Presentations from the 4th Europa Jupiter System Mission (EJSM) Instrument Workshop on July 26-29, 2010 are now available on the [[LINK||PAGE:europajupitersystemmissionejsm:2010ejsminstrumentworkshopproducts||OPFM Website]]. The workshop covered programmatic and technical aspects related to the EJSM mission, more specifically to both spacecraft (JGO and JEO). Among the topics addressed were: Jovian radiation models, the JEO system reliability model, radiation shielding modeling results, and the planned JEO and JGO architectures. In addition, two classes were offered as part of the workshop: a tutorial on the Jovian environments, and Planetary Protection considerations for instrument development. The presentations from this workshop provide relevant information to potential instrument providers who intend to respond to the Announcement of Opportunity (AO) for EJSM instruments, which is currently expected to be released in 2011.
Presentations available at: [[LINK||PAGE:europajupitersystemmissionejsm:2010ejsminstrumentworkshopproducts||https://opfm.jpl.nasa.gov/europajupitersystemmissionejsm/2010ejsminstrumentworkshopproducts/ ]]
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NASA and ESA are organizing the 4th Europa Jupiter System Mission (EJSM) Instrument Workshop on July 26-29, 2010 in the Pasadena, California area. This workshop will be covering programmatic and technical aspects related to the EJSM mission, more specifically to both spacecraft (JGO and JEO). Among the topics to be addressed are: Jovian radiation models, the JEO system reliability model, radiation shielding modeling results, and the planned JEO and JGO architectures. Two classes will be offered as part of the workshop: a tutorial on the Jovian environments, and Planetary Protection considerations for instrument development. This workshop will provide relevant information to potential instrument providers who intend to respond to the Announcement of Opportunity (AO) for EJSM instruments which is currently expected to be released in 2011.
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The Europa Jupiter System Mission (EJSM) will hold an Open Science Workshop on May 17-19, 2010 at ESA’s European Space Research and Technology Centre (ESTEC) in Noordwijk, the Netherlands.
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The Europa Jupiter System Mission (EJSM), Jupiter Europa Orbiter (JEO) project has made the current Approved Parts and Materials List (APML) available to the community. The APML is the selection source for all Electrical, Electronic, and Electromechanical (EEE) parts and materials to be used on the JEO spacecraft subsystems and instruments.
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The third Europa Jupiter System Mission (EJSM) Instrument Workshop was held on January 18-20, 2010 at ESA’s European Space Research and Technology Centre (ESTEC) in Noordwijk, the Netherlands.
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The third Europa Jupiter System Mission (EJSM) Instrument Workshop will be held on January 18-20, 2010 at ESA’s European Space Research and Technology Centre (ESTEC) in Noordwijk, the Netherlands.
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NASA scientists revealed Friday a first-of-its-kind image from space showing reflecting sunlight from a lake on Saturn's largest moon, Titan.
It's the first visual "smoking gun" evidence of liquid on the northern hemisphere of the moon, scientists said, and the first-ever photo from another world showing a "specular reflection" -- which is reflection of light from an extremely smooth surface and in this case, a liquid one.
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Dear Colleague, The Europa Jupiter System Mission (EJSM) was recently identified as the first priority mission for the Outer Planet Flagship Mission. EJSM involves the NASA Jupiter Europa Orbiter and ESA Jupiter Ganymede Orbiter. It might also involve other elements, such as a JAXA Magnetospheric Orbiter. In addition to the focus on Europa and Ganymede, substantial Jupiter and Jupiter system science will be conducted.
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At a meeting in Washington last week, National Aeronautics and Space Administration and European Space Agency officials decided to continue pursuing studies of a mission to...
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Planetary scientists have a rare opportunity to pick the destination for their next big mission. But will it be Titan or Europa. Eric Hand of Nature Magazine describe the decision process on the next Flagship.
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NASA and ESA announced today that the NASA-ESA Decision Board meeting for the Outer Planet Flagship mission selection has been delayed from January 30 to February 12, 2009. The NASA ESA Evaluation Board will still be meeting on January 28.
