The Wayfarer was a valuable trait in Remnant 2‚ offering the player an increase in traversal speed. With the recent release of The Forgotten Kingdom DLC‚ the Wayfarer trait has had some significant changes. In fact‚ it’s no longer in the game. Don’t worry‚ we have everything you need to know about the Wayfarer traits replacement in this guide. What happened to the Wayfarer trait in Remant 2&;#63; The Wayfarer trait has been a fan favorite in Remnant 2‚ offering players an increase in traversal speed including climbing up ladders‚ vaulting over barricades‚ etc. With the recent release of The Forgotten Kingdom DLC‚ alongside it came a long list of patch notes. The patch notes mention the Wayfarer trait has now been combined with the Swiftness trait. Originally‚ Swiftness only increased movement speed such as sprinting and dodging. The Swiftness trait will now include Wayfarer’s effects‚ increasing traversal speed. Below is the progression path for the Swiftness ...

Another grenade launcher enters the game&;#33; Here is the fastest way to complete the Patience and Forbearance quest in Destiny 2: Into the Light. Destiny 2: Fastest way to complete the Patience and Forbearance quest Let’s be honest‚ we have seen a decent amount of iterations of the Forbearance‚ but since we can’t have “too many” of those‚ we now have the Brave version of this grenade launcher‚ which is historically one of the most used grenade launchers in the game. Along the Hammerhead‚ the Forbearance launched as part of the third wave of Into the Light content for Destiny 2‚ and its quest – Patience and Forbearance – will have you complete one of the two objectives below: Rapidly defeat combatants using Breech-Loaded Grenade Launchers anywhere in the system. Bonus progress for rapid final blows in Onslaught. Defeat combatants in raids or dungeons using Grenade Launchers. Screenshot: PC Invasion Now‚ this isn’t the first time...

Richard Dawson is best known for hosting the popular game show Family Feud from 1976 until 1985 as well as for another season between 1994 and 1995. The British-born actor also starred on the sitcom Hogan's Heroes before launching his career as a game show staple. While today his open fondness for female contestants would be frowned upon‚ in his time Dawson's actions were largely accepted by many... Source

California’s electric vehicle agenda will require costly upgrades to the state’s electric grid infrastructure if it is to be realized‚ according to a new study published in the scientific journal Proceedings of the National Academy of Sciences. The state‚ often heralded as a national leader when it comes to EVs‚ is set to ban the sale of purely gas-powered passenger vehicles in the state after 2035 and heavy-duty trucks that burn fossil fuels starting in 2036. The infrastructure upgrades reportedly needed to support the projected rise of EVs in the state could cost anywhere between $6 billion and $20 billion‚ according to the study. The study identifies “feeders‚” or transmission lines that carry electricity from the site of generation to its end user‚ as a key type of infrastructure that needs extensive upgrades by 2045 in order to meet targets set by California’s aggressive EV policies. There is a “substantial need” for 50% of all feeders in the state to receive upgrades by 2035‚ and for 67% of feeders by 2045‚ according to the study. The state will also need to increase the amount of energy that it is able to distribute by about 25 gigawatts (GW) by 2045 to meet demand for public and private EV charging stations—upgrades that will cost anywhere between $6 billion and $20 billion‚ the study states. But it takes nearly 2.5 million solar panels or 310 utility-scale wind turbines to produce just 1 GW of power‚ according to the Department of Energy. “The imminent challenges confronting California serve as a microcosm of the forthcoming obstacles anticipated worldwide due to the prevailing global trend of EV adoption‚” the study states. California is also expecting to continue its advance toward its goal of having 100% zero-emissions power generation by 2045. The state figures to rely heavily on wind and solar power to meet that target‚ given that the state’s sole major nuclear power plant may have to close for good after its five-year life span extension granted by state regulators expires. While the state is changing how it sources electricity over time and adding demand with policies like those pushing EVs‚ the study’s authors project that electricity demand growth will actually drive down electricity costs in the state over time. California had the second-highest cost of electricity per unit of any state in the continental U.S. in January‚ trailing only Rhode Island‚ according to data from the U.S. Energy Information Administration. The office of Democratic California Gov. Gavin Newsom and the California Energy Commission did not respond immediately to requests for comment. Originally published by the Daily Caller News Foundation The post California’s EV Agenda Will Require Massive And Costly Infrastructure Upgrades‚ Analysis Finds appeared first on The Daily Signal.

