Wednesday, June 17, 2026

China Long March 12 Rocket Transport: Pre-launch of Internet Satellites in Hainan

China Long March 12 Rocket Transport: Pre-launch of Internet Satellites in Hainan

🚀A China Long March 12 Y17 rocket lifted off at 10:44am Beijing Time (BJT) on June 17, 2026, from Hainan province's Wenchang Commercial Space Launch Site with GuoWang SatNet low Earth orbit (LEO) Group 22 Internet satellites. 

The nine satellites represent the twenty-second group for the the GuoWang constellation and were produced by the China Academy of Spaceflight Technology (CAST).

The GuoWang (国网) constellation is operated by China Satellite Network Group, a state-owned enterprise and backed by the Chinese government. The China Satellite Network Group plans to provide worldwide Internet services; for now, China-focused services are the immediate priority.

After today’s launch, 177 GuoWang spacecraft are in orbit, functioning in and heading up to their operational orbits. This year, 310 satellites are expected to be deployed, followed by 900 in 2027, and 3,600 every year beginning in 2028 to sustain and grow the constellation. In the 2030s, up to 13,000 satellites could be in operational orbit.

GuoWang satellites launched atop of the Long March 12 and the Long March 8A use the mega-constellations’ small satellite platform, weighing about 695 kilograms each. A large satellite platform, around thirty percent bigger and weighing up to 1,000 kilograms, is launched via the Long March 5B and Long March 6A. Both platforms utilize electric propulsion systems to maneuver in orbit, powered by two solar panels.

Starting with this mission, the Long March 12’s 5.2-meter-diameter fairing has been switched to a lighter carbon fiber composite material, according to the Shanghai Academy of Spaceflight Technology. Improvements stated during previous flights have said that the launch vehicle has shed unnecessary weight as part of cost-optimization efforts while maintaining quality standards.

Another change implemented was the use of ‘high-energy’ kerosene in the second-stage and its two YF-115 engines.

This mission was the 6th launch of a Long March 12 vehicle, the 8th launch of the Shanghai Academy of Spaceflight Technology-supported Long March 12 series, and the 652nd launch of the Long March launch vehicle series. This was also the 42nd launch from China in 2026.

Guowang (国网), meaning "national network", is a state-sponsored low-Earth orbit satellite Internet constellation developed by China Aerospace Science and Industry Corporation (CASIC) and managed by China. The goal is to create a system of worldwide Internet coverage. It was created by China Aerospace Science and Industry Corporation (CASIC), a state-owned enterprise backed by the Chinese Academy of Space Technology (CAST).

The Long March 12 (Chang Zheng 12, abbreviated as CZ-12 within China), is a Chinese medium-lift launch vehicle carrier rocket. Both stages use liquid fuel: refined kerosene (RP-1) and liquid oxygen (LOX). The manufacturer is Shanghai Academy of Spaceflight Technology. It is capable of placing at least 12 tonnes (26,000 lb) of payload in low Earth orbit and at least 6 tonnes (13,000 lb) in a 700 kilometers (430 mi) Sun-synchronous orbit. Its first launch took place on November 30, 2024, from the Hainan International Commercial Aerospace Launch Site on Hainan island.


Video Credit: CASIC
Duration: 30 seconds
Date: June 14, 2026


#NASA #Space #Earth #Satellites #InternetSatellites #GuoWangConstellation #国网 #China #中国 #Rockets #LongMarch12Y17Rockets #长征十二号运载火箭 #MediumLiftRockets #CAST #CASIC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Wenchang #Spaceports #Hainan #STEM #Education #HD #Video

China Long March 12 Launch of GuoWang Internet Constellation Satellites in Hainan

China Long March 12 Launch of GuoWang Internet Constellation Satellites in Hainan

🚀A China Long March 12 Y17 rocket lifted off at 10:44am Beijing Time (BJT) on June 17, 2026, from Hainan province's Wenchang Commercial Space Launch Site with GuoWang SatNet low Earth orbit (LEO) Group 22 Internet satellites. 

The nine satellites represent the twenty-second group for the the GuoWang constellation and were produced by the China Academy of Spaceflight Technology (CAST).

The GuoWang (国网) constellation is operated by China Satellite Network Group, a state-owned enterprise and backed by the Chinese government. The China Satellite Network Group plans to provide worldwide Internet services; for now, China-focused services are the immediate priority.

After today’s launch, 177 GuoWang spacecraft are in orbit, functioning in and heading up to their operational orbits. This year, 310 satellites are expected to be deployed, followed by 900 in 2027, and 3,600 every year beginning in 2028 to sustain and grow the constellation. In the 2030s, up to 13,000 satellites could be in operational orbit.

GuoWang satellites launched atop of the Long March 12 and the Long March 8A use the mega-constellations’ small satellite platform, weighing about 695 kilograms each. A large satellite platform, around thirty percent bigger and weighing up to 1,000 kilograms, is launched via the Long March 5B and Long March 6A. Both platforms utilize electric propulsion systems to maneuver in orbit, powered by two solar panels.

Starting with this mission, the Long March 12’s 5.2-meter-diameter fairing has been switched to a lighter carbon fiber composite material, according to the Shanghai Academy of Spaceflight Technology. Improvements stated during previous flights have said that the launch vehicle has shed unnecessary weight as part of cost-optimization efforts while maintaining quality standards.

Another change implemented was the use of ‘high-energy’ kerosene in the second-stage and its two YF-115 engines.

This mission was the 6th launch of a Long March 12 vehicle, the 8th launch of the Shanghai Academy of Spaceflight Technology-supported Long March 12 series, and the 652nd launch of the Long March launch vehicle series. This was also the 42nd launch from China in 2026.

Guowang (国网), meaning "national network", is a state-sponsored low-Earth orbit satellite Internet constellation developed by China Aerospace Science and Industry Corporation (CASIC) and managed by China. The goal is to create a system of worldwide Internet coverage. It was created by China Aerospace Science and Industry Corporation (CASIC), a state-owned enterprise backed by the Chinese Academy of Space Technology (CAST).

The Long March 12 (Chang Zheng 12, abbreviated as CZ-12 within China), is a Chinese medium-lift launch vehicle carrier rocket. Both stages use liquid fuel: refined kerosene (RP-1) and liquid oxygen (LOX). The manufacturer is Shanghai Academy of Spaceflight Technology. It is capable of placing at least 12 tonnes (26,000 lb) of payload in low Earth orbit and at least 6 tonnes (13,000 lb) in a 700 kilometers (430 mi) Sun-synchronous orbit. Its first launch took place on November 30, 2024, from the Hainan International Commercial Aerospace Launch Site on Hainan island.


Video Credit: CASIC
Duration: 1 minute
Date: June 17, 2026


#NASA #Space #Earth #Satellites #InternetSatellites #GuoWangConstellation #国网 #China #中国 #Rockets #LongMarch12Y17Rockets #长征十二号运载火箭 #MediumLiftRockets #CAST #CASIC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Wenchang #Spaceports #Hainan #STEM #Education #HD #Video

China Long March 12 Launch of GuoWang Internet Constellation Satellites in Hainan

China Long March 12 Launch of GuoWang Internet Constellation Satellites in Hainan




Shanghai Academy of Spaceflight Technology’s Long March 12 Y7 launch mission emblem

🚀 A China Long March 12 Y17 rocket lifted off at 10:44am Beijing Time (BJT) on June 17, 2026, from Hainan province's Wenchang Commercial Space Launch Site with GuoWang SatNet low Earth orbit (LEO) Group 22 Internet satellites. 

