Improving science (communication) through data visualizationZachary Labe
Creating visuals of data is an important part of our jobs as scientists. We use figures for journal publications, presentations, posters, lab group meetings, science communication, and more. In this workshop, we'll use examples from climate science to discuss a framework and network of resources available for making accessible figures. I will also share examples of what not to do and how to improve these figures moving forward.
Improving scientific graphics of climate (change) dataZachary Labe
Creating visuals of data is a critical part of our jobs as scientists. We use figures for journal publications, presentations, posters, and science communication. This week we'll discuss a framework for making better figures, particularly in the climate sciences. I will also give examples of what not to do, and how we can improve these figures moving forward. e
Improving science (communication) through data visualizationZachary Labe
Creating visuals of data is an important part of our jobs as scientists. We use figures for journal publications, presentations, posters, lab group meetings, science communication, and more. In this workshop, we'll use examples from climate science to discuss a framework and network of resources available for making accessible figures. I will also share examples of what not to do and how to improve these figures moving forward.
Improving scientific graphics of climate (change) dataZachary Labe
Creating visuals of data is a critical part of our jobs as scientists. We use figures for journal publications, presentations, posters, and science communication. This week we'll discuss a framework for making better figures, particularly in the climate sciences. I will also give examples of what not to do, and how we can improve these figures moving forward. e
Flash presentation given by John Connolly, Dublin City University, at the 2015 Horizon 2020 SC5 Information Day, 21/10/2015, Herbert Park Hotel, Dublin
Flash presentation given by John Connolly, Dublin City University, at the 2015 Horizon 2020 SC5 Information Day, 21/10/2015, Herbert Park Hotel, Dublin
Kinetic Energy Transfer of Near-Earth Objects for Interplanetary Manned Missi...Winston Sanks
This report outlines the rationale, procedures, technical feasibility, risk assessment, and cost-benefit analysis of utilizing a Near-Earth Object, 101955 Bennu (provisional designation 1999 RQ36 - the target of the OSIRIS-REx mission), as a source of energy to minimize the propulsion requirements of an interplanetary spacecraft. The planet Mars is the target body in this study and the outbound Trans-Mars injection in the years between 2175 and 2199 will be analyzed (within this timeframe Bennu’s orbit is predicted to approach Earth within two Earth radii on at least 80 occasions). The Mars orbit insertion burn, Trans-Earth injection burn, and Earth orbit insertion burn are assumed to be achieved with propulsive maneuvers outlined in standard manned interplanetary mission architectures. To accomplish this mission, two methods of transferring kinetic energy are examined: direct capture and release of the asteroid by a spacecraft using a Kevlar net and an inertial reel, and indirect capture by establishing a station on the asteroid to manufacture compressed material from the carbonaceous regolith in order to fire a mass stream to be captured by the spacecraft. This mission architecture analysis takes into account the associated safety risks of perturbations within Bennu’s orbit (which could result in inaccurate rendezvous location predictions), the implications of altering the orbit of 101955 Bennu after transferring a portion of its energy (since there is a possibility of collision with Earth in the late 22nd century if the asteroid is slowed too significantly), g-limit restrictions of the spacecraft and its occupants during an acceleration by the asteroid, and the possibility of a collision between Bennu and the spacecraft. In addition, the cost-benefit considerations of this mission architecture are weighed. This examination concludes that a direct capture Net and Reel system aboard the spacecraft is not a viable capture method due to an insufficient maximum ΔV available through a best-case perfectly elastic collision (capture) with the asteroid, as well as a prohibitive weight penalty aboard the spacecraft due to the Net and Reel system. However, this report finds that the method of establishing a station on Bennu with the capability to separate mass from the asteroid and fire it at a spacecraft is a plausible (if costly) means of transferring a significant ΔV. A KETNEO-FIMM Asteroid Station mission architecture could also be used in subsequent interplanetary missions providing cost-sharing over many decades for future interplanetary missions.
Detectability of Solar Panels as a TechnosignatureSérgio Sacani
In this work, we assess the potential detectability of solar panels made of silicon on an Earth-like
exoplanet as a potential technosignature. Silicon-based photovoltaic cells have high reflectance in the
UV-VIS and in the near-IR, within the wavelength range of a space-based flagship mission concept
like the Habitable Worlds Observatory (HWO). Assuming that only solar energy is used to provide
the 2022 human energy needs with a land cover of ∼ 2.4%, and projecting the future energy demand
assuming various growth-rate scenarios, we assess the detectability with an 8 m HWO-like telescope.
Assuming the most favorable viewing orientation, and focusing on the strong absorption edge in the
ultraviolet-to-visible (0.34 − 0.52 µm), we find that several 100s of hours of observation time is needed
to reach a SNR of 5 for an Earth-like planet around a Sun-like star at 10pc, even with a solar panel
coverage of ∼ 23% land coverage of a future Earth. We discuss the necessity of concepts like Kardeshev
Type I/II civilizations and Dyson spheres, which would aim to harness vast amounts of energy. Even
with much larger populations than today, the total energy use of human civilization would be orders of
magnitude below the threshold for causing direct thermal heating or reaching the scale of a Kardashev
Type I civilization. Any extraterrrestrial civilization that likewise achieves sustainable population
levels may also find a limit on its need to expand, which suggests that a galaxy-spanning civilization
as imagined in the Fermi paradox may not exist.
Reference Guide To The International Space StationSérgio Sacani
The International Space Station is a unique place – a convergence of science, technology and human innovation that demonstrates new technologies and makes research breakthroughs not possible on Earth.
