Episodes
Monday Jul 24, 2023
Episode 544 - Metals recovering from fatigue
Monday Jul 24, 2023
Monday Jul 24, 2023
Cracks in metal can ultimately lead to fatigue failure, but is there a way to unwind the damage? Fatigue failure is a serious problem for everything from bridges to phones so finding a way to tackle it is important. One microcrack can turn into another as a metal fatigues, but what if the cracks could close themselves up again? Can a metal piece itself back together again? Maybe if its in a vacuum.
- Christopher M. Barr, Ta Duong, Daniel C. Bufford, Zachary Milne, Abhilash Molkeri, Nathan M. Heckman, David P. Adams, Ankit Srivastava, Khalid Hattar, Michael J. Demkowicz, Brad L. Boyce. Autonomous healing of fatigue cracks via cold welding. Nature, 2023; DOI: 10.1038/s41586-023-06223-0
Friday Jun 30, 2023
Episode 540 - On the shoulders of giants
Friday Jun 30, 2023
Friday Jun 30, 2023
The universe scaling work of the NANOGrav team stands on the shoulders of giants to understand giants lurking in our universe. Huge decade spanning scientific projects like NANOGrav are built of ideas and concepts which we can trace back to earlier pioneers. NANOGrav relies on Pulsars to map the universe but the discovery of them can be traced back to one key woman, Jocelyn Bell Burnell. This week we dive into the discovery of Pulsars and how they have been used to make a new way of looking at the universe. Finding a periodic signal in the noise can be helpful but a whole universe them of them can widen our understanding.
Tuesday Jun 20, 2023
Episode 539 - Dangerous but beautiful space weather
Tuesday Jun 20, 2023
Tuesday Jun 20, 2023
Weather in space, can seem far away but it's dazzling effects come with some danger. Aurora localised entirely around a satellite can cause a steamy situation for communications. Analysing space weather can lead to better designed satellites capable of withstanding 1-100 year solar storms. It's a balancing act when protecting satellites from solar weather, too much and too little protection can lead to disaster. Meteor showers are beautiful but how do you get one without an icey comet? The only way to get an asteroid to make a lovely meteor shower unfortunately involves a violent collision or big explosion.
- Nigel P. Meredith, Thomas E. Cayton, Michael D. Cayton, Richard B. Horne. Extreme Relativistic Electron Fluxes in GPS Orbit: Analysis of NS41 BDD‐IIR Data. Space Weather, 2023; 21 (6) DOI: 10.1029/2023SW003436
- W. Z. Cukier, J. R. Szalay. Formation, Structure, and Detectability of the Geminids Meteoroid Stream. The Planetary Science Journal, 2023; 4 (6): 109 DOI: 10.3847/PSJ/acd538
Monday Jun 12, 2023
Episode 538 - Colossal volcanic eruptions taking out satellites
Monday Jun 12, 2023
Monday Jun 12, 2023
When a volcano erupts we're used to imagining damage from lava, ash and even tsunamis. So why were satellites taken out? The colossal eruptions at Hunga-Tonga in 2022 caused pressure waves that caused damage 1000s of km away and even to satellites. Satellites, long distance radio and GPS all rely on the ionosphere, but large eruptions can wreck havoc and cause disruptions. When a pressure wave spreads out from a volcanic eruption, we can also get similar disruptions to the ionosphere. Sometimes even before shock wave hits. The way our ionosphere protects and responds to stellar radiation can be influenced by big events down here on Earth.
- Atsuki Shinbori, Takuya Sori, Yuichi Otsuka, Michi Nishioka, Septi Perwitasari, Takuo Tsuda, Atsushi Kumamoto, Fuminori Tsuchiya, Shoya Matsuda, Yoshiya Kasahara, Ayako Matsuoka, Satoko Nakamura, Yoshizumi Miyoshi, Iku Shinohara. Generation of equatorial plasma bubble after the 2022 Tonga volcanic eruption. Scientific Reports, 2023; 13 (1) DOI: 10.1038/s41598-023-33603-3
Tuesday May 16, 2023
Episode 534 - Finding a rocky asteroid belt around another star
Tuesday May 16, 2023
Tuesday May 16, 2023
Asteroid belts are harder to find than Sci-fi would have you believe. Spotting an asteroid belt is easier in the outer solar system, but closer in it gets a bit more blurry. Using the JWT we can use more than just visible light to find tricky interstellar objects. Asteroid belts are messy but they can tell us a lot about a solar system by what they leave in their wake.
