the satellite had to be performed to demonstrate the correct interfacing of the ground and space segments;
* mission Readiness Test with the [[Ground station|Ground Stations]] had to be performed;
* a Simulations Campaign was run.

=== Launch ===
[[File:Animation of Mars Express trajectory around Sun.gif|thumb|Animation of Mars Express's trajectory around Sun<br />{{legend2|magenta|Mars Express}}{{·}}{{legend2|Yellow|Sun}}{{·}}{{legend2|Royalblue|Earth}} {{·}}{{legend2|Lime|Mars}}]]
The spacecraft was launched on June 2, 2003, at 23:45 local time (17:45 UT, 1:45&nbsp;p.m. EDT) from [[Baikonur Cosmodrome]] in [[Kazakhstan]], using a [[Soyuz-FG]]/[[Fregat]] rocket. The ''Mars Express'' and Fregat booster were initially put into a 200&nbsp;km Earth [[parking orbit]], then the Fregat was fired again at 19:14 UT to put the spacecraft into a Mars transfer orbit. The Fregat and ''Mars Express'' separated at approximately 19:17 UT. The [[solar panel]]s were then deployed and a trajectory correction manoeuvre was performed on June 4 to aim ''Mars Express'' towards Mars and allow the Fregat booster to coast into interplanetary space. The ''Mars Express'' was the first Russian-launched probe to successfully make it out of low Earth orbit since the Soviet Union fell.

=== Near Earth commissioning phase ===
The Near Earth commissioning phase extended from the separation of the spacecraft from the launcher upper stage until the completion of the initial check out of the orbiter and payload. It included the solar array deployment, the initial attitude acquisition, the declamping of the Beagle-2 spin-up mechanism, the injection error correction manoeuvre and the first commissioning of the spacecraft and payload (final commissioning of payload took place after Mars Orbit Insertion). The payload was checked out one instrument at a time. This phase lasted about one month.

=== The interplanetary cruise phase ===
This five month phase lasted from the end of the Near Earth Commissioning phase until one month prior to the Mars capture manoeuvre and included trajectory correction manoeuvres and payloads calibration. The payload was mostly switched off during the cruise phase, with the exception of some intermediate check-outs. Although it was originally meant to be a "quiet cruise" phase, It soon became obvious that this "cruise" would be indeed very busy. There were [[star tracker]] problems, a power wiring problem, extra manoeuvres, and on October 28, the spacecraft was hit by one of the largest [[solar flare]]s ever recorded.
=== Lander jettison ===
The [[Beagle 2]] lander was released on December 19, 2003, at 8:31 UTC (9:31 CET) on a [[Ballistics|ballistic]] cruise towards the surface. It entered Mars' atmosphere on the morning of December 25. Landing was expected to occur at about 02:45 UT on December 25 (9:45&nbsp;p.m. EST December 24). However, after repeated attempts to contact the lander failed using the ''Mars Express'' craft and the [[NASA]] ''[[Mars Odyssey]]'' orbiter, it was declared lost on February 6, 2004, by the Beagle 2 management board. An inquiry was held and its findings were published later that year.<ref name="inquiry" />

=== Orbit insertion ===
[[File:Animation of Mars Express trajectory around Mars.gif |thumb |right |Animation of ''Mars Express''{{'s}} trajectory around [[Mars]] from December 25, 2003, to January 1, 2010<br />{{legend2|magenta| Mars Express}}{{·}}{{legend2| Lime|[[Mars]]}}]]''Mars Express'' arrived at Mars after a 400 million km journey and course corrections in September and in December 2003.

On December 20 ''Mars Express'' fired a short thruster burst to put it into position to orbit the planet. The ''Mars Express'' orbiter then fired its main engine and went into a highly elliptical initial-capture orbit of 250&nbsp;km × 150,000&nbsp;km with an inclination of 25 degrees on December 25 at 03:00 UT (10:00&nbsp;p.m., December 24 EST).

First evaluation of the orbital insertion showed that the orbiter had reached its first milestone at Mars. The orbit was later adjusted by four more main engine firings to the desired 259&nbsp;km × 11,560&nbsp;km near-polar (86 degree inclination) orbit with a period of 7.5 hours. Near [[periapsis]] (nearest to Mars) the top deck is pointed down towards the Martian surface and near [[apoapsis]] (farthest from Mars in its orbit) the high gain antenna will be pointed towards Earth for uplink and downlink.

After 100 days the apoapsis was lowered to 10,107&nbsp;km and periapsis raised to 298&nbsp;km to give an orbital period of 6.7 hours.

The [[MARSIS]] radar booms were originally scheduled to be deployed in April 2004, but this was delayed to 2005 out of fear that the deployment could damage the spacecraft through a whiplash effect.<ref name=":2" />[[File:Mars Express illustration highlighting MARSIS antenna.jpg|thumb|Illustration of ''Mars Express'' with [[MARSIS]] antenna deployed]]{{multiple image
| align             = right
| direction         = vertical
| image1            = PIA07944 Mars Express Seen by Mars Global Surveyor.jpg
| caption1          = Image of ''Mars Express'' in orbit, taken by [[Mars Global Surveyor]]
| image2            = PIA07944 Mars Express Seen by Mars Global Surveyor, Figure 1.jpg
| caption2          = Artist's impression of the expected appearance of ''Mars Express'' at the time of the Mars Global Surveyor image
| total_width       = 250
}}

=== Routine phase: science return ===
Since orbit insertion ''Mars Express'' has been progressively fulfilling its original scientific goals. Nominal science observations began during July 2005. Nominally the spacecraft points to Mars while acquiring science and then slews to Earth-pointing to downlink the data, although some instruments like [[MARSIS]] or Radio Science might be operated while spacecraft is Earth-pointing.

== Timeline of notable discoveries and events ==
For more than 20,000 orbits, ''Mars Express'' payload instruments have been nominally and regularly operated. The [[High Resolution Stereo Camera|HRSC camera]] has been consistently mapping the Martian surface with unprecedented resolution and has acquired many images.

=== First decade ===

==== 2004 ====
* January 23: ESA announced the discovery of water ice in the south polar ice cap, using data collected by the OMEGA instrument.

* January 28: ''Mars Express'' orbiter reaches final science orbit altitude around Mars.

* March 17: Orbiter detects polar ice caps that contain 85% [[carbon dioxide]] (CO<sub>2</sub>) ice and 15% water ice.<ref>{{cite web |url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Water_at_Martian_south_pole |title=Water at Martian South Pole |publisher=[[ESA]] |date=March 17, 2004 |access-date=March 29, 2016 }}</ref>

* March 30: A press release announces that the orbiter has detected [[Methane on Mars|methane in the Martian atmosphere]]. Although the amount is small, about 10 parts in a thousand million, it has excited scientists to question its source. Since methane is removed from the Martian atmosphere very rapidly, there must be a current source that replenishes it. Because one of the possible sources could be microbial life, it is planned to verify the reliability of these data and especially watch for difference in the concentration in various places on Mars. It is hoped that the source of this gas can be discovered by finding its location of release.<ref>{{cite journal |last1=Formisano |first1=V. |last2=Atreya |first2=S. |last3=Encrenaz |first3=T. |author3-link=Thérèse Encrenaz |last4=Ignatiev |first4=N. |last5=Giuranna |first5=M. |title=Detection of Methane in the Atmosphere of Mars |journal=[[Science (journal)|Science]] |date=2004 |volume=306 |pages=1758–1761 |doi=10.1126/science.1101732 |pmid=15514118 |issue=5702 |bibcode = 2004Sci...306.1758F |s2cid=13533388 |doi-access=free }}</ref>

* April 28: ESA announced that the deployment of the boom carrying the radar-based MARSIS antenna was delayed. It described concerns with the motion of the boom during deployment, which can cause the spacecraft to be struck by elements of it. Further investigations are planned to make sure that this will not happen.

