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Ancient Martian valley holds major clues to a past ocean

New images of Shalbatana Vallis from ESA’s Mars Express orbiter reveal well-preserved geological clues of past water and lava activity on ancient Mars. [ https://www.labroots.com/trending/space/30564/ancient-martia…st-ocean-2](https://www.labroots.com/trending/space/30564/ancient-martia…st-ocean-2)


How much water and lava flowed across the surface of Mars billions of years ago? This is what a recent image obtained from the European Space Agency’s Mars Express orbiter hopes to figure out as the more than two-decade-old orbiter captured incredible images that could help researchers piece together the environment on ancient Mars. This is because these images offer clues of past water and lava activity on Mars when the Red Planet was far warmer and wetter than it is today.

This latest image reveals a vast area comprised of a mixture of buried and visible impact craters, eroded hills and mesas, wrinkle ridges from lava cooling and contracting, chaotic terrain from the melting of ice, dark volcanic ash, and a massive channel called Shalbatana Vallis where researchers hypothesize was craved from massive amounts of groundwater that swelled up to the Martian surface. Because Mars lack plate tectonics like Earth, these landforms have been well-preserved for billions of years. Once Mars became incapable of having liquid water on its surface, the Martian wind and dust buried and eroded some of these features, though not to the extent as we see erosion on Earth.

Vast announces line of high-power satellite buses

WASHINGTON — Commercial space station developer Vast is moving into satellite manufacturing with a line of high-power satellite buses.

The company announced May 19 Vast Satellite, a product line that uses the technologies Vast developed for commercial space stations to make satellite buses designed for applications ranging from broadband communications to orbital data centers.

The first product is a bus that provides 15 kilowatts of power. The flat-panel bus, with primary dimensions of 2.2 by 3.6 meters, has a dry mass of 700 kilograms and can host payloads of at least 350 kilograms. Designed for initial use in low Earth orbit, the bus has an electric propulsion system that provides more than 500 meters per second of delta-v, or change in velocity.

Tailored drinks could provide space nutrition

Researchers have developed customizable omega-3 nanoemulsion drinks to protect astronauts’ bones and muscles from space radiation. [ https://www.labroots.com/trending/space/30563/tailored-drink…utrition-2](https://www.labroots.com/trending/space/30563/tailored-drink…utrition-2)


How could customizable drinks help provide astronauts on future, long-term space missions with the proper levels of nutrition? This is what a recent study published in ACS Food Science & Technology hopes to address as a team of researchers investigated novel methods for improving future astronaut diets. This study has the potential to help scientists, mission planners, and astronauts develop improved dietary plans, specifically as space mission durations are aimed to increase in the coming years.

For the study, the researchers introduced beverage nanoemulsion drinks, with emulsion drinks being a common drink that typically consists of a blended mixture of two normally non-mixable substances like an oily substance and watery substance with microscopic droplets within the liquid since they don’t full mix together. In this case, the researchers propose nanoemulsion drinks with even smaller droplets and consist of water and Omega-3 fatty acids (fish oil), which provide bone and muscle protection against space radiation.

In the end, the researchers found that customizable drinks with a variety of sweetness levels and flavors are the best options. Going forward, the researchers aspire to test the tastiness of the beverages under microgravity conditions, as they note the drinks taste like typical flat sodas after carbonation loss.

New lithium-plasma engine passes key Mars propulsion test

You’re on the fourth human mission to Mars, and you’re told the Odyssey spacecraft designed to take you there will be the smoothest ride you’ll ever take. It features a newly christened electric propulsion engine which was in the late stages of testing during the first three missions. The mission starts and the spacecraft travels at a crawl, and you wonder if it’s broken. A week goes by and you’re now traveling at more than 400,000 kilometers (250,000 miles) per hour, and your mind is blown as to how fast you’re going, how quickly that happened, and that this mission might be more awesome than you thought.

This scenario is quite possibly a decade away, at minimum, but that’s not stopping the bright minds at NASA from building and testing next-generation propulsion systems designed to take humans to Mars one day and send spacecraft across the solar system. This is because NASA engineers recently tested a next-generation electric propulsion system that achieved new records while requiring lithium metal vapor for fuel and holds the potential to be a game changer in propulsion systems for the future of space exploration.

In a remarkable achievement, the tests successfully set a new record in the United States of 120 kilowatts of power, which is estimated to be 25 times greater than NASA’s Psyche spacecraft, which is currently en route to asteroid 16 Psyche and contains the most powerful electric thrusters ever built.

Dark lunar craters could host ultrastable lasers for moon navigation

They rank among the darkest and coldest places in the solar system: Hundreds of lunar craters, many of them at the moon’s south pole, never receive direct sunlight and lie in permanent shadow. That’s exactly why physicist Jun Ye and his colleagues suggest that these craters are the perfect place to build a critical component for an ultrastable laser.

On the moon, a highly stable laser—a source of coherent light that has a nearly unwavering frequency, or color—could provide a master time signal and offer GPS-like lunar navigation, said Ye, who is affiliated with both the National Institute of Standards and Technology (NIST) and JILA, a joint institute of NIST and the University of Colorado Boulder. Multiple copies of these lunar lasers could precisely measure the distances between objects and potentially detect exotic physics phenomena such as ripples in spacetime.

