The sticky problem of Lunar Dust Get a mathematical solution

Apollo astronauts discovered unexpected enemy on the Moon.

Fine dust, start by their movements and attracted by static electricity coated everything.

It found its way through seals, scratched visors and clung to suits despite brushing.

Eugene Cernan described it one of most aggravating aspects of lunar operations.

Over five decades later humanity prepares to return to the Moon with sophisticated equipment solving the lunar dust problem has become critical.

Lunar Rover

Appolo

Researchers from the Beijing Institute of Technology, China Academy of Space Technology and Chinese Academy of Sciences have developed a detail theoretical model that explain how charged dust particles interact with spacecraft surfaces during low velocity collisions.

The challenge starts with Moon harsh environment.

On the dayside intense solar ultraviolet and X ray radiation strips electrons from both spacecraft and lunar surface leaving them positively charged.

This creates photoelectron sheath hovering above ground.

On the nightside spacecraft and regolith instead collect electrons from surrounding plasma becoming negative charged and forming what is called a Debye sheath.

The solar wind adds other layer of complexity continuously bathing in charged particles.

Within this electrically active environment dust particles themselves become charged and experience three distinct electrostatic forces as they approach a spacecraft.

Lunar Rover

Appolo

The electric field force acts on particle surface charge pulling it toward or pushing it away from vehicle depending on whether their charges areĀ  opposite or the same.

The dielectrophoretic forces arises because the dust particle distort the non uniform electric field around it creating attraction toward regions of stronger field regardless of particle charge.

The image force emerges when the approaching charged particle creates opposite charge in spacecraft conductive surface similar to how balloon sticks to wall creating additional attractive pull.

The researches model treats these electrostatic interactions in mathematical detail but recognizes that other forces dominate once contact starts.

When dust grain actually strikes a spacecraft coating adhesive van der Waals forces between molecules at surface become dominant for the slow velocity impacts common during lunar operations.

The collision itself unfolds in three stages. First comes adhesive elastic loading, where the particle compresses against the coating while attractive forces between surfaces grow.

Lunar Rover

Appolo

If impact is energetic enough the coating starts to deform, dissipating energy as material yields.

During unloading stage the particle either bounces away or remains stuck depending on whether the collision velocity falls within critical range.

The model announces several practical.

A dielectric coating with high thickness and low permittivity can reduce the electrostatic attraction between charged dust and spacecraft.

The particle surface charge density matter over spacecraft electrical potential in determining strength of electrostatic forces.

For particles carrying typical charge densities below o.1 milliColumbs per square meter.

The adhesive Van der Waals force overwhelms electrostatic effects during actual contact.

Most useful for mission planners the research shows that coating made from low surface energy material with rough textures can reduce dust adhesion.

Larger particles tend to have higher coefficients of restitution meaning they are more likely to bounce away rather than stick.

There exist a critical velocity range for negative charge particles where adhesion occurs. impacts slower or faster than this window permit particles to escape.

This latest mode can predict dust accumulation pattern guide selection of surface coating and help optimize dust removal systems.

Mission to moon grow more ambitious and long duration solving sticky problem of lunar dust moves from annoyance to operational necessity.

Lunar Rover

Appolo

Source

https://www.eurekalert.org/news-releases/1110112

https://www.universetoday.com/articles/the-sticky-problem-of-lunar-dust-gets-a-mathematical-solution

The ALMA Array is completed with 145 New Low Noise Amplifiers

For decades scientists have observed the cosmos with radio antennas to visualize the dark distant regions of the Universe.

This consist of the gas and dust of the interstellar medium ISM planet forming disks and objects that cannot be observed in visible light.

In this field the Atacama Large Millimeter/Submillimeter Array ALMA in Chile stands out as one of world powerful radio telescopes.

Using its 66 parabolic antennas, ALMA observes the millimeter and submillimeter radiation emitted byĀ  cold molecular clouds from which new stars are born.

Each antenna is equipped with high frequency receivers for ten wavelength ranges 35-50 GHZ and 787-950 GHZ known as Band 1.

The ALMA Array is completed with 145 New Low Noise Amplifiers

Thanks to Fraunhofer Institute for Applied Solid State Physics IAF and the Max Planck Institute for Radio Astronomy MPIFR, ALMA has received upgrade with addition of 145 new low noise amplifiers LNAs.

These amplifiers are part of facilities Band 2 coverage ranging from 67 to 116 GHz on the electromagnetic spectrum.

This coverage will allow researchers to study and gain better understanding of Universe.

They hope to gain new insights into cold interstellar medium the dust, gas radiation and magnetic fields from which stars are born.

Scientist will be able to study planet forming disk in better detail.

But certainly not least they will be able to study complex organic molecules COM in nearby galaxies which considered precursors to building blocks of life DNA, RNA.

These studies will allow astronomers and cosmologists to witness how stars and planetary systems form and evolve and how presence of organic molecules can lead to emergence of life.

Each LNA consist of a series of monolithic microwave integrated circuits MMICs developed by Frauhofer IAF using the semiconducting material indium gallium arsenide INGAAS.

The ALMA Array is completed with 145 New Low Noise Amplifiers

MMICs are based on metamorphic high electron mobility transistor mHEMT technologt a method for creating advance transistors that are flexible and allow for performance in high frequency receivers.

The addition of LNAs equipped with these circuits will amplify low noise signals and minimize background noisce increasing the sensitivity of ALMAs receivers.

Frauhofer IAF and MPIFR were commissioned by the European Southern Observatory ESO to provide amplifiers.

Frauhofer IAF was responsible for designing, testing and manufacturing the MMICs at room temperature, MPIFR was task with assembling and qualifying the LNA modules, then testing them in cryogenic conditions.

This is wonderful recognition of our fantastic collaboration with Fraunhofer IAF which shows that amplifiers are not only made in Germany but best in world said Prof Dr. Michael Kramer executive director at MPIFR.

Dr Fabian Thome head of subproject at Frauhofer IAF explained in IAF press release.

The performance of receivers depend on the performance of the first high frequency amplifiers installed in them.

Our technology is characterized by an average noise temperature of 22 K which is unmatched worldwide.

The ALMA Array is completed with 145 New Low Noise Amplifiers

New LNA signals can be amplified more than 300 fold in first step.

This enables the ALMA receivers to measure millimeter and submillimeter radiation from depths of universe much more precisely and obtain better data.

We are proud that our LNA technology is helping us to better understand the origin of stars and entire galaxies.

James Webb Telescope spies a monstrous molecular cloud shrouded in mystery Space Image of the Week

In this James Webb telescope photo the mega molecular cloud near our galaxy center appears as canvas of pink and purple clouds set against shadow backdrop.

Telescope

James Web Telescope

Stars shape in molecular clouds molecular clouds regions that are cold, dense, rich in molecules and filled with dust.

One huge cloud responsible for forming half of stars in Milky Way central region is Sagittarius B2 molecular cloud located in few hundred light years from our central supermassive black hole.

Boasting a mega mass between 3 million and 10 millions time that of sun and stretching 150 light year across.

It is one mega molecular clouds in galaxy.

It lies almost 26000 light years from Earth in constellation Sagittarius.

It is chemically rich.

Several complex molecules discovered.

Telescope

James Web Telescope

Telescope

James Web Telescope