* July 15: Scientists working with the PFS instrument announced that they tentatively discovered the spectral features of the compound [[ammonia]] in the Martian atmosphere. Just like methane discovered earlier (see above), ammonia breaks down rapidly in Mars' atmosphere and needs to be constantly replenished. This points towards the existence of active life or geological activity; two contending phenomena whose presence so far have remained undetected.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Water_and_methane_maps_overlap_on_Mars_a_new_clue|title=Water and methane maps overlap on Mars: a new clue?|publisher=[[ESA]]|date=September 20, 2004|access-date=March 29, 2016}}</ref>

==== 2005 ====
* In 2005, [[ESA]] scientists reported that the OMEGA (Visible and Infrared Mineralogical Mapping Spectrometer: "Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité") instrument data indicates the presence of hydrated sulphates, silicates and various rock-forming minerals.<ref>{{cite journal |last1=Mustard |first1=JF |title=Olivine and Pyroxene Diversity in the Crust of Mars |journal=Science |date=2005 |volume=307 |issue=5715 |pages=1594–7 |doi=10.1126/science.1109098|pmid=15718427 |bibcode=2005Sci...307.1594M |s2cid=15548016 |doi-access=free }}</ref><ref>{{cite journal |last1=Bargery |first1=AS|display-authors=etal|title=NEAR-INFRARED ANALYSIS OF TEMPE TERRA, OLYMPICA FOSSAE AND NILI FOSSAE FROM OMEGA DATA |journal=Lunar and Planetary Science |date=2006 |volume=XXXVII |page=1684}}</ref>
* February 8: The delayed deployment of the MARSIS antenna, planned for early May 2005, has been given a green light by ESA.<ref name=":2">{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Green_light_for_deployment_of_ESA_s_Mars_Express_radar|title=Green light for deployment of ESA's Mars Express radar|publisher=[[ESA]]|date=February 8, 2005|access-date=March 29, 2016}}</ref>

* May 5: The first boom of the MARSIS antenna was successfully deployed.<ref>{{cite news|url=http://news.bbc.co.uk/1/hi/sci/tech/4516535.stm|title=First Marsis radar boom deployed|work=[[BBC News Online]]|date=May 5, 2005|access-date=March 29, 2016}}</ref> At first, there was no indication of any problems, but later it was discovered that one segment of the boom did not lock.<ref>{{cite news|url=http://news.bbc.co.uk/1/hi/sci/tech/4528763.stm|title=Delay hits Mars radar deployment|work=[[BBC News Online]]|date=May 9, 2005|access-date=March 29, 2016}}</ref> The deployment of the second boom was delayed to allow for further analysis of the problem.

* May 11: Using the [[Sun]]'s heat to expand the segments of the MARSIS antenna, the last segment locked in successfully.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Operations/First_MARSIS_boom_successfully_deployed|title=First MARSIS boom successfully deployed|publisher=[[ESA]]|date=May 11, 2005|access-date=March 29, 2016}}</ref>

* June 14: The second boom was deployed, and on June 16 ESA announced it was a success.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Operations/Smooth_deployment_for_second_MARSIS_antenna_boom|title=Smooth deployment for second MARSIS antenna boom|publisher=[[ESA]]|date=June 16, 2005|access-date=March 29, 2016}}</ref>

* June 22: ESA announces that MARSIS is fully operational and will soon begin acquiring data. This comes after the deployment of the third boom on June 17, and a successful transmission test on June 19.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Mars_Express_radar_ready_to_work|title=Mars Express radar ready to work|publisher=[[ESA]]|date=June 22, 2005|access-date=March 29, 2016}}</ref>

==== 2006 ====
* September 21: The High Resolution Stereo Camera (HRSC) has obtained images of the [[Cydonia (region of Mars)|Cydonia region]], the location of the famous "[[Cydonia Mensae|Face on Mars]]". The massif became famous in a photo taken in 1976 by the American ''Viking 1'' Orbiter. The image recorded with a ground resolution of approximately 13.7 metres per pixel.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Cydonia_-_the_face_on_Mars|title=Cydonia – the face on Mars|publisher=[[ESA]]|date=September 21, 2006|access-date=March 29, 2016}}</ref>

* September 26: The ''Mars Express'' spacecraft emerged from an unusually demanding eclipse introducing a special, ultra-low-power mode nicknamed 'Sumo' – an innovative configuration aimed at saving the power necessary to ensure spacecraft survival. This mode was developed through teamwork between ESOC mission controllers, principal investigators, industry, and mission management.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Mars_Express_successfully_powers_through_eclipse_season|title=Mars Express successfully powers through eclipse season|publisher=[[ESA]]|date=September 26, 2006|access-date=March 29, 2016}}</ref>

* October: In October 2006 the ''Mars Express'' spacecraft encountered a superior solar conjunction (alignment of Earth-Sun-Mars-orbiter). The angle Sun-Earth-orbiter reached a minimum on October 23 at 0.39° at a distance of 2.66 [[Astronomical unit|AU]]. Operational measures were undertaken to minimize the impact of the link degradation, since the higher density of electrons in the solar plasma heavily impacts the radio frequency signal.<ref>{{cite web|url=https://issfd.org/ISSFD_2007/10-3.pdf|title=EFFECTS ON SPACECRAFT RADIOMETRIC DATA AT SUPERIOR SOLAR CONJUNCTION|last1=Morley|first1=Trevor|last2=Budnik|first2=Frank|publisher=European Space Operations Centre}}</ref>

* December: Following the loss of NASA's ''[[Mars Global Surveyor]]'' (MGS), ''Mars Express'' team was requested to perform actions in the hopes of visually identifying the American spacecraft. Based on last [[ephemeris]] of MGS provided by JPL, the on-board high definition HRSC camera swept a region of the MGS orbit. Two attempts were made to find the craft, both unsuccessful.

==== 2007 ====
[[File:Phobos over Mars' limb by HRSC.jpg|thumb|Greyscale view of [[Phobos (moon)|Phobos]] over Mars, 2007 (ESA/DLR/FU Berl|388x388px]]
* January: First agreements with NASA undertaken for the support by ''Mars Express'' on the landing of the American lander [[Phoenix (spacecraft)|''Phoenix'']] in May 2008.

* February: The small camera VMC (used only once to monitor the lander ejection) was recommissioned and first steps were taken to offer students the possibility to participate in a campaign "Command Mars Express Spacecraft and take your own picture of Mars".

