Mars Orbiter Mission

Indian space probe, launched in 2013

Mars Orbiter Mission
Mars Orbiter Mission spacecraft around Mars (illustration)
NamesMars Orbiter Mission, MOM, Mangalyaan
Mission typeMars orbiter
OperatorISRO
COSPAR ID2013-060A Edit this at Wikidata
SATCAT no.39370
Websitewww.isro.gov.in/pslv-c25-mars-orbiter-mission
Mission durationPlanned: 6 months[1]
Final: 7 years, 6 months, 8 days
Spacecraft properties
BusI-1K[2]
ManufacturerU R Rao Satellite Centre
Launch mass1,337.2 kg (2,948 lb)[3]
BOL mass≈550 kg (1,210 lb)[4]
Dry mass482.5 kg (1,064 lb)[3]
Payload mass13.4 kg (30 lb)[3]
Dimensions1.5 m (4.9 ft) cube
Power840 watts[2]
Start of mission
Launch date5 November 2013, 09:08 (2013-11-05UTC09:08) UTC[5][6]
RocketPSLV-XL C25[7]
Launch siteSatish Dhawan Space Centre, FLP
ContractorISRO
End of mission
Last contactApril 2022[8]
Mars orbiter
Orbital insertion24 September 2014, 02:10 UTC (7:40 IST)[9][10]
MSD 50027 06:27 AMT
3519 days / 3426 sols
Orbital parameters
Periareon altitude421.7 km (262.0 mi)[9]
Apoareon altitude76,993.6 km (47,841.6 mi)[9]
Inclination150.0°[9]
Instruments
MCCMars Colour Camera
TISThermal Infrared Imaging Spectrometer
MSMMethane Sensor for Mars
MENCAMars Exospheric Neutral Composition Analyser
LAPLyman Alpha Photometer

Insignia depicting journey from Earth to an elliptical Martian orbit using Mars symbol
Mars Orbiter Mission 2 →
 

The Mars Orbiter Mission (MOM), unofficially known as Mangalyaan[11] (from Sanskrit Maṅgala, 'Mars', and yāna, 'craft, vehicle'),[12][13] was a space probe orbiting Mars since 24 September 2014. It was launched on 5 November 2013 by the Indian Space Research Organisation (ISRO).[14][15][16][17] It was India's first interplanetary mission[18] and it made ISRO the fourth space agency to achieve Mars orbit, after Roscosmos, NASA, and the European Space Agency.[19] It made India the first Asian nation to reach the Martian orbit and the first nation in the world to do so on its maiden attempt.[20][21][22][23]

The Mars Orbiter Mission probe lifted off from the First Launch Pad at Satish Dhawan Space Centre (Sriharikota Range SHAR), Andhra Pradesh, using a Polar Satellite Launch Vehicle (PSLV) rocket C25 at 09:08 (UTC) on 5 November 2013.[5][24] The launch window was approximately 20 days long and started on 28 October 2013.[6] The MOM probe spent about a month in Earth orbit, where it made a series of seven apogee-raising orbital manœuvres before trans-Mars injection on 30 November 2013 (UTC).[25] After a 298-day transit to Mars, it was put into Mars orbit on 24 September 2014.

The mission was a technology demonstrator project to develop the technologies for designing, planning, management, and operations of an interplanetary mission.[26] It carried five scientific instruments.[27] The spacecraft was monitored from the Spacecraft Control Centre at ISRO Telemetry, Tracking and Command Network (ISTRAC) in Bengaluru with support from the Indian Deep Space Network (IDSN) antennae at Bengaluru, Karnataka.[28]

On 2 October 2022, it was reported that the orbiter had irrecoverably lost communications with Earth after entering a seven-hour eclipse period in April 2022 that it was not designed to survive.[29][30][31] The following day, ISRO released a statement that all attempts to revive MOM had failed and officially declared it dead, citing the loss of fuel and battery power to the probe's instruments.[32]

History

Mars Orbiter Mission spacecraft during encapsulation

In November 2008, the first public acknowledgement of an uncrewed mission to Mars was announced by then-ISRO chairman G. Madhavan Nair.[33] The MOM mission concept began with a feasibility study in 2010 by the Indian Institute of Space Science and Technology after the launch of lunar satellite Chandrayaan-1 in 2008. Prime Minister Manmohan Singh approved the project on 3 August 2012,[34][35] after the Indian Space Research Organisation completed 125 crore (US$16 million) of required studies for the orbiter.[36] The total project cost may be up to 454 crore (US$57 million).[14][37] The satellite costs 153 crore (US$19 million) and the rest of the budget has been attributed to ground stations and relay upgrades that will be used for other ISRO projects.[38]

