Goddard Engineers Improve NASA Lidar Tech for Exploration

Goddard Engineers Improve NASA Lidar Tech for Exploration

Like a sonar using light instead of sound, lidar technology increasingly helps NASA scientists and explorers with remote sensing and surveying, mapping, 3D-image scanning, hazard detection and avoidance, and navigation.

Cutting edge innovations by NASA researchers seek to refine lidars into smaller, lighter, more versatile tools for exploration.

“There are a lot of flavors of lidar right now,” said Cheryl Gramling, assistant chief for technology at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “It’s such an important technology because of the precision and versatility that it offers.”

Light detection and ranging, or lidar, is a remote sensing technology related to sonar and radar. Lidar uses pulses of light to measure distances and properties of objects accurately, by measuring the time it takes the light to reflect back to the lidar sensor.

Goddard innovators are looking to expand the usefulness of lidar applications in communication and navigation, planetary exploration, and space operations. Here are a few of the current investigations.

Foldable, Flat Lidar Optics

Origami-inspired lidar receiver
A prototype origami-pattern deployment sequence is demonstrated by graduate students Brandon Sargent (left) and Carolina Wright (right) of Brigham Young University. It shows the large expansion capability and the flexibility in the overall architecture.
Brigham Young University / Larry L. Howell

Research engineer Mark Stephen is developing a deployable, segmented telescope to capture the returning light signal using state-of-the-art flat-panel optics organized in foldable, origami-inspired panels. Working with researchers at Brigham Young University, their team seeks to provide future missions with the benefits of lidar technology without the current technologies’ high cost and limited efficiency.

Lidar typically is a high-cost technology that may not make the cut for tomorrow’s smaller, lighter, and more efficient missions. Size, weight, and power demands limit the technology’s ability to be implemented in more missions.

“Most people want really high performance,” Stephen said, “But they want it in a small, light, and power-efficient package. We’re trying to find the best balance, and cost matters. Often the cost comes more from the size, weight, and power than it does from the actual development if we’re launching something into space. That is where it gets expensive.”

Stephen is wrapping up a three-year effort to improve lidars through a Radical Innovation Initiative grant within Goddard’s Internal Research and Development (IRAD) program. Their project has been picked up by NASA’s Earth Science Technology Office to fund further improvements.

Typically, lidar receivers depend on bulky lenses to capture light, each lens needs a specific curvature and size to bend the light, in addition to the structures which hold the lenses, and other mechanics, Stephen said. Larger lenses are more effective, and that is where lidar technology tends to get heavy.

Flat optics use new types of nano-structured materials to manipulate individual photons, he said. These meta-materials allow thin and lightweight optics to perform the same functions as much larger and more expensive three-dimensional counterparts.

meta materials close-up
Silica wafers covered with structures smaller than the wavelengths of incoming light, these “meta-atomic” structures allow the lightweight, flat panel to perform the functions of lenses and mirrors without their bulk.
Nano Letters / L. Zhang, S. Chang, X. Chen, Y. Ding, T. Rahman, Y. Duan, M. Stephen, and X. Ni

“We are working toward being able to have a family of instruments where we have some flexibility and agility to meet the needs of a given mission,” Stephen said. “We want to develop a tool where you can make a better trade in terms of size, weight and power versus performance.”

One Laser, Many Wavelengths

Goddard engineer Guangning Yang is looking to improve lidar by producing multiple wavelengths of light from a single beam. Most modern lidars use multiple beams of a single wavelength to increase their accuracy.

Yang is the primary investigator for CASALS, or Concurrent Artificially intelligent Spectrometry and Adaptive Lidar System, a lidar technology that can sweep a large area more efficiently.

CASALS starts with one laser pulse, but instead of splitting that pulse into the many directions it needs to travel, their technology changes the wavelength of the laser at a very high speed. The different wavelengths of light then exit the laser transmitter at different angles based on their wavelength.

This pulse sequence produces a broom-like array sweeping across the object, landscape, or celestial body being studied.

“We have improved the efficiency,” Yang said, “and that will allow us to reduce the instrument’s size dramatically.”

Along with improvements in efficiency, CASALS is smaller than a typical lidar instrument. Yang said CASALS could help provide higher-density mapping of Earth and of other planets and moons as well as assisting with autonomous descents and landings.

Both flat optics and wavelength scanning offer new possibilities for lidar technology and are part of an array of investigations expected to unlock new opportunities in science and navigating distant worlds, Gramling said.

By Elizabeth Markham

NASA’s Goddard Space Flight Center in Greenbelt, Md.