The nine satellites represent the twenty-second group for the the GuoWang constellation and were produced by the China Academy of Spaceflight Technology (CAST).

The GuoWang (国网) constellation is operated by China Satellite Network Group, a state-owned enterprise and backed by the Chinese government. The China Satellite Network Group plans to provide worldwide Internet services; for now, China-focused services are the immediate priority.

After today’s launch, 177 GuoWang spacecraft are in orbit, functioning in and heading up to their operational orbits. This year, 310 satellites are expected to be deployed, followed by 900 in 2027, and 3,600 every year beginning in 2028 to sustain and grow the constellation. In the 2030s, up to 13,000 satellites could be in operational orbit.

GuoWang satellites launched atop of the Long March 12 and the Long March 8A use the mega-constellations’ small satellite platform, weighing about 695 kilograms each. A large satellite platform, around thirty percent bigger and weighing up to 1,000 kilograms, is launched via the Long March 5B and Long March 6A. Both platforms utilize electric propulsion systems to maneuver in orbit, powered by two solar panels.

Starting with this mission, the Long March 12’s 5.2-meter-diameter fairing has been switched to a lighter carbon fiber composite material, according to the Shanghai Academy of Spaceflight Technology. Improvements stated during previous flights have said that the launch vehicle has shed unnecessary weight as part of cost-optimization efforts while maintaining quality standards.

Another change implemented was the use of ‘high-energy’ kerosene in the second-stage and its two YF-115 engines.

This mission was the 6th launch of a Long March 12 vehicle, the 8th launch of the Shanghai Academy of Spaceflight Technology-supported Long March 12 series, and the 652nd launch of the Long March launch vehicle series. This was also the 42nd launch from China in 2026.

Guowang (国网), meaning "national network", is a state-sponsored low-Earth orbit satellite Internet constellation developed by China Aerospace Science and Industry Corporation (CASIC) and managed by China. The goal is to create a system of worldwide Internet coverage. It was created by China Aerospace Science and Industry Corporation (CASIC), a state-owned enterprise backed by the Chinese Academy of Space Technology (CAST).

The Long March 12 (Chang Zheng 12, abbreviated as CZ-12 within China), is a Chinese medium-lift launch vehicle carrier rocket. Both stages use liquid fuel: refined kerosene (RP-1) and liquid oxygen (LOX). The manufacturer is Shanghai Academy of Spaceflight Technology. It is capable of placing at least 12 tonnes (26,000 lb) of payload in low Earth orbit and at least 6 tonnes (13,000 lb) in a 700 kilometers (430 mi) Sun-synchronous orbit. Its first launch took place on November 30, 2024, from the Hainan International Commercial Aerospace Launch Site on Hainan island.


Image Credits: CASIC, CAST
Date: June 17, 2026


#NASA #Space #Earth #Satellites #InternetSatellites #GuoWangConstellation #国网 #China #中国 #Rockets #LongMarch12Y17Rockets #长征十二号运载火箭 #MediumLiftRockets #CAST #CASIC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Wenchang #Spaceports #Hainan #STEM #Education

Launch of Ariane 6 Rocket with Upgraded Boosters: Amazon Leo Satellites | ESA

Launch of Ariane 6 Rocket with Upgraded Boosters: Amazon Leo Satellites | ESA









"On June 17, 2026, at 09:21 local time (13:21 BST, 14:21 CEST), Ariane 6 flight VA269 soared to orbit from Europe’s Spaceport in French Guiana. Thirty-six satellites for Amazon’s Leo constellation left Earth powered by four P160C-based boosters, the first time these upgraded boosters were used—making this launch the most powerful so far for Europe’s heavy-lift rocket."

36 Amazon Leo satellites deployed

🔥 First flight with P160C boosters.

📦 Heaviest payload of an Ariane launcher.

📈 The biggest Amazon Leo stack launched to date

"With flight VA269, Ariane 6 has now launched 100 Amazon Leo satellites in five months.

The mission marks the third Ariane 6 launch dedicated to the deployment of the Amazon Leo constellation and is the eighth Ariane 6 launch and the third of the year.

The debut of the four new boosters based on the P160C solid-propellant rocket motor allowed 36 Leo satellites to be launched—four more than the two Leo launches Ariane 6 has delivered before. 

The P160C solid-rocket motor holds 156 tonnes of propellant, 14 tonnes more than its predecessor P120C and is 14.5 m tall. In the runup to an Ariane 6 launch the P160C motor is turned into an Ariane 6 booster by adding aerodynamic fairing and other hardware such as connections specific for Ariane 6. Although P160C is a meter taller than the P120C motor, the additional height does not affect the connection to Ariane 6’s central core nor the height of the Ariane 6 booster as there is room in the fairing to accommodate the height increase. 

Ariane 6 is the latest rocket in a long history of launchers to fly from Europe’s Spaceport in French Guiana—demonstrating the power of multinational cooperation for over five decades. Ariane 6 is Europe’s heavy-lift launcher and a key element of the European Space Agency’s efforts to ensure autonomous access to space for Europe’s citizens. Its modular and versatile design allows it to launch all types of missions, from low-Earth orbit to deep space. The new P160C boosters increase considerably performance, payload capacity and competitiveness, allowing for more satellites to be launched, further elevating the future of Europe."


Credits: ESA/CNES/Arianespace/ArianeGroup
Dates: June 15-17, 2026

#NASA #ESA #Space #Satellites #AmazonLeoSatellites #CommunicationsSatellites #CommercialSpace #Arianespace #Ariane6 #Ariane6Rocket #HeavyLiftRocket #RocketLaunch #MissionVA269 #GuianaSpaceCentre #KourouSpaceport #Kourou #FrenchGuiana #SouthAmerica #France #CNES #ArianeGroup #Europe #STEM #Education

Launch of Ariane 6 Rocket with Upgraded Boosters: Amazon Leo Satellites | ESA

Launch of Ariane 6 Rocket with Upgraded Boosters: Amazon Leo Satellites | ESA

"On June 17, 2026, at 09:21 local time (13:21 BST, 14:21 CEST), Ariane 6 flight VA269 soared to orbit from Europe’s Spaceport in French Guiana. Thirty-six satellites for Amazon’s Leo constellation left Earth powered by four P160C-based boosters, the first time these upgraded boosters were used—making this launch the most powerful so far for Europe’s heavy-lift rocket. 

36 Amazon Leo satellites deployed

🔥 First flight with P160C boosters.

📦 Heaviest payload of an Ariane launcher.

📈 The biggest Amazon Leo stack launched to date

With flight VA269, Ariane 6 has now launched 100 Amazon Leo satellites in five months.

