How do I Spot The Station?

How do I Spot The Station?

What does all this sighting information mean?

SpotTheStation! Time:  Wed Apr 25 7:45 PM, Visible: 4 min,  Max Height: 66 degrees,  Appears: WSW,  Disappears NE.”

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The International Space Station is seen in this 30 second exposure as it flies over Elkton, VA early in the morning, Saturday, August 1, 2015.
The International Space Station is seen in this 30 second exposure as it flies over Elkton, VA early in the morning, Saturday, August 1, 2015.
NASA/Bill Ingalls
  • Time is when the sighting opportunity will begin in your local time zone. All sightings will occur within a few hours before or after sunrise or sunset. This is the optimum viewing period as the sun reflects off the space station and contrasts against the darker sky.
  • Visible is the maximum time period the space station is visible before crossing back below the horizon.
  • Max Height is measured in degrees (also known as elevation). It represents the height of the space station from the horizon in the night sky. The horizon is at zero degrees, and directly overhead is ninety degrees. If you hold your fist at arm’s length and place your fist resting on the horizon, the top will be about 10 degrees.
  • Appears is the location in the sky where the station will be visible first. This value, like maximum height, also is measured in degrees from the horizon. The letters represent compass directions — N is north, WNW is west by northwest, and so on.
  • Disappears represents where in the night sky the International Space Station will leave your field of view.
The International Space Station orbits with an inclination of 51.6 degrees. This means that, as it orbits, the farthest north and south of the Equator it will ever go is 51.6 degrees latitude. If you live north or south of 51.6 degrees, the ISS will never go directly over your head- this includes places like Alaska. Spot The Station may not properly inform you of all visible space station passes in these locations. Spot The Station's sighting opportunities pages will give you a list of all possible space station sightings for your location.
The International Space Station orbits with an inclination of 51.6 degrees. This means that, as it orbits, the farthest north and south of the Equator it will ever go is 51.6 degrees latitude. If you live north or south of 51.6 degrees, the ISS will never go directly over your head- this includes places like Alaska. Spot The Station may not properly inform you of all visible space station passes in these locations. Spot The Station’s sighting opportunities pages will give you a list of all possible space station sightings for your location.
NASA

Important: The International Space Station orbits with an inclination of 51.6 degrees. This means that, as it orbits, the farthest north and south of the Equator it will ever go is 51.6 degrees latitude. If you live north or south of 51.6 degrees, the ISS will never go directly over your head- this includes places like Alaska. Spot The Station may not properly inform you of all visible space station passes in these locations. Spot The Station’s sighting opportunities pages will give you a list of all possible space station sightings for your location.

The space station looks like an airplane or a very bright star moving across the sky, except it doesn’t have flashing lights or change direction. It will also be moving considerably faster than a typical airplane (airplanes generally fly at about 600 miles (965 km) per hour; the space station flies at 17,500 miles (28,000 km) per hour).

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Mark A. Garcia

Spot the Station Frequently Asked Questions

Spot the Station Frequently Asked Questions

Aurora in brilliant green photographed from orbit with Earth below and crater visible on landscape
An astronaut aboard the International Space Station adjusted the camera for night imaging and captured the green veils and curtains of an aurora that spanned thousands of kilometers over Quebec, Canada.
NASA

Why is the space station up there?

The space station is Earth’s only microgravity laboratory. This football field-sized platform hosts a plethora of science and technology experiments that are continuously being conducted by crew members, or are automated. Research aboard the orbiting laboratory holds benefits for life back on Earth, as well as for future space exploration. The space station serves as a testbed for technologies and allows us to study the impacts of long-term spaceflight to humans, supporting NASA’s mission to push human presence farther into space. Learn more about the research happening on the space station, and opportunities to conduct your science there.

The sighting opportunity schedule indicates that the space station passed over my house last night; I’m signed up for alerts but didn’t get one, why not?

You will only receive an alert if the space station will reach a max height of at least 40° on flyover. Flyovers reaching at least 40° provide the best chance for a sighting opportunity because they are visible above most landscapes and buildings. Check the “Max Height” column of your sighting opportunity schedule for the flyovers that are 40° or more.

