Tuesday, September 01, 2026

What's Up for September 2026: Skywatching Tips from NASA | JPL

What's Up for September 2026: Skywatching Tips from NASA JPL

Here are examples of skywatching highlights for the northern hemisphere in September 2026: 

The Moon joins a tea party, Venus reaches peak brilliance, the seasons change, and the Harvest Moon meets up with planetary neighbors.

From September 14 through 20, use the Moon as a guide to spot Antares, the Teapot asterism, and—under especially dark skies—the center of our Milky Way galaxy.

On September 18, look low in the west shortly after sunset as Venus reaches peak brilliance for this evening appearance.

On September 19, celebrate International Observe the Moon Night! People around the world are invited to look up and connect with our nearest celestial neighbor while learning more about lunar science, exploration, and the many ways the moon has shaped cultures around the world. 

The September equinox arrives on September 22, marking the start of fall in the Northern Hemisphere and spring in the Southern Hemisphere.

Then on September 26, the Harvest Moon rises near Saturn with faint Neptune completing a wide triangle in the sky. Saturn is visible to the unaided eye, while Neptune requires binoculars or a telescope.

0:00 Intro

0:12 Moon near Antares and the Teapot

1:02 Venus reaches peak brilliance

1:49 September equinox

2:13 Harvest Moon, Saturn and Neptune

2:50 Moon phases


Video Credit: NASA's Jet Propulsion Laboratory
Duration: 3 minutes
Date: Sept. 1, 2026

#NASA #Astronomy #Space #Science #Skywatching #Earth #Moon #HarvestMoon #SeptemberEquinox #Planets #Venus #Saturn #Neptune #SolarSystem #Nebulae #Stars #TeapotAsterism #Constellations #MilkyWayGalaxy #Skywatching #JPL #California #UnitedStates #Canada #Mexico #NorthernHemisphere #STEM #Education #HD #Video

Journey to NGC 7253—Interacting Galaxies in Pegasus | Gemini North Telescope

Journey to NGC 7253Interacting Galaxies in Pegasus | Gemini North Telescope

Nā ʻUhane Māhoe Huki Pū i ke Ola is the Hawaiian name given to this image of NGC 7253—a pair of spiral galaxies caught in each other’s gravity in the constellation Pegasus. This image was captured by the Gemini North telescope on Maunakea, Hawaii, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab. The name of the image translates to “The Twin Spirits Pulling Together Creating Life.” It was chosen by the 2026 Project Hōkūlani interns.

NGC 7253 was discovered by the German-British astronomer Albert Marth on September 9, 1863. It is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 278, as an example of gravitationally interacting galaxies.

Of the pair, the galaxy to the north is known individually as NGC 7253A. The other galaxy in the pair is known individually as NGC 7253B. 

NGC 7253 has a possible active galactic nucleus (AGN), i.e. it has a compact region at the galaxy's center that emits a significant amount of energy across the electromagnetic spectrum with characteristics indicating that this luminosity is not produced by the stars.

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)
Duration: 1 minute
Release Date: Sept. 1, 2026

#NASA #Astronomy #Space #Science #Galaxies #NGC7253 #NGC7253A #NGC7253B #Arp278 #InteractingGalaxies #PegasusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

Close-up: NGC 7253—Interacting Galaxies in Pegasus | Gemini North Telescope

Close-up: NGC 7253Interacting Galaxies in Pegasus | Gemini North Telescope

Nā ʻUhane Māhoe Huki Pū i ke Ola is the Hawaiian name given to this image of NGC 7253—a pair of spiral galaxies caught in each other’s gravity in the constellation Pegasus. This image was captured by the Gemini North telescope on Maunakea, Hawaii, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab. The name of the image translates to “The Twin Spirits Pulling Together Creating Life.” It was chosen by the 2026 Project Hōkūlani interns.

NGC 7253 was discovered by the German-British astronomer Albert Marth on September 9, 1863. It is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 278, as an example of gravitationally interacting galaxies.

Of the pair, the galaxy to the north is known individually as NGC 7253A. The other galaxy in the pair is known individually as NGC 7253B. 

NGC 7253 has a possible active galactic nucleus (AGN), i.e. it has a compact region at the galaxy's center that emits a significant amount of energy across the electromagnetic spectrum with characteristics indicating that this luminosity is not produced by the stars.

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)
Duration: 30 seconds
Release Date: Sept. 1, 2026

#NASA #Astronomy #Space #Science #Galaxies #NGC7253 #NGC7253A #NGC7253B #Arp278 #InteractingGalaxies #PegasusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

NGC 7253: A Pair of Interacting Spiral Galaxies in Pegasus | Gemini North Telescope

NGC 7253: A Pair of Interacting Spiral Galaxies in Pegasus | Gemini North Telescope

Nā ʻUhane Māhoe Huki Pū i ke Ola is the Hawaiian name given to this image of NGC 7253—a pair of spiral galaxies caught in each other’s gravity in the constellation Pegasus. This image was captured by the Gemini North telescope on Maunakea, Hawaii, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab. The name of the image translates to “The Twin Spirits Pulling Together Creating Life.” It was chosen by the 2026 Project Hōkūlani interns.

