Literature DB >> 22970863

LIFE: Life Investigation For Enceladus A Sample Return Mission Concept in Search for Evidence of Life.

Peter Tsou1, Donald E Brownlee, Christopher P McKay, Ariel D Anbar, Hajime Yano, Kathrin Altwegg, Luther W Beegle, Richard Dissly, Nathan J Strange, Isik Kanik.   

Abstract

Life Investigation For Enceladus (LIFE) presents a low-cost sample return mission to Enceladus, a body with high astrobiological potential. There is ample evidence that liquid water exists under ice coverage in the form of active geysers in the "tiger stripes" area of the southern Enceladus hemisphere. This active plume consists of gas and ice particles and enables the sampling of fresh materials from the interior that may originate from a liquid water source. The particles consist mostly of water ice and are 1-10 μ in diameter. The plume composition shows H(2)O, CO(2), CH(4), NH(3), Ar, and evidence that more complex organic species might be present. Since life on Earth exists whenever liquid water, organics, and energy coexist, understanding the chemical components of the emanating ice particles could indicate whether life is potentially present on Enceladus. The icy worlds of the outer planets are testing grounds for some of the theories for the origin of life on Earth. The LIFE mission concept is envisioned in two parts: first, to orbit Saturn (in order to achieve lower sampling speeds, approaching 2 km/s, and thus enable a softer sample collection impact than Stardust, and to make possible multiple flybys of Enceladus); second, to sample Enceladus' plume, the E ring of Saturn, and the Titan upper atmosphere. With new findings from these samples, NASA could provide detailed chemical and isotopic and, potentially, biological compositional context of the plume. Since the duration of the Enceladus plume is unpredictable, it is imperative that these samples are captured at the earliest flight opportunity. If LIFE is launched before 2019, it could take advantage of a Jupiter gravity assist, which would thus reduce mission lifetimes and launch vehicle costs. The LIFE concept offers science returns comparable to those of a Flagship mission but at the measurably lower sample return costs of a Discovery-class mission.

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Year:  2012        PMID: 22970863     DOI: 10.1089/ast.2011.0813

Source DB:  PubMed          Journal:  Astrobiology        ISSN: 1557-8070            Impact factor:   4.335


  7 in total

Review 1.  Formation, habitability, and detection of extrasolar moons.

Authors:  René Heller; Darren Williams; David Kipping; Mary Anne Limbach; Edwin Turner; Richard Greenberg; Takanori Sasaki; Emeline Bolmont; Olivier Grasset; Karen Lewis; Rory Barnes; Jorge I Zuluaga
Journal:  Astrobiology       Date:  2014-08-22       Impact factor: 4.335

Review 2.  Microbial Morphology and Motility as Biosignatures for Outer Planet Missions.

Authors:  Jay Nadeau; Chris Lindensmith; Jody W Deming; Vicente I Fernandez; Roman Stocker
Journal:  Astrobiology       Date:  2016-08-23       Impact factor: 4.335

3.  Quantitative evaluation of the feasibility of sampling the ice plumes at Enceladus for biomarkers of extraterrestrial life.

Authors:  James S New; Bahar Kazemi; Vassilia Spathis; Mark C Price; Richard A Mathies; Anna L Butterworth
Journal:  Proc Natl Acad Sci U S A       Date:  2021-09-14       Impact factor: 12.779

Review 4.  Glaciers and Ice Sheets As Analog Environments of Potentially Habitable Icy Worlds.

Authors:  Eva Garcia-Lopez; Cristina Cid
Journal:  Front Microbiol       Date:  2017-07-28       Impact factor: 5.640

5.  Towards Determining Biosignature Retention in Icy World Plumes.

Authors:  Kathryn Bywaters; Carol R Stoker; Nelio Batista Do Nascimento; Lawrence Lemke
Journal:  Life (Basel)       Date:  2020-04-16

Review 6.  Concerns of Organic Contamination for Sample Return Space Missions.

Authors:  Queenie Hoi Shan Chan; Rhonda Stroud; Zita Martins; Hikaru Yabuta
Journal:  Space Sci Rev       Date:  2020-05-12       Impact factor: 8.017

7.  Evaluating Biosignatures for Life Detection.

Authors:  Andrew Pohorille; Joanna Sokolowska
Journal:  Astrobiology       Date:  2020-08-17       Impact factor: 4.335

  7 in total

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