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An international team of space researchers working with NASA’s Goddard Space Flight Center has found previously unknown organic molecules on Mars using a new experiment aboard the Curiosity rover. The results are published in the journal Nature Astronomy.

To date, NASA has sent nine orbiters and six rovers to Mars, in part to learn more about the possibility of extraterrestrial life. To that end, the planet has been photographed with various types of cameras. More recently, rovers have dug down into the Martian soil to collect samples for analysis. The goal of such work is to learn more about the chemicals in the soil on or near the surface, but more specifically, to see if it contains organic molecules. If so, they could be evidence of life or prior life on the planet. The rovers have found organic molecules, but samples were not sufficient to claim they were produced or used by a living organism. Thus, the search continues. In this new effort, after the Curiosity rover’s drill stopped working in 2,017 the control team chose to conduct a type of experiment that had not been done by the rover before.

Curiosity carries an instrument called the Sample Analysis at Mars, an array of cups that hold samples of soil as they are being analyzed. The array has 74 cups—all but nine of them are empty most of the time. The other nine hold chemicals that are used to conduct other kinds of experiments. Because of the drill malfunction, the team at NASA chose to drop into the cups containing the chemicals and then to analyze the chemicals released due to reactions. The researchers found in the that had never been seen on Mars before. While the new experiment did not find evidence of life, it did show that there are other novel ways to test for it on Mars and other planets.

Use the code “Undecided” to get Curiosity Stream for less than $15 a year! https://curiositystream.com/Undecided. Before you blow your fuse and start leaving your nuclear fusion jokes in the comments, there’s been a major fusion development we have to talk about and it’s kind of a nuclear bombshell… poor choice of words… it’s big news. It’s all about high temperature semiconductors (ie. magnets).

Watch Exploring the 1,000 Mile Car Battery — Aluminum Air Hype? https://youtu.be/9OOq3f6mUxU?list=PLnTSM-ORSgi7UWp64ZlOKUPNXePMTdU4d.

Special thanks to MIT (http://news.mit.edu/) and Commonwealth Fusion Systems (https://cfs.energy/) for some of the video and photos used, as well as Dr. Greenwald for his time and expertise.

Video script and citations:
https://undecidedmf.com/episodes/exploring-why-this-nuclear-…gh-matters.

Follow-up podcast:
Video version — https://www.youtube.com/channel/UC4-aWB84Bupf5hxGqrwYqLA
Audio version — http://bit.ly/stilltbdfm.

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Learning science is about understanding complex systems and interactions among their entities. Telescopes are for observing objects that are far away, and microscopes are for exploring the tiniest objects. But what tools do we have for visualizing general patterns, processes, or relationships that can be defined in terms of compact mathematical models? Visualizing the unseeable can be a powerful teaching tool.

SETI Institute affiliate Dr. Mojgan Haganikar has written a book, Visualizing Dynamic Systems, that categorizes the visualization skills needed for various types of scientific problems. With the emergence of new technologies, we have more powerful tools to visualize invisible concepts, complex systems, and large datasets by revealing patterns and inter-relations in new ways. Join the SETI Institute’s Pamela Harman as she explores what is possible with Haganikar.

If you like science, support the SETI Institute! We’re a non-profit research institution whose focus is understanding the nature and origins of life in the universe. Donate here: https://seti.org/donate.

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Should we Build a Dyson Sphere?

Water has been detected in the most massive galaxy in the early Universe, along with its neighbouring companion, according to new observations from the Atacama Large Millimeter/submillimeter Array (ALMA). In addition to H2O, astronomers found carbon monoxide (CO) in the galaxy pair, which are designated as SPT0311-58 and located 12.88 billion light years from Earth.

Detection of these two molecules in abundance suggests that the molecular Universe was already going strong, only a relatively short time after the forging of elements in early generations of stars. The new research is the most detailed study of molecular gas content of a galaxy in the early Universe to date and the most distant detection of H20 in a regular star-forming galaxy. The research is published this week in The Astrophysical Journal.

Astronomers discovered the two galaxies in 2017. The pair’s location, or time, places them within the Epoch of Reionization. This epoch, as highlighted in the diagram below, occurred when the Universe was only 5% of its current age – and the first stars and galaxies were being born. Scientists believe that the two galaxies may be merging, and that their rapid star formation is not only using up their gas, but may eventually evolve the pair into massive, elliptical galaxies like those seen in the Local Universe.

An international team of scientists from Austria and Germany has launched a new paradigm in magnetism and superconductivity, putting effects of curvature, topology, and 3D geometry into the spotlight of next-decade research. The results are published in Advanced Materials.

Traditionally, the primary field in which curvature plays a pivotal role is the theory of general relativity. In recent years, however, the impact of curvilinear geometry has entered various disciplines, ranging from solid-state physics to soft-matter physics to chemistry and biology; and giving rise to a plethora of emerging domains, such as curvilinear cell biology, semiconductors, superfluidity, optics, plasmonics and 2D van der Waals materials. In modern magnetism, superconductivity and , extending nanostructures into the has become a major research avenue because of geometry-, curvature-and topology-induced phenomena. This approach provides a means to improve conventional functionalities and to launch novel functionalities by tailoring the curvature and 3D shape.

“In recent years, there have appeared experimental and theoretical works dealing with curvilinear and three-dimensional superconducting and (anti-)ferromagnetic nano-architectures. However, these studies originate from different scientific communities, resulting in the lack of knowledge transfer between such fundamental areas of condensed matter physics as magnetism and superconductivity,” says Oleksandr Dobrovolskiy, head of the SuperSpin Lab at the University of Vienna. “In our group, we lead projects in both these topical areas and it was the aim of our perspective article to build a ‘bridge’ between the magnetism and superconductivity communities, drawing attention to the conceptual aspects of how extension of structures into the third dimension and curvilinear geometry can modify existing and aid launching novel functionalities upon solid-state systems.”