NGC 7253 was discovered by the German-British astronomer Albert Marth on September 9, 1863. It is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 278, as an example of gravitationally interacting galaxies.

Of the pair, the galaxy to the north is known individually as NGC 7253A. The other galaxy in the pair is known individually as NGC 7253B. 

NGC 7253 has a possible active galactic nucleus (AGN), i.e. it has a compact region at the galaxy's center that emits a significant amount of energy across the electromagnetic spectrum with characteristics indicating that this luminosity is not produced by the stars.

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)
Release Date: Sept. 1, 2026

#NASA #Astronomy #Space #Science #Galaxies #NGC7253 #NGC7253A #NGC7253B #Arp278 #InteractingGalaxies #PegasusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

China's PALLAS-1 Commercial Rocket Completes Successful First Test Flight

China's PALLAS-1 Commercial Rocket Completes Successful First Test Flight








China on Tuesday, September 1, 2026, successfully launched of Galactic Energy's PALLAS-1 Y1 carrier rocket into space from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China. The rocket blasted off at 10:00am Beijing Time and performed normally during the entire flight as it headed for a sun-synchronous orbit. All test objectives were achieved and the mission was a complete success.

This was the maiden flight of PALLAS-1.

PALLAS-1 Y1 carrier rocket is of two-stage configuration, designed for at least 25 reuse cycles, with a payload capacity of five to seven metric tons to low Earth orbit (LEO).

A year on from its first flight hardware static fires, Pallas-1 has opened a path towards future booster recovery and reuse.

The PALLAS-1 uses the self-developed CQ-50 pintle-type reusable liquid oxygen/kerosene engines. They had accumulated hot-fire tests exceeding 23,000 seconds. The rocket's first stage adopts a parallel configuration of seven CQ-50 engines.

Although no satellites were added to orbit, the two-stage to-be-reusable launch vehicle proved that all of its parts work in flight.

Departure from Earth under the power of seven CQ-50 engines went as planned. After using all of the available propellant, the first and second stages were released to go their separate ways. Utilizing a single CQ-50, the second-stage successfully completed the trek into orbit.

As for the first-stage, it tumbled back towards Earth after separation, as no grid fins or other components for booster recovery were installed. Progress on those components is well underway, and they are expected to be included from the third flight onwards.

No customer or internally-sourced spacecraft were housed within Pallas-1’s payload fairing for its debut ‘test flight’. The mission’s primary and only goal was to demonstrate that its systems can enable a successful flight using Galactic Energy-made parts, while also collecting useful data on in-flight performance.

Additional plans for Pallas-1 will see the launch vehicle gain an optional third-stage, based upon the twice-used ‘Eros’, to send customer satellites towards harder-to-reach orbits, such as those up to geostationary space.

Today’s launch was the 1st for the Pallas-1 launch vehicle, the 1st flight of the Pallas series, and Galactic Energy’s 25th orbital launch. This was also the 61st launch from China in 2026.

Galactic Energy successfully conducted its first launch in November 2020 with a Ceres-1 rocket. Galactic Energy became the second private company in China to put a satellite in orbit successfully.


Image Credit: Galactic Energy
Text Credit: CCTV, Jack C.
Release Date: Sept. 1, 2026

#NASA #Space #Science #Satellites #Earth #China #中国 #Rockets #PALLAS1 #PALLASY1Rocket #CQ50Engines #ReusableRockets #GalacticEnergy #星河动力 #CommercialSpace #Gansu #甘肃 #STEM #Education

China's PALLAS-1 Commercial Rocket Completes Successful First Test Flight

China's PALLAS-1 Commercial Rocket Completes Successful First Test Flight

China on Tuesday, September 1, 2026, successfully launched of Galactic Energy's PALLAS-1 Y1 carrier rocket into space from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China. The rocket blasted off at 10:00am Beijing Time and performed normally during the entire flight as it headed for a sun-synchronous orbit. All test objectives were achieved and the mission was a complete success.

This was the maiden flight of PALLAS-1.

PALLAS-1 Y1 carrier rocket is of two-stage configuration, designed for at least 25 reuse cycles, with a payload capacity of five to seven metric tons to low Earth orbit (LEO).

A year on from its first flight hardware static fires, Pallas-1 has opened a path towards future booster recovery and reuse.