The flyover schedule indicates the space station is both appearing and disappearing from the same direction, how is that possible? E.g. – Time: Mon Jul 15 11:57 PM, Visible: 2 min, Max Height: 51°, Appears: 51° above ENE, Disappears: 11° above ENE

The Spot the Station software rounds off directions to the nearest cardinal and intracardinal directions. This can result in it seeming as though the ISS will be appearing and disappearing in the same direction even though it is traveling across the sky. This typically happens on flyovers with a short window of visibility because the ISS is quickly moving into (or out of) the Earth’s dark shadow where, from our location on the ground, we can’t observe its full pass across the sky.

How often can I expect to see the space station?

The space station is visible because it reflects the light of the Sun – the same reason we can see the Moon. However, unlike the Moon, the space station isn’t bright enough to see during the day. It can only be seen when it is dawn or dusk at your location. As such, it can range from one sighting opportunity a month to several a week, since it has to be both dark where you are, and the space station has to happen to be going overhead.

Why aren’t there any sighting opportunities for my location?

It needs to be dark where you are and the space station needs to be overhead in order for you to see it. Since the space station’s orbit takes it all around the globe, it can be passing over you at times when it will not be visible- either in the middle of the day or the middle of the night. The space station must be 40 degrees or more above the horizon for it to be visible. Spot The Station will only send out notifications when you will have an opportunity to see the space station, not every time it will be overhead.

Do I need a telescope to see the space station?

No, you can see the space station with your bare eyes, no equipment required.

Can you explain how to identify the space station in the sky? Did I see the space station last night?

The space station looks like an airplane or a very bright star moving across the sky, except it doesn’t have flashing lights or change direction. It will also be moving considerably faster than a typical airplane (airplanes generally fly at about 600 miles (965 km) per hour; the space station flies at 17,500 miles (28,000 km) per hour).

Can you explain how to read the alert messages?

What does all this sighting information mean?

  • Time is when the sighting opportunity will begin in your local time zone. All sightings will occur within a few hours before or after sunrise or sunset. This is the optimum viewing period as the sun reflects off the space station and contrasts against the darker sky.
  • Visible is the maximum time period the space station is visible before crossing back below the horizon.
  • Max Height is measured in degrees (also known as elevation). It represents the height of the space station from the horizon in the night sky. The horizon is at zero degrees, and directly overhead is ninety degrees. If you hold your fist at arm’s length and place your fist resting on the horizon, the top will be about 10 degrees.
  • Appears is the location in the sky where the station will be visible first. This value, like maximum height, also is measured in degrees from the horizon. The letters represent compass directions — N is north, WNW is west by northwest, and so on.
  • Disappears represents where in the night sky the International Space Station will leave your field of view.
The International Space Station orbits with an inclination of 51.6 degrees. This means that, as it orbits, the farthest north and south of the Equator it will ever go is 51.6 degrees latitude. If you live north or south of 51.6 degrees, the ISS will never go directly over your head- this includes places like Alaska. Spot The Station may not properly inform you of all visible space station passes in these locations. Spot The Station's sighting opportunities pages will give you a list of all possible space station sightings for your location.
The International Space Station orbits with an inclination of 51.6 degrees. This means that, as it orbits, the farthest north and south of the Equator it will ever go is 51.6 degrees latitude. If you live north or south of 51.6 degrees, the ISS will never go directly over your head- this includes places like Alaska. Spot The Station may not properly inform you of all visible space station passes in these locations. Spot The Station’s sighting opportunities pages will give you a list of all possible space station sightings for your location.
NASA

How fast is the space station travelling?

The ISS circles the Earth every 90 minutes. It travels at about 17,500 miles (28,000 km) per hour, which gives the crew 16 sunrises and sunsets every day. In the more than 15 years that people have been living onboard, the Station has circumnavigated the Earth tens of thousands of times. You can see more facts about the ISS on the Space Station: Facts and Figures webpage .

Does the station appear and then disappear because of the light of the Moon?

The space station is visible because it is reflecting light from the Sun. This is the same reason that the Moon appears to shine. Even when the Moon hasn’t risen, you’ll still be able to see the space station.