Reference:
- András Gáspár, Schuyler Grace Wolff, George H. Rieke, Jarron M. Leisenring, Jane Morrison, Kate Y. L. Su, Kimberly Ward-Duong, Jonathan Aguilar, Marie Ygouf, Charles Beichman, Jorge Llop-Sayson, Geoffrey Bryden. Spatially resolved imaging of the inner Fomalhaut disk using JWST/MIRI. Nature Astronomy, 2023; DOI: 10.1038/s41550-023-01962-6
Monday Apr 24, 2023
Lagrange Point Episode 531 - Measuring the expansion of the universe
Monday Apr 24, 2023
Monday Apr 24, 2023
Understanding the future of the universe requires peering into the past. How quickly the universe is expanding has been an active area of science since the 1920s, with several prizes and breakthroughs. Each time we get new or more accurate measurements it forces scientists to re-evaluate the assumptions and formulas. These breakthroughs then need to be confirmed with follow up studies. The measurement of Hubble's constant using supernova won a Nobel Prize in 2011, and new gravitational lensing measurements have provided extra confirmation to those numbers. Dark matter can influence a lot in our universe, but measuring it is difficult but using lensing techniques a more accurate measurement can be derived.
- Mauricio Cruz Reyes, Richard I. Anderson. A 0.9% calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids. Astronomy & Astrophysics, 2023; 672: A85 DOI: 10.1051/0004-6361/202244775
- Princeton University. (2023, April 7). How to see the invisible: Using the dark matter distribution to test our cosmological model. ScienceDaily. Retrieved April 14, 2023 from www.sciencedaily.com/releases/2023/04/230407215847.htm
Monday Mar 20, 2023
Episode 526 - Capturing biological process in action
Monday Mar 20, 2023
Monday Mar 20, 2023
Seeing how something happens makes it much easier to understand. Biological process can be very hard to capture with images or video. Understanding how a protein requires thinking in 3D but to take images of them we often have to 'snap freeze' them in place. How can lasers, ions and quantum mechanics be used to help capture a protein in motion. PCR based diagnostics tests are accurate but require a lot of setup and expertise. Can you make a PCR test more like a point of care test using bio-luminescence.
- Shiny Maity, Brad D. Price, C. Blake Wilson, Arnab Mukherjee, Matthieu Starck, David Parker, Maxwell Z. Wilson, Janet E. Lovett, Songi Han, Mark S. Sherwin. Triggered Functional Dynamics of AsLOV2 by Time‐Resolved Electron Paramagnetic Resonance at High Magnetic Fields. Angewandte Chemie International Edition, 2023; 62 (13) DOI: 10.1002/anie.202212832
- Harmen J. van der Veer, Eva A. van Aalen, Claire M. S. Michielsen, Eva T. L. Hanckmann, Jeroen Deckers, Marcel M. G. J. van Borren, Jacky Flipse, Anne J. M. Loonen, Joost P. H. Schoeber, Maarten Merkx. Glow-in-the-Dark Infectious Disease Diagnostics Using CRISPR-Cas9-Based Split Luciferase Complementation. ACS Central Science, 2023; DOI: 10.1021/acscentsci.2c01467
Monday Feb 20, 2023
Episode 522 - Making hydrogen greenly from Seawater
Monday Feb 20, 2023
Monday Feb 20, 2023
Hydrogen comes in all kinds of colours but what does that mean? Hydrogen has a role to play in a decarbonised world as long as we can produce it greenly. It's no good producing green hydrogen if you use up another valuable resource or create another kind of waste. Water water everywhere, but not a drop to electrolyse. Using seawater to make hydrogen has challenges. How can we use the abundant seawater resource to make green energy sources without producing nasty by products?
