Thursday, September 25, 2025

Liftoff: Amazon Project Kuiper Satellites on Atlas V Rocket | United Launch Alliance

Liftoff: Amazon Project Kuiper Satellites on Atlas V Rocket | United Launch Alliance

A United Launch Alliance (ULA) Atlas V rocket lifts off from Space Launch Complex-41 at Cape Canaveral on Sept. 25, 2025 at 8:09 a.m. EDT carrying the Kuiper 3 mission for Amazon's Project Kuiper broadband satellite constellation. The ULA Atlas V 551 mission launched 27 operational broadband satellites, bringing the total number of Project Kuiper satellites launched by ULA to 81.

Project Kuiper is Amazon's low Earth orbit (LEO) satellite broadband network. Its mission is to provide fast, reliable Internet access to customers around the world, including those in unserved and underserved communities, using a constellation of more than 3,200 LEO satellites.



Credit: United Launch Alliance (ULA)
Duration: 19 seconds
Release Date: Sept. 25, 2025


#NASA #Space #Earth #Satellites #LEO #Amazon #ProjectKuiper #Kuiper3Mission #SatelliteConstellations #CommunicationsSatellites #BroadbandInternetServices #AtlasVRockets #ULA #CapeCanaveral #Florida #UnitedStates #CommercialSpace #STEM #Education #HD #Video

Atlas V Rocket Liftoff: Amazon Project Kuiper Satellites | United Launch Alliance

Atlas V Rocket Liftoff: Amazon Project Kuiper Satellites | United Launch Alliance








A United Launch Alliance (ULA) Atlas V rocket lifts off from Space Launch Complex-41 at Cape Canaveral on Sept. 25, 2025 at 8:09 a.m. EDT carrying the Kuiper 3 mission for Amazon's Project Kuiper broadband satellite constellation. The ULA Atlas V 551 mission launched 27 operational broadband satellites, bringing the total number of Project Kuiper satellites launched by ULA to 81.

Project Kuiper is Amazon's low Earth orbit (LEO) satellite broadband network. Its mission is to provide fast, reliable Internet access to customers around the world, including those in unserved and underserved communities, using a constellation of more than 3,200 LEO satellites.

United Launch Alliance (ULA) update:
https://newsroom.ulalaunch.com/releases/united-launch-alliance-propels-amazons-project-kuiper-to-enhance-broadband-access-to-connect-the-world


Credit: United Launch Alliance (ULA)
Release Date: Sept. 25, 2025


#NASA #Space #Earth #Satellites #LEO #Amazon #ProjectKuiper #Kuiper3Mission #SatelliteConstellations #CommunicationsSatellites #BroadbandInternetServices #AtlasVRockets #ULA #CapeCanaveral #Florida #UnitedStates #CommercialSpace #STEM #Education

Behind The Scenes: IMAP, SWFO-L1 & Carruthers Missions Pre-launch | NASA

Behind The Scenes: IMAP, SWFO-L1 & Carruthers Missions Pre-launch | NASA

A SpaceX Falcon 9 rocket with the National Oceanic and Atmospheric Administration's SWFO-L1 spacecraft and NASA’s IMAP and Carruthers Geocorona Observatory stands vertical at Launch Complex 39A during early morning on Monday, Sept. 22, 2025, at the agency’s Kennedy Space Center in Florida.
A SpaceX Falcon 9 rocket, with NASA’s IMAP and Carruthers Geocorona Observatory, as well as the National Oceanic and Atmospheric Administration's SWFO-L1 spacecraft attached, rolls to Launch Pad 39A on September 21, 2025, at NASA’s Kennedy Space Center in Florida.
A SpaceX Falcon 9 rocket, with NASA’s IMAP and Carruthers Geocorona Observatory, as well as the National Oceanic and Atmospheric Administration's SWFO-L1 spacecraft attached, rolls to Launch Pad 39A on Sunday, Sept. 21, 2025, at NASA’s Kennedy Space Center in Florida. 
The National Oceanic and Atmospheric Administration's SWFO-L1, along with NASA's Interstellar Mapping and Acceleration Probe (IMAP) and Carruthers Geocorona Observatory fully integrated for launch.
Technicians integrate NASA’s Carruthers Geocorona Observatory and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On Lagrange - 1 (SWFO-L1) satellite to the Evolved Expendable Launch Vehicle Secondary Payload Adapter Array Ring (ESPA) inside the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida on Friday, Sept. 5, 2025.