I haven’t received any emails or text messages.

If you signed up, entered your registration code and received an on-screen confirmation message then you’re signed up! Chances are the International Space Station just hasn’t passed over your location at dawn or dusk yet. Read the FAQ “Why aren’t there any sighting opportunities for my location” for more information.

If you signed up with your email address, check your spam folder to see if alert messages are going there. Add SpotTheStation@hq.nasa.gov to your list of allowed senders to prevent alerts from going to spam or junk email.

I haven’t received the code for sign up / renewal / unsubscribe?

If you signed up by email make sure the email containing the code didn’t end up in your spam folder. This email will appear to come from noreply@nasa.gov.

Add the SpotTheStation@hq.nasa.gov email address to your list of allowed senders.

If it has been more than one hour and you haven’t received the requested code please try the process again and if you’re still have problems, email us at SpotTheStation@hq.nasa.gov for assistance.

What if my city isn’t listed?

If your specific city or town isn’t listed, register using the next closest one. The space station is visible for an approximate 50 mile (80 km) radius around each of the listed locations.

When are alerts sent out?

Alerts are generally sent about 24 hours before the International Space Station pass. This means you’ll receive the message the night before for a morning pass and the morning of for an evening pass.

If you are not receiving the alerts on time, see related FAQs for an explanation.

Why am I receiving the alerts hours or even days after sightings?

Spot The Station alerts are sent out 24 hours before an upcoming space station pass. Unfortunately, some email providers queue messages in an unpredictable way. Adding SpotTheStation@hq.nasa.gov to list of allowed senders or contacts list might help.

You can also obtain a two-week schedule of space station passes from the website. Please see the next FAQ for details.

How can I receive a two-week schedule of upcoming sightings?

Visit the Sighting Opportunities page and enter your location to find out when the space station will be passing over you during the next two weeks.

You can bookmark this page or print the schedule for easy access.

Can I register more than one location to the same email address or phone number?

Unfortunately, no. Only one location can be registered per email address or mobile phone number. However, if you have multiple email addresses and/or both an email address and a mobile phone, you can register each of them to receive alerts for different locations.

I am getting errors when I try to register, renew or cancel my alerts.

“The email address / mobile number you entered is not valid” – Make sure you have entered a properly formatted email or SMS address. Mobile phone numbers do not require any formatting, you can simply enter as a string of digits; special characters like parenthesis and dashes are not required.

“The email address / mobile number you provided cannot be found” – You are attempting to renew or cancel alerts for an email address or mobile number that does not appear to be registered.

“It looks like you have already attempted this process but not yet completed it. Please check your email or text messages for an 8-digit code and instructions to complete the process or wait 24-hours and try again.” – You will receive this error message if you try to initiate the same request more than three times without entering your 8-digit code to complete the process. Please complete your request now or wait 24-hours and try again.

“The code you entered is not valid. Please try again.” – If you have received this message, verify the correct 8-digit code is entered and that the code is less than 24-hours old. Codes expire after 24-hours at which point a new code will be required.

“You must cancel your current alert before creating a new one or create a new alert using a different email address or mobile number.” – You can only sign up for one alert per email address or mobile number. If you want to change the alert you are receiving you have to cancel the existing alert and sign up for a new one. If you wish to have alerts sent to you for more than one location you can sign up using different email addresses or mobile numbers.

“You have already completed your sign up / renewal / cancellation” – You will receive this error message if you attempt to enter your 8-digit code more than once. No further action is required.

“You have exceeded the number of incomplete requests allowed from your IP address. Please wait 24-hours and try again.” – To prevent spam, Spot The Station limits the number of incomplete requests allowed from each IP address. Please complete your request now or wait 24-hours and try your request again

If you are receiving other error messages or continue to have trouble, please let us know.

What time zone is used for alert notifications?

All of the Spot The Station information is listed in the local time zone for the selected location. Spot The Station automatically adjusts for Daylight Saving Time.

What email address should I add to my “Allow/Safe Senders List” so I can make sure my alerts don’t end up in the spam folder?

The correct address is SpotTheStation@hq.nasa.gov

How do I change my email address or phone number?

