Do all Sun-like stars have planets? Inferences from the disc mass reservoirs of Class 0 protostars

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Protoplanetary Discs, Circumstellar Matter

Scientific paper

Protostars ˜0.1 Myr old are heavily obscured, but their circumstellar dust discs can be studied by millimetre interferometry that resolves out the obscuring envelope. Consistent estimates are made for the disc masses of Class 0 protostars, and these range over 7-660 MJup. A simple grain coagulation model reproduces the mass distributions of more evolved discs around Class I protostars and Class II T Tauri stars (at ≲1, ≲5 Myr), implying that their observed dust is remnant material. The conversion of most dust grains into planetesimals thus occurs very early, at ˜0.1 Myr. As this is concurrent with the formation of the star itself, much of the disc is expected to accrete on to the central object, and a correlation of bolometric luminosity and disc mass is observed that agrees well with disc models. The observed Class 0 discs all contain upwards of 20 M? of dust, allowing for the formation of ‘super-Earths’ around many Sun-like stars. Only 10 per cent of the dust mass needs to be converted into planetary cores to match the range of such core masses presently known.

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

Do all Sun-like stars have planets? Inferences from the disc mass reservoirs of Class 0 protostars 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 Do all Sun-like stars have planets? Inferences from the disc mass reservoirs of Class 0 protostars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Do all Sun-like stars have planets? Inferences from the disc mass reservoirs of Class 0 protostars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1398604

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