Literature DB >> 12624177

Fluid core size of Mars from detection of the solar tide.

C F Yoder1, A S Konopliv, D N Yuan, E M Standish, W M Folkner.   

Abstract

The solar tidal deformation of Mars, measured by its k2 potential Love number, has been obtained from an analysis of Mars Global Surveyor radio tracking. The observed k2 of 0.153 +/- 0.017 is large enough to rule out a solid iron core and so indicates that at least the outer part of the core is liquid. The inferred core radius is between 1520 and 1840 kilometers and is independent of many interior properties, although partial melt of the mantle is one factor that could reduce core size. Ice-cap mass changes can be deduced from the seasonal variations in air pressure and the odd gravity harmonic J3, given knowledge of cap mass distribution with latitude. The south cap seasonal mass change is about 30 to 40% larger than that of the north cap.

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Year:  2003        PMID: 12624177     DOI: 10.1126/science.1079645

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  5 in total

1.  Simulation of the planetary interior differentiation processes in the laboratory.

Authors:  Yingwei Fei
Journal:  J Vis Exp       Date:  2013-11-15       Impact factor: 1.355

Review 2.  SEIS: Insight's Seismic Experiment for Internal Structure of Mars.

Authors:  P Lognonné; W B Banerdt; D Giardini; W T Pike; U Christensen; P Laudet; S de Raucourt; P Zweifel; S Calcutt; M Bierwirth; K J Hurst; F Ijpelaan; J W Umland; R Llorca-Cejudo; S A Larson; R F Garcia; S Kedar; B Knapmeyer-Endrun; D Mimoun; A Mocquet; M P Panning; R C Weber; A Sylvestre-Baron; G Pont; N Verdier; L Kerjean; L J Facto; V Gharakanian; J E Feldman; T L Hoffman; D B Klein; K Klein; N P Onufer; J Paredes-Garcia; M P Petkov; J R Willis; S E Smrekar; M Drilleau; T Gabsi; T Nebut; O Robert; S Tillier; C Moreau; M Parise; G Aveni; S Ben Charef; Y Bennour; T Camus; P A Dandonneau; C Desfoux; B Lecomte; O Pot; P Revuz; D Mance; J tenPierick; N E Bowles; C Charalambous; A K Delahunty; J Hurley; R Irshad; Huafeng Liu; A G Mukherjee; I M Standley; A E Stott; J Temple; T Warren; M Eberhardt; A Kramer; W Kühne; E-P Miettinen; M Monecke; C Aicardi; M André; J Baroukh; A Borrien; A Bouisset; P Boutte; K Brethomé; C Brysbaert; T Carlier; M Deleuze; J M Desmarres; D Dilhan; C Doucet; D Faye; N Faye-Refalo; R Gonzalez; C Imbert; C Larigauderie; E Locatelli; L Luno; J-R Meyer; F Mialhe; J M Mouret; M Nonon; Y Pahn; A Paillet; P Pasquier; G Perez; R Perez; L Perrin; B Pouilloux; A Rosak; I Savin de Larclause; J Sicre; M Sodki; N Toulemont; B Vella; C Yana; F Alibay; O M Avalos; M A Balzer; P Bhandari; E Blanco; B D Bone; J C Bousman; P Bruneau; F J Calef; R J Calvet; S A D'Agostino; G de Los Santos; R G Deen; R W Denise; J Ervin; N W Ferraro; H E Gengl; F Grinblat; D Hernandez; M Hetzel; M E Johnson; L Khachikyan; J Y Lin; S M Madzunkov; S L Marshall; I G Mikellides; E A Miller; W Raff; J E Singer; C M Sunday; J F Villalvazo; M C Wallace; D Banfield; J A Rodriguez-Manfredi; C T Russell; A Trebi-Ollennu; J N Maki; E Beucler; M Böse; C Bonjour; J L Berenguer; S Ceylan; J Clinton; V Conejero; I Daubar; V Dehant; P Delage; F Euchner; I Estève; L Fayon; L Ferraioli; C L Johnson; J Gagnepain-Beyneix; M Golombek; A Khan; T Kawamura; B Kenda; P Labrot; N Murdoch; C Pardo; C Perrin; L Pou; A Sauron; D Savoie; S Stähler; E Stutzmann; N A Teanby; J Tromp; M van Driel; M Wieczorek; R Widmer-Schnidrig; J Wookey
Journal:  Space Sci Rev       Date:  2019-01-28       Impact factor: 8.017

3.  The early heat loss evolution of Mars and their implications for internal and environmental history.

Authors:  Javier Ruiz
Journal:  Sci Rep       Date:  2014-03-11       Impact factor: 4.379

4.  Present-day heat flow model of Mars.

Authors:  Laura M Parro; Alberto Jiménez-Díaz; Federico Mansilla; Javier Ruiz
Journal:  Sci Rep       Date:  2017-04-03       Impact factor: 4.379

5.  Repetitive marsquakes in Martian upper mantle.

Authors:  Weijia Sun; Hrvoje Tkalčić
Journal:  Nat Commun       Date:  2022-03-30       Impact factor: 14.919

  5 in total

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