The mission marks the third Ariane 6 launch dedicated to the deployment of the Amazon Leo constellation and is the eighth Ariane 6 launch and the third of the year.

The debut of the four new boosters based on the P160C solid-propellant rocket motor allowed 36 Leo satellites to be launched—four more than the two Leo launches Ariane 6 has delivered before. 

The P160C solid-rocket motor holds 156 tonnes of propellant, 14 tonnes more than its predecessor P120C and is 14.5 m tall. In the runup to an Ariane 6 launch the P160C motor is turned into an Ariane 6 booster by adding aerodynamic fairing and other hardware such as connections specific for Ariane 6. Although P160C is a meter taller than the P120C motor, the additional height does not affect the connection to Ariane 6’s central core nor the height of the Ariane 6 booster as there is room in the fairing to accommodate the height increase. 

Ariane 6 is the latest rocket in a long history of launchers to fly from Europe’s Spaceport in French Guiana—demonstrating the power of multinational cooperation for over five decades. Ariane 6 is Europe’s heavy-lift launcher and a key element of the European Space Agency’s efforts to ensure autonomous access to space for Europe’s citizens. Its modular and versatile design allows it to launch all types of missions, from low-Earth orbit to deep space. The new P160C boosters increase considerably performance, payload capacity and competitiveness, allowing for more satellites to be launched, further elevating the future of Europe."


Credits: ESA/CNES/Arianespace/ArianeGroup
Duration: 3 minutes, 37 seconds
Release Date: June 17, 2026

#NASA #ESA #Space #Satellites #AmazonLeoSatellites #CommunicationsSatellites #CommercialSpace #Arianespace #Ariane6 #Ariane6Rocket #HeavyLiftRocket #RocketLaunch #MissionVA269 #GuianaSpaceCentre #KourouSpaceport #Kourou #FrenchGuiana #SouthAmerica #France #CNES #ArianeGroup #Europe #STEM #Education #HD #Video

Tuesday, June 16, 2026

Rare Daytime Occultation of Planet Venus by Moon: View from California

Rare Daytime Occultation of Planet Venus by Moon: View from California

Astrophotographer David Pinsky: "This Wednesday, June 17th, 2026, you may wish to do something unusual. Go outside under the blue sky and stand in the shadow of a building. This is the best place to see the daylight occultation of Venus. Occultation refers to the process where a celestial body, such as a star or planet, temporarily obscures another body, allowing astronomers to study its properties."

"Can you really see this during the day?"

"You can! For the first time in 11 years, the crescent Moon will pass in front of Venus in broad daylight over the USA, both well separated from the Sun. The bright planet will disappear behind the Moon's dark edge and reappear about an hour later. Scan the blue sky with binoculars until you find the Moon's pale crescent. Once located, you'll discover the Moon and Venus are surprisingly easy to see with the naked eye. A smartphone camera zoomed and pointed in the right direction will have no trouble recording the scene."

Warning: Never point your optics at the Sun.

California is a state in the Western United States that lies on the Pacific Coast. It borders Oregon to the north, Nevada and Arizona to the east, and shares an international border with the Mexican state of Baja California to the south. 

Image Credit: David Pinsky
Text Credit: SpaceWeather[dot]com
Location: West Hollywood, California, USA
Image Details: Canon Rebel T3i, Celestron 5 inch Maksutov at prime focus at 1/40 sec, ISO 100
Release Date: Dec. 7, 2015

#NASA #Astronomy #Space #Science #SolarSystem #Planets #Venus #Earth #Moon #Occultation #Astrophotography #DavidPinsky #Astrophotographers #CitizenScience #WestHollywood #California #UnitedStates #STEM #Education

Journey to Terzan 5: A Milky Way Bulge Fossil Fragment | Webb & Hubble Telescopes

Journey to Terzan 5: A Milky Way Bulge Fossil Fragment | Webb & Hubble Telescopes

New observations from the James Webb Space Telescope combined with multiple observations from the Hubble Space Telescope demonstrate that Terzan 5 is a self-contained, self-enriching stellar system that contains up to four distinct star populations. It orbits within our Milky Way galaxy’s central bulge.

Researchers using two of humanity’s most powerful observatories—NASA’s James Webb and Hubble Space Telescopes—have definitively shown that Terzan 5 is not a globular star cluster as it was once classified, offering new insight into how galaxies like our own form and evolve over time. A globular star cluster typically has only one ancient star population. New data not only confirms the existence of two distinct populations of stars in Terzan 5, but also provides evidence for two more recent rounds of star formation. Although located within the crowded bulge of our Milky Way, our galaxy’s central, spherical region of older stars, Terzan 5 was massive enough to maintain its separate identity while lighter weight systems spread out and mixed to form the bulge billions of years ago. It is like a lump in an otherwise well-mixed cake batter.

“Webb’s new near-infrared observations, cross-referenced with Hubble’s archival observations, have given us a much clearer picture of the history of Terzan 5,” said Giorgia Zullo, who led the research and is a PhD student at the University of Bologna in Italy.

These results were presented at a press conference Tuesday, June 16, 2026, at the 248th meeting of the American Astronomical Society in Pasadena, California, and were published in Astronomy & Astrophysics.

New observations from Webb combined with multiple observations from Hubble show that Terzan 5 is a self-contained, self-enriching stellar system that contains up to four distinct star populations. It orbits within our Milky Way galaxy’s central bulge.

Four generations of stars
Discovered in 1968 by astronomer Azop Terzan, Terzan 5 resembles a globular cluster in many ways. However, in 2009 this system was discovered to harbor two distinct populations of stars. In 2016, Hubble provided the first estimate of their ages, showing that one formed roughly 12 billion years ago—as the Milky Way itself was assembling—and the other about 5 billion years ago, just before Earth started forming. This pointed to a more complex history than a typical globular cluster.

Studying Terzan 5 is complicated by its location in a region of our galaxy crowded with stars and heavily obscured by dust. This is where Webb stepped in. Its infrared view allowed the research team to peer through the dust and catalog many more stars, and fainter stars, than previous work. By measuring star colors and brightnesses, astronomers can classify them into populations across their ages and chemistries.

Webb was able to measure these key properties for every star within the field of view in the sky—both stars within Terzan 5 and unrelated foreground stars. To isolate the stars of Terzan 5, the team relied on the power and longevity of Hubble. The 12-year separation allowed the team to measure very small movements of individual stars, known as proper motions, to determine that stars belong to Terzan 5 and are part of the Milky Way's bulge.

By combining data from Webb and Hubble, the researchers found strong evidence for two more stellar populations, one that formed 3.8 billion years ago and another only 2.5 billion years ago. They also were able to determine the precise age of the previously known stellar populations, finding that they formed 12.5 billion and 4.7 billion years ago.

With the previously known two generations of stars, astronomers could not rule out the possibility that Terzan 5 interacted with another object, like a globular cluster or a giant molecular cloud, becoming enriched with new gas and dust that set off a second round of star formation. With four stellar generations, those explanations are ruled out.