The PALLAS-1 uses the self-developed CQ-50 pintle-type reusable liquid oxygen/kerosene engines. They had accumulated hot-fire tests exceeding 23,000 seconds. The rocket's first stage adopts a parallel configuration of seven CQ-50 engines.

Although no satellites were added to orbit, the two-stage to-be-reusable launch vehicle proved that all of its parts work in flight.

Departure from Earth under the power of seven CQ-50 engines went as planned. After using all of the available propellant, the first and second stages were released to go their separate ways. Utilizing a single CQ-50, the second-stage successfully completed the trek into orbit.

As for the first-stage, it tumbled back towards Earth after separation, as no grid fins or other components for booster recovery were installed. Progress on those components is well underway, and they are expected to be included from the third flight onwards.

No customer or internally-sourced spacecraft were housed within Pallas-1’s payload fairing for its debut ‘test flight’. The mission’s primary and only goal was to demonstrate that its systems can enable a successful flight using Galactic Energy-made parts, while also collecting useful data on in-flight performance.

Additional plans for Pallas-1 will see the launch vehicle gain an optional third-stage, based upon the twice-used ‘Eros’, to send customer satellites towards harder-to-reach orbits, such as those up to geostationary space.

Today’s launch was the 1st for the Pallas-1 launch vehicle, the 1st flight of the Pallas series, and Galactic Energy’s 25th orbital launch. This was also the 61st launch from China in 2026.

Galactic Energy successfully conducted its first launch in November 2020 with a Ceres-1 rocket. Galactic Energy became the second private company in China to put a satellite in orbit successfully.


Video Credit: Galactic Energy
Text Credit: CCTV, Jack C.
Duration: 1 minute, 50 seconds
Release Date: Sept. 1, 2026

#NASA #Space #Science #Satellites #Earth #China #中国 #Rockets #PALLAS1 #PALLASY1Rocket #CQ50Engines #ReusableRockets #GalacticEnergy #星河动力 #CommercialSpace #Gansu #甘肃 #STEM #Education #HD #Video

'Cannibal' Galaxy ESO 243-49 in Phoenix: Black Hole Location | Hubble

'Cannibal' Galaxy ESO 243-49 in Phoenix: Unusual Black Hole Location | Hubble

A star cluster surrounds the wayward black hole in distant 'cannibal' galaxy ESO 243-49 located above the galactic plane (circled). This spectacular edge-on galaxy in the Phoenix constellation, called ESO 243-49, is home to an intermediate-mass black hole that may have come from a cannibalized dwarf galaxy. The black hole has an estimated mass of 20,000 Suns. This is an unlikely place for such a massive back hole to exist, unless it belonged to a small galaxy that was gravitationally torn apart by ESO 243-49.

The circle identifies a unique X-ray source that pinpoints the black hole. The X-rays are believed to be radiation from a hot accretion disc around the black hole. The blue light not only comes from a hot accretion disc, but also from a cluster of hot young stars that formed around the black hole. 

Galaxy ESO 243-49 is 290 million light-years from Earth. Hubble cannot resolve the stars individually because the suspected cluster is too far away. Their presence is inferred from the color and brightness of the light coming from the black hole’s location.


Credit: NASA, European Space Agency (ESA), and S. Farrell (University of Sydney, Australia and University of Leicester, UK)
Release Date: Feb. 15, 2012

#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #StarClusters #Galaxies #ESO24349 #ESO24349 #HLX1 #BlackHoles #PhoenixConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

NASA's Nancy Grace Roman Space Telescope: Launch Recap | Kennedy Space Center

NASA's Nancy Grace Roman Space Telescope: Launch Recap | Kennedy Space Center

NASA’s Nancy Grace Roman Space Telescope successfully lifted off from NASA’s Kennedy Space Center in Florida at 7:26 a.m. EDT (1126 UTC) on Aug. 30, 2026.

Next, the telescope will go through initial tests and commissioning as it it travels to Sun-Earth Lagrange Point 2 (L2), about 1 million miles away.

This video recaps the highlights from Roman's launch day.

Learn more at: http://nasa.gov/roman

The Roman telescope and the discoveries it will support:
https://www.stsci.edu/roman

Roman’s namesake—Dr. Nancy Grace Roman, NASA’s first chief astronomer—made it her personal mission to make cosmic vistas readily accessible to all by paving the way for telescopes based in space.

“The mission will acquire enormous quantities of astronomical imagery that will permit scientists to make groundbreaking discoveries for decades to come, honoring Dr. Roman’s legacy in promoting scientific tools for the broader community,” said Jackie Townsend, Roman’s deputy project manager at NASA Goddard. “I like to think Dr. Roman would be extremely proud of her namesake telescope and thrilled to see what mysteries it will uncover in the coming years.”


