Jupiter Europa Orbiter (JEO) Concept
JEO is the NASA element of the EJSM. It is designed to follow-up on the major discoveries of the Galileo and Voyager missions at Europa, especially its ocean. JEO will be built to withstand the intense radiation in Europa orbit, and would consist of an orbiter with 11 science instruments designed for extensive mapping of Europa. On the way to Europa, JEO will tour the Jovian system and make routine and frequent observations of Jupiter, its satellites and its environment. Additional information can be found in the
EJSM Joint Summary Report.
Science Overview
Within the context of the EJSM themes and objectives, JEO will focus on its sub-goal:
Explore Europa to investigate its habitability. While the primary focus of JEO is to orbit Europa, the science return encompasses the entire Jovian system, especially as is relevant to Europa’s potential habitability. JEO uniquely includes flybys of Io and Europa, and includes flybys of Ganymede and Callisto, along with ~ 2.5 years observing Jupiter’s atmosphere, magnetosphere, and rings. The
NASA-ESA Joint Jupiter Science Definition Team (JJSDT) developed the science objectives, measurements, model payload, and science value assessments for the JEO element of the EJSM. The model payload was used to assess the feasibility of the science objectives and allow for system cost estimates. The actual payload will be selected via a competitive Announcement of Opportunity (AO) from NASA expected in 2011.

Science Objectives
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Europa’s Ocean: Characterize the extent of the ocean
and its relation to the deeper interior
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Europa’s Ice Shell: Characterize the ice shell and
any subsurface water, including their heterogeneity, and the nature of surface-ice-ocean exchange
-
Europa’s Chemistry: Determine global surface compositions
and chemistry, especially as related to habitability
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Europa’s Geology: Understand the formation of surface features, including sites of recent or current activity, and identify and characterize candidate sites for future in situ exploration
-
Jupiter System: Understand Europa in the context of the
Jupiter system
Mission Overview
JEO launches in February 2020 on an Atlas V 551 and, using a ballistic trajectory with Venus-Earth-Earth gravity assists (VEEGA), arrives at Jupiter in December 2025. Jupiter Orbit Insertion (JOI) begins a 30 month Jovian system tour followed by a 9 month science mapping phase after Europa Orbit Insertion (EOI) in July 2028. The orbiter will ultimately impact the surface of Europa after succumbing to radiation damage or running out of orbit maintenance fuel. Highlights of the Jovian tour and Europa mapping phase include:
Sample Jovian Tour
- 4 Io encounters, possibly including a volcanic plume flythrough
- 6 Europa encounters before EOI
- 6 Ganymede encounters, to survey Ganymede’s magnetosphere
- 9 Callisto encounters, at least one near-polar
- Continuous magnetospheric monitoring, regular monitoring of Io and Jupiter’s atmosphere
Europa Mapping
- Circular 200 km altitude orbit
- 95° – 100° inclination
- 2 – 4 pm local solar time
- Transfer to 100 km orbit ~one month after EOI
Flight System Overview
The JEO flight system is comparable in size and complexity to other spacecraft for similar missions such as Cassini or MRO. The concept would feature full redundancy for engineering functions, 3-axis stabilized pointing, a radio-isotope power source (RPS) with batteries for peak power management, bi-propellant chemical propulsion, a large gimbaled high gain antenna (HGA), and X-band and Ka-band transponders for tracking, telemetry and precision Doppler measurements. Radiation hardened electronics would be used throughout with shielding used to further reduce radiation levels for electronic components and assemblies. Remote sensing instruments are mounted and aligned to accommodate continuous nadir pointing in the Europa science orbit.

System Mass
- Launch Mass Capability, 5040 kg
- Launch Vehicle Adapter, 123 kg
- Flight System Mass, 1367 kg
- Propellant (for 2260 m/s), 2646 kg
- Remaining usable launch mass, 973 kg (for contingency and system margin)
Subsystems
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Model Payload (106 kg) |
Telecom
- 3m HGA with 2-axis gimbal
- 25 W X-band and Ka-band TWTAs
Attitude control
- 3-axis stabilized with reaction wheels
and coupled thrusters
Power
- 540W RPS (MMRTG or ASRG)
- Lithium Ion battery for peak
power management
Propulsion
- Bi-propellant
- 900N gimbaled engine
|
- Laser Altimeter (LA)
- Radio Science (RS)
- Ice Penetrating Radar (IPR)
- VIS-IR Imaging Spectrometer (VIRIS)
- UV Spectrometer (UVS)
- Ion and Neutral Mass Spectrometer (INMS)
- Thermal Instrument (TI)
- Narrow Angle Camera (NAC)
- Wide Angle Camera and Medium Angle Camera (WAC+MAC)
- Magnetometer (MAG)
- Particle and Plasma Instrument (PPI)
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