Measurements of the stellar composition of Terzan 5 populations made at the W. M. Keck Observatory and European Southern Observatory’s Very Large Telescope also point toward very distinct populations. “Along with the ages of these populations, the cluster preserves a fossil record of progressive enrichment of heavy elements by supernovae,” said co-author R. Michael Rich, a research astronomer at the University of California, Los Angeles.

Terzan 5 formed multiple generations of stars because it was able to retain the necessary raw materials. There is evidence of powerful supernova explosions in Terzan 5 that forged heavier elements that were swept up by subsequent generations of stars. In lighter weight systems, the force of the explosions themselves could have ejected the resulting elements as well as sweeping out leftover gas and dust. The progenitor of Terzan 5 had enough mass to retain those stars’ ejections, allowing new generations of stars to form over billions of years.

‘Bulge fossil fragment’
The results show that Terzan 5 is most likely the remnant of a much more massive stellar system that initially formed 12.5 billion years ago. Terzan 5 is extraordinary because it survived—and never merged or fully “mixed in” with the Milky Way’s bulge. “For some reason, this peculiar clump of stars formed separately from the bulge and was not destroyed as the bulge itself formed,” said Francesco R. Ferraro, a professor at the University of Bologna and principal investigator of the Webb observations. “Terzan 5 is what we now call a bulge fossil fragment because it resembles the primordial clumps that contributed to the formation of the bulge.”

To date, there is one other known cosmic object like Terzan 5. Liller 1 was the second to be reclassified from a globular star cluster to a bulge fossil fragment. It also contains multiple generations of stars. There may be more objects like it. Between 40 to 50 additional globular clusters that orbit within the bulge will be examined by Ferraro’s team to determine if their stellar populations are all the same, like globular clusters, or have several generations, like bulge fossil fragments. 

Potential parallels for galaxy formation near, far
Ultimately, this research may improve what we know about how the central bulges of galaxies form over hundreds of millions of years. “Based on observations and in-depth simulations, we think that galaxies in the early universe had huge disks of gas that fragmented into clumps and formed stars. These clumps migrated to the center of the galaxies, and many merged to form their bulges,” said Barbara Lanzoni, a co-author and associate professor at the University of Bologna. For example, Webb has turned up several examples of “clumpy” galaxies that were actively forming when the universe was only a few hundred million years old, like the clumps in the Firefly Sparkle galaxy. “Terzan 5 may provide direct evidence that can help explain how bulges formed in galaxies throughout the universe,” Lanzoni said.

Image Description: A dramatically crowded starfield that looks like a just-shaken snow globe. The black background of space, clearer at the edges, is covered by thousands of tiny white, orange, and blue points of light, that are stars. The stars are most concentrated in the center, forming a roughly circular orb, and sparser at the edges of the image. Several larger orange stars, particularly those largest near the edges of the frame, have prominent diffraction spikes.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).

The Hubble Space Telescope has been operating for over 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. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute (STScI) in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

Learn more about Webb:
https://science.nasa.gov/webb

Learn more about Hubble:
https://science.nasa.gov/hubble

Video: NASA, ESA, CSA, Alyssa Pagan (STScI); Acknowledgments: ESO, Pan-STARRS, DSS2, Akira Fujii
Duration: 30 seconds
Release Date: June 16, 2026

#NASA #ESA #Astronomy #Space #Science #Galaxies #SpiralGalaxies #MilkyWay #MilkyWayBulge  #Stars #StarClusters #Terzan5 #BulgeFossilFragment #Cosmos #Universe #JWST #InfraredAstronomy #HubbleSpaceTelescope #HST  #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Close-up: Terzan 5—A Milky Way Bulge Fossil Fragment | Webb & Hubble Telescopes

Close-up: Terzan 5A Milky Way Bulge Fossil Fragment | Webb & Hubble Telescopes

New observations from the James Webb Space Telescope combined with multiple observations from the Hubble Space Telescope demonstrate that Terzan 5 is a self-contained, self-enriching stellar system that contains up to four distinct star populations. It orbits within our Milky Way galaxy’s central bulge.

Researchers using two of humanity’s most powerful observatories—NASA’s James Webb and Hubble Space Telescopes—have definitively shown that Terzan 5 is not a globular star cluster as it was once classified, offering new insight into how galaxies like our own form and evolve over time. A globular star cluster typically has only one ancient star population. New data not only confirms the existence of two distinct populations of stars in Terzan 5, but also provides evidence for two more recent rounds of star formation. Although located within the crowded bulge of our Milky Way, our galaxy’s central, spherical region of older stars, Terzan 5 was massive enough to maintain its separate identity while lighter weight systems spread out and mixed to form the bulge billions of years ago. It is like a lump in an otherwise well-mixed cake batter.

“Webb’s new near-infrared observations, cross-referenced with Hubble’s archival observations, have given us a much clearer picture of the history of Terzan 5,” said Giorgia Zullo, who led the research and is a PhD student at the University of Bologna in Italy.

These results were presented at a press conference Tuesday, June 16, 2026, at the 248th meeting of the American Astronomical Society in Pasadena, California, and were published in Astronomy & Astrophysics.

New observations from Webb combined with multiple observations from Hubble show that Terzan 5 is a self-contained, self-enriching stellar system that contains up to four distinct star populations. It orbits within our Milky Way galaxy’s central bulge.

Four generations of stars
Discovered in 1968 by astronomer Azop Terzan, Terzan 5 resembles a globular cluster in many ways. However, in 2009 this system was discovered to harbor two distinct populations of stars. In 2016, Hubble provided the first estimate of their ages, showing that one formed roughly 12 billion years ago—as the Milky Way itself was assembling—and the other about 5 billion years ago, just before Earth started forming. This pointed to a more complex history than a typical globular cluster.

Studying Terzan 5 is complicated by its location in a region of our galaxy crowded with stars and heavily obscured by dust. This is where Webb stepped in. Its infrared view allowed the research team to peer through the dust and catalog many more stars, and fainter stars, than previous work. By measuring star colors and brightnesses, astronomers can classify them into populations across their ages and chemistries.

Webb was able to measure these key properties for every star within the field of view in the sky—both stars within Terzan 5 and unrelated foreground stars. To isolate the stars of Terzan 5, the team relied on the power and longevity of Hubble. The 12-year separation allowed the team to measure very small movements of individual stars, known as proper motions, to determine that stars belong to Terzan 5 and are part of the Milky Way's bulge.

By combining data from Webb and Hubble, the researchers found strong evidence for two more stellar populations, one that formed 3.8 billion years ago and another only 2.5 billion years ago. They also were able to determine the precise age of the previously known stellar populations, finding that they formed 12.5 billion and 4.7 billion years ago.

With the previously known two generations of stars, astronomers could not rule out the possibility that Terzan 5 interacted with another object, like a globular cluster or a giant molecular cloud, becoming enriched with new gas and dust that set off a second round of star formation. With four stellar generations, those explanations are ruled out.

Measurements of the stellar composition of Terzan 5 populations made at the W. M. Keck Observatory and European Southern Observatory’s Very Large Telescope also point toward very distinct populations. “Along with the ages of these populations, the cluster preserves a fossil record of progressive enrichment of heavy elements by supernovae,” said co-author R. Michael Rich, a research astronomer at the University of California, Los Angeles.

