"kilonova" meaning in All languages combined

See kilonova on Wiktionary

Noun [English]

Forms: kilonovas [plural], kilonovae [plural]
Etymology: kilo- + nova. From kilo- (“thousands”). From being much more luminous than a nova, but less so than a typical supernova. Etymology templates: {{prefix|en|kilo|nova}} kilo- + nova, {{m|en|kilo-||thousands}} kilo- (“thousands”), {{m|en|nova}} nova, {{m|en|supernova}} supernova Head templates: {{en-noun|s|kilonovae}} kilonova (plural kilonovas or kilonovae)
  1. (astronomy) A type of supernova that is underluminous, caused by the merger of two neutron stars Categories (topical): Astronomy, Black holes, Neutron stars
    Sense id: en-kilonova-en-noun-jdvWl4J6 Disambiguation of Black holes: 76 24 Disambiguation of Neutron stars: 73 27 Categories (other): English entries with incorrect language header, English entries with topic categories using raw markup, English terms prefixed with kilo-, Supernovas Disambiguation of English entries with incorrect language header: 74 26 Disambiguation of English entries with topic categories using raw markup: 69 31 Disambiguation of English terms prefixed with kilo-: 69 31 Disambiguation of Supernovas: 88 12 Topics: astronomy, natural-sciences
  2. (informal, physics) A radiation pattern typical of a kilonova. Tags: informal Categories (topical): Physics
    Sense id: en-kilonova-en-noun-xEgaj~vo Topics: natural-sciences, physical-sciences, physics
The following are not (yet) sense-disambiguated
Synonyms: KN, macronova Derived forms: KN Coordinate_terms: hypernova, supernova, unnova

Inflected forms

Alternative forms

Download JSON data for kilonova meaning in All languages combined (5.1kB)