Video Credit: NASA 
Duration: 2 minutes
Release Date: Aug. 31, 2026

#NASA #Space #Astronomy #Science #SpaceX #FalconHeavyRocket #NASARoman #RomanSpaceTelescope #Encapsulation #NancyGraceRomanSpaceTelescope #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #NASAKennedy #Florida #UnitedStates #STEM #Education #HD #Video

Monday, August 31, 2026

NASA Artemis III Crew Training Underway | Johnson Space Center

NASA Artemis III Crew Training Underway | Johnson Space Center

Image Description: From left, Artemis III crew members, NASA astronauts Andre Douglas and Randy Bresnick, European Space Agency (ESA) astronaut Luca Parmitano, and NASA astronaut Frank Rubio participate in training at NASA’s Johnson Space Center in Houston on Wednesday, Aug. 19, 2026.

After being assigned to the Artemis III mission on June 9, 2026, NASA astronauts Bresnik, Andre Douglas, Frank Rubio, and the European Space Agency (ESA) astronaut Luca Parmitano began an intensive training flow that covers Orion systems and operations, science objectives, leadership and team‑building exercises, as well as joint training with commercial human landing system providers.

The crew’s training is organized around major phases of the mission, including ascent, orbit and rendezvous operations, entry, and both pre‑ and post‑landing readiness.

Crew members are working in the Orion mockup at NASA’s Johnson Space Center in Houston, practicing daily spacecraft operations, such as mealtime routines, using equipment like the food warmer and potable water dispenser. They also are refining their camera skills to capture and share imagery from their mission in low Earth orbit.

The crew recently completed an introductory water survival class focused on hardware used during off‑nominal landings, along with a post‑landing emergency exiting course that introduced splashdown procedures and initial post‑landing conditions.

This week in NASA’s Neutral Buoyancy Lab, they donned their spacesuits and practiced exiting Orion in an upright configuration. The practice allowed the crew to demonstrate the proper use of their Orion Crew Survival System suits, survival hardware, life raft, and more.

The Artemis III crew also began integrated simulations with the flight control team, including the first simulation with the four crew members together. In these sessions, crew members and controllers rehearse mission timelines and respond to a variety of situations they could face in space, strengthening coordination, decision‑making, and procedures.

Planned to launch in 2027, the Artemis III Mission will practice docking the Orion spacecraft with two lunar landers in low Earth orbit. 

On future missions, including Artemis IV in 2028, landers will bring astronauts to the lunar surface. While Artemis III will not land on the Moon, it will test the complex capabilities NASA needs to return—this time to stay.

Learn more about NASA’s Artemis program:

Image Credit: NASA/Bill Stafford
Image Date: Aug. 19, 2026
Release Date: Aug. 27, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisIII #ArtemisIIIMission #LunarLanders #HLS #NASASLS #OrionSpacecraft #Astronauts #RandyBresnik #FrankRubio #AndreDouglas #LucaParmitano #Italy #Italia #Europe #HumanSpaceflight #SolarSystem #SpaceExploration #NASAJohnson #Houston #Texas #UnitedStates #STEM #Education

NASA's Stennis Space Center: Celebrating 65 Years of American Rocketry (1961-2026)

NASA's Stennis Space Center: Celebrating 65 Years of American Rocketry

October 25, 2026, will mark a major milestone—65 years since NASA announced it would build a rocket propulsion test site in Hancock County, Mississippi. Now, as NASA works to return American astronauts to the Moon through the Artemis program and to establish an enduring presence on the lunar surface, we are looking back at how it all began right here.

Over the next few weeks, we are taking you through the decades and celebrating 65 years of igniting America’s journey to space.


NASA's Stennis Space Center:

Video Credit: NASA's Stennis Space Center
Duration: 1 minute, 40 seconds
Release Date: Aug. 31, 2026

#NASA #Space #Science #Earth #Moon #ApolloProgram #ArtemisProgram #ArtemisIII #ArtemisIIIMission #RocketEngines #Rocketry #LunarLanders #HLS #NASASLS #OrionSpacecraft #OrionServiceModules #Astronauts #Italy #Italia #Europe #HumanSpaceflight #SolarSystem #MoonExploration #NASAStennis #HancockCounty #Mississippi #UnitedStates #History #STEM #Education #HD #Video

Planet Mars Images: Aug. 29-30, 2026 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Aug. 29-30, 2026 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1964
Mars 2020 - sol 1964
Mars 2020 - sol 1964
Mars 2020 - sol 1964
Mars 2020 - sol 1964
MSL - sol 4999
MSL - sol 4999
MSL - sol 4999

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https://www.friendsofnasa.org/p/friends-of-nasa.html

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We rely on public donations.
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Celebrating 14+ Years on Mars (2012-2026)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 5+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Release Dates: Aug. 29-30, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #SpaceExploration #SolarSystem #STEM #Education

Lunar Eclipses 'Flower' Mosaic: Views from Arizona & Chile

Lunar Eclipses 'Flower' Mosaic: Views from Arizona & Chile

In honor of the partial lunar eclipse on August 27, 2026, an array of lunar eclipses “blooms” red in this mosiac image. It is the result of over a decade of photography by the dedicated NOIRLab Audiovisual Ambassadors Petr Horálek and Rob Sparks, and their collaborators. The featured eclipses were captured at sites including U.S. National Science Foundation (NSF) Kitt Peak National Observatory (KPNO) and Cerro Tololo Inter-American Observatory (CTIO), Programs of NSF NOIRLab.

