Planet Mars Images: Sept. 30-Oct. 5, 2026 | NASA's Curiosity & Perseverance Rovers
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Planet Mars Images: Sept. 30-Oct. 5, 2026 | NASA's Curiosity & Perseverance Rovers
Dying Star Creates Brand New Planet | Hubble Space Telescope
What if a star’s death could give rise to an entirely new planet?
Astronomers revisiting decades-old observations from NASA’s Hubble Space Telescope found an unexpected chemical clue around a white dwarf: niobium, a heavy element forged during the final stages of a star’s life.
Combined with observations from other NASA missions, the evidence points to an intriguing possibility: a Jupiter-sized world may have formed from material expelled when the star died.
If confirmed, this “second-generation” planet could reveal that the death of a star is not always the end of its planetary system. It may result in the beginning of a new one.
Crew-12 Farewell & Change of Command Ceremony | International Space Station
Aboard the International Space Station, Crew-12 NASA astronauts Jessica Meir and Jack Hathaway as well as European Space Agency astronaut Sophie Adenot and Roscosmos cosmonaut Andrey Fedyaev of Russia, provided farewell remarks on Oct. 4, 2026, ahead of their upcoming departure from the space station.
Joining Crew-12 for the farewell remarks were NASA astronauts Jessica Watkins, Luke Delaney, and Anil Menon as well as Canadian Space Agency astronaut Josh Kutryk and Roscosmos cosmonauts Sergey Teteryatnikov, Andrey Fedyaev, Pyotr Dubrov, and Anna Kikina of Russia. Following the farewell remarks a change of command ceremony took place where Meir handed over command of the space station to Dubrov.
Crew-12 is slated to undock on Oct. 5 and splash down off the coast of California Oct. 6 after completing a long-duration science mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration missions. Such research benefits people on Earth and lays the groundwork for future human exploration through the agency’s Artemis missions that will send astronauts to the Moon to prepare for future expeditions to Mars.
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.
Video Credit: NASA's Johnson Space Center
Duration: 10 minutes
Date: Oct. 4, 2026
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Planetary Nebula IC 4634 in Ophiuchus: Glowing Waves | Hubble
This striking Hubble image of the planetary nebula IC 4634 reveals two shining, S-shaped ejections from a dying star. This star, awash in glowing material at the center of the picture, bloated as it aged and launched its outer layers off into space. The star’s very hot, exposed core has since beamed intense ultraviolet radiation at these lost shells of gas, making them glow in rich colors.
This process has been far from orderly or calm, however, as revealed by the distinct, separate waves of thrown-off gases. One is more distant and therefore was spewed first, followed by a more recently ejected tide of matter that formed the tighter S-shape. The result is remarkably symmetric on each side of the central star.
The NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2 (WFPC2) captured this image of IC 4634. It is found more than about 7,500 light-years away in the constellation of Ophiuchus (the Serpent Holder). IC 4634 and other objects like it are known as planetary nebulae due to their appearance through early telescopes as rounded, faintly luminous discs similar to the distant planets Uranus and Neptune.
This picture was created from images through five filters (F487N, F502N, F574M, F656N and F658N) that captured light emitted by elements in the gaseous features. The total aggregate exposure time was 4,000 seconds and the field of view is just 29 arcseconds across.
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Close-up: Nebula NGC 7380 in Cepheus | Kitt Peak National Observatory
NGC 7380 is a typical star-forming region in the direction of an outer spiral arm of our galaxy (around 7,000 light years distant). It is a young open cluster of stars in the northern circumpolar constellation of Cepheus, discovered by Caroline Herschel in 1787. This field contains many young energetic stars that make the natal gas surrounding them glow an intense pink/red. The majority of stars in this newly formed group are out of the field to the upper left. Their winds and radiation sculpt clouds of gas and dust into the mountainous ridges seen here. The darkest parts of this image are foreground clouds of dust thick enough to extinct the light beyond them. Also note the bright star (left of center) that is in a bluish bubble of gas. This may be a Wolf-Rayet star beginning to blow a bubble. Other famous examples of this action include The Bubble Nebula and Thor's Helmut.
This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.
NASA’s DAVINCI Probe Model Beats The Heat for Blistering Planet Venus Descent
This close-up photo shows the engineering development model for NASA’s Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI) probe. It was photographed prior to a major thermal evaluation, where the DAVINCI team demonstrated that it could insulate the instruments the probe will carry from the intense heat of planet Venus. The probe probe passed a key test that ran from Aug. 28 to Sept. 10, 2026.