Technicians integrate NASA’s Carruthers Geocorona Observatory and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On Lagrange - 1 (SWFO-L1) satellite to the Evolved Expendable Launch Vehicle Secondary Payload Adapter Array Ring (ESPA) inside the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida on Friday, Sept. 5, 2025.
The integration of the rideshares prepares for the next milestone of attaching NASA’s IMAP (Interstellar Mapping and Acceleration Probe) Sun mapping observatory to a payload adapter and stacking all three observatories together to prepare them for encapsulation in the payload fairing.
The National Oceanic and Atmospheric Administration's SWFO-L1 Observatory successfully positioned above a work stand during pre-launch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory above a work stand for integrations on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida.

A SpaceX Falcon 9 rocket successfully launched and deployed NASA’s Interstellar Mapping and Acceleration Probe (IMAP), the agency’s Carruthers Geocorona Observatory, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft. Launch took place on schedule at 7:30 a.m. EDT, Wednesday, Sept. 24, 2025, from Launch Complex 39A at NASA's Kennedy Space Center in Florida. 

The missions will each focus on different effects of the solar wind—the continuous stream of particles emitted by the Sun—and space weather—the changing conditions in space driven by the Sun—from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system. 

The Interstellar Mapping and Acceleration Probe (IMAP) will explore and map the heliosphere—the invisible cosmic shield surrounding our solar system—to answer great unknowns about how particles accelerate in the solar wind.


NASA’s Carruthers Geocorona Observatory is a small satellite that will observe Earth’s outermost atmospheric layer, the exosphere. It will image the faint glow of ultraviolet light from this region, called the geocorona, to better understand how space weather impacts our planet. The Carruthers mission continues the legacy of the Apollo era, expanding on measurements first taken during Apollo 16.

The SWFO-L1 spacecraft will monitor space weather and detect solar storms in advance, serving as an early warning beacon for potentially disruptive space weather, helping safeguard Earth’s critical infrastructure and technological-dependent industries. The SWFO-L1 spacecraft is the first NOAA observatory designed specifically for and fully dedicated to continuous, operational space weather observations.

Credit: SpaceX/NOAA/BAE Space & Mission Systems
Dates: Sept. 21-24, 2025


#NASA #NOAA #Space #Astronomy #Science #IMAPMission #IMAP #Stars #InterstellarMedium #ISM #Sun #Heliophysics #Heliosphere #Planets #Earth #SolarSystem #SolarPlasma #SolarWind #SpaceWeather #PrincetonU #SWFOL1 #CarruthersGeocoronaObservatory #GSFC #SpaceX #Falcon9Rocket #KSC #Florida #UnitedStates #STEM #Education

Planet Earth Aerosols: Inside the Visualization | NASA Goddard

Planet Earth Aerosols: Inside the Visualization | NASA Goddard

NASA uses satellites, ground measurements, and powerful computer models to track tiny particles floating in our air called aerosols. These small particles can travel thousands of miles, affecting the air we breathe and how far we can see, even far from where they originated. This visualization shows how these particles moved through Earth's atmosphere between August 1 and September 14, 2024.

Each color represents a type of aerosol: sea salt (blue), dust (pink/magenta), smoke from fires (orange/red), and sulfates from pollution and volcanoes (green). This visualization is based on NASA's Goddard Earth Observing System (GEOS) model. It provides realistic, high-resolution weather and aerosol data that enables customized environmental prediction and advances in artifical intelligence (AI) research.