This image brings together lunar eclipses photographed over the past decade. The red and orange Moons near the center were captured during totality, while the grey outer Moons show partial and penumbral eclipses. The longest eclipse of the century is in the center of the mosaic.

Their positions and sizes are aligned using the angular diameter of Earth’s inner shadow, or umbra, revealing the shadow’s circular form. Because the Moon follows an elliptical orbit, it appears about 14% larger when it is closer to Earth than when it is farther away. During totality, sunlight filtered and bent through Earth’s atmosphere illuminates the Moon in shades ranging from bright copper to deep red. The exact color and brightness depend on how deeply the Moon enters the shadow, as well as the amount of clouds, dust, and aerosols in Earth’s atmosphere at the time. When eclipses occur low over the horizon, the layers of Earth’s atmosphere can affect the appearance of the colors in even more interesting ways. Some of the total eclipses in this image have a difficult-to-observe blue band. This is caused by the absorption of red light by Earth’s ozone layer and indicates the Moon is near the edge of the Earth’s shadow.

The positions and angular sizes of the Moons in the Earth’s shadow are as accurate as possible while creating a pleasing flower shape, though the arrangement is not chronological. The images are color accurate.

Lunar eclipses occur at the full Moon phase. When Earth is positioned precisely between the Moon and Sun, Earth’s shadow falls upon the surface of the Moon, dimming it and sometimes turning the lunar surface a striking red over the course of a few hours. Each lunar eclipse is visible from half of Earth.

Learn more: https://science.nasa.gov/moon/eclipses/


Credit: KPNO/NOIRLab/NSF/AURA/Petr Horálek/Institute of Physics in Opava, Robert Sparks, Josef Kujal, John Melson, Dave Hash/Wikimedia
Release Date: Aug. 26, 2026


#NASA #Space #Astronomy #Science #Sun #SolarSystem #Moon #Earth #LunarEclipse #Umbra #Penumbra #Astrophotographers #PetrHorálek #RobSparks #Astrophotography #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #CTIO #Chile #STEM #Education

NASA's Nancy Grace Roman Space Telescope Launch | Kennedy Space Center

NASA's Nancy Grace Roman Space Telescope Launch | Kennedy Space Center









Now on a three-month, million-mile journey to its final orbit, NASA’s Nancy Grace Roman Space Telescope will soon reveal the universe’s darkest secrets. The mission launched at 7:26 a.m. EDT Sunday aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.

Roman pairs a large field of view with crisp infrared vision to explore vast swaths of the sky and probe deeply into cosmic history. This flagship mission will help astronomers explore dark matter, dark energy, and worlds outside of our solar system, known as exoplanets. Its surveys will support a broad range of research extending far beyond the mission’s main science goals.

The ground control team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, began receiving telemetry data from Roman seven minutes after launch. The Falcon Heavy rocket performed as expected, separating from the observatory 31 minutes into the flight. After separating from the center core, the rocket’s boosters safely returned to the launch site for refurbishment.

During launch and early orbit, Roman uses the Near Space Network’s ground stations and relay satellites to exchange tracking, telemetry, and command data with ground controllers. About 70 minutes after launch, the Deep Space Network takes over communications and guides Roman toward the second Sun-Earth Lagrange point, or L2, about one million miles from Earth. Roman connects to that network through the Canberra Deep Space Communication Complex in Australia first. Approximately six hours later it will transfer to the Madrid Deep Space Communication Complex in Spain and then to the Goldstone Deep Space Communication Complex in California, ensuring continuous contact with Roman throughout its journey.

The Roman team also confirmed successful deployment of the observatory’s solar panels and lower instrument sun shade an hour and 23 minutes after launch. Within the upcoming days, Roman’s high-gain antenna and visor-like deployable aperture cover will deploy, ground controllers will initiate the first of two-mid-course corrections, and the Coronagraph Instrument will power on. This instrument will demonstrate the technology that future missions like NASA’s Habitable Worlds Observatory concept could use to image Earth-like planets in the search for life in the universe. Roman’s Coronagraph will take a giant step in that direction by snapping pictures of Jupiter-like planets.

