APOD: 2026 October 14 – Mars and the Beehive Under an Aurora

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

The bright Mars is near the center of the Beehive cluster (M44) in the sky's horizon. A colorful aurora sits above in the sky, looking like a curtain of light. Dark trees and a river line the foreground.

Mars and the Beehive Under an Aurora

Explanation: What a cosmic coincidence! In today’s image, Mars joins the Beehive cluster (M44 or Praesepe) below an auroral curtain and above a horizon of happy little trees near Lansjärv, Sweden. An eruption off the Sun reached Earth on October 10th, 2026 causing strong disturbances in Earth’s magnetic field. Energetic particles from the eruption collide with and energize the molecules in Earth’s atmosphere, which release that extra energy as the colorful aurora captured here. Auroras, or guovssahasat in North Sámi, is traditionally viewed with respect by the Sámi people indigenous to Sweden and other Arctic regions. Coincidentally, Mars appeared closest to the center of the Beehive cluster in the sky at the time. Although bees have been to space, the Beehive cluster is actually a swarm of young stars. Their rotation periods have helped humanity learn about how stars spin slower over time as they lose mass through their stellar winds.

Tomorrow’s picture: open space

Date: October 14, 2026
Credit: Petr Horálek (Institute of Physics in Opava), Josef Kujal, Vojan Höfer
Authors & editors: Keighley Rockcliffe, Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

Source: science.nasa.gov

NASA to Discuss Artemis Acceleration, Status of Upcoming Moon Missions

As the Artemis II crew members came close to passing behind the Moon and experiencing a planned loss of signal, they captured this image of a crescent Earth setting on the Moon’s limb on April 6, 2026. The edge of the visible surface of the Moon is called the “lunar limb."
As the Artemis II crew members came close to passing behind the Moon and experiencing a planned loss of signal, they captured this image of a crescent Earth setting on the Moon’s limb on April 6, 2026. The edge of the visible surface of the Moon is called the “lunar limb.”
Credit: NASA

NASA will provide an update on its plans to return American astronauts to the surface of the Moon by 2028 at 2 p.m. EDT, Friday, Oct. 23, at the agency’s Kennedy Space Center in Florida.

Learn where to watch online:

https://www.nasa.gov/live

Participants in the briefing include:

  • NASA Administrator Jared Isaacman
  • NASA Associate Administrator Amit Kshatriya
  • Jeremy Parsons, NASA’s Artemis program manager

The update will include details about NASA’s Artemis III mission that will send four astronauts to low Earth orbit next year to test critical systems needed for future lunar landings, and how plans to return American astronauts to the Moon by 2028 are progressing.

U.S. media interested in attending in person must apply online by 12 p.m., Friday, Oct. 16. To ask questions remotely, media must request the dial-in number from the Kennedy newsroom no later than one hour prior to the start of the update by emailing: [email protected]. NASA’s media accreditation policy is online. 

As part of a Golden Age of innovation and exploration, NASA will send Artemis astronauts on increasingly difficult missions near the lunar South Pole to explore more of the Moon than ever before. In addition to providing economic benefits and advancing scientific discovery through its Moon missions, NASA will establish an enduring human presence on the lunar surface and build on the agency’s foundation for the first crewed mission to Mars.

Learn more about Artemis:

https://www.nasa.gov/artemis

-end-

Rachel Kraft
Headquarters, Washington
202-358-1600
[email protected]

Tiffany Fairley
Kennedy Space Center, Fla.
321-867-2468
[email protected]

Details

Last Updated

Oct 14, 2026

Related Terms

Source: www.nasa.gov

NASA Develops Batteries to Power Humanity’s Return to Moon

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Yi Lin, SPEARS testing and research lead at NASA Langley, holds one of the small coin-cell batteries that had just undergone thermal vacuum testing.
Yi Lin, SPEARS testing and research lead at NASA Langley, holds one of the small coin-cell batteries that had just undergone thermal vacuum testing.
NASA/Ryan Hill

If you’ve ever had your car start sluggishly, or not at all, on a particularly frigid winter morning, you know standard batteries do not like extreme cold. That’s why NASA researchers are working to develop a battery that could function in the brutal cold of the Moon’s South Pole, where nighttime temperatures plunge to minus 328 degrees Fahrenheit (minus 200 Celsius). 

For future lunar operations, a battery will need to work immediately when warmed up and be able to power everything from an astronaut’s emergency kit to a rover capable of exploring the Moon’s darkest craters — all without posing a fire hazard. 

