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Newsletter November 2024 | Menu of Newsletters

Single-molecule Microscopy Techniques and Negative-Stiffness Vibration Isolation Support DNA Superstructure Research at the University of Texas, Dallas

Imaging of samples using single-molecule microscopy is particularly challenged by Z-axis (vertical) noise, requiring a high-performance level of vibration isolation. Research into applications involving imaging and characterization of DNA and protein-DNA complexes, being performed at the University of Texas at Dallas, rely on atomic force microscopy supported by precision Negative-Stiffness vibration isolation.

DNA, or deoxyribonucleic acid, is the hereditary material in humans and almost all other organisms. Nearly every cell in a person's bodpersony has the same DNA, most of which is located in the cell nucleus. The DNA molecule is packaged into thread-like structures called chromosomes. Each chromosome is made up of DNA tightly coiled many times around proteins that support its structure. The information in DNA is stored as a code made up of four chemical bases: adenine, guanine, cytosine and thymine, which are present in pairs. Human DNA (i.e., the human genome) consists of about 3 billion DNA base pairs, and more than 99 percent of these base pairs are the same in all humans. The order, or sequence, of these DNA base pairs determines the information available for building and maintaining an organism.

DNA Superstructure Research at the University of Texas, Dallas
Research into the functions of DNA has had a significant impact on the fields of medicine, biotechnology, and the life sciences. One such group that has been conducting research into DNA is the Physical Genomics Laboratory in theDepartment of Bioengineering, University of Texas at Dallas. Under the direction of Dr. Stephen Levene, Professor of Bioengineering, research into the characterization of biological macromolecules of protein-DNA complexes (DNA superstructures) has been ongoing for a number of years. Levenes research on the flexibility and folding of DNA, mediated by protein-DNA interactions, has led to valuable insights into the physics and organizations of genomes, as well as gene regulation and genetic recombination. His work has been supported by the American Cancer Society, Department of Defense, National Institutes of Health, National Science Foundation and the Texas Higher Education Coordinating Board.

"I've been working on problems having to do with the interactions of proteins that organize DNA into tertiary structures that are biologically important, said Dr. Levene. We are interested in questions that have to do with DNA superstructures, higher-order structures that organize the human genome."

"It is not unusual in the genome of many organisms for genes to be regulated by sequences of DNA that are many thousands of base pairs away, continued Dr. Levene. In fact, chromosomes are probably organized into functional units where regulatory elements occupy the same domain and genes that they regulate. By regulatory elements, I mean sequences of DNA where proteins bind, and turn on or turn off the genes that are under the control of those sequences."

"So to that end, for most of my career I have been interested in what governs those interactions in physical terms, and more recently, how we can harness our understanding of those interactions to effect regulation of certain genes and to develop new strategies for diagnostics and therapeutics, added Dr. Levene." Dr. Levene's team performs experiments in both ensemble or bulk measurements (making measurements on huge numbers of molecules), as well as in living cells and on single molecules. Their group can thus infer the properties of these molecular species either indirectly or more directly visualize them using tools that resolve optical images of fluorescently labeled DNA molecules or visualize DNA structures by using atomic-force microscopy. There are advantages and disadvantages to both methodologies, so they pursue both of these scales simultaneously."


A unique aspect of Dr. Levene's research is that it combines its experimental research results with advanced computer models and other types of calculations to address very challenging physics issues.

"We study very complex problems - such as how DNA organizes under the constraints of environmental factors - requiring that we collect data on three-dimensional structure-dependent parameters," explained Dr. Levene. "For example, with coiling of DNA, which occurs spontaneously, called supercoiling - to interpret this, good theory is needed, which involves quite sophisticated physics, and requires using computer-simulation-based tools and or other computational-modeling approaches. Our group is probably regarded as one of the leading labs in terms of DNA tertiary structure. But this is largely because of a strong computational component through our research, which I think is unique."


Physical Genomics Laboratory's Leica Thunder fluorescence microscope system on Minus K MK26 vibration isolation workstation

Vibration problems & negative-stiffness isolation solutions article continued...




Salute to the James Webb Space Telescope - Monthly Image Share:
"Prelude to a Supernova"


Minus K's custom vibration isolators were used for the
Ground Testing of the James Webb Space Telescope


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Earlier Headlines:

- NASA’s Lunar Laser Communications to replace traditional radio communications in space

- Featured Product: The LC-4 Ultra Compact Low Frequency Vibration Isolator

- New Video About Minus K Shown on Bloomberg Television

- Announcing the 2025 Minus K Technology $25,000 Educational Giveaway
to U.S. Colleges and Universities deadline February 28, 2025 + Past Winners


- Vibe Check European Space Agency Micro-Vibration Platform

- NEW CT-10 Ultra-Thin Low-Height Tabletop Vibration Isolator at only 2.7" high

- NASA Previous Projects: Satellite/Aerospace ground testing:

- 30th Anniversary History Timeline

- 300 leading universities and private and government laboratories
in 52 countries use Minus K Technology


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The LC-4 Ultra Compact Low Frequency Vibration Isolator


Low Freq. Horiz LC-4
Dimensions:
4.75" W x 4.75" D x 7" H
(121mm W x 121mm D x 178mm H)


Ultra Low Freq. Horiz LC-4U
Dimensions:
4.75" W x 4.75" D x 8" H
(121mm W x 121mm D x 203mm H)


The LC-4 is an ultra compact, low-frequency negative-stiffness isolator. It comes in two configurations, our low horizontal frequency performance of 1.5 Hz or our ultra low horizontal frequency performance of 0.5 Hz. Both configurations offer our signature 0.5 Hz vertical natural frequency.