A few weeks into Roman’s voyage, its primary instrument, the Wide Field Instrument, will activate. This 300-megapixel infrared camera has 18 4K detectors, each about the size of a saltine cracker. These detectors collect photons of light that will be decoded into crisp cosmic panoramas. Thanks to the observatory’s rigid design and stable optical performance, it will rapidly scan the sky without needing substantial time between separate observations. The Roman telescope is designed to survey the universe a thousand times faster than NASA’s Hubble Space Telescope.

Throughout the rest of Roman’s three-month commissioning period, scientists will run the instruments through a series of calibrations and tests. NASA anticipates releasing Roman’s first images by early 2027.

Roman will send back 1.4 terabytes of data every day, the highest data rate of any NASA astrophysics mission, so far. Machine learning, artificial intelligence, and citizen scientists will help sift through it and flag significant findings, which astronomers can then study.

“We’ve never been able to view the universe with eyes like Roman’s before,” said Julie McEnery, Roman’s senior project scientist at NASA Goddard. “There’s no telling what more we’ll know and have seen by this time next year.”

Roman is the fourth primary mission NASA has launched on a Falcon Heavy rocket. Earlier this year, the agency’s Launch Services Program worked with SpaceX to accelerate the launch date to accommodate the space telescope’s early completion.

The telescope is managed at NASA Goddard with participation by the agency’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a team of scientists from various research institutions. The primary industrial partners are BAE Systems Inc., L3Harris Technologies, and Teledyne Scientific & Imaging. Contributions to Roman also are made by ESA, JAXA, the French space agency CNES (Centre National d’Études Spatiales), and the Max Planck Institute for Astronomy in Germany.

To learn more about the Roman mission, visit:
https://www.nasa.gov/roman


Image Credit: NASA/Joel Kowsky
Text Credit: NASA's Goddard Space Flight Center
Date: Aug. 30, 2026

#NASA #Space #Astronomy #Science #SpaceX #FalconHeavyRocket #NASARoman #RomanSpaceTelescope #Encapsulation #NancyGraceRomanSpaceTelescope #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Cosmos #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #NASAKennedy #Florida #UnitedStates #STEM #Education

Sunday, August 30, 2026

NASA's Nancy Grace Roman Space Telescope Launch | Kennedy Space Center

NASA's Nancy Grace Roman Space Telescope Launch | Kennedy Space Center








Now on a three-month, million-mile journey to its final orbit, NASA’s Nancy Grace Roman Space Telescope will soon reveal the universe’s darkest secrets. The mission launched at 7:26 a.m. EDT Sunday aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.

Roman pairs a large field of view with crisp infrared vision to explore vast swaths of the sky and probe deeply into cosmic history. This flagship mission will help astronomers explore dark matter, dark energy, and worlds outside of our solar system, known as exoplanets. Its surveys will support a broad range of research extending far beyond the mission’s main science goals.

The ground control team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, began receiving telemetry data from Roman seven minutes after launch. The Falcon Heavy rocket performed as expected, separating from the observatory 31 minutes into the flight. After separating from the center core, the rocket’s boosters safely returned to the launch site for refurbishment.

During launch and early orbit, Roman uses the Near Space Network’s ground stations and relay satellites to exchange tracking, telemetry, and command data with ground controllers. About 70 minutes after launch, the Deep Space Network takes over communications and guides Roman toward the second Sun-Earth Lagrange point, or L2, about one million miles from Earth. Roman connects to that network through the Canberra Deep Space Communication Complex in Australia first. Approximately six hours later it will transfer to the Madrid Deep Space Communication Complex in Spain and then to the Goldstone Deep Space Communication Complex in California, ensuring continuous contact with Roman throughout its journey.

The Roman team also confirmed successful deployment of the observatory’s solar panels and lower instrument sun shade an hour and 23 minutes after launch. Within the upcoming days, Roman’s high-gain antenna and visor-like deployable aperture cover will deploy, ground controllers will initiate the first of two-mid-course corrections, and the Coronagraph Instrument will power on. This instrument will demonstrate the technology that future missions like NASA’s Habitable Worlds Observatory concept could use to image Earth-like planets in the search for life in the universe. Roman’s Coronagraph will take a giant step in that direction by snapping pictures of Jupiter-like planets.

A few weeks into Roman’s voyage, its primary instrument, the Wide Field Instrument, will activate. This 300-megapixel infrared camera has 18 4K detectors, each about the size of a saltine cracker. These detectors collect photons of light that will be decoded into crisp cosmic panoramas. Thanks to the observatory’s rigid design and stable optical performance, it will rapidly scan the sky without needing substantial time between separate observations. The Roman telescope is designed to survey the universe a thousand times faster than NASA’s Hubble Space Telescope.

Throughout the rest of Roman’s three-month commissioning period, scientists will run the instruments through a series of calibrations and tests. NASA anticipates releasing Roman’s first images by early 2027.

