European Student Moon Orbiter

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The European Student Moon Orbiter (ESMO) was a proposed European student mission to the Moon. Student teams from 19 universities throughout Europe worked on the program. ESMO was conceived by the Student Space Exploration & Technology Initiative (SSETI) under the support of the European Space Agency (ESA); prior to the start of Phase A the full responsibility for the management of the program was transferred to the ESA Education Office.

In 2009, Surrey Satellite Technology Ltd (SSTL) was selected as prime contractor.[1] In April 2012, ESMO was scheduled for launch in 2014 or 2015,[1] but further ESA evaluation deemed the ESMO project's costs "unsustainable" given the ESA Education Office's budget.[2]

The mission objectives for ESMO were:[3]

  • To launch the first lunar spacecraft to be designed, built and operated by students across ESA Member States and ESA Cooperating States
  • To place and operate the spacecraft in a lunar orbit
  • To acquire images of the Moon from a stable lunar orbit and transmit them back to Earth for education outreach purposes
  • To perform new measurements relevant to advanced technology demonstration, lunar science and exploration

The educational aim of the project was to provide valuable hands-on experience to university students within a real space project. This is in order to fully prepare a qualified workforce for future ESA missions.[3]

Lunar transfer

The spacecraft of approximately 190 kg (420 lb) mass and a size of 76 × 74 × 74 cm (30 × 29 × 29 in) was designed to be launched as a secondary or auxiliary payload into Geostationary transfer orbit (GTO) in 2014/2015. From there, the spacecraft would use its on-board propulsion to travel to lunar orbit via a weak stability boundary transfer. This travel via the Sun-Earth L1 Lagrange point would take three months, but it requires much less propellant than a direct transfer (see Low energy transfer[4][5] and Interplanetary Transport Network).[1][3] ESMO is intended to be operated in lunar orbit for six months.

Payloads

Payloads that were considered for the orbiter included:[3]

  • Narrow Angle Camera (outreach payload): to take images of the lunar surface. High school students would have been able to propose a lunar site to be imaged.
  • LunaNet (technology demonstration payload): internet-like network at the Moon for communication between future spacecraft in lunar orbit, landers, rovers and ground stations on the Earth. The LunaNet experiment would have tested the associated communication protocols for the Lunar Internet.
  • Radiation Monitor (scientific payload): a compact and low power radiation monitor which could have provided inputs for space environment models.
  • Radar (scientific payload): to provide radar observations of the Moon (radar observations from Earth are limited to the Earth-facing side of the Moon).
  • Microwave Radiometric Sounder (scientific payload): a passive microwave radiometer to measure thermal and dielectric properties of the lunar regolith.

Technical facts

The table below provides an overview of the planned spacecraft platform and the ground segment.[3]

Subsystem Description
Attitude Determination and Control System (ADCS) 3-axis stabilized: 2 star trackers, 4 Sun sensors, 2 inertial measurement units, 4 reaction wheels, 8 cold gas thrusters
On-board Data Handling 2 ESA LEON2 processors (dual redundant) running data handling software (command timeline and simple FDIR) and ADCS software; 32 MB Serial Flash for payload data storage; CANbus data interfaces
Communications Low Gain Antennas for omni-directional coverage; S-band transponder with PSK-PM modulation and range and range rate capability for radio-navigation; 8 kbit/s downlink / 4 kbit/s uplink between Moon and Earth stations
Power Body-mounted 3J GaAs solar cells for 170 W beginning of life power and 122 W end of life power; 24-29 V unregulated bus; 1800 Wh capacity Li-ion batteries
Propulsion 4 liquid MON/MMH bipropellant thrusters: 22 N thrust each, 285 s specific impulse (modulated by AOCS software during burns for reaction control)
Structure CFRP/Al honeycomb construction box with load bearing central thrust tube
Thermal Control Passive: MLI and surface coatings; active: local heaters for eclipse (e.g. propellant tanks)
Ground Segment Ground stations: 25m S-band dish in Raisting and 15m S-band dish in Villafranca; Perth/Kourou for launch and early orbit phase and manoeuvres

Participating teams

References

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