Evidence map›Paper›PMID 39398102›Full record

ReviewSpace science reviews2024

The Mapping Imaging Spectrometer for Europa (MISE).

Diana L Blaney, Karl Hibbitts, Serina Diniega, Ashley Gerard Davies, Roger N Clark, Robert O Green, Matthew Hedman, Yves Langevin, Jonathan Lunine, Thomas B McCord and 29 more

Abstract readReview
PubMed Full text at PMC Publisher
In one paragraph

Review in Space science reviews, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

2 citing papers in PubMed.

  1. Article
  2. Review
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

39 authors.

Diana L BlaneyJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.ORCID 0000-0002-4267-7939
Karl HibbittsApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Serina DiniegaJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Ashley Gerard DaviesJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Roger N ClarkPlanetary Science Institute, Tucson, AZ USA.
Robert O GreenJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Matthew HedmanUniversity of Idaho, Moscow, ID USA.
Yves LangevinUniversity of Paris, Orsey, Paris, France.
Jonathan LunineCornell University, Ithaca, NY USA.
Thomas B McCordBear Fight Institute, Winthrop, WA USA.
Scott MurchieApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Chris ParanicasApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Frank SeelosApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Jason M SoderblomMassachusetts Institute of Technology, Cambridge, MA USA.
Morgan L CableJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Regina EckertJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
David R ThompsonJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Samantha K TrumboUC San Diego, San Diego, CA USA.
Carl BruceJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Sarah R LundeenJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Holly A BenderJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Mark C HelmlingerJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Lori B MooreJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Pantazis MouroulisJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Zachary SmallJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Hong TangJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Byron Van GorpJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Peter W SullivanJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Shannon ZarehJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Jose I RodriquezJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Ian McKinleyJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Daniel V HahnApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Matthew BowersApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Ramsey HouraniApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Brian A BryceApplied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
Danielle NudingJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Zachery BaileyJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Alessandro RetturaJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
Evan D ZarateJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The Mapping Imaging Spectrometer for Europa (MISE) is an infrared compositional instrument that will fly on NASA's Europa Clipper mission to the Jupiter system. MISE is designed to meet the Level-1 science requirements related to the mission's composition science objective to "understand the habitability of Europa's ocean through composition and chemistry" and to contribute to the geology science and ice shell and ocean objectives, thereby helping Europa Clipper achieve its mission goal to "explore Europa to investigate its habitability." MISE has a mass of 65 kg and uses an energy per flyby of 75.2 W-h. MISE will detect illumination from 0.8 to 5 μm with 10 nm spectral resolution, a spatial sampling of 25 m per pixel at 100 km altitude, and 300 cross-track pixels, enabling discrimination among the two principal states of water ice on Europa, identification of the main non-ice components of interest: salts, acids, and organics, and detection of trace materials as well as some thermal signatures. Furthermore, the spatial resolution and global coverage that MISE will achieve will be complemented by the higher spectral resolution of some Earth-based assets. MISE, combined with observations collected by the rest of the Europa Clipper payload, will enable significant advances in our understanding of how the large-scale structure of Europa's surface is shaped by geological processes and inform our understanding of the surface at microscale. This paper describes the planned MISE science investigations, instrument design, concept of operations, and data products.

Indexed as

CompositionEuropaEuropa ClipperMappingSpectrometer

Identifiers

PMID39398102
PMCPMC11464581

What OpenQuestion holds

Textmetadata
LicenceCC BY
Read underepoch 390

Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.