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The Earth Observer Editor’s Corner: July–September 2025
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By European Space Agency
Week in images: 08-12 September 2025
Discover our week through the lens
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By NASA
NSTGRO Homepage
Andrew Arends
University of California, Davis
Astronaut-Powered Laundry Machine
Allan Attia
Stanford University
Computational Modeling of Lithium Magnetoplasmadynamic Thruster for Nuclear Electric Propulsion
Michael Auth
University of California, Santa Barbara
Non-Contact, Real-Time Diagnostics of Battery Aging in 18650 Cells During the Lunar Night Using Acoustic Spectroscopy
Nicholas Brennan
Cornell University
Spin Wave-Based Neuromorphic Coprocessor for Advanced AI Applications
John Carter
Purdue University
Spectroscopic Measurements and Kinetic Modeling of Non-Boltzmann CN for Entry Systems Modeling
Thomas Clark
University of Colorado, Boulder
Data-Driven Representations of Trajectories in Cislunar Space
Nicholas Cmkovich
University of Wisconsin-Madison
Development of Radiation Tolerant Additively Manufactured Refractory Compositionally Complex Alloys
Kara Hardy
Michigan Technological University
Design and Optimization of Cuttlebone-Inspired Cellular Materials Using Turing Systems
Tyler Heggenes
Utah State University
Mitigating Spacecraft Charging Issues Through High-Precision, Temperature-Dependent Measurements of Dynamic Radiation Induced Conductivity
Joseph Hesse-Withbroe
University of Colorado, Boulder
Decreasing Astronaut Radiation Doses with Magnetic Shields
Niya Hope-Glenn
Massachusetts Institute of Technology
Investigating the Selectivity of CO2 Hydrogenation to Ethylene in a Plasma Reactor for Mars ISRU
Adrianna Hudyma
University of Minnesota
Biorthogonal Translation System for Production of Pharmaceuticals During Space Missions
Tushaar Jain
Carnegie Mellon University
Towards On-Demand Planetary Landing Through On-Board Autonomous Mapping and Cross-Modality Map Relative Localization
Devin Johnson
Purdue University
Numerical and Experimental Methodology to Optimize Propellant Injection, Mixing, and Response in Rotating Detonation Engines
Jack Joshi
University of Texas at Austin
State Representations for Measurement Fusion and Uncertainty Propagation in Cislunar Regime
John Knoll
William Marsh Rice University
Dexterous Manipulation via Vision-Intent-Action Models
Joseph Ligresti
Purdue University
Effects of Vacuum Conditions on FORP Reactivity and Long-Term Viability of MON-25/MMH Thrusters
Alexander Madison
University of Central Florida
Hybrid Microwave Sintering of Lunar Regolith with 2.45GHz and 18-28GHz
Aurelia Moriyama-Gurish
Yale University
Investigating Fundamental High Strain Rate Deformation Mechanisms to Bridge the Experiment-Computation Gap and Local Thermal Shock Response in C103
Sophia Nowak
University of Wisconsin-Madison
Pulsed Laser System for Calibration of High Resolution X-ray Microcalorimeters
Jacob Ortega
Missouri University of Science and Technology
Forging the Future Lunar Settlement with In-Situ Aluminum Extraction
John Riley O’Toole
University of Michigan
Laser-Based Measurements of Electron Properties in Hall Effect Thrusters with Non-Conventional Propellants Enabling for Cis-Lunar, Mars, and Deep Space Missions
Cort Reinarz
Texas A&M University
Utilizing Biometrics in Closed-Loop Compression Garment Systems as a Countermeasure for Orthostatic Intolerance
Erica Sawczynec
University of Texas at Austin
A Monolithic Cross-Dispersed Grism for Near-Infrared Spectroscopy
Ingrid Shan
California Institute of Technology
Micro-Architected Metallic Lattices for Lunar Dust Mitigation
Pascal Spino
Massachusetts Institute of Technology
Centimeter-Scale Robots for Accessing Europa’s Benthic Zone
Benjamin Stern
Northwestern University, Chicago
A Near-Field Thermoreflectance Approach for Nanoscale Thermal Mapping on Nanostructured Sige
Titus Szobody
William Marsh Rice University
Leveraging Polymeric Photochemistry in Ionic Liquid-Based Mirror Synthesis for Space Telescope Optics
Seneca Velling
California Institute of Technology
Constraining Weathering Kinetics Under Experimentally Simulated Venus Conditions
Zhuochen Wang
Georgia Institute of Technology
Optimal Covariance Steering on Lie Groups for Precision Powered Descent
Stanley Wang
Stanford University
Compact Robots with Long Reach for Space Exploration and Maintenance Tasks
Thomas Westenhofer
University of California, Irvine
Kinetic Modeling of Carbon Mass Loss in Nuclear Thermal Propulsion
Andrew Witty
Purdue University
Scalable Nanoporous Paints with High Solar Reflectance and Durability in Space Environments
Jonathan Wrieden
University of Maryland, College Park
A Stochastic Model for Predicting Charged Orbital Debris Probability Densities by Utilizing Earth’s Electromagnetic Field to Guide Active Debris Remediation Efforts
Jasen Zion
California Institute of Technology
Large-Format, Fast SNSPD Cameras Benchmarked with Neutral Atom Arrays
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Last Updated Sep 12, 2025 EditorLoura Hall Related Terms
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By European Space Agency
Image: Part of the Gibson Desert in Western Australia is featured in this image, captured by the Φsat-2 mission in June 2025. View the full article
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By NASA
Ames Science Directorate’s Stars of the Month: September 2025
The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Taejin Park, Lydia Schweitzer, and Rachel Morgan. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond.