The space agency had planned the launch on 28 October 2013 but was postponed to 5 November following the delay in ISRO's spacecraft tracking ships to take up pre-determined positions due to poor weather in the Pacific Ocean.[6] Launch opportunities for a fuel-saving Hohmann transfer orbit occur every 26 months, in this case the next two would be in 2016 and 2018.[39]

Assembly of the PSLV-XL launch vehicle, designated C25, started on 5 August 2013.[40] The mounting of the five scientific instruments was completed at Indian Space Research Organisation Satellite Centre, Bengaluru, and the finished spacecraft was shipped to Sriharikota on 2 October 2013 for integration to the PSLV-XL launch vehicle.[40] The satellite's development was fast-tracked and completed in a record 15 months,[41] partly due to using reconfigured Chandrayaan-2 orbiter bus.[42] Despite the US federal government shutdown, NASA reaffirmed on 5 October 2013 it would provide communications and navigation support to the mission "with their Deep Space Network facilities.".[43] During a meeting on 30 September 2014, NASA and ISRO officials signed an agreement to establish a pathway for future joint missions to explore Mars. One of the working group's objectives will be to explore potential coordinated observations and science analysis between the MAVEN orbiter and MOM, as well as other current and future Mars missions.[44]

On 2 October 2022, it was reported that the orbiter had irrecoverably lost communications with Earth after entering long eclipse period in April 2022 that it was not designed to survive. At the time of communications loss it was unknown whether the probe had lost power or inadvertently realigned its Earth-facing antenna during automatic maneuvers.[29]

Team

Some of the scientists of isro and engineers involved in the mission include:[45]

  • K. Radhakrishnan led as Chairman ISRO.
  • S. K. Shivakumar was the Director at the ISRO Satellite Centre. He was also a Project Director for the Indian Deep Space Network. Mars Orbiter Mission is the product of ISRO Satellite Centre (ISAC). He spearheaded the task of conceptualization, design and realization of the unique spacecraft MOM. He ingeniously planned to realize the spacecraft in a record time of 15 months
  • Mylswamy Annadurai was the Programme Director and was in charge of budget management as well as direction for spacecraft configuration, schedule and resources.
  • Subbiah Arunan was the Project Director at the Mars Orbiter Mission.
  • B Jayakumar was an Associate Project Director at the PSLV programme which was responsible for testing the rocket systems.
  • S Ramakrishnan was the Director who helped in the development of the liquid propulsion system of the PSLV launcher.
  • P. Kunhikrishnan was the Project Director in the PSLV programme. He was also a Mission director of the PSLV-C25/Mars Orbiter Mission.
  • Moumita Dutta was the Project manager of the Mars Orbiter Mission.
  • Nandini Harinath was the Deputy Operations Director of Navigation.
  • Ritu Karidhal was the Deputy Operations Director of Navigation.
  • BS Kiran was the Associate Project Director of Flight Dynamics.
  • V Kesava Raju was the Mars Orbiter Mission Director.
  • V Koteswara Rao was the ISRO scientific secretary.
  • Chandradathan was the Director of the Liquid Propulsion System.
  • A. S. Kiran Kumar was the Director of the Satellite Application Centre, who later went on to be the Chairman ISRO after this, when the team studied the Mard
  • M. Y. S. Prasad is the Director at Satish Dhawan Space Centre. He was also the chairman of the Launch Authorisation Board.
  • MS Pannirselvam was the Chief General Manager at the Sriharikota Rocket port and was tasked to maintain launch schedules.

Cost

The total cost of the mission was approximately 450 Crore (US$73 million),[46][47] making it the least-expensive Mars mission to date.[48] The low cost of the mission was ascribed by ISRO chairman K. Radhakrishnan to various factors, including a "modular approach", few ground tests and long working days (18 to 20 hours) for scientists.[49] BBC's Jonathan Amos specified lower worker costs, home-grown technologies, simpler design, and a significantly less complicated payload than NASA's MAVEN.[27]

Mission objectives

Rendering of the Mars Orbiter Mission spacecraft.

The primary objective of the mission is to develop the technologies required for designing, planning, management and operations of an interplanetary mission.[26] The secondary objective is to explore Mars' surface features, morphology, mineralogy and Martian atmosphere using indigenous scientific instruments.[50]

The main objectives are to develop the technologies required for designing, planning, management and operations of an interplanetary mission comprising the following major tasks:[51]: 42 

  • Orbit manoeuvres to transfer the spacecraft from Earth-centred orbit to heliocentric trajectory and finally, capture into Martian orbit
  • Development of force models and algorithms for orbit and attitude (orientation) computations and analysis
  • Navigation in all phases
  • Maintain the spacecraft in all phases of the mission
  • Meeting power, communications, thermal and payload operation requirements
  • Incorporate autonomous features to handle contingency situations

Scientific objectives

The scientific objectives deal with the following major aspects:[51]: 43 

  • Exploration of Mars surface features by studying the morphology, topography and mineralogy
  • Study the constituents of Martian atmosphere including methane and CO2 using remote sensing techniques
  • Study the dynamics of the upper atmosphere of Mars, effects of solar wind and radiation and the escape of volatiles to outer space

The mission would also provide multiple opportunities to observe the Martian moon Phobos and also offer an opportunity to identify and re-estimate the orbits of asteroids seen during the Martian Transfer Trajectory.[51]: 43  The spacecraft also provided the first views ever of the far side of Martian Moon Deimos.