- Suraj Loomba, Muhammad Waqas Khan, Muhammad Haris, Seyed Mahdi Mousavi, Ali Zavabeti, Kai Xu, Anton Tadich, Lars Thomsen, Christopher F. McConville, Yongxiang Li, Sumeet Walia, Nasir Mahmood. Nitrogen‐Doped Porous Nickel Molybdenum Phosphide Sheets for Efficient Seawater Splitting. Small, 2023; 2207310 DOI: 10.1002/smll.202207310
Tuesday Feb 14, 2023
Episode 521 - Galaxies at the Cosmic Dawn
Tuesday Feb 14, 2023
Tuesday Feb 14, 2023
Using the JWST to peer into the Cosmic dawn of the universe. The JWST enables researchers to peer into the earliest galaxies in our universe. 250 Million years is not a long time when it comes to a star or galaxy. With JWST researchers can see galaxies formed 250 million years after the Big Bang. To peer into the earliest universe you must use infrared to capture the faintest light. Using new instruments on the JWST researchers are able to see galaxies from 13.25 billion years ago. JWST also lets researchers investigate strange new types of spiral galaxies from the Cosmic Noon.
- Yoshinobu Fudamoto, Akio K. Inoue, Yuma Sugahara. Red Spiral Galaxies at Cosmic Noon Unveiled in the First JWST Image. The Astrophysical Journal Letters, 2022; 938 (2): L24 DOI: 10.3847/2041-8213/ac982b
- University of California - Santa Cruz. (2022, December 9). Astronomers report most distant known galaxies, detected and confirmed. ScienceDaily. Retrieved January 2, 2023 from www.sciencedaily.com/releases/2022/12/221209135542.htm
Monday Dec 26, 2022
Episode 515 - Do you really need oxygen for oxidation
Monday Dec 26, 2022
Monday Dec 26, 2022
How does chemistry change when you travel to another planet? When it comes to scientific experiments often we can be hampered by our own experience. Just because something is abundant on earth does not meant that it's a universal constant. Out of this world chemistry is hard to get your head around and it requires thinking outside the box. Is it possible to have oxidize minerals without oxygen?
- Kaushik Mitra, Eleanor L. Moreland, Greg J. Ledingham, Jeffrey G. Catalano. Formation of manganese oxides on early Mars due to active halogen cycling. Nature Geoscience, 2022; DOI: 10.1038/s41561-022-01094-y
Monday Dec 19, 2022
Episode 514 - Pushing water to the limits on earth and in space
Monday Dec 19, 2022
Monday Dec 19, 2022
What happens when you push water to the limits on earth and in Space? Water has really weird properties especially when it gets really cold. How can we understand and model the behaviour when it moves to fast for us to capture? How do droplets form and why do you need the ISS to study it? What can microgravity tell us about the way droplets form?
- Thomas E. Gartner, Pablo M. Piaggi, Roberto Car, Athanassios Z. Panagiotopoulos, Pablo G. Debenedetti. Liquid-Liquid Transition in Water from First Principles. Physical Review Letters, 2022; 129 (25) DOI: 10.1103/PhysRevLett.129.255702
- J. McCraney, J. Ludwicki, J. Bostwick, S. Daniel, P. Steen. Coalescence-induced droplet spreading: Experiments aboard the International Space Station. Physics of Fluids, 2022; 34 (12): 122110 DOI: 10.1063/5.0125279
Monday Dec 12, 2022
Episode 513 - An eerie glow in the Solar System
Monday Dec 12, 2022
Monday Dec 12, 2022
How do you measure the solar system and the universe whilst being inside of it? Too much light is a problem for astronomers and our solar system has it's own glow. If you take away all known light sources form the solar system, there is still a faint glow. We know about background radiation, but what about the solar systems background lighting? How can you test the curvature of the universe? To answer universal scale questions you need to start small. Really small. Using Bose Einstein condensates and getting really cold we can simulate curved universes in a molecule scale.
