Jump to main content
US EPA
United States Environmental Protection Agency
Search
Search
Main menu
Environmental Topics
Laws & Regulations
About EPA
Health & Environmental Research Online (HERO)
Contact Us
Print
Feedback
Export to File
Search:
This record has one attached file:
Add More Files
Attach File(s):
Display Name for File*:
Save
Citation
Tags
HERO ID
2587400
Reference Type
Journal Article
Title
A POSSIBLE ICY KUIPER BELT AROUND HD 181327
Author(s)
Chen, CH; Fitzgerald, MP; Smith, PS
Year
2008
Is Peer Reviewed?
1
Journal
The Astrophysical Journal
ISSN:
0004-637X
EISSN:
1538-4357
Volume
689
Issue
1
Page Numbers
539-544
Web of Science Id
WOS:000262929000047
Abstract
We have obtained a Gemini South T-ReCS Qa-band (18.3 mu m) image and a Spitzer MIPS SED-mode observation of HD181327, an F5/F6 V member of the similar to 12 Myr old beta Pictoris moving group. We resolve the disk in thermal emission for the first time and find that the northern arm of the disk is 1.4 times brighter than the southern arm. In addition, we detect a broad peak in the combined Spitzer IRS and MIPS spectra at 60-75 mu m that may be produced by emission from crystalline water ice. We model the IRS and MIPS data using a size distribution of amorphous olivine and water ice grains (dn/da proportional to a(-2.25), with a(min) consistent with the minimum blowout size and a(max) = 20 mu m) located at a distance of 86.3 AU from the central star, as observed in previously published scattered-light images. Since the photodesorption lifetime for the icy particles is similar to 1400 yr, significantly less than the estimated similar to 12 Myr age of the system, we hypothesize that we have detected debris that may be steadily replenished by collisions among icy Kuiper Belt object-like parent bodies in a newly forming planetary system.
Keywords
circumstellar matter; planetary systems: formation; stars: individual (HD 181327)
Home
Learn about HERO
Using HERO
Search HERO
Projects in HERO
Risk Assessment
Transparency & Integrity