Studies

In May–June 2015 Indian scientists got an opportunity to study the Solar Corona during the Mars conjunction when earth and Mars are on the opposite sides of the sun. During this period the S band waves emitted by MOM were transmitted through the Solar Corona that extends millions of kms into space. This event helped scientists study the Solar surface and regions where temperature changed abruptly.[52]

Spacecraft design

  • Mass: The lift-off mass was 1,337.2 kg (2,948 lb), including 852 kg (1,878 lb) of propellant.[3]
  • Bus: The spacecraft's bus is a modified I-1 K structure and propulsion hardware configuration, similar to Chandrayaan-1, India's lunar orbiter that operated from 2008 to 2009, with specific improvements and upgrades needed for a Mars mission.[50] The satellite structure is constructed of an aluminium and composite fibre reinforced plastic (CFRP) sandwich construction.[53]
  • Power: Electric power is generated by three solar array panels of 1.8 m × 1.4 m (5 ft 11 in × 4 ft 7 in) each (7.56 m2 (81.4 sq ft) total), for a maximum of 840 watts of power generation in Mars orbit. Electricity is stored in a 36 Ah Lithium-ion battery.[2][54]
  • Propulsion: A liquid fuel engine with a thrust of 440 newtons (99 lbf) is used for orbit raising and insertion into Mars orbit. The orbiter also has eight 22-newton (4.9 lbf) thrusters for attitude control (orientation).[55] Its propellant mass at launch was 852 kg (1,878 lb).[2]
  • Attitude and Orbit Control System: Maneuvering system that includes electronics with a MAR31750 processor, two star sensors, a solar panel Sun sensor, a coarse analog Sun sensor, four reaction wheels, and the primary propulsion system.[2][56]
  • Antennae: Low gain antenna, mid gain antenna, and high gain antenna.[2]

Scientific instruments

Scientific instruments
LAP Lyman-Alpha Photometer 1.97 kg (4.3 lb)
MSM Methane Sensor for Mars [57] 2.94 kg (6.5 lb)
MENCA Mars Exospheric Neutral
Composition Analyser
3.56 kg (7.8 lb)
TIS Thermal Infrared Imaging Spectrometer 3.20 kg (7.1 lb)
MCC Mars Colour Camera 1.27 kg (2.8 lb)
Animated assembly of Mars Orbiter Mission spacecraft

The 15 kg (33 lb) scientific payload consists of five instruments:[58][59][60]

  • Atmospheric studies:
    • Lyman-Alpha Photometer (LAP) – a photometer that measures the relative abundance of deuterium and hydrogen from Lyman-alpha emissions in the upper atmosphere. Measuring the deuterium/hydrogen ratio will allow an estimation of the amount of water loss to outer space. The nominal plan to operate LAP is between the ranges of approximately 3,000 km (1,900 mi) before and after Mars periapsis. Minimum observation duration for achieving LAP's science goals is 60 minutes per orbit during normal range of operation. The objectives of this instrument are as follows:[51]: 56, 57 
      • Estimation of D/H ratio
      • Estimation of escape flux of H2 corona
      • Generation of hydrogen and deuterium coronal profiles.
    • Methane Sensor for Mars (MSM) – was meant to measure methane in the atmosphere of Mars, if any, and map its sources with an accuracy of few 10s parts-per-billion (ppb).[58] After entering Mars orbit it was determined that the instrument, although in good working condition, had a design flaw and it was incapable of distinguishing methane on Mars. The instrument can accurately map Mars albedo at 1.65 um.[57][61]
      • MSM Design Flaw. The MSM sensor was expected to measure methane in the Mars atmosphere; methane on Earth is often associated with life. However, after it entered orbit, it was reported that there was an issue with how it collected and processed data. The spectrometer could measure intensity of different spectral bands, [such as methane] but instead of sending back the spectra, it sent back the sum of the sampled spectra and also the gaps between the sampled lines. The difference was supposed to be the methane signal, but since other spectra such as carbon dioxide could have varying intensities, it was not possible to determine the actual methane intensity. The device was repurposed as an albedo mapper.[62]
  • Particle environment studies:
    • Mars Exospheric Neutral Composition Analyser (MENCA) – is a quadrupole mass analyser capable of analysing the neutral composition of particles in the range of 1–300 amu (atomic mass unit) with unit mass resolution. The heritage of this payload is from Chandra's Altitudinal Composition Explorer (CHACE) payload aboard the Moon Impact Probe (MIP) in Chandrayaan-1 mission. MENCA is planned to perform five observations per orbit with one hour per observation.[51]: 58 
  • Surface imaging studies:
    • Thermal Infrared Imaging Spectrometer (TIS) – TIS measures the thermal emission and can be operated during both day and night. It would map surface composition and mineralogy of Mars and also monitor atmospheric CO2 and turbidity (required for the correction of MSM data). Temperature and emissivity are the two basic physical parameters estimated from thermal emission measurement. Many minerals and soil types have characteristic spectra in TIR region. TIS can map surface composition and mineralogy of Mars.[51]: 59 
    • Mars Colour Camera (MCC) – This tricolour camera gives images and information about the surface features and composition of Martian surface. It is useful to monitor the dynamic events and weather of Mars like dust storms/atmospheric turbidity. MCC will also be used for probing the two satellites of Mars, Phobos and Deimos. MCC would provide context information for other science payloads. MCC images are to be acquired whenever MSM and TIS data is acquired. Seven Apoareion Imaging of the entire disc and multiple Periareion images of 540 km × 540 km (340 mi × 340 mi) are planned in every orbit.[51]: 58 

