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By NASA
Almost a decade ago, then-grad student Kyle Helson contributed to early paperwork for NASA’s EXCITE mission. As a scientist at Goddard, Helson helped make this balloon-based telescope a reality: EXCITE launched successfully on Aug. 31.
Name: Kyle Helson
Title: Assistant Research Scientist
Organization: Observational Cosmology Lab (Code 665), via UMBC and the GESTAR II cooperative agreement with NASA Goddard
Dr. Kyle Helson is an assistant research scientist at NASA’s Goddard Space Flight Center in Greenbelt, Md. Photo credit: Dr. Amy Bender How did you know you wanted to work at NASA Goddard?
When I was finishing my physics Ph.D. at Brown University in 2016, I was talking to Ed Wollack and Dave Chuss at Goddard about the NASA postdoc program, and they suggested I apply. Luckily, I got the postdoc fellowship to come here to Goddard to work on cosmic microwave background detector testing and other related research.
I don’t think I would have realized or been interested in coming here had I not had that NASA Space Technology Research Fellowship when I was in grad school and gotten the opportunity to spend some time here and work with Ed and Dave.
What is the name of your team that you’re working with right now?
One of the projects I work on is the Exoplanet Climate Infrared TELescope (EXCITE). EXCITE is a scientific balloon-borne telescope that is designed to measure the spectra of hot, Jupiter-like exoplanet atmospheres in near-infrared light.
Related: NASA’s EXCITE Mission Prepared for Scientific Balloon Flight What is your role for that?
I do a little bit of everything. During grad school, I worked on the first few iterations of the proposal for EXCITE back in 2015 and 2016.
Over the past few years here at Goddard, I’ve been responsible for parts of a lot of the different subsystems like the cryogenic receiver, the gondola, the electronics, and integration and testing of the whole payload.
Last year, we went to Fort Sumner, New Mexico, for an engineering flight. Unfortunately, we were not able to fly for weather reasons. We went back last month, and I was again part of the field deployment team. We take the whole instrument, break it down, carefully ship it all out to New Mexico, put it back together, test it, and get it ready for a flight.
Kyle Helson (far right) and part of the EXCITE team stand in front of EXCITE Fort Sumner, New Mexico in Oct. 2023. EXCITE successfully launched on Aug. 31, 2024. Photo credit: Annalies Kleyheeg What is most interesting to you about your role here at Goddard?
What I like about working on a project like EXCITE is that we get to kind of do a little bit of everything.
We’ve been able to see the experiment from concept and design to actually getting built, tested and hopefully flown and then subsequent data analysis after the flight. What I think is really fun is being able be with an experiment for the entire life cycle.
How do you help support Goddard’s mission?
We’re studying exoplanets, which definitely fits within the scientific mission of Goddard. We’re also a collaboration between Goddard other academic institutions, like Arizona State, like Brown University, Cornell, and several other places, and so we’re also members of the larger scientific research community beyond NASA.
We also have a number of graduate students working on EXCITE. Ballooning is a good platform for training students and young researchers to learn how to build and design instruments, do data analysis, etc. One of the missions of NASA and Goddard is to train early career scientists like graduate students and post docs, and balloons provide a good platform for that as well.
Balloon missions like EXCITE also provide a good platform for technology advancement and demonstration in preparation for future satellite missions.
How did you know cosmology was what you wanted to pursue?
When I was a kid, I loved space. I wanted to be an astronaut when I was a kid. I even went to space camp.
The first time I ever got to see physics was a middle-school science class. That was the first time we ever learned physics or astronomy that was deeper than just identifying planets or constellations. We started to learn how we could use math to measure or predict experiments.
When I was in college, I remember talking to my undergraduate academic adviser, Glenn Starkman, and talking about what research I might like to do over the summer between sophomore and junior year of college. I wasn’t really sure what I wanted to do or what I was interested in, and he suggested I talk to some of the professors doing astrophysics and cosmology research and see if they had space for me in their lab.
I ended up finding a great opportunity working in a research lab in college — so it was working in the physics department in Case Western.
That’s where I first started learning about computer-aided design (CAD), and designing things in CAD, and that’s where I first learned how things get made in a machine shop, like on a mill, or a lathe. These skills have come in handy ever since, because I do a lot of design work in the lab. And I was lucky growing up that my dad was really hands-on and liked to fix things and build things and he taught me a lot of those skills as well.
“When I was a kid, I loved space,” said Kyle Helson. “I wanted to be an astronaut when I was a kid. I even went to space camp.”Photo courtesy of Kyle Helson Who has influenced you in your life?
