Wednesday, September 02, 2026

China's Kinastra-1 Upper Stage expected to make first flight next year

China's Kinastra-1 Upper Stage expected to make first flight next year

The Kinastra-1 Upper Stage, independently developed by Chinese company CAS Space, is expected to make its maiden flight in Q1 next year, the country’s Science and Technology department reported recently.

As the upper stage, the Kinastra-1 will work like a transport vehicle for satellites. After it is launched into space along with the satellite payload, the rocket drops off, and the Kinastra-1 Upper Stage takes over, transfering satellites between orbits.

And now, after completing months of testing, the upper stage has accumulated over 5,200 seconds of engine ignition tests and is ready for flight tests.

The chief designer of the Kinastra-1 says in the future, it will be used in tandem with the Kinetica-2 rocket (also known as Lijian-2) for a number of scenarios.

Kinetica-2 is a Chinese medium-lift orbital launch vehicle developed by CAS Space. Kinetica-2 uses two liquid-propellant rocket stages. In its initial configuration, first stage propulsion uses a modular rocket design with three identical rockets strapped together side-by-side. It is capable of lifting 12 t (12 long tons; 13 short tons) to low Earth orbit (LEO) or 8.0 t (7.9 long tons; 8.8 short tons) to a 500 km (310 mi) Sun-synchronous orbit (SSO).

CAS Space is a Chinese commercial space launch provider based in Guangzhou, capital and largest city of Guangdong province in southern China. CAS Space was founded in 2018 and is majority owned by the Chinese Academy of Sciences (CAS).

China's 15th Five Year Plan, started this year, aims turn the country's space industry into one of its "emerging pillar" industries along with integrated circuits and biomedicine.


Video Credit: SMG
Duration: 1 minute, 27 seconds
Date: Sept. 1, 2026

#NASA #Space #Satellites #Earth #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #Kinetica2 #力箭二号 #Kinetica2Rocket #Lijian2 #Kinastra1 #Kinastra1UpperStage #CommercialSpace #STEM #Education #HD #Video

Meir & Adenot on Spacewalk | International Space Station

Meir & Adenot on Spacewalk | International Space Station

European Space Agency (ESA) astronaut Sophie Adenot, with her spacesuit’s gold‑plated helmet visor down, is tethered to the International Space Station.
Expedition 75 commander Jessica Meir of NASA points her camera toward her spacesuit’s helmet visor and takes an out-of-this-world “space selfie.”
Expedition 75 commander Jessica Meir of NASA rides the Canadarm2 robotic arm during a spacewalk for navigation and science maintenance outside the International Space Station.
From left, the Soyuz MS‑29 crew spacecraft, docked to the Prichal module, and Northrop Grumman’s Cygnus XL cargo spacecraft, berthed to the Unity module, are pictured as the International Space Station orbited 261 miles above the Pacific Ocean west of Peru.
From left, flight engineer Jack Hathaway, station commander Jessica Meir, and flight engineer Anil Menon—NASA astronauts and members of Expedition 75—pose for a portrait inside the International Space Station’s Quest airlock.
From left, Expedition 75 crewmates Sophie Adenot of European Space Agency (ESA) and Jessica Meir of NASA, flight engineer and station commander respectively, smile for a portrait while working together inside the International Space Station’s Quest airlock.
From left, astronauts Jessica Meir of NASA and Sophie Adenot of the European Space Agency (ESA) pose for a portrait inside the International Space Station’s Quest airlock while configuring spacesuits the day before they conducted a spacewalk together.
From left, astronauts Jessica Meir of NASA and Sophie Adenot of the European Space Agency (ESA) pose for a portrait inside the International Space Station’s Quest airlock while configuring spacesuits the day before they conducted a spacewalk together. 

NASA astronaut Jessica Meir and the European Space Agency (ESA) astronaut Sophie Adenot concluded their spacewalk outside the International Space Station at 3:29 p.m. EDT, September 1, 2026.

