Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Kernphysik     Collection: Interplanetary Dust Physics     Display Documents



  history
ID: 276612.0, MPI für Kernphysik / Interplanetary Dust Physics
A new look into the Helios dust experiment data: presence of interstellar dust inside the Earth's orbit
Authors:Altobelli, N.; Grün, Eberhard; Landgraf, M.
Language:English
Research Context:ISM: dust, extinction -- interplanetary medium -- meteors, meteoroids
Date of Publication (YYYY-MM-DD):2006-03-02
Title of Journal:Astronomy and Astrophysics
Journal Abbrev.:A&A
Volume:448
Issue / Number:1
Start Page:243
End Page:252
Copyright:© ESO 2006
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:An analysis of the Helios in situ dust data for interstellar dust (ISD) is presented in this work. Recent in situ dust measurements with impact ionization detectors on-board various spacecraft (Ulysses, Galileo, and Cassini) showed the deep penetration of an ISD stream into the Solar System. The Helios dust data provide a unique opportunity to monitor and study the ISD stream alteration at very close heliocentric distances. This work completes therefore the comprehensive picture of the ISD stream properties within the heliosphere. In particular, we show that gravitation focusing facilitates the detection of big ISD grains (micrometer-size), while radiation pressure prevents smaller grains from penetrating into the innermost regions of the Solar System. A flux value of about 2.6±0.3x10-6m-2 s-1 is derived for micrometer-size grains. A mean radiation pressure-to-gravitation ratio (so-called ratio) value of 0.4 is derived for the grains, assuming spheres of astronomical silicates to modelize the grains surface optical properties. From the ISD flux measured on the Helios trajectory, we infer a lower limit of 3±3 x 10-25 kg m-3 to the spatial mass density of micron-sized grains in the Local Interstellar Cloud (LIC). In addition, compositional clues for ISD grains are obtained from the data provided by the time-of-flight mass spectrometer subsystem of the Helios instrument. No clustering of single minerals is observed but rather a varying mixture of various minerals and carbonaceous compounds.
Free Keywords:ISM: dust, extinction -- interplanetary medium -- meteors, meteoroids
External Publication Status:published
Document Type:Article
Affiliations:MPI für Kernphysik/Independent Research Groups/Heidelberg Dust Research Group (R. Srama)
External Affiliations:HIGP, University of Hawaii, Honolulu, USA
ESA/ESOC, Germany
Identifiers:DOI:10.1051/0004-6361:20053909
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.