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The Paranal solar ESPRESSO Telescope, a New Tool for Finding Exoplanets
The exoplanet census continues to grow at a prodigious rate, with 6,273 confirmed planets to date and close to 20,000 candidates awaiting confirmation. What’s more, the rate of discovery is accelerating, having passed 5,000 in early 2023 and 6,000 in September 2025. With such a large exoplanet census, along with improvements in instrumentation and data analysis, scientists are now focused on “exoplanet characterization” in addition to discovery. As always, the goal is to find planets that could be habitable for life as we know it (or “Earth-like”).
This is challenging, since Earth-like rocky planets are small compared to other classes (gas giants and super-Earths) and orbit closer to Sun-like stars, where they are subject to considerable “signal noise.” This challenge inspired an international team of astronomers to propose a dedicated facility called the Paranal solar ESPRESSO Telescope (PoET). This will collect solar light and channel it into the ESPRESSO spectrograph on the Very Large Telescope (VLT). This will aid astronomers by helping them identify the precise types of “noise” they need to comb through to find potential Earths.
The international team was led by Nuno C. Santos and his colleagues from the Institute of Astrophysics and Space Sciences (CAUP) and the University of Porto in Portugal. They were joined by researchers from similar institutes at the University of Lisbon, Coimbra, and the University of Geneva, as well as the European Southern Observatory (ESO), which operates the VLT and its Echelle SPectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO).
A Noise Problem
Of the more than 6,000 exoplanets confirmed to date, only 223 are terrestrial (rocky) planets. Of these, none orbit G-type main-sequence stars like our own and have mainly been found as part of systems orbiting low-mass, low-luminosity M-type stars (red dwarfs). This includes the closest exoplanet to the Solar System (Proxima b) and the seven rocky planets orbiting TRAPPIST-1. Nevertheless, scientists are confident that next-generation missions and instruments will make it easier to find Earth-like planets around G-type stars in the near future.
One of the most promising methods for detecting and characterizing exoplanets is high-resolution spectroscopy. This includes spectra obtained from an exoplanet’s atmosphere as it passes in front of its star relative to the observer (the Transit Method) and Doppler spectroscopy measurements of the stars themselves (the Radial Velocity Method). When combined, these methods provide constraints on an exoplanet’s size, mass, and mean density, which is vital to ascertaining its composition.
The greatest challenge to overcome is (as noted) the astrophysical ‘noise’ coming from the host stars, caused by sunspots, convective motions, oscillations, and magnetic activity. These produce variations in the observed line profiles and spectral positions, which can last for days or longer, depending on the star’s rotational period and long-term magnetic cycle. The convective pattern of plasma on a star’s surface (stellar granulation) is also a source of variability that can drown out signals.
To compensate for this interference, astronomers use different approaches to model the signals produced by these phenomena. But none have proven effective enough to correct RV time-series measurements required for the detection of Earth-like planets. The exoplanet science community has recognized that the processes driving stellar variability need to be identified in detail. This will allow astronomers to account for stellar noise and filter it from future signals, leaving signals generated by exoplanets intact.
Enter PoET
Since the goal is to find Earth-like planets orbiting Sun-like stars, the Sun is an ideal proxy, as it is the only one astronomers can fully resolve. Dedicated instruments with high-precision spectrographs have been developed to observe the “Sun-as-a-star,” such as the High Accuracy Radial velocity Planet Searcher North (HARPS-N) solar telescope and the HARPS spectrograph (HELIOS). The main drawback is that only disc-integrated spectra are obtained, precluding a detailed analysis of individual stellar features.
According to the team, what is needed is a telescope that can offer three vital things:
1. Spatially resolved spectroscopy with very high wavelength stability
2. Very high spectral resolution to adequately resolve photospheric line asymmetries
3. Extended wavelength coverage, for the simultaneous observation of thousands of spectral lines probing different physical conditions.
This, they claim, can be achieved by linking the ESPRESSO spectrograph to a solar telescope – in this case, PoET. The solar telescope will observe the Sun at different spatial scales, corresponding to sunspots and solar granules, and send the light it gathers to ESPRESSO via optical fibers. The overall system involves three telescopes, starting with the main telescope (MT) developed by Officina Stellare. This telescope has a Gregorian configuration, standard for solar observations, and will observe small areas of the solar disc.
Two additional telescopes, the “science” and “imaging” refractor instruments, act as the pointing telescope (PT) piggy-backed to the MT. The MT will also receive support from a custom instrument known as SHABAR (SHAdow BAnd Range), designed to measure random fluctuations in Earth’s atmosphere that cause refraction. The telescope is expected to be fully autonomous, with its operations overseen by PoET’s custom software.
