PLANET-C: Venus Climate Orbiter mission -Updates- Takehiko Satoh (Kumamoto Univ / JAXA) George Hashimoto (Kobe Univ) PLANET-C team
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1 PLANET-C: Venus Climate Orbiter mission -Updates- Takehiko Satoh (Kumamoto Univ / JAXA) George Hashimoto (Kobe Univ) PLANET-C team
2 Venus Climate Orbiter JAXA s 24th science spacecraft dedicated to the exploration of Venus meteorology (code name: PLANET-C) Atmospheric Dynamics - Imaging observations with 4 cameras (from UV to long-ir) + Lightning/Airglow Imager + radio science - Quasi-synchronous equatorial orbit
3 Complementary missions Instruments Main target Orbit VCO 4 cameras Lightning/Airglow Imager Radio science Atmospheric dynamics Equatorial Venus Express 3 spectrometers 1 camera Plasma analyzer Magnetometer Radio science Atmospheric chemistry and dynamics, Surface processes, Plasma environment Polar
4 Launch schedule Launch: June 2010 Arrival: December 2010 Mission life: > 2 years Mass: 480 kg (including fuel) Launch Vehicle: - M-V or H-IIA (still TBD) - No payload increase even with H-IIA (deccelaration needs) Launch of PLANET-B Mars orbiter by M-V (1998)
5 Science objectives Meteorology Mechanism of super-rotation Meridional circulation Meso-scale processes Cloud physics Lightning Solid planet Detection of active volcanism Inhomogeneity of surface material Zodiacal light (during cruise)
6 Concept of meteorological survey satellite Monitoring global structures Wide field of view Covering time scales from hours to months Continuous, systematic sampling Minimum interruption during the mission Local time coverage Equatorial orbit Meso-scales / Wind vectors High spatial
7 Spacecraft configuration Mass 480 kg (including fuel) Science payload 34 kg Attitude control Pointing accuracy 0.1 o Stability 0.01 o Oribit Periapsis 300km Apoapsis 13 Rv Period 30 hours
8 1-μm camera (IR1) Lightning and airglow camera (LAC) 2-μm camera (IR2) Longwave IR camera (LIR) Ultraviolet imager (UVI)
9 Test model of IR1 baffle Radiation test IR2 test model LIR test image (10μm) Thermal vacuum test
10 Science instruments (1) 1-μm camera (IR1) by Tokyo Univ. λ= 1.01 μm (near-ir window) Pixels: 1024x1024, Detector: Si-CSD/CCD Cloud (day/night) Surface (night) Status: Developing PM F/8 Optics (Lighter weight) Aluminum Housing IR-AE (PM) shared with IR2 Test model of IR1 baffle
11 Science instruments (2) 2-μm camera (IR2) by Kumamoto Univ. λ= 1.73, 2.26, 2.32 μm (near-ir window), 2.02 μm (CO 2 absorption), 1.65 μm (zodiacal light) Pixels: 1024x1024, Detector: PtSi (cooled to 65 K) Cloud / Particle size Carbon monooxide (night) Cloud top height (day) Zodiacal light (cruising) Status: Developing PM PtSi process (summer) Cold-plate material IR2 test model Galileo (2.3μm)
12 Science instruments (3) Ultraviolet imager (UVI) by Hokkaido Univ. λ= 283, 365 nm Pixels: 1024x1024, Detector: Si-CCD SO 2 / Unknown UV absorber (day) Longwave IR camera (LIR) by Inst. of Polar Res. λ= 10 μm Pixels: 240x320, Detector: un-cooled bolometer array Cloud top temperature (day/night) Lightning & Airglow camera (LAC) by Tohoku Univ. λ= 777, 551, 553, 558, 630 nm Pixels: 8x8, Detector: APD (50kHz sampling) Lightning (night) O 2 /O airglow (night)
13 Science instruments (4) Sensor Digital Electronics unit (DE) by JAXA Controlling cameras (IR1/2, UVI, LIR) Dark subtraction / Flat calibration / Noise reduction JPEG2000 data compression Status: Developing Simulator Matching test with IR-AE Tests with other cameras
14 Radio occultation Altitude coverage velocity (m s -1 ) (km) Sounding region 20 0 Unknown momentum transport Airglow (Visible) Cloud top temperature (IR) CO 2 absorption (Near-IR) SO 2/Unknown absorber (UV) Cloud layer Lightning Lower cloud (Near-IR) CO (Near-IR) Surface (Near-IR)
15 Observation plan -- Every revolution, More than 2 years -- Limb images (~0.5 hour) Successive Global images of atmosphere and ground surface (~24 hours) Orbital period: 30 hours Temperature / H 2 SO 4 vapor / Ionosphere by radio occultation Close-up images/ Lightning/Airglow (~3 hours x 2)
16 Orbital motion roughly synchronized with the super-rotational flow near the cloud base Spacecraft 60 m/s westward flow near the cloud base
17 Summary VCO is optimized for systematic, continuous sampling of meteorological data (essential to study atmospheric dynamics). Instruments (in PM-developing phase) are for global mapping of clouds and minor constituents, detection of lightning, and determining vertical structures of the atmosphere. VCO complements ESA s Venus Express which explores broad topics of Venusian environment with different approaches. VCO will be launched and arrive at Venus in 2010 (launch vehicle still TBD). The data will become open to the international science community after calibration.
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