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If you want to learn about prepping‚ from a common sense approach‚ you're in the right place. We're going to talk about all sorts of stuff. Politics‚ fire‚ where to stack your stuff‚ how to get away and general things like that. I try to upload a video every week and I do lots of shorts. We hope to see you around. As usual‚ stay safe and have a great day! Link to radio deal in this video - https://amzn.to/418ej9O Link to study in this video - https://www.finder.com/doomsday-prepper-statistics Support the channel: Prepper Store - https://www.amazon.com/shop/localprepper Patreon - https://www.patreon.com/localprepper Buy Me A Coffee - https://www.buymeacoffee.com/localprepper Link-Tree - https://linktr.ee/localprepper My Website - https://www.localprepper.net PrepStock 2024: https://www.prepstock.net/ Free Discord: https://discord.gg/rwtcBncck3 Snail mail: P.O. Box 12 Onancock‚ VA 23417 ❱❱❱ DISCLAIMER: - The opinions stated in this video are my own. - I have no sponsors... Yet. - I AM AN AMAZON AFFIALITE and SOME links are AFFIALIATE LINKS also know as "Paid Links" where I make‚ what I think are‚ about two cents for every dollar you spend. It costs you nothing extra. #news #israel #war #survival #prepper #shtf #prepardness #offgrid ​#nuclearwar #war #economy #survival #prepper #shtf #prepardness #offgrid ​#conflicted #localprepper #wwiii #russia #china #ukraine #survival #prepper #shtf #prepardness #nuclear #martiallaw #wrol #prisoner

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Astronomers know of about 60 rocky exoplanets orbiting in the habitable zones of their stars. When they try to determine how habitable these planets might be‚ detecting water in their atmospheres plays a huge role. But what if there was another way of measuring the water content in these worlds? Researchers are developing a way of modelling these worlds to determine how much water they have. Habitability likely requires surface water‚ as far as we can tell. But detecting surface water is next to impossible. The next best thing is to use the tools we have—like the James Webb Space Telescope—to detect and characterize exoplanet atmospheres. But despite the JWST’s power‚ it can’t examine every exoplanet atmosphere. Some are beyond its reach. But one team of researchers is using what we do know about exoplanets‚ tidal heating‚ and radiogenic heating to try to determine which exoplanets might have oceans‚ either on the surface or under the surface. The team of scientists examined the list of rocky exoplanets in habitable zones and used modelling to determine how likely it is that they have a thick‚ surface or subsurface ocean layer. They’re publishing their results in a paper titled “Water content of rocky exoplanets in the habitable zone.” The lead author is Adam Boldog from the Konkoly Observatory and the HUN-REN Research Centre for Astronomy and Earth Sciences in Budapest‚ Hungary. One of the obstacles exoplanet scientists face is the proliferation of M-dwarf stars or red dwarfs. Half of the stars in the Milky Way might be red dwarfs‚ and that’s where we’ve found most rocky planets in habitable zones. But red dwarfs exhibit significant flaring‚ and sometimes that flaring is far more powerful than anything our Sun produces. Since red dwarfs aren’t as luminous as Sun-like stars‚ their habitable zones are much closer to the star. That means that exoplanets in their habitable zones may have their atmospheres stripped away by the red dwarf’s powerful flaring. Once the atmosphere is gone‚ surface water is sure to follow. An artist’s conception of a violent flare erupting from a red dwarf star. Such flares can obliterate the atmospheres of nearby planets. Credit: NRAO/S. Dagnello. In those cases‚ the planet could still support life‚ even without atmospheres. It’s possible that rocky planets in red dwarf habitable zones have lots of liquid water‚ just not on the surface. They could be more like our Solar System’s ocean moons Europa‚ Enceladus‚ and others. They have ample water‚ more than Earth in some cases. But they have no surface water and only extremely tenuous atmospheres. JWST’s atmospheric spectroscopy can’t tell us much about these types of worlds and if they have oceans. “Therefore‚ it is important to explore other possible ways of studying the habitability of exoplanets that do not rely on the presence of an atmosphere‚” the authors explain. “In this study‚ we investigated the interiors of rocky exoplanets in order to identify those that may have large quantities of water‚” the authors write. “We modelled the interiors of 28 rocky exoplanets‚ assuming four different layers – an iron core‚ a rock mantle‚ a high-pressure ice layer‚ and a surface ice/water layer.” Aside from a planet’s structure‚ its heat budget plays a large role in its liquid water content. There are two ways a planet can generate heat. One is radiogenic heat that comes from the radioactive decay of isotopes of uranium‚ thorium‚ and potassium in the planet’s mantle and crust. The other is tidal heating‚ which comes from the friction generated by a planet’s orbit and rotation. The researchers included the likely amounts of both in their model. “We estimated the probability of the presence of a thick ocean layer in these planets‚ taking into account the effect of