A team of NASA researchers is working to make all that happen. The project is called Solid Power for Extreme Environment Adaptability and Resilience in Space (SPEARS), and it could provide NASA with an important tool to help power humanity’s sustained presence on the Moon through the Artemis campaign. 

“Batteries have become an important part of our lives here on Earth, which enable our laptops, cell phones, power tools, and even our vehicles,” said Donald Dornbusch, principal investigator for SPEARS at NASA’s Glenn Research Center in Cleveland, where the project is led. “We will need them on the Moon, too, and these batteries will be required to operate reliably and safely in this harsh environment. That’s why we’re working on this technology.” 

Yi Lin, left, SPEARS testing and research lead, and Ji Su, a polymer materials scientist and the task lead, during the removal of SPEARS batteries from thermal vacuum testing at NASA Langley.
Yi Lin, left, SPEARS testing and research lead, and Ji Su, a polymer materials scientist and the task lead, during the removal of SPEARS batteries from thermal vacuum testing at NASA Langley.
NASA/Ryan Hill

Splashy problem, solid solution

Traditional lithium-ion batteries like those in your cell phone and laptop have a critical weakness: they rely on liquid electrolytes. Cool a conventional battery to the Moon’s nighttime temperatures, and that liquid would freeze, potentially damaging the battery. Heat it up too much — say, to daytime lunar temperatures of 212 F (100 C) — and it won’t work until cooled. Expose the liquid to the vacuum of space, and it evaporates. 

SPEARS batteries solve these problems by replacing the liquid electrolyte with a solid ceramic- or polymer-based material. This change could unlock several advantages. First and foremost, they could operate in the heat and extreme cold. 

During recent thermal vacuum testing at NASA’s Langley Research Center in Hampton, Virginia, small prototype battery cells operated well up to 176 F (80 C), down to minus 76 F (minus 60 C), and with slightly reduced performance down to minus 112 F (minus 80 C). 

“We proved for the first time that these cells can work down to minus 80 degrees Celsius,” said Yi Lin, SPEARS testing and research lead at NASA Langley.  

Lin also said he’s confident they can improve performance and maybe even expand that range in coming years. 

The batteries need to remain reliable through exposure to the Moon’s wild temperature swings between day and night. The thermal vacuum testing showed that after exposure to temperature extremes from 212 F (100 C) to minus 274 F (minus 170 C), SPEARS batteries don’t sustain damage.  

Just like the chemistry in your earbuds is different from the chemistry in your phone, which is different from the chemistry in your car, all these chemistries can still function with a solid electrolyte. We can tune for energy, tune for power, tune for durability, depending on the application.

Yi Lin

Yi Lin

SPEARS testing and research lead

Not even solid-state batteries will function while they’re at a temperature as low as minus 274 F, but because solid electrolytes don’t freeze like a liquid, the batteries can survive the extreme low temperatures.  

In order to get the batteries working again after exposure to such cold, small heaters come into play. SPEARS batteries wouldn’t need to be kept warm all the time, just warmed up to operational temperature. That could reduce the need for heavy thermal management systems in spacecraft and lunar habitats, allowing for lighter designs, lower costs, and longer mission durations. 

Nike Lin, a support engineer/technician on the thermal vacuum team, holds up a battery.
Nike Lin, a support engineer/technician on the thermal vacuum team, takes weight measurements of batteries following thermal vacuum testing.
NASA/Ryan Hill

Power for Moon, Earth

The applications for these solid-state batteries are nearly limitless, from small tools like drills that must operate in shadowed lunar craters, to rovers and emergency power packs for astronauts. They also could provide power solutions for long-duration scientific instruments. 

“We can tune the chemistry by using different electrode materials,” said Lin. “Just like the chemistry in your earbuds is different from the chemistry in your phone, which is different from the chemistry in your car, all these chemistries can still function with a solid electrolyte. We can tune for energy, tune for power, tune for durability, depending on the application.” 

While SPEARS is designed for space, the technology could be spun off into Earth-based applications. In fact, SPEARS evolved out of a previous battery project Lin and Dornbusch worked on that focused on aeronautic applications. 