Earth Science Star: Taejin Park
Taejin Park is a NASA Earth eXchange (NEX) research scientist within the Biospheric Science Branch, for the Bay Area Environmental Research Institute (BAERI). As the Project Scientist for the Wildfire, Ecosystem Resilience, & Risk Assessment (WERK) project, he has exhibited exemplary leadership and teamwork leading to this multi-year study with the California Natural Resources Agency (CNRA) and California Air Resources Board (CARB) to develop tracking tools of statewide ecological condition, disturbance, and recovery efforts related to wildfires.
Space Science and Astrobiology Star: Lydia Schweitzer
Lydia Schweitzer is a research scientist within the Planetary Systems Branch for the Bay Area Environmental Research Institute (BAERI) as a member of the Neutron Spectrometer System (NSS) team with broad contributions in instrumentation, robotic rovers and lunar exploration. Lydia is recognized for her leadership on a collaborative project to design and build a complex interface unit that is crucial for NSS to communicate with the Japanese Space Agency’s Lunar Polar eXploration rover mission (LUPEX). In addition, she is recognized for her role as an instrument scientist for the Volatiles Investigating Polar Exploration Rover (VIPER) and MoonRanger missions.
Space Science and Astrobiology Star: Rachel Morgan
Rachel Morgan is an optical scientist in the Astrophysics Branch for the SETI Institute. As AstroPIC’s lead experimentalist and the driving force behind the recently commissioned photonic testbed at NASA Ames, this month she achieved a record 92 dB on-chip suppression on a single photonic-integrated chip (PIC) output channel. This advances critical coronagraph technology and is a significant milestone relevant to the Habitable Worlds Observatory.
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By NASA
Explore Webb Science James Webb Space Telescope (JWST) NASA Webb Looks at… Webb News Latest News Latest Images Webb’s Blog Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Webb Timeline Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Science Explainers Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Webb’s First Images Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 6 Min Read NASA Webb Looks at Earth-Sized, Habitable-Zone Exoplanet TRAPPIST-1 e
This artist’s concept shows the volatile red dwarf star TRAPPIST-1 and its four most closely orbiting planets. Full image and caption shown below. Credits:
Artwork: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI) Scientists are in the midst of observing the exoplanet TRAPPIST-1 e with NASA’s James Webb Space Telescope. Careful analysis of the results so far presents several potential scenarios for what the planet’s atmosphere and surface may be like, as NASA science missions lay key groundwork to answer the question, “are we alone in the universe?”
“Webb’s infrared instruments are giving us more detail than we’ve ever had access to before, and the initial four observations we’ve been able to make of planet e are showing us what we will have to work with when the rest of the information comes in,” said Néstor Espinoza of the Space Telescope Science Institute in Baltimore, Maryland, a principal investigator on the research team. Two scientific papers detailing the team’s initial results are published in the Astrophysical Journal Letters.
Image A: Trappist-1 e (Artist’s Concept)
This artist’s concept shows the volatile red dwarf star TRAPPIST-1 and its four most closely orbiting planets, all of which have been observed by NASA’s James Webb Space Telescope. Webb has found no definitive signs of an atmosphere around any of these worlds yet. Artwork: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI) Of the seven Earth-sized worlds orbiting the red dwarf star TRAPPIST-1, planet e is of particular interest because it orbits the star at a distance where water on the surface is theoretically possible — not too hot, not too cold — but only if the planet has an atmosphere. That’s where Webb comes in. Researchers aimed the telescope’s powerful NIRSpec (Near-Infrared Spectrograph) instrument at the system as planet e transited, or passed in front of, its star. Starlight passing through the planet’s atmosphere, if there is one, will be partially absorbed, and the corresponding dips in the light spectrum that reaches Webb will tell astronomers what chemicals are found there. With each additional transit, the atmospheric contents become clearer as more data is collected.
