{
  "annotation_id": "2594e9dc-7ae4-48d5-9b56-c2637af1b322",
  "date_created": "2026-03-02T18:01:17.178000Z",
  "date_modified": "2026-03-02T18:01:17.178000Z",
  "file_hash": "0edc62e015459c79349f245d088d5efc32c9ef0be99de37b2c12f4766debdc8c",
  "private": false,
  "record": {
    "abstract": "The Solar sail is a large thin film used to collect solar light pressure for\nmoving of space apparatus. Unfortunately, the solar radiation pressure is very\nsmall about 9 mkN/sq.m at Earth\u0027s orbit. However, the light force significantly\nincreases up to 0.2 - 0.35 N/sq.m near the Sun. The author offers his research\non a new revolutionary highly reflective solar sail which flyby (after special\nmaneuver) near Sun and attains velocity up to 400 km/sec and reaching far\nplanets of the Solar system in short time or enable flights out of Solar\nsystem. New, highly reflective sail-mirror allows avoiding the strong heating\nof the solar sail. It may be useful for probes close to the Sun and Mercury and\nVenus.\n  Key words: AB-solar sail, highly reflective solar sail, high speed\npropulsion.",
    "arxiv_id": "physics/0701073",
    "authors": [
      "A. Bolonkin"
    ],
    "categories": [
      "physics.gen-ph",
      "physics.space-ph"
    ],
    "title": "High Speed AB-Solar Sail",
    "url": "https://arxiv.org/abs/physics/0701073"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6e2f84ce-b6c8-4ea1-a753-d86704941cd5",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}