From left to right: Donald Dornbusch (NASA Glenn), Godfrey Sauti, Sang-Hyon Chu, Yi Lin (NASA Langley), and Malachi Mooney-Rivkin (NASA Ames), during a round of TVAC testing at NASA Langley.
From left to right: Donald Dornbusch (NASA Glenn), Godfrey Sauti, Sang-Hyon Chu, Yi Lin (NASA Langley), and Malachi Mooney-Rivkin (NASA Ames), during a round of TVAC testing at NASA Langley.
NASA

“The potential market for solid-state batteries is very broad,” said Ji Su, a polymer materials scientist and the task lead at NASA Langley. “Automobiles, cell phones, communication devices, drones — anything that needs a portable power supply.” 

The SPEARS project began in 2026 with funding through the Advanced Research and Technology division within the agency’s Research and Technology Mission Directorate. The project is set to focus on technology development in its first stages before potentially shifting toward commercial collaboration. NASA’s Ames Research Center in California’s Silicon Valley is working to develop flight hardware such as test boards and electronics to help prepare the SPEARS batteries for spaceflight and test them in space environments. 

Source: www.nasa.gov

NASA’s Space X CRS-35 Launch Jellyfish

The exhaust plumes of a SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft are seen illuminated by sunlight against the predawn sky.
NASA/John Kraus

Sunlight illuminates the exhaust plumes of a SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft on Oct. 13, 2026. This visual phenomenon is known as a “jellyfish”; it happens near sunrise or sunset when the exhaust plume from the rocket becomes brightly illuminated, creating a glowing shape resembling a jellyfish.

The mission lifted off at 6:33 a.m. EDT from Space Launch Complex 40 at Cape Canaveral Space Force Station, carrying scientific investigations, supplies, and equipment to the International Space Station on SpaceX’s 35th commercial resupply services mission for NASA. The rocket’s exhaust plumes were visible across the eastern United States.

Watch the uncrewed Dragon spacecraft rendezvous with and dock to the International Space Station on Oct. 15. Coverage begins at 9:15 a.m. EDT.

Image credit: NASA/John Kraus

Source: www.nasa.gov

NASA’s Chandra Breaks Down ‘Treble Clef’s’ Galaxy Cluster Collision

Using Chandra, astronomers have discovered that an outburst from a supermassive black hole, followed by a collision of two galaxy clusters, are the likely causes of an unusual formation in a galaxy cluster. The “Treble Clef” radio source was given its nickname because of a distinct shape in radio waves that resembles the musical symbol. This composite image of the Treble Clef and its galaxy cluster contains X-rays from Chandra and eROSITA, radio data from LOFAR, and infrared data from UKIRT.
X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

Astronomers have used NASA’s Chandra X-ray Observatory to break down the cause of a remarkable formation of radio waves they have nicknamed the “Treble Clef” because its distinct shape strongly resembles the musical symbol.

The researchers discovered the Treble Clef is likely caused by an outburst from a supermassive black hole, followed by a collision of two galaxy clusters. A paper describing the findings, led by Andrea Botteon of the National Institute for Astrophysics, or INAF, in Italy, published Wednesday in the Astronomy & Astrophysics journal.

An explanation for the Treble Clef has been particularly difficult to find because the formation lies almost directly behind the plane of the Milky Way, meaning that stars, gas, and dust from our home galaxy largely block the view from Earth. However, by using telescopes that can peer through the intervening material, a team of researchers was able to identify what is responsible for this uncommon structure.

NASA’s Chandra and the German Extended RÖntgen Survey with an Imaging Telescope Array (eROSITA) X-ray telescope found diffuse, hot gas at the location of the Treble Clef, showing that a galaxy cluster hosts the object. The researchers also determined the galaxy cluster is, in fact, two clusters in the process of merging. Galaxy clusters are some of the largest structures in the universe, containing hundreds of individual galaxies and huge reservoirs of superheated gas.

This new composite image of the Treble Clef and its cluster shows the multimillion-degree gas detected in X-rays by Chandra and eROSITA in blue, with some of the Chandra data derived from a special technique the authors used to highlight important features in the Chandra data. Radio data shown in red from the LOw Frequency ARray (LOFAR), a large network of radio telescopes in Europe reveals the doppelganger of the musical notation. The final piece of the combined image comes from infrared data obtained by the United Kingdom Infrared Telescope, appearing mostly white.

The authors concluded that the Treble Clef likely formed in a two-stage process. First, an earlier outburst from a supermassive black hole in the galaxy cluster’s center drove clouds of charged particles and magnetic fields away at close to the speed of light. This led to a type of cosmic crescendo and initially produced bright radio waves that later faded as the particles lost energy. Next, the collision between the two clusters compressed or reenergized the cloud, which became brighter again in radio waves. Shock waves — similar to the sonic booms from supersonic jets — from the collision may have played a role in this reenergizing process.