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Karl B. Hille

New Software Enables Atmospheric Modeling with Greater Resolution

New Software Enables Atmospheric Modeling with Greater Resolution

3 Min Read

New Software Enables Atmospheric Modeling with Greater Resolution

Credits:
Randall Martin / Washington University

PROJECT

High Performance GEOS-Chem

SNAPSHOT

An ESTO investment in software optimization helps researchers and citizen scientists model air quality and greenhouse gases with greater resolution, allowing them to better understand how global atmospheric trends impact local areas.

A data visualization describing atmospheric NO2 concentrations, produced using High Performance GEOS-Chem
Image credit: Randall Martin / Washington University

Next-generation software is making it easier for researchers, policy makers, and citizen scientists to model air quality and greenhouse gases using NASA meteorological data.

This novel software, “High Performance GEOS-Chem,” uses equations representing the Earth’s atmospheric chemistry and boundary conditions from NASA’s Goddard Earth Observation System (GEOS) to represent global atmospheric chemistry across three dimensions at a horizontal spatial resolution of 12 kilometers by 12 kilometers per pixel—an area about one-fifth the size of New York City.

For comparison, the original GEOS-Chem model that was developed in 2001 only produced global simulations at a spatial resolution of about 200 by 250 square kilometers – an area about twice as large as the entire state of New Jersey.

With this improved resolution, researchers interested in air quality and atmospheric chemistry in specific communities can use models, simulations, and visualizations built with NASA data to better understand how global atmospheric trends impact local areas.

GEOS-Chem is an open-source model freely accessible here. More information about High Performance Geos-Chem – including manuals and tutorials – can be found here.

“This new generation of High Performance GEOS-Chem offers major advancements for ease of use, computational performance, versatility, resolution, and accuracy,” said Randall Martin, a professor at Washington University’s McKelvey School of Engineering and Primary Investigator for the High Performance GEOS-Chem project.

In a recent technical demonstration of their improved GEOS-Chem software, Martin and his team showed two images mapping tropospheric nitrogen dioxide – a pollutant typically produced by burning fossil fuels.

The image produced with High Performance GEOS-Chem featured 200 million more grid cells than the image produced with the original GEOS-Chem software. In other words, High Performance GEOS-Chem creates images more resolute by a factor of about 200.

“We’re really excited. Many features can be examined that aren’t resolved at all at the coarser resolution,” said Martin.

For researchers interested in global air quality and atmospheric composition with local resolution, this new generation of the High Performance GEOS-Chem marks the beginning of a new era for creating descriptive models.

Two visualizations using the same data generated by High Performance GEOS-Chem (top) and the original GEOS-Chem software (bottom). High Performance GEOS-Chem created an image more resolute than the original GEOS-Chem software by a factor of 200.
(Image credit: Randall Martin / Washington University)

Martin and his team added a number of technological innovations to High Performance GEOS-Chem. In particular, they incorporated a cubed-sphere computation grid into their GEOS-Chem software, reducing noise at the poles and allowing for higher resolution.

High Performance GEOS-Chem also includes a cloud computing capability. This spreads the resource-intensive computation work of generating detailed atmospheric models across dispersed computing nodes, such as Amazon Web Services.

Martin and his team pride themselves on ensuring GEOS-Chem remains an open and accessible tool for anyone interested in simulating atmospheric composition. Their website includes a full suite of tutorial videos, manuals, and guides for using GEOS-Chem effectively.

“NASA enabled us to develop this new generation of GEOS-Chem that has both the additional technical performance and offers the ease of use that this large community requires,” said Martin.

Future iterations of GEOS-Chem could feature further improvements. Developing a better user interface and increasing the modularity of GEOS-Chem are just a few objectives Martin and his team have in mind.

NASA’s Advanced Information Systems Technology (AIST), a part of NASA’s Earth Science Technology Office (ESTO), funded this program.

PROJECT LEAD

Randall Martin, Washington University in St. Louis

SPONSORING ORGANIZATION

Earth Science Division’s Advanced Information Systems Technology (AIST) Program

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NASA’s Modern History Makers: Maricela Lizcano

NASA’s Modern History Makers: Maricela Lizcano

5 min read

NASA’s Modern History Makers: Maricela Lizcano

Maricela Lizcano stands inside NASA Glenn Research Center’s Aerospace Communications Facility. She is wearing a teal jacket and behind her there are mathematical equations on the wall.
Maricela Lizcano poses inside NASA Glenn Research Center’s Aerospace Communications Facility.
Credit: NASA/Bridget Caswell

>back to gallery

Maricela Lizcano never dreamed of working for NASA.

