Testing in the Clouds: NASA Flies to Improve Satellite Data
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Piloted by NASA’s Tim Williams, the ER-2 science aircraft ascends for one of the final science flights for the GSFC Lidar Observation and Validation Experiment (GLOVE) on Feb. 1, 2025. As a collaboration between engineers, scientists, and aircraft professionals, GLOVE aims to improve satellite data products for Earth Science applications.
NASA/Steve Freeman
In February, NASA’s ER-2 science aircraft flew instruments designed to improve satellite data products and Earth science observations. From data collection to processing, satellite systems continue to advance, and NASA is exploring how instruments analyzing clouds can improve data measurement methods.
Researchers participating in the Goddard Space Flight Center Lidar Observation and Validation Experiment (GLOVE) used the ER-2 – based at NASA’s Armstrong Flight Research Center in Edwards, California – to validate satellite data about cloud and airborne particles in the Earth’s atmosphere. Scientists are using GLOVE instruments installed onboard the aircraft to measure and validate data about clouds generated by satellite sensors already orbiting in space around Earth.
“The GLOVE data will allow us to test new artificial intelligence algorithms in data processing,” said John Yorks, principal investigator for GLOVE and research physical scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “These algorithms aim to improve the cloud and aerosol detection in data produced by the satellites.”
Jennifer Moore, a researcher from NASA’s Goddard Space Flight Center, checks the cabling on the Roscoe instrument at NASA’s Armstrong Flight Research Center in Edwards, California, for the GSFC Lidar Observation and Validation Experiment (GLOVE) on Feb. 1, 2025. The Roscoe instrument will be uploaded onto NASA’s ER-2 science aircraft.
NASA/Steve Freeman
The validation provided by GLOVE is crucial because it ensures the accuracy and reliability of satellite data. “The instruments on the plane provide a higher resolution measurement ‘truth’ to ensure the data is a true representation of the atmospheric scene being sampled,” Yorks said.
The ER-2 flew over various parts of Oregon, Arizona, Utah, and Nevada, as well as over the Pacific Ocean off the coast of California. These regions reflected various types of atmospheres, including cirrus clouds, marine stratocumulus, rain and snow, and areas with multiple types of clouds.
“The goal is to improve satellite data products for Earth science applications,” Yorks said. “These measurements allow scientists and decision-makers to confidently use this satellite information for applications like weather forecasting and hazard monitoring.”
Researcher Jackson Begolka from the University of Iowa examines instrument connectors onboard the ER-2 aircraft at NASA’s Armstrong Flight Research Center in Edwards, California, on Feb. 1, 2025. The GLOVE instrument will validate data from satellites orbiting the Earth.
NASA/Steve Freeman
The four instruments installed on the ER-2 were the Cloud Physics Lidar, the Roscoe Lidar, the enhanced Moderate Resolution Imaging Spectroradiometer Airborne Simulator, and the Cloud Radar System. These instruments validate data produced by sensors on NASA’s Ice, Cloud, and Land Elevation Satellite 2 (ICESat-2) and the Earth Cloud, Aerosol and Radiation Explorer (EarthCARE), a joint venture between the ESA (European Space Agency) and JAXA (Japan Aerospace Exploration Agency).
“Additionally, the EarthCARE satellite is flying the first ever Doppler radar for measurements of air motions within clouds,” Yorks said. While the ER-2 is operated by pilots and aircrew from NASA Armstrong, these instruments are supported by scientists from NASA Goddard, NASA’s Ames Research Center in California’s Silicon Valley, and the Naval Research Laboratory office in Monterey, California, as well as by students from the University of Iowa in Iowa City and the University of Maryland College Park.
Crew Departure, Dragon Mission, and Spacewalk Preps Fill Crew’s Day
Astronaut Nichole Ayers poses for a portrait inside the seven window cupola, the International Space Station’s “window to the world,” as the orbital outpost soared 263 miles above Russia near the Kazakhstan border.
NASA
Three International Space Station residents will return to Earth this weekend just a couple of days before the expected arrival of the next SpaceX Dragon cargo mission. Soon after that, two NASA astronauts will exit the orbital outpost for a solar array maintenance spacewalk.