To reveal evidence for the cluster collision in the Chandra data, the authors used a special technique that examined how much the cluster’s hot gas deviates from a symmetrical shape. Most of the hot gas is symmetrical and shaped approximately like an oval. The authors removed this symmetrical oval shape from the original X-ray image. The remaining X-ray emission in the residual image shows t is brightest on the left and right, and faintest in the center. The new composite image combines both the original X-ray and the residual X-ray images.

The brighter X-rays in the residual image, toward the left and right of the cluster’s center, imply that the collision between the two clusters likely occurred along the left-right direction as seen in the image. The researchers think the direct collision between the two clusters occurred a few hundred million years ago, and the clusters are now moving away from each other.

The resemblance to a treble clef is a case of pareidolia, the phenomenon when people see familiar shapes in random data, since there is no scientific connection to the musical notation.

NASA’s Marshall Space Flight Center in Huntsville, Alabama, 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.

To learn more about Chandra, visit:

https://nasa.gov/chandra

Visual Description

This release features a composite image of a remarkable radio wave formation that strongly resembles a treble clef musical symbol, hovering in the midst of two colliding galaxy clusters.

Here, galaxies in the galaxy clusters, plus foreground and background stars and galaxies, blanket the image with specks of light set against the blackness of space. At the center of the frame is a large, oval, blue-purple cloud with ragged edges. This is a multimillion-degree gas cloud in the two clusters detected in X-rays by Chandra and eROSITA, the Extended RÖntgen Survey with an Imaging Telescope Array.

In the middle of the purple field, tilting slightly to our left, is what appears to be a giant treble clef, loosely drawn with a neon pink marker. Like the musical notation for which it’s named, the formation has a strong vertical stroke with a continuous, fluid line swooping back and forth as it moves from top to bottom.

This radio wave formation appears to be the result of a two-stage process. First, charged particles and magnetic fields were driven from a supermassive black hole, producing bright radio waves. Those waves faded and lost energy over time, before being reenergized and compressed when the two galaxy clusters collided.

Details

Last Updated

Oct 14, 2026

Editor
Lee Mohon
Contact
Megan Watzke
Joel Wallace
Location
Marshall Space Flight Center

Source: science.nasa.gov

An Impact Structure With Legs

Several short, light-colored rocky ridges radiate out from a central point amid an orange and tan desert landscape.

Editor’s Note: Today’s story is the answer to the October Puzzler.

From above, the mere appearance of a curious geologic feature in Western Australia is enough to cause a fright. The aptly named Spider Crater, the product of a meteorite impact followed by hundreds of millions of years of erosion, sprawls across the landscape in the country’s Kimberley region.

The OLI (Operational Land Imager) on the NASA-USGS Landsat 9 satellite captured this image of the crater on September 20, 2026. The full impact structure has an oval shape measuring about 13 kilometers by 11 kilometers (8 miles by 7 miles), with the spiderlike central portion measuring about 4 kilometers (2.5 miles) across.

Geologists believe the unusual arachnoid pattern is the remnant of a central uplift, the raised portion of the crater floor that formed in the rebound of the initial impact shock. The light-colored “legs” are sandstone ridges that have endured while other rock layers in the impact zone have eroded away.

For decades after the feature’s discovery, scientists struggled to weave a tale about its formation. Some proposed it had a volcanic past. But with some legwork in the field, geologists identified telltale signs of a past impact: fan-shaped fractures called shatter cones. These fractures form only when intense shock waves travel through rock, and they are ubiquitous in Spider Crater’s central dome.

Scientists have subsequently performed lab analyses of shocked quartz and zircon crystals from the sandstone, which can help them reconstruct the angle of the meteorite’s impact. The date of the impact is uncertain, but estimates based on rocks in the region place it between about 900 million and 600 million years ago—making Spider Crater a creature of the late Precambrian.

NASA Earth Observatory image by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Lindsey Doermann.

References & Resources

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An Accidental Impact Crater Discovery 

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Source: science.nasa.gov

Hurricane Simon Lurks Off the Mexican Coast

The well-defined eye of Hurricane Simon lies just off Mexico’s Pacific coast. Some outer cloud bands of the spiraling storm extend over land.
Hurricane Simon churns off Mexico’s Pacific coast in this image acquired with the VIIRS (Visible Infrared Imaging Radiometer Suite) on the Suomi NPP satellite on October 11, 2026.
NASA Earth Observatory/Michala Garrison

Hurricane Simon, the latest in a long progression of tropical cyclones in the Eastern Pacific this season, passed close to the Mexican coast as a category 4 storm on October 11, 2026. Sustained winds reached 250 kilometers (155 miles) per hour as it crept north-northwest.