The DAVINCI team took the engineering model to a furnace at Rex Heat Treat in Bedford, Pennsylvania. It is one of few facilities capable of heating up to Venus-like temperatures as rapidly as the probe would experience. They slid the yoga ball-sized vessel into a ceramic-lined chamber with heat-scorched walls and ratcheted up the temperature to 869 F, or 465 C, over the course of about an hour—the same pace the probe will heat up during its descent to the surface of Venus.
They repeated the thermal cycling process five more times. The engineering model made it through every cycle unscathed, indicating that the probe can withstand extreme temperatures and protect its delicate scientific instruments while traveling through Venus’ atmosphere. During the testing, hardware simulating the instruments was closely monitored via more than a hundred thermal sensors.
“The experiment was a rousing success with six runs to Venus’ surface temperature on our descent timeline of 55–60 minutes with full internal instrumentation,” said Jim Garvin, the principal investigator for DAVINCI at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “There hasn’t been such a complete assessment of spacecraft-scale hardware at Venus temperatures in the U.S. since the mid-1970s.”
The DAVINCI spacecraft is being developed to travel to Venus to investigate numerous unsolved puzzles, including whether the planet once had oceans and was habitable, like Earth. To explore these mysteries, the spacecraft will release a probe that will withstand hellish temperatures for nearly an hour as it descends through Venus’ toxic atmosphere, collecting data along the way.
“It’s a huge engineering challenge given how harsh the Venus environment is,” said Kristen Brown, the DAVINCI probe manager at NASA Goddard. “We had to create a system that can protect the instruments from the planet’s overwhelming heat while strategically letting in its high-temperature gases to study through special inlet ports.”
Encased in a corrosion resistant, strong-yet-lightweight titanium shell, the DAVINCI probe will be equipped with a suite of instruments to sample the composition of the gases of the Venusian atmosphere to determine what molecules they are made of and learn about the atmosphere’s structure. It will also contain cameras that will snap the highest-resolution images of Venus’ surface ever. Scientists will use these to make a new 3D map. The probe also has a radio system to send data back to its orbiting spacecraft 5,600 miles (9,000 kilometers) overhead.
This heat testing follows on the heels of a campaign earlier this summer to demonstrate the probe’s imaging system. The mission is currently working toward gaining approval to move into the final design and fabrication phase. “The DAVINCI team has now met both of the major mission milestones this year on an accelerated timeline,” Garvin said. Showing that the DAVINCI probe can withstand the Venusian heat, brings scientists one step closer to learning why Earth’s “twin” varies greatly from our home.
Previous Probe Missions at Planet Venus
Thirteen probes successfully entered the Venusian atmosphere, including the two Venera-Halley probes. Ten of those successfully landed on the surface of the planet. Due to the extreme conditions, the probes could only survive for a short period on the surface, from 23 minutes to two hours.
The Venera program established a number of precedents in space exploration, among them being the first man-made devices to enter the atmosphere of another planet (Venera 3 on March 1, 1966), the first to make a soft landing on another planet (Venera 7 on December 15, 1970), the first to return images from another planet's surface (Venera 9 on June 8, 1975), the first to record sounds on another planet (Venera 13 on October 30, 1981), and the first to perform high-resolution radar mapping scans (Venera 15 on June 2, 1983). The intense pressures that led to the short lifespans of many of the probes was itself an important finding.
China's Rocket Launches Hit Record as Commercial Space Firms Scale Up
China carried out a record 70 rocket launch missions in the first nine months of 2026, up by about 19 percent from a year earlier, as its commercial space industry accelerated mass production, advanced reusable rocket technology and expanded satellite services overseas.
Ten launches took place in September alone. The Pallas-1 rocket made its maiden flight, adding a new model to China's commercial launch fleet, while Zhuque-2E and Gravity-1 became the first privately developed rockets to support the deployment of a low-Earth-orbit satellite internet constellation.
The surge in constellation launches is putting pressure on rocket makers to deliver vehicles faster and at lower cost. On Sept. 20, the Lijian-1 Y18 rocket placed nine satellites into orbit, continuing a launch cadence that has become roughly monthly for the model.
CAS Space, the commercial rocket maker behind Lijian-1, has cut the vehicle's final assembly cycle from three months to about 15 days by reorganizing production.
"We have adopted a pulse-line production model, dividing the final assembly of each rocket among six or seven fixed workstations, with different assembly tasks carried out at each one," said Xiang Zebin, deputy chief designer of the Lijian-1 carrier rocket at CAS Space.
