Hillier, J.K.; Green, S.F.; McBride, N.; Altobelli, N.; Kempf, S.; Postberg, F.; Schwanethal, J.; Srama, R.; McDonnell, J.A.M. and Gruen, E.
This is the latest version of this eprint.
|DOI (Digital Object Identifier) Link:||http://doi.org/10.1016/j.icarus.2007.03.024|
|Google Scholar:||Look up in Google Scholar|
During its cruise phase, prior to encountering Jupiter, the Cosmic Dust Analyser (CDA) onboard the Cassini spacecraft returned time of flight mass spectra (TOF MS) of two interplanetary dust particles. Both particles were found to be iron-rich, with possible traces of hydrogen, carbon, nickel, chromium, manganese, titanium, vanadium and minor silicates. Carbon, hydrogen, oxygen and potassium are also present as possible contaminants of the impact target of CDA. Silicates and magnesium do not feature predominantly in the spectra; this is surprising considering the expected dominance of silicate-rich minerals in interplanetary dust particles. The particle masses are and . The corresponding radii ranges for the particles, assuming densities from 7874–2500 kg m−3 are 0.7–4 μm and 2.6–6.8 μm, respectively. With the same density assumptions the β values (ratio of radiation pressure to gravitational force) are estimated as 0.027–0.21 and 0.016–0.06 respectively, allowing possible orbits to be calculated. The resulting orbits are bound and prograde with semi-major axes, eccentricities and inclinations in the region of 0.3–1.26 AU, 0.4–1.0 and 0–60° for the first particle and 0.8–2.5 AU, 0.2–0.9 and 0–30° for the second. The more probable orbits within these ranges indicate that the first particle is in an Aten-like orbit, whilst the second particle is in an Apollo-like orbit, despite both grains having very similar, predominantly metallic compositions. Other possible orbital solutions for both particles encompass orbits which more closely resemble those of Jupiter-family comets.
|Item Type:||Journal Article|
|Extra Information:||Refer to DOI for precise representation of formulae in abstract.|
|Academic Unit/Department:||Science > Physical Sciences
Science > Environment, Earth and Ecosystems
Other Departments > Other Departments
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Simon Green|
|Date Deposited:||30 Nov 2007|
|Last Modified:||14 Jan 2016 16:49|
|Share this page:|
Available Versions of this Item
The composition of Saturn's E-ring. (deposited 05 Feb 2008)
- Interplanetary dust detected by the Cassini CDA Chemical Analyser. (deposited 30 Nov 2007) [Currently Displayed]