Simon’s eye was about 50 kilometers (30 miles) offshore, between Manzanillo and Puerto Vallarta, when the VIIRS (Visible Infrared Imaging Radiometer Suite) on the Suomi NPP satellite acquired this image around 2:30 p.m. local time (20:30 Universal Time) on October 11.

By that time, sustained winds were about 210 kilometers (130 miles) per hour, according to the National Hurricane Center (NHC), and the storm’s inner core was brushing up against the coast. The topography of the Sierra Madre mountains appeared to temper the storm’s intensity somewhat and shrink the size of its wind field, the NHC noted. Still, the major hurricane delivered heavy rain and flooding to coastal areas, including the port city of Manzanillo, and raised the risk of mudslides in mountainous areas, according to news reports.

Gravity waves in the upper atmosphere appear as a semicircle of ripples in a nighttime, grayscale satellite image. Hurricane clouds and city lights in Mexico are also visible.
Atmospheric gravity waves generated by Hurricane Simon are visible via mesospheric airglow in this nighttime image acquired with the VIIRS (Visible Infrared Imaging Radiometer Suite) on the NOAA-21 satellite on October 11, 2026.
NASA Earth Observatory/Michala Garrison

In the early morning hours of October 11, satellites captured the storm’s effects extending into the upper atmosphere. This nighttime image (above), acquired with VIIRS on the NOAA-21 satellite, shows atmospheric gravity waves radiating from the hurricane. These ripples form when latent heat released near the tropical cyclone’s eyewall drives strong convection, building tall cumulonimbus clouds with updrafts that can send waves into the stratosphere and mesosphere.

But these waves are not always observable. Winds in the upper atmosphere can dissipate them before they reach the mesosphere, where they show up as ripples in airglow—faint light emitted by gases at those high altitudes. The VIIRS day-night band is sensitive to airglow but also detects reflected moonlight, which can wash it out. On the night this image was acquired, minimal illumination from the Moon helped the airglow stand out.

On the morning of October 13, forecasts of Simon’s intensity and path remained “very low confidence,” as the storm’s evolution continued to defy meteorologists’ expectations. The system may steer north and enter the Gulf of California before making landfall. Large swells causing dangerous nearshore conditions were expected along portions of the southwestern and west-central coasts of Mexico in the coming days.

NASA Earth Observatory images by Michala Garrison, using VIIRS data from NASA EOSDIS LANCE, GIBS/Worldview, the Suomi National Polar-orbiting Partnership, and the Joint Polar Satellite System (JPSS). Story by Lindsey Doermann.

References & Resources

You may also be interested in:

Stay up-to-date with the latest content from NASA as we explore the universe and discover more about our home planet.

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Source: science.nasa.gov

NASA Names Astronaut Christina Koch Acting Deputy Chief Engineer

NASA astronaut Christina Koch stands inside Kennedy Space Center’s Vehicle Assembly Building on July 14, 2021, in front of the agency’s Space Launch System (SLS) rocket that ultimately powered the Orion spacecraft on the Artemis I mission. Koch later served as a crew member on the Artemis II mission in 2026, and on Oct. 13, 2026, NASA announced she will serve next as the agency’s acting deputy chief engineer.
NASA astronaut Christina Koch stands inside Kennedy Space Center’s Vehicle Assembly Building on July 14, 2021, in front of the agency’s Space Launch System (SLS) rocket that ultimately powered the Orion spacecraft on the Artemis I mission. Koch later served as a crew member on the Artemis II mission in 2026, and on Oct. 13, 2026, NASA announced she will serve next as the agency’s acting deputy chief engineer.
NASA/Glenn Benson

NASA engineer and astronaut Christina Koch will serve as the agency’s acting deputy chief engineer beginning on Sunday, Nov. 1, following the retirement of Katherine Van Hooser, who will conclude more than 35 years of distinguished service to the agency on Wednesday, Oct. 21.

In her new role, Koch will help lead NASA’s engineering community, supporting technical oversight, mission readiness, and engineering excellence across the agency’s programs and projects. With this appointment, Koch will transition to management astronaut status and will no longer be eligible for future spaceflight assignments.