Terzan 5 formed multiple generations of stars because it was able to retain the necessary raw materials. There is evidence of powerful supernova explosions in Terzan 5 that forged heavier elements that were swept up by subsequent generations of stars. In lighter weight systems, the force of the explosions themselves could have ejected the resulting elements as well as sweeping out leftover gas and dust. The progenitor of Terzan 5 had enough mass to retain those stars’ ejections, allowing new generations of stars to form over billions of years.

‘Bulge fossil fragment’
The results show that Terzan 5 is most likely the remnant of a much more massive stellar system that initially formed 12.5 billion years ago. Terzan 5 is extraordinary because it survived—and never merged or fully “mixed in” with the Milky Way’s bulge. “For some reason, this peculiar clump of stars formed separately from the bulge and was not destroyed as the bulge itself formed,” said Francesco R. Ferraro, a professor at the University of Bologna and principal investigator of the Webb observations. “Terzan 5 is what we now call a bulge fossil fragment because it resembles the primordial clumps that contributed to the formation of the bulge.”

To date, there is one other known cosmic object like Terzan 5. Liller 1 was the second to be reclassified from a globular star cluster to a bulge fossil fragment. It also contains multiple generations of stars. There may be more objects like it. Between 40 to 50 additional globular clusters that orbit within the bulge will be examined by Ferraro’s team to determine if their stellar populations are all the same, like globular clusters, or have several generations, like bulge fossil fragments. 

Potential parallels for galaxy formation near, far
Ultimately, this research may improve what we know about how the central bulges of galaxies form over hundreds of millions of years. “Based on observations and in-depth simulations, we think that galaxies in the early universe had huge disks of gas that fragmented into clumps and formed stars. These clumps migrated to the center of the galaxies, and many merged to form their bulges,” said Barbara Lanzoni, a co-author and associate professor at the University of Bologna. For example, Webb has turned up several examples of “clumpy” galaxies that were actively forming when the universe was only a few hundred million years old, like the clumps in the Firefly Sparkle galaxy. “Terzan 5 may provide direct evidence that can help explain how bulges formed in galaxies throughout the universe,” Lanzoni said.

Image Description: A dramatically crowded starfield that looks like a just-shaken snow globe. The black background of space, clearer at the edges, is covered by thousands of tiny white, orange, and blue points of light, that are stars. The stars are most concentrated in the center, forming a roughly circular orb, and sparser at the edges of the image. Several larger orange stars, particularly those largest near the edges of the frame, have prominent diffraction spikes.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).

The Hubble Space Telescope has been operating for over 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. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute (STScI) in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

Learn more about Webb:
https://science.nasa.gov/webb

Learn more about Hubble:
https://science.nasa.gov/hubble

Credits: 
Image: NASA, ESA, CSA, STScI, Giorgia Zullo (University of Bologna), Francesco Ferraro (University of Bologna), N. Bartmann (ESA/Webb)
Image Processing: Alyssa Pagan (STScI)
Duration: 30 seconds
Release Date: June 16, 2026

#NASA #ESA #Astronomy #Space #Science #Galaxies #SpiralGalaxies #MilkyWay #MilkyWayBulge  #Stars #StarClusters #Terzan5 #BulgeFossilFragment #Cosmos #Universe #JWST #InfraredAstronomy #HubbleSpaceTelescope #HST  #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Terzan 5: A Milky Way Bulge Fossil Fragment | Webb & Hubble Space Telescopes

Terzan 5: A Milky Way Bulge Fossil Fragment | Webb & Hubble Space Telescopes

Image DescriptionA dramatically crowded starfield that looks like a just-shaken snow globe. The black background of space, clearer at the edges, is covered by thousands of tiny white, orange, and blue points of light, that are stars. The stars are most concentrated in the center, forming a roughly circular orb, and sparser at the edges of the image. Several larger orange stars, particularly those largest near the edges of the frame, have prominent diffraction spikes.

New observations from the James Webb Space Telescope combined with multiple observations from the Hubble Space Telescope demonstrate that Terzan 5 is a self-contained, self-enriching stellar system that contains up to four distinct star populations. It orbits within our Milky Way galaxy’s central bulge.

Researchers using two of humanity’s most powerful observatories—NASA’s James Webb and Hubble Space Telescopes—have definitively shown that Terzan 5 is not a globular star cluster as it was once classified, offering new insight into how galaxies like our own form and evolve over time. A globular star cluster typically has only one ancient star population. New data not only confirms the existence of two distinct populations of stars in Terzan 5, but also provides evidence for two more recent rounds of star formation. Although located within the crowded bulge of our Milky Way, our galaxy’s central, spherical region of older stars, Terzan 5 was massive enough to maintain its separate identity while lighter weight systems spread out and mixed to form the bulge billions of years ago. It is like a lump in an otherwise well-mixed cake batter.

“Webb’s new near-infrared observations, cross-referenced with Hubble’s archival observations, have given us a much clearer picture of the history of Terzan 5,” said Giorgia Zullo, who led the research and is a PhD student at the University of Bologna in Italy.

These results were presented at a press conference Tuesday, June 16, 2026, at the 248th meeting of the American Astronomical Society in Pasadena, California, and were published in Astronomy & Astrophysics.

New observations from Webb combined with multiple observations from Hubble show that Terzan 5 is a self-contained, self-enriching stellar system that contains up to four distinct star populations. It orbits within our Milky Way galaxy’s central bulge.

Four generations of stars
Discovered in 1968 by astronomer Azop Terzan, Terzan 5 resembles a globular cluster in many ways. However, in 2009 this system was discovered to harbor two distinct populations of stars. In 2016, Hubble provided the first estimate of their ages, showing that one formed roughly 12 billion years ago—as the Milky Way itself was assembling—and the other about 5 billion years ago, just before Earth started forming. This pointed to a more complex history than a typical globular cluster.

Studying Terzan 5 is complicated by its location in a region of our galaxy crowded with stars and heavily obscured by dust. This is where Webb stepped in. Its infrared view allowed the research team to peer through the dust and catalog many more stars, and fainter stars, than previous work. By measuring star colors and brightnesses, astronomers can classify them into populations across their ages and chemistries.

Webb was able to measure these key properties for every star within the field of view in the sky—both stars within Terzan 5 and unrelated foreground stars. To isolate the stars of Terzan 5, the team relied on the power and longevity of Hubble. The 12-year separation allowed the team to measure very small movements of individual stars, known as proper motions, to determine that stars belong to Terzan 5 and are part of the Milky Way's bulge.

By combining data from Webb and Hubble, the researchers found strong evidence for two more stellar populations, one that formed 3.8 billion years ago and another only 2.5 billion years ago. They also were able to determine the precise age of the previously known stellar populations, finding that they formed 12.5 billion and 4.7 billion years ago.

With the previously known two generations of stars, astronomers could not rule out the possibility that Terzan 5 interacted with another object, like a globular cluster or a giant molecular cloud, becoming enriched with new gas and dust that set off a second round of star formation. With four stellar generations, those explanations are ruled out.