* February 23: As result of the science return, the Science Program Committee (SPC) granted a mission extension until May 2009.<ref>{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/The_planetary_adventure_continues_-_Mars_Express_and_Venus_Express_operations_extended|title=The planetary adventure continues - Mars Express and Venus Express operations extended|publisher=[[ESA]]|date=February 27, 2007|access-date=March 29, 2016}}</ref>

* June 28: The High Resolution Stereo Camera (HRSC) has produced images of key tectonic features in [[Aeolis Mensae]].<ref name="aeolis">{{cite web
| title = Tectonic signatures at Aeolis Mensae
| work =ESA News
| publisher =European Space Agency
| date =June 28, 2007
| url =http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Tectonic_signatures_at_Aeolis_Mensae
| access-date =March 29, 2016}}</ref>

==== 2008 ====
* In March 2008, the ''Mars Express'' Team was the winner of the [[Sir Arthur Clarke Award]] for Best Team Achievement.<ref>{{Cite web |title=Sir Arthur Clarke Awards |url=https://www.bis-space.com/what-we-do/honours-and-awards/arthurs/ |access-date=2025-05-25 |website=The British Interplanetary Society |language=en-GB}}</ref>
* During a [[Phobos (moon)|Phobos]] flyby on 23 July 2008, ''Mars Express'' observed backscattering of [[solar wind]] protons at Phobos, a process previously reported at the Earth's [[Moon]], suggesting that it is common at airless bodies covered by [[regolith]].<ref>{{Cite journal |last1=Futaana |first1=Y. |last2=Barabash |first2=S. |last3=Holmström |first3=M. |last4=Fedorov |first4=A. |last5=Nilsson |first5=H. |last6=Lundin |first6=R. |last7=Dubinin |first7=E. |last8=Fränz |first8=M. |date=2010 |title=Backscattered solar wind protons by Phobos |url=https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2010JA015486 |journal=Journal of Geophysical Research: Space Physics |language=en |volume=115 |issue=A10 |doi=10.1029/2010JA015486 |bibcode=2010JGRA..11510213F |issn=2156-2202}}</ref> The next such observation occurred in January 2016.<ref>{{Cite journal |last1=Futaana |first1=Yoshifumi |last2=Holmström |first2=Mats |last3=Fedorov |first3=Andrey |last4=Barabash |first4=Stas |date=2021 |title=Does Phobos Reflect Solar Wind Protons? Mars Express Special Flyby Operations With and Without the Presence of Phobos |url=https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2021JE006969 |journal=Journal of Geophysical Research: Planets |language=en |volume=126 |issue=11 |pages=e2021JE006969 |doi=10.1029/2021JE006969 |bibcode=2021JGRE..12606969F |issn=2169-9100}}</ref>

==== 2009 ====
* February 4: The ESA's Science Programme Committee has extended the operations of ''Mars Express'' until December 31, 2009.<ref>{{cite web|url=http://sci.esa.int/solar-system/44174-mars-express-venus-express-cluster-missions-extended/|title=ESA extends missions studying Mars, Venus and Earth's magnetosphere|publisher=[[ESA]]|date=February 9, 2009|access-date=March 29, 2016}}</ref>

*October 7: ESA's Science Programme Committee has approved the extension of mission operations for ''Mars Express'' until December 31, 2012.<ref>{{cite web|url=http://sci.esa.int/director-desk/45685-mission-extensions-approved-for-science-missions/|title=Mission extensions approved for science missions|publisher=[[ESA]]|date=October 7, 2009|access-date=March 29, 2016}}</ref>
[[File:Orcus Patera by HRSC.jpg|thumb|[[Orcus Patera]] on Mars imaged by the [[High Resolution Stereo Camera|HRSC]] instrument aboard ''Mars Express'', 2010]]

==== 2010 ====
*March 5: Flyby of [[Phobos (moon)|Phobos]] to measure Phobos' gravity.<ref>{{cite news|url=http://spacefellowship.com/news/art18911/phobos-flyby-success.html|title=Phobos Flyby Success|work=[[Space Fellowship]]|date=March 5, 2010|access-date=March 29, 2016|archive-url=https://web.archive.org/web/20140221231830/http://spacefellowship.com/news/art18911/phobos-flyby-success.html|archive-date=February 21, 2014 }}</ref>

==== 2011 ====
*August 13: Safe mode following a Solid-State Mass Memory problem.<ref name="ESASCi">{{cite web|url=http://sci.esa.int/mars-express/49549-mars-express-observations-temporarily-suspended/|title=Mars Express observations temporarily suspended|publisher=[[ESA]]|date=November 24, 2011|access-date=March 29, 2016}}</ref>

*August 23: Solid-State Mass Memory problem.<ref name="ESASCi" />

*September 23: Safe mode following a Solid-State Mass Memory problem.<ref name="ESASCi" />

*October 11: Solid-State Mass Memory problem.<ref name="ESASCi" />

*October 16: Safe mode following a Solid-State Mass Memory problem.<ref name="ESASCi" />

*November 24: Science operations are resumed using the Short Mission Timeline and Command Files instead of the Long Time Line resident on the suspect Solid-State Mass Memory.<ref name="ESASCi2">{{cite web|url=http://www.esa.int/Our_Activities/Operations/Mars_Express_steadily_returns_to_routine_operation|title=Mars Express steadily returns to routine operation|publisher=[[ESA]]|date=November 24, 2011|access-date=March 29, 2016}}</ref>

==== 2012 ====
* February 16: Resumes full science operations. There is still enough fuel for up to 14 additional years of operation.<ref>{{cite web|url=http://spaceflightnow.com/news/n1202/15marsexpress/|title=Mars Express back in business at the red planet|publisher=Spaceflight Now|first=Stephen|last=Clark|date=February 15, 2012|access-date=March 29, 2016}}</ref>
* In March 2012, a paper was published in ''[[JGR Planets]]'' documenting the first detection of a faint infrared glow above the winter poles of Mars. This discovery was based on ''Mars Express''' OMEGA observations from 2004, 2005, and 2006.<ref>{{Cite web |title=ESA Science & Technology - A glow in the Martian night throws light on atmospheric circulation |url=https://sci.esa.int/web/mars-express/-/50198-a-glow-in-the-martian-night-throws-light-on-atmospheric-circulation |access-date=2025-05-18 |website=sci.esa.int |language=en-US}}</ref><ref>{{Cite journal |last1=Bertaux |first1=J. L. |last2=Gondet |first2=B. |last3=Lefèvre |first3=F. |last4=Bibring |first4=J. P. |last5=Montmessin |first5=F. |date=2012 |title=First detection of O 2 1.27 μ m nightglow emission at Mars with OMEGA/MEX and comparison with general circulation model predictions |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2011JE003890 |journal=Journal of Geophysical Research: Planets |language=en |volume=117 |issue=E11 |doi=10.1029/2011JE003890 |issn=0148-0227}}</ref>

* July: Solar corona studied with radio waves.<ref>{{cite web|url=http://sci.esa.int/mars-express/50629-radio-sounding-of-the-solar-corona-with-mars-express/|title=Radio sounding of the solar corona with Mars Express|publisher=[[ESA]]|date=July 24, 2012|access-date=March 29, 2016}}</ref>

* August 5/6: Assisted US probes ''[[Mars Odyssey]]'' and ''[[Mars Reconnaissance Orbiter]]'' in data collection and transfer on the [[Mars Science Laboratory]] landing.

