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    "story_id": "mp-2026-09-20-027",
    "source_story_id": "tmp-story-sn1983v-dust-front-rail",
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    "headline": "A 1983 Supernova Still Glowed Through Dust",
    "slug": "a-1983-supernova-still-glowed-through-dust",
    "dek": "JWST found a likely dusty remnant with about 0.0077 solar masses of dust more than four decades later.",
    "summary": "JWST found a likely dusty remnant with about 0.0077 solar masses of dust more than four decades later.",
    "body_text": "Serendipitous JWST infrared images contain a point source at the position of Type Ic supernova SN 1983V more than 40 years after the explosion. The source differs from nearby ionized regions, and archival Hubble data show a plausible hydrogen-alpha counterpart consistent with continuing shock interaction heating the dust. Modeling favors a torus and about 0.0077 solar masses of dust, which could reflect binary-linked mass loss. Spectroscopy is still needed to confirm that the source is the supernova remnant rather than an interloper.",
    "why_it_matters": "JWST found a likely dusty remnant with about 0.0077 solar masses of dust more than four decades later.",
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    "importance": 8,
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    "first_published_at": "2026-09-20T09:00:00.000-04:00",
    "modified_at": "2026-09-20T09:00:00.000-04:00",
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        "text": "JWST found a likely dusty remnant with about 0.0077 solar masses of dust more than four decades later.",
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    "source_ids": [
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    "tags": [
      "SN 1983V",
      "JWST",
      "cosmic dust"
    ],
    "image_url": null,
    "corrections": []
  },
  "sources": [
    {
      "source_id": "source-2026-09-20-016",
      "title": "arXiv preprint 2609.19263",
      "publisher": "arXiv",
      "url": "https://arxiv.org/abs/2609.19263",
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      "published_at": "2026-09-16T14:00:01.000-04:00",
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    "name": "The Machine Press",
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    "description": "A daily newspaper for the age of artificial intelligence."
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    "title": "A 1983 Supernova Still Glowed Through Dust",
    "publisher": "The Machine Press",
    "published_at": "2026-09-20T09:00:00.000-04:00",
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