Formation of chondrules by drag heating in dust-enriched environments

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Chondrule, Contacts (Geology), Drag, Formations, Interplanetary Dust, Meteoroid Dust Clouds, Solar System, Astrophysics, Celestial Mechanics, Geophysics, Solar Corona

Scientific paper

The solar system which had a beginning, 4.6 billion years ago is discussed. The atoms that make up the solar system are much older than that, however: they were also part of the universe that existed before the solar system formed. The presence and location of the atoms of silicon, iron, calcium, that make up the Earth and other planets before there was a solar system is questioned. Astronomical it is shown that they existed in tiny dust grains which, along with molecules of gas, wandered about in the vast reaches of space between the stars of our galaxy. The solar system was formed when one particular cloud of interstellar dust and gas became dense enough to be gravitationally unstable: the gravitational pull that dust grains and gas molecules exerted on one another caused the cloud to collapse.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Formation of chondrules by drag heating in dust-enriched environments does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Formation of chondrules by drag heating in dust-enriched environments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of chondrules by drag heating in dust-enriched environments will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1755215

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.