{"id":51,"date":"2024-03-13T10:54:32","date_gmt":"2024-03-13T09:54:32","guid":{"rendered":"http:\/\/localhost:8888\/wptest\/?page_id=51"},"modified":"2025-12-10T15:12:33","modified_gmt":"2025-12-10T14:12:33","slug":"mission","status":"publish","type":"page","link":"\/mirs-public\/mission\/","title":{"rendered":"Mission"},"content":{"rendered":"

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MIRS<\/h1>\n

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Mission<\/h2>\n

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<\/span><\/span>MMX<\/span><\/h3>\n
<\/span><\/span>La mission\u00a0Martian Moons eXploration\u00a0(MMX) de la JAXA (Japan Aerospace Exploration Agency)\u00a0<\/span><\/h5>\n
<\/span><\/span>est la premi\u00e8re mission de retour d\u2019\u00e9chantillons du satellite Phobos. Elle pr\u00e9voit \u00e9galement une exploration du syst\u00e8me de la plan\u00e8te Mars. L\u2019objectif principal de la mission est d\u2019\u00e9lucider l\u2019origine des lunes martiennes, ce qui fournira des informations importantes sur la formation des plan\u00e8tes et sur les conditions d\u2019apparition de l\u2019eau sur les plan\u00e8tes de type terrestre.<\/span><\/h6>\n

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<\/span><\/span>La sonde MMX<\/span><\/h4>\n

<\/b><\/p>\n

<\/span><\/span>La sonde MMX est compos\u00e9e de trois modules\u00a0:\u00a0<\/span><\/h5>\n

 <\/p>\n

<\/span><\/span>– un module de propulsion charg\u00e9 d’amener la sonde spatiale jusqu’\u00e0 Mars ;
– un module d’exploration comprenant la partie pour l’atterrissage \u00e0 quatre pieds et les deux syst\u00e8mes de pr\u00e9l\u00e8vement d’\u00e9chantillon du sol;
<\/span>– un module charg\u00e9 de ramener la capsule contenant les \u00e9chantillons de Phobos sur Terre.<\/p>\n

Au lancement la sonde MMX p\u00e8se 4200 kg.<\/span><\/h6>\n

[\/et_pb_text][et_pb_image src=\u00a0\u00bb\/mirs-public\/files\/2024\/03\/Plan-de-travail-8-1.png\u00a0\u00bb title_text=\u00a0\u00bbShema Sonde\u00a0\u00bb align=\u00a0\u00bbcenter\u00a0\u00bb admin_label=\u00a0\u00bbImage\u00a0\u00bb _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb height=\u00a0\u00bb460px\u00a0\u00bb height_tablet=\u00a0\u00bb267px\u00a0\u00bb height_phone=\u00a0\u00bb140px\u00a0\u00bb height_last_edited=\u00a0\u00bbon|tablet\u00a0\u00bb max_height=\u00a0\u00bb460px\u00a0\u00bb custom_margin=\u00a0\u00bb||-1px|||\u00a0\u00bb custom_padding=\u00a0\u00bb0px||0px|||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb text_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb text_font_size=\u00a0\u00bb13px\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

SONDE<\/span> MMX – LIRA<\/span><\/p>\n

[\/et_pb_text][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb header_4_font=\u00a0\u00bbCommissioner|700|||||||\u00a0\u00bb header_4_font_size=\u00a0\u00bb30px\u00a0\u00bb header_5_font=\u00a0\u00bbCommissioner|600|||||||\u00a0\u00bb header_5_font_size=\u00a0\u00bb23px\u00a0\u00bb header_5_line_height=\u00a0\u00bb1.4em\u00a0\u00bb header_6_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb header_6_font_size=\u00a0\u00bb20px\u00a0\u00bb header_6_line_height=\u00a0\u00bb2em\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

\u00c0 la d\u00e9couverte des lunes martiennes\u00a0: les grands questions<\/span><\/h5>\n

 <\/p>\n

<\/span><\/span><\/span>D\u00e8s la d\u00e9couverte des deux satellites de Mars (Phobos et Deimos) en 1877 par Asaph Hall, de nombreux d\u00e9bats ont vu le jour au sein de la communaut\u00e9 scientifique. Comment a \u00e9volu\u00e9 le syst\u00e8me martien ? Quelle est la composition de la surface de Phobos ? Comment se sont form\u00e9es Phobos et Deimos ?<\/span><\/h6>\n

