30b1c8486525c3c9a6315fa302ff46b6.ppt
- Количество слайдов: 22
Moon. LITE and Lunar. EX Rob Gowen and Alan Smith Mullard Space Science Laboratory, UCL PI Penetrator consortium space for science, enterprise and environment
Mullard Space Science Laboratory • • • A department of University College London Established in 1967 >200 sounding rockets and >35 satellite missions 150 Staff and research students Provided hardware or calibration facilities for 16 instruments on 14 spacecraft currently operating including NASA Swift, Cassini, Soho • In-house mechanical and electrical engineering design, manufacture and test • Provided stereo cameras for Beagle-2 • Leading Pan. Cam development for EXOMARS Hinode Launch 22 -9 -06 space for science, enterprise and environment
Consortium • Birkbeck College London – Lunar Science (Ian Crawford) • Open University – Large academic planetary group (Cassini Huygens Probe) – Science and instrumentation (Ion trap spectrometer, etc) • Imperial College London – Micro-Seismometers • Surrey Space Science Centre and SSTL – Platform technologies, delivery system technologies – Payload technologies (drill) space for science, enterprise and environment
Consortium • Southampton University – Optical fibres • University of Leicester – XRS (beagle 2/Mars 96) • Aberystwyth – Science (Chandrayaan-1) • Qineti. Q – Impact technologies – Platform & delivery systems technologies • Astrium (in discussion) – Platform & delivery systems technologies space for science, enterprise and environment
What are Penetrators ? • • • Instrumented projectiles Survive high speed impact ~ 300 m/s Penetrate surface ~ few metres An alternative to soft landing Lower cost and low mass => multi-site deployment space for science, enterprise and environment
Penetrator Heritage • Lunar-A – tested but not yet flown • DS-2 – tested but failed at Mars • Mars-96 – lower speed impact, tested but failed to leave Earth Orbit • Innumerable ground trials of instrumented shells • Validated impact modelling tools When asked to describe the condition of a probe that had impacted 2 m of concrete at 300 m/s a UK expert described the device as ‘a bit scratched’! Courtesy Qineti. Q space for science, enterprise and environment
Penetrator Design Concept Payload DETACHABLE PROPULSION STAGE • IMPACT ACCELEROMETER Platform • S/C SUPPORT • SEISMOMETERS/TILTMETER • AOCS • WATER/VOLATILES (ISRU DETECTION) • STRUCTURE • POWER/THERMAL • GEOCHEMISTRY • COMMS POINT OF SEPARATION • HEAT FLOW • CONTROL & DATA • DESCENT CAMERA HANDLING PAYLOAD INSTRUMENTS OR T RA ET N PE TM LE DU O DE N SCE ESTIMATED PENETRATOR SIZE • LENGTH: ~50 cm • DIAMETER: ~15 cm • MASS: ~10 -13 Kg space for science, enterprise and environment
Moon. LITE/Lunar. EX - Mission Description • Delivery and Communications Spacecraft (Orbiter). Deliver penetrators to ejection orbit, provide pre-ejection health status, and relay communications. • Orbiter Payload: 4 Descent Probes (each containing 10 -15 kg penetrator + 20 -25 kg de-orbit and attitude control). • Landing sites: Globally spaced Far side, Polar region(s), One near an Apollo landing site for calibration. • Duration: >1 year for seismic network. Other science does not require so long (perhaps a few Lunar cycles for heat flow and volatiles much less). • Penetrator Design: Single Body for simplicity and risk avoid. Ance. Battery powered with comprehensive power saving techniques. space for science, enterprise and environment
Moon. LITE/Lunar. EX – Mission Sequence • Launch & cruise phase • Deployment – Deploy descent probes from lunar orbit, using a de-orbit motor to achieve near vertical impact. – Attitude control to achieve orientation of penetrator to be aligned with velocity vector. – Penetration ~3 metres – Camera to be used during descent to characterize landing site – Telemetry transmission during descent for health status – Impact accelerometer (to determine penetration depth & regolith mechanical properties) • Landed Phase – Telemeter final descent images and accelerometer data – Perform and telemeter science for ~1 year. space for science, enterprise and environment
Moon. LITE/Lunar. EX – Mission Sequence • Launch & cruise phase • Deployment & descent • Landed phase space for science, enterprise and environment