Other commercial rocket companies are also beginning production before orders are finalized, shortening the time between receiving a contract and carrying out a launch. Several are developing multiple rocket models in parallel while building the capacity for batch deliveries.
"As we move from one rocket to 100, we have to think in industrial terms: can we produce rockets at scale while continuing to deliver successful launches? This depends on ensuring consistency from one vehicle to the next," said Bu Xiangwei, chairman of private Chinese launch company Orienspace.
Reusable technology is another focus as companies seek to lower costs and increase launch frequency for large satellite constellations.
On July 10, the Long March-10B completed the world's first recovery of a rocket stage using a net system at sea. On Aug. 19, LandSpace's Zhuque-3 Y2 carried out China's first controlled land recovery of an orbital-class rocket's first stage using landing legs. The two recovered stages are being inspected and refurbished in preparation for future flights.
"Reusing rockets multiple times can significantly reduce overall launch costs. I believe that within five to 10 years, we will be able to match international benchmarks for launch costs per kilogram," said Wang Xinyan, general manager of supply chain management at private rocket developer LandSpace.
China's commercial satellite companies are also looking overseas as domestic launch capacity expands. GalaxySpace's Lingzhi-09 Thai CubeSat was launched in August, marking the first time a Chinese commercial space company had completed satellite development, launch and in-orbit delivery for a Southeast Asian country.
"This demonstrates that our satellite products, end-to-end satellite solutions and service capabilities are ready for overseas markets. Over the next three to five years, we aim to build a well-developed network of resources and deliver successful projects in Belt and Road partner countries, particularly across ASEAN," said Huang Heping, general manager of international business development at commercial satellite maker GalaxySpace.
China's first-nine-month launch total was 11 higher than the 59 recorded in the same period last year. The rise reflects a broader shift from individual satellite missions toward constellation deployment, batch launches and a more diverse range of space-based services.
"The string of successful launches across multiple rocket types shows that both state-backed developers and private companies have reached a high level of technological maturity. Rocketry's advanced technologies are also helping drive upgrades in related products and manufacturing," said Yang Yuguang, chairman of the Space Transportation Committee of the International Astronautical Federation.
NASA Flies in California’s Pacific Airshow
Planetary Nebula NGC 6572 in Ophiuchus | Hubble Space Telescope
The NASA/European Space Agency Hubble Space Telescope has turned its eagle eye to the planetary nebula NGC 6572, a very bright example of these strange but beautiful objects. Planetary nebulae are created during the late stages of the evolution of certain stars that eject gas into space and emit intense ultraviolet radiation that makes the material glow. This picture of NGC 6572 shows the intricate shapes that can develop as stars exhale their last breaths. Hubble has even imaged the central white dwarf star, the origin of the dazzling nebula, but now a faint, but hot, vestige of its former glory.
NGC 6572 only began to shed its gases a few thousand years ago, so it is a fairly young planetary nebula. As a result the material is still quite concentrated. This explains why it is abnormally bright. The envelope of gas is currently racing out into space at a speed of around 15 kilometers every second and as it becomes more diffuse, it will dim.
NGC 6572 was discovered in 1825 by the German astronomer Friedrich Georg Wilhelm von Struve. He came from a family of distinguished stargazers. The name planetary nebula is left over from the time when the telescopes of early astronomers were not good enough to reveal the true nature of these objects. To many, the discs looked like the outer planets Uranus and Neptune. The application of spectral analysis, later in the 19th century, first revealed that they were glowing gas clouds.
NGC 6572 is magnitude 8.1, easily bright enough to make it an appealing target for amateur astronomers with telescopes. It is located within the large constellation of Ophiuchus (the Serpent Bearer) and at low magnification it will appear to be just a colored star, but higher magnification will reveal its shape. Observers report that NGC 6572 looks blue, while others state that it is green. Color as seen through the eyepiece is often a matter of interpretation, so you may make your own decision.
This picture was created from images taken with Hubble’s Wide Field Camera 2. Images through a blue filter that isolates the glow from hydrogen gas (Hβ, F487N, colored dark blue), a green filter that isolates emission from ionized oxygen (F502N, colored blue), a yellow broadband filter (F555W, colored green) and a red filter that passes emission from hydrogen (Hα, F656N) have been combined. The exposure times were 360 s, 240 s, 100 s and 180 s, respectively and the field of view is just 29 arcseconds across.
