Scientific rationale for Saturn's in situ exploration Article

Mousis, O, Fletcher, LN, Lebreton, JP et al. (2014). Scientific rationale for Saturn's in situ exploration . Planetary and Space Science, 104 29-47. 10.1016/j.pss.2014.09.014

Open Access Industry Collaboration International Collaboration

cited authors

  • Mousis, O; Fletcher, LN; Lebreton, JP; Wurz, P; Cavalie, T; Coustenis, A; Courtin, R; Gautier, D; Helled, R; Irwin, PGJ; Morse, AD; Nettelmann, N; Marty, B; Rousselot, P; Venot, O; Atkinson, DH; Waite, JH; Reh, KR; Simon, AA; Atreya, S; Andre, N; Blanc, M; Daglis, IA; Fischer, G; Geppertt, WD; Guillot, T; Hedman, MM; Hueso, R; Lellouch, E; Lunine, JI; Murray, CD; O'Donoghue, J; Rengel, M; Sanchez-Lavega, A; Schmider, FX; Spiga, A; Spilker, T; Petit, J-M; Tiscareno, MS; Ali-Dib, M; Altwegg, K; Bolton, SJ; Bouquet, A; Briois, C; Fouchet, T; Guerlet, S; Kostiuk, T; Lebleu, D; Moreno, R; Orton, GS; Poncy, J

sustainable development goals

authors

publication date

  • December 1, 2014

published in

keywords

  • Astronomy & Astrophysics
  • DOPPLER WIND EXPERIMENT
  • Elemental and isotopic composition
  • Entry probe
  • GIANT PLANETS
  • Giant planet formation
  • ISO-SWS OBSERVATIONS
  • ISOTOPE RATIOS
  • In situ measurements
  • JUPITERS ATMOSPHERE
  • POLAR NEPHELOMETER
  • PROBE
  • Physical Sciences
  • SPATIAL-DISTRIBUTION
  • Saturn atmosphere
  • Science & Technology
  • Solar system formation
  • WATER ABUNDANCE
  • ZONAL WIND

Digital Object Identifier (DOI)

start page

  • 29

end page

  • 47

volume

  • 104