Credit: NASA's Goddard Space Flight Center
Emme Watkins (eMITS): Lead Producer
Kathleen Greer (GSFC AMA): Lead Producer
Lesley Ott (HQ): Lead Scientist
Joseph V. Ardizzone (NASA/GSFC): Visualizer
Helen-Nicole Kostis (USRA): Visualizer
Duration: 3 minutes
Release Date: Sept. 25, 2025

#NASA #Space #Satellites #Science #Planets #Earth #Atmosphere #AirQuality #Aerosols #WildfireSmoke #Dust #Volcanoes #AirPollution #ClimateModels #ClimateChange #GlobalHeating #Climate #Environment #EarthObservation #RemoteSensing #GEOS #ArtificialIntelligence #AI #GSFC #UnitedStates #STEM #Education #Visualization #HD #Video

China Smart Dragon-3 Commercial Satellite Rocket Launch (Ship-based)

China Smart Dragon-3 Commercial Satellite Rocket Launch (Ship-based)





Lifting off at 07:56 UTC September 24, 2025, a Smart Dragon 3 (Jielong-3) rocket launched 11 GeeSat Geely-06 constellation satellites, plus another cubesat from the sea near Rizhao in east China's Shandong province. This was the eighth successful flight, further proving the Smart Dragon's capability to deliver 1,560 kg to a 500 km Sun-synchronous orbit. Smart Dragon-3 has a length of approximately 31 meters with a weight of 140 tons at liftoff.

The Jielong-3 rocket was developed by the China Academy of Launch Vehicle Technology (CALT), a subsidiary of the China Aerospace Science and Technology Corporation (CASC), the country’s state-owned main space contractor. The four-stage rocket is operated by China Rocket Co. Ltd., a commercial spinoff from CASC. 

The Geely-06 constellation, operated by Geely Holding Group, is a significant advancement in China's commercial satellite network. The constellation's first phase deployment includes 64 satellites, providing real-time global surface communications and supporting an extensive user base. The constellation is designed to serve 20 million users worldwide, handling up to 340 million messages per day. It supports high-frequency users and medium- to low-frequency users, transmitting 1,900-byte packets for text, voice, and images. The first phase is set to expand to 72 satellites, boosting capacity and service reliability. 

Geely is also piloting satellite-Internet of Things (IoT) technologies for smart vehicles, marine fisheries, heavy machinery, and logistics. The constellation's service frequency features strong diffraction characteristics to better ensure communication availability and reliability "above international standards".


Image Credit: CGTN
Date: Sept. 24, 2025

#NASA #Space #Satellites #Earth #China #中国 #SmartDragon3Rocket #Jielong3Rocket #捷龙三号运载火箭 #SolidFueledRocket #SeaLaunch #RocketLaunch #CALT #CASC #GeeSats #Geely06Constellation #Spaceflight #SpaceTechnology #CommercialSpace #TSLC #Rizhao #Shandong #STEM #Education

Wednesday, September 24, 2025

SpaceX Falcon 9 Launch: IMAP, SWFO-L1, & Carruthers Missions | NASA Kennedy

SpaceX Falcon 9 Launch: IMAP, SWFO-L1, & Carruthers Missions | NASA Kennedy

A SpaceX Falcon 9 rocket successfully launched and deployed NASA’s Interstellar Mapping and Acceleration Probe (IMAP), the agency’s Carruthers Geocorona Observatory, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft. Launch took place on schedule at 7:30 a.m. EDT, Wednesday, Sept. 24, 2025, from Launch Complex 39A at NASA's Kennedy Space Center in Florida. 

The missions will each focus on different effects of the solar wind—the continuous stream of particles emitted by the Sun—and space weather—the changing conditions in space driven by the Sun—from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system. 

The Interstellar Mapping and Acceleration Probe (IMAP) will explore and map the heliosphere—the invisible cosmic shield surrounding our solar system—to answer great unknowns about how particles accelerate in the solar wind.


NASA’s Carruthers Geocorona Observatory is a small satellite that will observe Earth’s outermost atmospheric layer, the exosphere. It will image the faint glow of ultraviolet light from this region, called the geocorona, to better understand how space weather impacts our planet. The Carruthers mission continues the legacy of the Apollo era, expanding on measurements first taken during Apollo 16.

The SWFO-L1 spacecraft will monitor space weather and detect solar storms in advance, serving as an early warning beacon for potentially disruptive space weather, helping safeguard Earth’s critical infrastructure and technological-dependent industries. The SWFO-L1 spacecraft is the first NOAA observatory designed specifically for and fully dedicated to continuous, operational space weather observations.