NASA Artemis III Rocket Nose Cone Assembly | Kennedy Space Center
Engineers with NASA’s Exploration Ground Systems complete integration of the aerodynamic nose cones onto the left and right forward segments on the twin Space Launch System (SLS) solid rocket boosters, finishing their stacking operations for Artemis III inside the Vehicle Assembly Building’s High Bay 3 at NASA’s Kennedy Space Center in Florida on Wednesday, Sept. 30, 2026. Each forward assembly contains an aerodynamic top, a forward skirt housing avionics, and frustum housing motors that allow the boosters to separate from the SLS core stage after launch. The twin solid boosters will help support the remaining rocket components and the Orion spacecraft during final assembly of the Artemis III rocket and provide more than 75 percent of the total SLS thrust during liftoff from NASA Kennedy’s Launch Pad 39B.
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.
NASA’s SpaceX Crew-13 Arrival & Welcoming Remarks | International Space Station
NASA astronauts Jessica Watkins and Luke Delaney, as well as Canadian Space Agency astronaut Joshua Kutryk and Roscosmos Sergey Teteryatnikov of Russia, docked to the forward port of the Harmony module of the International Space Station Oct. 1, 2026, following their launch less than nine hours prior on a SpaceX Dragon spacecraft and Falcon 9 rocket from Cape Canaveral in Florida. Following docking, the quartet opened the hatch and floated aboard the orbital outpost before providing welcoming remarks as their mission aboard the space station began.
Crew-13 will conduct a long-duration mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration flights as part of NASA’s Moon and Mars exploration approach, including lunar missions through NASA’s Artemis program.
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.
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Journey to Globular Star Cluster Messier 107 in Ophiuchus | MPG/ESO Telescope
In this zoom sequence we start with the spectacular vista of the central regions of the Milky Way galaxy. We then close in on a fuzzy ball of stars, the globular cluster Messier 107, also known as NGC 6171. It lies about 21, 000 light-years away in the constellation of Ophiuchus. The final close up view was created from exposures taken through blue, green and near-infrared filters, using the Wide Field Imager (WFI) on the MPG/ESO 2.2-meter telescope at La Silla Observatory, Chile.
Messier 107 is around 13 arcminutes across, equivalent to about 80 light-years at its distance. As is typical of globular clusters, a population of thousands of old stars in Messier 107 is densely concentrated into a volume that is only about twenty times the distance between our Sun and its nearest stellar neighbor, Alpha Centauri, across.
Learn about MPG/ESO 2.2-meter telescope: https://www.eso.org/public/teles-instr/lasilla/mpg22/
Wide-view: Globular Star Cluster Messier 107 in Ophiuchus | MPG/ESO Telescope
The globular cluster Messier 107, also known as NGC 6171, is located about 21,000 light-years away in the constellation of Ophiuchus. Messier 107 is around 13 arcminutes across, equivalent to about 80 light-years at its distance. As is typical of globular clusters, a population of thousands of old stars in Messier 107 is densely concentrated into a volume that is only about twenty times the distance between our Sun and its nearest stellar neighbor, Alpha Centauri, across.
This image was created from exposures taken through blue, green and near-infrared filters, using the Wide Field Imager (WFI) on the MPG/ESO 2.2-meter telescope at La Silla Observatory, Chile.
Learn about MPG/ESO 2.2-meter telescope: https://www.eso.org/public/teles-instr/lasilla/mpg22/
Earth Flyby: Europe's Jupiter Icy Moons Explorer (JUICE) | Jupiter Arrival in 2031
JUICE’s monitoring cameras provide 1024 x 1024 pixel snapshots that can be processed in color. Their main purpose is to monitor the spacecraft’s various booms and antennas, especially during the challenging period after launch. The photos they captured of Earth during the flyby are a bonus.
In the first seconds of the video we see a view from Juice monitoring camera 2—or JMC2—with Earth appearing as a thin crescent at the bottom right of the frame. Around ten seconds in, we switch to a view from JMC1, with almost the entire disc of Earth visible at the top right of the frame. The large land mass that we see is Africa. Even the Moon is visible as a tiny grey dot to Earth’s right. At the very end of the video, JMC1 gives us a final view of Earth in the distance as it flies away on September 29.
Barnard 68: The Black Cloud in Ophiuchus | European Southern Observatory
Hot-staging Maneuver on SpaceX Starship Flight 14 (Starship 1st stage view)
NASA plans to use a lunar lander version of Starship to deliver astronauts and cargo to the Moon during the Artemis IV mission and beyond through the Human Landing System (HLS) Program.