In fact, she wasn’t planning on furthering her education until she had a revelation in her late twenties.

“I was watching one of those forensic shows, and I loved the way they caught the criminals with science,” said Lizcano, research materials engineer at NASA’s Glenn Research Center in Cleveland. “I wanted to be able to do that. I realized I should be studying science and engineering.”

It took Lizcano about ten years to prepare mentally and financially to go back to school, and during that time, she received some startling news.

“I found out that I was losing my sight, and it was very scary,” Lizcano said. “I think that was one of the things that tossed me off the rails. I had so many questions: ‘What am I going to do? How am I going to work or go to school? How quickly am I losing my vision?’ There were no answers.”

Lizcano was diagnosed with Stargardt disease, a rare genetic eye disease that occurs when fatty material builds up on the macula — the small part of the retina needed for sharp, central vision.

“My Stargardt disease started on the outer edges of my macula, and over time, it grew to the center,” Lizcano said. “By the time I was 45 years old, it had pretty much taken all of my central vision, and now I rely on my peripheral vision to see.”

Eventually, Lizcano viewed this as another obstacle to hurdle, no different from any others she had experienced in her life. She attended the University of Texas–Pan American, now called the University of Texas Rio Grande Valley. She started during a second summer session, easing her way to full-time attendance while also holding a job.

Because of her new disability, she couldn’t see what professors were writing on the board. She taught herself to listen intently to the topics being discussed in the lecture, then after class, she read the textbook and rewrote the lecture notes using special magnification tools.

“It took that much longer, but you learn to adapt,” Lizcano said. “There are certain skills you develop because of the changes you have to make when you have a disability. I learned that I really have to listen.”

After five years, Lizcano completed her mechanical engineering degree. She didn’t get a job right away after graduation, so she continued her education and earned master’s and doctorate degrees.

“I can’t just look at my disability as some great thing that I really had to overcome,” Lizcano said. “I think a lot of people overcome many obstacles because we are driven by the desire to achieve things. You don’t see the challenges as challenges, you just see them as something to conquer to get to your goal.”

In 2010, former President Barack Obama signed an executive order to increase federal employment of individuals with disabilities. The executive order directed executive departments and agencies to improve their efforts to employ workers with disabilities through increased recruitment, hiring, and retention of these individuals.

“Through the Workforce Recruitment Program, I had the opportunity to interview with representatives from federal agencies,” Lizcano said. “I heard nothing for a long time, but then suddenly I got an email from NASA Glenn asking if I’d present my research.”

She accepted a job as a research materials engineer and now leads a team working on high-voltage materials for electrified aircraft. She collaborates with various universities to develop composite insulation materials and lightweight conductors.

Even now working at NASA, Lizcano faces challenges that she finds ways to overcome. She depends on her fellow colleagues to carpool to work and accessibility tools — like the magnifier app — to use her computer.

“Understanding my needs allowed me to get over the fact that I lost my independence,” Lizcano said. “It was a mind shift to be all right with asking for help.”

Lizcano’s recommends a science, technology, engineering, and mathematics career to anyone looking for a challenge or excitement.

“We’re always solving problems. If you’re one of those people who really wants to make a difference in the world, STEM careers are a good place to start,” Lizcano said. “Any challenge that you may have in result of a disability is no different than the challenge you’re trying to solve, and it will give you the motivation and unique skills you need to be successful.”

NASA is in a Golden Era of aeronautics and space exploration. In partnership with commercial and private businesses, NASA is currently making history with significant missions such as ArtemisQuesst, and electrified aviation. The NASA’s Modern History Makers series highlights members of NASA Glenn’s workforce who make these remarkable missions possible.

Jacqueline Minerd
NASA’s Glenn Research Center

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Kelly M. Matter

Why NASA’s Roman Mission Will Study Milky Way’s Flickering Lights

Why NASA’s Roman Mission Will Study Milky Way’s Flickering Lights

Many thousands of bright, explosive looking stars speckle the screen. The smallest ones are white pinpoints, strewn across the screen like spilled salt. Larger ones are yellow and bluish white and they have spiky outer edges like sea urchins.
A simulated image of Roman’s observations toward the center of our galaxy, spanning only less than 1 percent of the total area of Roman’s galactic bulge time-domain survey. The simulated stars were drawn from the Besançon Galactic Model.
Credit: Matthew Penny (Louisiana State University)

NASA’s Nancy Grace Roman Space Telescope will provide one of the deepest-ever views into the heart of our Milky Way galaxy. The mission will monitor hundreds of millions of stars in search of tell-tale flickers that betray the presence of planets, distant stars, small icy objects that haunt the outskirts of our solar system, isolated black holes, and more. Roman will likely set a new record for the farthest-known exoplanet, offering a glimpse of a different galactic neighborhood that could be home to worlds quite unlike the more than 5,500 that are currently known.