Measurements of the stellar composition of Terzan 5 populations made at the W. M. Keck Observatory and European Southern Observatory’s Very Large Telescope also point toward very distinct populations. “Along with the ages of these populations, the cluster preserves a fossil record of progressive enrichment of heavy elements by supernovae,” said co-author R. Michael Rich, a research astronomer at the University of California, Los Angeles.

Terzan 5 formed multiple generations of stars because it was able to retain the necessary raw materials. There is evidence of powerful supernova explosions in Terzan 5 that forged heavier elements that were swept up by subsequent generations of stars. In lighter weight systems, the force of the explosions themselves could have ejected the resulting elements as well as sweeping out leftover gas and dust. The progenitor of Terzan 5 had enough mass to retain those stars’ ejections, allowing new generations of stars to form over billions of years.

‘Bulge fossil fragment’
The results show that Terzan 5 is most likely the remnant of a much more massive stellar system that initially formed 12.5 billion years ago. Terzan 5 is extraordinary because it survived—and never merged or fully “mixed in” with the Milky Way’s bulge. “For some reason, this peculiar clump of stars formed separately from the bulge and was not destroyed as the bulge itself formed,” said Francesco R. Ferraro, a professor at the University of Bologna and principal investigator of the Webb observations. “Terzan 5 is what we now call a bulge fossil fragment because it resembles the primordial clumps that contributed to the formation of the bulge.”

To date, there is one other known cosmic object like Terzan 5. Liller 1 was the second to be reclassified from a globular star cluster to a bulge fossil fragment. It also contains multiple generations of stars. There may be more objects like it. Between 40 to 50 additional globular clusters that orbit within the bulge will be examined by Ferraro’s team to determine if their stellar populations are all the same, like globular clusters, or have several generations, like bulge fossil fragments. 

Potential parallels for galaxy formation near, far
Ultimately, this research may improve what we know about how the central bulges of galaxies form over hundreds of millions of years. “Based on observations and in-depth simulations, we think that galaxies in the early universe had huge disks of gas that fragmented into clumps and formed stars. These clumps migrated to the center of the galaxies, and many merged to form their bulges,” said Barbara Lanzoni, a co-author and associate professor at the University of Bologna. For example, Webb has turned up several examples of “clumpy” galaxies that were actively forming when the universe was only a few hundred million years old, like the clumps in the Firefly Sparkle galaxy. “Terzan 5 may provide direct evidence that can help explain how bulges formed in galaxies throughout the universe,” Lanzoni said.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).

The Hubble Space Telescope has been operating for over 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. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute (STScI) in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

Learn more about Webb:
https://science.nasa.gov/webb

Learn more about Hubble:
https://science.nasa.gov/hubble


Credits: 
Image: NASA, ESA, CSA, STScI, Giorgia Zullo (University of Bologna), Francesco Ferraro (University of Bologna)
Image Processing: Alyssa Pagan (STScI)
Release Date: June 16, 2026

#NASA #ESA #Astronomy #Space #Science #Galaxies #SpiralGalaxies #MilkyWay #MilkyWayBulge  #Stars #StarClusters #Terzan5 #BulgeFossilFragment #Cosmos #Universe #JWST #InfraredAstronomy #HubbleSpaceTelescope #HST  #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #STEM #Education

China Long March 3B/E Satellite Launch | Xichang Satellite Launch Center

China Long March 3B/E Satellite Launch | Xichang Satellite Launch Center


China Academy of Launch Vehicle Technology’s Long March 3B/E launch mission emblem
Shanghai Academy of Spaceflight Technology’s Shijian-31 satellite emblem

A China Long March 3B/E rocket launched the Shanghai Academy of Spaceflight Technology-made Shijian-31 satellite beyond low Earth orbit for space environment monitoring tasks from Launch Complex 2 at the Xichang Satellite Launch Center in the southwestern Sichuan province on June 16, 2026, 17:45pm China Standard Time (09:45am Universal Coordinated Time). See slow-motion video.

This mission was the 116th launch of a Long March 3B vehicle, and the 651st launch of the Long March launch vehicle series. This was also the 41st launch from China in 2026.

Shiyan is a satellite designation used for technology development spacecraft, and the name literally translates to "experiment".


Image Credits: China Aerospace Science and Technology Corporation (CAST), Shanghai Academy of Spaceflight Technology
Date: June 16, 2026


#NASA #Space #Satellites #China #中国 #LongMarchRocket #LongMarch3B #CZ3B #CALT #中国运载火箭技术研究院 #Shijian31 #实践三十一号卫星 #CAST #通信技术试验卫星二十五号 #XSLC #西昌卫星发射中心 #SichuanProvince #四川 #STEM #Education

China Long March 3B/E Satellite Launch | Xichang Satellite Launch Center

China Long March 3B/E Satellite Launch | Xichang Satellite Launch Center

A China Long March 3B/E rocket launched the Shanghai Academy of Spaceflight Technology-made Shijian-31 satellite beyond low Earth orbit for space environment monitoring tasks from Launch Complex 2 at the Xichang Satellite Launch Center in the southwestern Sichuan province on June 16, 2026, 17:45pm China Standard Time (09:45am Universal Coordinated Time). See slow-motion video.

This mission was the 116th launch of a Long March 3B vehicle, and the 651st launch of the Long March launch vehicle series. This was also the 41st launch from China in 2026.

Shiyan is a satellite designation used for technology development spacecraft, and the name literally translates to "experiment".


Video Credit: China Aerospace Science and Technology Corporation (CAST)
Duration: 46 seconds
Date: June 16, 2026


#NASA #Space #Satellites #China #中国 #LongMarchRocket #LongMarch3B #CZ3B #CALT #中国运载火箭技术研究院 #Shijian31 #实践三十一号卫星 #CAST #通信技术试验卫星二十五号 #XSLC #西昌卫星发射中心 #SichuanProvince #四川 #STEM #Education #HD #Video

A Bubblegum-pink Nebula: Gum 46 in Crux | European Southern Observatory

A Bubblegum-pink Nebula: Gum 46 in Crux | European Southern Observatory

This picture shows Gum 46, a stunning gas cloud 5500 light-years away, observed in detail with the European Southern Observatory’s Very Large Telescope (VLT). Why does it glow pink?

At the heart of Gum 46 there is a young, hot, and blue star called HD311999. Its intense radiation excites atoms in the surrounding gas. This then re-emit this energy at very specific colors or wavelengths. The pink shade that dominates this image is due to hydrogen atoms, the most abundant element in this nebula and the Universe as a whole.

The dark wispy clouds that surround the nebula make for a stunning sight, too. These clouds are not intrinsically dark. They are extremely dense regions of dust that block light passing through them, enshrouding the glowing heart of Gum 46.

This image was created as part of the European Southern Observatory (ESO) Cosmic Gems program, an outreach initiative to produce images of interesting, intriguing or visually attractive objects using ESO telescopes, for the purposes of education and public outreach. The program makes use of telescope time that cannot be used for science observations. All data collected may also be suitable for scientific purposes, and are made available to astronomers through ESO’s science archive.