In order to update your email address or phone number, you need to register using a different email address or mobile phone number. If you choose, you can cancel your original alert.

I moved, how can I change my location?

In order to change your location you need to cancel your existing alert and register again using the new location information.

What is my SMS Address?

Your SMS Address is an email address used to send text messages to mobile phones. The format is your 10-digit mobile number followed by the email address of your mobile carrier. For example, an AT&T SMS address would be 12345678910@text.att.net. Check with your individual carrier for their format.

Will I get charged for the mobile phone text alerts?

Check with your mobile carrier and the service plan you have to find out if you are charged for text messages. NASA’s Spot The Station is not responsible for any charges associated with the alerts.

How will I know when it’s necessary for me to renew my alert registration?

Your registration is good for one year. Spot The Station will email you when it is time to renew your registration so you can continue to receive alerts. This is a one-step process; all you need to do is follow the link in the renewal message.

How do I unsubscribe from alerts?

You can stop receiving email or mobile phone alerts by canceling them here. You will be sent an email or text message, simply follow the link provided in that message to complete your request.

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Mark A. Garcia

2024 NESC Technical Update

2024 NESC Technical Update

1 Min Read

2024 NESC Technical Update

Cover of the 2024 NESC Technical Update

Annual Report of NESC Technical Activities

On behalf of the NASA Engineering and Safety Center (NESC), I am pleased to provide you with the 2024 NESC Technical Update. This annual report summarizes the technical work, engineering advancements, and knowledge capture efforts we made in FY24. With support provided by members of our NASA community from across the centers, we focused our efforts on performing value-added independent testing, analysis, and assessments of NASA’s high-risk projects to ensure safety and mission success.

This report contains summaries of technical assessments requested by our stakeholders and the technical bulletins and innovative techniques that resulted from that assessment work. Several of the NASA Technical Fellows provide summaries of accomplishments in their respective disciplines, and expertise drawn from across the Agency is featured on the Center Pages. 

We appreciate the opportunity to share our progress and highlight the accomplishments of our technically and culturally diverse, multidisciplinary, multigenerational teams. All NESC knowledge products are available at nasa.gov/nesc. As always, we value your feedback and engagement. Thank you for your continuing support of the NESC.

Timmy R. Wilson

Director, NASA Engineering and Safety Center

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Daniel Hoffpauir

La NASA comparte resultados del escudo térmico de Orion, actualiza las misiones Artemis

La NASA comparte resultados del escudo térmico de Orion, actualiza las misiones Artemis

Read this release in English here.

Mediante la campaña Artemis, la NASA llevará a los siguientes astronautas estadounidenses y al primer astronauta internacional a la región del Polo Sur de la Luna. El jueves, la NASA anunció las últimas actualizaciones de sus planes de exploración lunar.

Un grupo de expertos examinó los resultados de la investigación de la NASA sobre el escudo térmico de la nave Orion, tras haber sufrido una inesperada pérdida de material carbonizado en su reentrada en la atmósfera durante el vuelo de prueba sin tripulación Artemis I. Para el vuelo de prueba tripulado Artemis II, los ingenieros seguirán preparando a Orion con el escudo térmico ya montado en la cápsula.

La agencia también anunció que ahora apunta a abril de 2026 para el lanzamiento de Artemis II y a mediados de 2027 para Artemis III. Los plazos actualizados de las misiones también contemplan el tiempo necesario para abordar los sistemas de control medioambiental y de soporte vital de Orion.

“La campaña Artemis es la iniciativa internacional más audaz, técnicamente desafiante y colaborativa que la humanidad se haya propuesto jamás”, dijo el administrador de la NASA, Bill Nelson. “Hemos logrado avances significativos en la campaña Artemis durante los últimos cuatro años, y estoy orgulloso del trabajo que nuestros equipos técnicos han hecho para prepararnos para este próximo paso adelante en la exploración, ya que buscamos aprender más sobre los sistemas de soporte vital de Orion para sustentar las operaciones de la tripulación durante Artemis II. Tenemos que hacer bien este próximo vuelo de prueba. Así es como la campaña Artemis triunfará”.