==== 2013 ====
*''Mars Express'' produced a near-complete topographical map of Mars' surface.<ref>{{cite news | first1 = Elizabeth |last1=Gibney | title = Spectacular flyover of Mars | date = October 28, 2013 | url = http://www.nature.com/news/spectacular-flyover-of-mars-1.14041 | work = Nature News | access-date = November 17, 2013}}</ref>
*On 29 December, ''Mars Express'' performed the closest flyby to date of [[Phobos (moon)|Phobos]]
=== Second decade ===

==== 2014 ====
[[File:Rabe Crater perspective ESA310887.jpg|thumb|[[Rabe (crater)|Rabe crater]], 2014]]
* In October 2014, ESA reported ''Mars Express'' was healthy after the [[C/2013 A1|Comet Siding Spring]] flyby of Mars on 19 October<ref name="ESA-20141020">{{cite web |last=Denis |first=Michel |title=Spacecraft in great shape – our mission continues |url=http://blogs.esa.int/mex/2014/10/20/spacecraft-in-great-shape-our-mission-continues/ |date=October 20, 2014 |work=[[European Space Agency]] |access-date=October 21, 2014 }}</ref> &mdash; as were all NASA Mars orbiters<ref name="NASA-20141019">{{cite web |last1=Webster |first1=Guy |last2=Brown |first2=Dwayne |last3=Jones |first3=Nancy |last4=Steigerwald |first4=Bill |title=All Three NASA Mars Orbiters Healthy After Comet Flyby |url=http://www.jpl.nasa.gov/news/news.php?feature=4347 |date=October 19, 2014 |work=[[NASA]] |access-date=October 20, 2014 }}</ref> and [[Indian Space Research Organisation|ISRO's]] orbiter, the [[Mars Orbiter Mission]].<ref name="ISRO MOM safe after Mars comet flyby">{{cite news |author=Staff |title=I'm safe and sound, tweets MOM after comet sighting |url=http://www.thehindu.com/sci-tech/science/im-safe-and-sound-tweets-mom-after-comet-sighting/article6520803.ece |date=October 21, 2014 |work=[[The Hindu]] |access-date=October 21, 2014 }}</ref>

==== 2016 ====
* During a [[Phobos (moon)|Phobos]] flyby in January 2016, ''Mars Express'' again observed [[solar wind]] proton backscattering from the moon's surface. This was only second such observation by the spacecraft (first occurred in 2008) and, as of 2025, this intermittency remains unexplained.<ref>{{Cite web |title=ESA's Mars Express unravels mystery of martian moon using 'fake' flybys |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/ESA_s_Mars_Express_unravels_mystery_of_martian_moon_using_fake_flybys |access-date=2025-05-25 |website=www.esa.int |language=en}}</ref><ref>{{Cite journal |last1=Futaana |first1=Yoshifumi |last2=Holmström |first2=Mats |last3=Fedorov |first3=Andrey |last4=Barabash |first4=Stas |date=2021 |title=Does Phobos Reflect Solar Wind Protons? Mars Express Special Flyby Operations With and Without the Presence of Phobos |url=https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2021JE006969 |journal=Journal of Geophysical Research: Planets |language=en |volume=126 |issue=11 |pages=e2021JE006969 |doi=10.1029/2021JE006969 |bibcode=2021JGRE..12606969F |issn=2169-9100}}</ref>
* October 19: Assisted with data collection and transfer for the [[Schiaparelli EDM lander]] landing.
[[File:Martian south pole during summer by HRSC.jpg|thumb|South pole of Mars by ''Mars Express'', 2015 (ESA/DLR/FU Berlin)]]

==== 2017 ====
*On 19 June, the spacecraft took a notable image spanning from the North Pole up to [[Alba Mons]] and even farther south.<ref name="esamars">{{Cite web|url=http://www.sci-news.com/space/esa-image-mars-05553.html|title=ESA Releases Stunning New Image of Mars &#124; Space Exploration &#124; Sci-News.com|website=Breaking Science News &#124; Sci-News.com|date=December 20, 2017 }}</ref> The image was released in December 20, 2017, and was captured by HRSC.<ref name="esamars" /><ref>{{Cite web|url=https://www.dlr.de/EN/Service/about-relaunch/explanation.html?cms_url=https%3A%2F%2Fwww.dlr.de%2Fdlr%2Fen%2Fdesktopdefault.aspx%2Ftabid-10081%2F151_read-25327%2F|title=Relaunch explanation|website=NAV_NODE DLR Portal|access-date=October 19, 2019|archive-date=October 19, 2019|archive-url=https://web.archive.org/web/20191019051624/https://www.dlr.de/EN/Service/about-relaunch/explanation.html?cms_url=https%3A%2F%2Fwww.dlr.de%2Fdlr%2Fen%2Fdesktopdefault.aspx%2Ftabid-10081%2F151_read-25327%2F }}</ref>
[[File:Elongated cloud on Mars – annotated ESA401960.jpg|thumb|Elongated cloud on Mars, 2018<ref>{{Cite web |title=ESA Science & Technology - Elongated cloud on Mars &ndash; 10 October |url=https://sci.esa.int/web/mars-express/-/60882-elongated-cloud-on-mars-10-october |access-date=2025-05-20 |website=sci.esa.int}}</ref>]]

==== 2018 ====
[[File:Mars-SubglacialWater-SouthPoleRegion-20180725.jpg|thumb|Mars [[Planum Australe|South Pole]], site of [[Water on Mars|subglacial water]] (July 25, 2018)|354x354px]]
*Activated new AOCMS software which includes a gyroless attitude estimator to prolong the lifetime of the spacecraft's laser gyros<ref>{{Cite web |title=Mars Express v2.0 |url=https://www.esa.int/Enabling_Support/Operations/Mars_Express_v2.0 |access-date=April 12, 2022 |website=ESA.int }}</ref>
*In July 2018, a discovery was reported based on MARSIS [[radar]] studies, of a [[Water on Mars#Subglacial liquid water|subglacial lake]] on [[Mars]], {{convert|1.5|km|mi|abbr=on}} below the [[Planum Australe|southern polar ice cap]], and about {{convert|20|km|mi|abbr=on}} wide, the first known stable body of water on Mars.<ref name="SCI-20180725">{{cite journal |author=Orosei, R.|display-authors=etal|title=Radar evidence of subglacial liquid water on Mars |date=July 25, 2018 |journal=[[Science (journal)|Science]] |volume=361|issue=6401|pages=490–493|doi=10.1126/science.aar7268 |pmid=30045881|arxiv=2004.04587|hdl=11573/1148029|doi-access=free |bibcode=2018Sci...361..490O}}</ref><ref name="NYT-20180725">{{cite news |last1=Chang |first1=Kenneth |last2=Overbye |first2=Dennis |author-link2=Dennis Overbye |title=A Watery Lake Is Detected on Mars, Raising the Potential for Alien Life - The discovery suggests that watery conditions beneath the icy southern polar cap may have provided one of the critical building blocks for life on the red planet. |url=https://www.nytimes.com/2018/07/25/science/mars-liquid-alien-life.html |date=July 25, 2018 |work=[[The New York Times]] |access-date=July 25, 2018 }}</ref><ref>{{cite web |title=Huge reservoir of liquid water detected under the surface of Mars |url=https://www.eurekalert.org/pub_releases/2018-07/aaft-hro072318.php |work=[[EurekAlert]]|date=July 25, 2018 |access-date=July 25, 2018 }}</ref><ref>{{cite web |title=Liquid water 'lake' revealed on Mars |url=https://www.bbc.co.uk/news/science-environment-44952710 |work=[[BBC News]]|date=July 25, 2018 |access-date=July 25, 2018 }}</ref>
* December 2018: ''Mars Express'' relays images of the 80-kilometer wide [[Korolev (Martian crater)|Korolev Crater]] filled with approximately 2200 cubic kilometers of water ice on the Martian surface.<ref name="DLR">{{cite web |title=A winter wonderland in red and white – Korolev Crater on Mars |url=https://www.dlr.de/dlr/en/desktopdefault.aspx/tabid-10081/151_read-31614/#/gallery/33106 |website=German Aerospace Center (DLR) |access-date=December 20, 2018}}</ref> Based on further evidence the crater ice is still part of much vaster ice resources at Mars poles.<ref name="TG1218">{{cite news |last=Sample |first=Ian |url=https://www.theguardian.com/science/2018/dec/21/mars-express-beams-back-images-of-ice-filled-korolev-crater |work=The Guardian |access-date=December 21, 2018 |title=Mars Express Beams Back Images of Ice-Filled Korolev Crater |date=December 21, 2018 }}</ref>