- Timothy Carleton, Rogier A. Windhorst, Rosalia O’Brien, Seth H. Cohen, Delondrae Carter, Rolf Jansen, Scott Tompkins, Richard G. Arendt, Sarah Caddy, Norman Grogin, Scott J. Kenyon, Anton Koekemoer, John MacKenty, Stefano Casertano, Luke J. M. Davies, Simon P. Driver, Eli Dwek, Alexander Kashlinsky, Nathan Miles, Nor Pirzkal, Aaron Robotham, Russell Ryan, Haley Abate, Hanga Andras-Letanovszky, Jessica Berkheimer, Zak Goisman, Daniel Henningsen, Darby Kramer, Ci’mone Rogers, Andi Swirbul. SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-sky Surface-brightness Measurements: II. First Limits on Diffuse Light at 1.25, 1.4, and 1.6 μm. The Astronomical Journal, 2022; 164 (5): 170 DOI: 10.3847/1538-3881/ac8d02
- Celia Viermann, Marius Sparn, Nikolas Liebster, Maurus Hans, Elinor Kath, Álvaro Parra-López, Mireia Tolosa-Simeón, Natalia Sánchez-Kuntz, Tobias Haas, Helmut Strobel, Stefan Floerchinger, Markus K. Oberthaler. Quantum field simulator for dynamics in curved spacetime. Nature, 2022; 611 (7935): 260 DOI: 10.1038/s41586-022-05313-9
Monday Sep 26, 2022
Episode 502 - Ignobel prizes ’22 - Blind dates and Mother Ducks
Monday Sep 26, 2022
Monday Sep 26, 2022
We celebrate the Ignobel prizes for 2022 with science that makes you laugh and then think. What connects a Fish, ducks and slipstream racing? How do mother ducks manage to keep all their ducklings in tow? Does swimming in formation help the ducks save energy? What's the best spot in the slipstream to be? We all know following in the slipstream is good, but if you're 3 or more back you can literally get pulled along. Complex fluid mechanics makes swimming in a line a way for a mother duck to pull the ducklings along. What happens physically when you find someone who is a good match? Is eye contact or heart rate a better measure of having a 'spark' with someone new?
- Wave-Riding and Wave-Passing by Ducklings in Formation Swimming,” Zhi-Ming Yuan, Minglu Chen, Laibing Jia, Chunyan Ji, and Atilla Incecik, Journal of Fluid Mechanics, vol. 928, no. R2, 2021.
- “Energy Conservation by Formation Swimming: Metabolic Evidence from Ducklings,” Frank E. Fish, in the book Mechanics and Physiology of Animal Swimming, 1994, pp. 193-204.
- Physiological Synchrony is Associated with Attraction in a Blind Date Setting,” Eliska Prochazkova, Elio Sjak-Shie, Friederike Behrens, Daniel Lindh, and Mariska E. Kret, Nature Human Behaviour, vol. 6, no. 2, 2022, pp. 269-278.
Monday Sep 05, 2022
Episode 499 - Air and atmospheres on exoplanets
Monday Sep 05, 2022
Monday Sep 05, 2022
CO2 gets a lot of bad press on earth, but in space, it could actually be incredibly helpful. On Mars, the Perseverance mission turned CO2 into Oxygen just like a tree. Making air on Mars requires a bit of Moxie and Perseverance. Mar's atmosphere may be thin, highly variable and full of CO2 but it can be harnessed to produce Oxygen. Could future mission to Mars make their own oxygen on the surface of Mars? Finding CO2 on exoplanets has been incredibly hard but the JWST helps shed light on this universal gas. Incredible hot, massive but not super dense, the Hot Jupiter WASP-39b becomes the latest target of the JWST. What can a hot Jupiter like WASP-39b teach us about exoplanet formation?