“Christina has seen NASA engineering from both sides of the equation: developing complex systems on the ground and trusting them with her life in space,” said NASA Administrator Jared Isaacman. “After spending nearly a year living and working aboard the International Space Station and helping lead America back around the Moon on Artemis II this year, she brings an extraordinary combination of technical expertise, operational experience, and judgment to this role. I am excited to see the impact she will have across NASA as we return Americans to the lunar surface, build the Moon Base, get underway on nuclear power in space, and develop the capabilities that will ultimately take us on to Mars.”

“Katherine has been an extraordinary leader throughout her career, bringing technical expertise, sound judgment, and an unwavering commitment to mission success to some of NASA’s most complex engineering challenges,” said Amit Kshatriya, NASA associate administrator and chief engineer. “Her leadership has strengthened our engineering community and helped guide the agency through critical milestones and transitions. Christina brings a unique combination of engineering expertise, operational experience, and proven leadership, both on the ground and in space. I am grateful to Katherine for her exceptional service and confident Christina will continue the tradition of technical excellence that is essential to everything we do at NASA.”

Koch most recently served as a mission specialist aboard NASA’s Artemis II mission in April, helping carry out the first crewed flight around the Moon in more than 50 years. She previously spent 328 consecutive days aboard the International Space Station, setting the record for the longest single spaceflight by a woman and participating in the first all-female spacewalks.

Koch began her NASA career as an electrical engineer at the agency’s Goddard Space Flight Center in Greenbelt, Maryland, developing scientific instruments for space missions. Before her selection as an astronaut in 2013, her experience also included scientific field engineering in Antarctica and the Arctic. She has since held leadership positions within NASA’s Astronaut Office and at the agency’s Johnson Space Center in Houston, bringing a combination of technical expertise, operational experience, and firsthand understanding of the demands of human spaceflight to her new role.

Van Hooser joined NASA in 1991 at the agency’s Marshall Space Flight Center in Huntsville, Alabama, beginning a distinguished career in propulsion engineering and technical leadership. Her early work focused on liquid rocket engine turbomachinery before she became chief engineer for the space shuttle main engine, leading engineering efforts through the final 21 shuttle flights. She later served as the first chief engineer for the Space Launch System’s Liquid Engines Element, helping advance the propulsion systems supporting NASA’s Artemis missions.

As Marshall’s chief engineer and, since 2023, NASA’s deputy chief engineer, Van Hooser provided critical technical leadership and oversight across the agency’s programs. Her steady guidance through complex engineering challenges and organizational transitions helped maintain continuity, strengthen collaboration, and keep mission readiness at the forefront of NASA’s work.

Learn more about NASA’s missions on the agency’s website:

https://www.nasa.gov/

George Alderman / Cheryl Warner
Headquarters, Washington
202-358-1600
[email protected] / [email protected]

Details

Last Updated

Oct 13, 2026

Source: www.nasa.gov

NASA Astronauts to Answer Questions from Florida Students

NASA astronaut Jessica Watkins assists NASA astronaut Luke Delaney as he practices suiting up in a spacesuit in an International Space Station airlock simulator on May, 5, 2026, at the agency's Johnson Space Center Space Vehicle Mockup Facility in Houston.
NASA astronaut Jessica Watkins assists NASA astronaut Luke Delaney as he practices suiting up in a spacesuit in an International Space Station airlock simulator on May 5, 2026, at the agency’s Johnson Space Center Space Vehicle Mockup Facility in Houston.
Credit: NASA

Students in Florida will hear from NASA astronauts Jessica Watkins and Luke Delaney as they answer prerecorded STEM questions while aboard the International Space Station.

The Earth-to-space call will begin at 12 p.m. EDT Friday, Oct. 16, and will stream live on the agency’s Learn With NASA YouTube channel.

This event is hosted by Sally Ride Elementary School in Orlando, Florida, for students in grades K-12, and the community. This unique opportunity aims to deepen understanding of space exploration and enhance awareness of STEM careers.

Media interested in covering the event must RSVP no later than 5 p.m. EDT, Thursday, Oct. 15, to Jenny Morgan at (407) 858-3100, or at [email protected].

For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs not possible on Earth. The space station helps NASA understand and overcome the challenges of human spaceflight, expand commercial opportunities in low Earth orbit, and build on the foundation for long-duration missions to the Moon, as part of the Artemis program, and to Mars.

For more information on NASA in-flight calls, visit:

https://www.nasa.gov/stemonstation

Source: www.nasa.gov