During the 6-hour, 49-minute spacewalk, Meir and Adenot installed a new retroflector on the forward port of the space station’s Harmony module to support spacecraft navigation during rendezvous and docking operations. The duo replaced a high-definition camera on the station’s truss and completed a swab of the space station’s exterior for microorganisms. They also partially completed work to install jumper cables for electrical systems and started work to prepare for the replacement of the Alpha Magnetic Spectrometer’s heat-rejecting radiator on a future spacewalk.

Mission Control deferred installing the remaining guide studs for the spectrometer’s replacement radiator so engineers can develop a plan to finish the work during a future spacewalk. As the crew fell behind the timeline, the mission control team also shifted completion of the remaining jumper cables and other noncritical tasks to a later date.

During the spacewalk, Adenot experienced mobility issues with her left arm. Meir took a look at Adenot’s suit and determined the glove heater harness was likely getting caught and causing limited movement in the left shoulder joint. Unzipping the joint seemed to resolve the issue ahead of the crew entering the airlock.

U.S. spacewalk 99 was Meir’s seventh and Adenot’s third. Meir now ranks third all-time among woman at NASA for total spacewalks, behind Peggy Whitson (10) and Suni Williams (9). It also was the 284th spacewalk in support of space station assembly, maintenance, and upgrades.

It also was the 284th spacewalk in support of space station assembly, maintenance, and upgrades.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

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 Credits: NASA's Johnson Space Center/A. Menon/S. Adenot
Image Dates: Aug. 28-Sept. 1, 2026


#NASA #Space #Science #ISS #Planets #Earth #Astronauts #Spacewalks #USSpacewalk99 #EVAs #Spacesuits #AnilMenon #SophieAdenot #France #CNES #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education

A New Decagon Detected Encircling Saturn’s South Pole | Hubble Space Telescope

A New Decagon Detected Encircling Saturn’s South Pole | Hubble Space Telescope

Two views of Saturn from NASA’s Hubble Space Telescope reveal a giant, evolving 10-sided atmospheric wave encircling the planet’s south pole. The feature, called a decagon, is the first large, persistent, regular-sided pattern observed at Saturn’s southern hemisphere.
By comparing observations taken over several years, researchers found that the pattern has become increasingly distinct since 2023, suggesting they may be witnessing a new atmospheric phenomenon develop on the gas giant. The “X” and dashed circle in the image on the right represent where data was not captured by Hubble.
A single wavelength of light from NASA’s Hubble Space Telescope's Wide Field Camera 3 provides a particularly clear view of the 10-sided atmospheric wave discovered encircling Saturn’s south pole. The feature, labeled “decagon,” is embedded within one of Saturn’s powerful jet streams. The wave is centered around 63 degrees south latitude, and its apparent position shifts slightly depending on the wavelength of light observed. Observations from Hubble at different wavelengths of light reveal the structure at different altitudes. Hubble observations also show that the feature was present as early as 2023 and has become more pronounced over subsequent years.
The “X” and dashed circle in the image represents where data was not captured by Hubble.

Recent NASA Hubble Space Telescope images show the gas giant Saturn and its southern pole, where astronomers have discovered a 10-sided atmospheric wave. Observations show the decagon extends through multiple layers of Saturn’s atmosphere.

Recent observations with NASA’s Hubble Space Telescope have revealed a giant, evolving, ten-sided atmospheric wave encircling Saturn's south pole. This discovery marks the first time a large, regular-sided jet pattern has been observed in the planet's southern hemisphere. The feature appears remarkably similar to Saturn's famous hexagon at its northern pole, but is also distinctly different, suggesting scientists may be witnessing a new atmospheric phenomenon develop on the iconic gas giant.

The results published Wednesday, Sept. 2, 2026, in the journal Science Advances

By piecing together several years of Hubble observations dating back to 2023, researchers found subtle hints of the structure beginning to emerge before it became a clearly defined pattern. Those observations were taken as part of Hubble’s Outer Planet Atmospheres Legacy (OPAL) program. It has photographed the outer planets annually for more than a decade. 