Primary atmosphere unlikely
Though multiple possibilities remain open for planet e because only four transits have been analyzed so far, the researchers feel confident that the planet does not still have its primary, or original, atmosphere. TRAPPIST-1 is a very active star, with frequent flares, so it is not surprising to researchers that any hydrogen-helium atmosphere with which the planet may have formed would have been stripped off by stellar radiation. However many planets, including Earth, build up a heavier secondary atmosphere after losing their primary atmosphere. It is possible that planet e was never able to do this and does not have a secondary atmosphere. Yet researchers say there is an equal chance there is an atmosphere, and the team developed novel approaches to working with Webb’s data to determine planet e’s potential atmospheres and surface environments.
World of (fewer) possibilities
The researchers say it is unlikely that the atmosphere of TRAPPIST-1 e is dominated by carbon dioxide, analogous to the thick atmosphere of Venus and the thin atmosphere of Mars. However, the researchers also are careful to note that there are no direct parallels with our solar system.
“TRAPPIST-1 is a very different star from our Sun, and so the planetary system around it is also very different, which challenges both our observational and theoretical assumptions,” said team member Nikole Lewis, an associate professor of astronomy at Cornell University.
If there is liquid water on TRAPPIST-1 e, the researchers say it would be accompanied by a greenhouse effect, in which various gases, particularly carbon dioxide, keep the atmosphere stable and the planet warm.
“A little greenhouse effect goes a long way,” said Lewis, and the measurements do not rule out adequate carbon dioxide to sustain some water on the surface. According to the team’s analysis, the water could take the form of a global ocean, or cover a smaller area of the planet where the star is at perpetual noon, surrounded by ice. This would be possible because, due to the TRAPPIST-1 planets’ sizes and close orbits to their star, it is thought that they all are tidally locked, with one side always facing the star and one side always in darkness.
Image B: TRAPPIST-1 e Transmission Spectrum (NIRSpec)
This graphic compares data collected by Webb’s NIRSpec (Near-Infrared Spectrograph) with computer models of exoplanet TRAPPIST-1 e with (blue) and without (orange) an atmosphere. Narrow colored bands show the most likely locations of data points for each model. Illustration: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI) Innovative new method
Espinoza and co-principal investigator Natalie Allen of Johns Hopkins University are leading a team that is currently making 15 additional observations of planet e, with an innovative twist. The scientists are timing the observations so that Webb catches both planets b and e transiting the star one right after the other. After previous Webb observations of planet b, the planet orbiting closest to TRAPPIST-1, scientists are fairly confident it is a bare rock without an atmosphere. This means that signals detected during planet b’s transit can be attributed to the star only, and because planet e transits at nearly the same time, there will be less complication from the star’s variability. Scientists plan to compare the data from both planets, and any indications of chemicals that show up only in planet e’s spectrum can be attributed to its atmosphere.
“We are really still in the early stages of learning what kind of amazing science we can do with Webb. It’s incredible to measure the details of starlight around Earth-sized planets 40 light-years away and learn what it might be like there, if life could be possible there,” said Ana Glidden, a post-doctoral researcher at Massachusetts Institute of Technology’s Kavli Institute for Astrophysics and Space Research, who led the research on possible atmospheres for planet e. “We’re in a new age of exploration that’s very exciting to be a part of,” she said.
The four transits of TRAPPIST-1 e analyzed in the new papers published today were collected by the JWST Telescope Scientist Team’s DREAMS (Deep Reconnaissance of Exoplanet Atmospheres using Multi-instrument Spectroscopy) collaboration.
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
To learn more about Webb, visit:
https://science.nasa.gov/webb
Related Information
Webb Blog: Reconnaissance of Potentially Habitable Worlds with NASA’s Webb
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Video: How do we learn about a planet’s Atmosphere?
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Trappist-1 e (Artist’s Concept)
This artist’s concept shows the volatile red dwarf star TRAPPIST-1 and its four most closely orbiting planets, all of which have been observed by NASA’s James Webb Space Telescope. Webb has found no definitive signs of an atmosphere around any of these worlds yet.
TRAPPIST-1 e Transmission Spectrum (NIRSpec)
This graphic compares data collected by Webb’s NIRSpec (Near-Infrared Spectrograph) with computer models of exoplanet TRAPPIST-1 e with (blue) and without (orange) an atmosphere. Narrow colored bands show the most likely locations of data points for each model.
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Last Updated Sep 08, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Location NASA Goddard Space Flight Center Contact Media Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov
Leah Ramsay
Space Telescope Science Institute
Baltimore, Maryland
Hannah Braun
Space Telescope Science Institute
Baltimore, Maryland
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James Webb Space Telescope (JWST) Exoplanets
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The science paper by N. Espinoza et al. The science paper by A. Glidden et al. JWST Telescope Science Team
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