Video Credit: SpaceX
Duration: 28 seconds
Date: Sept. 24, 2025


#NASA #NOAA #Space #Astronomy #Science #IMAPMission #IMAP #Stars #InterstellarMedium #ISM #Sun #Heliophysics #Heliosphere #Planets #Earth #SolarSystem #SolarPlasma #SolarWind #SpaceWeather #PrincetonU #SWFOL1 #CarruthersGeocoronaObservatory #GSFC #SpaceX #Falcon9Rocket #KSC #Florida #UnitedStates #STEM #Education #HD #Video

Stellar Nursery Sagittarius B2: MIRI versus NIRCam Views | Webb Telescope

Stellar Nursery Sagittarius B2: MIRI versus NIRCam Views | Webb Telescope

This video shows two views of a colorful array of massive stars and glowing cosmic dust in the Sagittarius B2 (Sgr B2) molecular cloud, the most massive and active star-forming region in our Milky Way galaxy.

The first image shown is Webb’s mid-infrared instrument (MIRI) view of the Sgr B2 region in mid-infrared light with warm dust glowing brightly. To the right is one clump of clouds that captured astronomers’ attention. It is redder than the rest of the clouds in the image and corresponds to an area that other telescopes have shown to be one of the most molecularly rich regions known. 

The second image shown is the molecular cloud glow in near-infrared light, captured by Webb’s near-infrared camera (NIRCam). In this light, astronomers see more of the region’s diverse, colorful stars, but less of its gas and dust structure.

Only the brightest stars in this region emit mid-infrared light that can be picked up by Webb’s MIRI instrument. This is why the first image has so many fewer stars than that captured by Webb’s NIRCam in the second image.


Credit: NASA, ESA, CSA, STScI, A. Ginsburg (University of Florida), N. Budaiev (University of Florida), T. Yoo (University of Florida), A. Pagan (STScI), N. Bartmann (ESA/Webb)
Duration: 30 seconds
Release Date: Sept. 24, 2025


#NASA #Astronomy #Space #Science #Stars #Nebulae #SagittariusB2 #SgrB2 #MolecularClouds #Sagittarius #Constellations #MilkyWayGalaxy #Universe #SpaceTelescopes #JWST #MIRI #NIRCam #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

Close-up: Molecular Cloud Sagittarius B2 (MIRI image) | Webb Telescope

Close-up: Molecular Cloud Sagittarius B2 (MIRI image) | Webb Telescope


Webb’s mid-infrared instrument (MIRI) shows the Sagittarius B2 (Sgr B2) region in mid-infrared light, with warm dust glowing brightly. To the right is one clump of clouds that captured astronomers’ attention. It is redder than the rest of the clouds in the image and corresponds to an area that other telescopes have shown to be one of the most molecularly rich regions known. Additional analysis of this intriguing region could yield important insights into why Sgr B2 is so much more productive in making stars than the rest of the galactic center.

Only the brightest stars in this region emit mid-infrared light that can be picked up by Webb’s MIRI instrument. This is why this image has so many fewer stars than that captured by Webb’s near-infrared camera (NIRCam). The darkest areas of the image are not empty space but areas where cosmic dust and gas are so dense that light cannot penetrate them to reach the telescope.

Image Description: Cosmic clouds of pink and purple are surrounded by dark areas that appear like black space dotted with bright blue stars. A group of small clouds to the right is more red than any other area of the image.


Credit: NASA, ESA, CSA, STScI, A. Ginsburg (University of Florida), N. Budaiev (University of Florida), T. Yoo (University of Florida)
Image Processing: A. Pagan (STScI)
Duration: 30 seconds
Release Date: Sept. 24, 2025

#NASA #Astronomy #Space #Science #Stars #Nebulae #SagittariusB2 #SgrB2 #MolecularClouds #Sagittarius #Constellations #MilkyWayGalaxy #Universe #SpaceTelescopes #JWST #MIRI #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

Molecular Cloud Sagittarius B2 (MIRI image) | James Webb Space Telescope

Molecular Cloud Sagittarius B2 (MIRI image) | James Webb Space Telescope

Webb’s mid-infrared instrument (MIRI) shows the Sagittarius B2 (Sgr B2) region in mid-infrared light, with warm dust glowing brightly. To the right is one clump of clouds that captured astronomers’ attention. It is redder than the rest of the clouds in the image and corresponds to an area that other telescopes have shown to be one of the most molecularly rich regions known. Additional analysis of this intriguing region could yield important insights into why Sgr B2 is so much more productive in making stars than the rest of the galactic center.