There's never a dull moment in the sports realm. Hollywood knows this‚ and that's why audiences are always gifted with spectacular sports films. Remember the Titans‚ Glory Road‚ and many more have touched the hearts of fans globally. Whether it's the underlying message in the movie or the chills you receive from the captivating drama‚ this genre is sure to have you invested. Things are even better... Source

Hearing a tiny buzz in your ear could be a sign that a mosquito is nearby. These pesky critters tend to come around during warm weather and aren't afraid to bite. In order to prevent mosquitoes from spreading viruses to humans and animals‚ people can use certain plants to repel them. Lavender is considered to be one of the most soothing scents and is often used in essential oils. Source

Trump Should Ignore Gag Order

The venerable Hubble Space Telescope is like a gift that keeps on giving. Not only is it still making astronomical discoveries after more than thirty years in operation. It is also making discoveries by accident&;#33; Thanks to an international team of citizen scientists‚ with the help of astronomers from the European Space Agency (ESA) and some machine learning algorithms‚ a new sample of over one thousand asteroids has been identified in Hubble‘s archival data. The methods used represent a new approach for finding objects in decades-old data that could be applied to other datasets as well. The research team was led by Pablo Garc&;iacute;a-Mart&;iacute;n‚ a researcher with the Department of Theoretical Physics at the Autonomous University of Madrid (UAM). It included members from the ESA‚ NASA’s Jet Propulsion Laboratory (JPL)‚ the Astronomical Institute of the Romanian Academy‚ the University of Craiova‚ the Universit&;eacute; C&;ocirc;te d’Azur‚ and Bastion Technologies. The paper that describes their findings‚ “Hubble Asteroid Hunter III. Physical properties of newly found asteroids‚” recently appeared in Astronomy &; Astrophysics. Ask any astronomers and they will tell you that asteroids are material left over from the formation of the Solar System ca. 4.5 billion years ago. These objects come in many shapes in sizes‚ ranging from peddle-sized rocks to planetoids. Observing these objects is challenging since they are faint and constantly in motion as they orbit the Sun. Because of its rapid geocentric orbit‚ Hubble can capture wandering asteroids thanks to the distinct curved trails they leave in Hubble exposures. As Hubble orbits Earth‚ its point of view changes while observing asteroids following their orbits. Hubble image of the barred spiral galaxy UGC 12158‚ with streaks left by photobombing asteroids. Credit: NASA‚ ESA‚ P. G. Mart&;iacute;n (AUM)/J. DePasquale (STScI)/A. Filippenko (UC Berkeley) Asteroids have also been known to “photobomb” images acquired by Hubble of distant cosmic objects like UGC 12158 (see image above). By knowing Hubble’s position when it took exposures of asteroids and measuring the curvature of the streaks they leave‚ scientists can determine the asteroids’ distances and estimate the shapes of their orbits. The ability to do this with large samples allows astronomers to test theories about Main Asteroid Belt formation and evolution. As Martin said in a recent ESA Hubble press release: “We are getting deeper into seeing the smaller population of main-belt asteroids. We were surprised to see such a large number of candidate objects. There was some hint that this population existed‚ but now we are confirming it with a random asteroid population sample obtained using the whole Hubble archive. This is important for providing insights into the evolutionary models of our Solar System.” According to one widely accepted model‚ small asteroids are fragments of larger asteroids that have been colliding and grinding each other down over billions of years. A competing theory states that small bodies formed as they appear today billions of years ago and have not changed much since. However‚ astronomers can offer no plausible mechanism for why these smaller asteroids would not accumulate more dust from the circumstellar disk surrounding our Sun billions of years ago (from which the planets formed). In addition‚ astronomers have known for some time that collisions would have left a certain signature that could be used to test the current Main Belt population. In 2019‚ astronomers from the European Science and Technology Centre (ESTEC) and the European Space Astronomy Center’s Science Data Center (ESDC) came together with the world’s largest and most popular citizen-science platform (Zooniverse) and Google to launch the citizen-science project Hubble Asteroid Hunter (HAH) to identify asteroids in archival Hubble data. This graph is based on Hubble Space Telescope archival data that were used to identify a largely unseen population of very small asteroids. Credit: NASA/ESA/P. G. Mart&;iacute;n (AUM)/E. Wheatley (STScI) The HAH team comprised 11‚482 citizen-science volunteers who perused 37‚000 Hubble images spanning 19 years. After providing nearly two million identifications‚ the team was given a training set for an automated algorithm to identify asteroids based on machine learning. This yielded 1‚701 asteroid trails‚ with 1‚031 corresponding to previously uncatalogued asteroids – about 400 of which were below 1 km (~1090 ft) in size. Said Martin: “Asteroid positions change with time‚ and therefore you cannot find them just by entering coordinates‚ because they might not be there at different times. As astronomers we don’t have time to go looking through all the asteroid images. So we got the idea to collaborate with more than 10‚000 citizen-science volunteers to peruse the huge Hubble archives.” This pioneering approach may be effectively applied to datasets accumulated by other asteroid-hunting observatories‚ such as NASA’s Spitzer Space Telescope and Stratospheric Observatory for Infrared Astronomy (SOFIA). Once the James Webb Space Telescope (JWST) has accumulated a large enough dataset‚ the same method could also be applied to its archival data. As a next step‚ the HAH project will examine the streaks of previously unknown asteroids to characterize their orbits‚ rotation periods‚ and other properties. Further Reading: ESA Hubble‚ Astronomy &; Astrophysics The post Hubble Has Accidentally Discovered Over a Thousand Asteroids appeared first on Universe Today.

