Friday, August 29, 2025

NASA’s New SPHEREx Mission Observes Interstellar Comet - UNIVERSE

Comet 3I/ATLAS

Cataloguing the journey of comet 3I/ATLAS through the solar system. Because the object comes from outside our solar system, it is just passing through – so we use all the tools at our disposal to observe it before it disappears back into the cosmic dark. A host of NASA missions are coming together to observe this interstellar object, which was first discovered in summer 2025, before it leaves forever. While the comet poses no threat to Earth, NASA’s space telescopes help support the agency's ongoing mission to find, track, and better understand solar system objects.

NASA/SPHEREx

NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observed interstellar comet 3I/ATLAS Aug. 7 to Aug. 15. The SPHEREx team has been analyzing insights from this data, and a research note is available online. The agency’s SPHEREx is one of NASA’s space telescopes observing this comet, together providing more information about its size, physical properties, and chemical makeup. For example, NASA’s Webb and Hubble space telescopes also recently observed the comet. While the comet poses no threat to Earth, NASA’s space telescopes help support the agency’s ongoing mission to find, track, and better understand solar system objects.


NASA/SPHEREx

Alise Fisher
NASA Headquarters, Washington

Source: NASA’s New SPHEREx Mission Observes Interstellar Comet - NASA Science

Can large language models figure out the real world? New metric measures AI's predictive power - Computer Sciences - Machine learning & AI

In the 17th century, German astronomer Johannes Kepler figured out the laws of motion that made it possible to accurately predict where our solar system's planets would appear in the sky as they orbit the sun. But it wasn't until decades later, when Isaac Newton formulated the universal laws of gravitation, that the underlying principles were understood.

Although they were inspired by Kepler's laws, they went much further, and made it possible to apply the same formulas to everything from the trajectory of a cannon ball to the way the moon's pull controls the tides on Earth—or how to launch a satellite from Earth to the surface of the moon or planets.

Today's sophisticated artificial intelligence systems have gotten very good at making the kind of specific predictions that resemble Kepler's orbit predictions. But do they know why these predictions work, with the kind of deep understanding that comes from basic principles like Newton's laws?

As the world grows ever-more dependent on these kinds of AI systems, researchers are struggling to try to measure just how they do what they do, and how deep their understanding of the real world actually is.

Now, researchers in MIT's Laboratory for Information and Decision Systems (LIDS) and at Harvard University have devised a new approach to assessing how deeply these predictive systems understand their subject matter, and whether they can apply knowledge from one domain to a slightly different one. And by and large, the answer at this point, in the examples they studied, is—not so much.

The findings were presented at the International Conference on Machine Learning (ICML 2025), in Vancouver, British Columbia, last month by Harvard postdoc Keyon Vafa, MIT graduate student in electrical engineering and computer science and LIDS affiliate Peter G. Chang, MIT assistant professor and LIDS principal investigator Ashesh Rambachan, and MIT professor, LIDS principal investigator, and senior author Sendhil Mullainathan.

"Humans all the time have been able to make this transition from good predictions to world models," says Vafa, the study's lead author. So the question their team was addressing was, "Have foundation models—has AI—been able to make that leap from predictions to world models? And we're not asking are they capable, or can they, or will they. It's just, have they done it so far?" he says.

"We know how to test whether an algorithm predicts well. But what we need is a way to test for whether it has understood well," says Mullainathan, the Peter de Florez Professor with dual appointments in the MIT departments of Economics and Electrical Engineering and Computer Science and the senior author on the study. "Even defining what understanding means was a challenge."

In the Kepler versus Newton analogy, Vafa says, "They both had models that worked really well on one task, and that worked essentially the same way on that task. What Newton offered was ideas that were able to generalize to new tasks." That capability, when applied to the predictions made by various AI systems, would entail having it develop a world model so it can "transcend the task that you're working on and be able to generalize to new kinds of problems and paradigms."

Another analogy that helps to illustrate the point is the difference between centuries of accumulated knowledge of how to selectively breed crops and animals, versus Gregor Mendel's insight into the underlying laws of genetic inheritance.

"There is a lot of excitement in the field about using foundation models to not just perform tasks, but to learn something about the world," for example, in the natural sciences, he says. "It would need to adapt, have a world model to adapt to any possible task."

Are AI systems anywhere near the ability to reach such generalizations? To test the question, the team looked at different examples of predictive AI systems, at different levels of complexity. On the very simplest of examples, the systems succeeded in creating a realistic model of the simulated system, but as the examples got more complex, that ability faded fast.

The team developed a new metric, a way of measuring quantitatively how well a system approximates real-world conditions. They call the measurement inductive bias—that is, a tendency or bias toward responses that reflect reality, based on inferences developed from looking at vast amounts of data on specific cases.