- The JWST Transiting Exoplanet Community Early Release Science Team et al. Identification of carbon dioxide in an exoplanet atmosphere. Nature (in press), 2022 [abstract]
- Jeffrey A. Hoffman, Michael H. Hecht, Donald Rapp, Joseph J. Hartvigsen, Jason G. Soohoo, Asad M. Aboobaker, John B. Mcclean, Andrew M. Liu, Eric D. Hinterman, Nasr, Shravan Hariharan, Kyle J. Horn, Forrest E. Meyen, Harald Okkels, Parker Steen, Singaravelu Elangovan, Christopher R. Graves, Piyush Khopkar, Morten B. Madsen, Gerald E. Voecks, Peter, H. Smith, Theis, L. Skafte, Koorosh R. Araghiand, David J. Eisenman. Mars Oxygen ISRU Experiment (MOXIE)—Preparing for human Mars exploration. Science Advances, 2022 DOI: DOI: 10.1126/sciadv.abp8636
Monday Aug 15, 2022
Episode 496 - Dwarf Planets and Massive collisions forming Moons
Monday Aug 15, 2022
Monday Aug 15, 2022
Dwarf planets are strange objects in our solar systems, but Ceres is unusual amongst that group. Why is Ceres' surface so strange and how could it have formed without a hot core? Ceres is too small to really have a molten core or large molten surfaces. How did Ceres end up with odd plateaus and continent like features without an active core? How could radiation cause Ceres to form in such an odd way? The Moon's relative size is puzzling but how can we prove that it was caused by a colossal collision?
- Scott D. King, Michael T. Bland, Simone Marchi, Carol A. Raymond, Christopher T. Russell, Jennifer E. C. Scully, Hanna G. Sizemore. Ceres’ Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection. AGU Advances, 2022; 3 (3) DOI: 10.1029/2021AV000571
- Patrizia Will, Henner Busemann, My E. I. Riebe, Colin Maden. Indigenous noble gases in the Moon’s interior. Science Advances, 2022; 8 (32) DOI: 10.1126/sciadv.abl4920
Monday Jul 18, 2022
Episode 492 - Finding hidden objects in the early universe
Monday Jul 18, 2022
Monday Jul 18, 2022
How can you find objects that are hard to see in the depths of space? There is plenty of gas in a galaxy, but trying to see a cloud amongst all those starts is not easy. The further back in time you look in the history of the universe, the colder and darker it gets. How do you figure out the structure of the earliest galaxies and their cold gas? A black hole roaming across a galaxy sounds like bad sci fi horror, but may have been found. How can you spot a black hole without any frame of reference? Detecting a roaming black hole is tricky but not impossible.
- Kieran A. Cleary, Jowita Borowska, Patrick C. Breysse, Morgan Catha, Dongwoo T. Chung, Sarah E. Church, Clive Dickinson, Hans Kristian Eriksen, Marie Kristine Foss, Joshua Ott Gundersen, Stuart E. Harper, Andrew I. Harris, Richard Hobbs, Håvard T. Ihle, Junhan Kim, Jonathon Kocz, James W. Lamb, Jonas G. S. Lunde, Hamsa Padmanabhan, Timothy J. Pearson, Liju Philip, Travis W. Powell, Maren Rasmussen, Anthony C. S. Readhead, Thomas J. Rennie, Marta B. Silva, Nils-Ole Stutzer, Bade D. Uzgil, Duncan J. Watts, Ingunn Kathrine Wehus, David P. Woody, Lilian Basoalto, J. Richard Bond, Delaney A. Dunne, Todd Gaier, Brandon Hensley, Laura C. Keating, Charles R. Lawrence, Norman Murray, Roberta Paladini, Rodrigo Reeves, Marco P. Viero, Risa H. Wechsler. COMAP Early Science. I. Overview. The Astrophysical Journal, 2022; 933 (2): 182 DOI: 10.3847/1538-4357/ac63cc