La decisión de la agencia se produce después de que una investigación exhaustiva de un problema con el escudo térmico de Artemis I demostrara que el escudo térmico de Artemis II es capaz de mantener a salvo a la tripulación durante la misión planeada con modificaciones en la trayectoria de Orion cuando entre en la atmósfera terrestre y reduzca su velocidad de unos 40.000 kilómetros por hora (casi 25.000 millas por hora) a unos 520 km/h (unas 325 mph) antes de que sus paracaídas se desplieguen para un amerizaje seguro en el océano Pacífico.

“Durante todo nuestro proceso para investigar el fenómeno del escudo térmico y determinar un camino a seguir, nos hemos mantenido fieles a los valores fundamentales de la NASA; pusimos primero la seguridad y el análisis basado en datos”, dijo Catherine Koerner, administradora asociada de la Dirección de Misión de Desarrollo de Sistemas de Exploración en la sede de la NASA en Washington. “Las actualizaciones de nuestros planes de misión son un paso positivo para asegurar que podemos cumplir con seguridad nuestros objetivos en la Luna y desarrollar las tecnologías y capacidades necesarias para las misiones tripuladas a Marte.”

La NASA seguirá acoplando los componentes de su cohete Sistema de Lanzamiento Espacial o SLS (un proceso que comenzó en noviembre) y lo preparará para su integración con Orion para Artemis II.

Durante el otoño boreal, la NASA, junto con un equipo de revisión independiente, estableció la causa técnica de un problema observado tras el vuelo de prueba sin tripulación Artemis I, en el que el material carbonizado del escudo térmico se desgastó de forma distinta a la esperada. Un análisis exhaustivo, que incluyó más de 100 pruebas en distintas instalaciones por todo el país, determinó que el escudo térmico de Artemis I no permitía evacuar suficientemente los gases generados en el interior de un material denominado Avcoat, lo que provocó que parte del material se agrietara y se desprendiera. El Avcoat está diseñado para desgastarse a medida que se calienta y es un material clave en el sistema de protección térmica que resguarda a Orion y a su tripulación de los casi 5.000 grados Fahrenheit de temperatura (2.760 grados Celsius) que se generan cuando Orion atraviesa la atmósfera terrestre al regresar de la Luna. Aunque durante Artemis I no había tripulación a bordo de Orion, los datos muestran que la temperatura en el interior de Orion hubiera sido agradable y segura de haber habido tripulación a bordo.

Los equipos de ingeniería ya están ensamblando e integrando la nave Orion para Artemis III basándose en las lecciones aprendidas de Artemis I e implementando mejoras en la forma de fabricar los escudos térmicos para los retornos de las misiones tripuladas de alunizaje con el fin de lograr uniformidad y permeabilidad constante. La reentrada atmosférica doble (“skip entry”) es necesaria para el retorno desde las velocidades previstas para las misiones de alunizaje.

“Victor, Christina, Jeremy y yo hemos estado siguiendo todos los aspectos de esta decisión y estamos agradecidos por la disposición de la NASA a sopesar todas las opciones y tomar decisiones en el mejor interés de los vuelos espaciales tripulados. Estamos entusiasmados por volar con la misión Artemis II y seguir allanando el camino para la exploración humana continua de la Luna y Marte”, declaró Reid Wiseman, astronauta de la NASA y comandante de Artemis II. “Hace poco estuvimos en el Centro Espacial Kennedy de la agencia en Florida y pudimos ver los propulsores de nuestro cohete SLS, la etapa central y la nave Orion. Es inspirador ver la escala de este esfuerzo, conocer a las personas que trabajan en esta máquina, y no podemos esperar a hacerla volar a la Luna”.

Wiseman, junto con los astronautas de la NASA Victor Glover y Christina Koch y el astronauta de la CSA (Agencia Espacial Canadiense) Jeremy Hansen, volarán a bordo del vuelo de prueba Artemis II, de 10 días de duración, alrededor de la Luna y de regreso. El vuelo proporcionará datos valiosos sobre los sistemas de Orion necesarios para sustentar a la tripulación en su viaje al espacio profundo y traerlos sanos y salvos de vuelta a casa, incluyendo la renovación del aire en la cabina, las funciones de vuelo manual y cómo interactúan los humanos con el resto del hardware y software de la nave espacial.