Veteran orbital residents Don Pettit of NASA and Alexey Ovchinin and Ivan Vagner, both from Roscosmos, are winding down a seven-month space research mission that began on Sept. 11, 2024. The Earthbound crewmates are scheduled to undock from the station’s Rassvet module at 5:57 p.m. EDT on Saturday inside their Soyuz MS-26 spacecraft ending the Expedition 72 mission. They will orbit Earth twice before firing the Soyuz’ braking engines, descend into the atmosphere, then parachute to a landing in Kazakhstan at 8:20 p.m. (6:20 a.m. on Sunday, April 20, in Kazakhstan).
The trio from NASA and Roscosmos spent the first half of Wednesday reviewing the steps they will perform to ready the Soyuz spacecraft for undocking, as well as the procedures they will use once they depart the station and head back to Earth. Pettit then continued packing up his personal gear for stowage aboard the Soyuz MS-26. Ovchinin and Vagner spent the last of half of their shift handing off their mission responsibilities to the orbiting lab’s two newest cosmonauts Sergey Ryzhikov and Alexey Zubritsky who arrived at the station on April 8.
Next, the new Expedition 73 crew will turn its attention to the arrival of the SpaceX Dragon cargo craft that will launch at 4:15 a.m. EDT on Monday, April 21, from NASA’s Kennedy Space Center. Dragon will dock to the Harmony module’s space-facing port at 8:20 a.m. the following day delivering about 6,700 pounds of new science experiments and station supplies. Flight Engineers Jonny Kim of NASA and Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) trained on Wednesday for the spacecraft’s arrival and will be on duty next week monitoring Dragon’s automated approach and docking.
Just over a week after Dragon’s arrival, NASA Flight Engineers Anne McClain and Nichole Ayers will put on their spacesuits and exit the orbiting lab’s Quest airlock for a six-and-half-hour spacewalk on May 1. First, the duo will install a modification kit to prepare the port side truss structure for a new rollout solar array. Next, they will relocate an antenna that communicates with approaching and departing commercial crew and cargo spacecraft. The astronauts spent Wednesday familiarizing themselves with the spacewalking tools and parts they will use and organizing them inside Quest.
Flight Engineer Kirill Peskov spent the first portion of his day collecting air samples from the Zvezda, Zarya, and Nauka modules for analysis. Later, he focused on orbital plumbing duties transferring water between the station’s U.S. and Roscosmos segments.
NASA and SpaceX are targeting no earlier than 4:15 a.m. EDT on Monday, April 21, for the next launch to deliver scientific investigations, supplies, and equipment to the International Space Station. Filled with about 6,700 pounds of supplies, the SpaceX Dragon spacecraft, on the company’s Falcon 9 rocket, will lift off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
This launch is the 32nd SpaceX commercial resupply services mission to the orbital laboratory for the agency, and the 12th SpaceX launch under the Commercial Resupply Services-2 (CRS) contract. The first 20 launches were under the original resupply services contract.
NASA’s live launch coverage will begin at 3:55 a.m. on NASA+. Learn how to watch NASA content through a variety of platforms.
NASA’s SpaceX 32nd commercial resupply mission will launch on the company’s Dragon spacecraft on the SpaceX Falcon 9 rocket to deliver research and supplies to the International Space Station
NASA
NASA’s SpaceX 32nd commercial resupply mission will launch from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Arrival & Departure
The SpaceX Dragon spacecraft will arrive at the space station and dock autonomously to the zenith port of the station’s Harmony module at approximately 8:20 a.m. Tuesday, April 22. Live coverage NASA’s coverage of the rendezvous and docking will begin at 6:45 a.m on NASA+. NASA astronaut Jonny Kim, Expedition 73 commander and JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi will monitor the arrival of the spacecraft, which will stay docked to the orbiting laboratory for about one month before splashing down and returning critical science and hardware to teams on Earth.
Astronauts Jonny Kim of NASA and Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) will monitor the arrival of the SpaceX Dragon cargo spacecraft from the International Space Station.
NASA
Research Highlights
Robotic Spacecraft Guidance
Smartphone Video Guidance Sensor-2 (SVGS-2) uses the space station’s Astrobee robots to demonstrate using a NASA developed, vision-based sensor to control a formation flight of small satellites.