Roman will send back 1.4 terabytes of data every day, the highest data rate of any NASA astrophysics mission, so far. Machine learning, artificial intelligence, and citizen scientists will help sift through it and flag significant findings, which astronomers can then study.

“We’ve never been able to view the universe with eyes like Roman’s before,” said Julie McEnery, Roman’s senior project scientist at NASA Goddard. “There’s no telling what more we’ll know and have seen by this time next year.”

Roman is the fourth primary mission NASA has launched on a Falcon Heavy rocket. Earlier this year, the agency’s Launch Services Program worked with SpaceX to accelerate the launch date to accommodate the space telescope’s early completion.

The telescope is managed at NASA Goddard with participation by the agency’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a team of scientists from various research institutions. The primary industrial partners are BAE Systems Inc., L3Harris Technologies, and Teledyne Scientific & Imaging. Contributions to Roman also are made by ESA, JAXA, the French space agency CNES (Centre National d’Études Spatiales), and the Max Planck Institute for Astronomy in Germany.

To learn more about the Roman mission, visit:
https://www.nasa.gov/roman


Image Credit: SpaceX
Text Credit: NASA's Goddard Space Flight Center
Date: Aug. 30, 2026

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NASA's Nancy Grace Roman Space Telescope Falcon Heavy Booster Landing

NASA's Nancy Grace Roman Space Telescope Falcon Heavy Booster Landing

The boosters from the SpaceX Falcon Heavy rocket successfully land after launching NASA's Nancy Grace Roman Space Telescope from Launch Complex 39A at Kennedy Space Center in Florida at 7:26 a.m. EDT Sunday, Aug. 30, 2026.

This was the first and third flight for the two first stage side boosters supporting this mission. They previously launched the SpaceX GOES-U and Viasat-3 F3 missions. Following stage separation, Falcon Heavy’s two side boosters landed on SpaceX’s Landing Zones 2 and 40 (LZ-2 and LZ-40) at Cape Canaveral in Florida.

Roman pairs a large field of view with crisp infrared vision to explore vast swaths of the sky and probe deeply into cosmic history. This flagship mission will help astronomers explore dark matter, dark energy, and worlds outside of our solar system, known as exoplanets. Its surveys will support a broad range of research extending far beyond the mission’s main science goals.

The ground control team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, began receiving telemetry data from Roman seven minutes after launch. The Falcon Heavy rocket performed as expected, separating from the observatory 31 minutes into the flight. After separating from the center core, the rocket’s boosters safely returned to the launch site for refurbishment.

The Roman team also confirmed successful deployment of the observatory’s solar panels and lower instrument sun shade an hour and 23 minutes after launch. Within the upcoming days, Roman’s high-gain antenna and visor-like deployable aperture cover will deploy, ground controllers will initiate the first of two-mid-course corrections, and the Coronagraph Instrument will power on. This instrument will demonstrate the technology that future missions like NASA’s Habitable Worlds Observatory concept could use to image Earth-like planets in the search for life in the universe. Roman’s Coronagraph will take a giant step in that direction by snapping pictures of Jupiter-like planets.

A few weeks into Roman’s voyage, its primary instrument, the Wide Field Instrument, will activate. This 300-megapixel infrared camera has 18 4K detectors, each about the size of a saltine cracker. These detectors collect photons of light that will be decoded into crisp cosmic panoramas. Thanks to the observatory’s rigid design and stable optical performance, it will rapidly scan the sky without needing substantial time between separate observations. The Roman telescope is designed to survey the universe a thousand times faster than NASA’s Hubble Space Telescope.

Throughout the rest of Roman’s three-month commissioning period, scientists will run the instruments through a series of calibrations and tests. NASA anticipates releasing Roman’s first images by early 2027.

Roman will send back 1.4 terabytes of data every day, the highest data rate of any NASA astrophysics mission, so far. Machine learning, artificial intelligence, and citizen scientists will help sift through it and flag significant findings, which astronomers can then study.

“We’ve never been able to view the universe with eyes like Roman’s before,” said Julie McEnery, Roman’s senior project scientist at NASA Goddard. “There’s no telling what more we’ll know and have seen by this time next year.”

Roman is the fourth primary mission NASA has launched on a Falcon Heavy rocket. Earlier this year, the agency’s Launch Services Program worked with SpaceX to accelerate the launch date to accommodate the space telescope’s early completion.

The telescope is managed at NASA Goddard with participation by the agency’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a team of scientists from various research institutions. The primary industrial partners are BAE Systems Inc., L3Harris Technologies, and Teledyne Scientific & Imaging. Contributions to Roman also are made by ESA, JAXA, the French space agency CNES (Centre National d’Études Spatiales), and the Max Planck Institute for Astronomy in Germany.

