See massive compact halo object on Wiktionary
{ "etymology_text": "Perhaps coined with the acronym, MACHO, in mind. See also WIMP, which represents a competing hypothesis.", "forms": [ { "form": "massive compact halo objects", "tags": [ "plural" ] } ], "head_templates": [ { "args": {}, "expansion": "massive compact halo object (plural massive compact halo objects)", "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": "Entries with translation boxes", "parents": [], "source": "w" }, { "kind": "other", "name": "Pages with 1 entry", "parents": [], "source": "w" }, { "kind": "other", "name": "Pages with entries", "parents": [], "source": "w" }, { "kind": "other", "name": "Terms with Finnish translations", "parents": [], "source": "w" }, { "kind": "other", "name": "Terms with Mandarin translations", "parents": [], "source": "w" }, { "kind": "topical", "langcode": "en", "name": "Astronomy", "orig": "en:Astronomy", "parents": [ "Sciences", "Space", "All topics", "Nature", "Fundamental" ], "source": "w" }, { "kind": "topical", "langcode": "en", "name": "Physics", "orig": "en:Physics", "parents": [ "Sciences", "All topics", "Fundamental" ], "source": "w" } ], "coordinate_terms": [ { "english": "WIMP", "word": "weakly interacting massive particle" }, { "alt": "SIMP", "word": "strongly interacting massive particle" }, { "alt": "RAMBO", "word": "robust associations of massive baryonic objects" } ], "derived": [ { "tags": [ "abbreviation" ], "word": "MACHO" } ], "glosses": [ "Any kind of astronomical body comprising normal baryonic matter that in sufficient numbers might explain the apparent presence of dark matter in galaxy halos." ], "hypernyms": [ { "english": "non-luminous matter needed to balance the orbital speeds observed in stars in galaxies with the observed luminous mass of the galaxy in question", "word": "dark matter" } ], "id": "en-massive_compact_halo_object-en-noun-Mdo1RFPn", "links": [ [ "astronomy", "astronomy" ], [ "physics", "physics" ], [ "astronomical", "astronomical" ], [ "baryonic", "baryonic" ], [ "dark matter", "dark matter" ], [ "galaxy", "galaxy" ], [ "halo", "halo" ] ], "raw_glosses": [ "(astronomy, physics) Any kind of astronomical body comprising normal baryonic matter that in sufficient numbers might explain the apparent presence of dark matter in galaxy halos." ], "synonyms": [ { "tags": [ "abbreviation" ], "word": "MACHO" }, { "word": "massive astronomical compact halo object" }, { "word": "massive astrophysical compact halo object" }, { "word": "massive and compact halo object" } ], "topics": [ "astronomy", "natural-sciences", "physical-sciences", "physics" ], "translations": [ { "code": "cmn", "lang": "Chinese Mandarin", "sense": "astronomical body", "word": "暈族大質量緻密天體" }, { "code": "cmn", "lang": "Chinese Mandarin", "roman": "yūnzú dàzhìliàng zhìmì tiāntǐ", "sense": "astronomical body", "word": "晕族大质量致密天体" }, { "code": "fi", "lang": "Finnish", "sense": "astronomical body", "word": "massiivinen kompakti halo-objekti" } ], "wikipedia": [ "Massive compact halo object" ] } ], "word": "massive compact halo object" }
{ "coordinate_terms": [ { "english": "WIMP", "word": "weakly interacting massive particle" }, { "alt": "SIMP", "word": "strongly interacting massive particle" }, { "alt": "RAMBO", "word": "robust associations of massive baryonic objects" } ], "derived": [ { "tags": [ "abbreviation" ], "word": "MACHO" } ], "etymology_text": "Perhaps coined with the acronym, MACHO, in mind. See also WIMP, which represents a competing hypothesis.", "forms": [ { "form": "massive compact halo objects", "tags": [ "plural" ] } ], "head_templates": [ { "args": {}, "expansion": "massive compact halo object (plural massive compact halo objects)", "name": "en-noun" } ], "hypernyms": [ { "english": "non-luminous matter needed to balance the orbital speeds observed in stars in galaxies with the observed luminous mass of the galaxy in question", "word": "dark matter" } ], "lang": "English", "lang_code": "en", "pos": "noun", "senses": [ { "categories": [ "English countable nouns", "English entries with incorrect language header", "English lemmas", "English multiword terms", "English nouns", "Entries with translation boxes", "Pages with 1 entry", "Pages with entries", "Terms with Finnish translations", "Terms with Mandarin translations", "en:Astronomy", "en:Physics" ], "glosses": [ "Any kind of astronomical body comprising normal baryonic matter that in sufficient numbers might explain the apparent presence of dark matter in galaxy halos." ], "links": [ [ "astronomy", "astronomy" ], [ "physics", "physics" ], [ "astronomical", "astronomical" ], [ "baryonic", "baryonic" ], [ "dark matter", "dark matter" ], [ "galaxy", "galaxy" ], [ "halo", "halo" ] ], "raw_glosses": [ "(astronomy, physics) Any kind of astronomical body comprising normal baryonic matter that in sufficient numbers might explain the apparent presence of dark matter in galaxy halos." ], "topics": [ "astronomy", "natural-sciences", "physical-sciences", "physics" ], "wikipedia": [ "Massive compact halo object" ] } ], "synonyms": [ { "tags": [ "abbreviation" ], "word": "MACHO" }, { "word": "massive astronomical compact halo object" }, { "word": "massive astrophysical compact halo object" }, { "word": "massive and compact halo object" } ], "translations": [ { "code": "cmn", "lang": "Chinese Mandarin", "sense": "astronomical body", "word": "暈族大質量緻密天體" }, { "code": "cmn", "lang": "Chinese Mandarin", "roman": "yūnzú dàzhìliàng zhìmì tiāntǐ", "sense": "astronomical body", "word": "晕族大质量致密天体" }, { "code": "fi", "lang": "Finnish", "sense": "astronomical body", "word": "massiivinen kompakti halo-objekti" } ], "word": "massive compact halo object" }
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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 2024-12-15 from the enwiktionary dump dated 2024-12-04 using wiktextract (8a39820 and 4401a4c). 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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