See Roche lobe on Wiktionary
{ "etymology_text": "Named after Édouard Roche.", "forms": [ { "form": "Roche lobes", "tags": [ "plural" ] } ], "head_templates": [ { "args": {}, "expansion": "Roche lobe (plural Roche lobes)", "name": "en-noun" } ], "lang": "English", "lang_code": "en", "pos": "noun", "senses": [ { "categories": [ { "kind": "other", "name": "English entries with incorrect language header", "parents": [ "Entries with incorrect language header", "Entry maintenance" ], "source": "w" }, { "kind": "other", "name": "English entries with language name categories using raw markup", "parents": [ "Entries with language name categories using raw markup", "Entry maintenance" ], "source": "w" }, { "kind": "other", "name": "English terms with non-redundant non-automated sortkeys", "parents": [ "Terms with non-redundant non-automated sortkeys", "Entry maintenance" ], "source": "w" }, { "kind": "other", "name": "Pages with 1 entry", "parents": [], "source": "w" }, { "kind": "other", "name": "Pages with entries", "parents": [], "source": "w" }, { "kind": "topical", "langcode": "en", "name": "Astronomy", "orig": "en:Astronomy", "parents": [ "Sciences", "Space", "All topics", "Nature", "Fundamental" ], "source": "w" } ], "examples": [ { "ref": "2002, Juhan Frank, Andrew King, Derek Raine, Accretion Power in Astrophysics, page 54:", "text": "A further interesting situation (although not one of much relevance for this book) comes about if both stars for some reason fill their Roche lobes simultaneously.", "type": "quote" }, { "ref": "2012, C. de Loore, C. Doom, Structure and Evolution of Single and Binary Stars, page 386:", "text": "Generally, mass transfer by Roche lobe overflow is required to power LMXRB's, since low mass stars never exhibit strong stellar winds.", "type": "quote" }, { "ref": "2013, Josef Kallrath, Eugene F. Milone, Eclipsing Binary Stars: Modeling and Analysis, page 85:", "text": "If only one component accurately fills its Roche lobe the system is semi-detached. If neither fills its Roche lobe, it is detached.", "type": "quote" } ], "glosses": [ "The teardrop-shaped region around a star in a binary system within which orbiting material is gravitationally bound to that star." ], "id": "en-Roche_lobe-en-noun-0lWImYyI", "links": [ [ "astronomy", "astronomy" ], [ "teardrop", "teardrop" ], [ "star", "star" ], [ "binary system", "binary system" ], [ "orbit", "orbit" ], [ "gravitationally", "gravitationally" ], [ "bound", "bind" ] ], "raw_glosses": [ "(astronomy) The teardrop-shaped region around a star in a binary system within which orbiting material is gravitationally bound to that star." ], "related": [ { "word": "Roche limit" }, { "word": "Roche sphere" } ], "topics": [ "astronomy", "natural-sciences" ], "wikipedia": [ "Roche lobe", "Édouard Roche" ] } ], "word": "Roche lobe" }
{ "etymology_text": "Named after Édouard Roche.", "forms": [ { "form": "Roche lobes", "tags": [ "plural" ] } ], "head_templates": [ { "args": {}, "expansion": "Roche lobe (plural Roche lobes)", "name": "en-noun" } ], "lang": "English", "lang_code": "en", "pos": "noun", "related": [ { "word": "Roche limit" }, { "word": "Roche sphere" } ], "senses": [ { "categories": [ "English countable nouns", "English entries with incorrect language header", "English entries with language name categories using raw markup", "English eponyms", "English lemmas", "English multiword terms", "English nouns", "English terms with non-redundant non-automated sortkeys", "English terms with quotations", "Pages with 1 entry", "Pages with entries", "en:Astronomy" ], "examples": [ { "ref": "2002, Juhan Frank, Andrew King, Derek Raine, Accretion Power in Astrophysics, page 54:", "text": "A further interesting situation (although not one of much relevance for this book) comes about if both stars for some reason fill their Roche lobes simultaneously.", "type": "quote" }, { "ref": "2012, C. de Loore, C. Doom, Structure and Evolution of Single and Binary Stars, page 386:", "text": "Generally, mass transfer by Roche lobe overflow is required to power LMXRB's, since low mass stars never exhibit strong stellar winds.", "type": "quote" }, { "ref": "2013, Josef Kallrath, Eugene F. Milone, Eclipsing Binary Stars: Modeling and Analysis, page 85:", "text": "If only one component accurately fills its Roche lobe the system is semi-detached. If neither fills its Roche lobe, it is detached.", "type": "quote" } ], "glosses": [ "The teardrop-shaped region around a star in a binary system within which orbiting material is gravitationally bound to that star." ], "links": [ [ "astronomy", "astronomy" ], [ "teardrop", "teardrop" ], [ "star", "star" ], [ "binary system", "binary system" ], [ "orbit", "orbit" ], [ "gravitationally", "gravitationally" ], [ "bound", "bind" ] ], "raw_glosses": [ "(astronomy) The teardrop-shaped region around a star in a binary system within which orbiting material is gravitationally bound to that star." ], "topics": [ "astronomy", "natural-sciences" ], "wikipedia": [ "Roche lobe", "Édouard Roche" ] } ], "word": "Roche lobe" }
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This page is a part of the kaikki.org machine-readable All languages combined dictionary. This dictionary is based on structured data extracted on 2025-02-22 from the enwiktionary dump dated 2025-02-02 using wiktextract (9e2b7d3 and f2e72e5). The data shown on this site has been post-processed and various details (e.g., extra categories) removed, some information disambiguated, and additional data merged from other sources. See the raw data download page for the unprocessed wiktextract data.
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