To construct a lunar laser, astronauts would first install a key component known as an optical silicon cavity —a block of silicon that permits only certain frequencies of light to bounce back and forth between mirrors on each end of the block. The distance between the two mirrors determines the frequencies that are allowed to resonate; for a highly stable optical cavity, that distance, and therefore those frequencies, does not vary.

Reanalyzed Hubble data challenges Europa plume claims

Dr. Kurt Retherford: “The new data has made us reconsider the strength of the previous paper’s conclusion regarding water vapor plumes.” [ https://www.labroots.com/trending/space/30560/reanalyzed-hub…e-claims-2](https://www.labroots.com/trending/space/30560/reanalyzed-hub…e-claims-2)


What can the vapor plumes on Jupiter’s moon Europa teach scientists about the small moon’s atmosphere? This is what a recent study published in Astronomy & Astrophysics hopes to address as a team of scientists investigated the origins of Europa’s vapor plumes. This study has the potential to help scientists better understand the geological activity occurring on Europa and how its subsurface ocean could influence the small moon’s fragile and thin atmosphere.

For the study, the researchers analyzed data obtained from NASA’s Hubble Space Telescope in 1999 and between 2012 and 2020 that displayed evidence of water vapor plumes from Europa and a hydrogen exosphere. An exosphere is the uppermost layer of an atmosphere and is where the atmosphere thins out and merges with the vacuum of space.

This study builds on a 2014 study published in Science from some of these same researchers that explored evidence of plume activity at Europa’s south pole. Now, this most recent study used a series of computer models to ascertain the accuracy of past Hubble data and from the 2014 study. In the end, the researchers discovered that while evidence of the hydrogen exosphere was present, evidence of water vapor plumes was not.

Generalization Dynamics of LM Pre-training

An AI has a limited amount of “capacity” (brainpower). Early in training, it develops quick, shallow circuits to memorize data because that’s the easiest way to get the right answer. Later, it develops complex circuits for actual reasoning. Because space is limited, these two internal systems are constantly competing for control. Whichever type of data the AI happens to be reading in a specific moment determines which circuit wins the battle.


People typically assume that LMs stably mature from pattern-matching parrots to generalizable intelligence during pre-training. We build a toy eval suite and show this mental model is wrong: throughout pre-training, LMs frequently and suddenly hop between parrot-like and intelligence-like modes, i.e. distinct algorithms implemented by distinct circuits. We call this mode-hopping. Across our suite, LMs can suddenly latch onto memorized or in-context patterns instead of in-context learning, use System 1 instead of System 2 thinking, pick up what sounds true instead of what is true, fail at multi-hop persona QA, out-of-context reasoning, and emergent misalignment — then just as suddenly revert and generalize. Mode-hopping is not explained by standard optimization dynamics: it is locally stable and can not be fixed by checkpoint averaging. We instead think of it as a capacity allocation problem: in a capacity-bounded model, generalizable circuits must compete with the shallow ones learned early in training, and the data in each pre-training window decides which circuits win. Our suite provides a cheap set of pre-training monitors and a new lens on generalization. Building upon our insights, we demonstrate three applications: (i) select intermediate pre-training checkpoints that strongly generalize reasoning and alignment, better than the final pre-or mid-training checkpoints, (ii) select pre-training data that controls and stabilizes generalization dynamics, and (iii) test prior generalization predictors, falsifying the monolithic belief that “simpler solutions generalize better”

Building general AI without generalization is doable but meh. We want an intelligence that learns deep, transferable structure, not a parrot that matches shallow patterns. Real generalization would unblock many today’s key open problems: data-efficient (online) learning, shortcut learning, transfer capabilities from verifiable domains (math, coding) to broader non-verifiable yet economically valuable domains, and maintain a coherent character that truly aligns with human values.

The distinction between parrots and intelligence is computational. Parrots repeat in-context patterns; intelligence infers in-context functions. Parrots encode a persona as bags of disconnected facts and traits; intelligence learns a shared persona representation that connects all. Parrots memorize reasoning steps; intelligence forms general reasoning circuits for entity tracking, backtracking, or even for highly abstract concepts like truth.

Designing in situ power stations for future Mars missions

You’re in the lab analyzing Martian regolith samples within your cozy Mars habitat serving on the fifth human mission to Mars. The power within the habitat has been flowing flawlessly thanks to the MARS-MES (Mars Atmospheric Resource & Multimodal Energy System), including the general habitat lighting, science lab, sleeping quarters, exercise equipment, the virtual reality headsets the crew use for rest & relaxation, oxygen and fuel generation, and water. All this from converting the Martian atmosphere into workable electricity.

While this scenario might be decades away, scientists on Earth are working hard to make this concept a reality today. This includes a team of scientists from China who propose using a novel concept for converting the thin Martian atmosphere into heat and electricity. Their findings were recently published in National Science Review and could help revolutionize how electricity is produced on Mars through a process called in situ resource utilization (ISRU) without the need for power or power supplies being shipped from Earth.

For the study, the researchers propose several concepts for producing power and electricity on a future human Mars mission, including Martian air capture, in situ power generation and storage, and life support resources transformation. The team notes all these methods carry their own benefits and challenges while emphasizing the importance of using ISRU for powering future human Mars missions.

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