"We've never seen anything quite like this in Saturn's southern hemisphere," said Amy Simon, study co-author and OPAL principal investigator, NASA's Goddard Space Flight Center in Greenbelt, Maryland. "The northern hexagon has been there every time we've looked for more than 40 years. This feature is different—it appears to be strengthening, giving us the rare opportunity to watch a giant atmospheric pattern develop."

The discovery was possible because Saturn's changing seasons gradually brought the planet's south pole back into view from Earth, where astronomers that collectively analyze images of Saturn from ground-based observatories first identified it.

Agustín Sánchez-Lavega, lead author of the new study, is a researcher at the University of the Basque Country in Spain. The university manages a website, called Planetary Virtual Observatory Laboratory, that accepts ground-based images of solar system planets contributed by observers all over the world. It was in those images, first in 2024, that Sánchez-Lavega and amateur astronomers Trevor Barry and Jean-Paul Oger noticed a subtle undulating band along the southern pole. Additional 2025 imagery taken from the ground hinted even more strongly toward this decagon structure.

This is when the Hubble observations come into the picture. Hubble’s view from space offers unmatched image sharpness and spatial resolution over full rotations of Saturn without smearing by Earth’s atmosphere. 

“Given Saturn’s symmetry in its north-south jet stream system, we have been searching for a counterpart to Saturn’s northern hexagon on the south pole in Hubble images since 1990,” Sánchez-Lavega said. “Images from NASA’s Cassini spacecraft, which orbited Saturn between 2004 and 2017, showed no inkling of a long-lived formation, either. The Hubble data confirmed the feature’s presence back to 2023.”

The wave sits within one of Saturn's powerful jet streams and extends through multiple layers of the atmosphere, indicating it is not just a cloud-level feature, but a vertically extended atmospheric structure. The decagon’s apparent position shifts slightly, because Hubble captures images from a range of wavelengths for a variety of altitudes in Saturn's atmosphere.

“The most intriguing part to me is that this seems to have just formed recently,” said Simon. “The question is, why did it suddenly form now when we haven't seen one before?” 

The authors say further study is needed from Hubble and NASA’s James Webb Space Telescope, as well as analysis of computer models, to understand how the decagon formed, how long it may last, and how it compares to the long-lived hexagon in the north.

Hubble’s long duration in operation has allowed astronomers to track changes over time in solar system planets and other astronomical objects as well.

Rather than providing a single snapshot, the OPAL program allows scientists to follow seasonal changes, track short-lived storms, and identify other atmospheric features that evolve slowly over time.

"When we started the OPAL program, we expected compelling surprises, but we didn't know what to expect specifically,” said Mike Wong, study co-author, University of California, Berkeley. “A lot of the discoveries we see coming from OPAL are not just based on one observation, but on years and years of data. Regular observations over time are enabling a lot of new findings."

The team plans to continue observing Saturn to determine whether the decagon settles into a long-lived, stable configuration like the northern hexagon or continues to evolve. Future observations also could help scientists determine what drives the wave, what it reveals about the atmospheric dynamics of giant planets throughout the solar system, and how they may relate to those we see here on Earth.

The Hubble Space Telescope has been operating for more than three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and the European Space Agency (ESA). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.


Image Credits: NASA, ESA, STScI, Agustin Sánchez-Lavega (UPV), Amy Simon (NASA-GSFC), Michael Wong (UC Berkeley)
Image Processing: Alyssa Pagan
Text Credit: NASA's Goddard Space Flight Center
Release Date: Sept. 2, 2026

#NASA #Hubble #Astronomy #Space #Science #Planets #Saturn #Atmospheres #SouthPole #Decagon #SolarSystem #SpaceExploration #Cosmos #Universe #HST #HubbleSpaceTelescope #WFC3 #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education

Space Cooperation Becomes Model for Chinese-Egyptian Relations

Space Cooperation Becomes Model for Chinese-Egyptian Relations

Space science and exploration has become a model field for cooperation between China and Egypt, and the partnership will be further strengthened by the Chang’e‑7 Mission, when China is scheduled to deliver an Egyptian payload to the lunar south pole.