- Casey Y. Lam, Jessica R. Lu, Andrzej Udalski, Ian Bond, David P. Bennett, Jan Skowron, Przemek Mroz, Radek Poleski, Takahiro Sumi, Michal K. Szymanski, Szymon Kozlowski, Pawel Pietrukowicz, Igor Soszynski, Krzysztof Ulaczyk, Lukasz Wyrzykowski, Shota Miyazaki, Daisuke Suzuki, Naoki Koshimoto, Nicholas J. Rattenbury, Matthew W. Hosek Jr., Fumio Abe, Richard Barry, Aparna Bhattacharya, Akihiko Fukui, Hirosane Fujii, Yuki Hirao, Yoshitaka Itow, Rintaro Kirikawa, Iona Kondo, Yutaka Matsubara, Sho Matsumoto, Yasushi Muraki, Greg Olmschenk, Clement Ranc, Arisa Okamura, Yuki Satoh, Stela Ishitani Silva, Taiga Toda, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Natasha S. Abrams, Shrihan Agarwal, Sam Rose, Sean K. Terry. An isolated mass gap black hole or neutron star detected with astrometric microlensing. Accepted to APJ Letters, 2022 [abstract]
- Kailash C. Sahu, Jay Anderson, Stefano Casertano, Howard E. Bond, Andrzej Udalski, Martin Dominik, Annalisa Calamida, Andrea Bellini, Thomas M. Brown, Marina Rejkuba, Varun Bajaj, Noe Kains, Henry C. Ferguson, Chris L. Fryer, Philip Yock, Przemek Mroz, Szymon Kozlowski, Pawel Pietrukowicz, Radek Poleski, Jan Skowron, Igor Soszynski, Michael K. Szymanski, Krzysztof Ulaczyk, Lukasz Wyrzykowski, Richard Barry, David P. Bennett, Ian A. Bond, Yuki Hirao, Stela Ishitani Silva, Iona Kondo, Naoki Koshimoto, Clement Ranc, Nicholas J. Rattenbury, Takahiro Sumi, Daisuke Suzuki, Paul J. Tristram, Aikaterini Vandorou, Jean-Philippe Beaulieu, Jean-Baptiste Marquette, Andrew Cole, Pascal Fouque, Kym Hill, Stefan Dieters, Christian Coutures, Dijana Dominis-Prester, Clara Bennett, Etienne Bachelet, John Menzies, Michael Alb-row, Karen Pollard, Andrew Gould, Jennifer Yee, William Allen, Leonardo Andrade de Almeida, Grant Christie, John Drummond, Avishay Gal-Yam, Evgeny Gorbikov, Francisco Jablonski, Chung-Uk Lee, Dan Maoz, Ilan Manulis, Jennie McCormick, Tim Natusch, Richard W. Pogge, Yossi Shvartzvald, Uffe G. Jorgensen, Khalid A. Alsubai, Michael I. Andersen, Valerio Bozza, Sebastiano Calchi Novati, Martin Burgdorf, Tobias C. Hinse, Markus Hundertmark, Tim-Oliver Husser, Eamonn Kerins, Penelope Longa-Pena, Luigi Mancini, Matthew Penny, Sohrab Rahvar, Davide Ricci, Sedighe Sajadian, Jesper Skottfelt, Colin Snodgrass, John Southworth, Jeremy Tregloan-Reed, Joachim Wambsganss, Olivier Wertz, Yiannis Tsapras, Rachel A. Street, Daniel M. Bramich, Keith Horne, Iain A. Steele. An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing. Accepted to APJ, 2022 [abstract]
Monday May 09, 2022
Episode 482 - Nova and Micronova not quite super still immensely powerful
Monday May 09, 2022
Monday May 09, 2022
Supernova get all the press, but Nova and Micronova are still pretty powerful. White dwarf stars are normally pretty inactive, unless some hydrogen ends up kickstarting them again. Enough helium leeched from a nearby star can ignite the entire surface of a white dwarf. Nova may not destroy the star, but they can create immensely powerful explosions and particles. The right combination of White Dwarf and Red Giant can create powerful particles near the speed of light. Micronova sound small but they are still colossal and brief explosions on white dwarf stars. Not powerful enough to ignite the whole surface of a star, but definitely enough to destroy a planet, micronova are quite deadly.