[\/et_pb_text][et_pb_image src=\u00a0\u00bb\/mirs-public\/upload\/pia17305_orig_web.jpg.webp\u00a0\u00bb title_text=\u00a0\u00bbpia17305_orig_web.jpg\u00a0\u00bb align=\u00a0\u00bbcenter\u00a0\u00bb _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb module_alignment=\u00a0\u00bbleft\u00a0\u00bb height=\u00a0\u00bb352px\u00a0\u00bb height_tablet=\u00a0\u00bb352px\u00a0\u00bb height_phone=\u00a0\u00bb100px\u00a0\u00bb height_last_edited=\u00a0\u00bbon|phone\u00a0\u00bb max_height=\u00a0\u00bb457px\u00a0\u00bb border_radii=\u00a0\u00bbon|20px|20px|20px|20px\u00a0\u00bb box_shadow_style=\u00a0\u00bbpreset3″ global_colors_info=\u00a0\u00bb{}\u00a0\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb text_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

NASA\/JPL-Caltech\/University of Arizona<\/span><\/p>\n

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<\/span><\/span>L’origine et les processus d’\u00e9volution des deux lunes sont encore inconnus, et deux hypoth\u00e8ses majeures sont actuellement d\u00e9battues :
1.<\/strong> Phobos et Deimos seraient de simples ast\u00e9ro\u00efdes captur\u00e9s par l\u2019attraction de Mars ?
2.<\/strong> Ces satellites pourraient \u00eatre n\u00e9s d\u2019un violent impact sur Mars, \u00e0 l\u2019instar de la formation de la Lune ?<\/span><\/h6>\n

[\/et_pb_text][et_pb_image src=\u00a0\u00bb\/mirs-public\/files\/2024\/03\/TSUNAMI_MARS_OUV-6398.jpeg\u00a0\u00bb title_text=\u00a0\u00bbTSUNAMI_MARS_OUV-6398″ align=\u00a0\u00bbcenter\u00a0\u00bb _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb height=\u00a0\u00bb320px\u00a0\u00bb max_height=\u00a0\u00bb320px\u00a0\u00bb custom_margin=\u00a0\u00bb||0px||false|false\u00a0\u00bb custom_padding=\u00a0\u00bb||32px||false|false\u00a0\u00bb filter_saturate=\u00a0\u00bb109%\u00a0\u00bb filter_brightness=\u00a0\u00bb114%\u00a0\u00bb filter_contrast=\u00a0\u00bb89%\u00a0\u00bb filter_sepia=\u00a0\u00bb4%\u00a0\u00bb border_radii=\u00a0\u00bbon|20px|20px|20px|20px\u00a0\u00bb box_shadow_style=\u00a0\u00bbpreset3″ global_colors_info=\u00a0\u00bb{}\u00a0\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb text_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb custom_padding=\u00a0\u00bb||0px|||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

VUE D\u2019ARTISTE D\u2019UN IMPACT SUR MARS. \u00a9 JOE TUCCIARONE<\/span><\/p>\n

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<\/span><\/span>Dans la premi\u00e8re hypoth\u00e8se, les similitudes compositionnelles et morphologiques avec les ast\u00e9ro\u00efdes primitives de type CD peuvent indiquer que Phobos et Deimos sont des ast\u00e9ro\u00efdes captur\u00e9s.
Dans la deuxi\u00e8me hypoth\u00e8se, les \u00e9jectas d’un impact g\u00e9ant sur Mars pourraient avoir form\u00e9 un disque circumplan\u00e9taire, avec diff\u00e9rents sc\u00e9narios :
<\/span><\/h6>\n
1.<\/strong> Phobos et Deimos sont les survivants d’une douzaine de corps r\u00e9accumul\u00e9s en orbite autour de Mars\u00a0 ; <\/span><\/h6>\n
2.<\/strong> Phobos subit de multiples cycles de destruction et de r\u00e9accr\u00e9tion par mar\u00e9e proches de la limite de Roche de Mars ; <\/span><\/h6>\n
3.<\/strong> Phobos et Deimos seraient constitu\u00e9s d’un m\u00e9lange (\u00e0 parts \u00e9gales) du manteau martien \u2028et de mat\u00e9riaux de l’impacteur dont la composition pourrait ressembler \u2028au manteau martien volatilis\u00e9 \u00a0; <\/span><\/h6>\n
4.<\/strong> Phobos et Deimos auraient pu se former \u00e0 partir de la d\u00e9sint\u00e9gration d’un corps parent commun qui tournait d\u00e9j\u00e0 autour de Mars \u00e0 proximit\u00e9 de la distance de l’orbite synchrone.\u00a0<\/span><\/h6>\n