==== 2019 ====
*Based on data from the HRSC camera, there is geological evidence of an ancient planet-wide groundwater system.<ref>{{cite journal | doi = 10.1029/2018JE005802 | pmid = 31007995 | pmc = 6472477 | title = Geological Evidence of Planet-Wide Groundwater System on Mars | date = 2019 | last1 = Salese | first1 = Francesco | last2 = Pondrelli | first2 = Monica | last3 = Neeseman  | first3 = Alicia | last4 = Schmidt | first4 = Gene | last5 = Ori  | first5 = Gian Gabriele | journal = Journal of Geophysical Research: Planets | volume = 124 | issue = 2 | pages = 374–395 | bibcode = 2019JGRE..124..374S}}</ref><ref name="ESA">{{cite web|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/First_evidence_of_planet-wide_groundwater_system_on_Mars|work=ESA|access-date=February 28, 2019|title=First evidence of planet-wide groundwater system on Mars}}</ref>

==== 2020 ====
*Between March and April 2020, ''Mars Express'' (along with other interplanetary missions by ESA) was briefly placed into a largely unattended safe configuration with science instruments turned off due to the worsening [[COVID-19 pandemic]] and the need to reduce on-site personnel at [[European Space Operations Centre|ESOC]].<ref>{{Cite web |title=ESA scales down science mission operations amid pandemic |url=https://www.esa.int/Science_Exploration/Space_Science/ESA_scales_down_science_mission_operations_amid_pandemic |access-date=2025-05-20 |website=www.esa.int |language=en}}</ref><ref>{{Cite web |title=Space missions return to science |url=https://www.esa.int/Enabling_Support/Operations/Space_missions_return_to_science |access-date=2025-05-20 |website=www.esa.int |language=en}}</ref>
*In September 2020, a discovery was reported based on MARSIS radar studies, of [[Water on Mars#Subglacial liquid water|three more subglacial lakes]] on Mars, {{convert|1.5|km|mi|abbr=on}} below the [[Planum Australe|southern polar ice cap]]. The size of the first lake found, and the largest, has been corrected to {{convert|30|km|mi|abbr=on}} wide. It is surrounded by 3 smaller lakes, each a few kilometres wide.<ref name="NatAstro">{{cite journal |last1=Lauro |first1=Sebastian Emanuel |last2=Pettinelli |first2=Elena |last3=Caprarelli |first3=Graziella |last4=Guallini |first4=Luca |last5=Rossi |first5=Angelo Pio |last6=Mattei |first6=Elisabetta |last7=Cosciotti |first7=Barbara |last8=Cicchetti |first8=Andrea |last9=Soldovieri |first9=Francesco |last10=Cartacci |first10=Marco |last11=Di Paolo |first11=Federico |last12=Noschese |first12=Raffaella |last13=Orosei |first13=Roberto |title=Multiple subglacial water bodies below the south pole of Mars unveiled by new MARSIS data |journal=Nature Astronomy |date=September 28, 2020 |volume=5 |pages=63–70 |doi=10.1038/s41550-020-1200-6 |publisher=Springer Nature Limited |arxiv=2010.00870 |s2cid=222125007 |issn=2397-3366}}</ref>
*A study published in December 2020 in ''[[JGR Planets]]'' utilized the wide field of view of the [[Visual Monitoring Camera]], in combination with other instruments on ''Mars Express'' and other orbiters, to describe the life cycle of a large elongated [[orographic cloud]] that grows and fades on a daily basis during spring and summer over [[Arsia Mons]].<ref>{{Cite journal |last1=Hernández-Bernal |first1=J. |last2=Sánchez-Lavega |first2=A. |last3=del Río-Gaztelurrutia |first3=T. |last4=Ravanis |first4=E. |last5=Cardesín-Moinelo |first5=A. |last6=Connour |first6=K. |last7=Tirsch |first7=D. |last8=Ordóñez-Etxeberria |first8=I. |last9=Gondet |first9=B. |last10=Wood |first10=S. |last11=Titov |first11=D. |last12=Schneider |first12=N. M. |last13=Hueso |first13=R. |last14=Jaumann |first14=R. |last15=Hauber |first15=E. |date=2021 |title=An Extremely Elongated Cloud Over Arsia Mons Volcano on Mars: I. Life Cycle |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2020JE006517 |journal=Journal of Geophysical Research: Planets |language=en |volume=126 |issue=3 |pages=e2020JE006517 |doi=10.1029/2020JE006517 |arxiv=2103.03919 |bibcode=2021JGRE..12606517H |issn=2169-9100}}</ref><ref>{{Cite web |title=Mars Express unlocks the secrets of curious cloud |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/Mars_Express_unlocks_the_secrets_of_curious_cloud |access-date=2025-05-21 |website=www.esa.int |language=en}}</ref> A follow-up study published in 2022 used [[computational modeling]] to describe the physical mechanisms behind the cloud's formation.<ref>{{Cite journal |last1=Hernández-Bernal |first1=J. |last2=Spiga |first2=A. |last3=Sánchez-Lavega |first3=A. |last4=del Río-Gaztelurrutia |first4=T. |last5=Forget |first5=F. |last6=Millour |first6=E. |date=2022 |title=An Extremely Elongated Cloud Over Arsia Mons Volcano on Mars: 2. Mesoscale Modeling |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022JE007352 |journal=Journal of Geophysical Research: Planets |language=en |volume=127 |issue=10 |pages=e2022JE007352 |doi=10.1029/2022JE007352 |arxiv=2410.03025 |bibcode=2022JGRE..12707352H |issn=2169-9100}}</ref>