Only the brightest stars in this region emit mid-infrared light that can be picked up by Webb’s MIRI instrument. This is why this image has so many fewer stars than that captured by Webb’s near-infrared camera (NIRCam). The darkest areas of the image are not empty space but areas where cosmic dust and gas are so dense that light cannot penetrate them to reach the telescope.

Image Description: Cosmic clouds of pink and purple are surrounded by dark areas that appear like black space dotted with bright blue stars. A group of small clouds to the right is more red than any other area of the image.


Credit: NASA, ESA, CSA, STScI, A. Ginsburg (University of Florida), N. Budaiev (University of Florida), T. Yoo (University of Florida)
Image Processing: A. Pagan (STScI)
Release Date: Sept. 24, 2025

#NASA #Astronomy #Space #Science #Stars #Nebulae #SagittariusB2 #SgrB2 #MolecularClouds #Sagittarius #Constellations #MilkyWayGalaxy #Universe #SpaceTelescopes #JWST #MIRI #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education 

Close-up: Sagittarius B2 Molecular Cloud (NIRCam image) | Webb Telescope

Close-up: Sagittarius B2 Molecular Cloud (NIRCam image) | Webb Telescope

Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s near-infrared camera (NIRCam). In this light, astronomers see more of the region’s diverse, colorful stars, but less of its gas and dust structure. Webb’s instruments each provide astronomers with important information that help build a more complete picture of what is happening in this intriguing portion of the center of our galaxy. 

Sagittarius B2 (Sgr B2) is located about 390 light years from the center of the Milky Way. This complex is the largest molecular cloud in the vicinity of the core and one of the largest in the galaxy, spanning a region about 150 light years across. The total mass of Sgr B2 is about 3 million times the mass of the Sun.

Sagittarius B2 is located only a few hundred light-years from the supermassive black hole at the heart of the galaxy called Sagittarius A*, a region densely packed with stars, star-forming clouds, and complex magnetic fields. The infrared light that Webb detects is able to pass through a portion of the area’s thick clouds to reveal young stars and the warm dust surrounding them. Astronomers think that analysis of Webb’s data will help unravel enduring mysteries of the star formation process, and why Sagittarius B2 is forming so many more stars than the rest of the galactic center.

However, one of the most notable aspects of Webb’s images of Sagittarius B2 are the portions that remain dark. These ironically empty-looking areas of space are actually so dense with gas and dust that even Webb cannot see through them. These thick clouds are the raw material of future stars and a cocoon for those still too young to shine.

Image Description: A wide view of a region of space filled with stars and clumps of orange clouds.


Credit: NASA, ESA, CSA, STScI, A. Ginsburg (University of Florida), N. Budaiev (University of Florida), T. Yoo (University of Florida). Image processing: A. Pagan (STScI)
Duration: 30 seconds
Release Date: Sept. 24, 2025

#NASA #Astronomy #Space #Science #Stars #Nebulae #SagittariusB2 #SgrB2 #MolecularClouds #Sagittarius #Constellations #MilkyWayGalaxy #Universe #SpaceTelescopes #JWST #NIRCam #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

Sagittarius B2 Molecular Cloud (NIRCam image) | James Webb Space Telescope

Sagittarius B2 Molecular Cloud (NIRCam image) | James Webb Space Telescope

Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s near-infrared camera (NIRCam). In this light, astronomers see more of the region’s diverse, colorful stars, but less of its gas and dust structure. Webb’s instruments each provide astronomers with important information that help build a more complete picture of what is happening in this intriguing portion of the center of our galaxy. 

Sagittarius B2 (Sgr B2) is located about 390 light years from the center of the Milky Way. This complex is the largest molecular cloud in the vicinity of the core and one of the largest in the galaxy, spanning a region about 150 light years across. The total mass of Sgr B2 is about 3 million times the mass of the Sun.

