{
  "id": "astro-ph/0410717",
  "version": "v1",
  "published": "2004-10-28T22:07:51.000Z",
  "updated": "2004-10-28T22:07:51.000Z",
  "title": "Composition of the Solar Interior: Information from Isotope Ratios",
  "authors": [
    "O. Manuel",
    "Stig Friberg"
  ],
  "comment": "4 pages, includes 6 figures, 1 Table, 39 references, 2002 SOHO 12/ GONG + 2002 Conference on Local and Global Helioseismology: The Present and Future, Big Bear Lake, CA",
  "categories": [
    "astro-ph"
  ],
  "abstract": "Measurements are reviewed showing that the interior of the Sun, the inner planets, and ordinary meteorites consist mostly of the same elements: Iron, oxygen, nickel, silicon, magnesium, sulfur and calcium. These results do not support the standard solar model.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2004-10-28T22:07:51.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "solar interior",
      "isotope ratios",
      "composition",
      "information",
      "standard solar model"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 663155
    }
  }
}