China has already helped Egypt build the Debris and Satellite Monitoring Station, providing the North African country with all the technologies needed, including laser-equipped telescopes.

The two countries have also worked together to launch a number of telecom and remote sensing satellites into space.

"China started opening its space program to the world. It began cooperation with Egypt, as a gateway for it, to introduce this technology and science to Africa," said Osama Shalabiea, dean at the Faculty of Navigation Science and Space Technology at Beni Suef University.

China has also equipped an Assembly, Integration and Test (AIT) center in Egypt with all the necessary tools to design, assemble and test payloads before launching them to space.

The upcoming Chang'e-7 launch will mark another milestone in this technological relationship, as China and Egypt team up with Bahrain for the Moon exploration mission.

"China is taking an ambitious and unprecedented step through the Chang'e-7 Mission. The mission surpasses what we would have imagined or hoped for. It’s a complex mission that involves countries from all over the world. We are installing a precision multi-spectrum camera that will take pictures of the Moon's surface. This is a great participation under Arab-Arab and the Arab-Chinese cooperation," said Shalabiea.

Besides technology, China is also providing post graduate scholarships to Egyptian students.

Cooperation with China has helped Egypt advance its space program. With Chang'e-7 setting a new standard in this advanced technological partnership, it has put Egypt among the first countries in the Middle East and Africa to deploy a camera to the South Pole of the Moon.


Video Credit: CCTV
Duration: 2 minutes
Release Date: Sept. 2, 2026

#NASA #CNSA #Space #Satellites #Astronomy #Science #China #中国 #Egypt #CAS #Moon #Geology #WaterIce #SouthPole #CLEP #Change7 #嫦娥七号 #SpaceRobotics #SpaceTechnology #LunarExploration #DeepSpace #SolarSystem #STEM #Education #Russia #InternationalCooperation #STEM #Education #HD #Video

Dark Nebula LDN 1165 in Cepheus | Hubble Space Telescope

Dark Nebula LDN 1165 in Cepheus | Hubble Space Telescope

This Hubble image captures a portion of a dark nebula in the constellation Cepheus. LDN 1165 is part of a collection called Lynds’ Catalog of Dark Nebulae, originally published in 1962. Dark nebulae― also called absorption nebulae―are clouds of gas and dust that neither emit nor reflect light, instead blocking light coming from behind them. These nebulae tend to contain large amounts of dust. This allows them to absorb visible light from stars or nebulae beyond them. Dark nebulae are so dark that they have been referred to as “holes in the sky,” but in reality they may be full of activity with stars sometimes forming inside their dense clouds.

Hubble observed this region as part of a study of protostars, hot dense cores of newly forming stars that are accumulating gas and dust as they undergo the starbirth process. The bright area in this image is likely a star-forming region that may hold one or more young protostars. Further study of dark nebulae like LDN 1165 will help us better understand the nature of these dark and dusty clouds and the stellar nurseries that may lurk within them.


Image Credit: NASA, ESA, T. Megeath (University of Toledo), and K. Stapelfeldt (Jet Propulsion Laboratory)
Image Processing: Gladys Kober (NASA/Catholic University of America)
Release Date: Oct. 24, 2021

#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Protostars #StellarNurseries #Nebulae #DarkNebulae #LDN1165 #CepheusConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

The Prawn Nebula in Scorpius: Visible light & infrared | Hubble

The Prawn Nebula in Scorpius: Visible light & infrared | Hubble

The Prawn Nebula is a massive stellar nursery located in the constellation Scorpius, about 6,000 light years from Earth. Although the nebula stretches 250 light-years and covers a space four times the size of the full Moon, it emits light primarily in wavelengths the human eye cannot detect, making it extremely faint to earthbound viewers. Hubble’s gaze, however, shows a small section of the nebula here in visible and invisible infrared light, capturing dazzling detail of the nebula’s structure, including bright areas of glowing gas.