Credit: European Southern Observatory (ESO)
Release Date: May 13, 2024

#NASA #ESO #Astronomy #Space #Science #Nebulae #Gum46 #EmissionNebulae #Stars #HD311999 #CruxConstellations #MilkyWayGalaxy #Cosmos #Universe #VST #ParanalObservatory #Chile #SouthAmerica #Europe #STEM #Education

Monday, June 15, 2026

Planets Venus, Jupiter & Mercury: View from Arizona

Planets Venus, Jupiter & Mercury: View from Arizona


Astrophotographer David Blanchard: "The planets Mercury, Venus, and Jupiter continue to put on a show during evening twilight, including a reflection of Mercury in the calm waters of the lake."

In astronomy, a conjunction refers to an event where two or more celestial bodies appear to meet or pass each other in the sky. A conjunction is an apparent phenomenon caused by an observer's perspective. However, the two objects involved are not actually close to one another in space.

Arizona is a landlocked state in the Southwestern region of the United States, sharing the Four Corners region of the western United States with Colorado, New Mexico, and Utah. It also borders Nevada to the northwest and California to the west, and shares an international border with the Mexican states of Sonora and Baja California to the south and southwest.


Image Credit: David Blanchard
Location: Lake Mary, Flagstaff, Arizona
Image Details: Nikon D850, 35mm, f/2.8, ISO 100, 8 seconds
Date: June 13, 2026

#NASA #Space #Astronomy #Science #Sun #SolarSystem #Planets #Earth #Mercury #Venus #Jupiter  #PlanetaryConjunctions #Astrophotography #Astrophotographers #DavidBlanchard #CitizenScience #LakeMary #Flagstaff #Arizona #UnitedStates #STEM #Education

China CAS Space Commercial Rocket Achieves Higher Launch Frequency

China CAS Space Commercial Rocket Achieves Higher Launch Frequency

A Kinetica-1 (Lijian-1) Y14 rocket, developed by Chinese commercial space company CAS Space, blasted off at 11:44 am Beijing Time (BJT) on June 15, 2026, from Dongfeng Commercial Space Innovation Test Zone in Northwest China delivering eight rideshare satellites into their designated orbits. These remote sensing satellites are now in Earth orbit and will image a variety of areas on behalf of Chinese provincial and municipal operators.

Kinetica-1 is now the first vehicle from a private Chinese provider to launch 100 satellites. Today’s launch was the 14th launch for Kinetica-1, and the 15th for CAS Space through its Kinetica family of launch vehicles. This was also the 40th launch from China in 2026. The CAS Space team continues to expand rocket production and launch frequency to meet rising commercial demand. The CAS Space factory in Guangzhou aims for low-cost, mass-production. The Kinetica-1 launch vehicle has flown for the third time in three months, delivering eight Chang Guang Satellite Technology (CGSTL) built satellites into orbit where they will begin imaging Earth below for provincial and municipal operators including:

CGSTL manufactured several satellites for this  launch mission, starting with its own Jilin Gaofen-07C04 (吉星高分07C04星), for an expansion of its Jilin-1 (吉林一号) Earth imaging constellation. Caiyun Opitcal-01 (彩云光学01星), a high-resolution optical remote sensing satellite dedicated to Yunnan province for geological disaster prevention and monitoring of natural resources, jointly backed by the Yunnan Provincial Bureau of Geology and Mineral Resources and the Yunnan Geological and Mining Group (云南地矿集团).

Antie-03 (安铁03星), also a high-resolution optical remote sensing satellite for Quanzhou Zhongke Xingqiao Aerospace Technology Co. Ltd. (泉州中科星桥空天技术有限公司), supported by Anxi County People’s Government for ‘smart’ crop monitoring and management for Fujian province’s tea industry as part of its digital upgrade plans.

‘Lichuan Red (利川红)’, another a high-resolution optical remote sensing satellite that is for the city of Lichuan in Hubei province, to monitor its ecological situation and resources, while supporting its tea industry, backed by Lichuan Municipal People's Government, who have technical support from Hubei Lirui Technology Co. Ltd.

Cultural Relics-01 (文物01星), tasked with monitoring cultural heritage sites from space by the National Cultural Heritage Administration via its high-resolution optical remote sensing capabilities.

Three other satellites launched were not yet named by CAS Space or their owner/operators.

Kinetica-1 is CAS Space’s first launch vehicle and consists of four stages, all burning solid fuel. CAS Space offers the ability to launch a single satellite to utilize all of the rocket’s payload capacity, however more ‘rideshare’ missions occur for multiple satellites to be delivered in one launch.

The payload capacity of the launch vehicle is:

2,000 kilograms to low Earth orbit

1,500 kilograms to a 500-kilometer sun-synchronous orbit

The first-stage is powered by a solid rocket booster that burns an unspecified solid fuel, generating 200 tons of thrust. The second-stage is also powered by a solid rocket booster, producing 110 tons of thrust with the same unidentified propellant. The-third stage, also using the undisclosed propellant, generates 45 tons of thrust. Finally, the fourth-stage is powered by another solid rocket booster, providing 8 tons of thrust with the same solid propellant.

On its launch pad, Kinetica-1 stands at 30 meters tall. The first two stages have a diameter of 2.65 meters, the fairing has a diameter of either 2.65 or 3.35 meters. When prepared for launch Kinetica-1 weighs a believed 135,000 kilograms.

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).


Video Credit: CAS Space/SMG
Text Credits: CAS Space, Xinhua, CGTN
Duration: 1 minute, 20 seconds
Date: June 15, 2026


#NASA #Space #Satellites #Earth #EarthObservation #RemoteSensing #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #Kinetica1 #Lijian1 #Lijian1Y14Rocket #Lijian1Y14 #LaunchVehicles #SolidFuelRockets #CGSTL #SatelliteLaunches #CommercialSpace #CAS #JiuquanSatelliteLaunchCenter #JSLC #InnerMongolia #STEM #Education #HD #Video

China CAS Space Commercial Rocket Launch of Eight Earth Observation Satellites

China CAS Space Commercial Rocket Launch of Eight Earth Observation Satellites

A Kinetica-1 (Lijian-1) Y14 rocket, developed by Chinese commercial space company CAS Space, blasted off at 11:44 am Beijing Time (BJT) on June 15, 2026, from Dongfeng Commercial Space Innovation Test Zone in Northwest China delivering eight rideshare satellites into their designated orbits. These remote sensing satellites are now in Earth orbit and will image a variety of areas on behalf of Chinese provincial and municipal operators.

Kinetica-1 is now the first vehicle from a private Chinese provider to launch 100 satellites. Today’s launch was the 14th launch for Kinetica-1, and the 15th for CAS Space through its Kinetica family of launch vehicles. This was also the 40th launch from China in 2026. The CAS Space team continues to expand rocket production and launch frequency to meet rising commercial demand. The CAS Space factory in Guangzhou aims for low-cost, mass-production. The Kinetica-1 launch vehicle has flown for the third time in three months, delivering eight Chang Guang Satellite Technology (CGSTL) built satellites into orbit where they will begin imaging Earth below for provincial and municipal operators including:

CGSTL manufactured several satellites for this  launch mission, starting with its own Jilin Gaofen-07C04 (吉星高分07C04星), for an expansion of its Jilin-1 (吉林一号) Earth imaging constellation. Caiyun Opitcal-01 (彩云光学01星), a high-resolution optical remote sensing satellite dedicated to Yunnan province for geological disaster prevention and monitoring of natural resources, jointly backed by the Yunnan Provincial Bureau of Geology and Mineral Resources and the Yunnan Geological and Mining Group (云南地矿集团).

