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Moon Through New Eyes
of
Korean Mission: KPLO/PolCam
Chae Kyung SIM(沈採耕)1, Young-Jun CHOI2
1Kyung Hee University 慶熙大學校
2Korea Astronomy and Space science Institute 韓國天文硏究員
2018/12/07
Galaxy Forum @ Beijing, China
Astronomy in Korean culture
Astronomy in Korea
•Scientific research
– KASI (Korea Astronomy and Space science Institute)
– Universities (Kyung Hee Univ., Seoul National Univ., Yonsei Univ., …
• Technological research
– KARI (Korea Aerospace Research Institute)
– Developing and operating satellites
– Planetary exploration program
Main Research Areas
 Optical Astronomy
- Galaxy Evolution, Variable Objects, KMTNet, BOAO, LOAO, SOAO, GMT
 Radio Astronomy
- Star Formation, Active Galactic Nuclei(AGNs), TRAO, KVN, ALMA, JCMT
 Space Science
- Space Astronomy, Space Geodesy, SLR,
Solar and Space Weather, Lunar and Planetary Science
 Theoretical Astronomy
- Cosmology, Astrophysics, Historical Astronomy
 Space Situational Awareness
- Technologies for Space Surveillance, Optical Surveillance, Radar Surveillance,
OWL-Net Development, Orbit Analysis and Estimation, Risk Analysis and Space
Catalog, Asteroid Characteristics and Risk Analysis
KASI facilities
 Overseas
PolSpeck, (KASI+KHU)
Lunar polarimetry
Speckle observation
The Moon
• It has been an old, good friend of ours.
The Moon
• Sometimes, we wanted to fly to the Moon.
• … and we did!
Jules Verne, «De la terre à la lune», 1865 Apollo 11, 1969
The Moon
• The journeys to the Moon had been decreased
and rejuvenated!
Korean lunar program - Plans
• Lead by KARI (Korea Aerospace Research Institute)
Phase 1 – Pathfinder orbiter
• Domestic Lead
+ International Collaboration
• To demonstrate the technology for
planetary exploration
• To build international cooperation
• To establish deep-space network
Phase 2 – Orbiter + Lander
• Domestic Development
• To demonstrate science / technology
• Landing site selection
• Support from international
collaboration
Phase 1: Korea Pathfinder Lunar Orbiter (KPLO)
• Overview
– Program started : 2016
– Launch date : end of 2020, Falcon-9 (SpaceX) @ Cape Canaveral, FL
– Budget : 197.8B KRW (~170M USD)
– Orbit : Polar orbit at altitudes of 100 ± 30 km
– Lifetime: 1 month (Trans-Lunar) + 1 year (on orbit)
– Mass : 550 kg (6 payloads)
Collaboration with NASA
Ju, 2017
Science payloads onboard KPLO
• LUTI (high-resolution camera) by KARI+
– Target-observations including future landing sites (R ~ 5 m)
• PolCam (wide-angle polarimectric camera) by KASI+
– First polarization map of the Moon, studying regolith and components of
its surface
• KMAG (magnetometer) by KHU+
– Measuring magnetic field of anomalies at lower altitudes (< 70 km)
• KGRS (gamma-ray spectrometer) by KIGAM+
– Mapping radiation and distribution of major elements near the surface
• ShadowCam (narrow angle camera) by NASA (ASU+)
– Measuring albedo patterns inside PSRs(permanently shadowed regions)
KPLO/PolCam – First polarimetry ever!
• Objectives
– Obtain the first polarimetry map of the lunar surface (|lat.| < 70 deeg.)