The Prawn Nebula, also known as IC 4628, is an emission nebula. This means its gas has been energized, or ionized, by the radiation of nearby stars. The radiation from these massive stars strips electrons from the nebula’s hydrogen atoms. As the energized electrons revert from their higher-energy state to a lower-energy state by recombining with hydrogen nuclei, they emit energy in the form of light, causing the nebula’s gas to glow. In this image, red indicates the presence of ionized iron (Fe II) emission.

This Hubble Space Telescope image was captured as part of a survey of massive- and intermediate-size “protostars,” or newly forming stars. Astronomers used the infrared sensitivity of Hubble’s Wide Field Camera 3 to look for hydrogen ionized by ultraviolet light ionized by the protostars, jets from the stars, and other features.


Credit: NASA, ESA, and J. Tan (Chalmers University of Technology); Processing; Gladys Kober (NASA/Catholic University of America)
Release Date: Oct. 24, 2021


#NASA #ESA #Hubble #Astronomy #Space #Science #Nebulae #PrawnNebula #EmissionNebulae #IC4628 #Gum56 #ScorpiusConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #WFC3 #OpticalAstronomy #InfraredAstronomy #GSFC #STScI #UnitedStates #Europe #STEM #Education

NASA & SpaceX Adjust Crew-13 Launch Date | International Space Station

NASA & SpaceX Adjust Crew-13 Launch Date | International Space Station

The four members of NASA's SpaceX Crew-13 mission to the International Space Station display their mission plaque inside a training mockup of a space station module. From left are, Commander Jessica Watkins and Pilot Luke Delaney, both from NASA, and Mission Specialists Joshua Kutryk of the Canadian Space Agency (CSA) and Sergey Teteryatnikov of Roscosmos (Russia).
NASA astronaut Jessica Watkins, commander of NASA’s SpaceX Crew-13 mission
Roscosmos cosmonaut Sergey Teteryatnikov of Russia, mission specialist of NASA’s SpaceX Crew-13 mission
NASA astronaut Luke Delaney, pilot of NASA’s SpaceX Crew-13 mission
Canadian Space Agency (CSA) astronaut Joshua Kutryk, mission specialist of NASA’s SpaceX Crew-13 mission
NASA's SpaceX Crew-13 emblem

NASA and SpaceX are adjusting the launch date for the agency’s Crew-13 mission to the International Space Station to address an oxidizer leak on their Dragon spacecraft’s propulsion system. It was detected during standard prelaunch spacecraft processing. Joint NASA and SpaceX teams are performing additional tests and data review and will complete any necessary rework prior to launch. A new target date will be announced once available.

NASA astronauts Jessica Watkins and Luke Delaney will serve as spacecraft commander and pilot, respectively. They will be joined by Canadian Space Agency (CSA) astronaut Joshua Kutryk and Roscosmos cosmonaut Sergey Teteryatnikov of Russia, who will serve as mission specialists. After arriving at the orbiting laboratory, Crew-13 will become members of the space station’s Expedition 75. The crew will enter quarantine about two weeks prior to flight from the agency’s Johnson Space Center in Houston.

Crew-13 will lift off aboard SpaceX’s Dragon spacecraft on the company’s Falcon 9 rocket from Space Launch Complex 40 in Cape Canaveral, Florida.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

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 Credits: NASA/Morgan Gridley, SpaceX
Release Date: Aug. 1, 2026

#NASA #Space #Science #Earth #ISS #SpaceXCrew13 #Astronauts #JessicaWatkins #LukeDelaney #JoshuaKutryk #CanadianSpaceAgency #CSA #Canada #SergeyTeteryatnikov #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition75 #NASAJSC #Houston #Texas #UnitedStates #STEM #Education

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

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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