both tidal and radiogenic heating‚” the authors explain. Some of the planets in the study are well-known. Proxima Centauri b is the closest exoplanet to Earth‚ making it an object of intense speculation and study. The TRAPPIST-1 planets made headlines when they were discovered a few years ago. Others‚ including TOI 700d‚ are intriguing Earth-size exoplanets. This is a Hubble image of our closest stellar neighbour‚ Proxima Centauri. Proxima Centauri b is a rocky exoplanet in the star’s habitable zone. Credit: ESA/Hubble &; NASA In their modelling‚ the researchers based the exoplanet structure on previous work showing that rocky exoplanets can have an iron core‚ a rocky mantle‚ a layer composed of high-pressure ice polymorphs (HPP)‚ and a surface ice/water layer. Based on the mass and radius of each planet‚ the researchers determined the water mass fractions for each of the 28 planets. This is a measure of how much of each planet’s mass is water. The modelling arrived at a range of water mass fractions for each planet. The input mass and sizes for some of the planets are more certain than others‚ and that is shown in the figure below with the resulting H2O mass fractions concentrated in a relatively narrow range‚ with the H2O mass fractions showing a peak in the distribution at the largest probabilities. “The colour and the numbers indicate the fraction of all modelled interiors that resulted in internal structures within a certain H2O mass fraction range‚” the authors explain. “If a large number of interiors had high H2O mass fractions for a given planet‚ that appears as a shift in the values and lighter colours in the figure towards the higher mass fraction ranges.” The researchers found that all 28 of the planets in their sample could have global ice or water surfaces. Some of them don’t even need atmospheres. This figure from the study shows the distribution of the resulting internal structures in different H2O mass fraction ranges for each of the 28 rocky exoplanets. Note that the top and bottom panels are in different percentage increments: 3% for the top and 6% for the bottom. For example‚ Kepler 62 f‚ 452 b and 442 b could all be water worlds. Image Credit: Boldog et al. 2023 “Our results show that all of these planets could have large enough H2O mass fractions to have global ice/water surfaces‚” the researchers write. “Planets with surface temperatures above the melting point ofice and large water mass fractions may have global oceans regardless of the presence of an atmosphere.” Planets with surface temperatures below the melting point could still have water‚ according to the research‚ but it would be covered by ice. “If the internal heat flux in these bodies is sufficiently high to cause melting in the HPP layer‚ these worlds may harbour underground liquid water reservoirs‚” they explain. Among the study’s intriguing results are the TRAPPIST-1 planets. Since we have more accurate data for them than some of the other 28 planets in the study‚ the researchers say their results are more likely to be accurate. “All of the modelled TRAPPIST-1 planets are likely to have extended H2O layers‚” the authors explain‚ adding that the nature of those layers needs to be determined to assess habitability. Three of the TRAPPIST-1 planets – TRAPPIST-1e‚ f and g – dwell in their star’s so-called habitable zone. This research concludes that the three planets also likely have extended H2O layers. Image Credit: NASA/JPL Some of the 28 planets have so much water that they may be ocean planets. In those cases‚ water vapour may provide enough atmospheric pressure to preserve surface oceans. “Our results suggest that Kepler-62 f‚ Kepler-452 b and Kepler-442 b could be members of the ocean-world class.” This figure from the research presents some of the results. The colour of each planet’s dot represents the probability of it having an internal ocean. Image Credit: Boldog et al. 2023 The study has some weak points‚ which the authors are quick to point out. For one thing‚ our understanding of radiogenic heating on worlds in other solar systems is based on a generalization from our Solar System. There could be far more or far less radiogenic elements in rocky planets in other solar systems. Tidal heating is similarly uncertain. “It is worth noting that tidal heating is strongly dependent on the eccentricity of the planetary orbit‚ which changes during the evolution of the planet‚” the authors explain. Planets on eccentric orbits experience tidal heating. But planets close to their stars eventually move toward circular orbits‚ which could eliminate that heat source. If some of these results are correct‚ there may be more worlds with subsurface oceans than we think. Who knows? Maybe it’s Earth that’s the oddball. “Subsurface oceans may be excellent sites for the development of life‚ although this may be difficult to observe with our current technology‚” the authors conclude. Studies like this can’t replace direct observation‚ but history shows how important they are in refining scientists’ thinking. Though we can’t observe these planets well enough to determine for certain if they have oceans or not‚ at least scientists can take what they do know and work toward an answer. The post Astronomers Calculate Which Exoplanets Are Most Likely to Have Water appeared first on Universe Today.

