"peribothron" meaning in All languages combined

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        "4": "",
        "5": "near"
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      "expansion": "Ancient Greek περί (perí, “near”)",
      "name": "uder"
    }
  ],
  "etymology_text": "Ancient Greek περί (perí, “near”) + βόθρος (bóthros, “pit”)",
  "forms": [
    {
      "form": "peribothra",
      "tags": [
        "plural"
      ]
    }
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      "expansion": "peribothron (plural peribothra)",
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  "lang": "English",
  "lang_code": "en",
  "pos": "noun",
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          "langcode": "en",
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          "name": "Black holes",
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      "examples": [
        {
          "ref": "2003 August, A Gould& AC Quillen, “Sagittarius A* companion S0-2: a probe of very high mass star formation”, in The Astrophysical Journal, volume 592, number 2",
          "text": "We also examine the final peribothra q of these orbits to ensure that they are consistent with the observed value for S0-2.",
          "type": "quotation"
        },
        {
          "ref": "2006 July, LM Dray, AR King, MB Davies, “Young stars in the Galactic Centre: a potential intermediate-mass star origin”, in Monthly Notices of the Royal Astronomical Society, volume 372, number 1",
          "text": "On subsequent peribothra further tidal interactions take place, gradually causing the orbit to decay.",
          "type": "quotation"
        },
        {
          "ref": "2011, C Wegg, JN Bode, “Multiple tidal disruptions as an indicator of binary supermassive black hole systems”, in The Astrophysical Journal Letters",
          "text": "Galaxies harboring an isolated SMBH at their center are expected to quickly clear a \"loss cone\" of orbits whose angular momenta about the black hole are low enough that their peribothra lie inside rₜ .",
          "type": "quotation"
        }
      ],
      "glosses": [
        "The point in an elliptical orbit around a black hole where the orbiting body is closest to the black hole."
      ],
      "id": "en-peribothron-en-noun-F6FmkbvB",
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          "astronomy",
          "astronomy"
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          "elliptical"
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        ],
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      "raw_glosses": [
        "(astronomy) The point in an elliptical orbit around a black hole where the orbiting body is closest to the black hole."
      ],
      "related": [
        {
          "word": "periapsis"
        }
      ],
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  "word": "peribothron"
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      "name": "uder"
    }
  ],
  "etymology_text": "Ancient Greek περί (perí, “near”) + βόθρος (bóthros, “pit”)",
  "forms": [
    {
      "form": "peribothra",
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  "pos": "noun",
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          "ref": "2003 August, A Gould& AC Quillen, “Sagittarius A* companion S0-2: a probe of very high mass star formation”, in The Astrophysical Journal, volume 592, number 2",
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        },
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          "ref": "2006 July, LM Dray, AR King, MB Davies, “Young stars in the Galactic Centre: a potential intermediate-mass star origin”, in Monthly Notices of the Royal Astronomical Society, volume 372, number 1",
          "text": "On subsequent peribothra further tidal interactions take place, gradually causing the orbit to decay.",
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          "ref": "2011, C Wegg, JN Bode, “Multiple tidal disruptions as an indicator of binary supermassive black hole systems”, in The Astrophysical Journal Letters",
          "text": "Galaxies harboring an isolated SMBH at their center are expected to quickly clear a \"loss cone\" of orbits whose angular momenta about the black hole are low enough that their peribothra lie inside rₜ .",
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      ],
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      ],
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        "(astronomy) The point in an elliptical orbit around a black hole where the orbiting body is closest to the black hole."
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  "word": "peribothron"
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