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Why look for water? PowerPoint Presentation
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Why look for water?

Why look for water?

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Why look for water?

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  1. Why look for water? • Humans exploring the Moon will need water: • Option 1: Carry it there. • Option 2: Use water that may be there already! • Carrying water to the Moon will be expensive! • Learning to “Live off the land”would make human lunar exploration easier.

  2. Living off the land • Even compared to many meteorites, the Moon is highly depleted in volatile elements and compounds, especially water. • However, oxygen does exist within various mineral structures. Hydrogen from the solar wind can also be obtained from the lunar soil. • Very energy intensive to obtain these key raw materials (have to heat regolith to at least 700° C). • Life would be much easier and cheaper if we could just find H2O on the Moon.

  3. Clementine bistatic radar - 1994 • Circular polarization ratio (CPR) consistent with ice crystals in the south polar regolith. • Later ground-based studies confirmed high-CPR in some permanently-shadowed craters. • However, Arecibo scans have also found high-CPR in some areas that are illuminated, probably due to surface roughness. • Are we seeing ice or rough terrain in dark polar craters?

  4. Hydrogen has been detected at the poles by Lunar Prospector in 1999. Is it water ice??? Lunar Prospector neutron spectrometer maps of the lunar poles. These low resolution data indicate elevated concentrations of hydrogen at both poles; it does not tell us the form of the hydrogen. Map courtesy of D. Lawrence, Los Alamos National Laboratory.

  5. Lunar Prospector Impact – July 31, 1999 • South pole impact at end of mission • Low angle (6.3°), low mass (161 kg), and low velocity (1.69 km/s) less than ideal for water ice detection. • No water detected. • Results not conclusive.

  6. How could there be water at the lunar poles? Clementine Mosaic - South Pole The sun never gets more then several degrees about the polar horizon, thus topography can provide “permanent” shade. Permanently shadowed regions (PSRs) may have temperatures < -200° C (-328° F). Over the history of the Moon, when comets or asteroids impact the Moon's surface they briefly produce a very tenuous atmosphere that quickly disperses into space. However, PSRs could act as cold-traps. Volatile gasses that enter could condense and accumulate for billions of years.

  7. Where will we look?

  8. How can we look for water? Lunar Crater Observation and Sensing Satellite LCROSS Lunar Reconnaissance Orbiter LRO

  9. Lunar Reconnaissance Orbiter • LROC – image and map the lunar surface in unprecedented detail • LOLA – provide precise global lunar topographic data through laser altimetry • LAMP – remotely probe the Moon’s permanently shadowed regions • CRaTER - characterize the global lunar radiation environment • DIVINER – measure lunar surface temperatures • LEND – measure neutron flux to study hydrogen concentrations in lunar soil

  10. LRO Mission Overview Lunar Orbit Insertion Sequence • On-board propulsion system used to capture at the Moon, insert into and maintain 50 km mean altitude circular polar reconnaissance orbit. • 1 year exploration mission followed by handover to NASA science mission directorate. Polar Mapping Phase, 50 km Altitude Circular Orbit, At least 1 Year Commissioning Phase, 30 x 216 km Altitude Quasi-Frozen Orbit, Up to 60 Days Minimum Energy Lunar Transfer

  11. LCROSS Mission Concept Ejecta Curtain • Impact the Moon at 2.5 km/sec with a Centaur upper stage and create an ejecta cloud that may reach over 10 km about the surface • Observe the impact and ejecta with instruments that can detect water Peter Schultz

  12. Excavating with 6.5-7 billion Joules • ~200 metric tons (220 tons) minimum of regolith will be excavated • Crater estimated to have ~20-25 m diameter and ~3 depth • Similar in size to East Crater at Apollo 11 landing site

  13. LCROSS Mission System • Shepherding Spacecraft: guides and aims the Centaur to its target and carries all of the critical instrumentation. • CentaurUpper Stage: provides the thrust to get us from Earth orbit to the Moon and will then be used as an impactor 14.5 m

  14. LCROSS Instruments

  15. Scheduled Launch: June 2009 • Both LCROSS and LRO will share space aboard an Atlas V launch vehicle • Launch will occur at Cape Canaveral

  16. Centaur-LCROSS-LRO at TLI

  17. LRO Separation

  18. LCROSS Lunar Flyby: L + 5 days

  19. LCROSS Trajectory: The Long and Winding Road • Flyby transitions to Lunar Gravity Assist Lunar Return Orbits (LGALRO) • Multiple LGALRO orbits about Earth (~38 day period) • Long transit also provides time to vent any remaining fuel from Centaur

  20. LCROSS Separation: Impact - 9 hrs

  21. Centaur Impact

  22. Centaur Impact

  23. Into the Plume • During the next 4 minutes, the Shepherding Spacecraft descends into the debris plume, measuring its morphology and composition, and transmitting this information back to Earth. • The Shepherding Spacecraft then ends its mission with a second impact on the Moon

  24. Impact Observation Campaign

  25. This is an exciting mission! • We believe reasonable grade amateur telescopes may be able to witness the impact plume. www.amateurastronomy.org

  26. Student Telemetry Program • GAVRT – Goldstone Apple Valley Radio Telescope run by Lewis Center for Educational Research • 34m DSS-12 &DSS-13 dishes • Used by thousands of K-12 students around the world

  27. Student Telemetry Program • Monitor spacecraft omni during LGALRO transit • Conduct Doppler studies en route • Monitor medium gain transmissions during terminal approach and determine time of LOS • Outstanding partnership opportunity for other mission post LCROSS, including LRO!

  28. Timing is everything! • LCROSS mission in 2009 corresponds with International Year of Astronomy • Also corresponds with International Polar Year. (Note: NASA’s IPY focus is on 6 poles – those of the Earth, Moon, and Mars) • Also corresponds with 50th anniversary of NASA

  29. LRO/LCROSS Launch Preview How Where When

  30. We will use the Atlas V Launch Vehicle Latest version in the Atlas family of boosters Early Atlas boosters were used for manned Mercury missions 1962-63 Atlas V has become a mainstay of U.S. satellite launches NASA has used Atlas V to launch MRO to Mars in 2004 and New Horizons to Pluto and the Kuiper Belt in 2006 How?

  31. We will launch from Space Launch Complex 41 (SLC-41) at Cape Canaveral Helios probes to the Sun Viking probes to Mars Voyager planetary flyby and deep space probes Mars Reconnaissance Orbiter New Horizons spacecraft to Pluto and Kuiper Belt Where?

  32. Atlas V first stage arrived by cargo aircraft

  33. Vertical Integration Facility

  34. What’s going to happen? First stage delivered to VIF

  35. First stage lifted into VIF

  36. First stage lifted into VIF

  37. Centaur stacked on first stage

  38. LRO and LCROSS will be stacked onto Centaur

  39. Mobile Launch Platform will transport spacecraft from VIF to pad

  40. When? LRO/LCROSS scheduled for June launch Currently looking at an early October impact for LCROSS Impact is currently targeting South Pole of the Moon

  41. Questions