==== 2021 ====
* Two studies published in December 2020<ref>{{Cite journal |last1=Fedorova |first1=Anna |last2=Montmessin |first2=Franck |last3=Korablev |first3=Oleg |last4=Lefèvre |first4=Franck |last5=Trokhimovskiy |first5=Alexander |last6=Bertaux |first6=Jean-Loup |date=2021 |title=Multi-Annual Monitoring of the Water Vapor Vertical Distribution on Mars by SPICAM on Mars Express |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2020JE006616 |journal=Journal of Geophysical Research: Planets |language=en |volume=126 |issue=1 |pages=e2020JE006616 |doi=10.1029/2020JE006616 |bibcode=2021JGRE..12606616F |issn=2169-9100}}</ref> and January 2021,<ref>{{Cite journal |last1=Chaufray |first1=J. -Y. |last2=Gonzalez-Galindo |first2=F. |last3=Lopez-Valverde |first3=M. A. |last4=Forget |first4=F. |last5=Quémerais |first5=E. |last6=Bertaux |first6=J. -L. |last7=Montmessin |first7=F. |last8=Chaffin |first8=M. |last9=Schneider |first9=N. |last10=Clarke |first10=J. T. |last11=Leblanc |first11=F. |last12=Modolo |first12=R. |last13=Yelle |first13=R. V. |date=2021-01-01 |title=Study of the hydrogen escape rate at Mars during martian years 28 and 29 from comparisons between SPICAM/Mars express observations and GCM-LMD simulations |url=https://www.sciencedirect.com/science/article/abs/pii/S0019103518306985 |journal=Icarus |series=From Mars Express to Exomars |volume=353 |pages=113498 |doi=10.1016/j.icarus.2019.113498 |bibcode=2021Icar..35313498C |issn=0019-1035}}</ref> that analyzed SPICAM data, show that water escape to space is accelerated by dust storms and Mars' proximity to the Sun, and suggest that some water may have retreated underground.<ref>{{Cite web |title=Mars water loss shaped by seasons and storms |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/Mars_water_loss_shaped_by_seasons_and_storms |access-date=2025-05-22 |website=www.esa.int |language=en}}</ref>
* A study published in April 2021, that used SPICAM data to analyze the relationship between ozone and water vapour in the atmosphere of Mars, identified a previously unknown problem with climate models, that might be relevant also to studying the Earth's atmosphere.<ref>{{Cite web |title=Better understanding of Earth's atmospheric chemistry from studying Mars? |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/Better_understanding_of_Earth_s_atmospheric_chemistry_from_studying_Mars |access-date=2025-05-24 |website=www.esa.int |language=en}}</ref><ref>{{Cite journal |last1=Lefèvre |first1=F. |last2=Trokhimovskiy |first2=A. |last3=Fedorova |first3=A. |last4=Baggio |first4=L. |last5=Lacombe |first5=G. |last6=Määttänen |first6=A. |last7=Bertaux |first7=J.-L. |last8=Forget |first8=F. |last9=Millour |first9=E. |last10=Venot |first10=O. |last11=Bénilan |first11=Y. |last12=Korablev |first12=O. |last13=Montmessin |first13=F. |date=2021 |title=Relationship Between the Ozone and Water Vapor Columns on Mars as Observed by SPICAM and Calculated by a Global Climate Model |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2021JE006838 |journal=Journal of Geophysical Research: Planets |language=en |volume=126 |issue=4 |pages=e2021JE006838 |doi=10.1029/2021JE006838 |bibcode=2021JGRE..12606838L |issn=2169-9100}}</ref>
* In November 2021, an experiment was performed to test whether ''Mars Express'' and the [[Trace Gas Orbiter|TGO]] lander relay communications radio could be used to perform [[radio occultation]] science,<ref>{{Cite web |title=ESA Mars orbiters: two-for-one science – Mars Express |url=https://blogs.esa.int/mex/2021/11/17/esa-mars-orbiters-two-for-one-science/ |access-date=April 11, 2022 }}</ref> as well as a series of tests of data relay from the CNSA [[Zhurong rover|''Zhurong'' rover]].<ref>{{Cite web |title=Mars Express keeps an ear out for Chinese rover – Mars Express |url=https://blogs.esa.int/mex/2021/10/27/mars-express-keeps-an-ear-out-for-chinese-rover/ |access-date=April 11, 2022 }}</ref>

==== 2022 ====
* In February 2022, a study was published in ''[[Earth and Planetary Science Letters]]'' demonstrating that liquid brines (water with [[perchlorate]] and [[chloride]]) are the best explanation for the [[MARSIS]] observations from 2018 interpreted as liquid water under the South pole of Mars. Such brines might not form actual underground lakes but could exist between grains of ice or sediment.<ref>{{Cite web |last= |first= |date=2022-01-26 |title=Brine-Ice Mixtures Exist beneath Martian South Polar Cap: Study {{!}} Sci.News |url=https://www.sci.news/space/brine-ice-mixtures-martian-south-polar-cap-10491.html |access-date=2025-06-01 |website=Sci.News: Breaking Science News |language=en-US}}</ref><ref>{{Cite journal |last1=Mattei |first1=Elisabetta |last2=Pettinelli |first2=Elena |last3=Lauro |first3=Sebastian Emanuel |last4=Stillman |first4=David E. |last5=Cosciotti |first5=Barbara |last6=Marinangeli |first6=Lucia |last7=Tangari |first7=Anna Chiara |last8=Soldovieri |first8=Francesco |last9=Orosei |first9=Roberto |last10=Caprarelli |first10=Graziella |date=2022-02-01 |title=Assessing the role of clay and salts on the origin of MARSIS basal bright reflections |url=https://www.sciencedirect.com/science/article/pii/S0012821X22000061 |journal=Earth and Planetary Science Letters |volume=579 |pages=117370 |doi=10.1016/j.epsl.2022.117370 |bibcode=2022E&PSL.57917370M |issn=0012-821X|url-access=subscription }}</ref>
* On 14 February 2022, ''Mars Express'' observed a rare astronomical event — [[Deimos (moon)|Deimos]] passing in front of Jupiter and its [[Galilean moons]]. Measuring the duration of the occultation enabled a more precise determination of the position and orbit of Deimos.<ref>{{Cite web |last= |first= |date=2022 |title=Mars Express Observes Rare Celestial Alignments in Solar System {{!}} Sci.News |url=https://www.sci.news/space/mars-express-alignments-11295.html |access-date=2025-06-01 |website=Sci.News: Breaking Science News |language=en-US}}</ref>
* In June 2022, the [[MARSIS]] instrument was upgraded from the original software based on [[Windows 98]] to "Mars 2022" in order to improve the performance of the instrument and to push its performance beyond some of the old limitations.<ref>{{Cite web |title=Software Upgrade for 19-Year-Old Martian Water-Spotter |url=https://www.esa.int/Enabling_Support/Operations/Software_upgrade_for_19-year-old_martian_water-spotter |access-date=July 2, 2022 }}</ref><ref>{{Cite web |title=This Mars Orbiter Is Finally Getting A Software Update From Windows 98 |date=June 29, 2022 |url=https://www.slashgear.com/912406/this-mars-orbiter-is-finally-getting-a-software-update-from-windows-98/ |access-date=July 2, 2022 }}</ref>
* On 23 September 2022, ''Mars Express'' conducted a close flyby of [[Phobos (moon)|Phobos]] and used the [[MARSIS]] instrument to probe the moon's subsurface structure from as close as 83 km. Operating MARSIS at such close distance was enabled by the recent software upgrade. The instrument was originally designed for studying Mars – at more than 250 km from the spacecraft.<ref>{{Cite web |title=A close encounter with a mysterious moon |url=https://www.esa.int/Enabling_Support/Operations/A_close_encounter_with_a_mysterious_moon |access-date=2025-06-01 |website=www.esa.int |language=en}}</ref>
* In November 2022, ''Mars Express'' performed data relay tests with NASA ''[[Perseverance (rover)|Perseverance]]'' rover, bringing the total number of other spacecraft supported by ''Mars Express'' in this way up to a record-breaking seven.<ref>{{Cite web |title=Mars Express sets data relay record |url=https://www.esa.int/Enabling_Support/Operations/Mars_Express_sets_data_relay_record |access-date=2025-06-01 |website=www.esa.int |language=en}}</ref>