Antie-03 (安铁03星), also a high-resolution optical remote sensing satellite for Quanzhou Zhongke Xingqiao Aerospace Technology Co. Ltd. (泉州中科星桥空天技术有限公司), supported by Anxi County People’s Government for ‘smart’ crop monitoring and management for Fujian province’s tea industry as part of its digital upgrade plans.

‘Lichuan Red (利川红)’, another a high-resolution optical remote sensing satellite that is for the city of Lichuan in Hubei province, to monitor its ecological situation and resources, while supporting its tea industry, backed by Lichuan Municipal People's Government, who have technical support from Hubei Lirui Technology Co. Ltd.

Cultural Relics-01 (文物01星), tasked with monitoring cultural heritage sites from space by the National Cultural Heritage Administration via its high-resolution optical remote sensing capabilities.

Three other satellites launched were not yet named by CAS Space or their owner/operators.

Kinetica-1 is CAS Space’s first launch vehicle and consists of four stages, all burning solid fuel. CAS Space offers the ability to launch a single satellite to utilize all of the rocket’s payload capacity, however more ‘rideshare’ missions occur for multiple satellites to be delivered in one launch.

The payload capacity of the launch vehicle is:

2,000 kilograms to low Earth orbit

1,500 kilograms to a 500-kilometer sun-synchronous orbit

The first-stage is powered by a solid rocket booster that burns an unspecified solid fuel, generating 200 tons of thrust. The second-stage is also powered by a solid rocket booster, producing 110 tons of thrust with the same unidentified propellant. The-third stage, also using the undisclosed propellant, generates 45 tons of thrust. Finally, the fourth-stage is powered by another solid rocket booster, providing 8 tons of thrust with the same solid propellant.

On its launch pad, Kinetica-1 stands at 30 meters tall. The first two stages have a diameter of 2.65 meters, the fairing has a diameter of either 2.65 or 3.35 meters. When prepared for launch Kinetica-1 weighs a believed 135,000 kilograms.

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).


Video Credit: CAS Space
Text Credits: CAS Space, Xinhua, CGTN
Duration: 27 seconds
Date: June 15, 2026


#NASA #Space #Satellites #Earth #EarthObservation #RemoteSensing #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #Kinetica1 #Lijian1 #Lijian1Y14Rocket #Lijian1Y14 #LaunchVehicles #SolidFuelRockets #CGSTL #SatelliteLaunches #CommercialSpace #CAS #JiuquanSatelliteLaunchCenter #JSLC #InnerMongolia #STEM #Education #HD #Video

China CAS Space Commercial Rocket Launch of Eight Earth Observation Satellites

China CAS Space Commercial Rocket Launch of Eight Earth Observation Satellites








A Kinetica-1 (Lijian-1) Y14 rocket, developed by Chinese commercial space company CAS Space, blasted off at 11:44 am Beijing Time (BJT) on June 15, 2026, from Dongfeng Commercial Space Innovation Test Zone in Northwest China delivering eight rideshare satellites into their designated orbits. These remote sensing satellites are now in Earth orbit and will image a variety of areas on behalf of Chinese provincial and municipal operators.

Kinetica-1 is now the first vehicle from a private Chinese provider to launch 100 satellites. Today’s launch was the 14th launch for Kinetica-1, and the 15th for CAS Space through its Kinetica family of launch vehicles. This was also the 40th launch from China in 2026. The CAS Space team continues to expand rocket production and launch frequency to meet rising commercial demand. The CAS Space factory in Guangzhou aims for low-cost, mass-production. The Kinetica-1 launch vehicle has flown for the third time in three months, delivering eight Chang Guang Satellite Technology (CGSTL) built satellites into orbit where they will begin imaging Earth below for provincial and municipal operators including:

CGSTL manufactured several satellites for this  launch mission, starting with its own Jilin Gaofen-07C04 (吉星高分07C04星), for an expansion of its Jilin-1 (吉林一号) Earth imaging constellation. Caiyun Opitcal-01 (彩云光学01星), a high-resolution optical remote sensing satellite dedicated to Yunnan province for geological disaster prevention and monitoring of natural resources, jointly backed by the Yunnan Provincial Bureau of Geology and Mineral Resources and the Yunnan Geological and Mining Group (云南地矿集团).

Antie-03 (安铁03星), also a high-resolution optical remote sensing satellite for Quanzhou Zhongke Xingqiao Aerospace Technology Co. Ltd. (泉州中科星桥空天技术有限公司), supported by Anxi County People’s Government for ‘smart’ crop monitoring and management for Fujian province’s tea industry as part of its digital upgrade plans.

‘Lichuan Red (利川红)’, another a high-resolution optical remote sensing satellite that is for the city of Lichuan in Hubei province, to monitor its ecological situation and resources, while supporting its tea industry, backed by Lichuan Municipal People's Government, who have technical support from Hubei Lirui Technology Co. Ltd.

Cultural Relics-01 (文物01星), tasked with monitoring cultural heritage sites from space by the National Cultural Heritage Administration via its high-resolution optical remote sensing capabilities.

Three other satellites launched were not yet named by CAS Space or their owner/operators.

Kinetica-1 is CAS Space’s first launch vehicle and consists of four stages, all burning solid fuel. CAS Space offers the ability to launch a single satellite to utilize all of the rocket’s payload capacity, however more ‘rideshare’ missions occur for multiple satellites to be delivered in one launch.

The payload capacity of the launch vehicle is:

2,000 kilograms to low Earth orbit

1,500 kilograms to a 500-kilometer sun-synchronous orbit

The first-stage is powered by a solid rocket booster that burns an unspecified solid fuel, generating 200 tons of thrust. The second-stage is also powered by a solid rocket booster, producing 110 tons of thrust with the same unidentified propellant. The-third stage, also using the undisclosed propellant, generates 45 tons of thrust. Finally, the fourth-stage is powered by another solid rocket booster, providing 8 tons of thrust with the same solid propellant.

On its launch pad, Kinetica-1 stands at 30 meters tall. The first two stages have a diameter of 2.65 meters, the fairing has a diameter of either 2.65 or 3.35 meters. When prepared for launch Kinetica-1 weighs a believed 135,000 kilograms.

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).


Image Credits: CAS Space
Text Credits: CAS Space, Xinhua, CGTN
Date: June 15, 2026


#NASA #Space #Satellites #Earth #EarthObservation #RemoteSensing #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #Kinetica1 #Lijian1 #Lijian1Y14Rocket #Lijian1Y14 #LaunchVehicles #SolidFuelRockets #CGSTL #SatelliteLaunches #CommercialSpace #CAS #JiuquanSatelliteLaunchCenter #JSLC #InnerMongolia #STEM #Education