极地研究 ›› 1995, Vol. 6 ›› Issue (2-English): 1-17.

• 目次 •    下一篇

A study on cosmic dust particles in Antarctic ice, snow and non-Antarctic region and their origins

 Wang Daode and Dai Chengda   

  1. Guangzhou Institute of Geochemistry, Academia Sinica, Guangzhou 510640, China
  • 出版日期:1945-06-30 发布日期:1945-06-30
  • 通讯作者: Wang Daode
  • 基金资助:

    This project was supported by the State Antarctic Committee of China and Chinese Academy of Sciences.

A study on cosmic dust particles in Antarctic ice, snow and non-Antarctic region and their origins

 Wang Daode and Dai Chengda   

  1. Guangzhou Institute of Geochemistry, Academia Sinica, Guangzhou 510640, China
  • Online:1945-06-30 Published:1945-06-30
  • Contact: Wang Daode
  • Supported by:

    This project was supported by the State Antarctic Committee of China and Chinese Academy of Sciences.

摘要:

A large number of cosmic dust particles, micrometeorites and volcanic dust bands have been found and collected in Antarctic ice, snow and glacial sediments, especially in meteorite concentrated regions. Extraterrestrial spherules also have been discovered from the stratosphere and deep-sea sediments. On the basis of their distributive characteristics the cosmic dust particles are classified into interplanetary dust particles and interstellar dust particles. According to their origins cosmic dust particles can be divided into cometary origin particles, asteroidal origin particles, ablation particles from meteorites and interstellar origin particles. The criteria for identifying cosmic dust particles have been established and the origins of cosmic dust particles are also discussed in aegis paper.

关键词: Antarctica, cosmic dust particles, interplanetary dust particles, interstellar dust particles

Abstract:

A large number of cosmic dust particles, micrometeorites and volcanic dust bands have been found and collected in Antarctic ice, snow and glacial sediments, especially in meteorite concentrated regions. Extraterrestrial spherules also have been discovered from the stratosphere and deep-sea sediments. On the basis of their distributive characteristics the cosmic dust particles are classified into interplanetary dust particles and interstellar dust particles. According to their origins cosmic dust particles can be divided into cometary origin particles, asteroidal origin particles, ablation particles from meteorites and interstellar origin particles. The criteria for identifying cosmic dust particles have been established and the origins of cosmic dust particles are also discussed in aegis paper.

Key words: Antarctica, cosmic dust particles, interplanetary dust particles, interstellar dust particles