- Scaringi, S., Groot, P.J., Knigge, C. et al. Localized thermonuclear bursts from accreting magnetic white dwarfs. Nature, 2022 DOI: 10.1038/s41586-022-04495-6
- V. A. Acciari, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, M. Artero, K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida, J. A. Barrio, I. Batković, J. Becerra González, W. Bednarek, L. Bellizzi, E. Bernardini, M. Bernardos, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, H. Bökenkamp, G. Bonnoli, Ž. Bošnjak, G. Busetto, R. Carosi, G. Ceribella, M. Cerruti, Y. Chai, A. Chilingarian, S. Cikota, S. M. Colak, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espiñeira, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, V. Fallah Ramazani, L. Fariña Alonso, A. Fattorini, M. V. Fonseca, L. Font, C. Fruck, S. Fukami, Y. Fukazawa, R. J. García López, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto, F. Giordano, P. Gliwny, N. Godinović, J. G. Green, D. Green, D. Hadasch, A. Hahn, T. Hassan, L. Heckmann, J. Herrera, J. Hoang, D. Hrupec, M. Hütten, T. Inada, K. Ishio, Y. Iwamura, I. Jiménez Martínez, J. Jormanainen, L. Jouvin, D. Kerszberg, Y. Kobayashi, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Martínez, A. Mas Aguilar, D. Mazin, S. Menchiari, S. Mender, S. Mićanović, D. Miceli, T. Miener, J. M. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, D. Morcuende, V. Moreno, E. Moretti, T. Nakamori, L. Nava, V. Neustroev, M. Nievas Rosillo, C. Nigro, K. Nilsson, K. Nishijima, K. Noda, S. Nozaki, Y. Ohtani, T. Oka, J. Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, L. Pavletić, P. Peñil, M. Persic, M. Pihet, P. G. Prada Moroni, E. Prandini, C. Priyadarshi, I. Puljak, W. Rhode, M. Ribó, J. Rico, C. Righi, A. Rugliancich, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, F. G. Saturni, B. Schleicher, K. Schmidt, T. Schweizer, J. Sitarek, I. Šnidarić, D. Sobczynska, A. Spolon, A. Stamerra, J. Strišković, D. Strom, M. Strzys, Y. Suda, T. Surić, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, L. Tosti, S. Truzzi, A. Tutone, S. Ubach, J. van Scherpenberg, G. Vanzo, M. Vazquez Acosta, S. Ventura, V. Verguilov, C. F. Vigorito, V. Vitale, I. Vovk, M. Will, C. Wunderlich, T. Yamamoto, D. Zarić, F. Ambrosino, M. Cecconi, G. Catanzaro, C. Ferrara, A. Frasca, M. Munari, L. Giustolisi, J. Alonso-Santiago, M. Giarrusso, U. Munari, P. Valisa. Proton acceleration in thermonuclear nova explosions revealed by gamma rays. Nature Astronomy, 2022; DOI: 10.1038/s41550-022-01640-z
Monday Apr 11, 2022
Monday Apr 11, 2022
Water has some pretty amazing properties. We dive into some of the strange things water does from the molecular level all the way to planet scale water flows. We all know H2O but studying the way water molecules move around each other is very difficult to isolate. H2O molecules had to be taken to 0.4 Kelvin and shot with a powerful laser to shed light on the way they shake. The way H2O interacts between molecules by moving, rotating and shaking can help explain some of the weird properties. H2O has weird properties like being at its highest density at 4 degrees. Turning salt water into fresh water often involves a lot of electricity, but a new method using Ionic salts may get by with barely any heat. How can water make its way down towards the core of the earth? Water masqueraded inside minerals to migrate deep down beneath the surface of the earth.
