The nature of micrometeorites

Clicks: 1
ID: 308140
1961
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This article has not been analysed, so there is no overall score — reader engagement is measured and shown alongside.
AI Quality Assessment
Not analyzed
Readership in this journal

Ranked #7,887 of 8,486 articles by views in american journal of science

Most read Least read

Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 8,486 in total.

Mint this article as an NFT
Not yet minted

Create a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.

5 SUSD one-off · no wallet required
Abstract
Meteorite showers are usually caused by the fragmentation of one large meteorite in its rapid course through our atmosphere, rather than by the invasion of a swarm of initially discrete particles. In the process of fracture many small particles, including microscopic dust particles, must get separated from the main mass. These small particles have the fusion crust and morphological properties of meteorites in general. They differ from cosmic dust that enters the atmosphere directly from interplanetary space in that the cosmic dust particles are practically unaltered by impact with our atmosphere.
Reference Key
openalex_W2006289307 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors E. L. Krinov
Journal american journal of science
Year 1961
DOI
10.2475/ajs.259.5.391
URL
Keywords Keywords not found

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

No comments yet. Be the first to comment on this article.