It is a microgravity laboratory in which an international crew of six people live and work while traveling at a speed of five miles per second, orbiting Earth every 90 minutes.
The space station has been continuously occupied since November 2000. In that time, more than 200 people from 15 countries have visited.
Crew members spend about 35 hours each week conducting research in many disciplines to advance scientific knowledge in Earth, space, physical, and biological sciences for the benefit of people living on our home planet.
The station facilitates the growth of a robust commercial market in low-Earth orbit, operating as a national laboratory for scientific research and facilitating the development of U.S. commercial cargo and commercial crew space transportation capabilities.
More than an acre of solar arrays provide power to the station, and also make it the next brightest object in the night sky after the moon. You don’t even need a telescope to see it zoom over your house. And we’ll even send you a text message or email alert to let you know when (and where) to look up, spot the station, and wave!
This was a talk I gave at CU Boulder SEDs in Nov 2011 to showcase the variety and opportunities for student-run science and engineering experiments on suborbital platforms. The area of suborbital space is rapidly expanding and is set to change how we expand our use of technology for future science and exploration space missions.
Most Viewed Article (Current Issue) in Academia - International Journal on S...ijsc
Soft computing is likely to play an important role in science and engineering in the future. The successful applications of soft computing and the rapid growth suggest that the impact of soft computing will be felt increasingly in coming years. Soft Computing encourages the integration of soft computing techniques and tools into both everyday and advanced applications. This Open access peer-reviewed journal serves as a platform that fosters new applications for all scientists and engineers engaged in research and development in this fast growing field.
SpaceX’s 22nd contracted cargo resupply mission (CRS) to the International Space
Station for NASA will deliver more than 7,300 pounds of science and research, crew
supplies and vehicle hardware to the orbital laboratory and its crew.
Launch is targeted for 1:29 p.m. EDT Thursday, June 3, 2021
1. Laser Astronaut Retrieval Propellant Development
Tyler Baxter1, John E. Sinko1,2, Clifford Schlecht2, and Mark Gill3
¹ Dept. of Physics and Astronomy, Saint Cloud State University, St. Cloud, MN 56301
² Institute for Materials, Energetics and Complexity, St. Cloud, MN 56301
³ ISELF 3D Printing Coordinator, Saint Cloud State University, St. Cloud, MN 56301
MOTIVATION
The development of the aerospace industry has recognized
the need for a method of retrieving both assets and humans
in the vacuum environment. This experimental process
explores and refines the idea of using lasers to create a
‘tractor beam’ retrieval effect by controlled laser ablation
using low-cost, low-risk propellant alternatives.
EXPERIMENTAL PROCEDURE
To demonstrate quantitative propellant thrust, an improvised 3D-
printed ablatant chamber casing was housed directly atop a force
sensor capable of measuring a thrust response. All components
were sealed under a vacuum chamber in which we plan to simulate
low-Earth orbit vacuum conditions.
Acknowledgements
This project was funded by the authors and by Saint Cloud
State University. The authors would also like to express thanks
to Dr. Michael Dvorak and Dr. Michael Jeannot of the Saint
Cloud State Chemistry Department for their input.
1. Target Irradiation
Targets were exposed to 30-
seconds of 3 watts continuous
laser output at a wavelength
of 514.5 nm.
2. Target Ablation
Following direct exposure,
ablatant targets offgas
residual chemical products
that fill the volume of the
ablation chamber.
3. Coordinated
Confinement
Residual byproducts of the
ablation process are directed
out of the casing through a
1mm diameter steel tubule to
be redirected for use
elsewhere as needed.
Figure 1. Ablation casing diagram.
References
1. National Aeronautics and Space Administration, NASA Strategic
Plan 2014, pp. 3, 11.
2. S. Yokoyama, H. Horisawa, I. Funaki, and H. Kuninaka,
“Fundamental Study of Laser Micro Propulsion Using Powdered-
Propellant” in International Electric Propulsion Conference, IEPC-
2007-230, pp. 1-7 (2007).
3. C. R. Phipps, J. R. Luke, G. G. McDuff, T. Lippert, “Laser-driven
micro-rocket”, Appl. Phys. A 77, pp. 193-201 (2003).
4. M. S. Egorov, Yu. A. Rezunkov, E. V. Repina, and A. L. Safronov,
“Laser corrective propulsion plant for spacecraft”, J. Opt. Technol.
77(3), pp. 159-164 (March 2010).
5. 9. J. T. Kare, “Laser Powered Heat Exchanger Rocket for Ground-to-
Orbit Launch”, J. Propulsion and Power, 11(3), pp. 535-543 (1995).
Figure 2. Ablation of propellant.
Figure 3. Dispersion of byproducts into
casing microtubule.
RESULTS
Using a carbon nanofoam propellant:
Figure 4. Experimental ‘tractor beam’ thrust response for carbon sample.
Figure 5. Magnification (80x) of carbon
foam propellant sample.
Figure 6. Carbon foam propellant casing.
Using a thin film ammonium carbonate propellant:
Figure 7. Size representation of the ammonium carbonate ablation casing.
Figure 8. Magnification (2.5x) of ammonium
carbonate crystals.
Figure 9. Live ablation of ammonium
carbonate target in vacuum.
ANALYSIS AND FUTURE WORK
Although the experiment was successful, several
further methods of refinement are possible. Future
work will include design of an ablation casing with a re-
sealable gasket to allow for swift comparison of other
carbonate-related compounds and minimal loss of
desired offgassed products.
Figure 10. Carbon ablation target irradiated by 514.5nm photons.