- Martina Havenith-Newen, Raffael Schwan, Chen Qu, Devendra Mani, Nitish Pal, Gerhard Schwaab, Lex van der Meer, Britta Redlich, Claude LeForestier, Joel Bowman. Observation of the low frequency spectrum of water dimer as a sensitive test of the water dimer potential and dipole moment surfaces. Angewandte Chemie International Edition, 2019; DOI: 10.1002/anie.201906048
- Hyungmook Kang, David E. Suich, James F. Davies, Aaron D. Wilson, Jeffrey J. Urban, Robert Kostecki. Molecular insight into the lower critical solution temperature transition of aqueous alkyl phosphonium benzene sulfonates. Communications Chemistry, 2019; 2 (1) DOI: 10.1038/s42004-019-0151-2
- Jun Tsuchiya, Koichiro Umemoto. First‐Principles Determination of the Dissociation Phase Boundary of Phase H MgSiO 4 H 2. Geophysical Research Letters, 2019; DOI: 10.1029/2019GL083472
Monday Jan 03, 2022
Episode 464 - Rogue Planets and glass in meteorites
Monday Jan 03, 2022
Monday Jan 03, 2022
Rogue planets hurtling across space without a place to call home. How do we detect intergalactic nomads like Rogue planets? Just how many rogue planets are out there? Are there rogue planets lurking in our own solar system? Glass inside meteorites can help us understand early earth. How does meteorite rock differ from rock here on earth? What can we piece together about the cataclysmic events that formed glass inside meteorites? Rapidly heating then even more rapidly cooling coalesced glass inside meteorites.
- Núria Miret-Roig, Hervé Bouy, Sean N. Raymond, Motohide Tamura, Emmanuel Bertin, David Barrado, Javier Olivares, Phillip A. B. Galli, Jean-Charles Cuillandre, Luis Manuel Sarro, Angel Berihuete, Nuria Huélamo. A rich population of free-floating planets in the Upper Scorpius young stellar association. Nature Astronomy, 2021; DOI: 10.1038/s41550-021-01513-x
- Nicole X. Nie, Xin-Yang Chen, Timo Hopp, Justin Y. Hu, Zhe J. Zhang, Fang-Zhen Teng, Anat Shahar, Nicolas Dauphas. Imprint of chondrule formation on the K and Rb isotopic compositions of carbonaceous meteorites. Science Advances, 2021; 7 (49) DOI: 10.1126/sciadv.abl3929
Monday Dec 06, 2021
Episode 460 - What shape is the heliosphere
Monday Dec 06, 2021
Monday Dec 06, 2021
Just what is the heliosphere and how doe sit work? What shape is the heliosphere (spoiler alert, probably not a sphere). At the very edge of our solar system lies the boundary between our neighborhood and interstellar space. Do outside forces from interstellar space jumble up the heliosphere? Sandwiched between Space and the Earth, the Ionsphere buzzes and hums with a pulsing generator. Winds from earth can bend and shape plasma in our ionsphere to make a generator. Moving a conducting object through a magnetic field can generate electricty, and its happening right now 100km above our heads.
- M. Opher, J. F. Drake, G. Zank, E. Powell, W. Shelley, M. Kornbleuth, V. Florinski, V. Izmodenov, J. Giacalone, S. Fuselier, K. Dialynas, A. Loeb, J. Richardson. A Turbulent Heliosheath Driven by the Rayleigh–Taylor Instability. The Astrophysical Journal, 2021; 922 (2): 181 DOI: 10.3847/1538-4357/ac2d2e
- Thomas J. Immel, Brian J. Harding, Roderick A. Heelis, Astrid Maute, Jeffrey M. Forbes, Scott L. England, Stephen B. Mende, Christoph R. Englert, Russell A. Stoneback, Kenneth Marr, John M. Harlander, Jonathan J. Makela. Regulation of ionospheric plasma velocities by thermospheric winds. Nature Geoscience, 2021; DOI: 10.1038/s41561-021-00848-4