My dad had a big influence. I think all the different people I’ve had the opportunity to learn from and work with who have been mentors along the way. My research advisers, professor John Ruhl in college, professor Greg Tucker in grad school, and Dr. Ed Wollack as a postdoc have all been very influential. Additionally, I have had the opportunity to work with a lot of very good post docs and research scientists during my career, Dr. Asad Aboobaker, Dr. Britt Reichborn-Kjennerud, Dr. Michele Limon, among others.
Throughout a career, there are tons of other people on the way from whom you pick up little things here and there that stick with you. You look back and you realize five years later you still do this one thing a certain way because someone helped you and taught you this skill or technique.
Where is a place you’d like to travel to?
Since I was lucky enough to go to Antarctica in graduate school, I figured that is the hardest continent to travel to, so now I have a mission to go to every continent. I’ve been to North America, I’ve been to South America, I’ve been to Asia, Europe, and Australia and New Zealand, but I’ve never been to Africa.
Kyle Helson (second from left) races the keirin at the Valley Preferred Cycling Center in Breinigsville, PA. Photo Credit Dr. Vishrut Garg What are your hobbies, or what do you enjoy doing?
I’m a competitive track cyclist. I started racing bikes in collegiate racing as a grad student at Brown. Many summers I’ve spent many weekends driving and flying all over the U.S. to race in the biggest track cycling events in the country.
What would be your three-word-memoir?
Curious, compassionate, cat-dad.
By Tayler Gilmore
NASA’s Goddard Space Flight Center in Greenbelt, Md
Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage.
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Last Updated Sep 10, 2024 EditorMadison OlsonContactRob Garnerrob.garner@nasa.govLocationGoddard Space Flight Center Related Terms
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By NASA
5 min read
How NASA Citizen Science Fuels Future Exoplanet Research
This artist’s concept shows the exoplanet K2-33b transiting its host star. Many citizen science projects at NASA invite the public to use transit data to make discoveries about exoplanets. NASA/JPL-Caltech NASA’s upcoming flagship astrophysics missions, the Nancy Grace Roman Space Telescope and the Habitable Worlds Observatory, will study planets outside our solar system, known as exoplanets. Over 5,000 exoplanets have been confirmed to date — and given that scientists estimate at least one exoplanet exists for every star in the sky, the hunt has just begun. Exoplanet discoveries from Roman and the Habitable Worlds Observatory may not be made only by professional researchers, but also by interested members of the public, known as citizen scientists.
Exoplanet research has a long involvement with citizen science. NASA’s TESS (Transiting Exoplanet Survey Satellite) mission and now-retired Kepler mission, which are responsible for the vast majority of exoplanet discoveries to date, both made observations freely available to the public immediately after processing. This open science policy paved the way for the public to get involved with NASA’s exoplanet science.
NASA’s Planet Hunters TESS project invites the public to classify exoplanet light curves from TESS online. Another project, Exoplanet Watch, allows citizen scientists to gather data about known exoplanets, submit their observations to NASA’s public data archive, and receive credit if their observation is used in a scientific paper. Participants don’t even need their own telescope — Exoplanet Watch also curates data from robotic telescopes for users to process.
Artist’s concept of NASA’s TESS (Transiting Exoplanet Survey Satellite). Data from TESS have been used in citizen science projects. NASA’s Goddard Space Flight Center “Anyone across the world who has access to a smartphone or a laptop can fully participate in a lot of these citizen science efforts to help us learn more about the cosmos,” said Rob Zellem, the project lead and project scientist for Exoplanet Watch and astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
NASA’s citizen science projects have discovered several new planets from Kepler and TESS data. They have also helped scientists refine the best time to observe important targets, saving hours of precious observation time on current flagship missions like NASA’s James Webb Space Telescope.
Roman and the Habitable Worlds Observatory provide even more possibilities for citizen science. Expected to launch by May 2027, Roman will discover exoplanets through direct imaging, transits, and gravitational microlensing. Following that, the Habitable Worlds Observatory will take direct images of stars in our solar neighborhood to find potentially habitable planets and study their atmospheres.
The general public can get Roman data as quickly as I can as a scientist working on the mission.
Rob Zellem
Exoplanet Watch Project Lead and Project Scientist; Nancy Grace Roman Space Telescope Deputy Project Scientist for Communications
Like Kepler and TESS before them, data from Roman and the Habitable Worlds Observatory will be available to both the scientific community and the public immediately after processing. With Roman’s surveys expected to deliver a terabyte of data to Earth every day — over 17 times as much as Webb — there is a huge opportunity for the public to help sift through the information.
“The general public can get Roman data as quickly as I can as a scientist working on the mission,” said Zellem, who also serves as Roman’s deputy project scientist for communications at NASA Goddard. “It truly makes Roman a mission for everyone and anyone.”
Although the Habitable Worlds Observatory’s full capabilities and instrumentation have yet to be finalized, the inclusion of citizen science is expected to continue. The team behind the mission is embracing a community-oriented planning approach by opening up working groups to volunteers who want to contribute.