Roman’s long-term sky monitoring, which will enable these results, represents a boon to what scientists call time-domain astronomy, which studies how the universe changes over time. Roman will join a growing, international fleet of observatories working together to capture these changes as they unfold. Roman’s Galactic Bulge Time-Domain Survey will focus on the Milky Way, using the telescope’s infrared vision to see through clouds of dust that can block our view of the crowded central region of our galaxy.

Watch this video to learn about time-domain astronomy and how time will be a key element in the Nancy Grace Roman Space Telescope’s galactic bulge survey. Credit: NASA’s Goddard Space Flight Center

“Roman will be an incredible discovery machine, pairing a vast view of space with keen vision,” said Julie McEnery, the Roman senior project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Its time-domain surveys will yield a treasure trove of new information about the cosmos.”

When Roman launches, expected by May 2027, the mission will scour the center of the Milky Way for microlensing events, which occur when an object such as a star or planet comes into near-perfect alignment with an unrelated background star from our viewpoint. Because anything with mass warps the fabric of space-time, light from the distant star bends around the nearer object as it passes close by. The nearer object therefore acts as a natural magnifying glass, creating a temporary spike in the brightness of the background star’s light. That signal lets astronomers know there’s an intervening object, even if they can’t see it directly.

In current plans, the survey will involve taking an image every 15 minutes around the clock for about two months. Astronomers will repeat the process six times over Roman’s five-year primary mission for a combined total of more than a year of observations.

A galaxy with a large, warmly glowing circular center and several purplish spiral arms extending outward, wrapped around the center like a cinnamon roll. Stars speckle the entire galaxy, but they are most densely packed near the center where they're yellower. Toward the outer edges, the stars are whiter. Overlaid on top of the galaxy is a small pink outline of a spacecraft located a little more than halfway out toward the bottom edge of the galaxy. A reddish search beam extends across the galaxy, about to the same point on the opposite side of the center of the galaxy.
This artist’s concept shows the region of the Milky Way Roman’s galactic bulge time-domain survey will cover. The higher density of stars in this direction will yield more than 50,000 microlensing events, which will reveal planets, black holes, neutron stars, trans-Neptunian objects, and enable exciting stellar science. The survey will also cover relatively uncharted territory when it comes to planet-finding. That’s important because the way planets form and evolve may be different depending on where in the galaxy they’re located. Our solar system is situated near the outskirts of the Milky Way, about halfway out on one of the galaxy’s spiral arms. A recent Kepler Space Telescope study showed that stars on the fringes of the Milky Way possess fewer of the most common planet types that have been detected so far. Roman will search in the opposite direction, toward the center of the galaxy, and could find differences in that galactic neighborhood, too.
Credit: NASA’s Goddard Space Flight Center/CI Lab

“This will be one of the longest exposures of the sky ever taken,” said Scott Gaudi, an astronomy professor at Ohio State University in Columbus, whose research is helping inform Roman’s survey strategy. “And it will cover territory that is largely uncharted when it comes to planets.”

Astronomers expect the survey to reveal more than a thousand planets orbiting far from their host stars and in systems located farther from Earth than any previous mission has detected. That includes some that could lie within their host star’s habitable zone – the range of orbital distances where liquid water can exist on the surface – and worlds that weigh in at as little as a few times the mass of the Moon.

Roman can even detect “rogue” worlds that don’t orbit a star at all using microlensing. These cosmic castaways may have formed in isolation or been kicked out of their home planetary systems. Studying them offers clues about how planetary systems form and evolve.

Roman’s microlensing observations will also help astronomers explore how common planets are around different types of stars, including binary systems. The mission will estimate how many worlds with two host stars are found in our galaxy by identifying real-life “Tatooine” planets, building on work started by NASA’s Kepler Space Telescope and TESS (the Transiting Exoplanet Survey Satellite).

Some of the objects the survey will identify exist in a cosmic gray area. Known as brown dwarfs, they’re too massive to be characterized as planets, but not quite massive enough to ignite as stars. Studying them will allow astronomers to explore the boundary between planet and star formation.