Sagittarius B2 is located only a few hundred light-years from the supermassive black hole at the heart of the galaxy called Sagittarius A*, a region densely packed with stars, star-forming clouds, and complex magnetic fields. The infrared light that Webb detects is able to pass through a portion of the area’s thick clouds to reveal young stars and the warm dust surrounding them. Astronomers think that analysis of Webb’s data will help unravel enduring mysteries of the star formation process, and why Sagittarius B2 is forming so many more stars than the rest of the galactic center.

However, one of the most notable aspects of Webb’s images of Sagittarius B2 are the portions that remain dark. These ironically empty-looking areas of space are actually so dense with gas and dust that even Webb cannot see through them. These thick clouds are the raw material of future stars and a cocoon for those still too young to shine.

Image Description: A wide view of a region of space filled with stars and clumps of orange clouds.


Credit: NASA, ESA, CSA, STScI, A. Ginsburg (University of Florida), N. Budaiev (University of Florida), T. Yoo (University of Florida). Image processing: A. Pagan (STScI)
Release Date: Sept. 24, 2025

#NASA #Astronomy #Space #Science #Stars #Nebulae #SagittariusB2 #SgrB2 #MolecularClouds #Sagittarius #Constellations #MilkyWayGalaxy #Universe #SpaceTelescopes #JWST #NIRCam #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education 

SpaceX Falcon 9 Liftoff: IMAP, SWFO-L1, & Carruthers Missions | NASA Kennedy

SpaceX Falcon 9 Liftoff: IMAP, SWFO-L1, & Carruthers Missions | NASA Kennedy

A SpaceX Falcon 9 rocket successfully launched and deployed NASA’s Interstellar Mapping and Acceleration Probe (IMAP), the agency’s Carruthers Geocorona Observatory, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft. Launch took place on schedule at 7:30 a.m. EDT, Wednesday, Sept. 24, 2025, from Launch Complex 39A at NASA's Kennedy Space Center in Florida. 

The missions will each focus on different effects of the solar wind—the continuous stream of particles emitted by the Sun—and space weather—the changing conditions in space driven by the Sun—from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system. 

The Interstellar Mapping and Acceleration Probe (IMAP) will explore and map the heliosphere—the invisible cosmic shield surrounding our solar system—to answer great unknowns about how particles accelerate in the solar wind.


NASA’s Carruthers Geocorona Observatory is a small satellite that will observe Earth’s outermost atmospheric layer, the exosphere. It will image the faint glow of ultraviolet light from this region, called the geocorona, to better understand how space weather impacts our planet. The Carruthers mission continues the legacy of the Apollo era, expanding on measurements first taken during Apollo 16.

The SWFO-L1 spacecraft will monitor space weather and detect solar storms in advance, serving as an early warning beacon for potentially disruptive space weather, helping safeguard Earth’s critical infrastructure and technological-dependent industries. The SWFO-L1 spacecraft is the first NOAA observatory designed specifically for and fully dedicated to continuous, operational space weather observations.

Video Credit: SpaceX
Duration: 26 seconds
Date: Sept. 24, 2025


#NASA #NOAA #Space #Astronomy #Science #IMAPMission #IMAP #Stars #InterstellarMedium #ISM #Sun #Heliophysics #Heliosphere #Planets #Earth #SolarSystem #SolarPlasma #SolarWind #SpaceWeather #PrincetonU #SWFOL1 #CarruthersGeocoronaObservatory #GSFC #SpaceX #Falcon9Rocket #KSC #Florida #UnitedStates #STEM #Education #HD #Video

Tuesday, September 23, 2025

Super Typhoon Ragasa over Western Pacific Ocean | International Space Station

Super Typhoon Ragasa over Western Pacific Ocean | International Space Station




Super typhoon Ragasa is headed for China's southern Guangdong province after lashing northern Luzon in the Philippines.

Typhoon season in the northwest Pacific has been quiet for most of 2025. Real-time estimates of accumulated cyclone energy from Colorado State University show that the basin was only half as active as usual as of September 23.

However, Typhoon Ragasa (also called Nando) has broken the quiet spell. The storm emerged on September 18 in the western Pacific Ocean a few hundred miles east of the Philippines. After periods of rapid intensification that brought it to Category 5 strength, the storm lashed northern Luzon on September 22, causing floods, landslides, and damage to crops and property. With sustained winds that reached more than 145 knots (270 kilometers or 165 miles per hour) late on September 21, the super typhoon ranked as the strongest typhoon of 2025. 