Con Artemis, la NASA explorará más de la Luna que nunca, aprenderá a vivir y trabajar más lejos de nuestro hogar y se preparará para la futura exploración humana del planeta rojo. El SLS de la NASA, los sistemas terrestres de exploración y la nave Orion, junto con el sistema de aterrizaje para seres humanos, los trajes espaciales de nueva generación, la estación espacial lunar Gateway y los futuros vehículos exploradores son los cimientos de la NASA para la exploración del espacio profundo.

Para más información sobre Artemis (en inglés), visita:

https://www.nasa.gov/artemis

-fin-

Meira Bernstein / Rachel Kraft / María José Viñas
Sede, Washington
202-358-1600
meira.b.bernstein@nasa.gov / rachel.h.kraft@nasa.gov / maria-jose.vinasgarcia@nasa.gov

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Abbey A. Donaldson

NASA Flights Map Critical Minerals from Skies Above Western US

NASA Flights Map Critical Minerals from Skies Above Western US

6 min read

NASA Flights Map Critical Minerals from Skies Above Western US

A hilly landscape is dotted with colors ranging from bright yellow to deep purple and blue, indicating the presence of different types of minerals.
Various minerals are revealed in vibrant detail in this sample mineral map of Cuprite, Nevada, following processing of imaging spectrometer data.
Credit: USGS

On a crystal-clear afternoon above a desert ghost town, a NASA aircraft scoured the ground for minerals.

The plane, a high-altitude ER-2 research aircraft, had taken off early that morning from NASA’s Armstrong Flight Research Center in Edwards, California. Below pilot Dean Neeley, the landscape looked barren and brown. But to the optical sensors installed on the plane’s belly and wing, it gleamed in hundreds of colors.

Neeley’s flight that day was part of GEMx, the Geological Earth Mapping Experiment led by NASA and the U.S. Geological Survey to map critical minerals across more than 190,000 square miles (500,000 square kilometers) of North American soil. Using airborne instruments, scientists are collecting these measurements over parts of California, Nevada, Arizona, and Oregon. That’s an area about the size of Spain.   

Against a bright blue sky streaked with clouds, a white airplane soars over snowy mountains.
An ER-2 science aircraft banks away during a flight over the southern Sierra Nevada. The high-altitude plane supports a wide variety of research missions, including the GEMx campaign, which is mapping critical minerals in the Western U.S. using advanced airborne imaging developed by NASA.
Credit: NASA/Carla Thomas

Lithium, aluminum, rare earth elements such as neodymium and cerium — these are a few of the 50 mineral commodities deemed essential to U.S. national security, to the tech industry, and to clean energy. They support a wide range of technologies from smartphones to steelmaking, from wind turbines to electric vehicle batteries. In 2023, the U.S. imported its entire supply of 12 of these minerals and imported at least 50% of its supply of another 29.

The GEMx team believes that undiscovered deposits of at least some of these minerals exist domestically, and modern mineral maps will support exploration by the private sector.

“We’ve been exploring the earth beneath our feet for hundreds of years, and we’re discovering that we’ve only just begun,” said Kevin Reath, NASA’s associate project manager for GEMx.

The View From 65,000 Feet

To jumpstart mineral exploration, USGS is leading a nationwide survey from the inside out, using tools like lidar and magnetic-radiometric sensors to probe ancient terrain in new detail.

The collaboration with NASA brings another tool to bear: imaging spectrometers. These advanced optical instruments need to stay cold as they fly high. From cryogenic vacuum chambers on planes or spacecraft, they detect hundreds of wavelengths of light — from the visible to shortwave infrared — reflected off planetary surfaces. The technology is now being used to help identify surface minerals across dry, treeless expanses of the Western U.S.

Every molecule reflects a unique pattern of light, like a fingerprint. Processed through a spectroscopic lens, a desert expanse can appear like an oil painting popping with different colorful minerals, including pale-green mica, blue kaolinite, and plummy gypsum.