Roman is also expected to spot more than a thousand neutron stars and hundreds of stellar-mass black holes. These heavyweights form after a massive star exhausts its fuel and collapses. The black holes are nearly impossible to find when they don’t have a visible companion to signal their presence, but Roman will be able to detect them even if unaccompanied because microlensing relies only on an object’s gravity. The mission will also find isolated neutron stars – the leftover cores of stars that weren’t quite massive enough to become black holes.

Astronomers will use Roman to find thousands of Kuiper belt objects, which are icy bodies scattered mostly beyond Neptune. The telescope will spot some as small as about six miles across (about 1 percent of Pluto’s diameter), sometimes by seeing them directly from reflected sunlight and others as they block the light of background stars.

This animation compares signals from two planet detection methods: microlensing (top) and transit (bottom) for both high- and low-mass planets. Microlensing creates spikes in a star’s brightness, while transits have the opposite effect. Since both methods involve tracking the amount of light we receive from stars over time, astronomers will be able to use the same data set for both methods. Credit: NASA’s Goddard Space Flight Center/CI Lab

A similar type of shadow play will reveal 100,000 transiting planets between Earth and the center of the galaxy. These worlds cross in front of their host star as they orbit and temporarily dim the light we receive from the star. This method will reveal planets orbiting much closer to their host stars than microlensing reveals, and likely some that lie in the habitable zone.

Scientists will also conduct stellar seismology studies on a million giant stars. This will involve analyzing brightness changes caused by sound waves echoing through a star’s gaseous interior to learn about its structure, age, and other properties.

All of these scientific discoveries and more will come from Roman’s Galactic Bulge Time-Domain Survey, which will account for less than a fourth of the observing time in Roman’s five-year primary mission. Its broad view of space will allow astronomers to conduct many of these studies in ways that have never been possible before, giving us a new view of an ever-changing universe.

The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory and Caltech/IPAC in Southern California, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from various research institutions. The primary industrial partners are Ball Aerospace and Technologies Corporation in Boulder, Colorado; L3Harris Technologies in Melbourne, Florida; and Teledyne Scientific & Imaging in Thousand Oaks, California.

Download high-resolution video and images from NASA’s Scientific Visualization Studio

By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.

​​Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center
301-286-1940

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Ashley Balzer

Follow NASA’s Starling Swarm in Real Time

Follow NASA’s Starling Swarm in Real Time

A computer rendering of a Starling spacecraft in orbit above the Earth.
The Starling spacecraft are digitally rendered in NASA’s Eyes on the Solar System interactive app, allowing users to track the swarm in real-time and observe their orbits relative to other space missions and celestial bodies.
NASA

NASA’s Starling CubeSats are zipping through low Earth orbit in the agency’s latest test of robotic swarm technologies for space.  The four Starling spacecraft, launched in July 2023, are testing a group of small satellites ability to coordinate and cooperate independently without real-time updates from mission control.

NASA invites the public to follow the Starling mission live in NASA’s Eyes on the Solar System 3D visualization, which uses real-time data in an interactive solar system simulation. The positions of the planets, moons, and spacecraft – including Starling – are shown as they travel through space.

The Starling mission, managed at NASA’s Ames Research Center in California’s Silicon Valley, will test multiple flight patterns and autonomous capabilities, including maneuvering to stay together as a group, creating and patching their own communications network, keeping track of each other’s relative position without use of GPS,  and autonomously changing their combined science data collection strategy based on the latest readings from onboard sensors.

Autonomous technologies are vital to NASA’s space science and exploration goals, especially when exploring environments far from Earth where signal delays make real-time maneuvering impractical or impossible. Satellites and spacecraft operating in a networked, autonomous, and coordinated capacity will help humanity explore the unknown and conduct better science than ever before.

NASA’s Ames Research Center leads the Starling project. NASA’s Small Spacecraft Technology program, based at Ames and within NASA’s Space Technology Mission Directorate (STMD), funds and manages the Starling mission. Blue Canyon Technologies designed and manufactured the spacecraft buses and is providing mission operations support. Rocket Lab USA, Inc. provided launch and integration services. Partners supporting Starling’s payload experiments include Stanford University’s Space Rendezvous Lab in Stanford, California, Emergent Space Technologies of Laurel, Maryland, CesiumAstro of Austin, Texas, L3Harris Technologies, Inc., of Melbourne, Florida, and NASA Ames – with funding support by NASA’s Game Changing Development program within STMD.

For news media:

Members of the news media interested in covering this topic should reach out to the NASA Ames newsroom.

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Arezu Sarvestani