Forecasters expect the storm to maintain a west-northwestward trajectory, making landfall in southern Guangdong province on September 24 before skirting the coast of the Gulf of Tonkin and moving into northern Vietnam and Laos. As it approaches China, Ragasa is expected to weaken only slightly. According to the Joint Typhoon Warning Center, the storm is moving through a “highly favorable environment characterized by strong radial outflow, warm sea surface temperatures, and low vertical wind shear.”

The Western Pacific typhoon season spans the entire year, but most storms form between May and November with a peak in activity in late August and early September. As of September 23, nineteen named typhoons had formed in 2025, though only two had achieved Category 3 or higher strength for a sustained period.


Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Image Credit: NASA's Johnson Space Center/J. Kim
Image Details: Nikon Z9 | 15/24/50–500mm
Date: Sept. 22, 2025


#NASA #Space #ISS #Science #Planets #Earth #Atmosphere #Weather #Meteorology #Typhoons #TyphoonRagasa #China #中国 #GuangdongProvince #广东 #PacificOcean #Environment #Climate #ClimateChange #GlobalHeating #GreenhouseGases #Astronauts #AstronautPhotography #JonnyKim #UnitedStates #Japan #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

SpaceX Falcon 9: IMAP, SWFO-L1, & Carruthers Missions Pre-launch | NASA

SpaceX Falcon 9: IMAP, SWFO-L1, & Carruthers Missions Pre-launch | NASA








A SpaceX Falcon 9 rocket with NASA’s Interstellar Mapping and Acceleration Probe (IMAP), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft atop stands vertical at Launch Complex 39A as the sun sets on Monday, Sept. 22, 2025, at the agency’s Kennedy Space Center in Florida. The missions will each focus on different effects of the solar wind—the continuous stream of particles emitted by the Sun—and space weather—the changing conditions in space driven by the Sun—from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system. 

Launch is targeted for 7:30 a.m. EDT, Wednesday Sept. 24, 2025, from Launch Complex 39A at NASA's Kennedy Space Center. Weather is currently 90% favorable.

The Interstellar Mapping and Acceleration Probe (IMAP) will soon be on its mission to explore and map the heliosphere—the invisible cosmic shield surrounding our solar system—and to answer some great unknowns about how particles accelerate in the solar wind.

Press Release "Princeton in space: IMAP prepares for launch"
https://www.princeton.edu/news/2025/09/17/princeton-space-imap-prepares-launch


NASA’s Carruthers Geocorona Observatory is a small satellite that will observe Earth’s outermost atmospheric layer, the exosphere. It will image the faint glow of ultraviolet light from this region, called the geocorona, to better understand how space weather impacts our planet. The Carruthers mission continues the legacy of the Apollo era, expanding on measurements first taken during Apollo 16.

The SWFO-L1 spacecraft will monitor space weather and detect solar storms in advance, serving as an early warning beacon for potentially disruptive space weather, helping safeguard Earth’s critical infrastructure and technological-dependent industries. The SWFO-L1 spacecraft is the first NOAA observatory designed specifically for and fully dedicated to continuous, operational space weather observations.

Image Credit: SpaceX
Date: Sept. 22, 2025


#NASA #NOAA #Space #Astronomy #Science #IMAPMission #IMAP #Stars #InterstellarMedium #ISM #Sun #Heliophysics #Heliosphere #Planets #Earth #SolarSystem #SolarPlasma #SolarWind #SpaceWeather #PrincetonU #SWFOL1 #CarruthersGeocoronaObservatory #GSFC #SpaceX #Falcon9Rocket #KSC #Florida #UnitedStates #STEM #Education

Typhoon Ragasa Steers Toward China | NASA Terra Earth Satellite [Budget Alert]

Typhoon Ragasa Steers Toward China | NASA Terra Earth Satellite [Budget Alert]


This satellite image shows Typhoon Ragasa swirling over the Luzon Strait between the northern Philippines and Taiwan on September 23, 2025. The storm’s eye is visible, surrounded by bands of clouds. In the second image, parts of southern China appear to the northwest of the storm, while the Philippines and Taiwan are labeled to the southeast and northeast. The super typhoon headed for Guangdong province after lashing northern Luzon in the Philippines.