==== 2023 ====
* In January 2023, the first global high-resolution map of aqueous minerals (formed through interaction with water) at Mars was published using data from ''Mars Express''<nowiki/>' OMEGA and [[Mars Reconnaissance Orbiter|MRO]]'s CRISM instruments.<ref>{{Cite web |title=New water map of Mars will prove invaluable for future exploration |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/New_water_map_of_Mars_will_prove_invaluable_for_future_exploration |access-date=2025-05-18 |website=www.esa.int |language=en}}</ref><ref>{{Cite journal |last1=Carter |first1=John |last2=Riu |first2=Lucie |last3=Poulet |first3=François |last4=Bibring |first4=Jean-Pierre |last5=Langevin |first5=Yves |last6=Gondet |first6=Brigitte |date=2023 |title=A Mars orbital catalog of aqueous alteration signatures (MOCAAS) |url=https://linkinghub.elsevier.com/retrieve/pii/S0019103522002664 |journal=Icarus |language=en |volume=389 |pages=115164 |doi=10.1016/j.icarus.2022.115164|bibcode=2023Icar..38915164C }}</ref>
* June 3: To celebrate the 20th anniversary of the spacecraft's launch, a [[livestream]] of images from the [[Visual Monitoring Camera]] was streamed online, marking the first livestream direct from Mars.<ref>{{Cite web |title=Tune in for first Mars livestream |url=https://www.esa.int/Enabling_Support/Operations/Tune_in_for_first_Mars_livestream |access-date=June 2, 2023 }}</ref>

=== Third decade ===
[[File:Olympus Mons - ESA Mars Express.png|thumb|[[Olympus Mons]] - ESA ''Mars Express'' [[High Resolution Stereo Camera|HRSC instrument]] image]]

==== 2024 ====
* Published in January 2024, a new research analysed [[MARSIS]] radar data collected over the preceding decade and concluded that the [[Medusae Fossae Formation]] at Mars equator, previously thought to be likely composed of dry deposits, instead includes a large amount of water ice.<ref>{{Cite web |title=Buried water ice at Mars's equator? |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/Buried_water_ice_at_Mars_s_equator |access-date=2025-05-18 |website=www.esa.int |language=en}}</ref><ref>{{Cite journal |last1=Watters |first1=Thomas R. |last2=Campbell |first2=Bruce A. |last3=Leuschen |first3=Carl J. |last4=Morgan |first4=Gareth A. |last5=Cicchetti |first5=Andrea |last6=Orosei |first6=Roberto |last7=Plaut |first7=Jeffrey J. |date=2024 |title=Evidence of Ice-Rich Layered Deposits in the Medusae Fossae Formation of Mars |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023GL105490 |journal=Geophysical Research Letters |language=en |volume=51 |issue=2 |pages=e2023GL105490 |doi=10.1029/2023GL105490 |bibcode=2024GeoRL..5105490W |issn=1944-8007|doi-access=free }}</ref>

* In May 2024, computers on ''Mars Express'' (as well as on another ESA mission, ''[[BepiColombo]]'') reported a sharp increase in the number of memory errors, coinciding with a massive [[solar flare]].<ref>{{Cite web |title=Can't stop won't stop: Solar Orbiter shows the Sun raging on |url=https://www.esa.int/Science_Exploration/Space_Science/Solar_Orbiter/Can_t_stop_won_t_stop_Solar_Orbiter_shows_the_Sun_raging_on |access-date=2025-05-18 |website=www.esa.int |language=en}}</ref>
* In June 2024, a new study was published in ''[[Nature Geoscience]]'', providing first evidence for water frost near Mars equator, specificaly atop the [[Tharsis]] volcanoes. This work used data from ESA's ''Mars Express'' and [[Trace Gas Orbiter|TGO]] missions.<ref>{{Cite web |date=2024-07-01 |title=Surprising Discovery of Frost on Martian Volcanoes Near Equator – "Thought Impossible" |url=https://scitechdaily.com/surprising-discovery-of-frost-on-martian-volcanoes-near-equator-thought-impossible/ |access-date=2025-05-18 |website=SciTechDaily |language=en-US}}</ref><ref>{{Cite journal |last1=Valantinas |first1=A. |last2=Thomas |first2=N. |last3=Pommerol |first3=A. |last4=Karatekin |first4=O. |last5=Ruiz Lozano |first5=L. |last6=Senel |first6=C. B. |last7=Temel |first7=O. |last8=Hauber |first8=E. |last9=Tirsch |first9=D. |last10=Bickel |first10=V. T. |last11=Munaretto |first11=G. |last12=Pajola |first12=M. |last13=Oliva |first13=F. |last14=Schmidt |first14=F. |last15=Thomas |first15=I. |date=2024 |title=Evidence for transient morning water frost deposits on the Tharsis volcanoes of Mars |url=https://www.nature.com/articles/s41561-024-01457-7 |journal=Nature Geoscience |language=en |volume=17 |issue=7 |pages=608–616 |doi=10.1038/s41561-024-01457-7 |bibcode=2024NatGe..17..608V |issn=1752-0908}}</ref>
* In July 2024, a study was published in ''[[Radio Science]]'' documenting the first routine use of mutual [[radio occultation]] technique at another planet, specifically the measurements of physical properties of the [[Atmosphere of Mars|Martian atmosphere]] conducted using a radio link between ESA's ''Mars Express'' and [[Trace Gas Orbiter|TGO]] orbiters between 2020 and 2023.<ref>{{Cite web |last1=Dunning |first1=Hayley |last2=London |first2=Imperial College |title=Repurposed technology used to probe new regions of Mars' atmosphere |url=https://phys.org/news/2024-07-repurposed-technology-probe-regions-mars.html |access-date=2025-05-18 |website=phys.org |language=en}}</ref><ref>{{Cite journal |last1=Parrott |first1=Jacob |last2=Svedhem |first2=Håkan |last3=Witasse |first3=Olivier |last4=Wilson |first4=Colin |last5=Müller-Wodarg |first5=Ingo |last6=Cardesín-Moinelo |first6=Alejandro |last7=Schmitz |first7=Peter |last8=Godfrey |first8=James |last9=Reboud |first9=Olivier |last10=Geiger |first10=Bernhard |last11=Sánchez-Cano |first11=Beatriz |last12=Nava |first12=Bruno |last13=Migoya-Orué |first13=Yenca |date=2024 |title=First Results of Mars Express—ExoMars Trace Gas Orbiter Mutual Radio Occultation |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023RS007873 |journal=Radio Science |language=en |volume=59 |issue=7 |pages=e2023RS007873 |doi=10.1029/2023RS007873 |bibcode=2024RaSc...5907873P |issn=1944-799X|hdl=10261/371076 |hdl-access=free }}</ref>