*Illustration of the location of PoET in Paranal. Upper-right: Schematic of science fibers path from PoET to ESPRESSO (one floor below). Lower-Right: Dome concept with main telescope. Credit: ESO*
Early in April, PoET completed its test observations and gathered its “first light.” The observations showed that the system is working and can acquire spectra of the entire solar disc and specific areas of it. Over the next few weeks, the team will test and optimize the system before commencing scientific observations. Alain Smette, the VLT Operations Staff Astronomer and a co-author on the proposal paper, expressed great confidence in PoET’s ability to assist exoplanet studies. As he explained in a recent ESO press release:
It is a great advantage to have ESPRESSO working in this way. By switching from the VLT at night to PoET during the day, we maximize the usage of this instrument to help us find and characterize exoplanets. Thanks to the exceptional location of the Paranal Observatory, the number of available days when weather conditions are suitable for observations of the Sun is expected to be very similar to that for nighttime observations.
Further Reading: ESO
News
Subaru Telescope Reveals New Data on the Interior Composition of 3I/ATLAS
On Jan. 7th, 2026, the Subaru Telescope joined many of the world’s observatories and space telescopes in observing the 3I/ATLAS, the third interstellar object (ISO) detected in our Solar System. This interstellar comet had just completed its closest approach to the Sun, which produced more intense outgassing. By observing the light from 3I/ATLAS’ coma, astronomers were able to examine the chemical composition of the comet’s interior and produce estimates of the ratio of carbon dioxide to water.
Prior observations largely provided insight into the composition of its outer layers, which have been subject to billions of years of cosmic irradiation. As the Subaru team reported in a recent study published in The Astrophysical Journal, their results showed that the ratio of carbon dioxide to water was much lower than that inferred from previous observations by space telescopes, providing clues about the ISO’s structure and suggesting that the chemistry of the coma is evolving.
The research was led by Yoshiharu Shinnaka and a team from the Koyama Space Science Institute at Kyoto Sangyo University. They were joined by researchers from the Division of Science at Kyoto Sangyo University, the University of Occupational and Environmental Health, the National Astronomical Observatory of Japan (NAOJ), and Kyoto-based optical instrument manufacturer Photocross Co.
Comet 3I/ATLAS (C/2025 N1) has garnered much attention since it was first detected on June 1st, 2025, by the Asteroid Terrestrial-impact Last Alert System (ATLAS). As the third ISO detected it as it passed through the Solar System, scientists eagerly monitored this comet as it approached our Sun and made its closest approach. Unlike 1I/’Oumuamua, scientists had confirmed the detection of 3I/ATLAS four months prior to it reaching perihelion.
And unlike 2I/Borisov, 3I/ATLAS was much larger and brighter, allowing for greater scientific returns. For their analysis, the team applied analytical methods and expertise accumulated from decades of observing comets in the Solar System. Based on this, the team estimated the CO2-to-water ratio in the coma, which provided hints about the nucleus’s structure and composition. The ratio they detected was lower than that observed by the many space telescopes during the same period.
Since asteroids and comets are essentially material left over from the formation of planetary systems, their interior compositions provide information about the conditions in these systems at the time. By studying these objects, scientists can learn what conditions are like elsewhere in the galaxy without having to send missions there. As Shinnaka commented in a NOAJ press release, the methods he and his colleagues employed will enable even greater scientific returns when future telescopes observe future ISOs:
With the full-scale operation of survey telescopes in the coming years, many more interstellar objects are expected to be discovered. By applying the observational and analytical techniques we have developed through studies of Solar System comets to interstellar objects, we can now directly compare comets hailing from both inside and outside the Solar System and explore differences in their composition and evolution.
Through studies of such objects, we hope to gain a deeper understanding of how planetesimals and planets formed in a wide variety of stellar systems, including our own Solar System.
Further Reading: Subaru Telescope
News
A historic $200-million USC gift from Nvidia board member aims to transform AI education
USC has received a $200-million gift from a major Silicon Valley venture capitalist and university trustee to expand artificial intelligence across campus through faculty recruitment, marking one of the largest donations in the university’s history, officials announced Tuesday.
The gift — from Mark Stevens and his wife, Mary — will rename USC’s School of Advanced Computing as the USC Mark and Mary Stevens School of Computing and Artificial Intelligence and fund a campuswide effort to make USC a national center of AI scholarship, including in film and the arts. It is also a major, early win for USC President Beong-Soo Kim, who was appointed in February.
The Stevens gift is the latest in a surge of nine-figure AI-related donations to major universities. In April, the Michael and Susan Dell Foundation gave $750 million to the University of Texas at Austin for a new medical center, including AI initiatives in health. Last month, the University of Wisconsin-Madison also received $100 million in donations for a new College of Computing and Artificial Intelligence.
In an interview, Kim said the donation comes during “an incredibly significant period of time” because AI is moving quickly from technical labs into “nearly every corner” of society. USC, he said, is positioned to compete by applying the technology across fields where the university already has strengths.
“It’s that intersection between AI and these other fields that we think is a perfect fit for USC,” Kim said, adding that the goal is for the money to help the university use AI for “positive societal impact.”
