Followup Observations of Newly Identified Debris Disks Associated with Solar-Mass Stars

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We propose to obtain new 70 and 160 micron observations for a carefully selected sub-sample of debris systems around solar-mass stars from the Formation and Evolution of Planetary Systems (FEPS) Spitzer Legacy Science Program. The new data, complemented by planned millimeter observations from the ground will constrain: 1) the outer radii of disks detected as part of FEPS; and 2) the amount of cold dust in these regions. Our proposed 70 and 160 micron observations are crucial in order to compare dust from 30 - 100 AU in newly identified debris disk systems with evolutionary models of our own Kuiper Belt. Our ultimate goal, then, is to use these results to assess whether solar systems like our own are common or rare among sun-like stars in the disk of the Milky Way. Our enhanced spectral energy distributions, and the subsequent well constrained accompanying debris disk models, will further the FEPS science legacy by serving as templates for, and be complementary with, existing Spitzer data sets that have been acquired by other GTO and GO surveys of sun-like stars.

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

Followup Observations of Newly Identified Debris Disks Associated with Solar-Mass Stars 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 Followup Observations of Newly Identified Debris Disks Associated with Solar-Mass Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Followup Observations of Newly Identified Debris Disks Associated with Solar-Mass Stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1167352

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