{
  "coordinate_terms": [
    {
      "_dis1": "0 0",
      "word": "hypernova"
    },
    {
      "_dis1": "0 0",
      "word": "supernova"
    },
    {
      "_dis1": "0 0",
      "word": "unnova"
    }
  ],
  "derived": [
    {
      "_dis1": "0 0",
      "word": "KN"
    }
  ],
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "kilo",
        "3": "nova"
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      "expansion": "kilo- + nova",
      "name": "prefix"
    },
    {
      "args": {
        "1": "en",
        "2": "kilo-",
        "3": "",
        "4": "thousands"
      },
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      "name": "m"
    },
    {
      "args": {
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        "1": "en",
        "2": "supernova"
      },
      "expansion": "supernova",
      "name": "m"
    }
  ],
  "etymology_text": "kilo- + nova. From kilo- (“thousands”). From being much more luminous than a nova, but less so than a typical supernova.",
  "forms": [
    {
      "form": "kilonovas",
      "tags": [
        "plural"
      ]
    },
    {
      "form": "kilonovae",
      "tags": [
        "plural"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {
        "1": "s",
        "2": "kilonovae"
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      "expansion": "kilonova (plural kilonovas or kilonovae)",
      "name": "en-noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
      "categories": [
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Astronomy",
          "orig": "en:Astronomy",
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          "source": "w"
        },
        {
          "_dis": "74 26",
          "kind": "other",
          "name": "English entries with incorrect language header",
          "parents": [
            "Entries with incorrect language header",
            "Entry maintenance"
          ],
          "source": "w+disamb"
        },
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          "_dis": "69 31",
          "kind": "other",
          "name": "English entries with topic categories using raw markup",
          "parents": [
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          "source": "w+disamb"
        },
        {
          "_dis": "69 31",
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          "parents": [],
          "source": "w+disamb"
        },
        {
          "_dis": "88 12",
          "kind": "other",
          "langcode": "en",
          "name": "Supernovas",
          "orig": "en:Supernovas",
          "parents": [],
          "source": "w+disamb"
        },
        {
          "_dis": "76 24",
          "kind": "topical",
          "langcode": "en",
          "name": "Black holes",
          "orig": "en:Black holes",
          "parents": [
            "Astronomy",
            "Astrophysics",
            "Gravity",
            "Relativity",
            "Sciences",
            "Space",
            "Physics",
            "Acceleration",
            "Mechanics",
            "All topics",
            "Nature",
            "Fundamental"
          ],
          "source": "w+disamb"
        },
        {
          "_dis": "73 27",
          "kind": "topical",
          "langcode": "en",
          "name": "Neutron stars",
          "orig": "en:Neutron stars",
          "parents": [
            "Astrophysics",
            "Gravity",
            "Neutron",
            "Relativity",
            "Stars",
            "Astronomy",
            "Physics",
            "Acceleration",
            "Mechanics",
            "Nuclear physics",
            "Celestial bodies",
            "Sciences",
            "Space",
            "Quantum mechanics",
            "All topics",
            "Nature",
            "Fundamental"
          ],
          "source": "w+disamb"
        }
      ],
      "glosses": [
        "A type of supernova that is underluminous, caused by the merger of two neutron stars"
      ],
      "id": "en-kilonova-en-noun-jdvWl4J6",
      "links": [
        [
          "astronomy",
          "astronomy"
        ],
        [
          "supernova",
          "supernova"
        ],
        [
          "neutron star",
          "neutron star"
        ]
      ],
      "raw_glosses": [
        "(astronomy) A type of supernova that is underluminous, caused by the merger of two neutron stars"
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ]
    },
    {
      "categories": [
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Physics",
          "orig": "en:Physics",
          "parents": [
            "Sciences",
            "All topics",
            "Fundamental"
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          "source": "w"
        }
      ],
      "examples": [
        {
          "ref": "2013 November, V Paschalidis, SL Shapiro, “A new scheme for matching general relativistic ideal magnetohydrodynamics to its force-free limit”, in Physical Review D",
          "text": "Moreover, during merger neutron-rich matter can be ejected that can shine as a kilonova due to the decay of r-process elements [2–13].",
          "type": "quotation"
        },
        {
          "ref": "2013 December, YZ Fan, YW Yu, D Xu, ZP Jin, XF Wu, “A supramassive magnetar central engine for GRB 130603B”, in The Astrophysical Journal Letters, volume 779, number 2",
          "text": "The observed energetics and temporal/spectral properties of the late infrared bump (ie, the \"kilonova\") are also found to be consistent with emission from the ejecta launched during a neutron star (NS)-NS merger and powered by a magnetar central engine.",
          "type": "quotation"
        },
        {
          "ref": "2015 January, R Fernandez, D Kasen, BD Metzger, “The effect of black hole spin on winds from neutron star merger remnant accretion disks”, in American Astronomical Society, AAS Meeting #225",
          "text": "Disk winds generally contribute to a ~week long transient peaking in the near-infrared (kilonova), although an optical precursor can manifest as a signature of delayed black hole formation or high black hole spin.",
          "type": "quotation"
        },
        {
          "ref": "2015, R Fernández, D Kasen, “Outflows from accretion discs formed in neutron star mergers: effect of black hole spin”, in (Please provide the book title or journal name)",