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Surface de mars prise par Viking 1 – NASA<\/span><\/p>\n

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<\/span><\/span>L’hypoth\u00e8se de l’impact g\u00e9ant explique l’orbite actuelle de Phobos et Deimos, mais ne peut pas reproduire les caract\u00e9ristiques spectrales actuellement observ\u00e9es de Phobos et Deimos. Ainsi, une implantation du vent solaire et\/ou des bombardements de microm\u00e9t\u00e9oro\u00efdes devraient \u00eatre n\u00e9cessaires pour d\u00e9montrer leurs spectres actuels. En revanche, l\u2019hypoth\u00e8se de la capture de l\u2019ast\u00e9ro\u00efde convient pour expliquer les formes, les propri\u00e9t\u00e9s spectroscopiques et de surface de ces lunes, mais leurs orbites actuelles quasi circulaires et \u00e0 faible inclinaison autour de Mars sont difficiles \u00e0 expliquer dynamiquement par capture externe.<\/span><\/h6>\n

[\/et_pb_text][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb header_4_font=\u00a0\u00bbCommissioner|700||||on|||\u00a0\u00bb header_4_font_size=\u00a0\u00bb40px\u00a0\u00bb header_4_line_height=\u00a0\u00bb1.4em\u00a0\u00bb header_5_font=\u00a0\u00bbCommissioner|600|||||||\u00a0\u00bb header_5_font_size=\u00a0\u00bb23px\u00a0\u00bb header_5_line_height=\u00a0\u00bb1.6em\u00a0\u00bb header_6_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb header_6_font_size=\u00a0\u00bb20px\u00a0\u00bb header_6_line_height=\u00a0\u00bb2em\u00a0\u00bb custom_padding=\u00a0\u00bb50px|||||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

<\/span>La mission<\/span><\/h4>\n

 <\/p>\n

<\/span><\/span><\/span>Pour bien r\u00e9pondre \u00e0 ces questions, la mission MMX sera lanc\u00e9e en Octobre 2026 \u2028vers le syst\u00e8me martien pour ramener des \u00e9chantillons de la surface de Phobos, \u2028effectuer des observations d\u00e9taill\u00e9es de Phobos et de Deimos et surveiller le climat de Mars.
La mission effectuera un voyage aller-retour en cinq ans, avec retour sur Terre des \u00e9chantillons \u2028de Phobos en Juillet 2031. La sonde arrivera dans le syst\u00e8me Martien en Ao\u00fbt 2027. \u2028Elle restera trois ans sur des orbites quasi-satellitaires (QSO) autour de Phobos \u2028\u00e0 diff\u00e9rentes altitudes pour s\u00e9lectionner les sites d\u2019\u00e9chantillonnage et d\u2019atterrissage.<\/span><\/h6>\n

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MMX ORBITES<\/span><\/span><\/span><\/p>\n

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MMX est \u00e9quip\u00e9 de 13 instruments dont le spectrom\u00e8tre fran\u00e7ais MIRS et le rover franco-allemand IDEFIX, un d\u00e9monstrateur de rover, et les deux m\u00e9canismes d\u2019\u00e9chantillonnage.<\/span><\/h6>\n

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<\/span>La charge utile comprendre les instruments scientifiques:<\/span><\/h5>\n

