Javascript must be enabled to continue!
The Production of Dust-Ice-Pebbles
View through CrossRef
<p>In the CoPhyLab at the TU Braunschweig, the goal is to simulate the physical behaviour of comets on Earth. Therefore, we are currently producing pebbles from silicate dust and water ice in order to subsequently investigate their properties and behaviour in various experiments. The pebbles we are producing consist of a mixture of water ice and dust, but also of pure water ice.</p>
<p><img src="" alt="" /></p>
<p><em>Figure 1: Sieved pebbles with diameters of 1mm to 1.6mm consisting of a mixture of dust and water ice with a ratio 3:1.</em></p>
<p>The materials are mixed and then shaken while low temperatures are secured. For a homogenous mixture some nitrogen is added during the mixing procedure. In order to be able to form the largest possible number of pebbles from a mixture, it is necessary to understand the process of pebble formation. Therefore, we have studied the formation behaviour of pebbles from mixtures with different mixing ratios and by using different shaking techniques. Recent experiments have shown that mixtures with different weight ratios of dust-to-water ice can form pebbles. Also, adding a certain amount of graphite to darken the mixture has no effect on the formation process.</p>
<p>To study and to quantify the properties of the pebbles, such as compressive strength and thawing behaviour, it is important to know the particle size distribution. For this purpose, the pebbles must be sieved. This has been successfully carried out at the TU Braunschweig. With the samples obtained in this way, it has already been possible to gain initial insights into, among other things, the thawing behaviour and porosity of the pebbles. It was found, for example, that pebbles with an higher dust content retain their structure and a baking effect occurs, which leads to a hardening of the material, whereas pebbles with a low dust content collapse.</p>
<p>During this conference we will present our pebble making technique and our findings about the formation of pebbles. Further, we want to introduce the audience to our shaking machine. The latest results about the thawing behaviour as well as other properties of the pebbles will be presented, too.&#160;</p>
Title: The Production of Dust-Ice-Pebbles
Description:
<p>In the CoPhyLab at the TU Braunschweig, the goal is to simulate the physical behaviour of comets on Earth.
Therefore, we are currently producing pebbles from silicate dust and water ice in order to subsequently investigate their properties and behaviour in various experiments.
The pebbles we are producing consist of a mixture of water ice and dust, but also of pure water ice.
</p>
<p><img src="" alt="" /></p>
<p><em>Figure 1: Sieved pebbles with diameters of 1mm to 1.
6mm consisting of a mixture of dust and water ice with a ratio 3:1.
</em></p>
<p>The materials are mixed and then shaken while low temperatures are secured.
For a homogenous mixture some nitrogen is added during the mixing procedure.
In order to be able to form the largest possible number of pebbles from a mixture, it is necessary to understand the process of pebble formation.
Therefore, we have studied the formation behaviour of pebbles from mixtures with different mixing ratios and by using different shaking techniques.
Recent experiments have shown that mixtures with different weight ratios of dust-to-water ice can form pebbles.
Also, adding a certain amount of graphite to darken the mixture has no effect on the formation process.
</p>
<p>To study and to quantify the properties of the pebbles, such as compressive strength and thawing behaviour, it is important to know the particle size distribution.
For this purpose, the pebbles must be sieved.
This has been successfully carried out at the TU Braunschweig.
With the samples obtained in this way, it has already been possible to gain initial insights into, among other things, the thawing behaviour and porosity of the pebbles.
It was found, for example, that pebbles with an higher dust content retain their structure and a baking effect occurs, which leads to a hardening of the material, whereas pebbles with a low dust content collapse.
</p>
<p>During this conference we will present our pebble making technique and our findings about the formation of pebbles.
Further, we want to introduce the audience to our shaking machine.
The latest results about the thawing behaviour as well as other properties of the pebbles will be presented, too.
&#160;</p>.
Related Results
Protoplanetary discs in the laboratory: the fate of icy pebbles undergoing sublimation
Protoplanetary discs in the laboratory: the fate of icy pebbles undergoing sublimation
Planet formation in protoplanetary discs is a process whereby the primitive solids that are initially of microscopic scale, must be converted into larger objects such as pebbles (m...
Linear polarization as a tool to characterize interplanetary, cometary, and extrasolar dust particles
Linear polarization as a tool to characterize interplanetary, cometary, and extrasolar dust particles
SummaryLinear polarization observations have suggested the presence of dust particles that scatter solar light within cometary comae and the interplanetary dust cloud. Recent progr...
Effect of ocean heat flux on Titan's topography and tectonic stresses
Effect of ocean heat flux on Titan's topography and tectonic stresses
INTRODUCTIONThe thermo-mechanical evolution of Titan's ice shell is primarily controlled by the mode of the heat transfer in the ice shell and the amount of heat coming from the oc...
Dust deposition and lifting at the Zhurong landing site
Dust deposition and lifting at the Zhurong landing site
IntroductionDust deposition poses the challenges to the survival of instruments and solar-powered missions on Mars [1, 2]. Zhurong in-situ observations provide an opportunity to st...
Viscous relaxation of Pluto's ice shell below Sputnik Planitia
Viscous relaxation of Pluto's ice shell below Sputnik Planitia
AbstractThe surface of Pluto is dominated by the Sputnik Planitia basin, possibly caused by an impact ~ 4 Gyr ago. To explain basin's unlikely position close to tidal axis with Cha...
Wind tunnel experimentation of ice particles transport in Martian-like environment
Wind tunnel experimentation of ice particles transport in Martian-like environment
Introduction:  The transport of ice by wind plays a major role in the surface mass balance of polar caps [1, 2]. Ice can be redistributed by wind due to (1) transport of i...
Grain growth of polycrystalline ice doped with soluble impurities
Grain growth of polycrystalline ice doped with soluble impurities
The grain size of polycrystalline ice affects key parameters related to planetary evolution such as the rheological and dielectric properties of Earth's glaciers and ice sheets as ...
Eccentricity variations trigger “subduction” in Europa’s ice shell
Eccentricity variations trigger “subduction” in Europa’s ice shell
IntroductionIcy moon Europa possesses one of the youngest surfaces in the Solar System. Overall smooth, yet rich in unique tectonic features, it records mostly extensional processe...

