NSTGRO 2025

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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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Loura Hall

Hubble Surveys Cloudy Cluster

This new NASA/ESA Hubble Space Telescope image features a cloudy starscape from an impressive star cluster. This scene is in the Large Magellanic Cloud, a dwarf galaxy situated about 160,000 light-years away in the constellations Dorado and Mensa. With a mass equal to 10–20% of the mass of the Milky Way, the Large Magellanic Cloud is the largest of the dozens of small galaxies that orbit our galaxy.

The Large Magellanic Cloud is home to several massive stellar nurseries where gas clouds, like those strewn across this image, coalesce into new stars. Today’s image depicts a portion of the galaxy’s second-largest star-forming region, which is called N11. (The most massive and prolific star-forming region in the Large Magellanic Cloud, the Tarantula Nebula, is a frequent target for Hubble.) We see bright, young stars lighting up the gas clouds and sculpting clumps of dust with powerful ultraviolet radiation.

This image marries observations made roughly 20 years apart, a testament to Hubble’s longevity. The first set of observations, which were carried out in 2002–2003, capitalized on the exquisite sensitivity and resolution of the then-newly-installed Advanced Camera for Surveys. Astronomers turned Hubble toward the N11 star cluster to do something that had never been done before at the time: catalog all the stars in a young cluster with masses between 10% of the Sun’s mass and 100 times the Sun’s mass.

The second set of observations came from Hubble’s newest camera, the Wide Field Camera 3. These images focused on the dusty clouds that permeate the cluster, providing us with a new perspective on cosmic dust.

Media Contact:

Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD

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Hubble Space Telescope

Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.

Hubble’s Nebulae

These ethereal veils of gas and dust tell the story of star birth and death.

Hubble’s Night Sky Challenge

35 Years of Hubble Images

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PAW Participant Discussion

Participants are encouraged to dialogue before, during, and after the workshop. Contact the organizing committee for further questions.

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NASA

Drag Prediction Workshop Series

The Drag Prediction Workshop series is an extensive international effort to improve transonic aerodynamic predictions. This long-running collaborative effort seeks to mobilize the international aerospace community to improve the computational methods and tools to predict transonic aircraft performance, particularly drag.

More details on the workshop can be found at the workshop website: https://www.aiaa-dpw.org

NASA has a storied history with the workshop series from DPW-I (hosted in 2001) through the upcoming DPW-8, held in concert with Aeroelastic Prediction Workshop 4. In addition to code and methods improvements, the series also resulted in the NASA/Boeing Common Research Model (https://commonresearchmodel.larc.nasa.gov/), an open-access, commercially-relevant aircraft geometry. This geometry has been extensively tested in many facilities throughout the world and been the subject of multiple workshop series.

NASA’s contributions to the upcoming DPW-8 and subsequent work will be highlighted on this page.

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Brent Pomeroy