<\/span><\/p>\n

<\/span><\/span><\/p>\n

    \n
  • \n
    MIRS (MMX InfraRed Spectrometer)<\/span><\/h6>\n<\/li>\n
  • \n
    OROCHI (Optical RadiOmeter composed of Chromatic Imagers)<\/span><\/h6>\n<\/li>\n
  • \n
    TENGOO (Telescopic Nadir for GeOmOrphology)
    <\/span><\/h6>\n<\/li>\n
  • \n
    LIDAR (Light Detection And Ranging)<\/span><\/h6>\n<\/li>\n
  • \n
    MEGANE (Mars-moon Exploration with Gamma rays and Neutrons)
    <\/span><\/h6>\n<\/li>\n
  • \n
    CMDM (Circum-Martian Dust Monitor)<\/span><\/h6>\n<\/li>\n
  • \n
    MSA (Mass Spectrum Analyzer)<\/span><\/h6>\n<\/li>\n
  • \n
    C-SMP (Coring sampler)<\/span><\/h6>\n<\/li>\n
  • \n
    P-SMP (Pneumatic sampler)<\/span><\/h6>\n<\/li>\n
  • \n
    ROVER-IDEFIX (Moving vehicle)<\/span><\/h6>\n<\/li>\n
  • \n
    SRC (Sample return capsule)<\/span><\/h6>\n<\/li>\n<\/ul>\n
      \n
    • \n
      SHV (Super Hi Vision Cameras)<\/span><\/h6>\n<\/li>\n
    • \n
      IREM (Interplanetary Radiation Enviroments Monitor)<\/span><\/h6>\n<\/li>\n<\/ul>\n

      [\/et_pb_text][et_pb_image src=\u00a0\u00bb\/mirs-public\/files\/2024\/03\/IMG_20240123_170731810-rotated-1.jpeg\u00a0\u00bb title_text=\u00a0\u00bbIMG_20240123_170731810″ align=\u00a0\u00bbcenter\u00a0\u00bb _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb height=\u00a0\u00bb579px\u00a0\u00bb height_tablet=\u00a0\u00bb579px\u00a0\u00bb height_phone=\u00a0\u00bb579px\u00a0\u00bb height_last_edited=\u00a0\u00bbon|phone\u00a0\u00bb max_height=\u00a0\u00bb318px\u00a0\u00bb custom_margin=\u00a0\u00bb||26px||false|false\u00a0\u00bb border_radii=\u00a0\u00bbon|20px|20px|20px|20px\u00a0\u00bb box_shadow_style=\u00a0\u00bbpreset3″ global_colors_info=\u00a0\u00bb{}\u00a0\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb text_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

      Maquette \u00e0 l\u2019\u00e9chelle 1:2 de la sonde MMX – JAXA<\/span><\/p>\n

      [\/et_pb_text][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb text_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb text_font_size=\u00a0\u00bb20px\u00a0\u00bb text_line_height=\u00a0\u00bb2em\u00a0\u00bb header_6_font=\u00a0\u00bb|600|||||||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

      <\/span><\/span>La sonde descendra pendant plusieurs heures sur la surface de Phobos pour collecter au moins \u202810 g du r\u00e9golithe de Phobos \u00e0 l\u2019aide de deux diff\u00e9rents m\u00e9canismes d\u2019\u00e9chantillonnage\u00a0: C-SMP (Coring Sampler) et P-SMP (Pneumating Sampler). MMX collectera des \u00e9chantillons de Phobos \u2028sur deux sites diff\u00e9rents.
      Apr\u00e8s le pr\u00e9l\u00e8vement des \u00e9chantillons, la sonde quittera le syst\u00e8me martien \u2028et ram\u00e8nera les \u00e9chantillons sur Terre, achevant le premier aller-retour vers le syst\u00e8me \u2028de la plan\u00e8te rouge.<\/span><\/p>\n

      [\/et_pb_text][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb header_4_font=\u00a0\u00bbCommissioner|700||||on|||\u00a0\u00bb header_4_font_size=\u00a0\u00bb40px\u00a0\u00bb header_4_letter_spacing=\u00a0\u00bb2px\u00a0\u00bb header_5_font=\u00a0\u00bbCommissioner|600|||||||\u00a0\u00bb header_5_font_size=\u00a0\u00bb23px\u00a0\u00bb header_5_line_height=\u00a0\u00bb1.6em\u00a0\u00bb header_6_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb header_6_font_size=\u00a0\u00bb20px\u00a0\u00bb header_6_line_height=\u00a0\u00bb2em\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

      <\/span><\/span>Les objectifs<\/span><\/h4>\n
      <\/h5>\n
      <\/h6>\n
      <\/span><\/span><\/span>Les objectives majeurs de cette mission sont de :<\/span><\/h6>\n