To learn more about the Roman mission, visit:
https://www.nasa.gov/roman

To learn more about NASA and the Kennedy Space Center please visit: 
https://www.nasa.gov/kennedy 


Credit: NASA 
Duration: 1 minute, 18 seconds
Release Date: Aug. 30, 2026

#NASA #Space #Astronomy #Science #SpaceX #FalconHeavyRocket #NASARoman #RomanSpaceTelescope #Encapsulation #NancyGraceRomanSpaceTelescope #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #NASAKennedy #Florida #UnitedStates #STEM #Education #HD #Video

NASA's Nancy Grace Roman Space Telescope Separates from Falcon Heavy Rocket

NASA's Nancy Grace Roman Space Telescope Separates from Falcon Heavy Rocket

Now on a three-month, million-mile journey to its final orbit, NASA’s Nancy Grace Roman Space Telescope will soon reveal the universe’s darkest secrets. The mission launched at 7:26 a.m. EDT Sunday aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.

Roman pairs a large field of view with crisp infrared vision to explore vast swaths of the sky and probe deeply into cosmic history. This flagship mission will help astronomers explore dark matter, dark energy, and worlds outside of our solar system, known as exoplanets. Its surveys will support a broad range of research extending far beyond the mission’s main science goals.

The ground control team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, began receiving telemetry data from Roman seven minutes after launch. The Falcon Heavy rocket performed as expected, separating from the observatory 31 minutes into the flight. After separating from the center core, the rocket’s boosters safely returned to the launch site for refurbishment.

During launch and early orbit, Roman uses the Near Space Network’s ground stations and relay satellites to exchange tracking, telemetry, and command data with ground controllers. About 70 minutes after launch, the Deep Space Network takes over communications and guides Roman toward the second Sun-Earth Lagrange point, or L2, about one million miles from Earth. Roman connects to that network through the Canberra Deep Space Communication Complex in Australia first. Approximately six hours later it will transfer to the Madrid Deep Space Communication Complex in Spain and then to the Goldstone Deep Space Communication Complex in California, ensuring continuous contact with Roman throughout its journey.

The Roman team also confirmed successful deployment of the observatory’s solar panels and lower instrument sun shade an hour and 23 minutes after launch. Within the upcoming days, Roman’s high-gain antenna and visor-like deployable aperture cover will deploy, ground controllers will initiate the first of two-mid-course corrections, and the Coronagraph Instrument will power on. This instrument will demonstrate the technology that future missions like NASA’s Habitable Worlds Observatory concept could use to image Earth-like planets in the search for life in the universe. Roman’s Coronagraph will take a giant step in that direction by snapping pictures of Jupiter-like planets.

A few weeks into Roman’s voyage, its primary instrument, the Wide Field Instrument, will activate. This 300-megapixel infrared camera has 18 4K detectors, each about the size of a saltine cracker. These detectors collect photons of light that will be decoded into crisp cosmic panoramas. Thanks to the observatory’s rigid design and stable optical performance, it will rapidly scan the sky without needing substantial time between separate observations. The Roman telescope is designed to survey the universe a thousand times faster than NASA’s Hubble Space Telescope.

Throughout the rest of Roman’s three-month commissioning period, scientists will run the instruments through a series of calibrations and tests. NASA anticipates releasing Roman’s first images by early 2027.

Roman will send back 1.4 terabytes of data every day, the highest data rate of any NASA astrophysics mission, so far. Machine learning, artificial intelligence, and citizen scientists will help sift through it and flag significant findings, which astronomers can then study.

“We’ve never been able to view the universe with eyes like Roman’s before,” said Julie McEnery, Roman’s senior project scientist at NASA Goddard. “There’s no telling what more we’ll know and have seen by this time next year.”

Roman is the fourth primary mission NASA has launched on a Falcon Heavy rocket. Earlier this year, the agency’s Launch Services Program worked with SpaceX to accelerate the launch date to accommodate the space telescope’s early completion.

The telescope is managed at NASA Goddard with participation by the agency’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a team of scientists from various research institutions. The primary industrial partners are BAE Systems Inc., L3Harris Technologies, and Teledyne Scientific & Imaging. Contributions to Roman also are made by ESA, JAXA, the French space agency CNES (Centre National d’Études Spatiales), and the Max Planck Institute for Astronomy in Germany.

To learn more about the Roman mission, visit:
https://www.nasa.gov/roman


Credit: NASA
Duration: 1 minute
Date: Aug. 30, 2026

#NASA #Space #Astronomy #Science #SpaceX #FalconHeavyRocket #NASARoman #RomanSpaceTelescope #Encapsulation #NancyGraceRomanSpaceTelescope #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #NASAKennedy #Florida #UnitedStates #STEM #Education #HD #Video