NASA
Smartphone Video Guidance Sensor-2 (SVGS-2) uses the space station’s Astrobee robots to demonstrate using a NASA developed, vision-based sensor to control a formation flight of small satellites. Based on a previous in-space demonstration of the technology, this investigation is designed to refine the maneuvers of multiple robots and integrate the information with spacecraft systems.
Potential benefits of this technology include improved accuracy and reliability of systems for guidance, navigation, and control that could be applied to docking crewed spacecraft in orbit and remotely operating multiple robots on the lunar or Martian surface.
Protection From Particles
The Aerosol Monitors investigation tests three different air quality monitors to determine which is best suited to protect crew health and ensure mission success.
NASA
During spaceflight, especially long-duration missions, concentrations of airborne particles must be kept within ranges safe for crew health and hardware performance. The Aerosol Monitors investigation tests three different air quality monitors to determine which is best suited to protect crew health and ensure mission success.
The investigation also tests a device for distinguishing between smoke and dust. Aboard the orbital outpost, the presence of dust can cause false smoke alarms that require crew member response. Reducing false alarms could save valuable crew time while continuing to protect astronaut safety.
Next-Generation Pharmaceutical Nanostructures
The newest Industrial Crystallization Cassette (ADSEP-ICC) investigation adds capabilities to an existing protein crystallization facility.
NASA
The newest Industrial Crystallization Cassette (ADSEP-ICC) investigation adds capabilities to an existing protein crystallization facility. The cassette can process more sample types, including tiny gold particles used in devices that detect cancer and other diseases or in targeted drug delivery systems. Microgravity makes it possible to produce larger and more uniform gold particles, which improves their use in research and real-life applications of technologies related to human health.
Better Materials, Better Drugs
The DNA Nano Therapeutics-Mission 2 produces a special type of molecule formed by DNA-inspired, customizable building blocks known as Janus base nanomaterials.
NASA
The DNA Nano Therapeutics-Mission 2 produces a special type of molecule formed by DNA-inspired, customizable building blocks known as Janus base nanomaterials. It also evaluates how well the materials reduce joint inflammation and whether they can help regenerate cartilage lost due to arthritis. These materials are less toxic, more stable, and more compatible with living tissues than current drug delivery technologies.
Environmental influences such as gravity can affect the quality of these materials and delivery systems. In microgravity, they are larger and have greater uniformity and structural integrity. This investigation could help identify the best formulations and methods for cost-effective in-space production. These nanomaterials also could be used to create novel systems targeting therapy delivery that improves patient outcomes with fewer side effects.
Helping Plants Grow
The Rhodium USAFA NIGHT payload examines how tomato plants respond to microgravity and whether a carbon dioxide replacement can reduce how much space-grown plants depend on photosynthesis.
NASA
The Rhodium USAFA NIGHT payload examines how tomato plants respond to microgravity and whether a carbon dioxide replacement can reduce how much space-grown plants depend on photosynthesis. Because photosynthesis needs light, which requires spacecraft power to generate, alternatives would reduce energy use.
The investigation also examines whether using supplements increases plant growth on the space station, which has been observed in preflight testing on Earth. In future plant production facilities aboard spacecraft or on celestial bodies, supplements could come from available organic materials such as waste.
Understanding how plants adapt to microgravity could help grow food during long-duration space missions or harsh environments on Earth.
Atomic Clocks in Space
An ESA (European Space Agency) investigation, Atomic Clock Ensemble in Space (ACES), examines fundamental physics concepts such as Einstein’s theory of relativity using two next-generation atomic clocks operated in microgravity.
NASA
An ESA (European Space Agency) investigation, Atomic Clock Ensemble in Space (ACES), examines fundamental physics concepts such as Einstein’s theory of relativity using two next-generation atomic clocks operated in microgravity. Results have applications to scientific measurement studies, the search for dark matter, and fundamental physics research that relies on highly accurate atomic clocks in space. The experiment also tests a technology for synchronizing clocks worldwide using global navigation satellite networks.
Cargo Highlights
NASA’s SpaceX 32nd commercial resupply mission will carry about 6,700 pounds of cargo to the International Space Station.