Private and military organizations are tracking some of the 170 million pieces of space junk orbiting the planet‚ but they’re limited to how small an object they can detect. Only chunks larger than a softball can be tracked with radar or optical systems‚ and that only accounts for less than 1% of the junk out there. But a new technique is being developed to resolve space junk to pieces smaller than one millimeter in diameter. Called Space Debris Identification and Tracking (SINTRA)‚ the project will test out a new technique that uses the state-of-the-art sensors to detect plasma waves created by fields of debris. The new sensors are used along with existing sensors‚ such as ground-based radar‚ tracking satellites‚ and optical sensors in order to identify and track space debris in the one-millimeter size range. “Right now‚ we detect space debris by looking for objects that reflect light or radar signals‚” said Nilton Renno‚ from the University of Michigan and a professor of climate and space sciences‚ and engineering and aerospace engineering. “The smaller the objects get‚ the harder it becomes to get sunlight or radar signals strong enough to detect them from the ground.” SINTRA is a 4-year project that will help advance the sensors needed for detecting orbital debris signatures. SIINTRA is a collaborative project funded by the Intelligence Advanced Research Projects Activity’s Space Debris Identification and Tracking Program. The project includes military contractor Blue Halo as well as several universities‚ such as the University of Michigan and the University of Alaska Fairbanks as well as MIT Lincoln Laboratory‚ Naval Research Laboratory‚ Los Alamos National Laboratory‚ and JHU Applied Physics Laboratory. Estimated number of objects in low Earth orbit. Credit: NASA The idea behind SINTRA is to search for the electrical signals emitted by clouds of space debris. Colliding pieces of space debris explode into tiny fragments‚ some of which vaporize into a charged gas due to the heat created by the impact.  “When the cloud of charged gas and debris fragments expands‚ it creates lightning-like energy bursts‚ similar to signals produced by static sparks that appear after rubbing a freshly laundered blanket‚” said Mojtaba Akhavan-Tafti‚ an assistant research scientist in climate and space sciences and engineering‚ and a lead scientist on the project for the University of Michigan. The charged gas and debris fragments can create electric field pulses whenever they come close enough to each other‚ producing additional electrical bursts. These signals last for only a fraction of a second‚ but they could help track pieces of space debris and clouds of microscopic fragments that form when debris collides. For example‚ when two pieces of aluminum collide at typical orbital speeds‚ they emit an electrical burst strong enough for a 26-meter dish with a high-quality radio receiver to detect from the ground‚ according to the University of Michigan team’s most recent computer simulations. The electric field pulses should similarly be detectable with more sensitive radio arrays‚ such as NASA’s Deep Space Network. A piece of space junk punched this hole into the hull of NASA’s Solar Max spacecraft. Image credit: NASA Orbital Debris Program Office. If successful‚ SINTRA would enable the first tracking capability for the ultra-small debris population‚ reducing risk to worldwide space operations. Space debris in low Earth orbit (LEO) have an average impact velocity of 36‚000 km/hr (22‚500 MPH). Therefore‚ even the smallest of debris can cause significant damage to operational satellites. But there’s a lot of work yet to do in making the SINTRA concept work. The frequency of the electrical signals can vary with the speed of the collision; additionally‚ what the debris is made of also changes many variables‚ which could complicate detection. In a press release from the University of Michigan‚ Akhavan-Tafti said that to see the electric signals‚ they need to be stronger than the ground instrument’s background signals and pass through Earth’s upper atmosphere. For the project‚ the team will start by measuring real signals with NASA’s Deep Space Network‚ and analyze data from hypervelocity experiments at the Naval Research Laboratory and NASA’s Ames Research Center. Using the facilities’ lasers‚ the team can launch different kinds of debris at targets over a range of orbital speeds and measure the characteristics of the electric emissions resulting from the impact. If such experiments reveal a way to detect a wide range of electrical signals generated during space debris collisions‚ they could determine not just where space debris is‚ but what it looks like and is made of. In a press release earlier this year‚ the US Intelligence Advanced Research Projects Activity agency said the goal of the SINTRA program is to fill gaps in current space debris-monitoring systems‚ which currently only track and monitor debris objects larger than four inches across. They said the detection‚ tracking‚ and characterization of lethal non-trackable space debris would support the safe operation of valuable space assets worldwide. For more information‚ see the SINTRA website. The post 99% of Space Junk is Undetectable. That Could Change Soon appeared first on Universe Today.

Billionaire entrepreneur Reid Hoffman has given a $250‚000 donation to Republican presidential candidate Nikki Haley’s campaign. 

Reggaetón music superstar Daddy Yankee‚ whose real name is Ramón Luis Ayala Rodríguez‚ is leaving the mainstream music scene to better focus on his faith.