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Volcanoes on a distant moon of the planet Saturn are erupting and spewing a gassy slurry of icy ammonia, water and methane into Titan's thick red, tar-like atmosphere, NASA scientists are reporting in San Francisco this week.
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Richard A. Kerr writes that “Planetary scientists are in the final stretch of a first-time competition designed to get the most science for the buck from the next big planetary mission while avoiding the fiscal debacles of the past”. Science writer Kerr relates the background and status of NASA’s Outer Planet Selection process in the December 19 issues Vol 322, 1780 [[LINK]]
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The Cassini spacecraft has observed possible cryovolcanic features in radar images of Titan
spurring a debate at the American Geophysical Union meeting in San Francisco on Dec 15 on the origin of these surface features.
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On Dec 9 and Dec 11, the NASA Science Panel chaired by Bill McKinnon and NASA Technical Management and Cost Review team (TMC) chaired by Brad Perry conducted site visits at JPL for the Titan Saturn System Mission (TSSM) and the Europa Jupiter System Mission (EJSM).
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The Outer Planets Assessment Group (OPAG) met in Tempe, AZ on November 6-7, and was briefed on the two Outer Planet Flagship Mission candidates: Europa Jupiter System Mission (EJSM) and Titan Saturn Systems Mission (TSSM). The NASA and ESA leadership teams were present to make the presentations. Jim Green gave an overview of the Planetary Science Division. It was announced that Bill McKinnon is taking over leadership of OPAG from Fran Bagenal.
Following OPAG the two study teams met to finalize the NASA-ESA Joint Summary Reports on the two flagship concepts, which are to be released on November 15.
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Data obtained by the Cassini Visual Infrared Mapping Spectrometer (VIMS) strongly points to Titan’s Ontario Lacus being filled with liquid ethane. The ethane is likely in solution with methane, nitrogen, and other low mass molecules.
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Titan is a fantastic laboratory for comparative studies with other bodies in the solar system and there is a great deal of knowledge still to be learned.
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The Joint Jupiter Science Definition Team met August 13-14 2008 in Columbia, MD. Primary topics of discussion included new graphic tools to communicate the science concepts for the final report and presentations, tweaking of the science value matrix so that scores reflect the updated ("sweet spot") payload, and specifications for the instruments in the new planning payload. The group also discussed synergistic science to be accomplished with JGO - this will be developed more fully at the next (and final) SDT meeting in London in September.
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The Joint Jupiter Science Definition Team met July 14-15 2008 in Monrovia, CA. This was the first meeting of the group after the 2nd interim review with Headquarters, which took place ~3 weeks earlier. That review was very successful, and the team is now moving into a new phase of the project.
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The first OPFM Instrument Workshop was held June 3-5, 2008, in Monrovia, California. Approximately 250 attendees from 8 different countries participated in this workshop designed to prepare the outer planet community for an upcoming opportunities to propose investigations for an international Outer Planet Flagship mission that is planned for a new start in fiscal 2009.
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The fifth meeting of the Titan Saturn System Mission (TSSM) JSDT chaired by Jonathan Lunine and Jean-Pierre Lebreton was conducted in Oxnard California just following the Ices Workshop. This JSDT session focused on finalizing the model orbiter payload and science scenarios for the Titan mission. A variety of issues were addressed, including the optimal strategy for mapping the currently poorly-understood middle atmosphere form 400-800 km altitude. Subgroups dealt with issues such as sensitivity of gravity mapping, radar altimetry versus sounding, and optimal landing sites for the Titan probe. The group also focused on defining payload and landing sites for the in situ elements. Further work by the group will continue to focus on orbiter science scenarios in situ payload.
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Mar 31- April 1. The spring meeting was held in Boulder, Colorado included briefings on the joint NASA and ESA outer planet exploration program. Curt Niebur described the NASA Outer Planet Flagship Program; Jean-Pierre Lebreton described ESA's Cosmic Vision program.
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The Titan Saturn System Mission Joint Science Definition Team met in Vienna Austria on April 15 and 16 in connection with the European Geophysical Union meeting taking place there.
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