Moon. LITE – Science The Origin and Evolution of Planetary Bodies Water and its profound implications for life and exploration NASA Lunar Prospector space for science, enterprise and environment
Science – Polar Volatiles A suite of instruments will detect and characterise volatiles (including water) within shaded craters at both poles • Astrobiologically important – possibly remnant of the orginal seeding of planets by comets – May provide evidence of important cosmic-ray mediated organic synsthesis • Vital to the future manned exploration of the Moon Prototype, ruggedized ion trap mass-spectrometer Open University NASA Lunar Prospector space for science, enterprise and environment
Science - Seismology A global network of seismometers will tell us: – – Size and physical state of the Lunar Core Structure of the Lunar Mantle Thickness of the far side crust The origin of the enigmatic shallow moonquakes – The seismic environment at potential manned landing sites space for science, enterprise and environment
Science - Geochemistry X-ray spectroscopy at multiple, diverse sites will address: – Lunar Geophysical diversity – Ground truth for remote sensing Leicester University XRS on Beagle-2 K, Ca, Ti, Fe, Rb, Sr, Zr space for science, enterprise and environment
Science – Heat Flow Heat flow measurements will be made at diverse sites, telling us: – Information about the composition and thermal evolution of planetary interiors – Whether the Th concentration in the PKT is a surface or mantle phenomina NASA Lunar Prospector space for science, enterprise and environment
Payload • Core – Seismology – Water and volatile detection – Accelerometer • Desirable – – – Heat Flow Geochemistry/XRF Descent camera Mineralogy Radiation Monitor Ion trap spectrometer (200 g, 10 -100 amu) (Open University) space for science, enterprise and environment
Key Technologies • Batteries – Availability (Lunar-A) • Communications – A trailing antenna would require development • Structure material (Steel or Titanium, carbon composite under consideration) • Sample acquisition • Thermal control (RHUs probably needed for polar penetrators) • AOCS (attitude control and de-orbit motor) • Spacecraft attachment and ejection mechanism space for science, enterprise and environment
Penetrator Development Programme Phase 1: Modelling (until Jan 2008) – Key trade studies (Power, Descent, Structure material, Data flow, Thermal) – Interface & System definition – Penetrator structure modelling – Procurement strategy Phase 2: Trials (until Jan 2010) – – Generic Payload element robustness proofing Penetrator structure trials Payload selection and definition Baseline accommodation Phase 3: EM (until Jan 2012) – Design and Qualification Phase 4: FM (until Jan 2013) – Flight build and non-destructive testing Mission Specific space for science, enterprise and environment
Current activities Generic penetrator development – Funded (>£ 600 k) under MSSL rolling grant – Started in earnest in April 07 – Full-scale trials March 2008 National Programme – Moon. LITE • Research Council commissioned a mission study by SSTL (delivered in Late 2006) • Proposed as national mission under current ‘Comprehensive Spending Review’. Indications expected in October/December 2007 – NASA/BNSC bi-lateral study ESA Cosmic Visions Programme – Lunar. EX (backed by industrial studies) – Jupiter-Europa – Titan-Enceladus space for science, enterprise and environment
Conclusions Moon. LITE - A focused mission with clear objectives based on a strong technology background Penetrator website: http: //www. mssl. ucl. ac. uk/planetary/missions/Micro_Penetrators. php space for science, enterprise and environment
Moon. LITE / Lunar. EX – UK Rationale • Scientifically focussed • Precursor to future penetrator programmes • High public interest • Impetus to industry • Affordable space for science, enterprise and environment
Examples of hi-gee electronic systems Designed and tested : – Communication systems • 36 GHz antenna, receiver and electronic fuze tested to 45 kgee – Dataloggers • 8 channel, 1 MHz sampling rate tested to 60 kgee – MEMS devices (accelerometers, gyros) • Tested to 50 kgee – MMIC devices • Tested to 20 kgee – TRL 6 MMIC chip tested to 20 kgee Communication system and electronic fuze tested to 45 kgee space for science, enterprise and environment
30b1c8486525c3c9a6315fa302ff46b6.ppt