Kim said the gift will help USC recruit “world class AI talent,” but not only researchers focused on AI development. The university is seeking scholars who can use AI to accelerate work in medicine, cybersecurity, national security, business, entertainment and other fields, he said.
The president did not disclose how many faculty or researchers could be hired but said the areas would include arts, social sciences, engineering, computing and health.
In health sciences, Kim pointed to USC research in regenerative medicine, neuroimaging and Alzheimer’s disease, saying AI is helping scientists understand disease at a cellular level and identify earlier interventions. He said one of the “biggest and most exciting” areas for AI will be “medical discovery and drug development.”
USC is also pitching AI as a creative tool, a sensitive claim in Los Angeles, where writers, actors, musicians and other workers have raised fears about automation. Kim said the School of Cinematic Arts has been “leaning into this new technology” and that AI is affecting fields including music, dance and dramatic arts — though he cautioned that the focus at USC is not to replace human creativity.
“What’s so critical to me as the leader of USC is making sure that as we provide these tools and as we extend our research prowess, we’re always centering on human values and agency,” Kim said.
For Stevens, who is a trustee and an alumnus, the gift marks a major addition on top of his years-long support for USC.
Stevens, 66, is a managing partner at S-Cubed Capital, an investment holding company based in Menlo Park. As of Tuesday, his net worth totaled more than $11 billion, according to Forbes. He is a former partner at Sequoia Capital and sits on the board of several tech firms, including Nvidia. Much of his wealth comes from his stake in the chipmaker. Before entering venture capital, Stevens worked in sales at Intel and as a technical staff member at Hughes Aircraft.
In an interview, Stevens said USC’s strengths in computer science, medicine, engineering, business and the arts make the university a strong place to expand AI.
“The gift is really aimed at sort of infusing AI techniques and tools technologies into all of those disciplines,” Stevens said. “With AI, we’re only in the first inning is what I tell people. And the world, 10 years from now, will be unrecognizable to us.”
In 2004, Stevens donated $22 million to establish what became the USC Stevens Center for Innovation. In 2015, he gave $50 million for the USC Mark and Mary Stevens Neuroimaging and Informatics Institute. USC launched the School of Advanced Computing, which is now named after him and his wife, in 2024.
Stevens said universities risk falling behind if they do not invest quickly in AI, especially because some major recent advances have come from private companies rather than academic labs.
“I think a lot of American universities are in danger of getting left behind if they don’t invest and raise money to further the AI revolution,” Stevens said.
Stevens also acknowledged the risks. “AI in the wrong hands … can be very destructive,” he said. “I think one of the jobs of universities in America is to understand, have a balanced approach, understand the guardrails and the safeguards that need to be adhered to as AI proliferates.”
Amy Eguchi, a teaching professor in the Department of Education Studies at UC San Diego who studies AI, said the gift fits into wider trends at U.S. campuses.
Universities are responding to AI in two ways, Eguchi said: by giving students and employees access to tools such as ChatGPT, and investing in AI research and applications across fields. The donation to USC, she said, reflects the second approach, even as campuses struggle with what the technology means for teaching and learning.
“The biggest issue AI creates for us as educators is that it’s harder to figure out what to do with this tool and what to do with students, because we don’t know what they need to learn at this point about AI because it’s changing so fast. And we need to focus on the best ways to use AI while not losing critical thinking skills,” Eguchi said. “Universities teach students to ask what does it mean to be human, right? But AI is complicating that question.”
Kim said a USC AI committee has been developing recommendations for classroom use, curriculum, academic integrity and ethics. He said the university is considering AI resources and courses for students in every major, along with coursework on AI’s impact on society, human values and ethics.
Some USC faculty say that expansion should proceed carefully. Sanjay Mahdav, an associate professor of technology and applied computing practice, said the gift presents an opportunity, but also raises difficult teaching questions.
“In my classes, students are increasingly using tools like ChatGPT to offload their critical thinking skills,” Mahdav said. “I honestly am unsure how to best continue to educate my students in a world where these AI tools exist.”
Mahdav said AI policies should not be imposed uniformly across campus. “Ultimately, regardless of what university-wide initiatives may come from this gift, I think it’s important that faculty continue to be able to make domain and class-specific decisions on AI use,” he said.
The debate mirrors broader concerns about whether AI will deepen learning or encourage students to outsource reasoning and problem-solving. Faculty and students have also raised worries about bias, creativity, accuracy and whether AI systems will replace forms of intellectual and professional work that colleges have long trained students to perform.
Kim acknowledged concern about the threats AI poses to human judgment, creativity and critical thinking, but said he believes USC is up to the task.
“While we see enormous opportunities for AI to enhance and save lives and address major societal problems, it also raises a number of important challenges that we need to address as a community and as a society,” Kim said. “And it’s our ambition not simply to be a university that leads in using AI… but also to be the most thoughtful university in terms of how to use AI in an ethical and responsible way.”
Times staff writer Queenie Wong contributed to this report.
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