“It’s already setting the tone for open science with the Habitable Worlds Observatory,” said Megan Ansdell, the program scientist for the mission at NASA Headquarters in Washington. “The process is as open as possible, and these working groups are open to anybody in the world who wants to join.” There are already over 1,000 community working group members participating, some of whom are citizen scientists.
The Roman Coronagraph, photographed during testing at NASA’s Jet Propulsion Lab in Southern California, is a technology demonstration designed to block starlight and allow scientists to see the faint light from planets outside our solar system. It represents one of multiple ways that Roman will contribute to exoplanet research. NASA/JPL-Caltech Future citizen science initiatives may be combined with cutting-edge tools such as artificial intelligence (AI) for greater efficacy. “AI can be exceptionally powerful in terms of classification and identifying anomalous things,” said Joshua Pepper, the deputy program scientist for the Habitable Worlds Observatory at NASA Headquarters. “But the evaluation of what those anomalous things are often requires human insight, intervention, and review, and I think that could be a really fantastic area for citizen scientists to participate.”
Before Roman and the Habitable Worlds Observatory launch, exoplanet citizen scientists still have plenty of data to analyze from the Kepler and TESS satellites, but the contributions of the community will become even more important when data begin pouring in from the new missions. As Zellem said, “We’re in a golden age of exoplanet science right now.”
NASA’s citizen science projects are collaborations between scientists and interested members of the public and do not require U.S. citizenship. Through these collaborations, volunteers (known as citizen scientists) have helped make thousands of important scientific discoveries. To get involved with a project, visit NASA’s Citizen Science page.
By Lauren Leese
Web Content Strategist for the Office of the Chief Science Data Officer
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By European Space Agency
An international team of astronomers using the NASA/ESA/CSA James Webb Space Telescope have directly imaged an exoplanet roughly 12 light-years from Earth. While there were hints that the planet existed, it had not been confirmed until Webb imaged it. The planet is one of the coldest exoplanets observed to date.
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By NASA
6 Min Read NASA’s Webb Images Cold Exoplanet 12 Light-Years Away
This image of the gas-giant exoplanet Epsilon Indi Ab was taken with the coronagraph on NASA’s James Webb Space Telescope’s MIRI (Mid-Infrared Instrument). A star symbol marks the location of the host star Epsilon Indi A, whose light has been blocked by the coronagraph, resulting in the dark circle marked with a dashed white line (full image below) An international team of astronomers using NASA’s James Webb Space Telescope has directly imaged an exoplanet roughly 12 light-years from Earth. The planet, Epsilon Indi Ab, is one of the coldest exoplanets observed to date.
The planet is several times the mass of Jupiter and orbits the K-type star Epsilon Indi A (Eps Ind A), which is around the age of our Sun, but slightly cooler. The team observed Epsilon Indi Ab using the coronagraph on Webb’s MIRI (Mid-Infrared Instrument). Only a few tens of exoplanets have been directly imaged previously by space- and ground-based observatories.
Image A: Exoplanet Epsilon Indi Ab
This image of the gas-giant exoplanet Epsilon Indi Ab was taken with the coronagraph on NASA’s James Webb Space Telescope’s MIRI (Mid-Infrared Instrument). A star symbol marks the location of the host star Epsilon Indi A, whose light has been blocked by the coronagraph, resulting in the dark circle marked with a dashed white line. Epsilon Indi Ab is one of the coldest exoplanets ever directly imaged. Light at 10.6 microns was assigned the color blue, while light at 15.5 microns was assigned the color orange. MIRI did not resolve the planet, which is a point source. “Our prior observations of this system have been more indirect measurements of the star, which actually allowed us to see ahead of time that there was likely a giant planet in this system tugging on the star,” said team member Caroline Morley of the University of Texas at Austin. “That’s why our team chose this system to observe first with Webb.”
“This discovery is exciting because the planet is quite similar to Jupiter — it is a little warmer and is more massive, but is more similar to Jupiter than any other planet that has been imaged so far,” added lead author Elisabeth Matthews of the Max Planck Institute for Astronomy in Germany.
Previously imaged exoplanets tend to be the youngest, hottest exoplanets that are still radiating much of the energy from when they first formed. As planets cool and contract over their lifetime, they become significantly fainter and therefore harder to image.
A Solar System Analog
“Cold planets are very faint, and most of their emission is in the mid-infrared,” explained Matthews. “Webb is ideally suited to conduct mid-infrared imaging, which is extremely hard to do from the ground. We also needed good spatial resolution to separate the planet and the star in our images, and the large Webb mirror is extremely helpful in this aspect.”