Planetary nebula are some of nature’s most stunning visual displays. The name is confusing since they’re the remains of stars‚ not planets. But that doesn’t detract from their status as objects of captivating beauty and intense scientific study. Like all planetary nebula‚ the Southern Ring Nebula is the remnant of a star like our Sun. As these stars age‚ they will eventually become red giants‚ expanding and shedding layers of gas out into space. Eventually‚ the red giant becomes a white dwarf‚ a stellar remnant bereft of fusion that emanates whatever residual thermal energy it has without ever generating anymore. The white dwarf lights up the shells of gas expelled earlier‚ and we get to enjoy the show. When the long-awaited JWST started delivering images‚ the Southern Ring Nebula (NGC 3132) was one of its first targets. It was one of five objects that made up the telescope’s first science results. The JWST’s images revealed something surprising about NGC 3132: it has two stars. The white dwarf is in the center of NGC 3132 and its companion is between 40 to 60 AU away‚ about the same distance as Pluto is from the Sun. Researchers wanted to understand more about the Southern Ring Nebula’s structure. The JWST works in the infrared and can image warm hydrogen in the nebula. But to get a more complete image of the nebula‚ a team of researchers from the Rochester Institute of Technology (RIT) turned to the Submillimeter Array (SMA). The SMA can sense the cooler CO (carbon monoxide) in the nebula beyond the JWST’s reach. It sensed CO’s presence and measured its velocity and the velocities of other molecules. The research is published in The Astrophysical Journal titled “The Molecular Exoskeleton of the Ring-like Planetary Nebula NGC 3132.” Professor Joel Kastner from the RIT School of Physics and Astronomy is the lead author. The new observations showed that most of the nebula’s hydrogen gas is in a large expanding ring and that a second expanding ring lies almost perpendicular to the first. “JWST showed us the molecules of hydrogen and how they stack up in the sky‚ while the Submillimeter Array shows us the carbon monoxide that is colder that you can’t see in the JWST image‚” explained Kastner. This figure from the study shows the velocities of three molecules in NGC 3132 as measured by the SMA. From left to right: 12CO‚ 13CO‚ and CN (cyanide.) The images clearly show the primary ring in the nebula. Image Credit: Kastner et al. 2024. “The extra velocity dimension from the array’s radio wavelength observations then effectively allows us to see the nebula in 3-D. When we started to turn the whole nebula around in 3-D‚ we immediately saw it really was a ring‚ and then we were amazed to see there was another ring‚” Kastner said. “Surprisingly‚ the data further reveal that the nebula also appears to harbor a second‚ dust-rich molecular ring (Ring 2)—detected in (dust) absorption‚ in low-excitation emission lines‚ in H2‚ and (now) in 12CO(2–1)—that appears to lie nearly perpendicular to Ring 1‚” the authors explain in their published research. This figure from the study shows the SMA observations of NGC 3132 in the left column and the JWST infrared image in the right column. The bottom images show the different velocities of molecules in the nebula. The light blue velocity shows the presence of the main ring‚ but the red and pink high-velocity clumps show the presence of a second ring. Image Credit: Kastner et al. 2024. The rings are offset from one another‚ which explains why the 3D view made the second one more visible. The team matched their observations to a geometric model that showed inclinations of 45° for Ring 1 and 78° for Ring 2. These panels from the published research show the two rings around NGC 3132. The left panel shows the rings with a 45° for Ring 1 and 78° for Ring 2. The right panel shows the two rings with a 15° for Ring 1. Image Credit: Kastner et al. 2024. Why does the Southern Ring Nebula have two offset rings&;#63; The authors say we have a pole-on view of a bipolar nebula shaped by the presence of a second star. There are many bipolar nebulae‚ including well-known ones like the Butterfly Nebula. The Butterfly Nebula as imaged by the Hubble Space Telescope. Image Credit: By NASA‚ ESA and the Hubble SM4 ERO Team – http://www.hubblesite.org/newscenter/archive/releases/2009/25/image/f/‚ Public Domain‚ https://commons.wikimedia.org/w/index.php&;#63;curid=7777740 However‚ the presence of a second star has complicated NGC 3132’s shape. “We suggest that this apparent two-ring structure may be the remnant of an ellipsoidal molecular envelope of AGB ejecta that has been mostly dispersed by a series of rapid-fire but misaligned collimated outflows or jets‚” the authors explain in their research. “Such a scenario would be consistent with the hypothesis that the mass-losing AGB progenitor of NGC 3132 was a member of an interacting triple star system.” It would be consistent‚ but the authors say there’s no way to conclude that a third star was involved with current research. “Detailed simulations of the dynamical effects of such multiple-star toppling jets systems on AGB molecular envelopes are required to test this speculative scenario for the shaping of the molecular exoskeleton of NGC 3132‚” the authors explain. The presence of all that molecular gas in the nebula surprised scientists. The intense UV from the white dwarf should break up the carbon monoxide and the molecular hydrogen. But it hasn’t. “Where does the carbon and the oxygen and the nitrogen in the universe come from&;#63;” said Kastner. “We’re seeing it generated in the sun-like stars that are dying‚ like the star that’s just died and created the Southern Ring. A lot of that molecular gas could wind up in planetary atmospheres and atmospheres can enable life.” The post See the Southern Ring Nebula in 3D appeared first on Universe Today.