       <\/p>\n

      1.<\/strong> R\u00e9soudre la controverse sur l’origine des lunes martiennes par des observations rapproch\u00e9es \u2028et des retours d’\u00e9chantillons<\/h6>\n
      2.<\/strong> Contraindre les processus de formation plan\u00e9taire, de transport de mat\u00e9riaux dans la r\u00e9gion \u2028de transition du Syst\u00e8me solaire interne et externe, et les conditions d\u2019apparition de l\u2019eau \u2028sur les plan\u00e8tes de type terrestre <\/span><\/h6>\n
      3.<\/strong> R\u00e9v\u00e9ler les processus \u00e9volutifs du syst\u00e8me martien dans les environnements circum-martiens<\/span><\/h6>\n
      <\/span><\/span>L’instrument MIRS, associ\u00e9 \u00e0 la charge utile MMX et \u00e0 l’analyse d’\u00e9chantillons, sera en mesure \u2028de d\u2019\u00e9lucider l’origine des lunes martiennes et pourrait \u00e9galement \u00eatre en mesure d’\u00e9clairer \u2028le processus d’\u00e9volution de l’environnement de Mars.<\/span><\/h6>\n
      <\/span><\/h5>\n
      <\/span><\/h5>\n
      <\/span><\/span>MMX est en cours de d\u00e9veloppement et de construction par la JAXA, avec des contributions du CNES, NASA, ESA et DLR.\u00a0<\/span><\/h5>\n

      [\/et_pb_text][et_pb_image src=\u00a0\u00bb\/mirs-public\/files\/2024\/03\/main-123.jpg\u00a0\u00bb title_text=\u00a0\u00bbmain-123″ align=\u00a0\u00bbcenter\u00a0\u00bb _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb width=\u00a0\u00bb60%\u00a0\u00bb max_width=\u00a0\u00bb60%\u00a0\u00bb height=\u00a0\u00bb331px\u00a0\u00bb height_tablet=\u00a0\u00bb260px\u00a0\u00bb height_phone=\u00a0\u00bb144px\u00a0\u00bb height_last_edited=\u00a0\u00bbon|tablet\u00a0\u00bb max_height=\u00a0\u00bb331px\u00a0\u00bb custom_margin=\u00a0\u00bb||30px|||\u00a0\u00bb border_radii=\u00a0\u00bbon|20px|20px|20px|20px\u00a0\u00bb box_shadow_style=\u00a0\u00bbpreset3″ global_colors_info=\u00a0\u00bb{}\u00a0\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00a0\u00bb4.24.2″ _module_preset=\u00a0\u00bbdefault\u00a0\u00bb text_font=\u00a0\u00bbCommissioner|300|||||||\u00a0\u00bb custom_margin=\u00a0\u00bb-10px|||||\u00a0\u00bb global_colors_info=\u00a0\u00bb{}\u00a0\u00bb]<\/p>\n

      Vue d\u2019artiste de la sonde MMX pos\u00e9e sur la surface de Phobos – JAXA<\/p>\n

      [\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"

      MIRSMissionMMX La mission\u00a0Martian Moons eXploration\u00a0(MMX) de la JAXA (Japan Aerospace Exploration Agency)\u00a0 est la premi\u00e8re mission de retour d\u2019\u00e9chantillons du satellite Phobos. Elle pr\u00e9voit \u00e9galement une exploration du syst\u00e8me de la plan\u00e8te Mars. L\u2019objectif principal de la mission est d\u2019\u00e9lucider l\u2019origine des lunes martiennes, ce qui fournira des informations importantes sur la formation des plan\u00e8tes […]<\/p>\n","protected":false},"author":93,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"","footnotes":""},"class_list":["post-51","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"\/mirs-public\/wp-json\/wp\/v2\/pages\/51","targetHints":{"allow":["GET"]}}],"collection":[{"href":"\/mirs-public\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"\/mirs-public\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"\/mirs-public\/wp-json\/wp\/v2\/users\/93"}],"replies":[{"embeddable":true,"href":"\/mirs-public\/wp-json\/wp\/v2\/comments?post=51"}],"version-history":[{"count":27,"href":"\/mirs-public\/wp-json\/wp\/v2\/pages\/51\/revisions"}],"predecessor-version":[{"id":3376,"href":"\/mirs-public\/wp-json\/wp\/v2\/pages\/51\/revisions\/3376"}],"wp:attachment":[{"href":"\/mirs-public\/wp-json\/wp\/v2\/media?parent=51"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}