Typhoon season in the northwest Pacific has been quiet for most of 2025. Real-time estimates of accumulated cyclone energy from Colorado State University show that the basin was only half as active as usual as of September 23.

However, Typhoon Ragasa (also called Nando) has broken the quiet spell. The storm emerged on September 18 in the western Pacific Ocean a few hundred miles east of the Philippines. After periods of rapid intensification that brought it to Category 5 strength, the storm lashed northern Luzon on September 22, causing floods, landslides, and damage to crops and property. With sustained winds that reached more than 145 knots (270 kilometers or 165 miles per hour) late on September 21, the super typhoon ranked as the strongest typhoon of 2025.

The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite acquired this image of Ragasa at 01:40 Universal Time on September 23, 2025. At the time, forecasters expected the storm to maintain a west-northwestward trajectory, making landfall in southern Guangdong province on September 24 before skirting the coast of the Gulf of Tonkin and moving into northern Vietnam and Laos. As it approaches China, Ragasa is expected to weaken only slightly. According to the Joint Typhoon Warning Center, the storm is moving through a “highly favorable environment characterized by strong radial outflow, warm sea surface temperatures, and low vertical wind shear.”

NASA's Terra and Aqua Earth satellites are being canceled in NASA's Fiscal Year 2026 Budget Request, along with 17 other active science missions. NASA's science budget is being reduced by nearly 50%. NASA's total budget will become the lowest since 1961, after accounting for inflation.

Contact your representatives in the United States Congress, House and Senate, to express your concerns about severe budget cuts at NASA:

As of September 23, the storm had displaced tens of thousands of people, caused multiple deaths, and led to power outages and extensive damage in the Philippines, according to news reports. As cleanup efforts began in the Philippines, life in several Chinese cities came to a standstill as people evacuated homes, schools, and workplaces ahead of the storm. Authorities in Vietnam evacuated thousands of households as well, according to news reports.

The Western Pacific typhoon season spans the entire year, but most storms form between May and November with a peak in activity in late August and early September. As of September 23, nineteen named typhoons had formed in 2025, though only two had achieved Category 3 or higher strength for a sustained period.


Image Credit: NASA Earth Observatory image by Wanmei Liang, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview
Text Credit: Adam Voiland
Release Date: Sept. 23, 2025

#NASA #Earth #Space #Satellites #TerraSatellite #Planets #Earth #Atmosphere #Weather #Meteorology #Storm #Typhoon #TyphoonRagasa #China #中国 #GuangdongProvince #广东 #LuzonStrait #PacificOcean #Environment #Climate #ClimateChange #GlobalHeating #GreenhouseGases #GHG #GSFC #UnitedStates #Infographics #STEM #Education

NASA Astronaut Candidate Anna Menon: Class of 2025

NASA Astronaut Candidate Anna Menon: Class of 2025

NASA astronaut candidate Anna Menon poses for a portrait at NASA’s Johnson Space Center in Houston, Texas. Menon was selected by NASA to join the 2025 astronaut candidate class and reported for duty in September 2025. In 2024, Menon flew to space as a mission specialist and medical officer aboard SpaceX’s Polaris Dawn. The mission saw a new female altitude record, the first commercial spacewalk, and the completion of approximately 40 research experiments. 

Menon earned her bachelor’s degree from Texas Christian University with a double major in mathematics and Spanish and holds a master’s in biomedical engineering from Duke University. Menon previously worked in Mission Control at NASA’s Johnson Space Center in Houston, supporting medical hardware and software aboard the International Space Station. At the time of her selection, Menon was a senior engineer at SpaceX.

NASA astronaut candidate Anna Menon Biography:
https://www.nasa.gov/people/nasa-astronaut-candidate-anna-menon/

Credit: NASA/Josh Valcarcel
Release Date: Sept. 16, 2025

#NASA #Space #Science #HumanSpaceflight #AnnaMenon #AstronautCandidates #AstronautCandidateSelection #ASCAN2025Class #ASCANProgram #Astronauts #CommercialAstronauts #CommercialSpace #SpaceX #PolarisDawnMission #BiomedicalEngineers #NASAJohnson #JSC #Houston #UnitedStates #STEM #Education