Astrobiologists continue to work towards determining which biosignatures might be best to look for when searching for life on other worlds. The most common idea has been to search for evidence of plants that use the green pigment chlorophyll‚ like we have on Earth. However‚ a new paper suggests that bacteria with purple pigments could flourish under a broader range of environments than their green cousins. That means current and next-generation telescopes should be looking for the emissions of purple lifeforms. “Purple bacteria can thrive under a wide range of conditions‚ making it one of the primary contenders for life that could dominate a variety of worlds‚” said L&;iacute;gia Fonseca Coelho‚ a postdoctoral associate at the Carl Sagan Institute (CSI) and first author of “Purple is the New Green: Biopigments and Spectra of Earth-like Purple Worlds‚” published in the Monthly Notices of the Royal Astronomical Society: Letters. Artist’s concept of Earth-like exoplanets‚ which strikes the careful balance between water and landmass. Credit: NASA According to NASA’s Exoplanet Archive‚ 5612 extrasolar planets have been found so far‚ as of this writing‚ and another 10‚000 more are considered planetary candidates‚ but have not yet been confirmed. Of all those‚ there are just over 30 potentially Earth-like worlds‚ planets that lie in their stars’ habitable zones where conditions are conducive to the existence of liquid water on surface. But Earth-like has a broad meaning‚ ranging from size‚ mass‚ composition‚ and various chemical makeups. While being within a star’s habitable zone certainly means there’s the potential for life‚ it doesn’t necessarily mean that life could have emerged there‚ or even if it did‚ the life on that world might look very different from Earth. “While oxygenic photosynthesis gives rise to modern green landscapes‚ bacteriochlorophyll-based anoxygenic phototrophs can also colour their habitats and could dominate a much wider range of environments on Earth-like exoplanets‚” Coelho and team wrote in their paper. “While oxygenic photosynthesis gives rise to modern green landscapes‚ bacteriochlorophyll-based anoxygenic phototrophs can also colour their habitats and could dominate a much wider range of environments on Earth-like exoplanets.” The researchers characterized the reflectance spectra of a collection of purple sulfur and purple non-sulfur bacteria from a variety of anoxic and oxic environments found here on Earth in a variety of environments‚ from shallow waters‚ coasts and marshes to deep-sea hydrothermal vents. Even though these are collectively referred to as “purple” bacteria‚ they actually include a range of colors from yellow‚ orange‚ brown and red due to pigments  — such as those that make tomatoes red and carrots orange. These bacteria thrive on low-energy red or infrared light using simpler photosynthesis systems utilizing forms of chlorophyll that absorb infrared and don’t make oxygen. They are likely to have been prevalent on early Earth before the advent of plant-type photosynthesis‚ the researchers said‚ and could be particularly well-suited to planets that circle cooler red dwarf stars – the most common type in our galaxy. A collection of bacteria samples in the Cornell University Space Sciences Building. Ryan Young/Cornell University. That means this type of bacteria might be more prevalent on more and a wider variety of exo-worlds. On a world where these bacteria might be dominant‚ it would produce a distinctive “light fingerprint” detectable by future telescopes. In their paper‚ Coelho and team presented models for Earth-like planets where purple bacteria might dominate the surface and show the impact of their signatures on the reflectance spectra of terrestrial exoplanets. “Our research provides a new resource to guide the detection of purple bacteria and improves our chances of detecting life on exoplanets with upcoming telescopes‚” the team wrote. “We need to create a database for signs of life to make sure our telescopes don’t miss life if it happens not to look exactly like what we encounter around us every day‚” said co-author Lisa Kaltenegger‚ CSI director and associate professor of astronomy at Cornell University‚ in a press release from Cornell. The post Purple Bacteria — Not Green Plants — Might Be the Strongest Indication of Life appeared first on Universe Today.