NASA
Hardware
Launch:
Catalytic Reactor – The catalytic reactor replacement unit oxidizes volatile organics from the wastewater so they can be removed by the gas separator and ion exchange bed replacement units as part of the station’s water recycling system. This unit failed in orbit and is being returned for analysis and refurbishment. This unit is being launched as an in-orbit spare.
Food Reach Tool Assembly – An L-shaped, hand-held tool that allows crew members to reach packages in the back of the food warmer without having to insert their hands. This tool is launching to replace a unit in orbit.
Reducer Cylinder Assembly – A cylinder tank that provides 15 minutes of oxygen to a crew member in case of an emergency. Launching two units as in-orbit spares.
Thermal Expansion Device – A device used to allow for thermal expansion of water within the Hydrogen Dome while it is being removed and replaced. Launching to maintain minimum in-orbit spares.
Return:
Urine Processor Assembly Pressure Control and Pump Assembly – This multi-tube purge pump enables the removal of non-condensable gas and water vapor from the distillation assembly within the greater urine processing assembly subsystem. This unit is returning to the ground for repair and refurbishment in support of the legacy environmental control and life support system fleet.
Assembly Contingency Transmitter Receiver Assembly – A part of the S-Band Radio Frequency Group, this assembly is a pressurized enclosure that contains electronics for this upper-level assembly. The Radio Frequency Group is used for command, control, and transmission communication for the space station. It was retrieved by NASA astronauts Suni Williams and Butch Wilmore during US EVA 92 and will return for repair.
High Gain Antenna Feed Assembly – Part of the S-Band Radio Frequency Group, this system features a two-axis, gimballed assembly with a pedestal and a large horn antenna. It was retrieved by NASA astronauts Suni Williams and Butch Wilmore during U.S. spacewalk 92 and will return for repair.
Low Gain Antenna Sub-Assembly – Part of the S-Band Radio Frequency Group, this sub-assembly consists of a helix antenna that provides a wide field of signal transmission capability. It was retrieved by NASA astronauts Suni Williams and Butch Wilmore during U.S. spacewalk 92 and will return for repair.
Planar Reflector Assembly – With an aluminum base and reflective element, visiting spacecraft reflect a laser to compute relative range, velocity, and attitude to the space station. This broken unit was retrieved and replaced by NASA astronaut Suni Williams during U.S. spacewalk 91 and will return for repair.
Multifiltration Bed – Supporting the water processor assembly, this spare unit will continue the International Space Station program’s effort to replace a degraded fleet of units in-orbit that improve water quality through a single bed. This unit will return for refurbishment and re-flight.
Watch and Engage
Live coverage of the launch from NASA Kennedy will air at 3:55 a.m. on NASA+..
A scrub jay perches on a branch near the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on June 22, 2020. Kennedy shares space with the Merritt Island National Wildlife Refuge, which is home to more than 65 amphibian and reptile, 25 mammal, 117 fish, and 330 bird species.
NASA’s Chandra Releases New 3D Models of Cosmic Objects
6 Min Read
NASA’s Chandra Releases New 3D Models of Cosmic Objects
New three-dimensional (3D) models of objects in space have been released by NASA’s Chandra X-ray Observatory. These 3D models allow people to explore — and print — examples of stars in the early and end stages of their lives. They also provide scientists with new avenues to investigate scientific questions and find insights about the objects they represent.
These 3D models are based on state-of-the-art theoretical models, computational algorithms, and observations from space-based telescopes like Chandra that give us accurate pictures of these cosmic objects and how they evolve over time.
However, looking at images and animations is not the only way to experience this data. The four new 3D printable models of Cassiopeia A (Cas A), G292.0+1.8 (G292), Cygnus Loop supernova remnants, and the star known as BP Tau let us experience the celestial objects in the form of physical structures that will allow anyone to hold replicas of these stars and their surroundings and examine them from all angles.
Cassiopeia A (Cas A)
Using NASA’s James Webb Space Telescope, astronomers uncovered a mysterious feature within the remnant, nicknamed the “Green Monster,” alongside a puzzling network of ejecta filaments forming a web of oxygen-rich material. When combined with X-rays from Chandra, the data helped astronomers shed light on the origin of the Green Monster and revealed new insights into the explosion that created Cas A about 340 years ago, from Earth’s perspective.