“We’re not digging for gold. We’re revealing what’s hidden in plain sight,” said Robert Green, a researcher at NASA’s Jet Propulsion Laboratory in Southern California, who helped pioneer spectroscopic imaging at NASA JPL in the late 1970s. Like many of the scientists involved with GEMx, he has spent years surveying other worlds, including the Moon and Mars.

A handful of such instruments exist on Earth, and Green is in charge of two of them. One, called EMIT (Earth Surface Mineral Dust Source Investigation) flies aboard the International Space Station. Surveying Earth’s surface from about 250 miles (410 kilometers) above, EMIT has captured thousands of images at a resolution of 50 by 50 miles (80 by 80 kilometers) in a wide belt around Earth’s mid-section.

The other instrument rides beneath the fuselage of the ER-2 aircraft. Called AVIRIS (Airborne Visible/Infrared Imaging Spectrometer), it’s helping guide geologists to critical minerals directly and indirectly, by spotting the types of rocks that often contain them. It’s joined by another instrument developed by NASA, the MODIS/ASTER Airborne Simulator (MASTER), which senses thermal infrared radiance. Both instruments provide finely detailed measurements of minerals that complement what EMIT sees on a broader scale.

A man in a yellow spacesuit and American flag-helmet sits on a chair as another man in a NASA shirt connects tubing between the suit and equipment on a table.
A crew of life support staff prepare pilot Dean Neeley for an ER-2 flight. A specialized suit – similar to an astronaut’s – allows the pilot to work, breathe, and eat at altitudes almost twice as high as a cruising passenger jet.
Credit: NASA/Carla Thomas

Old Mines, New Finds

In and around the multimillion-year-old magmas of the Great Basin of the Western U.S., lithium takes several forms. The silvery metal is found in salty brines, in clay, and locked in more than 100 different types of crystals. It can also be detected in the tailings of abandoned prospects like Hector Mine, near Barstow, California.

Abandoned years before a magnitude 7.1 earthquake rocked the region in 1999, the mine is located on a lode of hectorite, a greasy, lithium-bearing clay. Geologists from USGS are taking a second look at legacy mines like Hector as demand for lithium rises, driven primarily by lithium-ion batteries. A typical battery pack in an electric vehicle uses about 17 pounds (eight kilograms) of the energy-dense metal.

Australia and Chile lead worldwide production of lithium, which exceeded 180,000 tons in 2023. The third largest producer is China, which also hosts about 50% of global lithium refining capacity. Total U.S. production was around 1,000 tons, sourced entirely from a deposit in northern Nevada. Known reserves in the state are estimated to contain more than a million metric tons of lithium, according to data collected by the Nevada Bureau of Mines and Geology.

Mine wastes are also potential sources of lithium, said Bernard Hubbard, a remote sensing geologist at USGS, and many other byproduct commodities that are considered critical today but were discarded by previous generations.

“There are old copper and silver mines in the West that were abandoned long before anyone knew what lithium or rare earth element deposits were,” Hubbard said. “What has been a pollution source for communities could now be a resource.”

Following a winter pause, high-altitude GEMx flights over the American West will resume in the spring of 2025, after which USGS will process the raw data and release the first mineral maps. Already, the project has collected enough data to start producing a complete hyperspectral map of California — the first of its kind.

The value of these observations extends beyond identifying minerals. Scientists expect they’ll provide new insight into invasive plant species, waste from mines that can contaminate surrounding environments, and natural hazards such as earthquakes, landslides, and wildfires.

“We are just beginning to scratch the surface in applying these measurements to help the nation’s economy, security, and health,” said Raymond Kokaly, USGS research geophysicist and lead of the GEMx survey.

More About GEMx

The GEMx research project will last four years and is funded by the USGS Earth Mapping Resources Initiative (EarthMRI), through investments from the Bipartisan Infrastructure Law. The initiative will capitalize on both the technology developed by NASA for spectroscopic imaging as well as the expertise in analyzing the datasets and extracting critical mineral information from them.

Data collected by GEMx is available here.

By Sally Younger
NASA’s Earth Science News Team

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Last Updated
Dec 05, 2024
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