A shear heating origin for ridges on Triton

<!DOCTYPE html>     <html class="no-js" lang="en">  <head> <title>A shear heating origin for ridges on Triton - NASA/ADS</title>  <link rel="apple-touch-icon" sizes="180x180" href="//styles/favicon/apple-touch-icon.png" /> <link rel="icon" type="image/png" sizes="32x32" href="//styles/favicon/favicon-32x32.png" /> <link rel="icon" type="image/png" sizes="16x16" href="//styles/favicon/favicon-16x16.png" /> <link rel="manifest" href="//styles/favicon/site.webmanifest" /> <link rel="mask-icon" href="//styles/favicon/safari-pinned-tab.svg" color="#5bbad5" /> <meta name="apple-mobile-web-app-title" content="NASA ADS" /> <meta name="application-name" content="NASA ADS" /> <meta name="msapplication-TileColor" content="#ffc40d" /> <meta name="theme-color" content="#ffffff" />  <link rel="stylesheet" href="/styles/css/styles.css"> <meta name="robots" content="noarchive"> <link rel="canonical" href="http://ui.adsabs.harvard.edu/abs/2005GeoRL..3214202P/abstract"/> <meta name="description" content="Triton and Europa each display a variety of distinctive curvilinear ridges and associated troughs. Here we propose that ridges on Triton may have formed by diurnal tidal stresses, in a manner similar to that proposed for ridge formation on Europa. The greater width of ridges on Triton is likely a consequence of the lower surface temperature and greater brittle-ductile transition depth on this body compared to Europa. The magnitudes of the stresses and heat fluxes required to generate ridges of the correct scale are comparable to likely values generated during the latter part of Triton's orbital evolution from an initial highly eccentric state.">  <meta property="og:type" content="article"> <meta property="og:title" content="A shear heating origin for ridges on Triton"> <meta property="og:site_name" content="NASA/ADS"> <meta property="og:description" content="Triton and Europa each display a variety of distinctive curvilinear ridges and associated troughs. Here we propose that ridges on Triton may have formed by diurnal tidal stresses, in a manner similar to that proposed for ridge formation on Europa. The greater width of ridges on Triton is likely a consequence of the lower surface temperature and greater brittle-ductile transition depth on this body compared to Europa. The magnitudes of the stresses and heat fluxes required to generate ridges of the correct scale are comparable to likely values generated during the latter part of Triton's orbital evolution from an initial highly eccentric state."> <meta property="og:url" content="https://ui.adsabs.harvard.edu/abs/2005GeoRL..3214202P/abstract"> <meta property="og:image" content="https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg"> <meta property="article:published_time" content="07/2005"> <meta property="article:author" content="Prockter, Louise M."> <meta property="article:author" content="Nimmo, Francis"> <meta property="article:author" content="Pappalardo, Robert T.">  <meta name="citation_journal_title" content="Geophysical Research Letters"> <meta name="citation_authors" content="Prockter, Louise M.;Nimmo, Francis;Pappalardo, Robert T."> <meta name="citation_title" content="A shear heating origin for ridges on Triton"> <meta name="citation_date" content="07/2005"> <meta name="citation_volume" content="32"> <meta name="citation_issue" content="14"> <meta name="citation_firstpage" content="L14202"> <meta name="citation_doi" content="10.1029/2005GL022832"> <meta name="citation_issn" content="0094-8276"> <meta name="citation_language" content="en"> <meta name="citation_keywords" content="Planetary Sciences: Solar System Objects: Europa"> <meta name="citation_keywords" content="Planetary Sciences: Solar System Objects: Jovian satellites"> <meta name="citation_keywords" content="Planetary Sciences: Solar System Objects: Comparative planetology"> <meta name="citation_keywords" content="Planetary Sciences: Solar System Objects: Neptunian satellites"> <meta name="citation_keywords" content="Planetary Sciences: Solar System Objects: Triton"> <meta name="citation_abstract_html_url" content="https://ui.adsabs.harvard.edu/abs/2005GeoRL..3214202P/abstract"> <meta name="citation_publication_date" content="07/2005"> <link title="schema(PRISM)" rel="schema.prism" href="http://prismstandard.org/namespaces/1.2/basic/" /> <meta name="prism.publicationDate" content="07/2005" /> <meta name="prism.publicationName" content="GeoRL" /> <meta name="prism.issn" content="0094-8276" /> <meta name="prism.volume" content="32" /> <meta name="prism.startingPage" content="L14202" /> <link title="schema(DC)" rel="schema.dc" href="http://purl.org/dc/elements/1.1/" /> <meta name="dc.identifier" content="doi:10.1029/2005GL022832" /> <meta name="dc.date" content="07/2005" /> <meta name="dc.source" content="GeoRL" /> <meta name="dc.title" content="A shear heating origin for ridges on Triton" /> <meta name="dc.creator" content="Prockter, Louise M."> <meta name="dc.creator" content="Nimmo, Francis"> <meta name="dc.creator" content="Pappalardo, Robert T.">  <meta name="twitter:card" content="summary_large_image"/> <meta name="twitter:description" content="Triton and Europa each display a variety of distinctive curvilinear ridges and associated troughs. Here we propose that ridges on Triton may have formed by diurnal tidal stresses, in a manner similar to that proposed for ridge formation on Europa. The greater width of ridges on Triton is likely a consequence of the lower surface temperature and greater brittle-ductile transition depth on this body compared to Europa. The magnitudes of the stresses and heat fluxes required to generate ridges of the correct scale are comparable to likely values generated during the latter part of Triton's orbital evolution from an initial highly eccentric state."/> <meta name="twitter:title" content="A shear heating origin for ridges on Triton"/> <meta name="twitter:site" content="@adsabs"/> <meta name="twitter:domain" content="NASA/ADS"/> <meta name="twitter:image:src" content="https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg"/> <meta name="twitter:creator" content="@adsabs"/> <meta charset="utf-8"> <meta name="viewport" content="width=device-width, initial-scale=1, shrink-to-fit=no"> <base href="/"> <style> .btn-full-ads { color: #fff !important; background-color: #1a1a1a !important; border-color: #1a1a1a !important; margin-top: 9px !important; padding-bottom: 10px !important; padding-top: 10px !important; } .btn-full-ads:hover, .btn-full-ads:focus, .btn-full-ads:active, .btn-full-ads.active, 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A shear heating origin for ridges on Triton - NASA/ADS