3D Model of Cassiopeia A «Green Monster»
INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando
3D Model of Cassiopeia A
INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando
This 3D model shows a star less than 10 million years old that is surrounded by a disk of material. This class of objects is known as T Tauri stars, named after a young star in the Taurus star-forming region. The model describes the effects of multiple flares, or outbursts that are detected in X-rays by Chandra from one T Tauri star known as BP Tau. These flares interact with the disk of material and lead to the formation of an extended outer atmosphere composed by hot loops, connecting the disk to the developing star.
3D Model of BP Tau
INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando
Cygnus Loop
X-ray: NASA/SAO/CXC; Optical: John Stone (Astrobin); Image Processing: NASA/SAO/CXC/L. Frattre, N. Wolk
The Cygnus Loop (also known as the Veil Nebula) is a supernova remnant, the remains of the explosive death of a massive star. This 3D model is the result of a simulation describing the interaction of a blast wave from the explosion with an isolated cloud of the interstellar medium (that is, dust and gas in between the stars). Chandra sees the blast wave and other material that has been heated to millions of degrees. The Cygnus Loop is a highly extended, but faint, structure on the sky: At three degrees across, it has the diameter of six full moons.
3D Model of Cygnus Loop
INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando
This is a rare type of supernova remnant observed to contain large amounts of oxygen. The X-ray image of G292.0+1.8 from Chandra shows a rapidly expanding, intricately structured field left behind by the shattered star. By creating a 3D model of the system, astronomers have been able to examine the asymmetrical shape of the remnant that can be explained by a “reverse” shock wave moving back toward the original explosion.
3D Model of G292.0+1.8
INAF-Osservatorio Astronomico di Palermo/Salvatore Orlando
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
This release features visualizations of three supernova remnants and one star. Each is rendered as a composite image, and as a digital 3-dimensional model, presented in separate short video clips. The composite images are two dimensional and static, but the digital models rotate, showcasing their three-dimensionality.
The first featured supernova is Cassiopeia A. In the X-ray, optical, and infrared composite image, the debris from an exploded star resembles a round purple gas cloud, marbled with streaks of golden light. In the rotating, 3D model, the purple gas cloud is depicted as a flat disk, like a record or CD. Bursting out the front and back of the disk is an orange and white shape similar to a ball of coral, or a head of cauliflower lined with stubby tendrils. Most of the ball, and the majority of the tendrils, appear on one side of the disk. On the opposite side, the shape resembles dollops of thick whipped cream.
Next in the release is a star known as BP Tau. BP Tau is a developing star, less than 10 million years old, and prone to outbursts or flares. These flares interact with a disk of material that surrounds the young star, forming hot loops of extended atmosphere. In the composite image, BP Tau resembles a distant, glowing white dot surrounded by a band of pink light. The rotating, 3D model is far more dynamic and intriguing! Here, the disk of material resembles a large blue puck with round, ringed, concave surfaces. At the heart of the puck is a small, glowing red orb: the developing star. Shooting out of the orb are long, thin, green strands: the flares. Also emerging from the orb are orange and pink petal-shaped blobs: the loops of extended atmosphere. Together, the orb, strands, and petals resemble an exotic flowering orchid.
The third celestial object in this release is the supernova remnant called Cygnus Loop. In the composite image, the remnant resembles a wispy cloud in oranges, blues, purples, and whites, shaped like a backwards letter C. The 3D model examines this cloud of interstellar material interacting with the superheated, supernova blast wave. In the 3D model, the Cygnus Loop resembles a bowl with a thick base, and a wedge cut from the side like a slice of pie. The sides of the bowl are rendered in swirled blues and greens. However, inside the thick base, revealed by the wedge-shaped cut, are streaks of red and orange. Surrounding the shape are roughly parallel thin red strands, which extend beyond the top and bottom of the digital model.
The final supernova featured in this release is G292.0+1.8. The composite image depicts the remnant as a bright and intricate ball of red, blue, and white X-ray gas and debris set against a backdrop of gleaming stars. In the 3D model, the remnant is rendered in translucent icy blue and shades of orange. Here, the rotating shape is revealed to be somewhat like a bulbous arrowhead, or perhaps an iceberg on its side.