– Understanding space weathering process on the surface of airless bodies
– Supporting lunar landing site search
Science PI :
Sung-Soo Kim (KHU)
PI :
Young-Jun Choi (KASI)
KPLO
PolCam
Co-PI :
Kyungin Kang (SaTReC, KAIST)
Optics (Satbyul) Structure & Thermal (Mirae)
Polarimetry
– Polarimetric information is a function of phase angle
(source-target-observer angle)
– Multiband observation: 320 nm, 430 nm, 750 nm
P(%)
Phase angle, α (°)
Pmax map
Pmax
fitting phase curve
(positivebranch only)
Scientific Goals of PolCam
• Polarization map
– The first polarimetric map
• Regolith particle size
– Maturity (Age) estimation
• Titanium map
– Highest resolution Polarization Map
Particle size Map
Titanium map
Previous works
• Latitude dependency of particle size
– The agent of space weathering (SW)
– Parallel motion to ecliptic plane
(Jeong et al. 2015, ApJS)
• Latitude & longitude dependency of maturity index
– Major SW agent is solar wind flux (rather than micrometeoroids)
– Selective shield of magnetosphere of the Earth (Sim et al. 2017, GRL)
Latitudinal differences
Space-weathering agents
Longitudinal: Selective shield of geo-magnetotail
Mission operation analysis
• Phase angle coverage for one-year operation
Specifications
Classification Item Specification*
Imaging
Field of View 10° (across-track direction)
GSD Up to 100 m (in nominal orbit)
Swath Width Up to 35 km (in nominal orbit)
Type of Sensor CCD
Imaging Pixels 512 Pixel * 6 Channels
Spectral Bands 320, 430 & 750 nm
Polarization Filters
No polarization for 320 nm
0˚, 60˚, 120˚ for 430 nm
0˚, 90˚ for 750 nm
# of Head 2 Head
Optical Housing Material AL7075 (Black Anodized)
Mounting Direction
45˚ with respect to nadir
in the across-track direction.
Baseline design
• Structure
– Dimensions
• O-Box : 150 x 100 x 85 mm
• E-Box : 170 x 120 x 62 mm
– Mass : 3.0 kg
– Optical tilted angle : 45˚ from nadir for across track
Field-of-view
• Optical box and field-of-view
Focal plane
Lens
Bandpass filters layer
Filter base
Polarizer layer
CCD sensor
Sensor PCB
Plan-B: a sparse observation case
• Unfortunate cases of an orbiter mission
– mal-maneuver : offset from the intended phase angle
– observational gap due to mal-operation
– data gap due to wrong saving/downlink
– early termination
P(%)
Phase angle, α (°)
In a sparse observation case,
an approximate phase curve helps
to fit the curve
and estimate Pmax properly.
Pmax map
Phase 1
ImagesfromKARI
Phase 2
ImagesfromKARI
Phase 2
ImagesfromKARI
Phase 2
ImagesfromKARI
Stay tuned!
ImagesfromKARI

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Moon Through New Eyes of Korean Mission: KPLO/PolCam

  • 1. Moon Through New Eyes of Korean Mission: KPLO/PolCam Chae Kyung SIM(沈採耕)1, Young-Jun CHOI2 1Kyung Hee University 慶熙大學校 2Korea Astronomy and Space science Institute 韓國天文硏究員 2018/12/07 Galaxy Forum @ Beijing, China
  • 3. Astronomy in Korea •Scientific research – KASI (Korea Astronomy and Space science Institute) – Universities (Kyung Hee Univ., Seoul National Univ., Yonsei Univ., … • Technological research – KARI (Korea Aerospace Research Institute) – Developing and operating satellites – Planetary exploration program
  • 4. Main Research Areas  Optical Astronomy - Galaxy Evolution, Variable Objects, KMTNet, BOAO, LOAO, SOAO, GMT  Radio Astronomy - Star Formation, Active Galactic Nuclei(AGNs), TRAO, KVN, ALMA, JCMT  Space Science - Space Astronomy, Space Geodesy, SLR, Solar and Space Weather, Lunar and Planetary Science  Theoretical Astronomy - Cosmology, Astrophysics, Historical Astronomy  Space Situational Awareness - Technologies for Space Surveillance, Optical Surveillance, Radar Surveillance, OWL-Net Development, Orbit Analysis and Estimation, Risk Analysis and Space Catalog, Asteroid Characteristics and Risk Analysis
  • 5. KASI facilities  Overseas PolSpeck, (KASI+KHU) Lunar polarimetry Speckle observation
  • 6. The Moon • It has been an old, good friend of ours.
  • 7. The Moon • Sometimes, we wanted to fly to the Moon. • … and we did! Jules Verne, «De la terre à la lune», 1865 Apollo 11, 1969
  • 8. The Moon • The journeys to the Moon had been decreased and rejuvenated!