The simplest level of examples they looked at was known as a lattice model. In a one-dimensional lattice, something can move only along a line. Vafa compares it to a frog jumping between lily pads in a row. As the frog jumps or sits, it calls out what it's doing—right, left, or stay. If it reaches the last lily pad in the row, it can only stay or go back. If someone, or an AI system, can just hear the calls, without knowing anything about the number of lily pads, can it figure out the configuration?

The answer is yes: Predictive models do well at reconstructing the "world" in such a simple case. But even with lattices, as you increase the number of dimensions, the systems no longer can make that leap.

"For example, in a two-state or three-state lattice, we showed that the model does have a pretty good inductive bias toward the actual state," says Chang. "But as we increase the number of states, then it starts to have a divergence from real-world models."

A more complex problem is a system that can play the board game Othello, which involves players alternately placing black or white disks on a grid. The AI models can accurately predict what moves are allowable at a given point, but it turns out they do badly at inferring what the overall arrangement of pieces on the board is, including ones that are currently blocked from play.

The team then looked at five different categories of predictive models actually in use, and again, the more complex the systems involved, the more poorly the predictive modes performed at matching the true underlying world model.

With this new metric of inductive bias, "our hope is to provide a kind of test bed where you can evaluate different models, different training approaches, on problems where we know what the true world model is," Vafa says. If it performs well on these cases where we already know the underlying reality, then we can have greater faith that its predictions may be useful even in cases "where we don't really know what the truth is," he says.

People are already trying to use these kinds of predictive AI systems to aid in scientific discovery, including such things as properties of chemical compounds that have never actually been created, or of potential pharmaceutical compounds, or for predicting the folding behavior and properties of unknown protein molecules. "For the more realistic problems," Vafa says, "even for something like basic mechanics, we found that there seems to be a long way to go."

Chang says, "There's been a lot of hype around foundation models, where people are trying to build domain-specific foundation models—biology-based foundation models, physics-based foundation models, robotics foundation models, foundation models for other types of domains where people have been collecting a ton of data" and training these models to make predictions, "and then hoping that it acquires some knowledge of the domain itself, to be used for other downstream tasks."

This work shows there's a long way to go, but it also helps to show a path forward. "Our paper suggests that we can apply our metrics to evaluate how much the representation is learning, so that we can come up with better ways of training foundation models, or at least evaluate the models that we're training currently," Chang says. "As an engineering field, once we have a metric for something, people are really, really good at optimizing that metric." 

Source: Can large language models figure out the real world? New metric measures AI's predictive power   

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Thursday, August 28, 2025

Astronomers Map Stellar ‘Polka Dots’ Using NASA’s TESS, Kepler - UNIVERSE

Scientists have devised a new method for mapping the spottiness of distant stars by using observations from NASA missions of orbiting planets crossing their stars’ faces. The model builds on a technique researchers have used for decades to study star spots.

By improving astronomers’ understanding of spotty stars, the new model — called StarryStarryProcess — can help discover more about planetary atmospheres and potential habitability using data from telescopes like NASA’s upcoming Pandora mission.

“Many of the models researchers use to analyze data from exoplanets, or worlds beyond our solar system, assume that stars are uniformly bright disks,” said Sabina Sagynbayeva, a graduate student at Stony Brook University in New York. “But we know just by looking at our own Sun that stars are more complicated than that. Modeling complexity can be difficult, but our approach gives astronomers an idea of how many spots a star might have, where they are located, and how bright or dark they are.”

A paper describing StarryStarryProcess, led by Sagynbayeva, published Monday, August 25, in The Astrophysical Journal.

Watch to learn how a new tool uses data from exoplanets, worlds beyond our solar system, to tell us about their polka-dotted stars.
NASA’s Goddard Space Flight Center

NASA’s TESS (Transiting Exoplanet Survey Satellite) and now-retired Kepler Space Telescope were designed to identify planets using transits, dips in stellar brightness caused when a planet passes in front of its star.

These measurements reveal how the star’s light varies with time during each transit, and astronomers can arrange them in a plot astronomers call a light curve. Typically, a transit light curve traces a smooth sweep down as the planet starts passing in front of the star’s face. It reaches a minimum brightness when the world is fully in front of the star and then rises smoothly as the planet exits and the transit ends.  

By measuring the time between transits, scientists can determine how far the planet lies from its star and estimate its surface temperature. The amount of missing light from the star during a transit can reveal the planet’s size, which can hint at its composition.

Every now and then, though, a planet’s light curve appears more complicated, with smaller dips and peaks added to the main arc. Scientists think these represent dark surface features akin to sunspots seen on our own Sun — star spots.

The Sun’s total number of sunspots varies as it goes through its 11-year solar cycle. Scientists use them to determine and predict the progress of that cycle as well as outbreaks of solar activity that could affect us here on Earth.

Similarly, star spots are cool, dark, temporary patches on a stellar surface whose sizes and numbers change over time. Their variability impacts what astronomers can learn about transiting planets.