Epsilon Indi Ab is one of the coldest exoplanets to be directly detected, with an estimated temperature of 35 degrees Fahrenheit (2 degrees Celsius) — colder than any other imaged planet beyond our solar system, and colder than all but one free-floating brown dwarf. The planet is only around 180 degrees Fahrenheit (100 degrees Celsius) warmer than gas giants in our solar system. This provides a rare opportunity for astronomers to study the atmospheric composition of true solar system analogs.
“Astronomers have been imagining planets in this system for decades; fictional planets orbiting Epsilon Indi have been the sites of Star Trek episodes, novels, and video games like Halo,” added Morley. “It’s exciting to actually see a planet there ourselves, and begin to measure its properties.”
Not Quite As Predicted
Epsilon Indi Ab is the twelfth closest exoplanet to Earth known to date and the closest planet more massive than Jupiter. The science team chose to study Eps Ind A because the system showed hints of a possible planetary body using a technique called radial velocity, which measures the back-and-forth wobbles of the host star along our line of sight.
“While we expected to image a planet in this system, because there were radial velocity indications of its presence, the planet we found isn’t what we had predicted,” shared Matthews. “It’s about twice as massive, a little farther from its star, and has a different orbit than we expected. The cause of this discrepancy remains an open question. The atmosphere of the planet also appears to be a little different than the model predictions. So far we only have a few photometric measurements of the atmosphere, meaning that it is hard to draw conclusions, but the planet is fainter than expected at shorter wavelengths.”
The team believes this may mean there is significant methane, carbon monoxide, and carbon dioxide in the planet’s atmosphere that are absorbing the shorter wavelengths of light. It might also suggest a very cloudy atmosphere.
The direct imaging of exoplanets is particularly valuable for characterization. Scientists can directly collect light from the observed planet and compare its brightness at different wavelengths. So far, the science team has only detected Epsilon Indi Ab at a few wavelengths, but they hope to revisit the planet with Webb to conduct both photometric and spectroscopic observations in the future. They also hope to detect other similar planets with Webb to find possible trends about their atmospheres and how these objects form.
NASA’s upcoming Nancy Grace Roman Space Telescope will use a coronagraph to demonstrate direct imaging technology by photographing Jupiter-like worlds orbiting Sun-like stars – something that has never been done before. These results will pave the way for future missions to study worlds that are even more Earth-like.
These results were taken with Webb’s Cycle 1 General Observer program 2243 and have been published in the journal Nature.
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).
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Media Contacts
Laura Betz – laura.e.betz@nasa.gov, Rob Gutro – rob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Christine Pulliam – cpulliam@stsci.edu , Hannah Braun hbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
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Last Updated Jul 23, 2024 EditorStephen SabiaContactLaura Betzlaura.e.betz@nasa.gov Related Terms
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By NASA
2 min read
Arizona Students Go on an Exoplanet Watch
The instructor, teaching assistant, and students from the online exoplanet research course meeting synchronously via Zoom.
From left to right and top to bottom: Suber Corley, Molly Simon (instructor), Kimberly Merriam, Bradley Hutson, Elizabeth Catogni, Heather Hewitt (teaching assistant), Steve Marquez-Perez, Fred Noguer, Matthew Rice, Ty Perry, Mike Antares, Zachary Ruybal, Chris Kight, Kellan Reagan. Credit: Image collected by Molly Simon Exoplanets, planets outside of our own solar system, hold the keys to finding extraterrestrial life and understanding the origin of our own world. Now online students at Arizona State University (ASU) in a new course called Exoplanet Research Experience have become exoplanet scientists by taking part in NASA’s Exoplanet Watch project.
Fifteen students from ASU’s Astronomical and Planetary Sciences online degree program enroll in this course each year. These students analyze data on transits, events where the exoplanets block some of the light from their host stars. Each week, the class meets via Zoom to discuss progress, answer questions, and go over assignments. Students begin by completing a module from an online astrobiology course called Habitable Worlds, which is supported by NASA’s Infiniscope project. During the last 5 weeks of the course, students work to consolidate their work into a paper draft that is later submitted to a peer-reviewed journal with all of the students listed as co-authors.
“I think [the class] changed the course of my life…” said one student. “Not just in my confidence, but just knowing that people in the field have my back…I have tremendous support from them.”
“This course definitely helped kind of show what exactly scientists do and what the expectation is…especially for an online program, to have research opportunities is a great help…” another student said.
After participating in the course, students have gone on to participate in other research experiences, write their own first-author papers, participate in internships, and present their research at national astronomy conferences. An assessment of student outcomes was recently published in the Physics Review Physics Education Research Journal.
You don’t need to go to ASU to do real exoplanet research. Anyone can help collect and analyze exoplanet data through Exoplanet Watch, whether you own a telescope or just want to help analyze data. Visit the NASA Exoplanet Watch website to get started!
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Last Updated May 28, 2024 Related Terms
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