Moonraker: Enceladus Multiple Flyby Mission

被引:10
|
作者
Mousis, O. [1 ,2 ]
Bouquet, A. [1 ,3 ]
Langevin, Y. [4 ]
Andre, N. [5 ]
Boithias, H. [6 ]
Durry, G. [7 ]
Faye, F. [6 ]
Hartogh, P. [8 ]
Helbert, J. [9 ]
Iess, L. [10 ]
Kempf, S. [11 ]
Masters, A. [12 ]
Postberg, F. [13 ]
Renard, J. -B. [14 ]
Vernazza, P. [1 ]
Vorburger, A. [15 ]
Wurz, P. [15 ]
Atkinson, D. H. [16 ]
Barabash, S. [17 ]
Berthomier, M. [18 ]
Brucato, J. [19 ]
Cable, M. [16 ]
Carter, J. [1 ]
Cazaux, S. [20 ,21 ]
Coustenis, A. [22 ]
Danger, G. [2 ,3 ]
Dehant, V. [23 ]
Fornaro, T. [19 ]
Garnier, P. [5 ]
Gautier, T. [22 ,24 ]
Groussin, O. [1 ]
Hadid, L. Z. [25 ]
Ize, J. -C. [1 ]
Kolmasova, I. [26 ,27 ]
Lebreton, J. -P. [14 ]
Le Maistre, S. [23 ]
Lellouch, E. [22 ]
Lunine, J. I. [28 ]
Mandt, K. E. [29 ]
Martins, Z. [30 ,31 ]
Mimoun, D. [32 ]
Nenon, Q. [5 ]
Munoz Caro, G. M. [33 ]
Rannou, P. [7 ]
Rauer, H. [9 ]
Schmitt-Kopplin, P. [34 ,35 ]
Schneeberger, A. [1 ]
Simons, M. [36 ]
Stephan, K. [9 ]
Van Hoolst, T. [23 ]
机构
[1] Aix Marseille Univ, Inst Origines, CNRS, CNES,LAM, Marseille, France
[2] Inst Univ France IUF, Paris, France
[3] Aix Marseille Univ, Inst Origines, CNRS, PIIM, Marseille, France
[4] Univ Paris Saclay, Inst Astrophys Spatiale, IAS, CNRS, Orsay, France
[5] Inst Rech Astrophys & Planetol, 9 Ave Colonel Roche, F-31028 Toulouse 4, France
[6] Airbus Def & Space, Toulouse, France
[7] Univ Reims, Grp Spectrometrie Mol & Atmospher, CNRS, UMR 7331, Campus Sci Exactes & Nat,BP 1039, F-51687 Reims, France
[8] Max Planck Inst Sonnensyst Forsch, Gottingen, Germany
[9] DLR, Inst Planetary Res, Berlin, Germany
[10] Univ Roma La Sapienza, Dipartimento Ingn Meccan & Aerosp, Rome, Italy
[11] Univ Colorado, LASP, Boulder, CO 80309 USA
[12] Imperial Coll London, London, England
[13] Free Univ Berlin, Inst Geol Sci, Berlin, Germany
[14] Univ Orleans, CNRS, CNES, LPC2E, 3A Ave Rech Sci, F-45071 Orleans 2, France
[15] Univ Bern, Phys Inst, Bern, Switzerland
[16] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[17] Swedish Inst Space Phys, Kiruna, Sweden
[18] Ecole Polytech, Lab Phys Plasmas, Palaiseau, France
[19] INAF Astrophys Observ Arcetri, Florence, Italy
[20] Delft Univ Technol, Fac Aerosp Engn, Delft, Netherlands
[21] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
[22] Univ Paris, Sorbonne Univ, PSL Univ, LESIA,CNRS,Paris Observ, F-92190 Meudon, France
[23] Royal Observ Belgium, 3 Ave Circulaire, B-1180 Brussels, Belgium
[24] Sorbonne Univ, LATMOS IPSL, CNRS, UVSQ UPSaclay, Guyancourt, France
[25] Univ Paris Saclay, Sorbonne Univ, Ecole Polytech, Inst Polytech Paris,Lab Phys Plasmas LPP,CNRS,Obs, F-91120 Palaiseau, France
[26] Czech Acad Sci, Dept Space Phys, Inst Atmospher Phys, Prague 14100, Czech Republic
[27] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic
[28] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[29] Johns Hopkins Appl Phys Lab, Laurel, MD USA
[30] Univ Lisbon, Inst Mol Sci, Ctr Quim Estrut, Av Rovisco Pais 1, P-1049001 Lisbon, Portugal
[31] Univ Lisbon, Dept Chem Engn, Inst Super Tecn, Av Rovisco Pais 1, P-1049001 Lisbon, Portugal
[32] Univ Toulouse, ISAE SUPAERO, DEOS SSPA, Toulouse, France
[33] Ctr Astrobiol INTA CSIC, Ctra Ajalvir,Km 4, E-28850 Madrid, Spain
[34] Max Planck Inst Extraterr Phys, Ctr Astrochem Studies, MPI MPE, Garching, Germany
[35] Helmholtz Munich, Analyt Biochem BGC, Ingolstaedter Landstr 1, D-85764 Neuherberg, Germany
[36] CALTECH, Seismol Lab, 1200 E Calif Blvd, Pasadena, CA 91125 USA
[37] German Aerosp Ctr, Inst Quantum Technol, Ulm, Germany
来源
PLANETARY SCIENCE JOURNAL | 2022年 / 3卷 / 12期
基金
美国国家航空航天局;
关键词
MASS-SPECTROMETER; INTERIOR STRUCTURE; GRAVITY-FIELD; MU-M; CASSINI; PLUME; ION; ISOTOPOLOGUES; SPECTROSCOPY; CALIBRATION;
D O I
10.3847/PSJ/ac9c03
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky core. Further investigation of the composition of the plume formed by the jets is necessary to fully understand the ocean, its potential habitability, and what it tells us about Enceladus's origin. Moonraker has been proposed as an ESA M-class mission designed to orbit Saturn and perform multiple flybys of Enceladus, focusing on traversals of the plume. The proposed Moonraker mission consists of an ESA-provided platform with strong heritage from JUICE and Mars Sample Return and carrying a suite of instruments dedicated to plume and surface analysis. The nominal Moonraker mission has a duration of similar to 13.5 yr. It includes a 23-flyby segment with 189 days allocated for the science phase and can be expanded with additional segments if resources allow. The mission concept consists of investigating (i) the habitability conditions of present-day Enceladus and its internal ocean, (ii) the mechanisms at play for the communication between the internal ocean and the surface of the South Polar Terrain, and (iii) the formation conditions of the moon. Moonraker, thanks to state-of-the-art instruments representing a significant improvement over Cassini's payload, would quantify the abundance of key species in the plume, isotopic ratios, and the physical parameters of the plume and the surface. Such a mission would pave the way for a possible future landed mission.
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页数:12
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