* In September 2024, a new cloud atlas of Mars has been published, containing images of Martian clouds by ''Mars Express'' from the past 20 years.<ref>{{Cite web |last=Anderson |first=Paul Scott |date=2024-09-18 |title=New Cloud Atlas of Mars for cloudspotting on the red planet |url=https://earthsky.org/space/cloud-atlas-of-mars-clouds-dust-storms/ |access-date=2025-05-18 |website=earthsky.org |language=en-US}}</ref><ref>{{Cite report |url=https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-44.html |title=Clouds and Storms as seen by HRSC - A catalogue of atmospheric phenomena on Mars |last1=Tirsch |first1=Daniela |last2=Machado |first2=Pedro |last3=Brasil |first3=Francisco |last4=Hernández-Bernal |first4=Jorge |last5=Sánchez-Lavega |first5=Agustín |last6=Carter |first6=John |last7=Montmessin |first7=Franck |last8=Hauber |first8=Ernst |last9=Matz |first9=Klaus-Dieter |date=2024-07-03 |publisher=Copernicus Meetings |issue=EPSC2024-44 |doi=10.5194/epsc2024-44 |doi-access=free |language=en}}</ref>

==== 2025 ====
* In February 2025, a study was published in ''[[Nature Communications]]'' suggesting that the red color of Mars is caused by iron oxides containing water, known as [[ferrihydrite]], and not by [[hematite]] that forms under dry conditions, as thought before. This work used data from ''Mars Express'' and other spacecraft.<ref>{{Cite web |title=Have we been wrong about why Mars is red? |url=https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/Have_we_been_wrong_about_why_Mars_is_red |access-date=2025-05-18 |website=www.esa.int |language=en}}</ref><ref>{{Cite journal |last1=Valantinas |first1=Adomas |last2=Mustard |first2=John F. |last3=Chevrier |first3=Vincent |last4=Mangold |first4=Nicolas |last5=Bishop |first5=Janice L. |last6=Pommerol |first6=Antoine |last7=Beck |first7=Pierre |last8=Poch |first8=Olivier |last9=Applin |first9=Daniel M. |last10=Cloutis |first10=Edward A. |last11=Hiroi |first11=Takahiro |last12=Robertson |first12=Kevin |last13=Pérez-López |first13=Sebastian |last14=Ottersberg |first14=Rafael |last15=Villanueva |first15=Geronimo L. |date=2025-02-25 |title=Detection of ferrihydrite in Martian red dust records ancient cold and wet conditions on Mars |journal=Nature Communications |language=en |volume=16 |issue=1 |pages=1712 |doi=10.1038/s41467-025-56970-z |pmid=40000645 |pmc=11861699 |bibcode=2025NatCo..16.1712V |issn=2041-1723}}</ref>
* In May 2025, ESA updated the software solution from 2018 which was meant to prolong the lifetime of the spacecraft's gyroscopes. This new update could allow ''Mars Express'' to stay operational until 2034 and be ready to support the [[Martian Moons eXploration|MMX spacecraft]] in 2029.<ref>{{Cite web |title=Mars Express updates software, extends lifetime until 2034 |url=https://www.esa.int/Enabling_Support/Operations/Mars_Express_updates_software_extends_lifetime_until_2034 |access-date=2025-05-17 |website=www.esa.int |language=en}}</ref>
* In June 2025, a comprehensive data set from ''Mars Express''—[[Trace Gas Orbiter|TGO]] [[radio occultation]] observations has been made publicly available with a publication of a new study in [[JGR Planets]] analysing 71 full vertical profiles from such observations.<ref>{{Cite web |last=Stanley |first=Sarah |date=2025-06-20 |title=Orbiter Pair Expands View of Martian Ionosphere |url=https://eos.org/research-spotlights/orbiter-pair-expands-view-of-martian-ionosphere |access-date=2025-06-21 |website=Eos |language=en-US}}</ref><ref>{{Cite journal |last=Parrott |first=Jacob |last2=Svedhem |first2=Håkan |last3=Sánchez‐Cano |first3=Beatriz |last4=Witasse |first4=Olivier |last5=Wilson |first5=Colin |last6=Müller‐Wodarg |first6=Ingo |date=2025 |title=Ionospheric Analysis With Martian Mutual Radio Occultation |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JE008854 |journal=Journal of Geophysical Research: Planets |language=en |volume=130 |issue=6 |doi=10.1029/2024JE008854 |issn=2169-9097|doi-access=free }}</ref>

== See also ==
{{Portal|Spaceflight}}

* [[List of European Space Agency programmes and missions]]
* [[European Space Agency]]
* [[ExoMars]]
* [[Exploration of Mars]]
* [[List of Mars orbiters]]
* [[List of missions to Mars]]
* [[Space exploration]]
* [[Uncrewed space mission]]

== References ==
{{Reflist}}

== External links ==
{{Commons category}}
* [http://www.esa.int/Our_Activities/Space_Science/Mars_Express ''ESA Mars Express'' project] – official website
* [http://sci.esa.int/marsexpress/ ''ESA Mars Express'' project] – scientific website
* [http://www.esa.int/SPECIALS/Operations/SEM0RMQJNVE_0.html ''ESA Mars Express'' operations site]
* [http://mars.jpl.nasa.gov/express/gallery/artwork/ NASA Art Gallery of Mars Express]
* [https://www.eoportal.org/other-space-activities/mars-express-1 Mars Express article on eoPortal by ESA]

===Payload principal investigators links===
* HRSC [http://www.geoinf.fu-berlin.de/eng/projects/mars/index.php Mars Express FU Berlin]
* [http://www.marsis.com MARSIS] Uni Roma "La Sapienza"
* [http://www.uni-koeln.de/math-nat-fak/geomet/geo/index.html?/mitarbeiter/mitarb/mp.html MRSE] Uni Köln
* [http://www.aspera-3.org/ ASPERA]

{{Marsexpress}}
{{ESA projects}}
{{Planetary Missions Program Office|Discovery=y}}
{{Mars spacecraft}} 
{{Solar System probes}}
{{Orbital launches in 2003}}
{{Portal bar|Solar System}}

[[Category:Mars Express| ]]
[[Category:Attached spacecraft]]
[[Category:European Space Agency space probes|Mars Express]]
[[Category:Geography of Mars]]
[[Category:Missions to Mars|Express]]
[[Category:Satellites orbiting Mars|Express]]
[[Category:Spacecraft launched by Soyuz-FG rockets]]
[[Category:Space probes launched in 2003|Mars Express]]