This low frequency vibration isolator is for weight loads from 15 to 130 lbs. and 1/2 Hz performance vertical and horizontal.

LC-4 isolators can be combined into multi isolator systems to support heavier payloads while taking up very little room themselves. The isolators are passive, manually-adjustable and require no air or electricity. More...
  • Vertical natural frequency of 1/2 Hz or less can be achieved over the entire load range.
  • Horizontal natural frequency is load dependent. 1 1/2 Hz (low horiz. freq.) or 1/2 Hz (ultra low horiz. freq.) or less natural frequencies can be achieved at or near the nominal load.
  • See performance for a typical transmissibility curve with 1/2 Hz natural frequency.

Pricing & specs for LC-4


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NASA’s Lunar Laser Communications Demonstration is a viable alternative to replace traditional radio communications in space.

Minus K's negative-stiffness vibration isolator enables
space laser communications


NASA’s Lunar Atmosphere and Dust Environment Explorer (LADEE), pronounced Laddie, was a robotic mission launched in 2013 that orbited the moon to gather detailed information about the structure and composition of the thin lunar atmosphere, and the first-ever Lunar Laser Communications Demonstration (LLCD). The LLCD used lasers, not radio waves, like other spacecraft that have flown beyond close-Earth orbit have used, to communicate with controllers on Earth allowing the spacecraft to communicate at broadband speeds with the ground.

 
The probe was approximately 7.7ft x 4.75ft x 4.75ft, weighing 383kg (844 lb). The probe took about 30 days to get to the moon. LADEE then went through a checkout period for another 30 days. After that, the probe conducted a 100-day science mission and was even able to extend its mission for an additional month..

Once LADEEs mission was completed, NASA intentionally impacted the probe into the far side of the moon, away from historically important sites like the Apollo landing zones.

Lunar Laser Communications Demonstration
The LLCD was a project undertaken by MIT Lincoln Laboratory, NASA's Goddard Space Flight Center, and the Jet Propulsion Laboratory. It was NASAs first attempt to demonstrate optical communications between a lunar orbiting spacecraft and Earth-based ground receivers.

All prior communications with spacecraft beyond close-Earth orbits required spacecraft to have small, low-mass, low-power radio transmitters and giant satellite dishes on Earth to receive their messages. LLCD was an alternative process to replace traditional radio communications with specialized lasers and laser detection units to send information between lunar orbit and three receiving stations in the U.S. and Spain.

LLCD demonstrated error-free communication from the moon, including during broad daylight and even when the moon was within 3° of the sun, as seen from Earth. LLCD also operated error-free when the moon was less than 5° above the horizon, as seen from the ground station, which showed that wind and atmospheric turbulence didnt significantly impact the system. LLCD was even able to communicate through thin cirrus clouds.

The 30-day test was a much more comprehensive check of its utility for all-purpose communication. Rather than simply downloading a pre-arranged file, NASA used the device for real communication with LADEE, and real collection of data. While all LADEEs science data went to the ground via radio frequency (RF) link, the data sent by the LLCD test was verified against the RF data, demonstrating the feasibility of laser communication uplink/downlink for future missions.

The LLCD used a pulsed laser beam to transmit data over the 239,000 miles from the moon to Earth at a record-breaking data-download speed of 622 Megabits per second (Mbps), versus 75Mbps. This download speed was more than 6x faster than the speed achieved by the best radio system ever flown to the moon and would normally take several days to download.

LLCD also demonstrated a 20Mbps uplink, which was used to loop back error-free high-definition video to and from the moon, important for future human exploration missions, and also provided simultaneous centimeter-class precision ranging to the spacecraft, which can be used to improve the gravity models of planetary bodies.

The testing looked at more than raw download speed, prioritizing signal reliability and accuracy, along with possible distance effects. LLCD worked well even at extremely oblique angles, when the satellite was near the Earth’s horizon and its signals were forced to move through the thickest portions of the atmosphere. The laser signal could be read without error even in broad daylight and through light clouds.

In addition to this lack of error, the LLCD was able to switch from one ground station to the next as the Earth turned, in a manner that NASA compared to how a mobile phone network operates, and the system did so without human intervention. The system could even lock on to the ground stations without using a radio signal.

The real breakthrough of the LLCD demonstration, however, was the spectacular success of its essentially flawless operations, allowing the system to return real, high-value science data from LADEEs instruments investigating the moons environment and showing the promise of laser communication for future missions.

The downside for the future is range. Simply boosting power to the laser to make it cohere better over a longer distance is a losing game. A more reasonable solution, and one NASA is working toward, is the Lunar Communications Relay Demonstration (LCRD). This would see NASA pepper space with laser-routers to read and re-transmit laser signals from a new transmitter. LCRD is aboard the U.S. Department of Defenses Space Test Program Satellite 6 (STPSat-6) launched December 2021.


Article continued...




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NASA Telescope Project

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Spacecraft Vibration Isolation On the Ground

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