  • 9. Korean lunar program - Plans • Lead by KARI (Korea Aerospace Research Institute) Phase 1 – Pathfinder orbiter • Domestic Lead + International Collaboration • To demonstrate the technology for planetary exploration • To build international cooperation • To establish deep-space network Phase 2 – Orbiter + Lander • Domestic Development • To demonstrate science / technology • Landing site selection • Support from international collaboration
  • 10. Phase 1: Korea Pathfinder Lunar Orbiter (KPLO) • Overview – Program started : 2016 – Launch date : end of 2020, Falcon-9 (SpaceX) @ Cape Canaveral, FL – Budget : 197.8B KRW (~170M USD) – Orbit : Polar orbit at altitudes of 100 ± 30 km – Lifetime: 1 month (Trans-Lunar) + 1 year (on orbit) – Mass : 550 kg (6 payloads)
  • 12. Science payloads onboard KPLO • LUTI (high-resolution camera) by KARI+ – Target-observations including future landing sites (R ~ 5 m) • PolCam (wide-angle polarimectric camera) by KASI+ – First polarization map of the Moon, studying regolith and components of its surface • KMAG (magnetometer) by KHU+ – Measuring magnetic field of anomalies at lower altitudes (< 70 km) • KGRS (gamma-ray spectrometer) by KIGAM+ – Mapping radiation and distribution of major elements near the surface • ShadowCam (narrow angle camera) by NASA (ASU+) – Measuring albedo patterns inside PSRs(permanently shadowed regions)
  • 13. KPLO/PolCam – First polarimetry ever! • Objectives – Obtain the first polarimetry map of the lunar surface (|lat.| < 70 deeg.) – Understanding space weathering process on the surface of airless bodies – Supporting lunar landing site search Science PI : Sung-Soo Kim (KHU) PI : Young-Jun Choi (KASI) KPLO PolCam Co-PI : Kyungin Kang (SaTReC, KAIST) Optics (Satbyul) Structure & Thermal (Mirae)
  • 14. Polarimetry – Polarimetric information is a function of phase angle (source-target-observer angle) – Multiband observation: 320 nm, 430 nm, 750 nm P(%) Phase angle, α (°) Pmax map Pmax fitting phase curve (positivebranch only)
  • 15. Scientific Goals of PolCam • Polarization map – The first polarimetric map • Regolith particle size – Maturity (Age) estimation • Titanium map – Highest resolution Polarization Map Particle size Map Titanium map
  • 16. Previous works • Latitude dependency of particle size – The agent of space weathering (SW) – Parallel motion to ecliptic plane (Jeong et al. 2015, ApJS) • Latitude & longitude dependency of maturity index – Major SW agent is solar wind flux (rather than micrometeoroids) – Selective shield of magnetosphere of the Earth (Sim et al. 2017, GRL)
  • 18. Longitudinal: Selective shield of geo-magnetotail
  • 19. Mission operation analysis • Phase angle coverage for one-year operation
  • 20. Specifications Classification Item Specification* Imaging Field of View 10° (across-track direction) GSD Up to 100 m (in nominal orbit) Swath Width Up to 35 km (in nominal orbit) Type of Sensor CCD Imaging Pixels 512 Pixel * 6 Channels Spectral Bands 320, 430 & 750 nm Polarization Filters No polarization for 320 nm 0˚, 60˚, 120˚ for 430 nm 0˚, 90˚ for 750 nm # of Head 2 Head Optical Housing Material AL7075 (Black Anodized) Mounting Direction 45˚ with respect to nadir in the across-track direction.
  • 21. Baseline design • Structure – Dimensions • O-Box : 150 x 100 x 85 mm • E-Box : 170 x 120 x 62 mm – Mass : 3.0 kg – Optical tilted angle : 45˚ from nadir for across track
  • 22. Field-of-view • Optical box and field-of-view
  • 23. Focal plane Lens Bandpass filters layer Filter base Polarizer layer CCD sensor Sensor PCB
  • 24. Plan-B: a sparse observation case • Unfortunate cases of an orbiter mission – mal-maneuver : offset from the intended phase angle – observational gap due to mal-operation – data gap due to wrong saving/downlink – early termination P(%) Phase angle, α (°) In a sparse observation case, an approximate phase curve helps to fit the curve and estimate Pmax properly. Pmax map