          "text": "This component can give rise to an ≲1 d blue optical 'bump' in a kilonova light curve, even in the case of prompt BH formation, which may facilitate its detection.",
          "type": "quotation"
        }
      ],
      "glosses": [
        "A radiation pattern typical of a kilonova."
      ],
      "id": "en-kilonova-en-noun-xEgaj~vo",
      "links": [
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        ],
        [
          "radiation",
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      ],
      "raw_glosses": [
        "(informal, physics) A radiation pattern typical of a kilonova."
      ],
      "tags": [
        "informal"
      ],
      "topics": [
        "natural-sciences",
        "physical-sciences",
        "physics"
      ]
    }
  ],
  "synonyms": [
    {
      "_dis1": "0 0",
      "word": "KN"
    },
    {
      "_dis1": "0 0",
      "word": "macronova"
    }
  ],
  "wikipedia": [
    "kilonova"
  ],
  "word": "kilonova"
}
{
  "categories": [
    "English countable nouns",
    "English entries with incorrect language header",
    "English entries with topic categories using raw markup",
    "English lemmas",
    "English nouns",
    "English nouns with irregular plurals",
    "English terms prefixed with kilo-",
    "en:Black holes",
    "en:Neutron stars",
    "en:Supernovas"
  ],
  "coordinate_terms": [
    {
      "word": "hypernova"
    },
    {
      "word": "supernova"
    },
    {
      "word": "unnova"
    }
  ],
  "derived": [
    {
      "word": "KN"
    }
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  "etymology_templates": [
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    {
      "args": {
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        "2": "kilo-",
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        "4": "thousands"
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      "name": "m"
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    {
      "args": {
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    {
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        "1": "en",
        "2": "supernova"
      },
      "expansion": "supernova",
      "name": "m"
    }
  ],
  "etymology_text": "kilo- + nova. From kilo- (“thousands”). From being much more luminous than a nova, but less so than a typical supernova.",
  "forms": [
    {
      "form": "kilonovas",
      "tags": [
        "plural"
      ]
    },
    {
      "form": "kilonovae",
      "tags": [
        "plural"
      ]
    }
  ],
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    {
      "args": {
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    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
  "senses": [
    {
      "categories": [
        "en:Astronomy"
      ],
      "glosses": [
        "A type of supernova that is underluminous, caused by the merger of two neutron stars"
      ],
      "links": [
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      ],
      "raw_glosses": [
        "(astronomy) A type of supernova that is underluminous, caused by the merger of two neutron stars"
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ]
    },
    {
      "categories": [
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        "English terms with quotations",
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      ],
      "examples": [
        {
          "ref": "2013 November, V Paschalidis, SL Shapiro, “A new scheme for matching general relativistic ideal magnetohydrodynamics to its force-free limit”, in Physical Review D",
          "text": "Moreover, during merger neutron-rich matter can be ejected that can shine as a kilonova due to the decay of r-process elements [2–13].",
          "type": "quotation"
        },
        {
          "ref": "2013 December, YZ Fan, YW Yu, D Xu, ZP Jin, XF Wu, “A supramassive magnetar central engine for GRB 130603B”, in The Astrophysical Journal Letters, volume 779, number 2",
          "text": "The observed energetics and temporal/spectral properties of the late infrared bump (ie, the \"kilonova\") are also found to be consistent with emission from the ejecta launched during a neutron star (NS)-NS merger and powered by a magnetar central engine.",
          "type": "quotation"
        },
        {
          "ref": "2015 January, R Fernandez, D Kasen, BD Metzger, “The effect of black hole spin on winds from neutron star merger remnant accretion disks”, in American Astronomical Society, AAS Meeting #225",
          "text": "Disk winds generally contribute to a ~week long transient peaking in the near-infrared (kilonova), although an optical precursor can manifest as a signature of delayed black hole formation or high black hole spin.",
          "type": "quotation"
        },
        {
          "ref": "2015, R Fernández, D Kasen, “Outflows from accretion discs formed in neutron star mergers: effect of black hole spin”, in (Please provide the book title or journal name)",
          "text": "This component can give rise to an ≲1 d blue optical 'bump' in a kilonova light curve, even in the case of prompt BH formation, which may facilitate its detection.",
          "type": "quotation"
        }
      ],
      "glosses": [
        "A radiation pattern typical of a kilonova."
      ],
      "links": [
        [
          "physics",
          "physics"
        ],
        [
          "radiation",
          "radiation"
        ]
      ],
      "raw_glosses": [
        "(informal, physics) A radiation pattern typical of a kilonova."
      ],
      "tags": [
        "informal"
      ],
      "topics": [
        "natural-sciences",
        "physical-sciences",
        "physics"
      ]
    }
  ],
  "synonyms": [
    {
      "word": "KN"
    },
    {
      "word": "macronova"
    }
  ],
  "wikipedia": [
    "kilonova"
  ],
  "word": "kilonova"
}

This page is a part of the kaikki.org machine-readable All languages combined dictionary. This dictionary is based on structured data extracted on 2024-05-03 from the enwiktionary dump dated 2024-05-02 using wiktextract (f4fd8c9 and c9440ce). 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.

If you use this data in academic research, please cite Tatu Ylonen: Wiktextract: Wiktionary as Machine-Readable Structured Data, Proceedings of the 13th Conference on Language Resources and Evaluation (LREC), pp. 1317-1325, Marseille, 20-25 June 2022. Linking to the relevant page(s) under https://kaikki.org would also be greatly appreciated.