Scientists have previously analyzed transit light curves from exoplanets and their host stars to look at the smaller dips and peaks. This helps determine the host star’s properties, such as its overall level of spottiness, inclination angle of the planet’s orbit, the tilt of the star’s spin compared to our line of sight, and other factors. Sagynbayeva’s model uses light curves that include not only transit information, but also the rotation of the star itself to provide even more detailed information about these stellar properties.

This artist’s concept illustrates the varying brightness of star with a transiting planet and several star spots.

NASA’s Goddard Space Flight Center

“Knowing more about the star in turn helps us learn even more about the planet, like a feedback loop,” said co-author Brett Morris, a senior software engineer at the Space Telescope Science Institute in Baltimore. “For example, at cool enough temperatures, stars can have water vapor in their atmospheres. If we want to look for water in the atmospheres of planets around those stars — a key indicator of habitability — we better be very sure that we’re not confusing the two.”

To test their model, Sagynbayeva and her team looked at transits from a planet called TOI 3884 b, located around 141 light-years away in the northern constellation Virgo.

Discovered by TESS in 2022, astronomers think the planet is a gas giant about five times bigger than Earth and 32 times its mass.

The StarryStarryProcess analysis suggests that the planet’s cool, dim star — called TOI 3384 — has concentrations of spots at its north pole, which also tips toward Earth so that the planet passes over the pole from our perspective.

Currently, the only available data sets that can be fit by Sagynbayeva’s model are in visible light, which excludes infrared observations taken by NASA’s James Webb Space Telescope. But NASA’s upcoming Pandora mission will benefit from tools like this one. Pandora, a small satellite developed through NASA’s Astrophysics Pioneers Program, will study the atmospheres of exoplanets and the activity of their host stars with long-duration multiwavelength observations. The Pandora mission’s goal is to determine how the properties of a star’s light differs when it passes through a planet’s atmosphere so scientists can better measure those atmospheres using Webb and other missions.

“The TESS satellite has discovered thousands of planets since it launched in 2018,” said Allison Youngblood, TESS project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “While Pandora will study about 20 worlds, it will advance our ability to pick out which signals come from stars and which come from planets. The more we understand the individual parts of a planetary system, the better we understand the whole — and our own.”

By Jeanette Kazmierczak
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Source: Astronomers Map Stellar ‘Polka Dots’ Using NASA’s TESS, Kepler - NASA Science

Zoo populations may hold key to saving Pacific pocket mouse - Biology Plants & Animals - Ecology

Endangered Pacific pocket mice, native to Southern California, were once thought to be extinct until a tiny remnant population was rediscovered in the mid-1990s.

San Diego Zoo Wildlife Alliance established a conservation breeding and reintroduction program to save the species from extinction. Though there has been significant success with breeding and reintroduction, the species is still at risk of losing genetic diversity, which reduces its survival and reproduction.

In a study published in Science, San Diego Zoo Wildlife Alliance researchers demonstrate how genetic rescue can be used as an effective strategy for the conservation of this species. This strategy includes introducing Pacific pocket mice from genetically distinct populations for breeding purposes to boost genetic diversity and, in turn, the health of the population.

The research findings provide a contrast to commonly held perceptions about the risks of outbreeding depression that currently limit the use of genetic rescue in conservation programs.

"When species are restricted to small, isolated populations, genetic erosion can lead to poor health. Our study examined the trade-offs between genetic erosion and outbreeding depression in Pacific pocket mice, and we find that the benefits of genetic rescue outweigh the risks of keeping these populations in isolation," said lead author, Aryn Wilder, San Diego Zoo Wildlife Alliance Conservation Genetics researcher. 


The researchers suggest shifting the focus from maintaining the genetic uniqueness of populations to maximizing the genetic health of the species. They also highlight the important role that zoos and managed care facilities play in preventing species extinction.

"Erosion in diversity seen in wild populations was reversed when we mixed mice from different populations," said Wilder.

"The genetically healthier population had higher survival and reproductive success. Although different numbers of chromosomes carried by the mice from different populations increase the risk of incompatibilities in the mixed breeding program, the non-mixed mice have even lower fitness, indicating a greater risk of extinction if the populations remain isolated."

San Diego Zoo Wildlife Alliance researchers have been studying the factors, including genomic variation, that maximize the health of populations and ensure the successful production of the fittest offspring for release into the wild. San Diego Zoo Wildlife Alliance brought in 49 mice from the wild and produced more than 700 mice at its facility, including 94 births last year.

In 2024, San Diego Zoo Wildlife Alliance and partners also began releasing Pacific pocket mice to a second site, resulting in 100 pups born in the wild at that site.

With two-thirds of Earth's species undergoing population decline, the implications of this research extend beyond Pacific pocket mice and demonstrate the value of genetic rescue for species facing extinction. It also highlights how zoos can serve a vital role in conservation of at-risk species. 

Source: Zoo populations may hold key to saving Pacific pocket mouse  

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