Telemetry and command

The ISRO Telemetry, Tracking and Command Network performed navigation and tracking operations for the launch with ground stations at Sriharikota and Port Blair in India, Brunei and Biak in Indonesia,[63] and after the spacecraft's apogee became more than 100,000 km, an 18 m (59 ft) and a 32 m (105 ft) diameter antenna of the Indian Deep Space Network were utilised.[64] The 18 m (59 ft) dish antenna was used for communication with the craft until April 2014, after which the larger 32 m (105 ft) antenna was used.[65] NASA's Deep Space Network is providing position data through its three stations located in Canberra, Madrid and Goldstone on the US West Coast during the non-visible period of ISRO's network.[66] The South African National Space Agency's (SANSA) Hartebeesthoek (HBK) ground station is also providing satellite tracking, telemetry and command services.[67]

Communications

Communications are handled by two 230-watt TWTAs and two coherent transponders. The antenna array consists of a low-gain antenna, a medium-gain antenna and a high-gain antenna. The high-gain antenna system is based on a single 2.2-metre (7 ft 3 in) reflector illuminated by a feed at S-band. It is used to transmit and receive the telemetry, tracking, commanding and data to and from the Indian Deep Space Network.[2]

Mission profile

Timeline of Operations
Phase Date Event Detail Result References
Geocentric phase 5 November 2013 09:08 UTC Launch Burn time: 15:35 min in 5 stages Apogee: 23,550 km (14,630 mi) [68]
6 November 2013 19:47 UTC Orbit raising manoeuvre Burn time: 416 sec Apogee: 28,825 km (17,911 mi) [69]
7 November 2013 20:48 UTC Orbit raising manoeuvre Burn time: 570.6 sec Apogee: 40,186 km (24,970 mi) [70][71]
8 November 2013 20:40 UTC Orbit raising manoeuvre Burn time: 707 sec Apogee: 71,636 km (44,513 mi) [70][72]
10 November 2013 20:36 UTC Orbit raising manoeuvre Incomplete burn Apogee: 78,276 km (48,638 mi) [73]
11 November 2013 23:33 UTC Orbit raising manoeuvre (supplementary) Burn time: 303.8 sec Apogee: 118,642 km (73,721 mi) [70]
15 November 2013 19:57 UTC Orbit raising manoeuvre Burn time: 243.5 sec Apogee: 192,874 km (119,846 mi) [70][74]
30 November 2013 19:19 UTC Trans-Mars injection Burn time: 1328.89 sec Heliocentric insertion [75]
Heliocentric phase December 2013 – September 2014 En route to Mars – The probe travelled a distance of 780,000,000 kilometres (480,000,000 mi) in a Hohmann transfer orbit[39] around the Sun to reach Mars.[65] This phase plan included up to four trajectory corrections if needed. [76][77][78][79][80]
11 December 2013 01:00 UTC 1st Trajectory correction Burn time: 40.5 sec Success [70][78][79][80]
9 April 2014 2nd Trajectory correction (planned) Not required Rescheduled for 11 June 2014 [77][80][81][82][83]
11 June 2014 11:00 UTC 2nd Trajectory correction Burn time: 16 sec Success [81][84]
August 2014 3rd Trajectory correction (planned) Not required[81][85] [77][80]
22 September 2014 3rd Trajectory correction Burn time: 4 sec Success [77][80][86]
Areocentric phase 24 September 2014 Mars orbit insertion Burn time: 1388.67 sec Success [9]
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